C. B. Jackson - University of California, Department of Physics, Berkeley, CA, USA

C. B. Jackson
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Name
C. B. Jackson
Affiliation
University of California, Department of Physics, Berkeley, CA, USA
City
Berkeley
Country
United States

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Pub Categories

 
Instrumentation and Methods for Astrophysics (12)
 
High Energy Physics - Experiment (11)
 
Cosmology and Nongalactic Astrophysics (9)
 
High Energy Physics - Phenomenology (8)
 
Physics - Instrumentation and Detectors (8)
 
Astrophysics of Galaxies (8)
 
Physics - Strongly Correlated Electrons (5)
 
Quantum Physics (4)
 
Physics - Materials Science (4)
 
High Energy Astrophysical Phenomena (3)
 
Physics - Mesoscopic Systems and Quantum Hall Effect (3)
 
Computer Science - Cryptography and Security (2)
 
Physics - Accelerator Physics (1)
 
Physics - Other (1)
 
Statistics - Applications (1)
 
Computer Science - Software Engineering (1)
 
Physics - Atmospheric and Oceanic Physics (1)
 
Computer Science - Computers and Society (1)
 
Quantitative Biology - Neurons and Cognition (1)
 
Solar and Stellar Astrophysics (1)
 
Statistics - Methodology (1)
 
Mathematics - Numerical Analysis (1)

Publications Authored By C. B. Jackson

In the context of quantum tomography, quantities called a partial determinants\cite{jackson2015detecting} were recently introduced. PDs (partial determinants) are explicit functions of the collected data which are sensitive to the presence of state-preparation-and-measurement (SPAM) correlations. In this paper, we demonstrate further applications of the PD and its generalizations. Read More

In the context of quantum tomography, we recently introduced a quantity called a partial determinant \cite{jackson2015detecting}. PDs (partial determinants) are explicit functions of the collected data which are sensitive to the presence of state-preparation-and-measurment (SPAM) correlated errors. As such, PDs bypass the need to estimate state-preparation or measurement parameters individually. Read More

Synchrotron emission pervades the Galactic plane at low radio frequencies, originating from cosmic ray electrons interacting with the Galactic magnetic field. Using a low-frequency radio telescope, the Murchison Widefield Array (MWA), we measure the free-free absorption of this Galactic synchrotron emission by intervening HII regions along the line of sight. These absorption measurements allow us to calculate the Galactic cosmic-ray electron emissivity behind and in front of 47 detected HII regions in the region $250^\circ < l < 355^\circ$, $|b| < 2^\circ$. Read More

Cyber has changed the scope of the national security mission and is placing new strains on our diplomatic, warfighting, legal, and economic/budgetary processes. Cybersecurity processes and techniques are increasingly critical to our warfighting missions, but they can also inhibit the pace and potential for high impact, game-changing innovation. Throughout its history, the Navy has shown the ability of innovation (in policy, process, and technology) to change the game when our security is on the line. Read More

We discuss the Seebeck coefficient and the Hall mobility of electrons confined in narrow SrTiO3 quantum wells as a function of the three-dimensional carrier density and temperature. The quantum wells contain a fixed sheet carrier density of ~ 7x10^14 cm^-2 and their thickness is varied. At high temperatures, both properties exhibit apparent Fermi liquid behavior. Read More

In the context of quantum tomography, we recently introduced a quantity called a partial determinant \cite{jackson2015detecting}. PDs (partial determinants) are explicit functions of the collected data which are sensitive to the presence of state-preparation-and-measurement (SPAM) correlations. Importantly, this is done without any need to estimate state-preparation or measurement parameters. Read More

The next grand challenges for society and science are in the brain sciences. A collection of 60+ scientists from around the world, together with 10+ observers from national, private, and foundations, spent two days together discussing the top challenges that we could solve as a global community in the next decade. We eventually settled on three challenges, spanning anatomy, physiology, and medicine. Read More

We describe the performance of the Boolardy Engineering Test Array (BETA), the prototype for the Australian Square Kilometre Array Pathfinder telescope ASKAP. BETA is the first aperture synthesis radio telescope to use phased array feed technology, giving it the ability to electronically form up to nine dual-polarization beams. We report the methods developed for forming and measuring the beams, and the adaptations that have been made to the traditional calibration and imaging procedures in order to allow BETA to function as a multi-beam aperture synthesis telescope. Read More

In model comparisons with observational data, not all data contain information that is useful for answering a specific science question. If non-relevant or highly uncertain data are included in a comparison metric, they can reduce the significance of other observations that matter for the scientific process of interest. Sources of noise and correlations among summed quantities within a comparison metric affect the significance of a signal that is useful for testing model skill. Read More

2016Apr

We describe a new hit-based $b$-tagging technique for high energy jets and study its performance with a Geant4-based simulation. The technique uses the fact that at sufficiently high energy a B meson or baryon can live long enough to traverse the inner layers of pixel detectors such as those in the ATLAS, ALICE, or CMS experiments prior to decay. By first defining a "jet" via the calorimeter, and then counting hits within that jet between pixel layers at increasing radii, we show it is possible to identify jets that contain $b$-quarks by detecting a jump in the number of hits. Read More

The GaLactic and Extragalactic All-sky MWA survey (GLEAM) is a new relatively low resolution, contiguous 72-231 MHz survey of the entire sky south of declination +25 deg. In this paper, we outline one approach to determine the relative contribution of system noise, classical confusion and sidelobe confusion in GLEAM images. An understanding of the noise and confusion properties of GLEAM is essential if we are to fully exploit GLEAM data and improve the design of future low-frequency surveys. Read More

This paper outlines how the new GaLactic and Extragalactic All-sky MWA Survey (GLEAM, Wayth et al. 2015), observed by the Murchison Widefield Array covering the frequency range 72 - 231 MHz, allows identification of a new large, complete, sample of more than 2000 bright extragalactic radio sources selected at 151 MHz. With a flux density limit of 4 Jy this sample is significantly larger than the canonical fully-complete sample, 3CRR (Laing, Riley & Longair 1983). Read More

The Boolardy Engineering Test Array is a 6 x 12 m dish interferometer and the prototype of the Australian Square Kilometre Array Pathfinder (ASKAP), equipped with the first generation of ASKAP's phased array feed (PAF) receivers. These facilitate rapid wide-area imaging via the deployment of simultaneous multiple beams within a 30 square degree field of view. By cycling the array through 12 interleaved pointing positions and using 9 digitally formed beams we effectively mimic a traditional 1 hour x 108 pointing survey, covering 150 square degrees over 711 - 1015 MHz in 12 hours of observing time. Read More

