Bounding the graviton mass with binary pulsar observations

Patrick J. Sutton, Lee Samuel Finn

Research output: Contribution to journalArticlepeer-review

16 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 languageEnglish (US)
Pages (from-to)1355-1360
Number of pages6
JournalClassical and Quantum Gravity
Volume19
Issue number7
DOIs
StatePublished - Apr 7 2002

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy (miscellaneous)

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