Mathematical Research Data Initiative
Main page
Recent changes
Random page
Help about MediaWiki
Create a new Item
Create a new Property
Create a new EntitySchema
Merge two items
In other projects
Discussion
View source
View history
Purge
English
Log in

The phase-integral method and black hole normal modes

From MaRDI portal
Publication:4032972
Jump to:navigation, search

DOI10.1088/0264-9381/10/4/009zbMath0766.58060OpenAlexW2044711048MaRDI QIDQ4032972

No author found.

Publication date: 23 May 1993

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: http://hdl.handle.net/11858/00-001M-0000-0013-10B2-9


zbMATH Keywords

black holesrelativistic starsphase-integral method


Mathematics Subject Classification ID

Relativistic cosmology (83F05) Black holes (83C57) Applications of global analysis to the sciences (58Z05) Gravitational waves (83C35)


Related Items

Two simple models for gravitational-wave modes of compact stars ⋮ On the Liouvillian solutions to the perturbation equations of the Schwarzschild black hole ⋮ Scattering of axial gravitational wave pulses by monopole black holes and QNMs: a semianalytic approach ⋮ Quasi-normal modes of stars and black holes



Retrieved from "https://portal.mardi4nfdi.de/w/index.php?title=Publication:4032972&oldid=17749252"
Tools
What links here
Related changes
Special pages
Printable version
Permanent link
Page information
MaRDI portal item
This page was last edited on 6 February 2024, at 03:48.
Privacy policy
About MaRDI portal
Disclaimers
Imprint
Powered by MediaWiki