Superfluidity of &#923-Hyperons Admixed in Neutron Star Cores

Details Superfluidity of &#923-Hyperons Admixed in Neutron Star Cores Superfluidity of &#923-Hyperons Admixed in Neutron Star Cores

Nov 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999pthph.102.1043t&link_type=abstract

Progress of Theoretical Physics, Vol. 102, No. 5, pp. 1043-1048

Physics

14

Scientific paper

Λ-superfluidity in a hyperon core of neutron stars is studied with a realistic approach. It is found that Λ-superfluid exists in a restricted density region ρ =~ (ρt - ρd ) with ρt =~ 2▊ (▊ being the nuclear density) and ρd =~ (2.6 - 4.6) ▊ depending on the pairing interaction and the hyperon core model. This restriction suggests that neutron stars compatible with hyperon cooling would be not so massive.

Affiliated with

Also associated with

No associations

Rating

Superfluidity of &#923-Hyperons Admixed in Neutron Star Cores 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 Superfluidity of &#923-Hyperons Admixed in Neutron Star Cores, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Superfluidity of &#923-Hyperons Admixed in Neutron Star Cores will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1513154