BOUNCING UNIVERSE WITH THE NON-MINIMALLY COUPLED SCALAR FIELD AND ITS RECONSTRUCTION

2009/04/01 by J. Sadeghi, Farzad Milani, F. Milani +2 · 27 citations
Physics and Astronomy · #Advanced Differential Geometry Research #Black Holes and Theoretical Physics #Classical field theory #Classical mechanics #Cosmology and Gravitation Theories #Equation of state #Field (mathematics) #Geometry #Gravitation #Mathematical physics #Physics #Quantum mechanics #Scalar (mathematics) #Scalar field #Scalar theories of gravitation #Stability (learning theory) #Theoretical physics #Universe #gr-qc

paper · pdf · doi:10.1142/s0217732309030783

published in Modern Physics Letters A 24(29), 2363-2376 (World Scientific) · 16 pages, 9 figures. Accepted in MPLA

arxiv created 2009/04/01 · openalex publication_date 2009/09/21 · arxiv updated 2010/04/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

In this paper we consider a non-minimally coupled scalar field, and show that its equation of state parameter can cross over -1, ω→-1, and bouncing condition. Also we obtain the stability conditions and consider reconstructing for our model.

Citations

• Phantom Energy: Dark Energy withw<−1Causes a Cosmic Doomsday
• WMAP constraints on low redshift evolution of dark energy
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Cosmology with a time-variable cosmological 'constant'
• Quantum effects can renderw<−1on cosmological scales
• Cosmology as geodesic motion
• Cosmological evolution of a quintom model of dark energy
• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Preliminary Maps and Basic Results
• Constraints on linear negative potentials in quintessence and phantom models from recent supernova data
• Accelerating Universes with Scaling Dark Matter
• First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Determination of Cosmological Parameters
• Reconstruction of the deceleration parameter and the equation of state of dark energy

Cited by

• The bouncing cosmology with F(R) gravity and its reconstructing
• Bouncing universe with the modified gravity coupled to the Weyl tensor
• Scalar-tensor cosmologies with a potential in the general relativity limit: Time evolution