Quasinormal modes of the test fields in the consistent 4D Einstein-Gauss-Bonnet-(anti)de Sitter gravity
Identifikátory výsledku
Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19630%2F21%3AA0000143" target="_blank" >RIV/47813059:19630/21:A0000143 - isvavai.cz</a>
Výsledek na webu
<a href="https://www.sciencedirect.com/science/article/pii/S0003491621000312?via%3Dihub" target="_blank" >https://www.sciencedirect.com/science/article/pii/S0003491621000312?via%3Dihub</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1016/j.aop.2021.168425" target="_blank" >10.1016/j.aop.2021.168425</a>
Alternativní jazyky
Jazyk výsledku
angličtina
Název v původním jazyce
Quasinormal modes of the test fields in the consistent 4D Einstein-Gauss-Bonnet-(anti)de Sitter gravity
Popis výsledku v původním jazyce
The regularization proposed in Glavan and Lin (2020) led to the black hole solutions which turned out to be the solutions of the consistent well-defined 4-dimensional Einstein-Gauss-Bonnet theory of gravity suggested in Aoki et al. (2020). Recently the quasinormal modes of bosonic and fermionic fields for this theory were studied. Here we calculate quasinormal frequencies of the test scalar, electromagnetic and Dirac fields for the spherically symmetric black hole in the consistent 4D Einstein-Gauss-Bonnet-de Sitter and anti-de Sitter theories. The values of the quasinormal modes, calculated by the sixth order WKB method with Pade approximants and the time-domain integration, show that both real oscillation frequency and the damping rate are suppressed by increasing of the cosmological constant. While the stability of the scalar and electromagnetic fields follows directly from the positive definiteness of the effective potential, there is no such positive definiteness for the Dirac field. Here, with the help of the time domain integration, taking into account all the modes, we demonstrate stability of the Dirac field in 4D Einstein-Gauss-Bonnet-de Sitter and anti-de Sitter theories.
Název v anglickém jazyce
Quasinormal modes of the test fields in the consistent 4D Einstein-Gauss-Bonnet-(anti)de Sitter gravity
Popis výsledku anglicky
The regularization proposed in Glavan and Lin (2020) led to the black hole solutions which turned out to be the solutions of the consistent well-defined 4-dimensional Einstein-Gauss-Bonnet theory of gravity suggested in Aoki et al. (2020). Recently the quasinormal modes of bosonic and fermionic fields for this theory were studied. Here we calculate quasinormal frequencies of the test scalar, electromagnetic and Dirac fields for the spherically symmetric black hole in the consistent 4D Einstein-Gauss-Bonnet-de Sitter and anti-de Sitter theories. The values of the quasinormal modes, calculated by the sixth order WKB method with Pade approximants and the time-domain integration, show that both real oscillation frequency and the damping rate are suppressed by increasing of the cosmological constant. While the stability of the scalar and electromagnetic fields follows directly from the positive definiteness of the effective potential, there is no such positive definiteness for the Dirac field. Here, with the help of the time domain integration, taking into account all the modes, we demonstrate stability of the Dirac field in 4D Einstein-Gauss-Bonnet-de Sitter and anti-de Sitter theories.
Klasifikace
Druh
J<sub>imp</sub> - Článek v periodiku v databázi Web of Science
CEP obor
—
OECD FORD obor
10308 - Astronomy (including astrophysics,space science)
Návaznosti výsledku
Projekt
—
Návaznosti
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Ostatní
Rok uplatnění
2021
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Údaje specifické pro druh výsledku
Název periodika
Annals Of Physics
ISSN
0003-4916
e-ISSN
1096-035X
Svazek periodika
427
Číslo periodika v rámci svazku
April
Stát vydavatele periodika
US - Spojené státy americké
Počet stran výsledku
13
Strana od-do
„168425-1“-„168425-13“
Kód UT WoS článku
000634879800003
EID výsledku v databázi Scopus
2-s2.0-85102024533