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

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