Limits on Neutron Lorentz Violation from Pulsar Timing

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dc.creatorAltschul, B.
dc.date2006-08-08
dc.date2006-12-11
dc.date.accessioned2026-07-07T10:41:56Z
dc.date.available2026-07-07T10:41:56Z
dc.descriptionPulsars are the most accurate naturally occurring clocks, and data about them can be used to set bounds on neutron-sector Lorentz violations. If SO(3) rotation symmetry is completely broken for neutrons, then pulsars' rotation speeds will vary periodically. Pulsar timing data limits the relevant Lorentz-violating coefficients to be smaller than 1.7 x 10^(-8) at at least 90% confidence.
dc.description10 pages, version to appear in Phys. Rev. D
dc.identifierhttps://arxiv.org/abs/hep-ph/0608094
dc.identifierhttp://arxiv.org/abs/hep-ph/0608094
dc.identifierPhys.Rev.D75:023001,2007
dc.identifierdoi:10.1103/PhysRevD.75.023001
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181782
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleLimits on Neutron Lorentz Violation from Pulsar Timing
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