Identification of dark matter is one of the most urgent problems in cosmology. I describe the astrophysical case for dark matter, from both an observational and a theoretical perspective.
Lʼidentification de la matière noire est lʼun des problèmes les plus urgents de lʼastrophysique. Je décris lʼaspect astrophysique du problème, dans une perspective observationnelle autant que théorique.
Mot clés : Matière noire, Astrophysique
Joseph Silk 1
@article{CRPHYS_2012__13_6-7_724_0, author = {Joseph Silk}, title = {Dark matter: {The} astrophysical case}, journal = {Comptes Rendus. Physique}, pages = {724--729}, publisher = {Elsevier}, volume = {13}, number = {6-7}, year = {2012}, doi = {10.1016/j.crhy.2012.06.002}, language = {en}, }
Joseph Silk. Dark matter: The astrophysical case. Comptes Rendus. Physique, Volume 13 (2012) no. 6-7, pp. 724-729. doi : 10.1016/j.crhy.2012.06.002. https://comptes-rendus.academie-sciences.fr/physique/articles/10.1016/j.crhy.2012.06.002/
[1] Helv. Phys. Acta, 6 (1933), pp. 110-127
[2] arXiv
, 2012 |[3] Publ. Astron. Soc. Japan, 64 (2012) no. 2
[4] Astron. Astrophys., 26 (1973), p. 483
[5] Astrophys. J. Lett., 225 (1978), p. L107
[6] Astrophys. J., 159 (1970), p. 379
[7] Ann. Rev. Astron. Astrophys., 39 (2001), p. 137
[8] Astrophys. J., 176 (1972), p. 315
[9] Astrophys. J., 160 (1970), p. 811
[10] Astrophys. J. Lett., 193 (1974), p. L1
[11] Nature, 250 (1974), p. 309
[12] J. Sellwood, Review, in: G. Gilmore (Ed.), Planets, Stars and Stellar Systems, vol. 5, in press, , 2010. | arXiv
[13] Astrophys. J., 723 (2010), p. 54
[14] Astrophys. J., 294 (1985), p. 494
[15] Astrophys. J., 483 (1997), p. 103
[16] arXiv
, 2012 |[17] Astrophys. J., 696 (2009), p. 2179
[18] Mon. Not. Roy. Astron. Soc., 415 (2011), p. L40
[19] Nature, 442 (2006), p. 539
[20] Mon. Not. Roy. Astron. Soc., 421 (2012), p. 3464 | arXiv
[21] Astron. J., 142 (2011), p. 24 | arXiv
[22] Mon. Not. Roy. Astron. Soc., 397 (2009), p. 44 | arXiv
[23] Mon. Not. Roy. Astron. Soc., 416 (2011), p. 2318 | arXiv
[24] et al. Astrophys. J., 742 (2011), p. 117
[25] Astrophys. J., 738 (2011), p. 41
[26] et al. Astrophys. J., 664 (2007), p. 123
[27] et al. Astrophys. J., 737 (2011), p. 74
[28] ARAA, 49 (2011), pp. 409-470
[29] Mon. Not. Roy. Astron. Soc., 227 (1987), pp. 1-27
[30] et al. Mon. Not. Roy. Astron. Soc., 415 (2011), p. 2892 | arXiv
[31] et al. Mon. Not. Roy. Astron. Soc., 418 (2011), p. 1707 | arXiv
[32] et al., 2012 | arXiv
[33] et al. Astrophys. J., 749 (2012), p. 90
[34] Astrophys. J., 743 (2011), p. 28
[35] arXiv
, 2012 (Phys. Rep.) |[36] et al. Mon. Not. Roy. Astron. Soc., 423 (2012), p. 1726 | arXiv
[37] Mon. Not. Roy. Astron. Soc., 419 (2012), p. 771 | arXiv
[38] Astrophys. J. Lett., 744 (2012), p. L9 | arXiv
[39] et al. Nature, 463 (2010), pp. 203-206
[40] Astrophys. J., 725 (2011), p. 556
[41] Astrophys. J., 741 (2011), p. 18 | arXiv
[42] Mon. Not. Roy. Astron. Soc., 402 (2010), p. 1995
[43] Adv. Astron. (2010) (article id. 281913) | arXiv
[44] Mon. Not. Roy. Astron. Soc., 422 (2012), p. 1203 | arXiv
[45] I. Ferrero, M.G. Abadi, J.F. Navarro, L.V. Sales, S. Gurovich, Mon. Not. Roy. Astron. Soc., submitted for publication, , 2011. | arXiv
[46] Mon. Not. Roy. Astron. Soc., 415 (2011), p. 257 | arXiv
[47] et al. Mon. Not. Roy. Astron. Soc., 424 (2012), p. 1105 | arXiv
[48] Mon. Not. Roy. Astron. Soc., 397 (2009), p. 1776
[49] et al. Mon. Not. Roy. Astron. Soc., 415 (2011), p. 3571 | arXiv
[50] et al. Astron. Astrophys., 533 (2011), p. 119 | arXiv
[51] Astrophys. J., 729 (2011), p. 118 | arXiv
[52] Astrophys. J., 735 (2011), p. L13
[53] Astron. Astrophys., 512 (2010), p. 17 | arXiv
[54] Astrophys. J., 270 (1983), p. 365
[55] Phys. Rev. Lett., 106 (2011), p. 121303 | arXiv
[56] Astrophys. J., 714 (2010), p. 320
[57] Astrophys. J., 719 (2010), pp. 119-125
[58] Mon. Not. Roy. Astron. Soc., 407 (2010), p. 263 | arXiv
[59] arXiv
, 2011 (Astrophys. J.) |[60] Mon. Not. Roy. Astron. Soc., 407 (2010), pp. 2328-2338
[61] Astrophys. J., 712 (2010), p. L81-L85
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