Chaplygin gas quantum universe in the presence of the cosmological constant
From MaRDI portal
Publication:967600
DOI10.1007/s10714-009-0877-8zbMath1187.83083OpenAlexW2010283010MaRDI QIDQ967600
Shahram Jalalzadeh, Pouria Pedram
Publication date: 30 April 2010
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10714-009-0877-8
Relativistic cosmology (83F05) Quantization of the gravitational field (83C45) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)
Related Items (5)
Viscous varying generalized Chaplygin gas with cosmological constant and space curvature ⋮ Quantization of Friedmann-Robertson-Walker spacetimes in the presence of a cosmological constant and stiff matter ⋮ The Dirichlet problem for a 3D elliptic equation with two singular coefficients ⋮ Viscous new varying modified cosmic Chaplygin gas with cosmological constant in non-flat universe ⋮ The osgood criterion and finite-time cosmological singularities
Cites Work
- Unnamed Item
- Stephani-Schutz quantum cosmology
- Quantum FRW cosmological solutions in the presence of Chaplygin gas and perfect fluid
- Using spectral method as an approximation for solving hyperbolic PDEs
- The holographic dark energy in non-flat Brans-Dicke cosmology
- Holographic Chaplygin gas model
- Avoidance of big rip in phantom cosmology by gravitational back reaction
- Perfect fluid quantum universe in the presence of negative cosmological constant
- Dynamical vacuum in quantum cosmology
- Irreversible processes in a universe modelled as a mixture of a Chaplygin gas and radiation
- Quantum cosmological perfect fluid models
- Density perturbations in a universe dominated by the Chaplygin gas
- Mass power spectrum in a universe dominated by the Chaplygin gas
- Schrödinger-Wheeler-DeWitt equation in Chaplygin gas FRW cosmological model
- The cosmological constant and dark energy
- Perfect Fluids in General Relativity: Velocity Potentials and a Variational Principle
- The cosmological constant problem and quintessence
- Two-component formulation of the Wheeler–DeWitt equation
- Radiation-dominated quantum Friedmann models
- Canonical wave packets in quantum cosmology
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Cosmological Imprint of an Energy Component with General Equation of State
- Quantum Stephani exact cosmological solutions and the selection of time variable
- The cosmological constant problem
- Quantum Theory of Gravity. I. The Canonical Theory
- \(k\)-inflation
- An alternative to quintessence
- Supersymmetric Chaplygin gas
- Relativistic Chaplygin gas with field-dependent Poincaré symmetry
This page was built for publication: Chaplygin gas quantum universe in the presence of the cosmological constant