Time-dependent perturbation theory in quantum cosmology
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Publication:678309
DOI10.1016/S0550-3213(97)80043-0zbMath0939.83018arXivgr-qc/9610045OpenAlexW1980003288MaRDI QIDQ678309
Publication date: 16 April 1997
Published in: Nuclear Physics. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/gr-qc/9610045
spacetimeWheeler-DeWitt equationtransition amplitudesreduction formulamatter interaction Hamiltonian
Related Items (5)
Dirac's observables for the rest-frame instant form of tetrad gravity in a completely fixed 3-orthogonal gauge ⋮ TIME IN COSMOLOGY ⋮ Time-dependent Green functions in quantum cosmology ⋮ Analogue gravity ⋮ The rest-frame instant form of metric gravity.
Cites Work
- Unnamed Item
- Unnamed Item
- Particle creation by black holes
- Time-dependent Green functions in quantum cosmology
- Particle creation and non-adiabatic transitions in quantum cosmology.
- PHYSICAL INTERPRETATION OF BLACK HOLE EVAPORATION AS A VACUUM INSTABILITY
- Wave function of the Universe
- Quantized Fields and Particle Creation in Expanding Universes. I
- Quantum Fields in Curved Space
- Notes on Connes' construction of the standard model
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