Love numbers and magnetic susceptibility of charged black holes

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Love numbers and magnetic susceptibility of charged black holes. / Pereniguez, David; Cardoso, Vitor.

In: Physical Review D, Vol. 105, No. 4, 044026, 11.02.2022.

Research output: Contribution to journalJournal articleResearchpeer-review

Harvard

Pereniguez, D & Cardoso, V 2022, 'Love numbers and magnetic susceptibility of charged black holes', Physical Review D, vol. 105, no. 4, 044026. https://doi.org/10.1103/PhysRevD.105.044026

APA

Pereniguez, D., & Cardoso, V. (2022). Love numbers and magnetic susceptibility of charged black holes. Physical Review D, 105(4), [044026]. https://doi.org/10.1103/PhysRevD.105.044026

Vancouver

Pereniguez D, Cardoso V. Love numbers and magnetic susceptibility of charged black holes. Physical Review D. 2022 Feb 11;105(4). 044026. https://doi.org/10.1103/PhysRevD.105.044026

Author

Pereniguez, David ; Cardoso, Vitor. / Love numbers and magnetic susceptibility of charged black holes. In: Physical Review D. 2022 ; Vol. 105, No. 4.

Bibtex

@article{6450f03a15804ff9b8b53635d1835c32,
title = "Love numbers and magnetic susceptibility of charged black holes",
abstract = "The response of black holes to companions is of fundamental importance in the context of their dynamics and of gravitational-wave emission. Here, we explore the effect of charge on the static response of black holes. With a view to constraining broader setups, we consider charged geometries in an arbitrary number of spacetime dimensions D > 4. Tensor tidal Love numbers are shown to follow a power law in the H , and thus vanish at extremality. In contrast, the black hole charge Q excites new modes of polarization in the vector sector that are otherwise not responsive in the neutral limit. In four dimensions, Love numbers and magnetic susceptibilities vanish for all values of the charge that respect the extremality bound. Using the theory of Fuchsian equations we are able to obtain analytical results in most cases, even beyond the hypergeometric instances.",
keywords = "PERTURBATIONS, FIELD",
author = "David Pereniguez and Vitor Cardoso",
year = "2022",
month = feb,
day = "11",
doi = "10.1103/PhysRevD.105.044026",
language = "English",
volume = "105",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "American Physical Society",
number = "4",

}

RIS

TY - JOUR

T1 - Love numbers and magnetic susceptibility of charged black holes

AU - Pereniguez, David

AU - Cardoso, Vitor

PY - 2022/2/11

Y1 - 2022/2/11

N2 - The response of black holes to companions is of fundamental importance in the context of their dynamics and of gravitational-wave emission. Here, we explore the effect of charge on the static response of black holes. With a view to constraining broader setups, we consider charged geometries in an arbitrary number of spacetime dimensions D > 4. Tensor tidal Love numbers are shown to follow a power law in the H , and thus vanish at extremality. In contrast, the black hole charge Q excites new modes of polarization in the vector sector that are otherwise not responsive in the neutral limit. In four dimensions, Love numbers and magnetic susceptibilities vanish for all values of the charge that respect the extremality bound. Using the theory of Fuchsian equations we are able to obtain analytical results in most cases, even beyond the hypergeometric instances.

AB - The response of black holes to companions is of fundamental importance in the context of their dynamics and of gravitational-wave emission. Here, we explore the effect of charge on the static response of black holes. With a view to constraining broader setups, we consider charged geometries in an arbitrary number of spacetime dimensions D > 4. Tensor tidal Love numbers are shown to follow a power law in the H , and thus vanish at extremality. In contrast, the black hole charge Q excites new modes of polarization in the vector sector that are otherwise not responsive in the neutral limit. In four dimensions, Love numbers and magnetic susceptibilities vanish for all values of the charge that respect the extremality bound. Using the theory of Fuchsian equations we are able to obtain analytical results in most cases, even beyond the hypergeometric instances.

KW - PERTURBATIONS

KW - FIELD

U2 - 10.1103/PhysRevD.105.044026

DO - 10.1103/PhysRevD.105.044026

M3 - Journal article

VL - 105

JO - Physical Review D

JF - Physical Review D

SN - 2470-0010

IS - 4

M1 - 044026

ER -

ID: 303683571