Matter-gravity scattering in the presence of spontaneous Lorentz violation
arXiv:1304.2090 · doi:10.1103/PhysRevD.88.025005
Abstract
Considering quantum gravity within the framework of effective field theory, we investigated the consequences of spontaneous Lorentz violation for the gravitational potential. In particular, we focus our attention on the bumblebee models, in which the graviton couples to a vector that assumes a nonzero vacuum expectation value. The leading order corrections for the nonrelativistic potential are obtained from calculation of the scattering matrix of two scalar particles interacting gravitationally. These corrections imply anisotropic properties associated with the bumblebee background and also add a Darwin-like term for Newton's potential.
19 pages, 2 figures, new references added, Eqs. (30) and (34) are corrected, and results and conclusions are improved. Version published in Phys. Rev. D
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- Testing EGB gravity coupled to bumblebee field and black hole parameter estimation with EHT observations
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- Constraining the Lorentz-Violating Bumblebee Vector Field with Big Bang Nucleosynthesis and Gravitational Baryogenesis
- Implications of a Simpson-Visser solution in Verlinde's framework
- Exact modifications on a vacuum spacetime due to a gradient bumblebee field at its vacuum expectation value
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- Properties of an axisymmetric Lorentzian non-commutative black hole
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- Violation of Hod's Conjecture and Probing it with Optical properties of a 5-D black hole in Einstein Gauss-Bonnet Bumblebee theory of gravity
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- Full Classification of Static Spherical Vacuum Solutions to Bumblebee Gravity with General VEVs
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- Estimating the strength of Lorentzian distribution in non-commutative geometry by solar system tests
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- Quasinormal Modes and Hawking Radiation Sparsity of GUP corrected Black Holes in Bumblebee Gravity with Topological Defects
- Non-minimal matter sector couplings in Lorentz-violating gravity: Self-consistent traversable wormholes and quasinormal modes