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Energetics of Buchdahl stars and the magnetic Penrose process

Energetics of Buchdahl stars and the magnetic Penrose process

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_8bffdee8e0e9418d845d4989e508721e

Energetics of Buchdahl stars and the magnetic Penrose process

About this item

Full title

Energetics of Buchdahl stars and the magnetic Penrose process

Publisher

Berlin/Heidelberg: Springer Berlin Heidelberg

Journal title

The European physical journal. C, Particles and fields, 2024-10, Vol.84 (10), p.1015-12, Article 1015

Language

English

Formats

Publication information

Publisher

Berlin/Heidelberg: Springer Berlin Heidelberg

More information

Scope and Contents

Contents

Buchdahl star is the most compact object without an event horizon and is an excellent candidate for a black hole mimicker. Unlike black holes, rotating Buchdahl star can be over-extremal with respect to the black hole, sustaining a larger spin. We show that it can also develop an ergosphere above the threshold spin
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Alternative Titles

Full title

Energetics of Buchdahl stars and the magnetic Penrose process

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_doaj_primary_oai_doaj_org_article_8bffdee8e0e9418d845d4989e508721e

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_8bffdee8e0e9418d845d4989e508721e

Other Identifiers

ISSN

1434-6052,1434-6044

E-ISSN

1434-6052

DOI

10.1140/epjc/s10052-024-13419-9

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