2016Jan
Authors: R. Acciarri, M. A. Acero, M. Adamowski, C. Adams, P. Adamson, S. Adhikari, Z. Ahmad, C. H. Albright, T. Alion, E. Amador, J. Anderson, K. Anderson, C. Andreopoulos, M. Andrews, R. Andrews, I. Anghel, J. d. Anjos, A. Ankowski, M. Antonello, A. ArandaFernandez, A. Ariga, T. Ariga, D. Aristizabal, E. Arrieta-Diaz, K. Aryal, J. Asaadi, D. Asner, M. S. Athar, M. Auger, A. Aurisano, V. Aushev, D. Autiero, M. Avila, J. J. Back, X. Bai, B. Baibussinov, M. Baird, A. B. Balantekin, B. Baller, P. Ballett, B. Bambah, M. Bansal, S. Bansal, G. J. Barker, W. A. Barletta, G. Barr, N. Barros, L. Bartoszek, A. Bashyal, M. Bass, F. Bay, J. Beacom, B. R. Behera, G. Bellettini, V. Bellini, O. Beltramello, P. A. Benetti, A. Bercellie, M. Bergevin, E. Berman, H. Berns, R. Bernstein, S. Bertolucci, B. Bhandari, V. Bhatnagar, B. Bhuyan, J. Bian, K. Biery, M. Bishai, T. Blackburn, A. Blake, F. d. M. Blaszczyk, E. Blaufuss, B. Bleakley, E. Blucher, V. Bocean, F. Boffelli, J. Boissevain, S. Bolognesi, T. Bolton, M. Bonesini, T. Boone, C. Booth, S. Bordoni, M. Borysova, B. Bourguille, S. B. Boyd, D. Brailsford, A. Brandt, J. Bremer, S. Brice, C. Bromberg, G. Brooijmans, G. Brown, R. Brown, G. Brunetti, X. Bu, N. Buchanan, H. Budd, B. Bugg, P. Calafiura, E. Calligarich, E. Calvo, L. Camilleri, M. Campanelli, C. Cantini, B. Carls, R. Carr, M. Cascella, C. Castromonte, E. CatanoMur, F. Cavanna, S. Centro, A. CerveraVillanueva, V. B. Chandratre, A. Chatterjee, S. Chattopadhyay, S. Chattopadhyay, L. Chaussard, S. Chembra, H. Chen, K. Chen, M. Chen, D. Cherdack, C. Chi, S. Childress, S. Choubey, B. C. Choudhary, G. Christodoulou, C. Christofferson, E. Church, D. Cianci, D. Cline, T. Coan, A. Cocco, J. Coelho, P. Cole, G. Collin, J. M. Conrad, M. Convery, R. Corey, L. Corwin, J. Cranshaw, P. Crivelli, D. Cronin-Hennessy, A. Curioni, J. Cushing, D. L. Adams, D. Dale, S. R. Das, T. Davenne, G. S. Davies, J. Davies, J. Dawson, K. De, A. deGouvea, J. K. deJong, P. deJong, P. DeLurgio, M. Decowski, A. Delbart, C. Densham, R. Dharmapalan, N. Dhingra, S. DiLuise, M. Diamantopoulou, J. S. Diaz, G. DiazBautista, M. Diwan, Z. Djurcic, J. Dolph, G. Drake, D. Duchesneau, M. Duvernois, H. Duyang, D. A. Dwyer, S. Dye, S. Dytman, B. Eberly, R. Edgecock, D. Edmunds, S. Elliott, M. Elnimr, S. Emery, E. Endress, S. Eno, A. Ereditato, C. O. Escobar, J. Evans, A. Falcone, L. Falk, A. Farbin, C. Farnese, Y. Farzan, A. Fava, L. Favilli, J. Felde, J. Felix, S. Fernandes, L. Fields, A. Finch, M. Fitton, B. Fleming, T. Forest, J. Fowler, W. Fox, J. Fried, A. Friedland, S. Fuess, B. Fujikawa, A. Gago, H. Gallagher, S. Galymov, T. Gamble, R. Gandhi, D. Garcia-Gamez, S. Gardiner, G. Garvey, V. M. Gehman, A. Gendotti, G. d. Geronimo, C. Ghag, P. Ghoshal, D. Gibin, I. Gil-Botella, R. Gill, D. Girardelli, A. Giri, S. Glavin, D. Goeldi, S. Golapinni, M. Gold, R. A. Gomes, J. J. GomezCadenas, M. C. Goodman, D. Gorbunov, S. Goswami, N. Graf, N. Graf, M. Graham, E. Gramelini, R. Gran, C. Grant, N. Grant, V. Greco, H. Greenlee, L. Greenler, C. Greenley, M. Groh, S. Grullon, T. Grundy, K. Grzelak, E. Guardincerri, V. Guarino, E. Guarnaccia, G. P. Guedes, R. Guenette, A. Guglielmi, A. T. Habig, R. W. Hackenburg, A. Hackenburg, H. Hadavand, R. Haenni, A. Hahn, M. D. Haigh, T. Haines, T. Hamernik, T. Handler, S. Hans, D. Harris, J. Hartnell, T. Hasegawa, R. Hatcher, A. Hatzikoutelis, S. Hays, E. Hazen, M. Headley, A. Heavey, K. Heeger, J. Heise, K. Hennessy, J. Hewes, A. Higuera, T. Hill, A. Himmel, M. Hogan, P. Holanda, A. Holin, W. Honey, S. Horikawa, G. Horton-Smith, B. Howard, J. Howell, P. Hurh, J. Huston, J. Hylen, R. Imlay, J. Insler, G. Introzzi, D. Ioanisyan, A. Ioannisian, K. Iwamoto, A. Izmaylov, C. Jackson, D. E. Jaffe, C. James, E. James, F. Jediny, C. Jen, A. Jhingan, S. Jiménez, J. H. Jo, M. Johnson, R. Johnson, J. Johnstone, B. J. Jones, J. Joshi, H. Jostlein, C. K. Jung, T. Junk, A. Kaboth, R. Kadel, T. Kafka, L. Kalousis, Y. Kamyshkov, G. Karagiorgi, D. Karasavvas, Y. Karyotakis, A. Kaur, P. Kaur, B. Kayser, N. Kazaryan, E. Kearns, P. Keener, S. Kemboi, E. Kemp, S. H. Kettell, M. Khabibullin, M. Khandaker, A. Khotjantsev, B. Kirby, M. Kirby, J. Klein, T. Kobilarcik, S. Kohn, G. Koizumi, A. Kopylov, M. Kordosky, L. Kormos, U. Kose, V. A. Kostelecky, M. Kramer, I. Kreslo, R. Kriske, W. Kropp, Y. Kudenko, V. A. Kudryavtsev, S. Kulagin, A. Kumar, G. K. Kumar, J. Kumar, L. Kumar, T. Kutter, A. Laminack, K. Lande, C. Lane, K. Lang, F. Lanni, J. Learned, P. Lebrun, D. Lee, H. Lee, K. Lee, W. M. Lee, M. A. LeiguideOliveira, Q. Li, S. Li, S. Li, X. Li, Y. Li, Z. Li, J. Libo, C. S. Lin, S. Lin, J. Ling, J. Link, Z. Liptak, D. Lissauer, L. Littenberg, B. Littlejohn, Q. Liu, T. Liu, S. Lockwitz, N. Lockyer, T. Loew, M. Lokajicek, K. Long, M. D. L. Lopes, J. P. Lopez, J. Losecco, W. Louis, J. Lowery, M. Luethi, K. B. Luk, B. Lundberg, T. Lundin, X. Luo, T. Lux, J. Lykken, A. A. Machado, J. R. Macier, S. Magill, G. Mahler, K. Mahn, M. Malek, S. Malhotra, D. Malon, F. Mammoliti, S. Mancina, S. K. Mandal, S. Mandodi, S. L. Manly, A. Mann, A. Marchionni, W. Marciano, C. Mariani, J. Maricic, A. Marino, M. Marshak, C. Marshall, J. Marshall, J. Marteau, J. Martin-Albo, D. Martinez, S. Matsuno, J. Matthews, C. Mauger, K. Mavrokoridis, D. Mayilyan, E. Mazzucato, N. McCauley, E. McCluskey, N. McConkey, K. McDonald, K. S. McFarland, A. M. McGowan, C. McGrew, R. McKeown, D. McNulty, R. McTaggart, A. Mefodiev, M. Mehrian, P. Mehta, D. Mei, O. Mena, S. Menary, H. Mendez, A. Menegolli, G. Meng, Y. Meng, H. Merritt, D. Mertins, M. Messier, W. Metcalf, M. Mewes, H. Meyer, T. Miao, R. Milincic, W. Miller, G. Mills, O. Mineev, O. Miranda, C. S. Mishra, S. R. Mishra, B. Mitrica, D. Mladenov, I. Mocioiu, R. Mohanta, N. Mokhov, C. Montanari, D. Montanari, J. Moon, M. Mooney, C. Moore, J. Morfin, B. Morgan, C. Morris, W. Morse, Z. Moss, C. Mossey, C. A. Moura, J. Mousseau, L. Mualem, M. Muether, S. Mufson, S. Murphy, J. Musser, R. Musser, Y. Nakajima, D. Naples, J. Navarro, D. Navas, J. Nelson, M. Nessi, M. Newcomer, Y. Ng, R. Nichol, T. C. Nicholls, K. Nikolics, E. Niner, B. Norris, F. Noto, P. Novakova, P. Novella, J. Nowak, M. S. Nunes, H. O'Keeffe, R. Oldeman, R. Oliveira, T. Olson, Y. Onishchuk, J. Osta, T. Ovsjannikova, B. Page, S. Pakvasa, S. Pal, O. Palamara, A. Palazzo, J. Paley, C. Palomares, E. Pantic, V. Paolone, V. Papadimitriou, J. Park, S. Parke, Z. Parsa, S. Pascoli, R. Patterson, S. Patton, T. Patzak, B. Paulos, L. Paulucci, Z. Pavlovic, G. Pawloski, S. Peeters, E. Pennacchio, A. Perch, G. N. Perdue, L. Periale, J. D. Perkin, H. Pessard, G. Petrillo, R. Petti, A. Petukhov, F. Pietropaolo, R. Plunkett, S. Pordes, M. Potekhin, R. Potenza, B. Potukuchi, N. Poudyal, O. Prokofiev, N. Pruthi, P. Przewlocki, D. Pushka, X. Qian, J. L. Raaf, R. Raboanary, V. Radeka, A. Radovic, G. Raffelt, I. Rakhno, H. T. Rakotondramanana, L. Rakotondravohitra, Y. A. Ramachers, R. Rameika, J. Ramsey, A. Rappoldi, G. Raselli, P. Ratoff, B. Rebel, C. Regenfus, J. Reichenbacher, D. Reitzner, A. Remoto, A. Renshaw, S. Rescia, M. Richardson, K. Rielage, K. Riesselmann, M. Robinson, L. Rochester, O. B. Rodrigues, P. Rodrigues, B. Roe, M. Rosen, R. M. Roser, M. Ross-Lonergan, M. Rossella, A. Rubbia, C. Rubbia, R. Rucinski, C. RudolphvonRohr, B. Russell, D. Ruterbories, R. Saakyan, N. Sahu, P. Sala, N. Samios, F. Sanchez, M. Sanchez, B. Sands, S. Santana, R. Santorelli, G. Santucci, N. Saoulidou, A. Scaramelli, H. Schellman, P. Schlabach, R. Schmitt, D. Schmitz, J. Schneps, K. Scholberg, A. Schukraft, J. Schwehr, E. Segreto, S. Seibert, J. A. Sepulveda-Quiroz, F. Sergiampietri, L. Sexton-Kennedy, D. Sgalaberna, M. Shaevitz, J. Shahi, S. Shahsavarani, P. Shanahan, S. U. Shankar, R. Sharma, R. K. Sharma, T. Shaw, R. Shrock, I. Shyrma, N. Simos, G. Sinev, I. Singh, J. Singh, J. Singh, V. Singh, G. Sinnis, W. Sippach, D. Smargianaki, M. Smy, E. Snider, P. Snopok, J. Sobczyk, H. Sobel, M. Soderberg, N. Solomey, W. Sondheim, M. Sorel, A. Sousa, K. Soustruznik, J. Spitz, J. Spitz, N. J. Spooner, M. Stancari, I. Stancu, D. Stefan, H. M. Steiner, J. Stewart, J. Stock, S. Stoica, J. Stone, J. Strait, M. Strait, T. Strauss, S. Striganov, R. Sulej, G. Sullivan, Y. Sun, L. Suter, C. M. Sutera, R. Svoboda, B. Szczerbinska, A. Szelc, S. Söldner-Rembold, R. Talaga, M. Tamsett, S. Tariq, E. Tatar, R. Tayloe, C. Taylor, D. Taylor, K. Terao, M. Thiesse, J. Thomas, L. F. Thompson, M. Thomson, C. Thorn, M. Thorpe, X. Tian, D. Tiedt, S. C. Timm, A. Tonazzo, T. Tope, A. Topkar, F. R. Torres, M. Torti, M. Tortola, F. Tortorici, M. Toups, C. Touramanis, M. Tripathi, I. Tropin, Y. Tsai, K. V. Tsang, R. Tsenov, S. Tufanli, C. Tull, J. Turner, M. Tzanov, E. Tziaferi, Y. Uchida, J. Urheim, T. Usher, M. Vagins, P. Vahle, G. A. Valdiviesso, L. Valerio, Z. Vallari, J. Valle, R. VanBerg, R. VandeWater, P. VanGemmeren, F. Varanini, G. Varner, G. Vasseur, K. Vaziri, G. Velev, S. Ventura, A. Verdugo, T. Viant, T. V. Vieira, C. Vignoli, C. Vilela, B. Viren, T. Vrba, T. Wachala, D. Wahl, M. Wallbank, N. Walsh, B. Wang, H. Wang, L. Wang, T. Wang, T. K. Warburton, D. Warner, M. Wascko, D. Waters, T. B. Watson, A. Weber, M. Weber, W. Wei, A. Weinstein, D. Wells, D. Wenman, M. Wetstein, A. White, L. Whitehead, D. Whittington, M. Wilking, J. Willhite, P. Wilson, R. J. Wilson, L. Winslow, P. Wittich, S. Wojcicki, H. H. Wong, K. Wood, E. Worcester, M. Worcester, S. Wu, T. Xin, C. Yanagisawa, S. Yang, T. Yang, K. Yarritu, J. Ye, M. Yeh, N. Yershov, K. Yonehara, B. Yu, J. Yu, J. Zalesak, A. Zalewska, B. Zamorano, L. Zang, A. Zani, A. Zani, G. Zavala, G. Zeller, C. Zhang, C. Zhang, E. D. Zimmerman, M. Zito, R. Zwaska

This document presents the Conceptual Design Report (CDR) put forward by an international neutrino community to pursue the Deep Underground Neutrino Experiment at the Long-Baseline Neutrino Facility (LBNF/DUNE), a groundbreaking science experiment for long-baseline neutrino oscillation studies and for neutrino astrophysics and nucleon decay searches. The DUNE far detector will be a very large modular liquid argon time-projection chamber (LArTPC) located deep underground, coupled to the LBNF multi-megawatt wide-band neutrino beam. DUNE will also have a high-resolution and high-precision near detector. Read More

New data are reported from a second run of the 2-liter PICO-2L C$_3$F$_8$ bubble chamber with a total exposure of 129$\,$kg-days at a thermodynamic threshold energy of 3.3$\,$keV. These data show that measures taken to control particulate contamination in the superheated fluid resulted in the absence of the anomalous background events observed in the first run of this bubble chamber. Read More

