Gyroscopic precession and centrifugal force in the Ernst spacetime
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Publication:1356638
DOI10.1023/A:1010216801417zbMath0877.70004OpenAlexW110137960MaRDI QIDQ1356638
C. V. Vishveshwara, K. Rajesh Nayak
Publication date: 10 December 1997
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1023/a:1010216801417
circular photon orbitsgyroscopic precessionFrenet-Serret formalismMelvin universezero mass parameter
Relativistic dynamics for problems in Hamiltonian and Lagrangian mechanics (70H40) Equations of motion in general relativity and gravitational theory (83C10) Motion of the gyroscope (70E05)
Related Items (3)
Gyroscopic precession in the vicinity of a static blackhole's event horizon ⋮ Rotospheres in stationary axisymmetric spacetimes ⋮ Gyroscopic precession and inertial forces in axially symmetric stationary spacetimes
Cites Work
- Type \(N\) twisting vacuum gravitational fields
- Integration methods within existing tetrad formalisms in general relativity
- Killing vectors in empty space algebraically special metrics. I
- The \(GHP\) conformal Killing equations and their integrability conditions, with application to twisting type \(N\) vacuum spacetimes
- Integration in the GHP formalism. I: A coordinate approach with applications to twisting type \(N\) spaces
- Symmetries of vacuum type-N metrics
- An Approach to Gravitational Radiation by a Method of Spin Coefficients
- Third-order ODEs for twisting type-N vacuum solutions
- A space-time calculus based on pairs of null directions
- Type-<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>N</mml:mi></mml:math>Gravitational Field with Twist
- Spacetimes with a preferred null direction and a two-dimensional group of isometries: the null dust case
- Behavior of Asymptotically Flat Empty Spaces
- A Class of Null Flat-Space Coordinate Systems
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