Brans-Dicke gravity and the capture of stars by black holes: some asymptotic results

Chauvineau, Bertrand; Spallicci, Alessandro D. A. M.; Fournier, Jean-Daniel

Published 2005 | Version v1

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Brans-Dicke gravity and the capture of stars by black holes: some asymptotic results

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Astrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux (ARTEMIS) ; Université Nice Sophia Antipolis (1965 - 2019) (UNS) ; COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur ; COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)

In the context of star capture by a black hole, a new noticeable difference between Brans-Dicke theory and general relativity gravitational radiation is pointed out. This feature stems from the non-stationarity of the black hole state, barring Hawking's theorem.

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4 pages.

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URL: https://hal.science/hal-00138810
URN: urn:oai:HAL:hal-00138810v1

Origin repository: UNICA

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Brans-Dicke gravity and the capture of stars by black holes: some asymptotic results

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