2016Jan
Authors: R. Acciarri, M. A. Acero, M. Adamowski, C. Adams, P. Adamson, S. Adhikari, Z. Ahmad, C. H. Albright, T. Alion, E. Amador, J. Anderson, K. Anderson, C. Andreopoulos, M. Andrews, R. Andrews, I. Anghel, J. d. Anjos, A. Ankowski, M. Antonello, A. ArandaFernandez, A. Ariga, T. Ariga, D. Aristizabal, E. Arrieta-Diaz, K. Aryal, J. Asaadi, D. Asner, M. S. Athar, M. Auger, A. Aurisano, V. Aushev, D. Autiero, M. Avila, J. J. Back, X. Bai, B. Baibussinov, M. Baird, A. B. Balantekin, B. Baller, P. Ballett, B. Bambah, M. Bansal, S. Bansal, G. J. Barker, W. A. Barletta, G. Barr, N. Barros, L. Bartoszek, A. Bashyal, M. Bass, F. Bay, J. Beacom, B. R. Behera, G. Bellettini, V. Bellini, O. Beltramello, P. A. Benetti, A. Bercellie, M. Bergevin, E. Berman, H. Berns, R. Bernstein, S. Bertolucci, B. Bhandari, V. Bhatnagar, B. Bhuyan, J. Bian, K. Biery, M. Bishai, T. Blackburn, A. Blake, F. d. M. Blaszczyk, E. Blaufuss, B. Bleakley, E. Blucher, V. Bocean, F. Boffelli, J. Boissevain, S. Bolognesi, T. Bolton, M. Bonesini, T. Boone, C. Booth, S. Bordoni, M. Borysova, B. Bourguille, S. B. Boyd, D. Brailsford, A. Brandt, J. Bremer, S. Brice, C. Bromberg, G. Brooijmans, G. Brown, R. Brown, G. Brunetti, X. Bu, N. Buchanan, H. Budd, B. Bugg, P. Calafiura, E. Calligarich, E. Calvo, L. Camilleri, M. Campanelli, C. Cantini, B. Carls, R. Carr, M. Cascella, C. Castromonte, E. CatanoMur, F. Cavanna, S. Centro, A. CerveraVillanueva, V. B. Chandratre, A. Chatterjee, S. Chattopadhyay, S. Chattopadhyay, L. Chaussard, S. Chembra, H. Chen, K. Chen, M. Chen, D. Cherdack, C. Chi, S. Childress, S. Choubey, B. C. Choudhary, G. Christodoulou, C. Christofferson, E. Church, D. Cianci, D. Cline, T. Coan, A. Cocco, J. Coelho, P. Cole, G. Collin, J. M. Conrad, M. Convery, R. Corey, L. Corwin, J. Cranshaw, P. Crivelli, D. Cronin-Hennessy, A. Curioni, J. Cushing, D. L. Adams, D. Dale, S. R. Das, T. Davenne, G. S. Davies, J. Davies, J. Dawson, K. De, A. deGouvea, J. K. deJong, P. deJong, P. DeLurgio, M. Decowski, A. Delbart, C. Densham, R. Dharmapalan, N. Dhingra, S. DiLuise, M. Diamantopoulou, J. S. Diaz, G. DiazBautista, M. Diwan, Z. Djurcic, J. Dolph, G. Drake, D. Duchesneau, M. Duvernois, H. Duyang, D. A. Dwyer, S. Dye, S. Dytman, B. Eberly, R. Edgecock, D. Edmunds, S. Elliott, M. Elnimr, S. Emery, E. Endress, S. Eno, A. Ereditato, C. O. Escobar, J. Evans, A. Falcone, L. Falk, A. Farbin, C. Farnese, Y. Farzan, A. Fava, L. Favilli, J. Felde, J. Felix, S. Fernandes, L. Fields, A. Finch, M. Fitton, B. Fleming, T. Forest, J. Fowler, W. Fox, J. Fried, A. Friedland, S. Fuess, B. Fujikawa, A. Gago, H. Gallagher, S. Galymov, T. Gamble, R. Gandhi, D. Garcia-Gamez, S. Gardiner, G. Garvey, V. M. Gehman, A. Gendotti, G. d. Geronimo, C. Ghag, P. Ghoshal, D. Gibin, I. Gil-Botella, R. Gill, D. Girardelli, A. Giri, S. Glavin, D. Goeldi, S. Golapinni, M. Gold, R. A. Gomes, J. J. GomezCadenas, M. C. Goodman, D. Gorbunov, S. Goswami, N. Graf, N. Graf, M. Graham, E. Gramelini, R. Gran, C. Grant, N. Grant, V. Greco, H. Greenlee, L. Greenler, C. Greenley, M. Groh, S. Grullon, T. Grundy, K. Grzelak, E. Guardincerri, V. Guarino, E. Guarnaccia, G. P. Guedes, R. Guenette, A. Guglielmi, A. T. Habig, R. W. Hackenburg, A. Hackenburg, H. Hadavand, R. Haenni, A. Hahn, M. D. Haigh, T. Haines, T. Hamernik, T. Handler, S. Hans, D. Harris, J. Hartnell, T. Hasegawa, R. Hatcher, A. Hatzikoutelis, S. Hays, E. Hazen, M. Headley, A. Heavey, K. Heeger, J. Heise, K. Hennessy, J. Hewes, A. Higuera, T. Hill, A. Himmel, M. Hogan, P. Holanda, A. Holin, W. Honey, S. Horikawa, G. Horton-Smith, B. Howard, J. Howell, P. Hurh, J. Huston, J. Hylen, R. Imlay, J. Insler, G. Introzzi, D. Ioanisyan, A. Ioannisian, K. Iwamoto, A. Izmaylov, C. Jackson, D. E. Jaffe, C. James, E. James, F. Jediny, C. Jen, A. Jhingan, S. Jiménez, J. H. Jo, M. Johnson, R. Johnson, J. Johnstone, B. J. Jones, J. Joshi, H. Jostlein, C. K. Jung, T. Junk, A. Kaboth, R. Kadel, T. Kafka, L. Kalousis, Y. Kamyshkov, G. Karagiorgi, D. Karasavvas, Y. Karyotakis, A. Kaur, P. Kaur, B. Kayser, N. Kazaryan, E. Kearns, P. Keener, S. Kemboi, E. Kemp, S. H. Kettell, M. Khabibullin, M. Khandaker, A. Khotjantsev, B. Kirby, M. Kirby, J. Klein, T. Kobilarcik, S. Kohn, G. Koizumi, A. Kopylov, M. Kordosky, L. Kormos, U. Kose, A. Kostelecky, M. Kramer, I. Kreslo, R. Kriske, W. Kropp, Y. Kudenko, V. A. Kudryavtsev, S. Kulagin, A. Kumar, G. Kumar, J. Kumar, L. Kumar, T. Kutter, A. Laminack, K. Lande, C. Lane, K. Lang, F. Lanni, J. Learned, P. Lebrun, D. Lee, H. Lee, K. Lee, W. M. Lee, M. A. LeiguideOliveira, Q. Li, S. Li, S. Li, X. Li, Y. Li, Z. Li, J. Libo, C. S. Lin, S. Lin, J. Ling, J. Link, Z. Liptak, D. Lissauer, L. Littenberg, B. Littlejohn, Q. Liu, T. Liu, S. Lockwitz, N. Lockyer, T. Loew, M. Lokajicek, K. Long, M. D. L. Lopes, J. P. Lopez, J. Losecco, W. Louis, J. Lowery, M. Luethi, K. Luk, B. Lundberg, T. Lundin, X. Luo, T. Lux, J. Lykken, A. A. Machado, J. R. Macier, S. Magill, G. Mahler, K. Mahn, M. Malek, S. Malhotra, D. Malon, F. Mammoliti, S. Mancina, S. K. Mandal, S. Mandodi, S. L. Manly, A. Mann, A. Marchionni, W. Marciano, C. Mariani, J. Maricic, A. Marino, M. Marshak, C. Marshall, J. Marshall, J. Marteau, J. Martin-Albo, D. Martinez, S. Matsuno, J. Matthews, C. Mauger, K. Mavrokoridis, D. Mayilyan, E. Mazzucato, N. McCauley, E. McCluskey, N. McConkey, K. McDonald, K. S. McFarland, A. M. McGowan, C. McGrew, R. McKeown, D. McNulty, R. McTaggart, A. Mefodiev, M. Mehrian, P. Mehta, D. Mei, O. Mena, S. Menary, H. Mendez, A. Menegolli, G. Meng, Y. Meng, H. Merritt, D. Mertins, M. Messier, W. Metcalf, M. Mewes, H. Meyer, T. Miao, R. Milincic, W. Miller, G. Mills, O. Mineev, O. Miranda, C. S. Mishra, S. R. Mishra, B. Mitrica, D. Mladenov, I. Mocioiu, R. Mohanta, N. Mokhov, C. Montanari, D. Montanari, J. Moon, M. Mooney, C. Moore, J. Morfin, B. Morgan, C. Morris, W. Morse, Z. Moss, C. Mossey, C. A. Moura, J. Mousseau, L. Mualem, M. Muether, S. Mufson, S. Murphy, J. Musser, R. Musser, Y. Nakajima, D. Naples, J. Navarro, D. Navas, J. Nelson, M. Nessi, M. Newcomer, Y. Ng, R. Nichol, T. C. Nicholls, K. Nikolics, E. Niner, B. Norris, F. Noto, P. Novakova, P. Novella, J. Nowak, M. S. Nunes, H. O'Keeffe, R. Oldeman, R. Oliveira, T. Olson, Y. Onishchuk, J. Osta, T. Ovsjannikova, B. Page, S. Pakvasa, S. Pal, O. Palamara, A. Palazzo, J. Paley, C. Palomares, E. Pantic, V. Paolone, V. Papadimitriou, J. Park, S. Parke, Z. Parsa, S. Pascoli, R. Patterson, S. Patton, T. Patzak, B. Paulos, L. Paulucci, Z. Pavlovic, G. Pawloski, S. Peeters, E. Pennacchio, A. Perch, G. N. Perdue, L. Periale, J. D. Perkin, H. Pessard, G. Petrillo, R. Petti, A. Petukhov, F. Pietropaolo, R. Plunkett, S. Pordes, M. Potekhin, R. Potenza, B. Potukuchi, N. Poudyal, O. Prokofiev, N. Pruthi, P. Przewlocki, D. Pushka, X. Qian, J. L. Raaf, R. Raboanary, V. Radeka, A. Radovic, G. Raffelt, I. Rakhno, H. T. Rakotondramanana, L. Rakotondravohitra, Y. A. Ramachers, R. Rameika, J. Ramsey, A. Rappoldi, G. Raselli, P. Ratoff, B. Rebel, C. Regenfus, J. Reichenbacher, D. Reitzner, A. Remoto, A. Renshaw, S. Rescia, M. Richardson, K. Rielage, K. Riesselmann, M. Robinson, L. Rochester, O. B. Rodrigues, P. Rodrigues, B. Roe, M. Rosen, R. M. Roser, M. Ross-Lonergan, M. Rossella, A. Rubbia, C. Rubbia, R. Rucinski, C. RudolphvonRohr, B. Russell, D. Ruterbories, R. Saakyan, N. Sahu, P. Sala, N. Samios, F. Sanchez, M. Sanchez, B. Sands, S. Santana, R. Santorelli, G. Santucci, N. Saoulidou, A. Scaramelli, H. Schellman, P. Schlabach, R. Schmitt, D. Schmitz, J. Schneps, K. Scholberg, A. Schukraft, J. Schwehr, E. Segreto, S. Seibert, J. A. Sepulveda-Quiroz, F. Sergiampietri, L. Sexton-Kennedy, D. Sgalaberna, M. Shaevitz, J. Shahi, S. Shahsavarani, P. Shanahan, S. U. Shankar, R. Sharma, R. K. Sharma, T. Shaw, R. Shrock, I. Shyrma, N. Simos, G. Sinev, I. Singh, J. Singh, J. Singh, V. Singh, G. Sinnis, W. Sippach, D. Smargianaki, M. Smy, E. Snider, P. Snopok, J. Sobczyk, H. Sobel, M. Soderberg, N. Solomey, W. Sondheim, M. Sorel, A. Sousa, K. Soustruznik, J. Spitz, N. J. Spooner, M. Stancari, I. Stancu, D. Stefan, H. M. Steiner, J. Stewart, J. Stock, S. Stoica, J. Stone, J. Strait, M. Strait, T. Strauss, S. Striganov, R. Sulej, G. Sullivan, Y. Sun, L. Suter, C. M. Sutera, R. Svoboda, B. Szczerbinska, A. Szelc, S. Söldner-Rembold, R. Talaga, M. Tamsett, S. Tariq, E. Tatar, R. Tayloe, C. Taylor, D. Taylor, K. Terao, M. Thiesse, J. Thomas, L. F. Thompson, M. Thomson, C. Thorn, M. Thorpe, X. Tian, D. Tiedt, S. C. Timm, A. Tonazzo, T. Tope, A. Topkar, F. R. Torres, M. Torti, M. Tortola, F. Tortorici, M. Toups, C. Touramanis, M. Tripathi, I. Tropin, Y. Tsai, K. V. Tsang, R. Tsenov, S. Tufanli, C. Tull, J. Turner, M. Tzanov, E. Tziaferi, Y. Uchida, J. Urheim, T. Usher, M. Vagins, P. Vahle, G. A. Valdiviesso, L. Valerio, Z. Vallari, J. Valle, R. VanBerg, R. VandeWater, P. VanGemmeren, F. Varanini, G. Varner, G. Vasseur, K. Vaziri, G. Velev, S. Ventura, A. Verdugo, T. Viant, T. V. Vieira, C. Vignoli, C. Vilela, B. Viren, T. Vrba, T. Wachala, D. Wahl, M. Wallbank, N. Walsh, B. Wang, H. Wang, L. Wang, T. Wang, T. K. Warburton, D. Warner, M. Wascko, D. Waters, T. B. Watson, A. Weber, M. Weber, W. Wei, A. Weinstein, D. Wells, D. Wenman, M. Wetstein, A. White, L. Whitehead, D. Whittington, M. Wilking, J. Willhite, P. Wilson, R. J. Wilson, L. Winslow, P. Wittich, S. Wojcicki, H. H. Wong, K. Wood, E. Worcester, M. Worcester, S. Wu, T. Xin, C. Yanagisawa, S. Yang, T. Yang, K. Yarritu, J. Ye, M. Yeh, N. Yershov, K. Yonehara, B. Yu, J. Yu, J. Zalesak, A. Zalewska, B. Zamorano, L. Zang, A. Zani, A. Zani, G. Zavala, G. Zeller, C. Zhang, C. Zhang, E. D. Zimmerman, M. Zito, R. Zwaska

