Quantization of Friedmann-Robertson-Walker spacetimes in the presence of a cosmological constant and stiff matter
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Publication:382871
DOI10.1007/s10773-013-1590-7zbMath1276.83013OpenAlexW2019723946MaRDI QIDQ382871
Publication date: 22 November 2013
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-013-1590-7
negative cosmological constantWheeler-DeWitt equationexpectation valueinitial singularitystiff matter
Methods of quantum field theory in general relativity and gravitational theory (83C47) Exact solutions to problems in general relativity and gravitational theory (83C15)
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Cites Work
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- Stephani-Schutz quantum cosmology
- Cold dark matter in non-standard cosmologies, PAMELA, ATIC and fermi LAT
- A multidomain spectral method for solving elliptic equations
- Using spectral method as an approximation for solving hyperbolic PDEs
- Does the Big Rip survive quantization?
- Perfect fluid quantum universe in the presence of negative cosmological constant
- Chaplygin gas quantum universe in the presence of the cosmological constant
- Spectral methods for numerical relativity
- The large \(N\) limit of superconformal field theories and supergravity
- Quantum cosmological perfect fluid models
- Spectral methods in general relativistic astrophysics
- A quantum cosmological model with static and dynamic wormholes
- Perfect Fluids in General Relativity: Velocity Potentials and a Variational Principle
- Numerical evolution of axisymmetric vacuum spacetimes: a code based on the Galerkin method
- Generalized Hamiltonian dynamics
- The theory of gravitation in Hamiltonian form
- Fixation of Coordinates in the Hamiltonian Theory of Gravitation
- Peaks in the Hartle–Hawking wavefunction from sums over topologies
- Spacetime Foam and the Cosmological Constant
- Radiation-dominated quantum Friedmann models
- Quantum Stephani exact cosmological solutions and the selection of time variable
- Generalized Hamiltonian Dynamics
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