Kinematical and dynamical aspects of ghost-matter cosmologies
From MaRDI portal
Publication:5162056
DOI10.1088/1361-6382/ABAD82zbMath1479.83243arXiv2004.02935OpenAlexW3047716886MaRDI QIDQ5162056
John D. Barrow, Christos G. Tsagas, Ameya Chavda
Publication date: 1 November 2021
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2004.02935
Relativistic cosmology (83F05) Geometrodynamics and the holographic principle (83E05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Gravitational energy and conservation laws; groups of motions (83C40)
Cites Work
- A cyclic universe approach to fine tuning
- Stability of certain spatially homogeneous cosmological models
- Non-singular bouncing cosmology with positive spatial curvature and flat scalar potential
- A dynamical study of the Friedmann equations
- A Cyclic Model of the Universe
- Bouncing universes with varying constants
- On the stability of static ghost cosmologies
- Scalar fields in curved spacetimes
- COSMOLOGY WITH NEGATIVE POTENTIALS WITH wϕ<-1
- GHOST COSMOLOGY: EXACT SOLUTIONS, TRANSITIONS BETWEEN STANDARD COSMOLOGIES AND GHOST EVOLUTION
- Mach’s principle and the creation of matter
This page was built for publication: Kinematical and dynamical aspects of ghost-matter cosmologies