Stellar tidal disruption events in general relativity
From MaRDI portal
Publication:1729998
DOI10.1007/S10714-019-2510-9zbMath1414.83039arXiv1801.10180OpenAlexW2787299997WikidataQ128416379 ScholiaQ128416379MaRDI QIDQ1729998
Nicholas C. Stone, Roseanne M. Cheng, Michael Kesden, Sjoert van Velzen
Publication date: 7 March 2019
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1801.10180
general relativityrelativistic astrophysicsblack hole spintesting Kerr spacetimetidal disruption event
Related Items (2)
Topical collection: testing the Kerr spacetime with gravitational-wave and electromagnetic observations ⋮ Tidal disruption near black holes and their mimickers
Cites Work
- Unnamed Item
- Unnamed Item
- On quadratic first integrals of the geodesic equations for type [22 spacetimes]
- Relativistic tidal compressions of a star by a massive black hole
- Mechanics of the affine star model
- Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
- Solution to the equations of parallel transport in Kerr geometry; tidal tensor
- Shock waves in tidally compressed stars by massive black holes
- Maximal Analytic Extension of the Kerr Metric
- Global Structure of the Kerr Family of Gravitational Fields
- Fermi Normal Coordinates and Some Basic Concepts in Differential Geometry
- The spin of supermassive black holes
- General Relativity
This page was built for publication: Stellar tidal disruption events in general relativity