Bounding the graviton mass with binary pulsar observations

Patrick J. Sutton; Lee Samuel Finn

doi:10.1088/0264-9381/19/7/318

Bounding the graviton mass with binary pulsar observations

Patrick J. Sutton
, Lee Samuel Finn

Physics

Research output: Contribution to journal › Article › peer-review

18 Scopus citations

Abstract

By comparing the observed orbital decay of the binary pulsars PSR B1913+16 and PSR B1534+12 to that predicted by general relativity due to gravitational-wave emission, we are able to bound the mass of the graviton to be less than 7.6 × 10^-20 eV/c² at 90% confidence. This is the first such bound to be derived from dynamic gravitational fields. It is approximately two orders of magnitude weaker than the static-field bound from solar system observations, and will improve with further observations.

Original language	English (US)
Pages (from-to)	1355-1360
Number of pages	6
Journal	Classical and Quantum Gravity
Volume	19
Issue number	7
DOIs	https://doi.org/10.1088/0264-9381/19/7/318
State	Published - Apr 7 2002

All Science Journal Classification (ASJC) codes

Physics and Astronomy (miscellaneous)

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10.1088/0264-9381/19/7/318

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abstract = "By comparing the observed orbital decay of the binary pulsars PSR B1913+16 and PSR B1534+12 to that predicted by general relativity due to gravitational-wave emission, we are able to bound the mass of the graviton to be less than 7.6 × 10-20 eV/c2 at 90\% confidence. This is the first such bound to be derived from dynamic gravitational fields. It is approximately two orders of magnitude weaker than the static-field bound from solar system observations, and will improve with further observations.",

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AU - Finn, Lee Samuel

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AB - By comparing the observed orbital decay of the binary pulsars PSR B1913+16 and PSR B1534+12 to that predicted by general relativity due to gravitational-wave emission, we are able to bound the mass of the graviton to be less than 7.6 × 10-20 eV/c2 at 90% confidence. This is the first such bound to be derived from dynamic gravitational fields. It is approximately two orders of magnitude weaker than the static-field bound from solar system observations, and will improve with further observations.

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DO - 10.1088/0264-9381/19/7/318

M3 - Article

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SN - 0264-9381

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EP - 1360

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 7

ER -

Bounding the graviton mass with binary pulsar observations

Abstract

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