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Semi-classical Dust Collapse and Regular Black Holes

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Regular Black Holes

Part of the book series: Springer Series in Astrophysics and Cosmology ((SSAC))

Abstract

Semi-classical corrections at large curvature are employed in toy models of spherically symmetric gravitational collapse in order to avoid the formation of singularities. The resulting spacetimes may produce bounces, compact remnants or regular black holes in place of the usual Schwarzschild black hole. Within these models, a whole class of collapse scenarios leading to the formation of regular black holes may be obtained from General Relativity coupled to some theory of non-linear electrodynamics. In the present chapter we provide a thorough exposition of semi-classical dust collapse with particular attention to the conditions for the formation of regular black holes as the endstate of collapse.

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Notes

  1. 1.

    Notice that \(j(q)=0\) in this case.

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Acknowledgements

DM acknowledges support from Nazarbayev University Faculty Development Competitive Research Grant No. 11022021FD2926.

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Authors and Affiliations

  1. Department of Physics, Nazarbayev University, Kabanbay Batyr 53, 010000, Astana, Kazakhstan

    Daniele Malafarina

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  1. Daniele Malafarina
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Correspondence to Daniele Malafarina .

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  1. Department of Physics, Fudan University, Shanghai, China

    Cosimo Bambi

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Malafarina, D. (2023). Semi-classical Dust Collapse and Regular Black Holes. In: Bambi, C. (eds) Regular Black Holes. Springer Series in Astrophysics and Cosmology. Springer, Singapore. https://doi.org/10.1007/978-981-99-1596-5_12

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