Self-gravitating relativistic fluids:the continuation and termination of a free phase boundary.

DOI10.1007/BF00375147zbMath1075.83517MaRDI QIDQ1918325

Demetrios Christodoulou

Publication date: 1996

Published in: Archive for Rational Mechanics and Analysis (Search for Journal in Brave)

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items

Self-gravitating relativistic fluids: the formation of a free phase boundary in the phase transition from hard to soft ⋮ The global structure of spherically symmetric charged scalar field spacetimes ⋮ On ``hard stars in general relativity ⋮ On the asymptotic behavior of static perfect fluids ⋮ Rigid elastic solids in relativity ⋮ Theorems on existence and global dynamics for the Einstein equations ⋮ Local and global existence theorems for the Einstein equations ⋮ Theorems on existence and global dynamics for the Einstein equations ⋮ Local and global existence theorems for the Einstein equations ⋮ Self-gravitating relativistic fluids: The formation of a free phase boundary in the phase transition from soft to hard

Cites Work

• Self-gravitating relativistic fluids: A two-phase model