Counter-rotating Kerr manifolds separated by a fluid shell

Abstract

We describe a spheroidal fluid shell between two Kerr vacuum regions which have opposite rotation parameters. The shell has a stiff equation of state and a heat flow vector related to the rotational Killing current. The shell description is useful in exploring the significance of counter-rotation in Kerr metric matches.

References in corpus (3)

• Spectacular Shells in the Host Galaxy of the QSO MC2 1635+119
• Negative Komar Mass of Single Objects in Regular, Asymptotically Flat Spacetimes
• Spinning Up Asymptotically Flat Spacetimes

Cited by in corpus (5)

• Collapsing thin shells with rotation
• Counterrotational effects on stability of 2+1-dimensional thin-shell wormholes
• Approximate Metric for a Rotating Deformed Mass
• Scalarization of Chern-Simons Kerr Black Hole Solutions and Wormholes
• Signatures of the Israel Junction II: Double Photon Rings in Slowly Rotating Kerr Spacetime with Thin Shell