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Circular orbits and relative strains in Schwarzschild space-time

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Publication:1205544
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DOI10.1007/BF00756949zbMath0762.53049MaRDI QIDQ1205544

S. Usseglio-Tomasset, Fernando de Felice

Publication date: 1 April 1993

Published in: General Relativity and Gravitation (Search for Journal in Brave)


zbMATH Keywords

black holesSchwarzschild space-timehair theoremrelative strain


Mathematics Subject Classification ID

Black holes (83C57) Applications of differential geometry to physics (53Z05) Geodesics in global differential geometry (53C22)


Related Items (5)

Strains and rigidity in black-hole fields ⋮ On the local detectability of the passage through the Schwarzschild horizon ⋮ Extracting information on black hole horizons ⋮ Gyroscopic precession in non-circular orbits: a phase-locked tetrad approach ⋮ Repulsive gravity effects in horizon formation. Horizon remnants in naked singularities




Cites Work

  • Rotating coordinates as tools for calculating circular geodesics and gyroscopic precession
  • Unnamed Item




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