Quantum Vacuum Instability Near Rotating Stars
arXiv:gr-qc/9212004 · doi:10.1103/PhysRevD.47.1557
Abstract
We discuss the Starobinskii-Unruh process for the Kerr black hole. We show how this effect is related to the theory of squeezed states. We then consider a simple model for a highly relativistic rotating star and show that the Starobinskii-Unruh effect is absent.
17 Pages, (accepted by PRD), (previously incorrect header files have been corrected)
Cited by in corpus (23)
- Quantum Radiation from a 5-Dimensional Rotating Black Hole
- The Rotating Quantum Vacuum
- The renormalized stress tensor in Kerr space-time: general results
- Kermions: quantization of fermions on Kerr space-time
- Quantum Aspects of Ergoregion Instability
- Acceleration radiation of an atom freely falling into a Kerr black hole and near-horizon conformal quantum mechanics
- Superradiance and the Statistical-Mechanical Entropy of Rotating BTZ Black Holes
- Quantum optics meets black hole thermodynamics via conformal quantum mechanics: II. Thermodynamics of acceleration radiation
- Spontaneous excitation of an atom in a Kerr spacetime
- Is the brick-wall model unstable for a rotating background?
- Entanglement dynamics in a Kerr spacetime
- Density Fluctuations in the Oscillatory Phase of Nonclassical Inflaton in FRW Universe
- Instability of nonminimally coupled scalar fields in the spacetime of slowly rotating compact objects
- Entanglement from superradiance and rotating quantum fluids of light
- Zero-point excitation of a circularly moving detector in an atomic condensate and phonon laser dynamical instabilities
- Entanglement Entropy Renormalization for the NC scalar field coupled to classical BTZ geometry
- Quantization of a charged scalar field on a charged black hole background
- Particle creation in the oscillatory phase of inflaton
- Rotating Black Hole Entropy from Two Different Viewpoints
- Atom-field dynamics in curved spacetime
- Quantum Ergoregion Instability
- Quantum Radiation Properties of General Nonstationary Black Hole
- Squeezed Thermal State Representation of the Inflaton and Particle Production in Bianchi type-I Universe