Scalar field collapse in a conformally flat spacetime
arXiv:1609.01868 · doi:10.1140/epjc/s10052-017-4740-x
Abstract
The collapse scenario of a scalar field along with a perfect fluid distribution is investigated for a conformally flat spacetime. The theorem for the integrability of an anharmonic oscillator has been utilized. For a pure power law potential of the form , it is found that a central singularity is formed which is covered by an apparent horizon for and . Some numerical results have also been presented for a combination of two different powers of in the potential.
14 pages, 3 figures
References in corpus (4)
Cited by in corpus (15)
- Spherical inhomogeneous solutions of Einstein and scalar-tensor gravity: a map of the land
- Conformally Flat Collapsing Stars in f (R) gravity
- Some aspects of reconstruction using a scalar field in f (T ) Gravity
- Scalar field collapse in Gauss-Bonnet gravity
- Collapsing spherical star in Scalar-Einstein-Gauss-Bonnet gravity with a quadratic coupling
- Exact Solutions and Accelerating Universe in Modified Brans-Dicke Theories
- Self Similar Collapse and the Raychaudhuri equation
- Collapse driven by a scalar field without final singularity
- Reconstruction of lagrangian from a massive scalar field
- Electromagnetic effect on anisotropic scalar field collapse in higher curvature gravity
- Matter shear and vorticity in conformally flat spacetimes
- Spherically symmetric gravitational collapse in the background of Chaplygin gas
- Spherically Symmetric Gravitational Collapse Of Inhomogeneous Dust Cloud In The Background Of Dark Energy
- Critical phenomena in gravitational collapse of Husain-Martinez-Nunez scalar field
- Singularity formation in radiating star with dark energy background