S. Munir - APCTP, Pohang & Uppsala University

S. Munir
Are you S. Munir?

Claim your profile, edit publications, add additional information:

Contact Details

Name
S. Munir
Affiliation
APCTP, Pohang & Uppsala University
Location

Pubs By Year

Pub Categories

 
High Energy Physics - Phenomenology (33)
 
High Energy Physics - Experiment (7)
 
Cosmology and Nongalactic Astrophysics (1)

Publications Authored By S. Munir

2016Oct
Authors: D. de Florian1, C. Grojean2, F. Maltoni3, C. Mariotti4, A. Nikitenko5, M. Pieri6, P. Savard7, M. Schumacher8, R. Tanaka9, R. Aggleton10, M. Ahmad11, B. Allanach12, C. Anastasiou13, W. Astill14, S. Badger15, M. Badziak16, J. Baglio17, E. Bagnaschi18, A. Ballestrero19, A. Banfi20, D. Barducci21, M. Beckingham22, C. Becot23, G. Bélanger24, J. Bellm25, N. Belyaev26, F. U. Bernlochner27, C. Beskidt28, A. Biekötter29, F. Bishara30, W. Bizon31, N. E. Bomark32, M. Bonvini33, S. Borowka34, V. Bortolotto35, S. Boselli36, F. J. Botella37, R. Boughezal38, G. C. Branco39, J. Brehmer40, L. Brenner41, S. Bressler42, I. Brivio43, A. Broggio44, H. Brun45, G. Buchalla46, C. D. Burgard47, A. Calandri48, L. Caminada49, R. Caminal Armadans50, F. Campanario51, J. Campbell52, F. Caola53, C. M. Carloni Calame54, S. Carrazza55, A. Carvalho56, M. Casolino57, O. Cata58, A. Celis59, F. Cerutti60, N. Chanon61, M. Chen62, X. Chen63, B. Chokoufé Nejad64, N. Christensen65, M. Ciuchini66, R. Contino67, T. Corbett68, D. Curtin69, M. Dall'Osso70, A. David71, S. Dawson72, J. de Blas73, W. de Boer74, P. de Castro Manzano75, C. Degrande76, R. L. Delgado77, F. Demartin78, A. Denner79, B. Di Micco80, R. Di Nardo81, S. Dittmaier82, A. Dobado83, T. Dorigo84, F. A. Dreyer85, M. Dührssen86, C. Duhr87, F. Dulat88, K. Ecker89, K. Ellis90, U. Ellwanger91, C. Englert92, D. Espriu93, A. Falkowski94, L. Fayard95, R. Feger96, G. Ferrera97, A. Ferroglia98, N. Fidanza99, T. Figy100, M. Flechl101, D. Fontes102, S. Forte103, P. Francavilla104, E. Franco105, R. Frederix106, A. Freitas107, F. F. Freitas108, F. Frensch109, S. Frixione110, B. Fuks111, E. Furlan112, S. Gadatsch113, J. Gao114, Y. Gao115, M. V. Garzelli116, T. Gehrmann117, R. Gerosa118, M. Ghezzi119, D. Ghosh120, S. Gieseke121, D. Gillberg122, G. F. Giudice123, E. W. N. Glover124, F. Goertz125, D. Gonçalves126, J. Gonzalez-Fraile127, M. Gorbahn128, S. Gori129, C. A. Gottardo130, M. Gouzevitch131, P. Govoni132, D. Gray133, M. Grazzini134, N. Greiner135, A. Greljo136, J. Grigo137, A. V. Gritsan138, R. Gröber139, S. Guindon140, H. E. Haber141, C. Han142, T. Han143, R. Harlander144, M. A. Harrendorf145, H. B. Hartanto146, C. Hays147, S. Heinemeyer148, G. Heinrich149, M. Herrero150, F. Herzog151, B. Hespel152, V. Hirschi153, S. Hoeche154, S. Honeywell155, S. J. Huber156, C. Hugonie157, J. Huston158, A. Ilnicka159, G. Isidori160, B. Jäger161, M. Jaquier162, S. P. Jones163, A. Juste164, S. Kallweit165, A. Kaluza166, A. Kardos167, A. Karlberg168, Z. Kassabov169, N. Kauer170, D. I. Kazakov171, M. Kerner172, W. Kilian173, F. Kling174, K. Köneke175, R. Kogler176, R. Konoplich177, S. Kortner178, S. Kraml179, C. Krause180, F. Krauss181, M. Krawczyk182, A. Kulesza183, S. Kuttimalai184, R. Lane185, A. Lazopoulos186, G. Lee187, P. Lenzi188, I. M. Lewis189, Y. Li190, S. Liebler191, J. Lindert192, X. Liu193, Z. Liu194, F. J. Llanes-Estrada195, H. E. Logan196, D. Lopez-Val197, I. Low198, G. Luisoni199, P. Maierhöfer200, E. Maina201, B. Mansoulié202, H. Mantler203, M. Mantoani204, A. C. Marini205, V. I. Martinez Outschoorn206, S. Marzani207, D. Marzocca208, A. Massironi209, K. Mawatari210, J. Mazzitelli211, A. McCarn212, B. Mellado213, K. Melnikov214, S. B. Menari215, L. Merlo216, C. Meyer217, P. Milenovic218, K. Mimasu219, S. Mishima220, B. Mistlberger221, S. -O. Moch222, A. Mohammadi223, P. F. Monni224, G. Montagna225, M. Moreno Llácer226, N. Moretti227, S. Moretti228, L. Motyka229, A. Mück230, M. Mühlleitner231, S. Munir232, P. Musella233, P. Nadolsky234, D. Napoletano235, M. Nebot236, C. Neu237, M. Neubert238, R. Nevzorov239, O. Nicrosini240, J. Nielsen241, K. Nikolopoulos242, J. M. No243, C. O'Brien244, T. Ohl245, C. Oleari246, T. Orimoto247, D. Pagani248, C. E. Pandini249, A. Papaefstathiou250, A. S. Papanastasiou251, G. Passarino252, B. D. Pecjak253, M. Pelliccioni254, G. Perez255, L. Perrozzi256, F. Petriello257, G. Petrucciani258, E. Pianori259, F. Piccinini260, M. Pierini261, A. Pilkington262, S. Plätzer263, T. Plehn264, R. Podskubka265, C. T. Potter266, S. Pozzorini267, K. Prokofiev268, A. Pukhov269, I. Puljak270, M. Queitsch-Maitland271, J. Quevillon272, D. Rathlev273, M. Rauch274, E. Re275, M. N. Rebelo276, D. Rebuzzi277, L. Reina278, C. Reuschle279, J. Reuter280, M. Riembau281, F. Riva282, A. Rizzi283, T. Robens284, R. Röntsch285, J. Rojo286, J. C. Romão287, N. Rompotis288, J. Roskes289, R. Roth290, G. P. Salam291, R. Salerno292, R. Santos293, V. Sanz294, J. J. Sanz-Cillero295, H. Sargsyan296, U. Sarica297, P. Schichtel298, J. Schlenk299, T. Schmidt300, C. Schmitt301, M. Schönherr302, U. Schubert303, M. Schulze304, S. Sekula305, M. Sekulla306, E. Shabalina307, H. S. Shao308, J. Shelton309, C. H. Shepherd-Themistocleous310, S. Y. Shim311, F. Siegert312, A. Signer313, J. P. Silva314, L. Silvestrini315, M. Sjodahl316, P. Slavich317, M. Slawinska318, L. Soffi319, M. Spannowsky320, C. Speckner321, D. M. Sperka322, M. Spira323, O. Stål324, F. Staub325, T. Stebel326, T. Stefaniak327, M. Steinhauser328, I. W. Stewart329, M. J. Strassler330, J. Streicher331, D. M. Strom332, S. Su333, X. Sun334, F. J. Tackmann335, K. Tackmann336, A. M. Teixeira337, R. Teixeira de Lima338, V. Theeuwes339, R. Thorne340, D. Tommasini341, P. Torrielli342, M. Tosi343, F. Tramontano344, Z. Trócsányi345, M. Trott346, I. Tsinikos347, M. Ubiali348, P. Vanlaer349, W. Verkerke350, A. Vicini351, L. Viliani352, E. Vryonidou353, D. Wackeroth354, C. E. M. Wagner355, J. Wang356, S. Wayand357, G. Weiglein358, C. Weiss359, M. Wiesemann360, C. Williams361, J. Winter362, D. Winterbottom363, R. Wolf364, M. Xiao365, L. L. Yang366, R. Yohay367, S. P. Y. Yuen368, G. Zanderighi369, M. Zaro370, D. Zeppenfeld371, R. Ziegler372, T. Zirke373, J. Zupan374
