Constraining Asymmetric Bosonic Non-interacting Dark Matter with Neutron Stars

Details Constraining Asymmetric Bosonic Non-interacting Dark Matter with Neutron Stars Constraining Asymmetric Bosonic Non-interacting Dark Matter with Neutron Stars

2012-04-11

arxiv.org/abs/1204.2564v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

Scientific paper

The Hawking evaporation of small black holes formed by the collapse of dark matter at the center of neutron stars plays a key role in loosing the constraint on the mass of asymmetric bosonic non-interacting dark matter particles. Different from previous works we show that such a kind of dark matter is viable in the mass range from 3.3 GeV to ~ 10 TeV, which covers the most attractive regions, including the preferred asymmetric dark matter mass ~ 5.7 GeV as well as the 5-15 GeV range favored by DAMA and CoGeNT.

Affiliated with

Also associated with

No associations

Rating

Constraining Asymmetric Bosonic Non-interacting Dark Matter with Neutron Stars 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 Constraining Asymmetric Bosonic Non-interacting Dark Matter with Neutron Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Constraining Asymmetric Bosonic Non-interacting Dark Matter with Neutron Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-311325