Multi-body spherically symmetric steady states of Newtonian self-gravitating elastic matter
From MaRDI portal
Publication:2007750
DOI10.1007/s00220-019-03380-0zbMath1434.85005arXiv1807.03062OpenAlexW3102536575MaRDI QIDQ2007750
Publication date: 22 November 2019
Published in: Communications in Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1807.03062
Related Items (2)
Cites Work
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Unnamed Item
- Ground states of self-gravitating elastic bodies
- The state of deformation in earthlike self-gravitating objects
- Orbital stability of spherical galactic models
- Existence of axially symmetric solutions to the Vlasov-Poisson system
- Newtonian stellar models.
- Stationary and static stellar dynamic models with axial symmetry
- Spherically symmetric static solutions of the Einstein equations with elastic matter source
- Spherically Symmetric Equilibria for Self-Gravitating Kinetic or Fluid Models in the Nonrelativistic and Relativistic Case---A Simple Proof for Finite Extension
- Stellar Structure and Evolution
- Spherically symmetric steady states of John elastic bodies in general relativity
- Existence and properties of spherically symmetric static fluid bodies with a given equation of state
- Theory of Newtonian self-gravitating stationary spherically symmetric systems
- Discontinuous equilibrium solutions and cavitation in nonlinear elasticity
- Static shells for the Vlasov-Poisson and Vlasov-Einstein systems
- Static, self–gravitating elastic bodies
- On the symmetries of equilibrium stellar models
- Existence and stability of static shells for the Vlasov–Poisson system
This page was built for publication: Multi-body spherically symmetric steady states of Newtonian self-gravitating elastic matter
