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2016

Status of CMSSM in light of current LHC Run-2 and LUX data

Han, Chengcheng, Hikasa, Ken-ichi, Wu, Lei et al.

Understand

Motivated by the latest results of the LHC Run-2 and LUX experiments, we examine the status of the constrained minimal supersymmetric standard model (CMSSM) by performing a global fit.

We construct a likelihood function including the electroweak precision observables, $B$-physics measurements, LHC Run-1 and -2 data of SUSY direct searches, Planck observation of the dark matter relic density and the combined LUX Run-3 and -4 detection limits.
Based on the profile likelihood functions of 1 billion samples, we obtain the following observations: (i) The stau coannihilation region has been mostly excluded by the latest LHC Run-2 data; (ii) The focus point region has been largely covered by the LUX-2016 limits while the $A$-funnel region has been severely restricted by flavor observables like $B_s \to \mu^+\mu^-$.
The remaining parts of both regions will be totally covered by the future LZ dark matter experiment; (iii) The masses of the stop, the lightest neutralino and the gluino have been pushed up to 1033 GeV, 449 GeV and 2285 GeV, respectively.

Built on

R. Barbieri and G. F. Giudice, Nucl. Phys. B 306
1988
Earlier work this paper cites.
G. L. Kane, C. F. Kolda, L. Roszkowski and J. D. Wells, Phys. Rev. D 49
1994
Earlier work this paper cites.
J. L. Feng, K. T. Matchev and T. Moroi, Phys. Rev. D 61
2000
Earlier work this paper cites.
S. Heinemeyer, W. Hollik and G. Weiglein, Comput. Phys. Commun. 124
2000
Earlier work this paper cites.
C. Boehm, A. Djouadi and M. Drees, Phys. Rev. D 62
2000
Earlier work this paper cites.
B. C. Allanach, Comput. Phys. Commun. 143
2002
Earlier work this paper cites.
J. R. Ellis, K. A. Olive and Y. Santoso, Astropart. Phys. 18
2003
Earlier work this paper cites.
Y. Santoso, Nucl. Phys. Proc. Suppl. 124
2003
Earlier work this paper cites.
J. Edsjo, M. Schelke, P. Ullio and P. Gondolo, JCAP 0304
2003
Earlier work this paper cites.
R. R. de Austri, R. Trotta, L. Roszkowski, JHEP 0605
2006
Earlier work this paper cites.
G. Belanger, F. Boudjema, A. Pukhov and A. Semenov, Comput. Phys. Commun. 149
2006
Earlier work this paper cites.
S. Schael et al
2006
Earlier work this paper cites.
T. Sjostrand, S. Mrenna and P. Z. Skands, JHEP 0605
2006
Earlier work this paper cites.
R. Ruiz de Austri, R. Trotta and L. Roszkowski, JHEP 0605
2006
Earlier work this paper cites.
F. Mahmoudi, Comput. Phys. Commun. 180
Original
2009
Earlier work this paper cites.
K. Hagiwara, R. Liao, A. D. Martin, D. Nomura and T. Teubner, J. Phys. G 38
Original
2011
Earlier work this paper cites.
B. Allanach, Phys.Rev. D83
2011
Earlier work this paper cites.
N. Chen, D. Feldman, Z. Liu, P. Nath and G. Peim, Phys. Rev. D 83
Original
2011
Earlier work this paper cites.
G. Aad et al
Original
2012
Earlier work this paper cites.
S. Chatrchyan et al
Original
2012
Earlier work this paper cites.
O. Buchmueller et al
Original
2012
Earlier work this paper cites.
J. Cao, Z. Heng, J. M. Yang and J. Zhu, JHEP 1210
Original
2012
Earlier work this paper cites.