4.4 Article

Heavy Majorana neutrinos from Wγ fusion at hadron colliders

期刊

JOURNAL OF HIGH ENERGY PHYSICS
卷 -, 期 2, 页码 -

出版社

SPRINGER
DOI: 10.1007/JHEP02(2015)072

关键词

Beyond Standard Model; Neutrino Physics

资金

  1. Brazilian agency FAPESP
  2. U.S. Department of Energy [DE-FG02-95ER40896]
  3. PITT-PACC
  4. University of Pittsburgh
  5. generosity of the Institute for High Energy Physics Center for Future High Energy Physics
  6. Korea Institute for Advance Science
  7. National Research Foundation of Korea [00000001] Funding Source: Korea Institute of Science & Technology Information (KISTI), National Science & Technology Information Service (NTIS)

向作者/读者索取更多资源

Vector boson fusion processes become increasingly more important at higher collider energies and for probing larger mass scales due to collinear logarithmic enhancements of the cross section. In this context, we revisit the production of a hypothetic heavy Majorana neutrino (N) at hadron colliders. Particular attention is paid to the fusion process W gamma -> Nl(+/-). We systematically categorize the contributions from a photon initial state in the elastic, inelastic, and deeply inelastic channels. Comparing with the leading channel via the Drell-Yan production q (q) over bar' -> W* -> Nl(+/-) at NNLO in QCD, we find that the W gamma fusion process becomes relatively more important at higher scales, surpassing the DY mechanism at m(N) similar to 1 TeV (770 GeV), at the 14TeV LHC (100TeV VLHC). We investigate the inclusive heavy Majorana neutrino signal, including QCD corrections, and quantify the Standard Model backgrounds at future hadron colliders. We conclude that, with the currently allowed mixing vertical bar V-mu N vertical bar(2) < 6 x 10(-3), a 5 sigma discovery can be made via the same-sign dimuon channel for m(N) = 530 (1070) GeV at the 14TeV LHC (100TeV VLHC) after 1 ab(-1). Reversely, for m(N) = 500GeV and the same integrated luminosity, a mixing vertical bar V-mu N vertical bar(2) of the order 1.1 x 10(-3) (2.5 x 10(-4)) may be probed.

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