Tidal and centripetal stress in a model human falling deep into a Kerr black hole

DOI10.1088/0264-9381/32/24/245008zbMath1331.83007OpenAlexW2294569851MaRDI QIDQ2788975

Michael B. Callaham

Publication date: 23 February 2016

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1088/0264-9381/32/24/245008

zbMATH Keywords

general relativityKerr metricrigid body rotationtidal stress

Mathematics Subject Classification ID

Black holes (83C57) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Equations of motion in general relativity and gravitational theory (83C10)

Cites Work

• Black holes: complementarity or firewalls?
• Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
• An ellipsoidal particle–finite element method for hypervelocity impact simulation
• Structure of the singularity inside a realistic rotating black hole
• Oscillatory Null Singularity inside Realistic Spinning Black Holes
• Global Structure of the Kerr Family of Gravitational Fields

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