The matter Lagrangian of an ideal fluid
arXiv:2011.04175 · doi:10.1142/S0219887821500596
Abstract
We show that the matter Lagrangian of an ideal fluid equals (up to a sign -depending on its definition and on the chosen signature of the metric) the total energy density of the fluid, i.e. rest energy density plus internal energy density.
5 pages, accepted for publication in: International Journal of Geometric Methods in Modern Physics (IJGMMP)
References in corpus (7)
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- f(R,L_m) gravity
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- Generalized curvature-matter couplings in modified gravity
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- The first variation of the matter energy-momentum tensor with respect to the metric, and its implications on modified gravity theories
- Effects of the matter Lagrangian degeneracy in gravity
- Anisotropic Tolman V Solutions by Decoupling Approach in Gravity
- Late-Time Anisotropy Sourced by a 2-Form Field Non-Minimally Coupled to Cold Dark Matter
- Tunneling to Holographic Traversable Wormholes
- Gravitational Collapse via Wheeler-DeWitt Equation
- Gravitation with modified fluid Lagrangian: Variational principle and an early dark energy model
- Probing Strong Field Gravity and Ultra-Dense Matter with the Structure and Thermal Evolution of Neutron Stars
- Cosmologies in theory with non-minimal coupling between geometry and matter
- Black hole spectra from Vaz's quantum gravitational collapse
- Relations between Newtonian and relativistic cosmology
- The matter Lagrangian of a non-perfect fluid