On trapped surface formation in gravitational collapse II

Abstract

Further to our consideration on trapped surfaces in gravitational collapse, where pressures were allowed to be negative while satisfying weak energy condition to avoid trapped surface formation, we discuss here several other attempts of similar nature in this direction. Certain astrophysical aspects are pointed out towards examining the physical realization of such a possibility in realistic gravitational collapse.

References in corpus (3)

• Gravitational collapse of homogeneous scalar fields
• Gravitational collapse of an isentropic perfect fluid with a linear equation of state
• A Time-Like Naked Singularity

Cited by in corpus (5)

• Naked Singularities as Particle Accelerators II
• Einstein-Cartan gravitational collapse of a homogeneous Weyssenhoff fluid
• Trapped surfaces and nature of singularities in Lyra's geometry
• Gravitational collapse with tachyon field and barotropic fluid
• Singularity Avoidance in Gravitational Collapse of an Inhomogeneous Fluid in Rastall Gravity