Built on

R. Howl, S. F. King, JHEP 0801
Original
1909
Earlier work this paper cites.
J. Ellis, J.S. Hagelin, D.V. Nanopoulos, K.A. Olive and M. Srednicki, Nucl. Phys. B 238
1983
Earlier work this paper cites.
J. E. Kim and H. P. Nilles, Phys. Lett. B 138
Original
1984
Earlier work this paper cites.
P. Binetruy, S. Dawson, I. Hinchliffe, M. Sher, Nucl. Phys. B 273
1987
Earlier work this paper cites.
H. Yuksel, M. D. Kistler and T. Stanev, arXiv:0810.2784 [astro-ph]; D. Hooper, P. Blasi and P. D. Serpico, arXiv:0810.1527 [astro-ph]; I. Buesching, O. C. de Jager, M. S. Potgieter and C. Venter, arXiv:0804.0220 [astro-ph]; L. Zhang and K. S. Cheng, Astron. Astrophys. 368
Original
1995
Earlier work this paper cites.

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Later among the works it cites.
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J. R. Ellis and K. A. Olive, Phys. Lett. B 514
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2009

Neutralino Dark Matter with Inert Higgsinos and Singlinos

Hall, Jonathan P., King, Stephen F.

Understand

We discuss neutralino dark matter arising from supersymmetric models with extra inert Higgsinos and singlinos, where inert means that their scalar partners do not get vacuum expectation values.

As an example, we consider the extended neutralino sector of the E$_6$SSM, which predicts three families of Higgs doublet pairs, plus three singlets, plus a $Z'$, together with their fermionic superpartners.
We show that the two families of inert doublet Higgsinos and singlinos predicted by this model provide an almost decoupled neutralino sector with a naturally light LSP which can account for the cold dark matter relic abundance independently of the rest of the model, providing that the ratio of the two usual Higgs doublets satisfies tan beta < 2.

Built on

R. Howl, S. F. King, JHEP 0801
Original
1909
Earlier work this paper cites.
J. Ellis, J.S. Hagelin, D.V. Nanopoulos, K.A. Olive and M. Srednicki, Nucl. Phys. B 238
1983
Earlier work this paper cites.
J. E. Kim and H. P. Nilles, Phys. Lett. B 138
Original
1984
Earlier work this paper cites.
P. Binetruy, S. Dawson, I. Hinchliffe, M. Sher, Nucl. Phys. B 273
1987
Earlier work this paper cites.
H. Yuksel, M. D. Kistler and T. Stanev, arXiv:0810.2784 [astro-ph]; D. Hooper, P. Blasi and P. D. Serpico, arXiv:0810.1527 [astro-ph]; I. Buesching, O. C. de Jager, M. S. Potgieter and C. Venter, arXiv:0804.0220 [astro-ph]; L. Zhang and K. S. Cheng, Astron. Astrophys. 368
Original
1995
Earlier work this paper cites.

Similar

G. Jungman, M. Kamionkowski and K. Griest, Phys. Rept. 267
1996
Cited alongside, same era.
G. L. Kane and S. F. King, Phys. Lett. B 451
1999
Cited alongside, same era.
G. L. Kane, C. F. Kolda, L. Roszkowski and J. D. Wells, Phys. Rev. D 49
2002
Cited alongside, same era.
For a recent review see e.g. D. J. H. Chung, L. L. Everett, G. L. Kane, S. F. King, J. Lykken, L. T. Wang, Phys. Rept. 407
2005
Cited alongside, same era.
G. Belanger, F. Boudjema, A. Pukhov and A. Semenov, arXiv:0803.2360 [hep-ph]; G. Belanger, F. Boudjema, A. Pukhov and A. Semenov, Comput. Phys. Commun. 176
Original
2006
Cited alongside, same era.
P. Athron, S. F. King, D. J. Miller, S. Moretti and R. Nevzorov, arXiv:0904.2169 [hep-ph]; P. Athron, S. F. King, D. J. 2. Miller, S. Moretti and R. Nevzorov, arXiv:0901.1192 [hep-ph]

Then

S. F. King, S. Moretti, R. Nevzorov, Phys. Rev. D 73
2007
Later among the works it cites.
S. F. King, S. Moretti, R. Nevzorov, Phys. Lett. B 650
2007
Later among the works it cites.
J. R. Ellis and K. A. Olive, Phys. Lett. B 514
Original
2007
Later among the works it cites.
S. F. King, R. Luo, D. J. Miller, R. Nevzorov, JHEP 0812
2008
Later among the works it cites.
J. Dunkley et al
2009
Closest in time.