A description of the proposed detector(s) for DUNE at LBNF Read More

2015Dec
Authors: DUNE Collaboration, R. Acciarri, M. A. Acero, M. Adamowski, C. Adams, P. Adamson, S. Adhikari, Z. Ahmad, C. H. Albright, T. Alion, E. Amador, J. Anderson, K. Anderson, C. Andreopoulos, M. Andrews, R. Andrews, I. Anghel, J. d. Anjos, A. Ankowski, M. Antonello, A. ArandaFernandez, A. Ariga, T. Ariga, D. Aristizabal, E. Arrieta-Diaz, K. Aryal, J. Asaadi, D. Asner, M. S. Athar, M. Auger, A. Aurisano, V. Aushev, D. Autiero, M. Avila, J. J. Back, X. Bai, B. Baibussinov, M. Baird, A. B. Balantekin, B. Baller, P. Ballett, B. Bambah, M. Bansal, S. Bansal, G. J. Barker, W. A. Barletta, G. Barr, N. Barros, L. Bartoszek, A. Bashyal, M. Bass, F. Bay, J. Beacom, B. R. Behera, G. Bellettini, V. Bellini, O. Beltramello, P. A. Benetti, A. Bercellie, M. Bergevin, E. Berman, H. Berns, R. Bernstein, S. Bertolucci, B. Bhandari, V. Bhatnagar, B. Bhuyan, J. Bian, K. Biery, M. Bishai, T. Blackburn, A. Blake, F. d. M. Blaszczyk, E. Blaufuss, B. Bleakley, E. Blucher, V. Bocean, F. Boffelli, J. Boissevain, S. Bolognesi, T. Bolton, M. Bonesini, T. Boone, C. Booth, S. Bordoni, M. Borysova, B. Bourguille, S. B. Boyd, D. Brailsford, A. Brandt, J. Bremer, S. Brice, C. Bromberg, G. Brooijmans, G. Brown, R. Brown, G. Brunetti, X. Bu, N. Buchanan, H. Budd, B. Bugg, P. Calafiura, E. Calligarich, E. Calvo, L. Camilleri, M. Campanelli, C. Cantini, B. Carls, R. Carr, M. Cascella, C. Castromonte, E. CatanoMur, F. Cavanna, S. Centro, A. CerveraVillanueva, V. B. Chandratre, A. Chatterjee, S. Chattopadhyay, S. Chattopadhyay, L. Chaussard, S. Chembra, H. Chen, K. Chen, M. Chen, D. Cherdack, C. Chi, S. Childress, S. Choubey, B. C. Choudhary, G. Christodoulou, C. Christofferson, E. Church, D. Cianci, D. Cline, T. Coan, A. Cocco, J. Coelho, P. Cole, G. Collin, J. M. Conrad, M. Convery, R. Corey, L. Corwin, J. Cranshaw, P. Crivelli, D. Cronin-Hennessy, A. Curioni, J. Cushing, D. L. Adams, D. Dale, S. R. Das, T. Davenne, G. S. Davies, J. Davies, J. Dawson, K. De, A. deGouvea, J. K. deJong, P. deJong, P. DeLurgio, M. Decowski, A. Delbart, C. Densham, R. Dharmapalan, N. Dhingra, S. DiLuise, M. Diamantopoulou, J. S. Diaz, G. DiazBautista, M. Diwan, Z. Djurcic, J. Dolph, G. Drake, D. Duchesneau, M. Duvernois, H. Duyang, D. A. Dwyer, S. Dye, S. Dytman, B. Eberly, R. Edgecock, D. Edmunds, S. Elliott, M. Elnimr, S. Emery, E. Endress, S. Eno, A. Ereditato, C. O. Escobar, J. Evans, A. Falcone, L. Falk, A. Farbin, C. Farnese, Y. Farzan, A. Fava, L. Favilli, J. Felde, J. Felix, S. Fernandes, L. Fields, A. Finch, M. Fitton, B. Fleming, T. Forest, J. Fowler, W. Fox, J. Fried, A. Friedland, S. Fuess, B. Fujikawa, A. Gago, H. Gallagher, S. Galymov, T. Gamble, R. Gandhi, D. Garcia-Gamez, S. Gardiner, G. Garvey, V. M. Gehman, A. Gendotti, G. d. Geronimo, C. Ghag, P. Ghoshal, D. Gibin, I. Gil-Botella, R. Gill, D. Girardelli, A. Giri, S. Glavin, D. Goeldi, S. Golapinni, M. Gold, R. A. Gomes, J. J. GomezCadenas, M. C. Goodman, D. Gorbunov, S. Goswami, N. Graf, N. Graf, M. Graham, E. Gramelini, R. Gran, C. Grant, N. Grant, V. Greco, H. Greenlee, L. Greenler, C. Greenley, M. Groh, S. Grullon, T. Grundy, K. Grzelak, E. Guardincerri, V. Guarino, E. Guarnaccia, G. P. Guedes, R. Guenette, A. Guglielmi, A. T. Habig, R. W. Hackenburg, A. Hackenburg, H. Hadavand, R. Haenni, A. Hahn, M. D. Haigh, T. Haines, T. Hamernik, T. Handler, S. Hans, D. Harris, J. Hartnell, T. Hasegawa, R. Hatcher, A. Hatzikoutelis, S. Hays, E. Hazen, M. Headley, A. Heavey, K. Heeger, J. Heise, K. Hennessy, J. Hewes, A. Higuera, T. Hill, A. Himmel, M. Hogan, P. Holanda, A. Holin, W. Honey, S. Horikawa, G. Horton-Smith, B. Howard, J. Howell, P. Hurh, J. Huston, J. Hylen, R. Imlay, J. Insler, G. Introzzi, D. Ioanisyan, A. Ioannisian, K. Iwamoto, A. Izmaylov, C. Jackson, D. E. Jaffe, C. James, E. James, F. Jediny, C. Jen, A. Jhingan, S. Jiménez, J. H. Jo, M. Johnson, R. Johnson, J. Johnstone, B. J. Jones, J. Joshi, H. Jostlein, C. K. Jung, T. Junk, A. Kaboth, R. Kadel, T. Kafka, L. Kalousis, Y. Kamyshkov, G. Karagiorgi, D. Karasavvas, Y. Karyotakis, A. Kaur, P. Kaur, B. Kayser, N. Kazaryan, E. Kearns, P. Keener, S. Kemboi, E. Kemp, S. H. Kettell, M. Khabibullin, M. Khandaker, A. Khotjantsev, B. Kirby, M. Kirby, J. Klein, T. Kobilarcik, S. Kohn, G. Koizumi, A. Kopylov, M. Kordosky, L. Kormos, U. Kose, V. A. Kostelecky, M. Kramer, I. Kreslo, R. Kriske, W. Kropp, Y. Kudenko, V. A. Kudryavtsev, S. Kulagin, A. Kumar, G. Kumar, J. Kumar, L. Kumar, T. Kutter, A. Laminack, K. Lande, C. Lane, K. Lang, F. Lanni, J. Learned, P. Lebrun, D. Lee, H. Lee, K. Lee, W. M. Lee, M. A. LeiguideOliveira, Q. Li, S. Li, S. Li, X. Li, Y. Li, Z. Li, J. Libo, C. S. Lin, S. Lin, J. Ling, J. Link, Z. Liptak, D. Lissauer, L. Littenberg, B. Littlejohn, Q. Liu, T. Liu, S. Lockwitz, N. Lockyer, T. Loew, M. Lokajicek, K. Long, M. D. L. Lopes, J. P. Lopez, J. Losecco, W. Louis, J. Lowery, M. Luethi, K. Luk, B. Lundberg, T. Lundin, X. Luo, T. Lux, J. Lykken, A. A. Machado, J. R. Macier, S. Magill, G. Mahler, K. Mahn, M. Malek, S. Malhotra, D. Malon, F. Mammoliti, S. Mancina, S. K. Mandal, S. Mandodi, S. L. Manly, A. Mann, A. Marchionni, W. Marciano, C. Mariani, J. Maricic, A. Marino, M. Marshak, C. Marshall, J. Marshall, J. Marteau, J. Martin-Albo, D. Martinez, S. Matsuno, J. Matthews, C. Mauger, K. Mavrokoridis, D. Mayilyan, E. Mazzucato, N. McCauley, E. McCluskey, N. McConkey, K. McDonald, K. S. McFarland, A. M. McGowan, C. McGrew, R. McKeown, D. McNulty, R. McTaggart, A. Mefodiev, M. Mehrian, P. Mehta, D. Mei, O. Mena, S. Menary, H. Mendez, A. Menegolli, G. Meng, Y. Meng, H. Merritt, D. Mertins, M. Messier, W. Metcalf, M. Mewes, H. Meyer, T. Miao, R. Milincic, W. Miller, G. Mills, O. Mineev, O. Miranda, C. S. Mishra, S. R. Mishra, B. Mitrica, D. Mladenov, I. Mocioiu, R. Mohanta, N. Mokhov, C. Montanari, D. Montanari, J. Moon, M. Mooney, C. Moore, J. Morfin, B. Morgan, C. Morris, W. Morse, Z. Moss, C. Mossey, C. A. Moura, J. Mousseau, L. Mualem, M. Muether, S. Mufson, S. Murphy, J. Musser, R. Musser, Y. Nakajima, D. Naples, J. Navarro, D. Navas, J. Nelson, M. Nessi, M. Newcomer, Y. Ng, R. Nichol, T. C. Nicholls, K. Nikolics, E. Niner, B. Norris, F. Noto, P. Novakova, P. Novella, J. Nowak, M. S. Nunes, H. O'Keeffe, R. Oldeman, R. Oliveira, T. Olson, Y. Onishchuk, J. Osta, T. Ovsjannikova, B. Page, S. Pakvasa, S. Pal, O. Palamara, A. Palazzo, J. Paley, C. Palomares, E. Pantic, V. Paolone, V. Papadimitriou, J. Park, S. Parke, Z. Parsa, S. Pascoli, R. Patterson, S. Patton, T. Patzak, B. Paulos, L. Paulucci, Z. Pavlovic, G. Pawloski, S. Peeters, E. Pennacchio, A. Perch, G. N. Perdue, L. Periale, J. D. Perkin, H. Pessard, G. Petrillo, R. Petti, A. Petukhov, F. Pietropaolo, R. Plunkett, S. Pordes, M. Potekhin, R. Potenza, B. Potukuchi, N. Poudyal, O. Prokofiev, N. Pruthi, P. Przewlocki, D. Pushka, X. Qian, J. L. Raaf, R. Raboanary, V. Radeka, A. Radovic, G. Raffelt, I. Rakhno, H. T. Rakotondramanana, L. Rakotondravohitra, Y. A. Ramachers, R. Rameika, J. Ramsey, A. Rappoldi, G. Raselli, P. Ratoff, B. Rebel, C. Regenfus, J. Reichenbacher, D. Reitzner, A. Remoto, A. Renshaw, S. Rescia, M. Richardson, K. Rielage, K. Riesselmann, M. Robinson, L. Rochester, O. B. Rodrigues, P. Rodrigues, B. Roe, M. Rosen, R. M. Roser, M. Ross-Lonergan, M. Rossella, A. Rubbia, C. Rubbia, R. Rucinski, C. RudolphvonRohr, B. Russell, D. Ruterbories, R. Saakyan, N. Sahu, P. Sala, N. Samios, F. Sanchez, M. Sanchez, B. Sands, S. Santana, R. Santorelli, G. Santucci, N. Saoulidou, A. Scaramelli, H. Schellman, P. Schlabach, R. Schmitt, D. Schmitz, J. Schneps, K. Scholberg, A. Schukraft, J. Schwehr, E. Segreto, S. Seibert, J. A. Sepulveda-Quiroz, F. Sergiampietri, L. Sexton-Kennedy, D. Sgalaberna, M. Shaevitz, J. Shahi, S. Shahsavarani, P. Shanahan, S. U. Shankar, R. Sharma, R. K. Sharma, T. Shaw, R. Shrock, I. Shyrma, N. Simos, G. Sinev, I. Singh, J. Singh, J. Singh, V. Singh, G. Sinnis, W. Sippach, D. Smargianaki, M. Smy, E. Snider, P. Snopok, J. Sobczyk, H. Sobel, M. Soderberg, N. Solomey, W. Sondheim, M. Sorel, A. Sousa, K. Soustruznik, J. Spitz, J. Spitz, N. J. Spooner, M. Stancari, I. Stancu, D. Stefan, H. M. Steiner, J. Stewart, J. Stock, S. Stoica, J. Stone, J. Strait, M. Strait, T. Strauss, S. Striganov, R. Sulej, G. Sullivan, Y. Sun, L. Suter, C. M. Sutera, R. Svoboda, B. Szczerbinska, A. Szelc, S. Söldner-Rembold, R. Talaga, M. Tamsett, S. Tariq, E. Tatar, R. Tayloe, C. Taylor, D. Taylor, K. Terao, M. Thiesse, J. Thomas, L. F. Thompson, M. Thomson, C. Thorn, M. Thorpe, X. Tian, D. Tiedt, S. C. Timm, A. Tonazzo, T. Tope, A. Topkar, F. R. Torres, M. Torti, M. Tortola, F. Tortorici, M. Toups, C. Touramanis, M. Tripathi, I. Tropin, Y. Tsai, K. V. Tsang, R. Tsenov, S. Tufanli, C. Tull, J. Turner, M. Tzanov, E. Tziaferi, Y. Uchida, J. Urheim, T. Usher, M. Vagins, P. Vahle, G. A. Valdiviesso, L. Valerio, Z. Vallari, J. Valle, R. VanBerg, R. VandeWater, P. VanGemmeren, F. Varanini, G. Varner, G. Vasseur, K. Vaziri, G. Velev, S. Ventura, A. Verdugo, T. Viant, T. V. Vieira, C. Vignoli, C. Vilela, B. Viren, T. Vrba, T. Wachala, D. Wahl, M. Wallbank, N. Walsh, B. Wang, H. Wang, L. Wang, T. Wang, T. K. Warburton, D. Warner, M. Wascko, D. Waters, T. B. Watson, A. Weber, M. Weber, W. Wei, A. Weinstein, D. Wells, D. Wenman, M. Wetstein, A. White, L. Whitehead, D. Whittington, M. Wilking, J. Willhite, P. Wilson, R. J. Wilson, L. Winslow, P. Wittich, S. Wojcicki, H. H. Wong, K. Wood, E. Worcester, M. Worcester, S. Wu, T. Xin, C. Yanagisawa, S. Yang, T. Yang, K. Yarritu, J. Ye, M. Yeh, N. Yershov, K. Yonehara, B. Yu, J. Yu, J. Zalesak, A. Zalewska, B. Zamorano, L. Zang, A. Zani, G. Zavala, G. Zeller, C. Zhang, C. Zhang, E. D. Zimmerman, M. Zito, R. Zwaska

The Physics Program for the Deep Underground Neutrino Experiment (DUNE) at the Fermilab Long-Baseline Neutrino Facility (LBNF) is described. Read More

We use observations from the Boolardy Engineering Test Array (BETA) of the Australian Square Kilometre Array Pathfinder (ASKAP) telescope to search for transient radio sources in the field around the intermittent pulsar PSR J1107-5907. The pulsar is thought to switch between an "off" state in which no emission is detectable, a weak state and a strong state. We ran three independent transient detection pipelines on two-minute snapshot images from a 13 hour BETA observation in order to 1) study the emission from the pulsar, 2) search for other transient emission from elsewhere in the image and 3) to compare the results from the different transient detection pipelines. Read More

The authors present a Polynomial Chaos (PC)-based Bayesian inference method for quantifying the uncertainties of the K-Profile Parametrization (KPP) within the MIT General Circulation Model (MITgcm) of the tropical pacific. The inference of the uncertain parameters is based on a Markov Chain Monte Carlo (MCMC) scheme that utilizes a newly formulated test statistic taking into account the different components representing the structures of turbulent mixing on both daily and seasonal timescales in addition to the data quality, and filters for the effects of parameter perturbations over those due to changes in the wind. To avoid the prohibitive computational cost of integrating the MITgcm model at each MCMC iteration, we build a surrogate model for the test statistic using the PC method. Read More