Affiliations: 1eds., 2eds., 3eds., 4eds., 5eds., 6eds., 7eds., 8eds., 9eds., 10The LHC Higgs Cross Section Working Group, 11The LHC Higgs Cross Section Working Group, 12The LHC Higgs Cross Section Working Group, 13The LHC Higgs Cross Section Working Group, 14The LHC Higgs Cross Section Working Group, 15The LHC Higgs Cross Section Working Group, 16The LHC Higgs Cross Section Working Group, 17The LHC Higgs Cross Section Working Group, 18The LHC Higgs Cross Section Working Group, 19The LHC Higgs Cross Section Working Group, 20The LHC Higgs Cross Section Working Group, 21The LHC Higgs Cross Section Working Group, 22The LHC Higgs Cross Section Working Group, 23The LHC Higgs Cross Section Working Group, 24The LHC Higgs Cross Section Working Group, 25The LHC Higgs Cross Section Working Group, 26The LHC Higgs Cross Section Working Group, 27The LHC Higgs Cross Section Working Group, 28The LHC Higgs Cross Section Working Group, 29The LHC Higgs Cross Section Working Group, 30The LHC Higgs Cross Section Working Group, 31The LHC Higgs Cross Section Working Group, 32The LHC Higgs Cross Section Working Group, 33The LHC Higgs Cross Section Working Group, 34The LHC Higgs Cross Section Working Group, 35The LHC Higgs Cross Section Working Group, 36The LHC Higgs Cross Section Working Group, 37The LHC Higgs Cross Section Working Group, 38The LHC Higgs Cross Section Working Group, 39The LHC Higgs Cross Section Working Group, 40The LHC Higgs Cross Section Working Group, 41The LHC Higgs Cross Section Working Group, 42The LHC Higgs Cross Section Working Group, 43The LHC Higgs Cross Section Working Group, 44The LHC Higgs Cross Section Working Group, 45The LHC Higgs Cross Section Working Group, 46The LHC Higgs Cross Section Working Group, 47The LHC Higgs Cross Section Working Group, 48The LHC Higgs Cross Section Working Group, 49The LHC Higgs Cross Section Working Group, 50The LHC Higgs Cross Section Working Group, 51The LHC Higgs Cross Section Working Group, 52The LHC Higgs Cross Section Working Group, 53The LHC Higgs Cross Section Working Group, 54The LHC Higgs Cross Section Working Group, 55The LHC Higgs Cross Section Working Group, 56The LHC Higgs Cross Section Working Group, 57The LHC Higgs Cross Section Working Group, 58The LHC Higgs Cross Section Working Group, 59The LHC Higgs Cross Section Working Group, 60The LHC Higgs Cross Section Working Group, 61The LHC Higgs Cross Section Working Group, 62The LHC Higgs Cross Section Working Group, 63The LHC Higgs Cross Section Working Group, 64The LHC Higgs Cross Section Working Group, 65The LHC Higgs Cross Section Working Group, 66The LHC Higgs Cross Section Working Group, 67The LHC Higgs Cross Section Working Group, 68The LHC Higgs Cross Section Working Group, 69The LHC Higgs Cross Section Working Group, 70The LHC Higgs Cross Section Working Group, 71The LHC Higgs Cross Section Working Group, 72The LHC Higgs Cross Section Working Group, 73The LHC Higgs Cross Section Working Group, 74The LHC Higgs Cross Section Working Group, 75The LHC Higgs Cross Section Working Group, 76The LHC Higgs Cross Section Working Group, 77The LHC Higgs Cross Section Working Group, 78The LHC Higgs Cross Section Working Group, 79The LHC Higgs Cross Section Working Group, 80The LHC Higgs Cross Section Working Group, 81The LHC Higgs Cross Section Working Group, 82The LHC Higgs Cross Section Working Group, 83The LHC Higgs Cross Section Working Group, 84The LHC Higgs Cross Section Working Group, 85The LHC Higgs Cross Section Working Group, 86The LHC Higgs Cross Section Working Group, 87The LHC Higgs Cross Section Working Group, 88The LHC Higgs Cross Section Working Group, 89The LHC Higgs Cross Section Working Group, 90The LHC Higgs Cross Section Working Group, 91The LHC Higgs Cross Section Working Group, 92The LHC Higgs Cross Section Working Group, 93The LHC Higgs Cross Section Working Group, 94The LHC Higgs Cross Section Working Group, 95The LHC Higgs Cross Section Working Group, 96The LHC Higgs Cross Section Working Group, 97The LHC Higgs Cross Section Working Group, 98The LHC Higgs Cross Section Working Group, 99The LHC Higgs Cross Section Working Group, 100The LHC Higgs Cross Section Working Group, 101The LHC Higgs Cross Section Working Group, 102The LHC Higgs Cross Section Working Group, 103The LHC Higgs Cross Section Working Group, 104The LHC Higgs Cross Section Working Group, 105The LHC Higgs Cross Section Working Group, 106The LHC Higgs Cross Section Working Group, 107The LHC Higgs Cross Section Working Group, 108The LHC Higgs Cross Section Working Group, 109The LHC Higgs Cross Section Working Group, 110The LHC Higgs Cross Section Working Group, 111The LHC Higgs Cross Section Working Group, 112The LHC Higgs Cross Section Working Group, 113The LHC Higgs Cross Section Working Group, 114The LHC Higgs Cross Section Working Group, 115The LHC Higgs Cross Section Working Group, 116The LHC Higgs Cross Section Working Group, 117The LHC Higgs Cross Section Working Group, 118The LHC Higgs Cross Section Working Group, 119The LHC Higgs Cross Section Working Group, 120The LHC Higgs Cross Section Working Group, 121The LHC Higgs Cross Section Working Group, 122The LHC Higgs Cross Section Working Group, 123The LHC Higgs Cross Section Working Group, 124The LHC Higgs Cross Section Working Group, 125The LHC Higgs Cross Section Working