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Matter-Sector Lorentz Violation in Binary Pulsars

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arxiv 1510.03798 v1 pith:I7LOR5ML submitted 2015-10-13 gr-qc hep-ph

Ross J. Jennings , Jay D. Tasson , Shun Yang This is my paper · ORCID
classification gr-qchep-ph
keywords lorentzmatter-sectorpulsarsystemsviolationanalysisbinarycoupled
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Violations of local Lorentz invariance in the gravitationally coupled matter sector have yet to be sought in strong-gravity systems. We present the implications of matter-sector Lorentz violation for orbital perturbations in pulsar systems and show that the analysis of pulsar data can provide sensitivities to these effects that exceed the current reach of solar system and laboratory tests by several orders of magnitude.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Lorentz-violating matter-gravity couplings in small-eccentricity binary pulsars

    hep-ph 2019-08 accept novelty 6.0 of 10

    Using three small-eccentricity relativistic binary pulsars, this paper obtains order-of-magnitude upper limits on SME matter-gravity coefficients for neutrons, protons, and electrons.

  2. Modified gravitational wave propagations in linearized gravity with Lorentz and diffeomorphism violations and their gravitational wave constraints

    gr-qc 2025-01 conditional novelty 5.0 of 10

    No evidence of Lorentz or diffeomorphism violation is found in GWTC-3 gravitational waves, yielding 90% bounds on the lowest-dimension SME coefficients k(2)(I)00 and k(3)(V)jm.

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