Mirror matter-type dark matter

Details Mirror matter-type dark matter Mirror matter-type dark matter

2004-07-30

arxiv.org/abs/astro-ph/0407623v1

Int.J.Mod.Phys.D13:2161-2192,2004

Astronomy and Astrophysics

Astrophysics

about 30 pages

Scientific paper

10.1142/S0218271804006449

There are six main things which any non-baryonic dark matter theory should endeavour to explain: (1) The basic dark matter particle properties [mass, stability, darkness]; (2) The similarity in cosmic abundance between ordinary and non-baryonic dark matter, $\Omega_B \sim \Omega_{dark}$; (3) Large scale structure formation; (4) Microlensing (MACHO) events; (5) Asymptotically flat rotation curves in spiral galaxies; (6) The impressive DAMA/NaI annual modulation signal. Only mirror matter-type dark matter is capable of explaining all six of these desirable features. The purpose of this article is to provide an up-to-date and pedagogical review of this dark matter candidate.

Affiliated with

Also associated with

No associations

Rating

Mirror matter-type dark matter does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Mirror matter-type dark matter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mirror matter-type dark matter will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-503296