Group, 126The LHC Higgs Cross Section Working Group, 127The LHC Higgs Cross Section Working Group, 128The LHC Higgs Cross Section Working Group, 129The LHC Higgs Cross Section Working Group, 130The LHC Higgs Cross Section Working Group, 131The LHC Higgs Cross Section Working Group, 132The LHC Higgs Cross Section Working Group, 133The LHC Higgs Cross Section Working Group, 134The LHC Higgs Cross Section Working Group, 135The LHC Higgs Cross Section Working Group, 136The LHC Higgs Cross Section Working Group, 137The LHC Higgs Cross Section Working Group, 138The LHC Higgs Cross Section Working Group, 139The LHC Higgs Cross Section Working Group, 140The LHC Higgs Cross Section Working Group, 141The LHC Higgs Cross Section Working Group, 142The LHC Higgs Cross Section Working Group, 143The LHC Higgs Cross Section Working Group, 144The LHC Higgs Cross Section Working Group, 145The LHC Higgs Cross Section Working Group, 146The LHC Higgs Cross Section Working Group, 147The LHC Higgs Cross Section Working Group, 148The LHC Higgs Cross Section Working Group, 149The LHC Higgs Cross Section Working Group, 150The LHC Higgs Cross Section Working Group, 151The LHC Higgs Cross Section Working Group, 152The LHC Higgs Cross Section Working Group, 153The LHC Higgs Cross Section Working Group, 154The LHC Higgs Cross Section Working Group, 155The LHC Higgs Cross Section Working Group, 156The LHC Higgs Cross Section Working Group, 157The LHC Higgs Cross Section Working Group, 158The LHC Higgs Cross Section Working Group, 159The LHC Higgs Cross Section Working Group, 160The LHC Higgs Cross Section Working Group, 161The LHC Higgs Cross Section Working Group, 162The LHC Higgs Cross Section Working Group, 163The LHC Higgs Cross Section Working Group, 164The LHC Higgs Cross Section Working Group, 165The LHC Higgs Cross Section Working Group, 166The LHC Higgs Cross Section Working Group, 167The LHC Higgs Cross Section Working Group, 168The LHC Higgs Cross Section Working Group, 169The LHC Higgs Cross Section Working Group, 170The LHC Higgs Cross Section Working Group, 171The LHC Higgs Cross Section Working Group, 172The LHC Higgs Cross Section Working Group, 173The LHC Higgs Cross Section Working Group, 174The LHC Higgs Cross Section Working Group, 175The LHC Higgs Cross Section Working Group, 176The LHC Higgs Cross Section Working Group, 177The LHC Higgs Cross Section Working Group, 178The LHC Higgs Cross Section Working Group, 179The LHC Higgs Cross Section Working Group, 180The LHC Higgs Cross Section Working Group, 181The LHC Higgs Cross Section Working Group, 182The LHC Higgs Cross Section Working Group, 183The LHC Higgs Cross Section Working Group, 184The LHC Higgs Cross Section Working Group, 185The LHC Higgs Cross Section Working Group, 186The LHC Higgs Cross Section Working Group, 187The LHC Higgs Cross Section Working Group, 188The LHC Higgs Cross Section Working Group, 189The LHC Higgs Cross Section Working Group, 190The LHC Higgs Cross Section Working Group, 191The LHC Higgs Cross Section Working Group, 192The LHC Higgs Cross Section Working Group, 193The LHC Higgs Cross Section Working Group, 194The LHC Higgs Cross Section Working Group, 195The LHC Higgs Cross Section Working Group, 196The LHC Higgs Cross Section Working Group, 197The LHC Higgs Cross Section Working Group, 198The LHC Higgs Cross Section Working Group, 199The LHC Higgs Cross Section Working Group, 200The LHC Higgs Cross Section Working Group, 201The LHC Higgs Cross Section Working Group, 202The LHC Higgs Cross Section Working Group, 203The LHC Higgs Cross Section Working Group, 204The LHC Higgs Cross Section Working Group, 205The LHC Higgs Cross Section Working Group, 206The LHC Higgs Cross Section Working Group, 207The LHC Higgs Cross Section Working Group, 208The LHC Higgs Cross Section Working Group, 209The LHC Higgs Cross Section Working Group, 210The LHC Higgs Cross Section Working Group, 211The LHC Higgs Cross Section Working Group, 212The LHC Higgs Cross Section Working Group, 213The LHC Higgs Cross Section Working Group, 214The LHC Higgs Cross Section Working Group, 215The LHC Higgs Cross Section Working Group, 216The LHC Higgs Cross Section Working Group, 217The LHC Higgs Cross Section Working Group, 218The LHC Higgs Cross Section Working Group, 219The LHC Higgs Cross Section Working Group, 220The LHC Higgs Cross Section Working Group, 221The LHC Higgs Cross Section Working Group, 222The LHC Higgs Cross Section Working Group, 223The LHC Higgs Cross Section Working Group, 224The LHC Higgs Cross Section Working Group, 225The LHC Higgs Cross Section Working Group, 226The LHC Higgs Cross Section Working Group, 227The LHC Higgs Cross Section Working Group, 228The LHC Higgs Cross Section Working Group, 229The LHC Higgs Cross Section Working Group, 230The LHC Higgs Cross Section Working Group, 231The LHC Higgs Cross Section Working Group, 232The LHC Higgs Cross Section Working Group, 233The LHC Higgs Cross Section Working Group, 234The LHC Higgs Cross Section Working Group, 235The LHC Higgs Cross Section Working Group, 236The LHC Higgs Cross Section Working Group, 237The LHC Higgs Cross Section Working Group, 238The LHC Higgs Cross Section Working Group, 239The LHC Higgs Cross Section Working Group, 240The LHC Higgs Cross Section Working Group, 241The LHC Higgs Cross Section Working Group, 242The LHC Higgs Cross Section Working Group, 243The LHC Higgs Cross Section Working Group, 244The LHC Higgs Cross Section Working Group, 245The LHC Higgs Cross Section Working Group, 246The LHC Higgs Cross Section Working Group, 247The LHC Higgs Cross Section Working Group, 248The LHC Higgs Cross Section Working Group, 249The LHC Higgs Cross Section Working Group, 250The LHC Higgs