Gravitational collapse of Hagedorn fluids

    Research output: Contribution to journalArticle

    4 Citations (Scopus)

    Abstract

    We consider a toy model for the relativistic collapse of a homogeneous perfect fluid that takes into account an equation of state for high density matter, in the form of a Hagedorn phase, and semiclassical corrections in the strong field. We show that collapse reaches a critical minimum size and then bounces. We discuss the conditions needed for the collapse to halt and form a compact object. We argue that implications of models such as the one presented here are of great importance for astrophysics as they show that black holes may not be the only final outcome of collapse of very massive stars.

    Original languageEnglish
    Article number104042
    JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
    Volume93
    Issue number10
    DOIs
    Publication statusPublished - May 23 2016

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    gravitational collapse
    fluids
    massive stars
    astrophysics
    equations of state

    ASJC Scopus subject areas

    • Nuclear and High Energy Physics

    Cite this

    Gravitational collapse of Hagedorn fluids. / Malafarina, Daniele.

    In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 93, No. 10, 104042, 23.05.2016.

    Research output: Contribution to journalArticle

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