M. Gorbahn

M. Gorbahn
Are you M. Gorbahn?

Claim your profile, edit publications, add additional information:

Contact Details

Name
M. Gorbahn
Affiliation
Location

Pubs By Year

Pub Categories

 
High Energy Physics - Phenomenology (31)
 
High Energy Physics - Experiment (10)
 
High Energy Physics - Lattice (2)

Publications Authored By M. Gorbahn

The quantity $\varepsilon'/\varepsilon$ measures direct CP violation in Kaon decays. Recent SM predictions show a $2.9\sigma$ tension with data, with the theoretical uncertainty dominating. Read More

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

We examine the constraints on the trilinear Higgs coupling $\lambda$ that originate from associated ($Vh$) and vector boson fusion (VBF) Higgs production in $pp$ collisions in the context of the Standard Model effective field theory. The 1-loop contributions to $pp \to V h$ and $pp \to jj h$ that stem from insertions of the dimension-6 operator $O_6 = - \lambda \left (H^\dagger H \right )^3$ are calculated and combined with the ${\cal O} (\lambda)$ corrections to the partial decay widths of the Higgs boson. Employing next-to-next-to-leading order QCD predictions, we analyse the sensitivity of current and forthcoming measurements of the signal strengths in $Vh$ and VBF Higgs production to changes in $\lambda$. Read More

In the framework of the Standard Model effective field theory, we examine the indirect constraints on the trilinear Higgs coupling $\lambda$ that arise from Higgs production in gluon-gluon-fusion and diphoton Higgs decays. We calculate 2-loop contributions to the $gg \to h$ and $h \to \gamma \gamma$ amplitudes that are affected by modifications of the trilinear Higgs-boson vertex. This calculation involves both the computation of anomalous dimensions and finite matching corrections. Read More

We present a new analysis of the ratio epsilon'/epsilon within the Standard Model (SM) using a formalism that is manifestly independent of the values of leading (V-A)x(V-A) QCD penguin, and EW penguin hadronic matrix elements of the operators Q_4, Q_9, and Q_10, and applies to the SM as well as extensions with the same operator structure. It is valid under the assumption that the SM exactly describes the data on CP-conserving K -> pi pi amplitudes. As a result of this and the high precision now available for CKM and quark mass parameters, to high accuracy epsilon'/epsilon depends only on two non-perturbative parameters, B_6^(1/2) and B_8^(3/2), and perturbatively calculable Wilson coefficients. Read More

Precise measurements of SM particles properties at the LHC allows to look for heavy New Physics in the context of an Effective Field Theory (EFT). These searches, however, often rely on kinematic regions where the validity of the EFT may be compromised. In this paper we propose to address this issue by comparing with benchmark models. Read More

We use currently available data of nonleptonic charmless 2-body $B\to MM$ decays ($MM = PP, PV, VV$) that are mediated by $b\to (d, s)$ QCD- and QED-penguin operators to study weak annihilation and new-physics effects in the framework of QCD factorization. In particular we introduce one weak annihilation parameter for decays related by ($u \leftrightarrow d$) quark interchange and test this universality assumption. Within the standard model, the data supports this assumption with the only exceptions in the $B\to K \pi$ system, which exhibits the well-known "$\Delta A_{CP}$ puzzle", and some tensions in $B \to K^* \phi$. Read More

A discovery of flavour-changing Higgs-boson decays would constitute an undeniable signal of new physics. We derive model-independent constraints on the tch and tuh couplings that arise from the bounds on hadronic electric dipole moments. Comparisons of the present and future sensitivities with both the direct LHC constraints and the indirect limits from D-meson physics are also presented. Read More

We calculate the full two-loop electroweak matching corrections to the operator governing the decay B_q --> l^+ l^- in the Standard Model. Their inclusion removes an electroweak scheme and scale uncertainty of about 7% of the branching ratio. Using different renormalization schemes of the involved electroweak parameters, we estimate residual perturbative electroweak and QED uncertainties to be less than 1% at the level of the branching ratio. Read More

We combine our new results for the O(alpha_em) and O(alpha_s^2) corrections to B_{s,d} -> l^+ l^-, and present updated branching ratio predictions for these decays in the standard model. Inclusion of the new corrections removes major theoretical uncertainties of perturbative origin that have just begun to dominate over the parametric ones. For the recently observed muonic decay of the B_s meson, our calculation gives BR(B_s -> mu^+ mu^-) = (3. Read More

