skip to main content
US FlagAn official website of the United States government
dot gov icon
Official websites use .gov
A .gov website belongs to an official government organization in the United States.
https lock icon
Secure .gov websites use HTTPS
A lock ( lock ) or https:// means you've safely connected to the .gov website. Share sensitive information only on official, secure websites.


Title: Methods for relativistic self-gravitating fluids: from binary neutron stars to black hole-disks and magnetized rotating neutron stars
Award ID(s):
2006066 1662211
PAR ID:
10332076
Author(s) / Creator(s):
;
Date Published:
Journal Name:
General Relativity and Gravitation
Volume:
54
Issue:
6
ISSN:
0001-7701
Format(s):
Medium: X
Sponsoring Org:
National Science Foundation
More Like this
  1. We analyze effects of neutron-antineutron transitions in neutron stars, specifically on (i) cooling, (ii) rotation rate, and (iii) for binary pulsars, the increase in the orbital period. We show that these effects are negligibly small. 
    more » « less