Partially massless gravitons do not destroy general relativity black holes

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Partially massless gravitons do not destroy general relativity black holes. / Brito, Richard; Cardoso, Vitor; Pani, Paolo.

I: Physical Review D, Bind 87, Nr. 12, 124024, 20.06.2013.

Publikation: Bidrag til tidsskriftTidsskriftartikelForskningfagfællebedømt

Harvard

Brito, R, Cardoso, V & Pani, P 2013, 'Partially massless gravitons do not destroy general relativity black holes', Physical Review D, bind 87, nr. 12, 124024. https://doi.org/10.1103/PhysRevD.87.124024

APA

Brito, R., Cardoso, V., & Pani, P. (2013). Partially massless gravitons do not destroy general relativity black holes. Physical Review D, 87(12), [124024]. https://doi.org/10.1103/PhysRevD.87.124024

Vancouver

Brito R, Cardoso V, Pani P. Partially massless gravitons do not destroy general relativity black holes. Physical Review D. 2013 jun. 20;87(12). 124024. https://doi.org/10.1103/PhysRevD.87.124024

Author

Brito, Richard ; Cardoso, Vitor ; Pani, Paolo. / Partially massless gravitons do not destroy general relativity black holes. I: Physical Review D. 2013 ; Bind 87, Nr. 12.

Bibtex

@article{ad253021b0f64f16854fc96ea5d09954,
title = "Partially massless gravitons do not destroy general relativity black holes",
abstract = "Recent nonlinear completions of Fierz-Pauli theory for a massive spin-2 field include nonlinear massive gravity and bimetric theories. The spectrum of black-hole solutions in these theories is rich and comprises the same vacuum solutions of Einstein's gravity enlarged to include a cosmological constant. It was recently shown that Schwarzschild (de Sitter) black holes in these theories are generically unstable against spherical perturbations. Here we show that a notable exception is partially massless gravity, where the mass of the graviton is fixed in terms of the cosmological constant by mu(2) = 2 Lambda/3 and a new gauge invariance emerges. We find that general relativity black holes are stable in this limit. Remarkably, the spectrum of massive gravitational perturbations is isospectral.",
author = "Richard Brito and Vitor Cardoso and Paolo Pani",
year = "2013",
month = jun,
day = "20",
doi = "10.1103/PhysRevD.87.124024",
language = "English",
volume = "87",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "American Physical Society",
number = "12",

}

RIS

TY - JOUR

T1 - Partially massless gravitons do not destroy general relativity black holes

AU - Brito, Richard

AU - Cardoso, Vitor

AU - Pani, Paolo

PY - 2013/6/20

Y1 - 2013/6/20

N2 - Recent nonlinear completions of Fierz-Pauli theory for a massive spin-2 field include nonlinear massive gravity and bimetric theories. The spectrum of black-hole solutions in these theories is rich and comprises the same vacuum solutions of Einstein's gravity enlarged to include a cosmological constant. It was recently shown that Schwarzschild (de Sitter) black holes in these theories are generically unstable against spherical perturbations. Here we show that a notable exception is partially massless gravity, where the mass of the graviton is fixed in terms of the cosmological constant by mu(2) = 2 Lambda/3 and a new gauge invariance emerges. We find that general relativity black holes are stable in this limit. Remarkably, the spectrum of massive gravitational perturbations is isospectral.

AB - Recent nonlinear completions of Fierz-Pauli theory for a massive spin-2 field include nonlinear massive gravity and bimetric theories. The spectrum of black-hole solutions in these theories is rich and comprises the same vacuum solutions of Einstein's gravity enlarged to include a cosmological constant. It was recently shown that Schwarzschild (de Sitter) black holes in these theories are generically unstable against spherical perturbations. Here we show that a notable exception is partially massless gravity, where the mass of the graviton is fixed in terms of the cosmological constant by mu(2) = 2 Lambda/3 and a new gauge invariance emerges. We find that general relativity black holes are stable in this limit. Remarkably, the spectrum of massive gravitational perturbations is isospectral.

U2 - 10.1103/PhysRevD.87.124024

DO - 10.1103/PhysRevD.87.124024

M3 - Journal article

VL - 87

JO - Physical Review D

JF - Physical Review D

SN - 2470-0010

IS - 12

M1 - 124024

ER -

ID: 300165433