The observables epsilon_K and Delta M_K play a prominent role in particle physics due to their sensitivity to new physics at short distances. To take advantage of this potential, a firm theoretical prediction of the standard-model background is essential. The charm-quark contribution is a major source of theoretical uncertainty. Read More

Rare decays were essential in the discovery of the CKM mechanism of flavour and CP violation and are highly sensitive probes of physics beyond the Standard Model. In this summary the current status and future prospects of experimental measurements and the Standard Model theory predictions of various rare B, D and K decay observables are discussed. The specific new physics sensitivities of each mode are also briefly reviewed. Read More

The rare K -> pi nu anti-nu decays play a central role in testing the Standard Model and its extensions. Upcoming experiments plan to measure the decay rates with high accuracy. Yet, unknown higher-order electroweak corrections result in a sizeable theory error. Read More

We perform a next-to-next-to-leading order (NNLO) QCD analysis of the charm-top-quark contribution eta_ct to the effective Delta S = 2 Hamiltonian in the Standard Model. eta_ct represents an important part of the short distance contribution to the parameter epsilon_K. We calculate the three-loop anomalous dimension of the leading operator Q_S2, the three-loop mixing of the current-current and penguin operators into Q_S2, and the corresponding two-loop matching conditions at the electroweak, the bottom-quark, and the charm-quark scale. Read More

We compute the conversion factors needed to obtain the MS-bar and RGI up, down, and strange-quark masses at next-to-next-to-leading order from the corresponding parameters renormalized in the recently proposed RI/SMOM and RI/SMOM_gamma_mu renormalization schemes. This is important for obtaining the MS-bar masses with the best possible precision from numerical lattice-QCD simulations, because the customary RI(')/MOM scheme is afflicted with large irreducible uncertainties both on the lattice and in perturbation theory. We find that the smallness of the known one-loop matching coefficients is accompanied by even smaller two-loop contributions. Read More

We discuss the theory prediction of epsilon_K and the rare K -> pi nu nu-bar decays and review the structure and current status of higher-order contributions to these flavour changing processes in the standard model in some detail. This includes the next-to-next-to-leading order QCD calculation to the charm quark contribution to K+ -> pi+ nu nu-bar and to the charm-top quark contribution to epsilon_K. Electroweak corrections to the rare kaon decays are also discussed. Read More

We match the Higgs sector of the most general flavour breaking and CP violating minimal supersymmetric standard model (MSSM) onto a generic two-Higgs-doublet model, paying special attention to the definition of tan beta in the effective theory. In particular no tan beta-enhanced loop corrections appear in the relation to tan beta defined in the DRbar scheme in the MSSM. The corrections to the Higgs-mediated flavour-changing amplitudes which result from this matching are especially relevant for the B_d and B_s mass differences dM_s,d for minimal flavour violation, where the superficially leading contribution vanishes. Read More

We compute the leading-log QED, the next-to-leading-log QED-QCD, and the electroweak corrections to the charm quark contribution relevant for the rare decay K+ -> pi+ nu nu-bar. The corresponding parameter P_c(X) is increased by up to 2% with respect to the pure QCD estimate to P_c(X) = 0.372 +- 0. Read More

Combining our results for various O(alpha_s^2) corrections to the weak radiative B-meson decay, we are able to present the first estimate of the branching ratio at the next-to-next-to-leading order in QCD. We find BR(B -> X_s gamma) = (3.15 +_ 0. Read More

We calculate the charm-quark contribution to the decay K_L -> mu^+ mu^- in next-to-next-to-leading order of QCD. This new contribution reduces the theoretical uncertainty in the relevant parameter P_c from +/-22% down to +/-7%, corresponding to scale uncertainties of +/-3% and +/-6% in the short-distance part of the branching ratio and the determination of the Wolfenstein parameter rhobar from K_L -> mu^+ mu^-. The error in P_c = 0. Read More

We calculate the complete NNLO QCD corrections to the charm contribution of the rare decay K+ -> pi+ nu nu-bar. We encounter several new features, which were absent in lower orders. We discuss them in detail and present the results for the 2-loop matching conditions of the Wilson coefficients, the 3-loop anomalous dimensions, and the 2-loop matrix elements of the relevant operators that enter the NNLO renormalization group analysis of the Z-penguin and the electroweak box contribution. Read More

We calculate the charm quark contribution to the rare decay K+ -> pi+ nu anti-nu in the next-to-next-to-leading order of QCD. This new contribution reduces the theoretical uncertainty in the relevant parameter Pc from +/- 10.1% down to +/- 2. Read More

