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T. Hamada and E. E. Salpeter, Astrophys. J. 134
1961
Earlier work this paper cites.
G. R. Blumenthal, S. M. Faber, R. Flores and J. R. Primack, Astrophys. J. 301
1986
Earlier work this paper cites.
A. Gould, Astrophys. J. 388
1987
Earlier work this paper cites.
R. Kippenhahn and A. Weigert, Stellar Structure and Evolution, XVI, Springer-Verlag, Berlin, Heidelberg, New York (1994)
1994
Earlier work this paper cites.
J. F. Navarro, C. S. Frenk and S. D. M. White, Astrophys. J. 462
1997
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F. Prada et al
Original
1999
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F. Petriello and K. M. Zurek, arXiv:0806.3989 [hep-ph]; C. Savage, G. Gelmini, P. Gondolo and K. Freese, JCAP 0904
Original
2001
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S. Chang, G. D. Kribs, D. Tucker-Smith and N. Weiner, arXiv:0807.2250 [hep-ph]; D. R. Smith and N. Weiner, Phys. Rev. D 64
Original
2001
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2010

Hooper, Dan, Spolyar, Douglas, Vallinotto, Alberto et al.

Dark matter in the form of weakly interacting massive particles is predicted to become gravitationally captured and accumulate in stars.

While the subsequent annihilations of such particles lead to the injection of energy into stellar cores, elastically scattering dark matter particles do not generally yield enough energy to observably impact stellar phenomenology.
Dark matter particles which scatter inelastically with nuclei (such that they reconcile the annual modulation reported by DAMA with the null results of CDMS and other experiments), however, can be captured by and annihilate in compact stars at a much higher rate.
As a result, old white dwarf stars residing in high dark matter density environments can be prevented from cooling below several thousand degrees Kelvin.

T. Hamada and E. E. Salpeter, Astrophys. J. 134
1961
Earlier work this paper cites.
G. R. Blumenthal, S. M. Faber, R. Flores and J. R. Primack, Astrophys. J. 301
1986
Earlier work this paper cites.
A. Gould, Astrophys. J. 388
1987
Earlier work this paper cites.
R. Kippenhahn and A. Weigert, Stellar Structure and Evolution, XVI, Springer-Verlag, Berlin, Heidelberg, New York (1994)
1994
Earlier work this paper cites.
J. F. Navarro, C. S. Frenk and S. D. M. White, Astrophys. J. 462
1997
Earlier work this paper cites.
F. Prada et al
Original
1999
Earlier work this paper cites.
F. Petriello and K. M. Zurek, arXiv:0806.3989 [hep-ph]; C. Savage, G. Gelmini, P. Gondolo and K. Freese, JCAP 0904
Original
2001
Earlier work this paper cites.
S. Chang, G. D. Kribs, D. Tucker-Smith and N. Weiner, arXiv:0807.2250 [hep-ph]; D. R. Smith and N. Weiner, Phys. Rev. D 64
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2001
Earlier work this paper cites.
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2002
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A. Bottino, G. Fiorentini, N. Fornengo, B. Ricci, S. Scopel and F. L. Villante, Phys. Rev. D 66
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Cited alongside, same era.
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Cited alongside, same era.
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2007