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Astrophysical Constraints on the Bumblebee Model

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arxiv 1409.2022 v2 pith:4QMBUSG3 submitted 2014-09-06 astro-ph.SR

Jorge Páramos , Gonçalo Guiomar This is my paper · ORCID
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keywords modelastrophysicalbumblebeeconstraintsbodiesbreakingconsideredcontext
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In this work the Bumblebee model for spontaneous Lorentz symmetry breaking is considered in the context of spherically symmetric astrophysical bodies. A discussion of the modified equations of motion is presented and constraints on the parameters of the model are perturbatively obtained.

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Cited by 1 Pith paper

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  1. Stationary scalar clouds around a rotating BTZ-like black hole in the Einstein-bumblebee gravity

    gr-qc 2025-01 conditional novelty 6.0 of 10

    Fundamental stationary scalar clouds exist around rotating BTZ-like black holes in Einstein-bumblebee gravity, with the Lorentz-breaking parameter and angular quantum number having opposite effects and sometimes produ...

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