2015Aug
Authors: SNO+ Collaboration1, :2, S. Andringa3, E. Arushanova4, S. Asahi5, M. Askins6, D. J. Auty7, A. R. Back8, Z. Barnard9, N. Barros10, E. W. Beier11, A. Bialek12, S. D. Biller13, E. Blucher14, R. Bonventre15, D. Braid16, E. Caden17, E. Callaghan18, J. Caravaca19, J. Carvalho20, L. Cavalli21, D. Chauhan22, M. Chen23, O. Chkvorets24, K. Clark25, B. Cleveland26, I. T. Coulter27, D. Cressy28, X. Dai29, C. Darrach30, B. Davis-Purcell31, R. Deen32, M. M. Depatie33, F. Descamps34, F. Di Lodovico35, N. Duhaime36, F. Duncan37, J. Dunger38, E. Falk39, N. Fatemighomi40, R. Ford41, P. Gorel42, C. Grant43, S. Grullon44, E. Guillian45, A. L. Hallin46, D. Hallman47, S. Hans48, J. Hartnell49, P. Harvey50, M. Hedayatipour51, W. J. Heintzelman52, R. L. Helmer53, B. Hreljac54, J. Hu55, T. Iida56, C. M. Jackson57, N. A. Jelley58, C. Jillings59, C. Jones60, P. G. Jones61, K. Kamdin62, T. Kaptanoglu63, J. Kaspar64, P. Keener65, P. Khaghani66, L. Kippenbrock67, J. R. Klein68, R. Knapik69, J. N. Kofron70, L. L. Kormos71, S. Korte72, C. Kraus73, C. B. Krauss74, K. Labe75, I. Lam76, C. Lan77, B. J. Land78, S. Langrock79, A. LaTorre80, I. Lawson81, G. M. Lefeuvre82, E. J. Leming83, J. Lidgard84, X. Liu85, Y. Liu86, V. Lozza87, S. Maguire88, A. Maio89, K. Majumdar90, S. Manecki91, J. Maneira92, E. Marzec93, A. Mastbaum94, N. McCauley95, A. B. McDonald96, J. E. McMillan97, P. Mekarski98, C. Miller99, Y. Mohan100, E. Mony101, M. J. Mottram102, V. Novikov103, H. M. O'Keeffe104, E. O'Sullivan105, G. D. Orebi Gann106, M. J. Parnell107, S. J. M. Peeters108, T. Pershing109, Z. Petriw110, G. Prior111, J. C. Prouty112, S. Quirk113, A. Reichold114, A. Robertson115, J. Rose116, R. Rosero117, P. M. Rost118, J. Rumleskie119, M. A. Schumaker120, M. H. Schwendener121, D. Scislowski122, J. Secrest123, M. Seddighin124, L. Segui125, S. Seibert126, T. Shantz127, T. M. Shokair128, L. Sibley129, J. R. Sinclair130, K. Singh131, P. Skensved132, A. Soerensen133, T. Sonley134, R. Stainforth135, M. Strait136, M. I. Stringer137, R. Svoboda138, J. Tatar139, L. Tian140, N. Tolich141, J. Tseng142, H. W. C. Tseung143, R. Van Berg144, E. Vázquez-Jáuregui145, C. Virtue146, B. von Krosigk147, J. M. G. Walker148, M. Walker149, O. Wasalski150, J. Waterfield151, R. F. White152, J. R. Wilson153, T. J. Winchester154, A. Wright155, M. Yeh156, T. Zhao157, K. Zuber158
Affiliations: 1Laboratório de Instrumentaçao e Física Experimental de Partículas, 2Laboratório de Instrumentaçao e Física Experimental de Partículas, 3Laboratório de Instrumentaçao e Física Experimental de Partículas, 4Queen Mary, University of London, School of Physics and Astronomy, London, UK, 5Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 6University of California, Davis, CA, USA, 7University of Alberta, Department of Physics, Edmonton, AB, Canada, 8Queen Mary, University of London, School of Physics and Astronomy, London, UK, 9Laurentian University, Sudbury, ON, Canada, 10Laboratório de Instrumentaçao e Física Experimental de Partículas, 11University of Pennsylvania, Department of Physics and Astronomy, Philadelphia, PA, USA, 12University of Alberta, Department of Physics, Edmonton, AB, Canada, 13University of Oxford, The Denys Wilkinson Building, Oxford, UK, 14The Enrico Fermi Institute and Department of Physics, The University of Chicago, Chicago, IL, USA, 15University of Pennsylvania, Department of Physics and Astronomy, Philadelphia, PA, USA, 16Laurentian University, Sudbury, ON, Canada, 17Laurentian University, Sudbury, ON, Canada, 18University of Pennsylvania, Department of Physics and Astronomy, Philadelphia, PA, USA, 19University of California, Department of Physics, Berkeley, CA, USA, 20Universidade de Coimbra, Laboratório de Instrumentaçao e Física Experimental de Partículas and Departamento de Física, Coimbra, Portugal, 21University of Oxford, The Denys Wilkinson Building, Oxford, UK, 22Laboratório de Instrumentaçao e Física Experimental de Partículas, 23Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 24Laurentian University, Sudbury, ON, Canada, 25Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 26Laurentian University, Sudbury, ON, Canada, 27University of Pennsylvania, Department of Physics and Astronomy, Philadelphia, PA, USA, 28Laurentian University, Sudbury, ON, Canada, 29Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 30Laurentian University, Sudbury, ON, Canada, 31TRIUMF, Vancouver, BC, Canada, 32University of Pennsylvania, Department of Physics and Astronomy, Philadelphia, PA, USA, 33Laurentian University, Sudbury, ON, Canada, 34University of California, Department of Physics, Berkeley, CA, USA, 35Queen Mary, University of London, School of Physics and Astronomy, London, UK, 36Laurentian University, Sudbury, ON, Canada, 37Laurentian University, Sudbury, ON, Canada, 38University of Oxford, The Denys Wilkinson Building, Oxford, UK, 39University of Sussex, Physics and Astronomy, Falmer, Brighton, UK, 40Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 41Laurentian University, Sudbury, ON, Canada, 42University of Alberta, Department of Physics, Edmonton, AB, Canada, 43University of California, Davis, CA, USA, 44University of Pennsylvania, Department of Physics and Astronomy, Philadelphia, PA, USA, 45Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 46University of Alberta, Department of Physics, Edmonton, AB, Canada, 47Laurentian University, Sudbury, ON, Canada, 48Brookhaven National Laboratory, Chemistry Department, Upton, NY, USA, 49University of Sussex, Physics and Astronomy, Falmer, Brighton, UK, 50Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 51University of Alberta, Department of Physics, Edmonton, AB, Canada, 52University of Pennsylvania, Department of Physics and Astronomy, Philadelphia, PA, USA, 53TRIUMF, Vancouver, BC, Canada, 54Laurentian University, Sudbury, ON, Canada, 55University of Alberta, Department of Physics, Edmonton, AB, Canada, 56Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 57University of California, Department of Physics, Berkeley, CA, USA, 58University of Oxford, The Denys Wilkinson Building, Oxford, UK, 59Laurentian University, Sudbury, ON, Canada, 60University of Oxford, The Denys Wilkinson Building, Oxford, UK, 61Queen Mary, University of London, School of Physics and Astronomy, London, UK, 62University of California, Department of Physics, Berkeley, CA, USA, 63University of Pennsylvania, Department of Physics and Astronomy, Philadelphia, PA, USA, 64University of Washington, Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, Seattle, WA, USA, 65University of Pennsylvania, Department of Physics and Astronomy, Philadelphia, PA, USA, 66Laurentian University, Sudbury, ON, Canada, 67University of Washington, Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, Seattle, WA, USA, 68University of Pennsylvania, Department of Physics and Astronomy, Philadelphia, PA, USA, 69University of Pennsylvania, Department of Physics and Astronomy, Philadelphia, PA, USA, 70University of Washington, Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, Seattle, WA, USA, 71Lancaster University, Physics Department, Lancaster, UK, 72Laurentian University, Sudbury, ON, Canada, 73Laurentian University, Sudbury, ON, Canada, 74University of Alberta, Department of Physics, Edmonton, AB, Canada, 75The Enrico Fermi Institute and Department of Physics, The University of Chicago, Chicago, IL, USA, 76Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 77Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 78University of California, Department of Physics, Berkeley, CA, USA, 79Queen Mary, University of London, School of Physics and Astronomy, London, UK, 80The Enrico Fermi Institute and Department of Physics, The University of Chicago, Chicago, IL, USA, 81Laurentian University, Sudbury, ON, Canada, 82University of Sussex, Physics and Astronomy, Falmer, Brighton, UK, 83University of Sussex, Physics and Astronomy, Falmer, Brighton, UK, 84University of Oxford, The Denys Wilkinson Building, Oxford, UK, 85Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 86Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 87Technische Universität Dresden, Institut für Kern- und Teilchenphysik, Dresden, Germany, 88Brookhaven National Laboratory, Chemistry Department, Upton, NY, USA, 89Laboratório de Instrumentaçao e Física Experimental de Partículas, 90University of Oxford, The Denys Wilkinson Building, Oxford, UK, 91Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 92Laboratório de Instrumentaçao e Física Experimental de Partículas, 93University of Pennsylvania, Department of Physics and Astronomy, Philadelphia, PA, USA, 94University of Pennsylvania, Department of Physics and Astronomy, Philadelphia, PA, USA, 95University of Liverpool, Department of Physics, Liverpool, UK, 96Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 97University of Sheffield, Department of Physics and Astronomy, Sheffield, UK, 98University of Alberta, Department of Physics, Edmonton, AB, Canada, 99Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 100University of Pennsylvania, Department of Physics and Astronomy, Philadelphia, PA, USA, 101Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 102Queen Mary, University of London, School of Physics and Astronomy, London, UK, 103Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 104Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 105Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 106University of Pennsylvania, Department of Physics and Astronomy, Philadelphia, PA, USA, 107Lancaster University, Physics Department, Lancaster, UK, 108University of Sussex, Physics and Astronomy, Falmer, Brighton, UK, 109University of California, Davis, CA, USA, 110University of Alberta, Department of Physics, Edmonton, AB, Canada, 111Laboratório de Instrumentaçao e Física Experimental de Partículas, 112University of California, Department of Physics, Berkeley, CA, USA, 113Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 114University of Oxford, The Denys Wilkinson Building, Oxford, UK, 115University of Liverpool, Department of Physics, Liverpool, UK, 116University of Liverpool, Department of Physics, Liverpool, UK, 117Brookhaven National Laboratory, Chemistry Department, Upton, NY, USA, 118Laurentian University, Sudbury, ON, Canada, 119Laurentian University, Sudbury, ON, Canada, 120Laurentian University, Sudbury, ON, Canada, 121Laurentian University, Sudbury, ON, Canada, 122University of Washington, Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, Seattle, WA, USA, 123Armstrong Atlantic State University, Savannah, GA, USA, 124Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 125University of Oxford, The Denys Wilkinson Building, Oxford, UK, 126University of Pennsylvania, Department of Physics and Astronomy, Philadelphia, PA, USA, 127Laurentian University, Sudbury, ON, Canada, 128University of Pennsylvania, Department of Physics and Astronomy, Philadelphia, PA, USA, 129University of Alberta, Department of Physics, Edmonton, AB, Canada, 130University of Sussex, Physics and Astronomy, Falmer, Brighton, UK, 131University of Alberta, Department of Physics, Edmonton, AB, Canada, 132Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 133Technische Universität Dresden, Institut für Kern- und Teilchenphysik, Dresden, Germany, 134Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 135University of Liverpool, Department of Physics, Liverpool, UK, 136The Enrico Fermi Institute and Department of Physics, The University of Chicago, Chicago, IL, USA, 137University of Sussex, Physics and Astronomy, Falmer, Brighton, UK, 138University of California, Davis, CA, USA, 139University of Washington, Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, Seattle, WA, USA, 140Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 141University of Washington, Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, Seattle, WA, USA, 142University of Oxford, The Denys Wilkinson Building, Oxford, UK, 143University of Washington, Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, Seattle, WA, USA, 144University of Pennsylvania, Department of Physics and Astronomy, Philadelphia, PA, USA, 145SNOLAB, Sudbury, ON, Canada, 146Laurentian University, Sudbury, ON, Canada, 147Technische Universität Dresden, Institut für Kern- und Teilchenphysik, Dresden, Germany, 148University of Liverpool, Department of Physics, Liverpool, UK, 149Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 150TRIUMF, Vancouver, BC, Canada, 151University of Sussex, Physics and Astronomy, Falmer, Brighton, UK, 152University of Sussex, Physics and Astronomy, Falmer, Brighton, UK, 153Queen Mary, University of London, School of Physics and Astronomy, London, UK, 154University of Washington, Center for Experimental Nuclear Physics and Astrophysics, and Department of Physics, Seattle, WA, USA, 155Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 156Brookhaven National Laboratory, Chemistry Department, Upton, NY, USA, 157Queen's University, Department of Physics, Engineering Physics and Astronomy, Kingston, ON, Canada, 158Technische Universität Dresden, Institut für Kern- und Teilchenphysik, Dresden, Germany