Cross Section Working Group, 251The LHC Higgs Cross Section Working Group, 252The LHC Higgs Cross Section Working Group, 253The LHC Higgs Cross Section Working Group, 254The LHC Higgs Cross Section Working Group, 255The LHC Higgs Cross Section Working Group, 256The LHC Higgs Cross Section Working Group, 257The LHC Higgs Cross Section Working Group, 258The LHC Higgs Cross Section Working Group, 259The LHC Higgs Cross Section Working Group, 260The LHC Higgs Cross Section Working Group, 261The LHC Higgs Cross Section Working Group, 262The LHC Higgs Cross Section Working Group, 263The LHC Higgs Cross Section Working Group, 264The LHC Higgs Cross Section Working Group, 265The LHC Higgs Cross Section Working Group, 266The LHC Higgs Cross Section Working Group, 267The LHC Higgs Cross Section Working Group, 268The LHC Higgs Cross Section Working Group, 269The LHC Higgs Cross Section Working Group, 270The LHC Higgs Cross Section Working Group, 271The LHC Higgs Cross Section Working Group, 272The LHC Higgs Cross Section Working Group, 273The LHC Higgs Cross Section Working Group, 274The LHC Higgs Cross Section Working Group, 275The LHC Higgs Cross Section Working Group, 276The LHC Higgs Cross Section Working Group, 277The LHC Higgs Cross Section Working Group, 278The LHC Higgs Cross Section Working Group, 279The LHC Higgs Cross Section Working Group, 280The LHC Higgs Cross Section Working Group, 281The LHC Higgs Cross Section Working Group, 282The LHC Higgs Cross Section Working Group, 283The LHC Higgs Cross Section Working Group, 284The LHC Higgs Cross Section Working Group, 285The LHC Higgs Cross Section Working Group, 286The LHC Higgs Cross Section Working Group, 287The LHC Higgs Cross Section Working Group, 288The LHC Higgs Cross Section Working Group, 289The LHC Higgs Cross Section Working Group, 290The LHC Higgs Cross Section Working Group, 291The LHC Higgs Cross Section Working Group, 292The LHC Higgs Cross Section Working Group, 293The LHC Higgs Cross Section Working Group, 294The LHC Higgs Cross Section Working Group, 295The LHC Higgs Cross Section Working Group, 296The LHC Higgs Cross Section Working Group, 297The LHC Higgs Cross Section Working Group, 298The LHC Higgs Cross Section Working Group, 299The LHC Higgs Cross Section Working Group, 300The LHC Higgs Cross Section Working Group, 301The LHC Higgs Cross Section Working Group, 302The LHC Higgs Cross Section Working Group, 303The LHC Higgs Cross Section Working Group, 304The LHC Higgs Cross Section Working Group, 305The LHC Higgs Cross Section Working Group, 306The LHC Higgs Cross Section Working Group, 307The LHC Higgs Cross Section Working Group, 308The LHC Higgs Cross Section Working Group, 309The LHC Higgs Cross Section Working Group, 310The LHC Higgs Cross Section Working Group, 311The LHC Higgs Cross Section Working Group, 312The LHC Higgs Cross Section Working Group, 313The LHC Higgs Cross Section Working Group, 314The LHC Higgs Cross Section Working Group, 315The LHC Higgs Cross Section Working Group, 316The LHC Higgs Cross Section Working Group, 317The LHC Higgs Cross Section Working Group, 318The LHC Higgs Cross Section Working Group, 319The LHC Higgs Cross Section Working Group, 320The LHC Higgs Cross Section Working Group, 321The LHC Higgs Cross Section Working Group, 322The LHC Higgs Cross Section Working Group, 323The LHC Higgs Cross Section Working Group, 324The LHC Higgs Cross Section Working Group, 325The LHC Higgs Cross Section Working Group, 326The LHC Higgs Cross Section Working Group, 327The LHC Higgs Cross Section Working Group, 328The LHC Higgs Cross Section Working Group, 329The LHC Higgs Cross Section Working Group, 330The LHC Higgs Cross Section Working Group, 331The LHC Higgs Cross Section Working Group, 332The LHC Higgs Cross Section Working Group, 333The LHC Higgs Cross Section Working Group, 334The LHC Higgs Cross Section Working Group, 335The LHC Higgs Cross Section Working Group, 336The LHC Higgs Cross Section Working Group, 337The LHC Higgs Cross Section Working Group, 338The LHC Higgs Cross Section Working Group, 339The LHC Higgs Cross Section Working Group, 340The LHC Higgs Cross Section Working Group, 341The LHC Higgs Cross Section Working Group, 342The LHC Higgs Cross Section Working Group, 343The LHC Higgs Cross Section Working Group, 344The LHC Higgs Cross Section Working Group, 345The LHC Higgs Cross Section Working Group, 346The LHC Higgs Cross Section Working Group, 347The LHC Higgs Cross Section Working Group, 348The LHC Higgs Cross Section Working Group, 349The LHC Higgs Cross Section Working Group, 350The LHC Higgs Cross Section Working Group, 351The LHC Higgs Cross Section Working Group, 352The LHC Higgs Cross Section Working Group, 353The LHC Higgs Cross Section Working Group, 354The LHC Higgs Cross Section Working Group, 355The LHC Higgs Cross Section Working Group, 356The LHC Higgs Cross Section Working Group, 357The LHC Higgs Cross Section Working Group, 358The LHC Higgs Cross Section Working Group, 359The LHC Higgs Cross Section Working Group, 360The LHC Higgs Cross Section Working Group, 361The LHC Higgs Cross Section Working Group, 362The LHC Higgs Cross Section Working Group, 363The LHC Higgs Cross Section Working Group, 364The LHC Higgs Cross Section Working Group, 365The LHC Higgs Cross Section Working Group, 366The LHC Higgs Cross Section Working Group, 367The LHC Higgs Cross Section Working Group, 368The LHC Higgs Cross Section Working Group, 369The LHC Higgs Cross Section Working Group, 370The LHC Higgs Cross Section Working Group, 371The LHC Higgs Cross Section Working Group, 372The LHC Higgs Cross Section Working Group, 373The LHC Higgs Cross Section Working Group, 374The LHC Higgs Cross Section Working Group

