The Dynamics of the Formation of Degenerate Heavy Neutrino Stars

Details The Dynamics of the Formation of Degenerate Heavy Neutrino Stars The Dynamics of the Formation of Degenerate Heavy Neutrino Stars

2000-08-16

arxiv.org/abs/astro-ph/0008230v2

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures, Minor changes only

Scientific paper

Through reformulating the cold, self-gravitating fermion gas as a Bose
condensate by identifying their mutual Thomas-Fermi limits, the dissipationless
formation of a heavy neutrino star in gravitational collapse is numerically
demonstrated. Such stars offer an alternative to supermassive black holes for
the compact dark objects at the centers of galaxies.

Affiliated with

Also associated with

No associations

Rating

The Dynamics of the Formation of Degenerate Heavy Neutrino 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 The Dynamics of the Formation of Degenerate Heavy Neutrino Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Dynamics of the Formation of Degenerate Heavy Neutrino Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-673972