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WIMPless Dark Matter · Around

2009

WIMPless Dark Matter

Feng, Jonathan L., Kumar, Jason

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We describe the scenario of WIMPless dark matter.

In this scenario of gauge-mediated supersymmetry breaking, a dark matter candidate in the hidden sector is found to naturally have approximately the right relic density to explain astronomical dark matter observations, but with a wide range of possible masses.

Built on

M. Dine, W. Fischler and M. Srednicki, Nucl. Phys. B 189
1982
Earlier work this paper cites.
Ya. B. Zeldovich, Adv. Astron. Astrophys. 3
1986
Earlier work this paper cites.
K. Griest and M. Kamionkowski, Phys. Rev. Lett. 64
1990
Earlier work this paper cites.

Similar

M. Dine, A. E. Nelson and Y. Shirman, Phys. Rev. D 51
1996
Cited alongside, same era.
J. L. Feng and J. Kumar, Phys. Rev. Lett. 101
Original
2008
Cited alongside, same era.
J. L. Feng, J. Kumar and L. E. Strigari, Phys. Lett. B 670
Original
2008
Cited alongside, same era.
D. Hooper and K. M. Zurek, arXiv:0801.3686 [hep-ph]
Original
Cited in the paper.

Then

J. L. Feng, H. Tu and H. B. Yu, JCAP 0810
Original
2009
Closest in time.
K. M. Zurek, Phys. Rev. D 79
Original
2009
Closest in time.

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