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Astrophysical tests of mirror dark matter · Around

2008

Astrophysical tests of mirror dark matter

Ciarcelluti, P.

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Understand

Mirror matter is a self-collisional dark matter candidate.

If exact mirror parity is a conserved symmetry of the nature, there could exist a parallel hidden (mirror) sector of the Universe which has the same kind of particles and the same physical laws of our (visible) sector.
The two sectors interact each other only via gravity, therefore mirror matter is naturally "dark".
The most promising way to test this dark matter candidate is to look at its astrophysical signatures, as Big Bang nucleosynthesis, primordial structure formation and evolution, cosmic microwave background and large scale structure power spectra.

Built on

T. D. Lee, and C. N. Yang, Phys. Rev. , 104
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Z.G. Berezhiani, A.D. Dolgov, and R.N. Mohapatra, Phys. Lett. B , 375
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S. Blinnikov, astro-ph/9801015; R. Foot, Phys. Lett. B , 452
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Similar

Z. Berezhiani, D. Comelli and F. L. Villante, Phys. Lett. B , 503
2001
Cited alongside, same era.
A.Yu. Ignatiev, and R.R. Volkas, Phys. Rev. D , 68
2003
Cited alongside, same era.
P. Ciarcelluti, PhD thesis , [astro-ph/0312607]; Z. Berezhiani, P. Ciarcelluti, D. Comelli, and F. Villante, Int. J. Mod. Phys. D , 14
2004
Cited alongside, same era.
L. B. Okun, hep-ph/0606202
Cited in the paper.
P. Ciarcelluti, A. Lepidi, arXiv:0809.0677
Original
Cited in the paper.

Then

P. Ciarcelluti, Int. J. Mod. Phys. D , 14
2005
Later among the works it cites.
P. Ciarcelluti, Int. J. Mod. Phys. D , 14
2005
Later among the works it cites.
Z. Berezhiani, P. Ciarcelluti, S. Cassisi, A. Pietrinferni, Astropart. Phys. 24
2006
Later among the works it cites.

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