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Collapse of uniformly rotating stars to black holes and the formation of disks
Stuart L. Shapiro
Physics
Astronomy
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Dive into the research topics of 'Collapse of uniformly rotating stars to black holes and the formation of disks'. Together they form a unique fingerprint.
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Keyphrases
Equation of State
100%
Rotating Star
100%
Angular Momentum
33%
As(III)
33%
Thermal Radiation
33%
Central Hole
33%
Total Mass
33%
Energy Functional
33%
Massive Stars
33%
Radiation Pressure
33%
Kerr Black Hole
33%
Adiabatic Index
33%
Semi-analytic
33%
General Relativity
33%
Polytropic Index
33%
Residual Gas
33%
Neutron Stars
33%
Supermassive Stars
33%
Post-Newtonian
33%
Energy Variational Principle
33%
Stiff Equations
33%
Polytropic Stars
33%
Physics
Equations of State
100%
Black Holes
100%
Angular Momentum
33%
Massive Star
33%
Radiation Pressure
33%
Kerr Black Holes
33%
Thermal Radiation
33%
General Relativity
33%
Neutron Stars
33%
Residual Gas
33%
Shedding
33%
Supermassive Star
33%
Variational Principle
33%
Polytropes
33%