Strong cosmic censorship: The nonlinear story

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt

Standard

Strong cosmic censorship : The nonlinear story. / Luna, Raimon; Zillao, Miguel; Cardoso, Vitor; Costa, Joao L.; Natario, Jose.

I: Physical Review D, Bind 99, Nr. 6, 064014, 15.03.2019.

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt

Harvard

Luna, R, Zillao, M, Cardoso, V, Costa, JL & Natario, J 2019, 'Strong cosmic censorship: The nonlinear story', Physical Review D, bind 99, nr. 6, 064014. https://doi.org/10.1103/PhysRevD.99.064014

APA

Luna, R., Zillao, M., Cardoso, V., Costa, J. L., & Natario, J. (2019). Strong cosmic censorship: The nonlinear story. Physical Review D, 99(6), [064014]. https://doi.org/10.1103/PhysRevD.99.064014

Vancouver

Luna R, Zillao M, Cardoso V, Costa JL, Natario J. Strong cosmic censorship: The nonlinear story. Physical Review D. 2019 mar. 15;99(6). 064014. https://doi.org/10.1103/PhysRevD.99.064014

Author

Luna, Raimon ; Zillao, Miguel ; Cardoso, Vitor ; Costa, Joao L. ; Natario, Jose. / Strong cosmic censorship : The nonlinear story. I: Physical Review D. 2019 ; Bind 99, Nr. 6.

Bibtex

@article{c42f50bb3e714d85bf01654f616d1937,
title = "Strong cosmic censorship: The nonlinear story",
abstract = "A satisfactory formulation of the laws of physics entails that the future evolution of a physical system should be determined from appropriate initial conditions. The existence of Cauchy horizons in solutions of the Einstein field equations is therefore problematic and expected to be an unstable artifact of general relativity. This is asserted by the strong cosmic censorship conjecture, which was recently put into question by an analysis of the linearized equations in the exterior of charged black holes in an expanding universe. Here, we numerically evolve the nonlinear Einstein-Maxwell-scalar field equations with a positive cosmological constant, under spherical symmetry, and provide strong evidence that mass inflation indeed does not occur in the near extremal regime. This shows that nonlinear effects might not suffice to save the strong cosmic censorship conjecture.",
keywords = "MASS-INFLATION, BLACK-HOLES, INTERIOR, SCALAR",
author = "Raimon Luna and Miguel Zillao and Vitor Cardoso and Costa, {Joao L.} and Jose Natario",
year = "2019",
month = mar,
day = "15",
doi = "10.1103/PhysRevD.99.064014",
language = "English",
volume = "99",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "American Physical Society",
number = "6",

}

RIS

TY - JOUR

T1 - Strong cosmic censorship

T2 - The nonlinear story

AU - Luna, Raimon

AU - Zillao, Miguel

AU - Cardoso, Vitor

AU - Costa, Joao L.

AU - Natario, Jose

PY - 2019/3/15

Y1 - 2019/3/15

N2 - A satisfactory formulation of the laws of physics entails that the future evolution of a physical system should be determined from appropriate initial conditions. The existence of Cauchy horizons in solutions of the Einstein field equations is therefore problematic and expected to be an unstable artifact of general relativity. This is asserted by the strong cosmic censorship conjecture, which was recently put into question by an analysis of the linearized equations in the exterior of charged black holes in an expanding universe. Here, we numerically evolve the nonlinear Einstein-Maxwell-scalar field equations with a positive cosmological constant, under spherical symmetry, and provide strong evidence that mass inflation indeed does not occur in the near extremal regime. This shows that nonlinear effects might not suffice to save the strong cosmic censorship conjecture.

AB - A satisfactory formulation of the laws of physics entails that the future evolution of a physical system should be determined from appropriate initial conditions. The existence of Cauchy horizons in solutions of the Einstein field equations is therefore problematic and expected to be an unstable artifact of general relativity. This is asserted by the strong cosmic censorship conjecture, which was recently put into question by an analysis of the linearized equations in the exterior of charged black holes in an expanding universe. Here, we numerically evolve the nonlinear Einstein-Maxwell-scalar field equations with a positive cosmological constant, under spherical symmetry, and provide strong evidence that mass inflation indeed does not occur in the near extremal regime. This shows that nonlinear effects might not suffice to save the strong cosmic censorship conjecture.

KW - MASS-INFLATION

KW - BLACK-HOLES

KW - INTERIOR

KW - SCALAR

U2 - 10.1103/PhysRevD.99.064014

DO - 10.1103/PhysRevD.99.064014

M3 - Journal article

VL - 99

JO - Physical Review D

JF - Physical Review D

SN - 2470-0010

IS - 6

M1 - 064014

ER -

ID: 298644573