Relativistic collapse and explosion of rotating supermassive stars with thermonuclear effects

@article{Montero2012RelativisticCA,
  title={Relativistic collapse and explosion of rotating supermassive stars with thermonuclear effects},
  author={P. Montero and Hans-Thomas Janka and E. M{\"u}ller},
  journal={The Astrophysical Journal},
  year={2012},
  volume={749},
  pages={37}
}
  • P. Montero, Hans-Thomas Janka, E. Müller
  • Published 2012
  • Physics
  • The Astrophysical Journal
  • We present results of general relativistic simulations of collapsing supermassive stars with and without rotation using the two-dimensional general relativistic numerical code Nada, which solves the Einstein equations written in the BSSN formalism and the general relativistic hydrodynamic equations with high-resolution shock-capturing schemes. These numerical simulations use an equation of state that includes the effects of gas pressure and, in a tabulated form, those associated with radiation… CONTINUE READING
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    References

    SHOWING 1-10 OF 51 REFERENCES
    Spherical collapse of supermassive stars: Neutrino emission and gamma-ray bursts
    • 30
    • PDF
    Evolution of Rotating Supermassive Stars to the Onset of Collapse
    • 88
    • PDF
    Collapse of differentially rotating supermassive stars: Post black hole formation
    • 16
    • Highly Influential
    • PDF
    Formation of supermassive black holes by direct collapse in pre-galactic haloes
    • 478
    • PDF
    Collapse of a Rotating Supermassive Star to a Supermassive Black Hole: Fully Relativistic Simulations
    • 136
    • Highly Influential
    • PDF