It is well known that a majorana mass induces a (small) transition magnetic moment. The converse is also true; in this paper we estimate the loop contribution of transition magnetic moments $[\mu]_{\alpha \beta}$ to the neutrino mass matrix $[m]_{\alpha \beta}$. We show that for hierarchical neutrino masses, the contribution of $[\mu]_{e \tau}$ to $[m]_{e \tau}$ can exceed the experimental value of $[m]_{e \tau}$. Read More

We calculate the complete three-loop O(alpha_s^3) anomalous dimension matrix for the dimension-five dipole operators that arise in the Standard Model after integrating out the top quark and the heavy electroweak bosons. Our computation completes the three-loop anomalous dimension matrix of operators that govern low-energy |Delta F| = 1 flavor-changing processes, and represents an important ingredient of the next-to-next-to-leading order QCD analysis of the Bbar -> X_s gamma decay. Read More

We compute the effective hamiltonian for non-leptonic |Delta F| = 1 decays in the standard model including next-to-next-to-leading order QCD corrections. In particular, we present the complete three-loop anomalous dimension matrix describing the mixing of current-current and QCD penguin operators. The calculation is performed in an operator basis which allows to consistently use fully anticommuting gamma_5 in dimensional regularization at an arbitrary number of loops. Read More

We complete the next-to-next-to-leading order QCD calculation of the branching ratio for B -> X_s l^+ l^- including recent results for the three-loop anomalous dimension matrix and two-loop matrix elements. These new contributions modify the branching ratio in the low-q^2 region, BR_ll, by about +1% and -4%, respectively. We furthermore discuss the appropriate normalization of the electromagnetic coupling alpha and calculate the dominant higher order electroweak effects, showing that, due to accidental cancellations, they change BR_ll by only -1. Read More

We compute the complete O(alphas^2) anomalous dimension matrix relevant for the b to s gamma, b to s gluon and b to s l+l- transitions in the standard model and some of its extensions. For radiative decays we confirm the results of Misiak and Munz, and of Chetyrkin, Misiak and Munz. The O(alphas^2) mixing of four-quark into semileptonic operators is instead a new result and represents one of the last missing ingredients of the next-to-next-to-leading-order analysis of rare semileptonic B meson decays. Read More

We perform an exhaustive analysis of the most general Higgs sector of the minimal left-right symmetric model (MLRM). We find that the CP properties of the vacuum state are connected to the Higgs spectrum: if CP is broken spontaneously, the MLRM does not approach the Standard Model in the limit of a decoupling left-right symmetry breaking scale. Depending on the size of the CP phases scenarios with extra non-decoupling flavor-violating doublet Higgses or very light SU(2) triplet Higgses emerge, both of which are ruled out by phenomenology. Read More

We analyze the CP violating ratio epsilon'/epsilon and rare K and B decays in the MSSM with minimal flavour and CP violation, including NLO QCD corrections and imposing constraints on the supersymmetric parameters coming from epsilon, B_{d,s}^0-\bar B_{d,s}^0 mixings, B to X_s gamma, Delta rho in the electroweak precision studies and from the lower bound on the neutral Higgs mass. We provide a compendium of phenomenologically relevant formulae in the MSSM. Denoting by T(Q) the MSSM prediction for a given quantity normalized to the Standard Model result we find the ranges: 0. Read More

We make the simple observation that there exists a universal unitarity triangle for all models, like the SM, the Two Higgs Doublet Models I and II and the MSSM with minimal flavour violation, that do not have any new operators beyond those present in the SM and in which all flavour changing transitions are governed by the CKM matrix with no new phases beyond the CKM phase. This universal triangle can be determined in the near future from the ratio (Delta M)_d/(Delta M)_s and sin(2 beta) measured first through the CP asymmetry in B_d^0 to psi K_S and later in K to pi nu nubar decays. Also suitable ratios of the branching ratios for B to X_{d,s} nu nubar and B_{d,s} to mu^+ mu^- and the angle gamma measured by means of CP asymmetries in B decays can be used for this determination. Read More

We analyze the CP violating ratio \epe=epsilon'/epsilon in the Standard Model in view of the new KTeV results. We review the present status of the most important non-perturbative parameters B_6, B_8, B_K and of the strange quark mass m_s. We also briefly discuss the issues of final state interactions and renormalization scheme dependence. Read More