Singularity formation for the relativistic Euler equations of Chaplygin gases in Schwarzschild spacetime
From MaRDI portal
Publication:6661984
DOI10.1111/SAPM.12775MaRDI QIDQ6661984
Publication date: 13 January 2025
Published in: Studies in Applied Mathematics (Search for Journal in Brave)
Black holes (83C57) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)
Cites Work
- Title not available (Why is that?)
- Title not available (Why is that?)
- Weakly regular fluid flows with bounded variation on the domain of outer communication of a Schwarzschild black hole spacetime
- Quantum FRW cosmological solutions in the presence of Chaplygin gas and perfect fluid
- The formation of trapped surfaces in spherically-symmetric Einstein-Euler spacetimes with bounded variation
- Global radial solutions to 3D relativistic Euler equations for non-isentropic Chaplygin gases
- Blowup of smooth solutions for relativistic Euler equations
- Simple waves and a characteristic decomposition of the two-dimensional compressible Euler equations
- Global existence of a class of smooth 3D spherically symmetric flows of Chaplygin gases with variable entropy
- Strichartz estimates on Schwarzschild black hole backgrounds
- Evolution of a Schwarzschild black hole in phantom-like Chaplygin gas cosmologies
- Uniform decay of local energy and the semi-linear wave equation on Schwarzschild space
- Global solutions of the relativistic Euler equations
- A numerical study of the relativistic Burgers and Euler equations on a Schwarzschild black hole exterior
- The lifespan of 3D radial solutions to the non-isentropic relativistic Euler equations
- Weakly regular fluid flows with bounded variation on the domain of outer communication of a Schwarzschild black hole spacetime. II
- Editor's note: On the gravitational field of a mass point according to Einstein's theory by K. Schwarzschild
- Weakly regular Einstein-Euler spacetimes with Gowdy symmetry: the global areal foliation
- Global entropy solutions and Newtonian limit for the relativistic Euler equations
- Formation of singularities of solutions to the compressible Euler equations for a Chaplygin gas
- Small-amplitude nonlinear waves on a black hole background
- Compressibility effects in aerodynamics.
- Future stability of the FLRW spacetime for a large class of perfect fluids
- Nonlinear stability of self-gravitating irrotational Chaplygin fluids in a FLRW geometry
- Behavior of anisotropic fluids with Chaplygin equation of state in Buchdahl spacetime
- Singularity for the one-dimensional rotating Euler equations of Chaplygin gases
- Blow-up and lifespan estimate to a nonlinear wave equation in Schwarzschild spacetime
- Formation of singularities in one-dimensional Chaplygin gas
- DYNAMICS OF DARK ENERGY
- Classical solutions to the relativistic Euler equations for a linearly degenerate equation of state
- Relativistic sonic geometry for isothermal accretion in the Schwarzschild metric
- Convergence of the finite volume method on a Schwarzschild background
- Finite Time Singularities for Hyperbolic Systems
- A Geometry-Preserving Finite Volume Method for Compressible Fluids on Schwarzschild Spacetime
- Two-Dimensional Subsonic Flow of Compressible Fluids
- Development of singularities in the relativistic Euler equations
- General black-hole metric mimicking Schwarzschild spacetime
- Singularity formation for the cylindrically symmetric rotating relativistic Euler equations of Chaplygin gases
This page was built for publication: Singularity formation for the relativistic Euler equations of Chaplygin gases in Schwarzschild spacetime
Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q6661984)