This Report summarizes the results of the activities of the LHC Higgs Cross Section Working Group in the period 2014-2016. The main goal of the working group was to present the state-of-the-art of Higgs physics at the LHC, integrating all new results that have appeared in the last few years. The first part compiles the most up-to-date predictions of Higgs boson production cross sections and decay branching ratios, parton distribution functions, and off-shell Higgs boson production and interference effects. Read More

In models with extended Higgs sectors, it is possible that the Higgs boson discovered at the LHC is not the lightest one. We show that in a realistic model (the Type I 2-Higgs Doublet Model), when the sum of the masses of a light scalar and a pseudoscalar ($h$ and $A$) is smaller than the $Z$ boson mass, the Electroweak (EW) production of an $hA$ pair can dominate over QCD production by orders of magnitude, a fact not previously highlighted. This is because in the $gg$-initiated process, $hA$ production via a resonant $Z$ in the $s$-channel is prohibited according to the Landau-Yang theorem, which is not the case for the $q\bar{q}$-initiated process. Read More

Traditional taxi systems in metropolitan areas often suffer from inefficiencies due to uncoordinated actions as system capacity and customer demand change. With the pervasive deployment of networked sensors in modern vehicles, large amounts of information regarding customer demand and system status can be collected in real time. This information provides opportunities to perform various types of control and coordination for large-scale intelligent transportation systems. Read More

After the discovery of the 125 GeV Higgs boson, the Next-to-Minimal Supersymmetric Standard Model (NMSSM) has become more interesting as a model for new physics since new tree-level contributions to the Higgs mass makes it easier to accommodate the relatively high measured value, as compared to the MSSM. One very distinctive feature of the NMSSM is the possible existence of a light singlet-like pseudoscalar. As this pseudoscalar may be lighter than the discovered Higgs boson without conflict with data, it may lead to LHC signatures rather different to what is usually searched for in terms of new physics. Read More

We study neutralino dark matter (DM) with large singlino fractions in the next-to-minimal supersymmetric Standard Model (NMSSM). We perform a detailed analysis of the parameter space regions of the model that give rise to such singlino-dominated neutralinos while satisfying the constraints from Higgs boson searches at the Large Electron Positron (LEP) collider and the Large Hadron Collider (LHC), as well as from b-physics experiments. We find that this DM can yield a thermal relic density consistent with the Planck measurement in mass regions where the lightest neutralino of the minimal supersymmetric Standard Model (MSSM) generally cannot. Read More

