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Recent Developments in General Relativity, Genoa 2000 pp 301–315Cite as

Black Hole Formation in Supernovae: Prospects of Unveiling Fallback Emission

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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.

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Author information

Authors and Affiliations

  1. INFN, and Dipartimento di Fisica, Università di Padova, Via F. Marzolo 8, 35131, Padova, Italy

    L. Zampieri

Authors
  1. L. Zampieri
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Editor information

Editors and Affiliations

  1. Dipartimento di Metodi e Modelli Matematici (DIMET), Università di Genova, Genova, Italy

    R. Cianci

  2. Dipartimento di Fisica, Università di Genova and Istituto Nazionale di Fisica Nucleare, Sezione di Genova, Genova, Italy

    R. Collina

  3. Dipartimento di Matematica, Università di Torino, Torino, Italy

    M. Francaviglia

  4. Dipartimento di Fisica Teorica, Università di Torino and Istituto Nazionale di Fisica Nucleare, Sezione di Torino, Torino, Italy

    P. Fré

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© 2002 Springer-Verlag Italia

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Zampieri, L. (2002). Black Hole Formation in Supernovae: Prospects of Unveiling Fallback Emission. In: Cianci, R., Collina, R., Francaviglia, M., Fré, P. (eds) Recent Developments in General Relativity, Genoa 2000. Springer, Milano. https://doi.org/10.1007/978-88-470-2101-3_21

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  • DOI: https://doi.org/10.1007/978-88-470-2101-3_21

  • Publisher Name: Springer, Milano

  • Print ISBN: 978-88-470-0162-6

  • Online ISBN: 978-88-470-2101-3

  • eBook Packages: Springer Book Archive

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