SNO+ is a large liquid scintillator-based experiment located 2km underground at SNOLAB, Sudbury, Canada. It reuses the Sudbury Neutrino Observatory detector, consisting of a 12m diameter acrylic vessel which will be filled with about 780 tonnes of ultra-pure liquid scintillator. Designed as a multipurpose neutrino experiment, the primary goal of SNO+ is a search for the neutrinoless double-beta decay (0$\nu\beta\beta$) of 130Te. Read More

Whereas in standard quantum state tomography one estimates an unknown state by performing various measurements with known devices, and whereas in detector tomography one estimates the POVM elements of a measurement device by subjecting to it various known states, we consider here the case of SPAM (state preparation and measurement) tomography where neither the states nor the measurement device are assumed known. For $d$-dimensional systems measured by $d$-outcome detectors, we find there are at most $d^2(d^2-1)$ "gauge" parameters that can never be determined by any such experiment, irrespective of the number of unknown states and unknown devices. For the case $d=2$ we find new gauge-invariant quantities that can be accessed directly experimentally and that can be used to detect and describe SPAM errors. Read More

The funnel plot is a graphical visualisation of summary data estimates from a meta-analysis, and is a useful tool for detecting departures from the standard modelling assumptions. Although perhaps not widely appreciated, a simple extension of the funnel plot can help to facilitate an intuitive interpretation of the mathematics underlying a meta-analysis at a more fundamental level, by equating it to determining the centre of mass of a physical system. We used this analogy, with some success, to explain the concepts of weighing evidence and of biased evidence to a young audience at the Cambridge Science Festival, without recourse to precise definitions or statistical formulae. Read More

For certain conditions of layer thickness, the interface between GdTiO$_3$ (GTO) and SrTiO$_3$ (STO) in multilayer samples has been found to form a two-dimensional electron gas (2DEG) with very interesting properties including high mobilities and ferromagnetism. We have here studied two trilayer samples of the form [2 nm GTO/1.0 or 1. Read More

The interfaces between two condensed phases often exhibit emergent physical properties that can lead to new physics and novel device applications, and are the subject of intense study in many disciplines. We here apply novel experimental and theoretical techniques to the characterization of one such interesting interface system: the two-dimensional electron gas (2DEG) formed in multilayers consisting of SrTiO$_3$ (STO) and GdTiO$_3$ (GTO). This system has been the subject of multiple studies recently and shown to exhibit very high carrier charge densities and ferromagnetic effects, among other intriguing properties. Read More

We present HI imaging of the galaxy group IC 1459 carried out with six antennas of the Australian SKA Pathfinder equipped with phased-array feeds. We detect and resolve HI in eleven galaxies down to a column density of $\sim10^{20}$ cm$^{-2}$ inside a ~6 deg$^2$ field and with a resolution of ~1 arcmin on the sky and ~8 km/s in velocity. We present HI images, velocity fields and integrated spectra of all detections, and highlight the discovery of three HI clouds -- two in the proximity of the galaxy IC 5270 and one close to NGC 7418. Read More

GLEAM, the GaLactic and Extragalactic All-sky MWA survey, is a survey of the entire radio sky south of declination +25 deg at frequencies between 72 and 231 MHz, made with the Murchison Widefield Array (MWA) using a drift scan method that makes efficient use of the MWA's very large field-of-view. We present the observation details, imaging strategies and theoretical sensitivity for GLEAM. The survey ran for two years, the first year using 40 kHz frequency resolution and 0. Read More

2015Apr

The Dark Energy Camera is a new imager with a 2.2-degree diameter field of view mounted at the prime focus of the Victor M. Blanco 4-meter telescope on Cerro Tololo near La Serena, Chile. Read More

This report describes the 2014 study by the Science Definition Team (SDT) of the Wide-Field Infrared Survey Telescope (WFIRST) mission. It is a space observatory that will address the most compelling scientific problems in dark energy, exoplanets and general astrophysics using a 2.4-m telescope with a wide-field infrared instrument and an optical coronagraph. Read More

We report the discovery of a new 21-cm HI absorption system using commissioning data from the Boolardy Engineering Test Array of the Australian Square Kilometre Array Pathfinder (ASKAP). Using the 711.5 - 1015. Read More

We give an overview of complementarity and synergy in cosmology between the Square Kilometre Array and future survey projects in other wavelengths. In the SKA era, precision cosmology will be limited by systematic errors and cosmic variance, rather than statistical errors. However, combining and/or cross-correlating multi-wavelength data, from the SKA to the cosmic microwave background, optical/infrared and X-ray, substantially reduce these limiting factors. Read More

Astronomy at or below the 'survey threshold' has expanded significantly since the publication of the original 'Science with the Square Kilometer Array' in 1999 and its update in 2004. The techniques in this regime may be broadly (but far from exclusively) defined as 'confusion' or 'P(D)' analyses (analyses of one-point statistics), and 'stacking', accounting for the flux-density distribution of noise-limited images co-added at the positions of objects detected/isolated in a different waveband. Here we discuss the relevant issues, present some examples of recent analyses, and consider some of the consequences for the design and use of surveys with the SKA and its pathfinders. Read More

Radio-loud AGN (>10^{22} W/Hz at 1.4 GHz) will be the dominant bright source population detected with the SKA. The high resolution that the SKA will provide even in wide-area surveys will mean that, for the first time sensitive, multi-frequency total intensity and polarisation imaging of large samples of radio-loud active galactic nuclei (AGN) will become available. Read More

This paper describes the system architecture of a newly constructed radio telescope - the Boolardy Engineering Test Array, which is a prototype of the Australian Square Kilometre Array Pathfinder telescope. Phased array feed technology is used to form multiple simultaneous beams per antenna, providing astronomers with unprecedented survey speed. The test array described here is a 6-antenna interferometer, fitted with prototype signal processing hardware capable of forming at least 9 dual-polarisation beams simultaneously, allowing several square degrees to be imaged in a single pointed observation. Read More

After the extraordinary discovery of the Higgs boson at the LHC, the next goal is to pin down its underlying dynamics by measuring the Higgs self-couplings, along with its couplings to gauge and matter particles. As a prototype model of new physics in the scalar sector, we consider the Two Higgs Doublet Model (2HDM) with CP-conservation, and evaluate the prospects for measuring the trilinear scalar couplings among the CP-even Higgs bosons $h$ and $H$ ($\lambda^{hhh}$, $\lambda^{hhH}$, $\lambda^{hHH}$) at LHC14. The continuum and resonant production of CP-even Higgs boson pairs, $hh$ and $hH$, offer complementary probes of the scalar potential away from the light-Higgs decoupling limit. Read More

We advocate a search for an extended scalar sector at the LHC via $hh$ production, where $h$ is the 125 GeV Higgs boson. A resonance feature in the $hh$ invariant mass is a smoking gun of an $s$-channel heavy Higgs resonance, $H$. With one $h$ decaying to two photons and the other decaying to $b$-quarks, the resonant signal may be discoverable above the $hh$ continuum background for $M_H<$ 1 TeV. Read More

We consider a simplified model of fermionic dark matter which couples exclusively to the right-handed top quark via a renormalizable interaction with a color-charged scalar. We first compute the relic abundance of this type of dark matter and investigate constraints placed on the model parameter space by the latest direct detection data. We also perform a detailed analysis for the production of dark matter at the LHC for this model. Read More

The electrical and structural characteristics of SmTiO3/SrTiO3/SmTiO3 and GdTiO3/SrTiO3/GdTiO3 heterostructures are compared. Both types of structures contain narrow SrTiO3 quantum wells, which accommodate a confined, high-density electron gas. As shown previously [Phys. Read More

We simulate the measurement of the triscalar Higgs coupling at LHC(8,14) via pair production of h(125 GeV). We find that the most promising hh final state is bb gamma gamma. We account for deviations of the triscalar coupling from its SM value and study the effects of this coupling on the hh cross-section and distributions with cut-based and multivariate methods. Read More

We investigate the angular dependence of the magnetoresistance of thin (< 1 nm), metallic SrTiO3 quantum wells epitaxially embedded in insulating, ferrimagnetic GdTiO3 and insulating, antiferromagnetic SmTiO3, respectively. The SrTiO3 quantum wells contain a high density of mobile electrons (~7x10^14 cm^-2). We show that the longitudinal and transverse magnetoresistance in the structures with GdTiO3 are consistent with anisotropic magnetoresistance, and thus indicative of induced ferromagnetism in the SrTiO3, rather than a nonequilibrium proximity effect. Read More

To encourage users to use stronger and more secure passwords, modern web browsers offer users password management services, allowing users to save previously entered passwords locally onto their hard drives. We present Lupin, a tool that automatically extracts these saved passwords without the user's knowledge. Lupin allows a network adversary to obtain passwords as long as the login form appears on a non-HTTPS page. Read More

In its Vision and Strategy for Software for Science, Engineering, and Education the NSF states that it will invest in activities that: "Recognize that software strategies must include the secure and reliable deployment and operation of services, for example by campuses or national facilities or industry, where identity, authentication, authorization and assurance are crucial operational capabilities." and "Result in high-quality, usable, secure, vulnerability-free, sustainable, robust, well-tested, and maintainable/evolvable software; and which promotes the sustainability of solid and useful on-going investments." Such statements evidence that security should indeed be a first-class consideration of the software ecosystem. Read More

Cation displacements, oxygen octahedral tilts, and magnetism of epitaxial, ferrimagnetic, insulating GdTiO3 films sandwiched between cubic SrTiO3 layers are studied using scanning transmission electron microscopy and magnetization measurements. With decreasing GdTiO3 film thickness, structural (GdFeO3-type) distortions are reduced, concomitant with a reduction in the Curie temperature. Ferromagnetism persists to smaller deviations from the cubic perovskite structure than is the case for the bulk rare earth titanates. Read More

