Probing Schwarzschild-like black holes in metric-affine bumblebee gravity with accretion disk, deflection angle, greybody bounds, and neutrino propagation
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Publication:6121294
DOI10.1088/1475-7516/2023/12/026arXiv2309.13594OpenAlexW4389662523MaRDI QIDQ6121294
Ali Övgün, Reggie C. Pantig, Unnamed Author, Gaetano Lambiase
Publication date: 26 February 2024
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2309.13594
Cites Work
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- Quasinormal modes of bumblebee wormhole
- Effects of Lorentz Breaking on the Accretion onto a Schwarzschild-like Black Hole*
- Bumblebee gravity and particle motion in Snyder noncommutative spacetime structures
- Bumblebee field as a source of cosmological anisotropies
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- Dehnen halo effect on a black hole in an ultra-faint dwarf galaxy
- Gödel solution in the bumblebee gravity
- Applications of the Gauss–Bonnet theorem to gravitational lensing
- Nonlinear electrodynamics effects on the black hole shadow, deflection angle, quasinormal modes and greybody factors
- Constraints on charged symmergent black hole from shadow and lensing
- Braneworlds in bumblebee gravity
- Black Hole in Quantum Wave Dark Matter
- Quasiperiodic oscillations, weak field lensing and shadow cast around black holes in symmergent gravity
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