2017
DOI: 10.1088/1475-7516/2017/03/030
|View full text |Cite
|
Sign up to set email alerts
|

Quasinormal modes of asymptotically (A)dS black hole in Lovelock background

Abstract: We study the quasinormal modes of the massless scalar field in asymptotically (A)dS black holes in Lovelock spacetime by using the sixth order of the WKB approximation. We consider the effects of the second and third order of Lovelock coupling constants on quasinormal frequencies spectrum as well as cosmological constant.

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2

Citation Types

0
2
0

Year Published

2019
2019
2019
2019

Publication Types

Select...
1

Relationship

0
1

Authors

Journals

citations
Cited by 1 publication
(2 citation statements)
references
References 70 publications
0
2
0
Order By: Relevance
“…The latter yields that the representation (21) is equivalent to (20) up to the given order k, i. e. the coefficients Q 0 , Q 1 , . .…”
Section: Further Improvement Of the Wkb Formula Accuracymentioning
confidence: 99%
See 1 more Smart Citation
“…The latter yields that the representation (21) is equivalent to (20) up to the given order k, i. e. the coefficients Q 0 , Q 1 , . .…”
Section: Further Improvement Of the Wkb Formula Accuracymentioning
confidence: 99%
“…In order to increase accuracy of the higher-order WKB formula, it has been recently proposed to use Padé approximants [61] for the usual WKB formula [4]. Within this approach one has to define a polynomial P k (ǫ) by introducing powers of the order parameter ǫ in the righthand side of the WKB formula (17) as follows, (20) where the polynomial order k coincides with the order of the WKB formula. Formal parameter ǫ is introduced in the same way as in [2] in order to keep track of orders in the WKB approximation, and the squared frequency can be obtained by taking ǫ = 1,…”
Section: Further Improvement Of the Wkb Formula Accuracymentioning
confidence: 99%