2013Jul
Authors: LBNE Collaboration, Corey Adams1, David Adams2, Tarek Akiri3, Tyler Alion4, Kris Anderson5, Costas Andreopoulos6, Mike Andrews7, Ioana Anghel8, João Carlos Costa dos Anjos9, Maddalena Antonello10, Enrique Arrieta-Diaz11, Marina Artuso12, Jonathan Asaadi13, Xinhua Bai14, Bagdat Baibussinov15, Michael Baird16, Baha Balantekin17, Bruce Baller18, Brian Baptista19, D'Ann Barker20, Gary Barker21, William A. Barletta22, Giles Barr23, Larry Bartoszek24, Amit Bashyal25, Matt Bass26, Vincenzo Bellini27, Pietro Angelo Benetti28, Bruce E. Berger29, Marc Bergevin30, Eileen Berman31, Hans-Gerd Berns32, Adam Bernstein33, Robert Bernstein34, Babu Bhandari35, Vipin Bhatnagar36, Bipul Bhuyan37, Jianming Bian38, Mary Bishai39, Andrew Blake40, Flor Blaszczyk41, Erik Blaufuss42, Bruce Bleakley43, Edward Blucher44, Steve Blusk45, Virgil Bocean46, F. Boffelli47, Jan Boissevain48, Timothy Bolton49, Maurizio Bonesini50, Steve Boyd51, Andrew Brandt52, Richard Breedon53, Carl Bromberg54, Ralph Brown55, Giullia Brunetti56, Norman Buchanan57, Bill Bugg58, Jerome Busenitz59, E. Calligarich60, Leslie Camilleri61, Giada Carminati62, Rachel Carr63, Cesar Castromonte64, Flavio Cavanna65, Sandro Centro66, Alex Chen67, Hucheng Chen68, Kai Chen69, Daniel Cherdack70, Cheng-Yi Chi71, Sam Childress72, Brajesh Chandra Choudhary73, Georgios Christodoulou74, Cabot-Ann Christofferson75, Eric Church76, David Cline77, Thomas Coan78, Alfredo Cocco79, Joao Coelho80, Stephen Coleman81, Janet M. Conrad82, Mark Convery83, Robert Corey84, Luke Corwin85, Jack Cranshaw86, Daniel Cronin-Hennessy87, A. Curioni88, Helio da Motta89, Tristan Davenne90, Gavin S. Davies91, Steven Dazeley92, Kaushik De93, Andre de Gouvea94, Jeffrey K. de Jong95, David Demuth96, Chris Densham97, Milind Diwan98, Zelimir Djurcic99, R. Dolfini100, Jeffrey Dolph101, Gary Drake102, Stephen Dye103, Hongue Dyuang104, Daniel Edmunds105, Steven Elliott106, Muhammad Elnimr107, Sarah Eno108, Sanshiro Enomoto109, Carlos O. Escobar110, Justin Evans111, A. Falcone112, Lisa Falk113, Amir Farbin114, Christian Farnese115, Angela Fava116, John Felde117, S. Fernandes118, Fernando Ferroni119, Farshid Feyzi120, Laura Fields121, Alex Finch122, Mike Fitton123, Bonnie Fleming124, Jack Fowler125, Walt Fox126, Alex Friedland127, Stu Fuess128, Brian Fujikawa129, Hugh Gallagher130, Raj Gandhi131, Gerald Garvey132, Victor M. Gehman133, Gianluigi de Geronimo134, Daniele Gibin135, Ronald Gill136, Ricardo A. Gomes137, Maury C. Goodman138, Jason Goon139, Nicholas Graf140, Mathew Graham141, Rik Gran142, Christopher Grant143, Nick Grant144, Herbert Greenlee145, Leland Greenler146, Sean Grullon147, Elena Guardincerri148, Victor Guarino149, Evan Guarnaccia150, Germano Guedes151, Roxanne Guenette152, Alberto Guglielmi153, Marcelo M. Guzzo154, Alec T. Habig155, Robert W. Hackenburg156, Haleh Hadavand157, Alan Hahn158, Martin Haigh159, Todd Haines160, Thomas Handler161, Sunej Hans162, Jeff Hartnell163, John Harton164, Robert Hatcher165, Athans Hatzikoutelis166, Steven Hays167, Eric Hazen168, Mike Headley169, Anne Heavey170, Karsten Heeger171, Jaret Heise172, Robert Hellauer173, Jeremy Hewes174, Alexander Himmel175, Matthew Hogan176, Pedro Holanda177, Anna Holin178, Glenn Horton-Smith179, Joe Howell180, Patrick Hurh181, Joey Huston182, James Hylen183, Richard Imlay184, Jonathan Insler185, G. Introzzi186, Zeynep Isvan187, Chris Jackson188, John Jacobsen189, David E. Jaffe190, Cat James191, Chun-Min Jen192, Marvin Johnson193, Randy Johnson194, Robert Johnson195, Scott Johnson196, William Johnston197, John Johnstone198, Ben J. P. Jones199, H. Jostlein200, Thomas Junk201, Richard Kadel202, Karl Kaess203, Georgia Karagiorgi204, Jarek Kaspar205, Teppei Katori206, Boris Kayser207, Edward Kearns208, Paul Keener209, Ernesto Kemp210, Steve H. Kettell211, Mike Kirby212, Joshua Klein213, Gordon Koizumi214, Sacha Kopp215, Laura Kormos216, William Kropp217, Vitaly A. Kudryavtsev218, Ashok Kumar219, Jason Kumar220, Thomas Kutter221, Franco La Zia222, Kenneth Lande223, Charles Lane224, Karol Lang225, Francesco Lanni226, Richard Lanza227, Tony Latorre228, John Learned229, David Lee230, Kevin Lee231, Qizhong Li232, Shaorui Li233, Yichen Li234, Zepeng Li235, Jiang Libo236, Steve Linden237, Jiajie Ling238, Jonathan Link239, Laurence Littenberg240, Hu Liu241, Qiuguang Liu242, Tiankuan Liu243, John Losecco244, William Louis245, Byron Lundberg246, Tracy Lundin247, Jay Lundy248, Ana Amelia Machado249, Cara Maesano250, Steve Magill251, George Mahler252, David Malon253, Stephen Malys254, Francesco Mammoliti255, Samit Kumar Mandal256, Anthony Mann257, Paul Mantsch258, Alberto Marchionni259, William Marciano260, Camillo Mariani261, Jelena Maricic262, Alysia Marino263, Marvin Marshak264, John Marshall265, Shiegenobu Matsuno266, Christopher Mauger267, Konstantinos Mavrokoridis268, Nate Mayer269, Neil McCauley270, Elaine McCluskey271, Kirk McDonald272, Kevin McFarland273, David McKee274, Robert McKeown275, Robert McTaggart276, Rashid Mehdiyev277, Dongming Mei278, A. Menegolli279, Guang Meng280, Yixiong Meng281, David Mertins282, Mark Messier283, William Metcalf284, Radovan Milincic285, William Miller286, Geoff Mills287, Sanjib R. Mishra288, Nikolai Mokhov289, Claudio Montanari290, David Montanari291, Craig Moore292, Jorge Morfin293, Ben Morgan294, William Morse295, Zander Moss296, Célio A. Moura297, Stuart Mufson298, David Muller299, Jim Musser300, Donna Naples301, Jim Napolitano302, Mitch Newcomer303, Ryan Nichol304, Tim Nicholls305, Evan Niner306, Barry Norris307, Jaroslaw Nowak308, Helen O'Keeffe309, Roberto Oliveira310, Travis Olson311, Brian Page312, Sandip Pakvasa313, Ornella Palamara314, Jon Paley315, Vittorio Paolone316, Vaia Papadimitriou317, Seongtae Park318, Zohreh Parsa319, Kinga Partyka320, Bob Paulos321, Zarko Pavlovic322, Simon Peeters323, Andy Perch324, Jon D. Perkin325, Roberto Petti326, Andre Petukhov327, Francesco Pietropaolo328, Robert Plunkett329, Chris Polly330, Stephen Pordes331, Maxim Potekhin332, Renato Potenza333, Arati Prakash334, Oleg Prokofiev335, Xin Qian336, Jennifer L. Raaf337, Veljko Radeka338, Igor Rakhno339, Yorck Ramachers340, Regina Rameika341, John Ramsey342, A. Rappoldi343, G. L. Raselli344, Peter Ratoff345, Shreyas Ravindra346, Brian Rebel347, Juergen Reichenbacher348, Dianne Reitzner349, Sergio Rescia350, Martin Richardson351, Kieth Rielage352, Kurt Riesselmann353, Matt Robinson354, Leon Rochester355, Michael Ronquest356, Marc Rosen357, M. Rossella358, Carlo Rubbia359, Russ Rucinski360, Sandeep Sahijpal361, Himansu Sahoo362, Paola Sala363, Delia Salmiera364, Nicholas Samios365, Mayly Sanchez366, Alberto Scaramelli367, Heidi Schellman368, Richard Schmitt369, David Schmitz370, Jack Schneps371, Kate Scholberg372, Ettore Segreto373, Stanley Seibert374, Liz Sexton-Kennedy375, Mike Shaevitz376, Peter Shanahan377, Rahul Sharma378, Terri Shaw379, Nikolaos Simos380, Venktesh Singh381, Gus Sinnis382, William Sippach383, Tomasz Skwarnicki384, Michael Smy385, Henry Sobel386, Mitch Soderberg387, John Sondericker388, Walter Sondheim389, Alexandre Sousa390, Neil J. C. Spooner391, Michelle Stancari392, Ion Stancu393, Dorota Stefan394, Andy Stefanik395, James Stewart396, Sheldon Stone397, James Strait398, Matthew Strait399, Sergei Striganov400, Gregory Sullivan401, Yujing Sun402, Louise Suter403, Andrew Svenson404, Robert Svoboda405, Barbara Szczerbinska406, Andrzej Szelc407, Matthew Szydagis408, Stefan Söldner-Rembold409, Richard Talaga410, Matthew Tamsett411, Salman Tariq412, Rex Tayloe413, Charles Taylor414, David Taylor415, Artin Teymourian416, Harry Themann417, Matthew Thiesse418, Jenny Thomas419, Lee F. Thompson420, Mark Thomson421, Craig Thorn422, Matt Thorpe423, Xinchun Tian424, Doug Tiedt425, Walter Toki426, Nikolai Tolich427, M. Torti428, Matt Toups429, Christos Touramanis430, Mani Tripathi431, Igor Tropin432, Yun-Tse Tsai433, Craig Tull434, Martin Tzanov435, Jon Urheim436, Shawn Usman437, Mark Vagins438, Gustavo Valdiviesso439, Rick Van Berg440, Richard Van de Water441, Peter Van Gemmeren442, Filippo Varanini443, Gary Varner444, Kamran Vaziri445, Gueorgui Velev446, Sandro Ventura447, Chiara Vignoli448, Brett Viren449, Dan Wahl450, Abby Waldron451, Christopher W. Walter452, Hanguo Wang453, Wei Wang454, Karl Warburton455, David Warner456, Ryan Wasserman457, Blake Watson458, Alfons Weber459, Wenzhao Wei460, Douglas Wells461, Matthew Wetstein462, Andy White463, Hywel White464, Lisa Whitehead465, Denver Whittington466, Joshua Willhite467, Robert J. Wilson468, Lindley Winslow469, Kevin Wood470, Elizabeth Worcester471, Matthew Worcester472, Tian Xin473, Kevin Yarritu474, Jingbo Ye475, Minfang Yeh476, Bo Yu477, Jae Yu478, Tianlu Yuan479, A. Zani480, Geralyn P. Zeller481, Chao Zhang482, Chao Zhang483, Eric D. Zimmerman484, Robert Zwaska485
Affiliations: 1Yale University, 2Brookhaven National Lab, 3Duke University, 4Univ. of South Carolina, 5Fermi National Accelerator Lab, 6Univ. of Liverpool, 7Fermi National Accelerator Lab, 8Iowa State University, 9Centro Brasileiro de Pesquisas Físicas, 10Laboratori Nazionali del Gran Sasso, 11Michigan State University, 12Syracuse University, 13Syracuse University, 14South Dakota School of Mines and Technology, 15Univ. of Padova, 16Indiana University, 17Univ. of Wisconsin, 18Fermi National Accelerator Lab, 19Indiana University, 20Univ. of South Dakota, 21Univ. of Warwick, 22Massachusetts Institute of Technology, 23Univ. of Oxford, 24Los Alamos National Laboratory, 25Univ. of Texas, 26Colorado State University, 27Univ. di Catania, 28Univ. of Pavia, INFN Sezione di Pavia, 29Colorado State University, 30Univ. of California, 31Fermi National Accelerator Lab, 32Univ. of California, 33Lawrence Livermore National Lab, 34Fermi National Accelerator Lab, 35Univ. of Houston, 36Panjab University, 37Indian Institute of Technology Guwahati, 38Univ. of Minnesota, 39Brookhaven National Lab, 40Univ. of Cambridge, 41Louisiana State University, 42Univ. of Maryland, 43South Dakota State University, 44Univ. of Chicago, 45Syracuse University, 46Fermi National Accelerator Lab, 47Univ. of Pavia, INFN Sezione di Pavia, 48Los Alamos National Laboratory, 49Kansas State University, 50Univ. of Milano and INFN Sezione di Milano Bicocca, 51Univ. of Warwick, 52Univ. of Texas, 53Univ. of California, 54Michigan State University, 55Brookhaven National Lab, 56Fermi National Accelerator Lab, 57Colorado State University, 58Univ. of Tennessee, 59Univ. of Alabama, 60Univ. of Pavia, INFN Sezione di Pavia, 61Columbia University, 62Univ. of California, 63Columbia University, 64Univ. Federal de Goias, 65Yale University, 66Univ. of Padova, 67Fermi National Accelerator Lab, 68Brookhaven National Lab, 69Brookhaven National Lab, 70Colorado State University, 71Columbia University, 72Fermi National Accelerator Lab, 73Univ. of Delhi, 74Univ. of Liverpool, 75South Dakota School of Mines and Technology, 76Yale University, 77Univ. of California, 78Southern Methodist University, 79Univ. di Napoli, 80Tufts University, 81Univ. of Colorado, 82Massachusetts Institute of Technology, 83SLAC National Acceleratory Laboratory, 84South Dakota School of Mines and Technology, 85South Dakota School of Mines and Technology, 86Argonne National Lab, 87Univ. of Minnesota, 88Univ. of Milano and INFN Sezione di Milano Bicocca, 89Centro Brasileiro de Pesquisas Físicas, 90STFC Rutherford Appleton Laboratory, 91Iowa State University, 92Lawrence Livermore National Lab, 93Univ. of Texas, 94Northwestern University, 95Univ. of Oxford, 96Univ. of Minnesota, 97STFC Rutherford Appleton Laboratory, 98Brookhaven National Lab, 99Argonne National Lab, 100Univ. of Pavia, INFN Sezione di Pavia, 101Brookhaven National Lab, 102Argonne National Lab, 103Univ. of Hawaii, 104Univ. of South Carolina, 105Michigan State University, 106Los Alamos National Laboratory, 107Univ. of Alabama, 108Univ. of Maryland, 109Univ. of Washington, 110Fermi National Accelerator Lab, 111Univ. of Manchester, 112Univ. of Pavia, INFN Sezione di Pavia, 113Univ. of Sussex, 114Univ. of Texas, 115Univ. of Padova, 116Univ. of Padova, 117Univ. of Maryland, 118Univ. of Alabama, 119Univ. of Pavia, INFN Sezione di Pavia, 120Univ. of Wisconsin, 121Northwestern University, 122Lancaster University, 123STFC Rutherford Appleton Laboratory, 124Yale University, 125Duke University, 126Indiana University, 127Los Alamos National Laboratory, 128Fermi National Accelerator Lab, 129Lawrence Berkeley National Lab, 130Tufts University, 131Harish-Chandra Research Institute, 132Los Alamos National Laboratory, 133Lawrence Berkeley National Lab, 134Brookhaven National Lab, 135Univ. of Padova, 136Brookhaven National Lab, 137Univ. Federal de Goias, 138Argonne National Lab, 139Univ. of South Dakota, 140Univ. of Pittsburgh, 141SLAC National Acceleratory Laboratory, 142Univ. of Minnesota, 143Univ. of California, 144Lancaster University, 145Fermi National Accelerator Lab, 146Univ. of Wisconsin, 147Univ. of Pennsylvania, 148Los Alamos National Laboratory, 149Argonne National Lab, 150Virginia Tech, 151Univ. Estadual de Feira de Santana, 152Yale University, 153Univ. of Padova, 154Univ. de Campinas, 155Univ. of Minnesota, 156Brookhaven National Lab, 157Univ. of Texas, 158Fermi National Accelerator Lab, 159Univ. of Warwick, 160Los Alamos National Laboratory, 161Univ. of Tennessee, 162Brookhaven National Lab, 163Univ. of Sussex, 164Colorado State University, 165Fermi National Accelerator Lab, 166Univ. of Tennessee, 167Fermi National Accelerator Lab, 168Boston University, 169South Dakota Science and Technology Authority, 170Fermi National Accelerator Lab, 171Yale University, 172South Dakota Science and Technology Authority, 173Univ. of Maryland, 174Univ. of Manchester, 175Duke University, 176Colorado State University, 177Univ. de Campinas, 178University College London, 179Kansas State University, 180Fermi National Accelerator Lab, 181Fermi National Accelerator Lab, 182Michigan State University, 183Fermi National Accelerator Lab, 184Louisiana State University, 185Louisiana State University, 186Univ. of Pavia, INFN Sezione di Pavia, 187Brookhaven National Lab, 188Univ. of Texas, 189Univ. of Maryland, 190Brookhaven National Lab, 191Fermi National Accelerator Lab, 192Virginia Tech, 193Fermi National Accelerator Lab, 194Univ. of Cincinnati, 195Univ. of Colorado, 196Univ. of Colorado, 197Colorado State University, 198Fermi National Accelerator Lab, 199Massachusetts Institute of Technology, 200Fermi National Accelerator Lab, 201Fermi National Accelerator Lab, 202Lawrence Berkeley National Lab, 203Univ. of Minnesota, 204Columbia University, 205Univ. of Washington, 206Massachusetts Institute of Technology, 207Fermi National Accelerator Lab, 208Boston University, 209Univ. of Pennsylvania, 210Univ. de Campinas, 211Brookhaven National Lab, 212Fermi National Accelerator Lab, 213Univ. of Pennsylvania, 214Fermi National Accelerator Lab, 215Univ. of Texas, 216Lancaster University, 217Univ. of California, 218Univ. of Sheffield, 219Panjab University, 220Univ. of Hawaii, 221Louisiana State University, 222Univ. di Catania, 223Univ. of Pennsylvania, 224Drexel University, 225Univ. of Texas, 226Brookhaven National Lab, 227Massachusetts Institute of Technology, 228Univ. of Pennsylvania, 229Univ. of Hawaii, 230Los Alamos National Laboratory, 231Univ. of California, 232Fermi National Accelerator Lab, 233Brookhaven National Lab, 234Brookhaven National Lab, 235Duke University, 236Univ. of South Carolina, 237Boston University, 238Brookhaven National Lab, 239Virginia Tech, 240Brookhaven National Lab, 241Univ. of Houston, 242Los Alamos National Laboratory, 243Southern Methodist University, 244Univ. of Notre Dame, 245Los Alamos National Laboratory, 246Fermi National Accelerator Lab, 247Fermi National Accelerator Lab, 248Univ. of Texas, 249INFN, Laboratori Nazionali del Gran Sasso, 250Univ. of California, 251Argonne National Lab, 252Brookhaven National Lab, 253Argonne National Lab, 254National Geospatial-Intelligence Agency, 255Univ. di Catania, 256Univ. of Delhi, 257Tufts University, 258Fermi National Accelerator Lab, 259Fermi National Accelerator Lab, 260Brookhaven National Lab, 261Virginia Tech, 262Univ. of Hawaii, 263Univ. of Colorado, 264Univ. of Minnesota, 265Univ. of Cambridge, 266Univ. of Hawaii, 267Los Alamos National Laboratory, 268Univ. of Liverpool, 269Tufts University, 270Univ. of Liverpool, 271Fermi National Accelerator Lab, 272Princeton University, 273Univ. of Rochester, 274Kansas State University, 275College of William and Mary, 276South Dakota State University, 277Univ. of Texas, 278Univ. of South Dakota, 279Univ. of Pavia, INFN Sezione di Pavia, 280Univ. of Padova, 281Univ. of California, 282Univ. of Alabama, 283Indiana University, 284Louisiana State University, 285Univ. of Hawaii, 286Univ. of Minnesota, 287Los Alamos National Laboratory, 288Univ. of South Carolina, 289Fermi National Accelerator Lab, 290Univ. of Pavia, INFN Sezione di Pavia, 291Fermi National Accelerator Lab, 292Fermi National Accelerator Lab, 293Fermi National Accelerator Lab, 294Univ. of Warwick, 295Brookhaven National Lab, 296Massachusetts Institute of Technology, 297ABC Federal University, 298Indiana University, 299SLAC National Acceleratory Laboratory, 300Indiana University, 301Univ. of Pittsburgh, 302Rensselaer Polytechnic Inst, 303Univ. of Pennsylvania, 304University College London, 305STFC Rutherford Appleton Laboratory, 306Indiana University, 307Fermi National Accelerator Lab, 308Lancaster University, 309Lancaster University, 310Univ. de Campinas, 311Tufts University, 312Michigan State University, 313Univ. of Hawaii, 314Yale University, 315Argonne National Lab, 316Univ. of Pittsburgh, 317Fermi National Accelerator Lab, 318Univ. of Texas, 319Brookhaven National Lab, 320Yale University, 321Univ. of Wisconsin, 322Los Alamos National Laboratory, 323Univ. of Sussex, 324University College London, 325Univ. of Sheffield, 326Univ. of South Carolina, 327South Dakota School of Mines and Technology, 328Univ. of Padova, 329Fermi National Accelerator Lab, 330Fermi National Accelerator Lab, 331Fermi National Accelerator Lab, 332Brookhaven National Lab, 333Univ. di Catania, 334Massachusetts Institute of Technology, 335Fermi National Accelerator Lab, 336Brookhaven National Lab, 337Fermi National Accelerator Lab, 338Brookhaven National Lab, 339Fermi National Accelerator Lab, 340Univ. of Warwick, 341Fermi National Accelerator Lab, 342Los Alamos National Laboratory, 343Univ. of Pavia, INFN Sezione di Pavia, 344Univ. of Pavia, INFN Sezione di Pavia, 345Lancaster University, 346Univ. of Texas, 347Fermi National Accelerator Lab, 348Univ. of Alabama, 349Fermi National Accelerator Lab, 350Brookhaven National Lab, 351Univ. of Sheffield, 352Los Alamos National Laboratory, 353Fermi National Accelerator Lab, 354Univ. of Sheffield, 355SLAC National Acceleratory Laboratory, 356Los Alamos National Laboratory, 357Univ. of Hawaii, 358Univ. of Pavia, INFN Sezione di Pavia, 359INFN, Laboratori Nazionali del Gran Sasso, 360Fermi National Accelerator Lab, 361Panjab University, 362Argonne National Lab, 363Univ. di Milano, 364Univ. of Pavia, INFN Sezione di Pavia, 365Brookhaven National Lab, 366Iowa State University, 367Univ. di Milano, 368Northwestern University, 369Fermi National Accelerator Lab, 370Univ. of Chicago, 371Tufts University, 372Duke University, 373Laboratori Nazionali del Gran Sasso, 374Univ. of Pennsylvania, 375Fermi National Accelerator Lab, 376Columbia University, 377Fermi National Accelerator Lab, 378Brookhaven National Lab, 379Fermi National Accelerator Lab, 380Brookhaven National Lab, 381Banaras Hindu University, 382Los Alamos National Laboratory, 383Columbia University, 384Syracuse University, 385Univ. of California, 386Univ. of California, 387Syracuse University, 388Brookhaven National Lab, 389Los Alamos National Laboratory, 390Univ. of Cincinnati, 391Univ. of Sheffield, 392Fermi National Accelerator Lab, 393Univ. of Alabama, 394Laboratori Nazionali del Gran Sasso, 395Fermi National Accelerator Lab, 396Brookhaven National Lab, 397Syracuse University, 398Fermi National Accelerator Lab, 399Univ. of Chicago, 400Fermi National Accelerator Lab, 401Univ. of Maryland, 402Univ. of Hawaii, 403Argonne National Lab, 404Univ. of South Carolina, 405Univ. of California, 406Dakota State University, 407Yale University, 408Univ. of California, 409Univ. of Manchester, 410Argonne National Lab, 411Univ. of Sussex, 412Fermi National Accelerator Lab, 413Indiana University, 414Los Alamos National Laboratory, 415South Dakota Science and Technology Authority, 416Univ. of California, 417Brookhaven National Lab, 418Univ. of Sheffield, 419University College London, 420Univ. of Sheffield, 421Univ. of Cambridge, 422Brookhaven National Lab, 423STFC Rutherford Appleton Laboratory, 424Univ. of South Carolina, 425South Dakota School of Mines and Technology, 426Colorado State University, 427Univ. of Washington, 428Univ. of Pavia, INFN Sezione di Pavia, 429Massachusetts Institute of Technology, 430Univ. of Liverpool, 431Univ. of California, 432Fermi National Accelerator Lab, 433SLAC National Acceleratory Laboratory, 434Lawrence Berkeley National Lab, 435Louisiana State University, 436Indiana University, 437National Geospatial-Intelligence Agency, 438Kavli IPMU, Univ. of Tokyo, 439Univ. Federal de Alfenas em Poços de Caldas, 440Univ. of Pennsylvania, 441Los Alamos National Laboratory, 442Argonne National Lab, 443Univ. of Padova, 444Univ. of Hawaii, 445Fermi National Accelerator Lab, 446Fermi National Accelerator Lab, 447Univ. of Padova, 448Laboratori Nazionali del Gran Sasso, 449Brookhaven National Lab, 450Univ. of Wisconsin, 451Univ. of Sussex, 452Duke University, 453Univ. of California, 454College of William and Mary, 455Univ. of Sheffield, 456Colorado State University, 457Colorado State University, 458Univ. of Texas, 459Univ. of Oxford, 460Univ. of South Dakota, 461South Dakota School of Mines and Technology, 462Univ. of Chicago, 463Univ. of Texas, 464Los Alamos National Laboratory, 465Univ. of Houston, 466Indiana University, 467South Dakota Science and Technology Authority, 468Colorado State University, 469Univ. of California, 470Univ. of South Carolina, 471Brookhaven National Lab, 472Brookhaven National Lab, 473Iowa State University, 474Los Alamos National Laboratory, 475Southern Methodist University, 476Brookhaven National Lab, 477Brookhaven National Lab, 478Univ. of Texas, 479Univ. of Colorado, 480Univ. of Pavia, INFN Sezione di Pavia, 481Fermi National Accelerator Lab, 482Brookhaven National Lab, 483Brookhaven National Lab, 484Univ. of Colorado, 485Fermi National Accelerator Lab

