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Black Hole Formation in Supernovae: Prospects of Unveiling Fallback Emission

  • L. Zampieri
Conference paper

Abstract

We review the formation mechanism of neutron stars and black holes in corecollapse supernovae and the conditions for establishing a copious fallback of stellar material onto the newly born compact remnant. Accretion from the base of the envelope is capable both to turn the neutron star into a black hole and to give rise to detectable emission of radiation. The potential of unveiling the emission from fallback onto a black hole and its observational implications are discussed in detail.

Keywords

Neutron Star Light Curve Accretion Rate Black Hole Formation Accretion Flow 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag Italia 2002

Authors and Affiliations

  • L. Zampieri
    • 1
  1. 1.INFN, and Dipartimento di FisicaUniversità di PadovaPadovaItaly

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