Built on

A. H. Chamseddine, R. L. Arnowitt and P. Nath, Phys. Rev. Lett. 49
1983
Earlier work this paper cites.
For some early work, see V. M. Chechetkin, M. Y. Khlopov and M. G. Sapozhnikov, Riv. Nuovo Cim. 5N10
1985
Earlier work this paper cites.
T. Moroi, H. Murayama and M. Yamaguchi, Phys. Lett. B 303
1993
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G. F. Giudice and R. Rattazzi, Phys. Rept. 322
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G. D. Kribs and I. Z. Rothstein, Phys. Rev. D 55
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A. Brignole, F. Feruglio, M. L. Mangano and F. Zwirner, Nucl. Phys. B 526
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For a review, see G. D’Ambrosio, G. F. Giudice, G. Isidori and A. Strumia, Nucl. Phys. B 645
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B. C. Allanach, Comput. Phys. Commun. 143
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J. L. Feng, S. Su and F. Takayama, Phys. Rev. D 70
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M. Kawasaki, K. Kohri and T. Moroi, Phys. Rev. D 71
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W. Beenakker, R. Hopker, M. Spira and P. M. Zerwas, Nucl. Phys. B 492
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For an overview of MSSM physics and phenomenology, see M. Drees, R. Godbole, P. Roy, “Theory and phenomenology of sparticles: An account of four-dimensional N=1 supersymmetry in high energy physics,” Hackensack, USA: World Scientific (2004) 555 p; H. Baer, X. Tata, “Weak scale supersymmetry: From superfields to scattering events,” Cambridge, UK: Univ. Pr. (2006) 537 p; S. P. Martin, In *Kane, G.L. (ed.): Perspectives on supersymmetry II* 1-153 [hep-ph/9709356]; H. K. Dreiner, H. E. Haber and S. P. Martin, Phys. Rept. 494
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K. Jedamzik, Phys. Rev. D 74
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2012

The New Look pMSSM with Neutralino and Gravitino LSPs

Cahill-Rowley, Matthew W., Hewett, JoAnne L., Hoeche, Stefan et al.

Understand

The pMSSM provides a broad perspective on SUSY phenomenology.

In this paper we generate two new, very large, sets of pMSSM models with sparticle masses extending up to 4 TeV, where the lightest supersymmetric particle (LSP) is either a neutralino or gravitino.
The existence of a gravitino LSP necessitates a detailed study of its cosmological effects and we find that Big Bang Nucleosynthesis places strong constraints on this scenario.
Both sets are subjected to a global set of theoretical, observational and experimental constraints resulting in a sample of \sim 225k viable models for each LSP type.

Built on

A. H. Chamseddine, R. L. Arnowitt and P. Nath, Phys. Rev. Lett. 49
1983
Earlier work this paper cites.
For some early work, see V. M. Chechetkin, M. Y. Khlopov and M. G. Sapozhnikov, Riv. Nuovo Cim. 5N10
1985
Earlier work this paper cites.
T. Moroi, H. Murayama and M. Yamaguchi, Phys. Lett. B 303
1993
Earlier work this paper cites.
G. F. Giudice and R. Rattazzi, Phys. Rept. 322
1996
Earlier work this paper cites.
G. D. Kribs and I. Z. Rothstein, Phys. Rev. D 55
1997
Earlier work this paper cites.
A. Brignole, F. Feruglio, M. L. Mangano and F. Zwirner, Nucl. Phys. B 526
2000
Earlier work this paper cites.
For a review, see G. D’Ambrosio, G. F. Giudice, G. Isidori and A. Strumia, Nucl. Phys. B 645
2002
Earlier work this paper cites.
B. C. Allanach, Comput. Phys. Commun. 143
2002
Earlier work this paper cites.
M. Fujii and T. Yanagida, Phys. Lett. B 549
2002
Earlier work this paper cites.
A. L. Read, J. Phys. G G 28
2002
Earlier work this paper cites.
J. L. Feng, S. Su and F. Takayama, Phys. Rev. D 70
2004
Earlier work this paper cites.
X. -L. Chen and M. Kamionkowski, Phys. Rev. D 70
2004
Earlier work this paper cites.
M. Kawasaki, K. Kohri and T. Moroi, Phys. Rev. D 71
2005
Earlier work this paper cites.
W. Beenakker, R. Hopker, M. Spira and P. M. Zerwas, Nucl. Phys. B 492
2005
Earlier work this paper cites.
For an overview of MSSM physics and phenomenology, see M. Drees, R. Godbole, P. Roy, “Theory and phenomenology of sparticles: An account of four-dimensional N=1 supersymmetry in high energy physics,” Hackensack, USA: World Scientific (2004) 555 p; H. Baer, X. Tata, “Weak scale supersymmetry: From superfields to scattering events,” Cambridge, UK: Univ. Pr. (2006) 537 p; S. P. Martin, In *Kane, G.L. (ed.): Perspectives on supersymmetry II* 1-153 [hep-ph/9709356]; H. K. Dreiner, H. E. Haber and S. P. Martin, Phys. Rept. 494
Original
2006
Earlier work this paper cites.
K. Jedamzik, Phys. Rev. D 74
2006
Earlier work this paper cites.
M. Kaplinghat and A. Rajaraman, Phys. Rev. D 74
2006
Earlier work this paper cites.