The preponderance of matter over antimatter in the early Universe, the dynamics of the supernova bursts that produced the heavy elements necessary for life and whether protons eventually decay --- these mysteries at the forefront of particle physics and astrophysics are key to understanding the early evolution of our Universe, its current state and its eventual fate. The Long-Baseline Neutrino Experiment (LBNE) represents an extensively developed plan for a world-class experiment dedicated to addressing these questions. LBNE is conceived around three central components: (1) a new, high-intensity neutrino source generated from a megawatt-class proton accelerator at Fermi National Accelerator Laboratory, (2) a near neutrino detector just downstream of the source, and (3) a massive liquid argon time-projection chamber deployed as a far detector deep underground at the Sanford Underground Research Facility. Read More

The Astro2010 Decadal Survey recommended a Wide Field Infrared Survey Telescope (WFIRST) as its top priority for a new large space mission. As conceived by the decadal survey, WFIRST would carry out a dark energy science program, a microlensing program to determine the demographics of exoplanets, and a general observing program utilizing its ultra wide field. In October 2012, NASA chartered a Science Definition Team (SDT) to produce, in collaboration with the WFIRST Project Office at GSFC and the Program Office at JPL, a Design Reference Mission (DRM) for an implementation of WFIRST using one of the 2. Read More

The Astro2010 Decadal Survey recommended a Wide Field Infrared Survey Telescope (WFIRST) as its top priority for a new large space mission. The report of the WFIRST-AFTA Science Definition Team (SDT) presents a Design Reference Mission for WFIRST that employs one of the 2.4-m, Hubble-quality mirror assemblies recently made available to NASA. Read More

As direct and indirect dark matter detection experiments continue to place stringent constraints on WIMP masses and couplings, it becomes imperative to expand the scope of the search for particle dark matter by looking in new and exotic places. One such place may be the core of active galactic nuclei where the density of dark matter is expected to be extremely high. Recently, several groups have explored the possibility of observing signals of dark matter from its interactions with the high-energy jets emanating from these galaxies. Read More

Lines in the energy spectrum of gamma rays are a fascinating experimental signal, which are often considered "smoking gun" evidence of dark matter annihilation. The current generation of gamma ray observatories are currently closing in on parameter space of great interest in the context of dark matter which is a thermal relic. We consider theories in which the dark matter's primary connection to the Standard Model is via the top quark, realizing strong gamma ray lines consistent with a thermal relic through the forbidden channel mechanism proposed in the Higgs in Space Model. Read More