Gravitational radiation from differentially rotating and oscillating white dwarfs View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2006-04

AUTHORS

D. M. Sedrakian, K. M. Shahabasyan, M. K. Shahabasyan

ABSTRACT

We examine the possible emission of gravitational waves from white dwarfs undergoing self-similar oscillations driven by the energy released during relaxation of their differential rotation. Two distributions of the initial angular momentum are considered. It is assumed that 1% of the energy dissipated by a rotating white dwarf is converted into the energy of self-similar oscillations and, therefore, into gravitational radiation. The relative amplitude of the gravitational radiation from an isolated white dwarf at a distance of 50 pc is found to be less than 10−27. The emission from the galactic population of white dwarfs may create a background which overlaps the random cosmological background of gravitational radiation for the improved decihertz detectors currently being proposed. More... »

PAGES

201-210

Journal

TITLE

Astrophysics

ISSUE

2

VOLUME

49

Author Affiliations

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/s10511-006-0021-3

DOI

http://dx.doi.org/10.1007/s10511-006-0021-3

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1023911809


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