Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...235..199s&link_type=abstract
Astrophysical Journal, Part 1, vol. 235, Jan. 1, 1980, p. 199-215.
Astronomy and Astrophysics
Astronomy
47
Black Holes (Astronomy), Computer Programs, Gravitational Collapse, Magnetohydrodynamics, Neutron Stars, Space-Time Functions, Astronomical Models, Equations Of State, Equilibrium Equations, Relativity, Singularity (Mathematics), Stellar Models
Scientific paper
A new, general relativistic, hydrodynamical computer code for spherical, stellar collapse to neutron stars and black holes is presented. The code is employed to construct spacetimes for the geometrodynamical evolution of spherical masses which are initially at rest and obey an adiabatic Gamma-law equation of state. Collapse to a black hole can be followed accurately; the evolution outside the event horizon can be determined far into the future without having the integration terminate because of spacetime singularities inside. Three possible outcomes for adiabatic core collapse are distinguished: homologous core bounce, nonhomologous core bounce, and catastrophic collapse to a black hole.
Shapiro Stuart L.
Teukolsky Saul A.
No associations
LandOfFree
Gravitational collapse to neutron stars and black holes - Computer generation of spherical spacetimes 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 Gravitational collapse to neutron stars and black holes - Computer generation of spherical spacetimes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gravitational collapse to neutron stars and black holes - Computer generation of spherical spacetimes will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-880618