Published February 2008
| Version v1
Journal article
Reconstruction of scalar potentials in two-field cosmological models
- 1. V A Fock Department of Theoretical Physics, Saint Petersburg State University, 198904 S.-Petersburg (Russian Federation)
- 2. INFN, Via Irnerio 46, I-40126 Bologna (Italy)
- 3. Dipartimento di Fisica, Via Irnerio 46, I-40126 Bologna (Italy)
Description
We study the procedure of the reconstruction of phantom-scalar field potentials in two-field cosmological models. It is shown that, while in the one-field case the chosen cosmological evolution defines uniquely the form of the scalar potential, in the two-field case one has an infinite number of possibilities. The classification of a large class of possible potentials is presented and the dependence of cosmological dynamics on the choice of initial conditions is investigated qualitatively and numerically for two particular models
Availability note (English)
Available from http://dx.doi.org/10.1088/1475-7516/2008/02/015Additional details
Identifiers
- DOI
- 10.1088/1475-7516/2008/02/015;
- PII
- S1475-7516(08)71980-3;
Publishing Information
- Journal Title
- Journal of Cosmology and Astroparticle Physics
- Journal Volume
- 2008
- Journal Issue
- 02
- Journal Page Range
- [18 p.]
- ISSN
- 1475-7516
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44092529
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMOLOGICAL MODELS; GALACTIC EVOLUTION; POTENTIALS; SCALAR FIELDS
- Descriptors DEC
- EVOLUTION; MATHEMATICAL MODELS