Published August 15, 2010
| Version v1
Journal article
Observables for a Friedmann-Robertson-Walker model with a cosmological constant in the framework of loop cosmology
- 1. Theoretical Physics Department, Institute for Nuclear Studies, 00-681 Warszawa, Hoza 69 (Poland)
- 2. Astronomical Observatory, Jagiellonian University, 30-244 Krakow, Orla 171 (Poland)
Description
We consider a flat cosmological model with a free massless scalar field and the cosmological constant Λ in the framework of loop quantum cosmology. The scalar field plays the role of an intrinsic time. We apply the reduced phase space approach. The dynamics of the model is solved analytically. We identify elementary observables and their algebra. The compound physical observables like the volume and the energy density of matter field are analyzed. Both compound observables are bounded and oscillate in the Λ<0 case. The energy density is bounded and oscillates in the Λ>0 case. However, the volume is unbounded from above, but periodic. The difference between standard and nonstandard loop quantum cosmology is described.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.82.043529;
- arXiv
- arXiv:1001.3999v3;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 82
- Journal Issue
- 4
- Journal Page Range
- p. 043529-043529.10
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42015330
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMOLOGICAL CONSTANT; COSMOLOGICAL MODELS; COSMOLOGY; ENERGY DENSITY; MATTER; PERIODICITY; PHASE SPACE; SCALAR FIELDS; SIMULATION
- Descriptors DEC
- MATHEMATICAL MODELS; MATHEMATICAL SPACE; SPACE; VARIATIONS
Optional Information
- Notes
- (c) 2010 American Institute of Physics