Built on

J. R. Ellis, K. Enqvist, D. V. Nanopoulos and F. Zwirner, Mod. Phys. Lett. A 1
1986
Earlier work this paper cites.
R. Barbieri and G. F. Giudice, Nucl. Phys. B 306
1988
Earlier work this paper cites.
H. E. Haber and R. Hempfling, Phys. Rev. Lett. 66
1991
Earlier work this paper cites.
For calculations of radiative corrections to the h b b ¯ hb\bar{b} coupling, see for example: M. S. Carena, S. Mrenna and C. E. M. Wagner, Phys. Rev. D 60
1996
Earlier work this paper cites.
A. Djouadi, J. Kalinowski and M. Spira, Comput. Phys. Commun. 108
1998
Earlier work this paper cites.
H. E. Haber, M. J. Herrero, H. E. Logan, S. Penaranda, S. Rigolin and D. Temes, Phys. Rev. D 63
2001
Earlier work this paper cites.
B. C. Allanach, Comput. Phys. Commun. 143
2002
Earlier work this paper cites.
M. S. Carena and H. E. Haber, Prog. Part. Nucl. Phys. 50
2003
Earlier work this paper cites.

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2012

The Higgs Sector and Fine-Tuning in the pMSSM

Cahill-Rowley, Matthew W., Hewett, JoAnne L., Ismail, Ahmed et al.

Understand

The recent discovery of a 125 GeV Higgs, as well as the lack of any positive findings in searches for supersymmetry, has renewed interest in both the supersymmetric Higgs sector and fine-tuning.

Here, we continue our study of the phenomenological MSSM (pMSSM), discussing the light Higgs and fine-tuning within the context of two sets of previously generated pMSSM models.
We find an abundance of models with experimentally-favored Higgs masses and couplings.
We investigate the decay modes of the light Higgs in these models, finding strong correlations between many final states.

Built on

J. R. Ellis, K. Enqvist, D. V. Nanopoulos and F. Zwirner, Mod. Phys. Lett. A 1
1986
Earlier work this paper cites.
R. Barbieri and G. F. Giudice, Nucl. Phys. B 306
1988
Earlier work this paper cites.
H. E. Haber and R. Hempfling, Phys. Rev. Lett. 66
1991
Earlier work this paper cites.
For calculations of radiative corrections to the h b b ¯ hb\bar{b} coupling, see for example: M. S. Carena, S. Mrenna and C. E. M. Wagner, Phys. Rev. D 60
1996
Earlier work this paper cites.
A. Djouadi, J. Kalinowski and M. Spira, Comput. Phys. Commun. 108
1998
Earlier work this paper cites.
H. E. Haber, M. J. Herrero, H. E. Logan, S. Penaranda, S. Rigolin and D. Temes, Phys. Rev. D 63
2001
Earlier work this paper cites.
B. C. Allanach, Comput. Phys. Commun. 143
2002
Earlier work this paper cites.
M. S. Carena and H. E. Haber, Prog. Part. Nucl. Phys. 50
2003
Earlier work this paper cites.

Similar

S. Heinemeyer, W. Hollik and G. Weiglein, Phys. Rept. 425
2006
Cited alongside, same era.
A. Djouadi, J. L. Kneur and G. Moultaka, Comput. Phys. Commun. 176
2007
Cited alongside, same era.
A. Djouadi, M. M. Muhlleitner and M. Spira, Acta Phys. Polon. B 38
2007
Cited alongside, same era.
S. P. Martin and M. T. Vaughn, Phys. Rev. D 50
2008
Cited alongside, same era.
C. F. Berger, J. S. Gainer, J. L. Hewett and T. G. Rizzo, JHEP 0902
Original
2011
Cited alongside, same era.
G. L. Kane, G. D. Kribs, S. P. Martin and J. D. Wells, Phys. Rev. D 53
Original
2011
Cited alongside, same era.