Geodesics, accretion disk, gravitational lensing, time delay, and effects on neutrinos induced by a non-commutative black hole

Abstract

This paper explores gravitational phenomena associated with a non-commutative black hole. Geodesic equations are derived, and a thin accretion disk is analyzed to model the black hole shadow image, considering an optically thin, radiating, and infalling gas. Retrolensing effects are examined to trace photon emission configurations, while gravitational lensing is investigated through weak and strong deflection limits, with lensing equations and observables applied to Sagittarius A*. The study also includes calculations of time delay, energy deposition rate from neutrino annihilation, phase and probability of neutrino oscillation, and neutrino gravitational lensing.

arXiv comment44 pages, 9 figures and 2 tables -- version accepted for publication in Journal of Cosmology and Astroparticle Physics

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Cited by in corpus (8)

• Influence of a Kalb-Ramond black hole on neutrino behavior
• Quasinormal Modes, Grebody Factors, and Hawking Radiation Sparsity of Black Holes Influenced by a Global Monopole Charge in Kalb-Ramond Gravity
• Axisymmetric black hole in a non-commutative gauge theory: classical and quantum gravity effects
• Accretion of matter of a new bumblebee black hole
• Imprints of non-commutativity on charged black holes
• Light propagation and quasinormal modes of a topologically charged Schwarzschild-Klinkhamer wormhole
• Effects of bumblebee gravity on neutrino motion
• Shadow of a Noncommutative Thin-Shell Gravastar