We analyse the discovery prospects of the charged Higgs boson, $H^\pm$, via its decay in the $W^\pm h$ channel in the minimal supersymmetric Standard Model (MSSM) as well as several 2-Higgs Doublet Models (2HDMs). $h$, the lightest scalar Higgs boson in these models, is identified with the recently discovered $\sim 125$ GeV state, $H_\text{obs}$, at the Large Hadron Collider (LHC). We find that, while it provides an important input in the kinematic selection of signal events, the measured $H_\text{obs}$ mass renders this channel inaccessible in the MSSM. Read More

We analyse the impact of explicit CP-violation in the Higgs sector of the Next-to-Minimal Supersymmetric Standard Model (NMSSM) on its consistency with the Higgs boson data from the Large Hadron Collider (LHC). Through detailed scans of the parameter space of the complex NMSSM for certain fixed values of one of its CP-violating (CPV) phases, we obtain a large number of points corresponding to five phenomenologically relevant scenarios containing $\sim 125$ GeV Higgs boson(s). We focus, in particular, on the scenarios where the visible peaks in the experimental samples can actually be explained by two nearly mass-degenerate neutral Higgs boson states. Read More

We analyze the prospects of the detection of a $\mathcal{O}(1)$ GeV neutralino dark matter, $\widetilde{\chi}^0_{1}$, in the Next-to-Minimal Supersymmetric Standard Model at the 14 TeV LHC. We perform dedicated scans of the relevant parameter space of the model and find a large number of points where the thermal relic abundance due to such a dark matter is consistent with the PLANCK measurement. We note that this dark matter is highly singlino-dominated and is always accompanied by a pseudoscalar, $A_1$, with a mass around twice its own, which is responsible for its resonant annihilation. Read More

2015Feb
Affiliations: 1Warsaw, Inst. Nucl. Studies, 2Southampton U., 3APCTP, Pohang & Uppsala U., 4Warsaw, Inst. Nucl. Studies and Sheffield U.

We revisit the light pseudoscalar $A_1$ in the Next-to-Minimal Supersymmetric Standard Model (NMSSM) with partial universality at some high unification scale in order to delineate the parameter space regions consistent with up-to-date theoretical and experimental constraints and examine to what extent this state can be probed by the Large Hadron Collider (LHC) during Run 2. We find that it can be accessible through a variety of signatures proceeding via $A_1\to \tau^+\tau^-$ and/or $b\bar b$, the former assuming hadronic decays and the latter two $b$-tags within a fat jet or two separate slim ones. Herein, the light pseudoscalar state is produced from a heavy Higgs boson decay in either pairs or singly in association with a $Z$ boson (in turn decaying into electrons/muons). Read More

The presence of two light higgsinos nearly degenerate in mass is one of the important characteristics of suspersymmetric models meeting the naturalness criteria. Probing such higgsinos at the LHC is very challenging, in particular when the mass-splitting between them is less than 5 GeV. In this study, we analyze such a degenerate higgsino scenario by exploiting the high collinearity between the two muons which originate from the decay of the heavier higgsino into the lighter one and which are accompanied by a high-$p_T$ QCD jet. Read More

The recent observation of a 125 GeV neutral Higgs boson ($H_{\rm obs}$) provides additional input for charged Higgs boson searches in the $H^\pm \to W^\pm H_{\rm obs}$ decay channel at the Large Hadron Collider (LHC). We reassess the discovery potential in this channel, which is important for $H^\pm$ heavier than the top quark mass. When $H_{\rm obs}$ decays to a $b\bar{b}$ pair, knowledge of the Higgs mass aids in the kinematic selection of signal events. Read More

In light of the recent discovery of a neutral Higgs boson, $H_{\rm obs}$, with a mass near 125 GeV, we reassess the LHC discovery potential of a charged Higgs boson, $H^\pm$, in the $W^\pm H_{\rm obs}$ decay channel. This decay channel can be particularly important for a $H^\pm$ heavier than the top quark, when it is produced through the $pp \rightarrow tH^\pm$ process. The knowledge of the mass of $H_{\rm obs}$ provides an additional handle in the kinematic selection when reconstructing a Breit-Wigner resonance in the $H_{\rm obs} \rightarrow b\bar{b}$ decay channel. Read More

The discovery of a light, singlet-like pseudoscalar Higgs boson, $A_1$, of the Next-to-Minimal Supersymmetric Standard Model (NMSSM) could provide a hallmark signature of non-minimal supersymmetry. We review here the potential of the LHC to probe such a light $A_1$ in the decays of one of the heavier scalar Higgs bosons of the NMSSM. We find the production of pairs of the $A_1$, with a mass below 60 GeV or so, via decays of the two lightest scalar states to be especially promising, for an integrated luminosity as low as 30/fb. Read More

The Next-to-Minimal Supersymmetric Standard Model (NMSSM) contains a singlet-like pseudoscalar Higgs boson in addition to the doublet-like pseudoscalar of the Minimal Supersymmetric Standard Model. This new pseudoscalar can have a very low mass without violating the LEP exclusion constraints and it can potentially provide a hallmark signature of non-minimal supersymmetry at the LHC. In this analysis we revisit the light pseudoscalar in the NMSSM with partial universality at some high unification scale. Read More

In the Next-to-Minimal Supersymmetric Standard Model (NMSSM) a variety of parameter configurations yields a Higgs boson consistent with the one observed at the LHC. Additionally, the Higgs sector of the model can contain explicit CP-violating phases even at the tree level, in contrast with the Minimal Supersymmetric Standard Model (MSSM). In this article we present the one-loop Higgs boson mass matrix of the complex NMSSM in the renormalisation-group-improved effective potential approach. Read More

We propose an experimental test of a scenario in the Next-to-Minimal Supersymmetric Standard Model in which both the lightest scalar and the lightest pseudoscalar Higgs bosons have masses around 125 GeV. The pseudoscalar can contribute significantly to the gamma.gamma rate at the LHC due to light Higgsino-like charginos in its effective one-loop coupling to two photons. Read More

