Rigid covariance, equivalence principle and Fermi rigid coordinates: gravitational waves
From MaRDI portal
Publication:1618044
DOI10.1007/S10714-018-2466-1zbMath1403.83005arXiv1807.06344OpenAlexW3124916203WikidataQ129088667 ScholiaQ129088667MaRDI QIDQ1618044
Publication date: 13 November 2018
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1807.06344
Applications of differential geometry to physics (53Z05) Equations of motion in general relativity and gravitational theory (83C10) Gravitational waves (83C35)
Related Items (1)
Cites Work
- Unnamed Item
- On the meaning of Painlevé-Gullstrand synchronization
- Rigid motions and generalized Newtonian gravitation
- Extended Fermi coordinates
- Homothetic motions and Newtonian cosmology
- Rigid covariance as a natural extension of Painlevé-Gullstrand space-times: gravitational waves
- Relativity in rotating frames. Relativistic physics in rotating reference frames
- Expansions of the affinity, metric and geodesic equations in Fermi normal coordinates about a geodesic
- Reference frames and rigid motions in relativity
- Coupled inertial and gravitational effects in the proper reference frame of an accelerated, rotating observer
- Feynman’s proof of the Maxwell equations
- Riemann normal coordinates, Fermi reference system and the geodesic deviation equation
- Fermi Normal Coordinates and Some Basic Concepts in Differential Geometry
This page was built for publication: Rigid covariance, equivalence principle and Fermi rigid coordinates: gravitational waves