Using binary stars to bound the mass of the graviton
Physical Review D - Particles, Fields, Gravitation and Cosmology, ISSN: 1550-2368, Vol: 61, Issue: 10, Page: 104008
2000
- 43Citations
- 128Usage
- 4Captures
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Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
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Metrics Details
- Citations43
- Citation Indexes43
- 43
- CrossRef29
- Usage128
- Downloads110
- Abstract Views18
- Captures4
- Readers4
Article Description
Interacting white dwarf binary star systems, including helium cataclysmic variable (HeCV) systems, are expected to be strong sources of gravitational radiation, and should be detectable by proposed space-based laser interferometer gravitational wave observatories such as LISA. Several HeCV star systems are presently known and can be studied optically, which will allow electromagnetic and gravitational wave observations to be correlated. Comparisons of the phases of a gravitational wave signal and the orbital light curve from an interacting binary white dwarf star system can be used to bound the mass of the graviton. Observations of typical HeCV systems by LISA could potentially yield an upper bound on the inverse mass of the graviton as strong as (Formula presented) km (Formula presented) eV), more than two orders of magnitude better than present solar system derived bounds. © 2000 The American Physical Society.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=17144363953&origin=inward; http://dx.doi.org/10.1103/physrevd.61.104008; https://link.aps.org/doi/10.1103/PhysRevD.61.104008; http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.61.104008/fulltext; http://link.aps.org/article/10.1103/PhysRevD.61.104008; https://digitalcommons.usu.edu/physics_facpub/458; https://digitalcommons.usu.edu/cgi/viewcontent.cgi?article=1457&context=physics_facpub
American Physical Society (APS)
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