While the properties of the 125 GeV Higgs boson-like particle observed by the ATLAS and CMS collaborations are largely compatible with those predicted for the Standard Model state, significant deviations are present in some cases. We, therefore, test the viability of a Beyond the Standard Model scenario based on Supersymmetry, the CP-violating Next-to-Minimal Supersymmetric Standard Model, against the corresponding experimental observations. Namely, we identify possible model configurations in which one of its Higgs bosons is consistent with the LHC observation and evaluate the role of the explicit complex phases in both the mass and diphoton decay of such a Higgs boson. Read More

We present the first global analysis of the Constrained NMSSM that investigates the impact of the recent discovery of a 126 GeV Higgs-like boson, of the observation of a signal for BR(B_s->\mu^+\mu^-), and of constraints on supersymmetry from ~5/fb of data accumulated at the LHC, as well as of other relevant constraints from colliders, flavor physics and dark matter. We consider three possible cases, assuming in turn that the discovered Higgs boson is: i) the lightest Higgs boson of the model; ii) the next-to-lightest Higgs boson; and iii) a combination of both roughly degenerate in mass. The likelihood function for the Higgs signal uses signal rates in the \gamma\gamma\ and ZZ --> 4l channels, while that for the Higgs exclusion limits assumes decay through the \gamma\gamma, \tau\tau, ZZ and W^+W^- channels. Read More

We present an updated and extended global analysis of the Constrained MSSM (CMSSM) taking into account new limits on supersymmetry from ~5/fb data sets at the LHC. In particular, in the case of the razor limit obtained by the CMS Collaboration we simulate detector efficiency for the experimental analysis and derive an approximate but accurate likelihood function. We discuss the impact on the global fit of a possible Higgs boson with mass near 125 GeV, as implied by recent data, and of a new improved limit on BR(B_s->\mu\mu). Read More

Many models beyond the Standard Electroweak Theory, top-down or bottom-up, contain extensions of the gauge symmetry group by extra U(1)' factors which can be understood or treated as subgroups of E(6). A brief overview of such models is followed by a sketch of a systematic classification. We then describe how the resulting extra massive neutral gauge bosons can be searched for and in case of positive evidence diagnosed using electroweak and collider data. Read More

We study the effect of explicit CP violation in the Higgs sectors of the MSSM in the di-photon decay of the lightest CP-mixed Higgs state. Further it is shown that the gluon fusion production mechanism along with the di-photon decay enhances CP-violating effects for a large set of suitably chosen parameter values. Read More

We revisit the CDF data on di-muon production to impose constraints on a large class of Z' bosons occurring in a variety of E_6 GUT based models. We analyze the dependence of these limits on various factors contributing to the production cross-section, showing that currently systematic and theoretical uncertainties play a relatively minor role. Driven by this observation, we emphasize the use of the Bayesian statistical method, which allows us to straightforwardly (i) vary the gauge coupling strength, g', of the underlying U(1)'; (ii) include interference effects with the Z' amplitude (which are especially important for large g'); (iii) smoothly vary the U(1)' charges; (iv) combine these data with the electroweak precision constraints as well as with other observables obtained from colliders such as LEP 2 and the LHC; and (v) find preferred regions in parameter space once an excess is seen. Read More

The CDF collaboration has set lower limits on the masses of the Z' bosons occurring in a range of E_6 GUT based models. We revisit their analysis and extend it to certain other E_6 scenarios as well as to some general classes of models satisfying the anomaly cancellation conditions, which are not included in the CDF analysis. We also suggest a Bayesian statistical method for finding exclusion limits on the Z' mass, which allows one to explore a wide range of the U(1)' gauge coupling parameter. Read More

We analysed the sensitivity of the process gg to H_1 to gamma-gamma to the explicitly CP-violating phases phi_mu and phi_{A_f} in the Minimal Supersymmetric Standard Model (MSSM) at the Large Hadron Collider (LHC), where H_1 is the lightest Supersymmetric Higgs boson. We conclude that depending on these phases, the overall production and decay rates of H_1 can vary up to orders of magnitude compared to the CP-conserving case. Read More

We tested several models in which the Standard Model (SM) gauge group is extended by an additional U(1) gauge symmetry, against available electroweak precision data to impose limits on the mass of the neutral Z' boson, M_Z', predicted in all such models, and on the Z-Z' mixing angle, theta_ZZ', at 95% C.L. We found lower limits on M_Z' of order 1 TeV in most cases, while theta_ZZ' was found to be constrained to very small values. Read More

We analyze various models with an extra U(1) gauge symmetry in addition to the Standard Model (SM) gauge group at low energies, and impose limits on the mass of the neutral Z' boson, M_Z', predicted in all such models, and on the Z-Z' mixing angle, theta_ZZ'. The precision electroweak data strongly constrain theta_ZZ' to very small values and for most models we find lower limits on M_Z' of order 1 TeV. In one case we obtain a somewhat better fit than in the SM (although this is only marginally statistically significant) and here we find a weak upper limit at the 90% C. Read More

2009Mar
Affiliations: 1IPPP, University of Durham, UK, 2University of Southampton, UK, 3Instituto de Fisica, Mexico, 4IIT Guwahati, India

We prove the strong sensitivity of the gg --> H1 --> gamma.gamma cross section at the Large Hadron Collider on the explicitly CP-violating phases of the Minimal Supersymmetric Standard Model, where H1 is the lightest Supersymmetric Higgs boson. Read More

2007Oct
Affiliations: 1University of Southampton, 2University of Southampton, 3University of Southampton, 4University of Southampton

Physical Higgs particles in the Minimal Supersymmetric Standard Model (MSSM) with explicit CP violation are CP mixed states. The decay of these Higgs particles can be analysed to study the CP properties of the MSSM. In the present work we consider the di-photon channel of the lightest neutral Higgs boson for this purpose. Read More

2007Oct
Affiliations: 1University of Southampton, 2University of Southampton, 3University of Southampton, 4University of Southampton

