Two simple models for gravitational-wave modes of compact stars

Andersson, Nils (1996) Two simple models for gravitational-wave modes of compact stars General Relativity and Gravitation, 28, (12), pp. 1433-1445. (doi:10.1007/BF02113773).


Full text not available from this repository.


Two simple model problems relevant for the gravitational-wave modes of relativistic stars are discussed. It is shown that the entire mode-spectrum can be obtained if one considers the modes as arising because of the trapping of gravitational waves by the spacetime curvature. The stellar fluid need play no dynamic role. Furthermore, it is shown that two distinct families of gravitational-wave modes exist. The first corresponds to waves trapped inside the star, while the second is similar to acoustic waves scattered off a hard sphere. An infinite number of the first kind of modes exist, but the latter family will only have a few members.

Item Type: Article
Digital Object Identifier (DOI): doi:10.1007/BF02113773
ISSNs: 0001-7701 (print)
ePrint ID: 29416
Date :
Date Event
Date Deposited: 06 Feb 2007
Last Modified: 16 Apr 2017 22:22
Further Information:Google Scholar

Actions (login required)

View Item View Item