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1988
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1991
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S. Colombi, S. Dodelson and L. M. Widrow, Astrophys. J. 458
1996
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X. -D. Shi and G. M. Fuller, Phys. Rev. Lett. 82
1999
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W. H. Press, P. Schechter ApJ, 187, 425 (1974); J. R. Bond, S. Cole, G. Efstathiou, N. Kaiser ApJ, 379, 440 (1991); R. K. Sheth, G. Tormen MNRAS, 308, 119 (1999) [arXiv:astro-ph/9901122]
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M. Kaplinghat, Phys. Rev. D 72
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K. Abazajian, Phys. Rev. D 73
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F. Bezrukov, H. Hettmansperger and M. Lindner, Phys. Rev. D 81
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2014

Production of Sterile Neutrino Dark Matter and the 3.5 keV line

Merle, Alexander, Schneider, Aurel

Understand

The recent observation of an X-ray line at an energy of 3.5 keV mainly from galaxy clusters has initiated a discussion about whether we may have seen a possible dark matter signal.

If confirmed, this signal could stem from a decaying sterile neutrino of a mass of 7.1 keV.
Such a particle could make up all the dark matter, but it is not clear how it was produced in the early Universe.
In this letter we show that it is possible to discriminate between different production mechanisms with present-day astronomical data.

Built on

J. Bernstein, Kinetic Theory In The Expanding Universe , University Press, Cambridge, USA, 1988
1988
Earlier work this paper cites.
B. W. Lee and S. Weinberg, Phys. Rev. Lett. 39
1991
Earlier work this paper cites.
S. Dodelson and L. M. Widrow, Phys. Rev. Lett. 72
1994
Earlier work this paper cites.
S. Colombi, S. Dodelson and L. M. Widrow, Astrophys. J. 458
1996
Earlier work this paper cites.
X. -D. Shi and G. M. Fuller, Phys. Rev. Lett. 82
1999
Earlier work this paper cites.
W. H. Press, P. Schechter ApJ, 187, 425 (1974); J. R. Bond, S. Cole, G. Efstathiou, N. Kaiser ApJ, 379, 440 (1991); R. K. Sheth, G. Tormen MNRAS, 308, 119 (1999) [arXiv:astro-ph/9901122]
1999
Earlier work this paper cites.
M. Kaplinghat, Phys. Rev. D 72
2005
Earlier work this paper cites.
K. Abazajian, Phys. Rev. D 73
2006
Earlier work this paper cites.
F. Bezrukov, H. Hettmansperger and M. Lindner, Phys. Rev. D 81
Original
2008
Earlier work this paper cites.
A. Kusenko, Phys. Rev. Lett. 97
Original
2008
Earlier work this paper cites.
K. Petraki, Phys. Rev. D 77
Original
2008
Earlier work this paper cites.
E. Aprile et al
Original
2009
Earlier work this paper cites.