Built on

K. Griest and H. E. Haber, Phys. Rev. D 37, 719 (1988); A. Djouadi, J. Kalinowski and P. M. Zerwas, Z. Phys. C 57, 569 (1993); G. G. Ross and K. Schmidt-Hoberg, arXiv:1108.1284
Original
1993
Earlier work this paper cites.
K. Belotsky, D. Fargion, M. Khlopov, R. Konoplich, K. Shibaev, Phys. Rev. D 68 (2003) 054027 [arXiv:
2003
Earlier work this paper cites.
R. Barate
2003
Earlier work this paper cites.
A. Datta, K. Huitu, J. Laamanen and B. Mukhopadhyaya, Phys. Rev. D 70, 075003 (2004) [arXiv:hep-ph/0404056]
2004
Earlier work this paper cites.
R. Shrock, M. Suzuki, Phys. Lett. B 110 (1982) 250; O. J. P. Eboli and D. Zeppenfeld, Phys. Lett. B 495, 147 (2000) [arXiv:hep-ph/0009158]; R. M. Godbole, M. Guchait, K. Mazumdar, S. Moretti and D. P. Roy, Phys. Lett. B 571, 184 (2003) [arXiv:hep-ph/0304137]; M. Duhrssen, S. Heinemeyer, H. Logan, D. Rainwater, G. Weiglein and D. Zeppenfeld, Phys. Rev. D 70, 113009 (2004) [arXiv:hep-ph/0406323]; H. Davoudiasl, T. Han and H. E. Logan, Phys. Rev. D 71, 115007 (2005) [arXiv:hep-ph/0412269]
2005
Earlier work this paper cites.
R. Schabinger and J. D. Wells, Phys. Rev. D 72, 093007 (2005)
2005
Earlier work this paper cites.

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2011

Raidal, Martti, Strumia, Alessandro

We reconsider Higgs boson invisible decays into Dark Matter in the light of recent Higgs searches at the LHC.

Present hints in the CMS and ATLAS data favor a non-standard Higgs boson with approximately 50% invisible branching ratio, and mass around 143 GeV.
This situation can be realized within the simplest thermal scalar singlet Dark Matter model, predicting a Dark Matter mass around 50 GeV and direct detection cross section just below present bound.
The present runs of the Xenon100 and LHC experiments can test this possibility.

K. Griest and H. E. Haber, Phys. Rev. D 37, 719 (1988); A. Djouadi, J. Kalinowski and P. M. Zerwas, Z. Phys. C 57, 569 (1993); G. G. Ross and K. Schmidt-Hoberg, arXiv:1108.1284
Original
1993
Earlier work this paper cites.
K. Belotsky, D. Fargion, M. Khlopov, R. Konoplich, K. Shibaev, Phys. Rev. D 68 (2003) 054027 [arXiv:
2003
Earlier work this paper cites.
R. Barate
2003
Earlier work this paper cites.
A. Datta, K. Huitu, J. Laamanen and B. Mukhopadhyaya, Phys. Rev. D 70, 075003 (2004) [arXiv:hep-ph/0404056]
2004
Earlier work this paper cites.
R. Shrock, M. Suzuki, Phys. Lett. B 110 (1982) 250; O. J. P. Eboli and D. Zeppenfeld, Phys. Lett. B 495, 147 (2000) [arXiv:hep-ph/0009158]; R. M. Godbole, M. Guchait, K. Mazumdar, S. Moretti and D. P. Roy, Phys. Lett. B 571, 184 (2003) [arXiv:hep-ph/0304137]; M. Duhrssen, S. Heinemeyer, H. Logan, D. Rainwater, G. Weiglein and D. Zeppenfeld, Phys. Rev. D 70, 113009 (2004) [arXiv:hep-ph/0406323]; H. Davoudiasl, T. Han and H. E. Logan, Phys. Rev. D 71, 115007 (2005) [arXiv:hep-ph/0412269]
2005
Earlier work this paper cites.
R. Schabinger and J. D. Wells, Phys. Rev. D 72, 093007 (2005)
2005
Earlier work this paper cites.

R. Barbieri, L. J. Hall and V. S. Rychkov, Phys. Rev. D 74, 015007 (2006) [arXiv:hep-ph/0603188]
2006
Cited alongside, same era.
M. J. Strassler and K. M. Zurek, Phys. Lett. B 651, 374 (2007)
2007
Cited alongside, same era.
J. McDonald, Phys. Rev. D 50, 3637 (1994); C. P. Burgess, M. Pospelov and T. ter Veldhuis, Nucl. Phys. B 619, 709 (2001); V. Barger
2008
Cited alongside, same era.
DAMA Collaboration, Eur. Phys. J. C56 (2008) 333 [arXiv:
Original
2008
Cited alongside, same era.
ATLAS note ATL-PHYS-PUB-2009-061,
2009
Cited alongside, same era.
M. Kadastik, K. Kannike and M. Raidal, Phys. Rev. D 81, 015002 (2010) [arXiv:0903.2475]
Original

alphaXiv searches the wider corpus for related work and actual follow-ups.

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2010

Cited alongside, same era.

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