Gravitational Radiation from Close Binaries with Time-varying Masses

Holgado, A. Miguel; Ricker, Paul M.

doi:10.3847/1538-4357/ab3293

Title: Gravitational Radiation from Close Binaries with Time-varying Masses

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. Further, 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. Finally, we show that gravitational radiation from mass variation can be orders of magnitude greater than that of orbital motion.

Authors:

^[1];

^[1]

Univ. of Illinois at Urbana-Champaign, IL (United States)

Publication Date:: 2019-08-30

Research Org.:: Krell Institute, Ames, IA (United States)

Sponsoring Org.:: USDOE National Nuclear Security Administration (NNSA); National Science Foundation (NSF)

OSTI Identifier:: 1614433

Grant/Contract Number:: NA0003864

Resource Type:: Accepted Manuscript

Journal Name:: The Astrophysical Journal (Online)

Additional Journal Information:: Journal Name: The Astrophysical Journal (Online); Journal Volume: 882; Journal Issue: 1; Journal ID: ISSN 1538-4357

Publisher:: Institute of Physics (IOP)

Country of Publication:: United States

Language:: English

Subject:: 79 ASTRONOMY AND ASTROPHYSICS; astronomy & astrophysics; binaries: close; gravitational waves

Citation Formats


                    Holgado, A. Miguel, and Ricker, Paul M. Gravitational Radiation from Close Binaries with Time-varying Masses.  United States: N. p., 2019. 
Web.  doi:10.3847/1538-4357/ab3293.

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                    Holgado, A. Miguel, & Ricker, Paul M. Gravitational Radiation from Close Binaries with Time-varying Masses.  United States.  https://doi.org/10.3847/1538-4357/ab3293

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                    Holgado, A. Miguel, and Ricker, Paul M. Fri .  
"Gravitational Radiation from Close Binaries with Time-varying Masses".  United States.  https://doi.org/10.3847/1538-4357/ab3293.  https://www.osti.gov/servlets/purl/1614433.

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@article{osti_1614433,

  title        = {Gravitational Radiation from Close Binaries with Time-varying Masses},

  author       = {Holgado, A. Miguel and Ricker, Paul M.},

  abstractNote = {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. Further, 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. Finally, we show that gravitational radiation from mass variation can be orders of magnitude greater than that of orbital motion.},

  doi          = {10.3847/1538-4357/ab3293},

  journal      = {The Astrophysical Journal (Online)},

  number       = 1,

  volume       = 882,

  place        = {United States},

  year         = {2019},

  month        = {8}

}

Copy to clipboard

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Stochastic gravitational wave background from accreting primordial black hole binaries during early inspiral stage
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Title: Gravitational Radiation from Close Binaries with Time-varying Masses

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Orbital Evolution of Mass-Transferring Eccentric Binary Systems. ii. Secular Evolution journal, June 2016

GW170817: Observation of gravitational waves from a binary neutron star inspiral text, January 2017

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A Comprehensive Study of Binary Compact Objects as Gravitational Wave Sources: Evolutionary Channels, Rates, and Physical Properties journal, June 2002

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Gravitational Radiation from Point Masses in a Keplerian Orbit journal, July 1963

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Two-body problem with variable mass: A new approach journal, January 1963

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GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence journal, June 2016

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The NumPy Array: A Structure for Efficient Numerical Computation journal, March 2011

CASSPER is a semantic segmentation-based particle picking algorithm for single-particle cryo-electron microscopy journal, February 2021

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GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence journal, October 2017

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journal, January 1966

Disentangling Coalescing Neutron-Star–White-Dwarf Binaries for LISA
journal, September 2018

A Comprehensive Study of Binary Compact Objects as Gravitational Wave Sources: Evolutionary Channels, Rates, and Physical Properties
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journal, July 1963

Orbital Characteristics of Binary Systems after Asymmetric Supernova Explosions
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journal, January 1963

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text, January 1964

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Testing the Binary Hypothesis: Pulsar Timing Constraints on Supermassive Black Hole Binary Candidates
journal, March 2018

Asymptotic expansions in the perturbed two-body problem with application to systems with variable mass
journal, February 1975

Can environmental effects spoil precision gravitational-wave astrophysics?
journal, May 2014

Evolutionary Processes in Close Binary Systems
journal, September 1971

The NumPy Array: A Structure for Efficient Numerical Computation
journal, March 2011

CASSPER is a semantic segmentation-based particle picking algorithm for single-particle cryo-electron microscopy
journal, February 2021

The NANOGrav 11 Year Data Set: Pulsar-timing Constraints on the Stochastic Gravitational-wave Background
journal, May 2018

Prospects for Multiband Gravitational-Wave Astronomy after GW150914
journal, June 2016

Gravitational Waves from Accreting Neutron Stars Undergoing Common-envelope Inspiral
journal, April 2018

GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
journal, October 2017

Testing The Binary Hypothesis: Pulsar Timing Constraints On Supermassive Black Hole Binary Candidates
text, January 2017

The effects of sudden mass loss and a random kick velocity produced in a supernova explosion on the dynamics of a binary star of arbitrary orbital eccentricity - Applications to X-ray binaries and to the binary pulsars
journal, April 1983

GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
other, January 2017

GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
other, January 2016

LISA - Laser Interferometer Space Antenna for gravitational wave measurements
conference, August 1995

Testing The Binary Hypothesis: Pulsar Timing Constraints On Supermassive Black Hole Binary Candidates
text, January 2017

GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
other, January 2017

Orbital evolution of mass-transferring eccentric binary systems. I. Phase-dependent evolution
text, January 2016

Orbital evolution of mass-transferring eccentric binary systems. II. Secular Evolution
text, January 2016

Testing the binary hypothesis: pulsar timing constraints on supermassive black hole binary candidates
text, January 2017

Gravitational Waves from Accreting Neutron Stars undergoing Common-Envelope Inspiral
text, January 2017

GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
text, January 2017

GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence
text, January 2017

The NANOGrav 11-year Data Set: Pulsar-timing Constraints On The Stochastic Gravitational-wave Background
text, January 2018

Pulsar Timing Constraints on the Fermi Massive Black-Hole Binary Blazar Population
text, January 2018

Stochastic gravitational wave background from accreting primordial black hole binaries during early inspiral stage
journal, November 2019

Gravitational waves from supernova mass loss and natal kicks in close binaries
journal, October 2019

Stochastic gravitational wave background from accreting primordial black hole binaries during early inspiral stage
text, January 2019