ON THE SEMICLASSICAL LIMIT OF LOOP QUANTUM COSMOLOGY
DOI10.1142/S0218271812500769zbMath1277.83005arXiv1105.2804WikidataQ57564325 ScholiaQ57564325MaRDI QIDQ2865302
Edison Montoya, Alejandro Corichi
Publication date: 29 November 2013
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1105.2804
Relativistic cosmology (83F05) Quantum field theory on curved space or space-time backgrounds (81T20) Quantization of the gravitational field (83C45) Methods of quantum field theory in general relativity and gravitational theory (83C47) Research exposition (monographs, survey articles) pertaining to relativity and gravitational theory (83-02)
Related Items (5)
Cites Work
- Loop quantum cosmology: An overview
- Loop quantum cosmology and the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>k</mml:mi><mml:mo>=</mml:mo><mml:mo>−</mml:mo><mml:mn>1</mml:mn></mml:math>Robertson-Walker model
- Loop quantum cosmology of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>k</mml:mi><mml:mo>=</mml:mo><mml:mn>1</mml:mn></mml:math>FRW models
- Quantum nature of the big bang: Improved dynamics
- Semiclassical states in quantum cosmology: Bianchi I coherent states
- Closed Friedmann–Robertson–Walker model in loop quantum cosmology
- Quantum Nature of the Big Bang
- Background independent quantum gravity: a status report
- Modern Canonical Quantum General Relativity
- The flat FRW model in LQC: self-adjointness
- Loop quantum cosmology
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