Built on

G. Angloher, M. Bauer, I. Bavykina, A. Bento, C. Bucci, C. Ciemniak, G. Deuter and F. von Feilitzsch et al
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2013

Cornering light Neutralino Dark Matter at the LHC

Calibbi, Lorenzo, Lindert, Jonas M., Ota, Toshihiko et al.

Understand

We investigate the current status of the light neutralino dark matter scenario within the minimal supersymmetric standard model (MSSM) taking into account latest results from the LHC.

A discussion of the relevant constraints, in particular from the dark matter relic abundance, leads us to a manageable simplified model defined by a subset of MSSM parameters.
Within this simplified model we reinterpret a recent search for electroweak supersymmetric particle production based on a signature including multi-taus plus missing transverse momentum performed by the ATLAS collaboration.
In this way we derive stringent constraints on the light neutralino parameter space.

Built on

G. Angloher, M. Bauer, I. Bavykina, A. Bento, C. Bucci, C. Ciemniak, G. Deuter and F. von Feilitzsch et al
Original
1971
Earlier work this paper cites.
B. W. Lee and S. Weinberg, Phys. Rev. Lett. 39
1977
Earlier work this paper cites.
J. R. Ellis, J. M. Frère, J. S. Hagelin, G. L. Kane and S. T. Petcov, Phys. Lett. B 132
1983
Earlier work this paper cites.
A. Bartl, H. Fraas and W. Majerotto, Nucl. Phys. B 278
1986
Earlier work this paper cites.
R. Barbieri, G. Gamberini, G. F. Giudice and G. Ridolfi, Phys. Lett. B 195
1987
Earlier work this paper cites.
K. Griest and H. E. Haber, Phys. Rev. D 37
1988
Earlier work this paper cites.
H. Baer, C.-H. Chen, F. Paige and X. Tata, Phys. Rev. D 49
1994
Earlier work this paper cites.
C. G. Lester and D. J. Summers, Phys. Lett. B 463
1999
Earlier work this paper cites.
M. Dobbs and J. B. Hansen, Comput. Phys. Commun. 134
2001
Earlier work this paper cites.
D. Hooper and T. Plehn, Phys. Lett. B 562
2003
Earlier work this paper cites.
A. Bottino, N. Fornengo and S. Scopel, Phys. Rev. D 67
2003
Earlier work this paper cites.
A. J. Buras, P. H. Chankowski, J. Rosiek and Ł. Sławianowska, Nucl. Phys. B 659
2003
Earlier work this paper cites.
A. Barr, C. Lester and P. Stephens, J. Phys. G 29
2003
Earlier work this paper cites.
A. Bottino, F. Donato, N. Fornengo and S. Scopel, Phys. Rev. D 70
2004
Earlier work this paper cites.
G. Abbiendi et al
2004
Earlier work this paper cites.
A. Birkedal, K. Matchev and M. Perelstein, Phys. Rev. D 70
2004
Earlier work this paper cites.
S. Schael et al
2006
Earlier work this paper cites.
G. Isidori and P. Paradisi, Phys. Lett. B 639
2006
Earlier work this paper cites.
A. Djouadi, J.-L. Kneur and G. Moultaka, Comput. Phys. Commun. 176
2007
Earlier work this paper cites.
A. Djouadi, M. M. Mühlleitner and M. Spira, Acta Phys. Polon. B 38
2007
Earlier work this paper cites.
C. E. Yaguna, Phys. Rev. D 76
Original
2007
Earlier work this paper cites.
R. Bernabei et al
Original
2008
Earlier work this paper cites.
A. Bottino, F. Donato, N. Fornengo and S. Scopel, Phys. Rev. D 78
Original
2008
Earlier work this paper cites.
S. Heinemeyer, W. Hollik, A. M. Weber and G. Weiglein, JHEP 0804
Original
2008
Earlier work this paper cites.
M. Bahr, S. Gieseke, M. A. Gigg, D. Grellscheid, K. Hamilton, O. Latunde-Dada, S. Platzer and P. Richardson et al
Original
2008
Earlier work this paper cites.