• DOI:10.1088/0004-637X/749/1/37
Corpus ID: 119098587

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

View PDF on arXiv

Save to Library

Create Alert

Cite

Launch Research Feed