The Minimal Supersymmetric Standard Model (MSSM) with explicit CP violation is studied with the help of the di-photon decay channel of the lightest neutral Higgs boson. Effects of CP violation, entering via the scalar/pseudo-scalar mixing at higher order as well as through the Higgs-sfermion-sfermion couplings at tree-level, are analyzed in the MSSM with and without light sparticles. A light stop may have a strong impact on the decay width and Branching Ratio (BR) of the decay process H_1 -> gamma gamma, whereas other light sparticles have only little influence. Read More

2007Jun
Affiliations: 1University of Southampton, 2University of Southampton, 3University of Southampton, 4University of Southampton

The di-photon decay channel of the lightest Higgs boson is considerd as a probe to explore CP violation in the Minimal Supersymmetric Standard Model (MSSM). The scalar/pseudo-scalar mixing is considered along with CP violation entering through the Higgs-sfermion-sfermion couplings, with and without light sparticles. The impact of a light stop on the decay width and Branching Ratio (BR) is established through a detailed study of the amplitude of the process H1 --> gamma. Read More

2007Feb
Affiliations: 1University of Southampton, 2University of Southampton, 3University of Southampton

The MSSM with explicit CP violation is studied through the di-photon decay channel of the lightest neutral Higgs boson. Through the leading one-loop order H1 --> gammar.gamma is affected by a large number of Higgs-sparticle couplings, which could be complex. Read More

2006Aug

We show how the LHC potential to detect a rather light CP-even Higgs boson of the NMSSM, H1 or H2, decaying into CP-odd Higgs states, A1A1, can be improved if Higgs-strahlung off W bosons and (more marginally) off top-antitop pairs are employed alongside vector boson fusion as production modes. Our results should help extracting at least one Higgs boson signal over the NMSSM parameter space. Read More

2006Aug
Authors: S. Kraml, E. Accomando, A. G. Akeroyd, E. Akhmetzyanova, J. Albert, A. Alves, N. Amapane, M. Aoki, G. Azuelos, S. Baffioni, A. Ballestrero, V. Barger, A. Bartl, P. Bechtle, G. Belanger, A. Belhouari, R. Bellan, A. Belyaev, P. Benes, K. Benslama, W. Bernreuther, M. Besancon, G. Bevilacqua, M. Beyer, M. Bluj, S. Bolognesi, M. Boonekamp, F. Borzumati, F. Boudjema, A. Brandenburg, T. Brauner, C. P. Buszello, J. M. Butterworth, M. Carena, D. Cavalli, G. Cerminara, S. Y. Choi, B. Clerbaux, C. Collard, J. A. Conley, A. Deandrea, S. De Curtis, R. Dermisek, A. De Roeck, G. Dewhirst, M. A. Diaz, J. L. Diaz-Cruz, D. D. Dietrich, M. Dolgopolov, D. Dominici, M. Dubinin, O. Eboli, J. Ellis, N. Evans, L. Fano, J. Ferland, S. Ferrag, S. P. Fitzgerald, H. Fraas, F. Franke, S. Gennai, I. F. Ginzburg, R. M. Godbole, T. Gregoire, G. Grenier, C. Grojean, S. B. Gudnason, J. F. Gunion, H. E. Haber, T. Hahn, T. Han, V. Hankele, C. Hays, S. Heinemeyer, S. Hesselbach, J. L. Hewett, K. Hidaka, M. Hirsch, W. Hollik, D. Hooper, J. Hosek, J. Hubisz, C. Hugonie, J. Kalinowski, S. Kanemura, V. Kashkan, T. Kernreiter, W. Khater, V. A. Khoze, W. Kilian, S. F. King, O. Kittel, G. Klamke, J. L. Kneur, C. Kouvaris, M. Krawczyk, P. Krstonosic, A. Kyriakis, P. Langacker, M. P. Le, H. -S. Lee, J. S. Lee, M. C. Lemaire, Y. Liao, B. Lillie, V. Litvin, H. E. Logan, B. McElrath, T. Mahmoud, E. Maina, C. Mariotti, P. Marquard, A. D. Martin, K. Mazumdar, D. J. Miller, P. Mine, K. Moenig, G. Moortgat-Pick, S. Moretti, M. M. Muhlleitner, S. Munir, R. Nevzorov, H. Newman, P. Niezurawski, A. Nikitenko, R. Noriega-Papaqui, Y. Okada, P. Osland, A. Pilaftsis, W. Porod, H. Przysiezniak, A. Pukhov, D. Rainwater, A. Raspereza, J. Reuter, S. Riemann, S. Rindani, T. G. Rizzo, E. Ros, A. Rosado, D. Rousseau, D. P. Roy, M. G. Ryskin, H. Rzehak, F. Sannino, E. Schmidt, H. Schroder, M. Schumacher, A. Semenov, E. Senaha, G. Shaughnessy, R. K. Singh, J. Terning, L. Vacavant, M. Velasco, A. Villanova del Moral, F. von der Pahlen, G. Weiglein, J. Williams, K. Williams, A. F. Zarnecki, D. Zeppenfeld, D. Zerwas, P. M. Zerwas, A. R. Zerwekh, J. Ziethe

There are many possibilities for new physics beyond the Standard Model that feature non-standard Higgs sectors. These may introduce new sources of CP violation, and there may be mixing between multiple Higgs bosons or other new scalar bosons. Alternatively, the Higgs may be a composite state, or there may even be no Higgs at all. Read More

2006Mar

The NMSSM contains a Higgs singlet in addition to the two Higgs doublets typical of the MSSM, thus resulting in a total of seven physical Higgs mass states. Therefore, the phenomenology of the NMSSM Higgs sector can vary considerably from that of the MSSM and there are good prospects of finding in regions of the NMSSM parameter space Higgs signals that cannot be reproduced in the MSSM. We examined here the two-photon decay mode of a Higgs boson and found that up to three neutral Higgs states, heavy and/or light, could be simultaneously observable at the LHC, a possibility precluded to the MSSM. Read More