Асосий контентга ўтиш
AkademIndex

Маҳсулотлар

Ишлаб чиқувчилар учун

AkademBaseЭкотизим учун очиқ API
Мақола

Pure Lovelock black holes in dimensions <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>d</mml:mi><mml:mo>=</mml:mo><mml:mn>3</mml:mn><mml:mi>N</mml:mi><mml:mo>+</mml:mo><mml:mn>1</mml:mn></mml:math> are stable

Radouane GannoujiInstituto de Física, Pontificia Universidad Católica de Valparaíso, Casilla 4950, Valparaíso, ChileYolbeiker Rodríguez BaezInstituto de Física, Pontificia Universidad Católica de Valparaíso, Casilla 4950, Valparaíso, ChileNaresh DadhichIUCAA, Post Bag 4, Ganeshkhind, Pune 411 007, India
2019lv
ABI

Аннотация

In this paper, we show that pure Lovelock static Schwarzschild's analogue black holes in dimensions $d&gt;3N+1$, where $N$ is the degree of Lovelock polynomial action, are stable even though pure Gauss-Bonnet $N=2$ black holes are unstable in dimensions $d&lt;7$. We also discuss and compare quasinormal modes for pure Lovelock and the corresponding Einstein black hole in the same dimension. We find that perturbations decay with a characteristic time which is weakly dimensional dependent as it depends only on the gravitational potential of the background solution, while the frequency of oscillations depend on the dimension. Also, we show that the spectrum of perturbations is not isospectral except in $d=4$.

Ҳали таржима қилинмаган

Идентификаторлар

Иқтибослар ва манбалар

4 та иқтибос0 та фойдаланилган манба