Pulsar Radiation and Quantum Gravity

dc.creatorKaaret, Philip
dc.date1999-03-30
dc.date.accessioned2026-07-07T02:31:03Z
dc.date.available2026-07-07T02:31:03Z
dc.descriptionQuantum gravity may lead to an energy dependence in the speed of light. The high energy radiation from gamma-ray pulsars can be used to place limits on such effects. We find that emission from the Crab pulsar at energies above 2 GeV trails that at 70-100 MeV by no more than 0.35 ms (95% confidence) and place a lower bound on the energy scale of quantum gravitational effects on the speed of light of 1.8 x 10^15 GeV. This bound might be improved by two orders of magnitude by observation of pulsations from the Crab at higher energies, 50-100 GeV, in the near future.
dc.descriptionAccepted to Astronomy and Astrophysics Letters, 3 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/9903464
dc.identifierhttp://arxiv.org/abs/astro-ph/9903464
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14030
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titlePulsar Radiation and Quantum Gravity
dc.typetext

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