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/10.1088/1475-7516/2008/02/015

Additional 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