PulseExploreJournal ClubDebatesTrendingResearchersJournals
Instagram
HomeExploreJournal ClubTrending
Synapse
⌘+K
Synapse
March 25, 2026International Journal of Gravitation and Theoretical Physics4 citationsOpen Access

An Efficient Higher-Order WKB Code for Quasinormal Modes and Greybody Factors

JMJerzy MatyjasekRKR. A. KonoplyaAZA. Zhidenko

Key Points

  • The aim is to enhance the efficiency and accuracy of a higher-order WKB code for computing quasinormal modes.
  • Updated higher-order WKB Mathematica® code implementation
  • Used Padé resummation to improve accuracy
  • Expanded effective potential using Taylor series around its maximum
  • Substantial reduction in computation time for calculating quasinormal modes
  • Speed gains can reach several orders of magnitude for complex potentials
  • Accuracy of the method is maintained despite increased efficiency

Abstract

The higher-order WKB Mathematica® code for computing quasinormal modes, whose accuracy was significantly enhanced through extensions to higher orders and, in particular, through the use of Pad´e resummation, has been widely employed in numerous studies over the past several years. In this work, we present an updated and optimized version of the code. The main improvement consists in expanding the effective potential in a Taylor series around its maximum, rather than evaluating the full analytic expression of the WKB formula for each specific potential. This modification leads to a substantial reduction in computation time. In cases where the effective potential is complicated and involves non-rational functions, the speed gain can reach several orders of magnitude, while preserving the accuracy of the method.

Ask AI
Helpful
Bookmark
Share
View Full Paper

Cite This Study

Matyjasek et al. (2026) studied this question.

synapsesocial.com/papers/69c37b74b34aaaeb1a67de07https://doi.org/10.53941/ijgtp.2026.100005
Ask AI
Helpful
Bookmark
Share
View Full Paper