Tidal effects away from the equatorial plane in Kerr backgrounds

DOI10.1016/j.physletb.2019.05.048zbMath1421.83052arXiv1812.08642OpenAlexW2949392996WikidataQ127752867 ScholiaQ127752867MaRDI QIDQ2273769

Suvankar Paul, Tapobrata Sarkar, Pritam Banerjee, Rajibul Shaikh

Publication date: 18 September 2019

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1812.08642

Mathematics Subject Classification ID

Black holes (83C57) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (2)

Shadows and optical appearance of black bounces illuminated by a thin accretion disk ⋮ Tidal disruption near black holes and their mimickers

Cites Work

• Unnamed Item
• Distinguishing between Kerr and rotating JNW space-times via frame dragging and tidal effects
• Solution to the equations of parallel transport in Kerr geometry; tidal tensor
• Numerical Study of the Tidal Disruption of Neutron Stars Moving around a Black Hole: -- Compressible Jeans and Roche Problems --
• Fermi Normal Coordinates and Some Basic Concepts in Differential Geometry

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