Photo from wikipedia
We study stationary and axially symmetric black hole-disk systems, assuming a combination of the DD2 and Timmes-Swesty equations of state and a three-parameter family of rotation laws. There exist two… Click to show full abstract
We study stationary and axially symmetric black hole-disk systems, assuming a combination of the DD2 and Timmes-Swesty equations of state and a three-parameter family of rotation laws. There exist two branches of solutions that are shown to bifurcate, for a suitable specific entropy and a parameter in the rotation law. Low entropy nuclear matter allows for the existence of moderately massive Keplerian disks.
Keywords:
stationary massive;
disks around;
massive disks;
black holes;
state;
around black
Journal Title: Physical Review D
Year Published: 2021
Link to full text (if available)
Share on Social Media: Sign Up to like & get
recommendations!
Journal Title: Physical Review D
Year Published: 2021
Link to full text (if available)
Share on Social Media: Sign Up to like & get
recommendations!