Gravitational waves from compact binary systems

M. Vasúth, János Majár

Research output: Contribution to journalArticle

Abstract

Inspiralling compact binaries are among the plausible sources of detectable gravitational radiation. Here we compute the gravitational wave polarizations in the extreme mass ratio limit and give their formal expressions with the inclusion of higher order corrections beyond the standard quadrupole term. We discuss the effects caused by the rotation of the central, massive body.

Original languageEnglish
Article number012044
JournalJournal of Physics: Conference Series
Volume66
Issue number1
DOIs
Publication statusPublished - May 1 2007

Fingerprint

gravitational waves
mass ratios
quadrupoles
inclusions
polarization

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Gravitational waves from compact binary systems. / Vasúth, M.; Majár, János.

In: Journal of Physics: Conference Series, Vol. 66, No. 1, 012044, 01.05.2007.

Research output: Contribution to journalArticle

@article{49b1a40b1cb540cea7f74e7e687240b9,
title = "Gravitational waves from compact binary systems",
abstract = "Inspiralling compact binaries are among the plausible sources of detectable gravitational radiation. Here we compute the gravitational wave polarizations in the extreme mass ratio limit and give their formal expressions with the inclusion of higher order corrections beyond the standard quadrupole term. We discuss the effects caused by the rotation of the central, massive body.",
author = "M. Vas{\'u}th and J{\'a}nos Maj{\'a}r",
year = "2007",
month = "5",
day = "1",
doi = "10.1088/1742-6596/66/1/012044",
language = "English",
volume = "66",
journal = "Journal of Physics: Conference Series",
issn = "1742-6588",
publisher = "IOP Publishing Ltd.",
number = "1",

}

TY - JOUR

T1 - Gravitational waves from compact binary systems

AU - Vasúth, M.

AU - Majár, János

PY - 2007/5/1

Y1 - 2007/5/1

N2 - Inspiralling compact binaries are among the plausible sources of detectable gravitational radiation. Here we compute the gravitational wave polarizations in the extreme mass ratio limit and give their formal expressions with the inclusion of higher order corrections beyond the standard quadrupole term. We discuss the effects caused by the rotation of the central, massive body.

AB - Inspiralling compact binaries are among the plausible sources of detectable gravitational radiation. Here we compute the gravitational wave polarizations in the extreme mass ratio limit and give their formal expressions with the inclusion of higher order corrections beyond the standard quadrupole term. We discuss the effects caused by the rotation of the central, massive body.

UR - http://www.scopus.com/inward/record.url?scp=34250888838&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=34250888838&partnerID=8YFLogxK

U2 - 10.1088/1742-6596/66/1/012044

DO - 10.1088/1742-6596/66/1/012044

M3 - Article

AN - SCOPUS:34250888838

VL - 66

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

SN - 1742-6588

IS - 1

M1 - 012044

ER -