Spherical Self-Similar Solutions in Einstein-Multi-Scalar Gravity

Abstract

We consider a general non-linear sigma model coupled to Einstein gravity and show that in spherical symmetry and for a simple realization of self-similarity, the spacetime can be completely determined. We also examine some more specific matter models and discuss their relation to critical collapse.

11 pages, 1 figure

References in corpus (2)

• Structure and stability of cold scalar-tensor black holes
• Perturbations and Critical Behavior in the Self-Similar Gravitational Collapse of a Massless Scalar Field

Cited by in corpus (2)

• Gravitational Collapse of Phantom Fluid in (2+1)-Dimensions
• Gravitational Collapse of an Imperfect Non Adiabatic Fluid