Gravitational Radiation from Close Binaries with Time-varying Masses

A. Miguel Holgado, Paul M. Ricker

Research output: Contribution to journalArticle

Abstract

In the quadrupole approximation of general relativity in the weak-field limit, a time-varying quadrupole moment generates gravitational radiation. Binary orbits are one of the main mechanisms for producing gravitational waves and are the main sources and backgrounds for gravitational-wave detectors across the multiband spectrum. In this paper, we introduce additional contributions to the gravitational radiation from close binaries that arise from time-varying masses along with those produced by orbital motion. We derive phase-dependent formulae for these effects in the quadrupolar limit for binary point masses, which reduce to the formulae that Peters & Mathews derived when the mass of each component is taken to be constant. We show that gravitational radiation from mass variation can be orders of magnitude greater than that of orbital motion.

Original languageEnglish (US)
Article number39
JournalAstrophysical Journal
Volume882
Issue number1
DOIs
StatePublished - Sep 1 2019

Fingerprint

gravitational waves
orbits
quadrupoles
relativity
radiation
moments
detectors
approximation

Keywords

  • binaries: close
  • gravitational waves

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Gravitational Radiation from Close Binaries with Time-varying Masses. / Holgado, A. Miguel; Ricker, Paul M.

In: Astrophysical Journal, Vol. 882, No. 1, 39, 01.09.2019.

Research output: Contribution to journalArticle

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