Vacuum polarization of a massive scalar field in a wormhole spacetime
arXiv:1003.0344 · doi:10.1103/PhysRevD.81.084034
Abstract
We calculate the vacuum average value of the field square and the stress-energy tensor of a massive scalar field, with non-minimal coupling to the curvature in the short-throat flat-space wormhole background. The obtained results are not suitable for an analytical analysis and for this reason we provide a numerical analysis for different values of the coupling constant, . It was shown that the vacuum polarization cannot self-consistently support the wormhole. Otherwise, the energy-momentum tensor does not violate the null energy condition near the throat.
arXiv comment7 pages, 5 figures
References in corpus (17)
- Heat kernel expansion: user's manual
- Geometric structure of the generic static traversable wormhole throat
- Dynamic wormholes, anti-trapped surfaces, and energy conditions
- Self-consistent Wormhole Solutions of Semiclassical Gravity
- Self sustained phantom wormholes in semi-classical gravity
- Self-sustained traversable wormholes in noncommutative geometry
- Heat trace asymptotics with transmittal boundary conditions and quantum brane-world scenario
- Self Sustained Traversable Wormholes?
- Ground state energy in a wormhole space-time
- Casimir effect in a wormhole spacetime
- Stress-energy of a quantized scalar field in static wormhole spacetimes
- Vacuum polarization of a scalar field in wormhole spacetimes
- Rotating vacuum wormhole
- Self-force on a scalar particle in a class of wormhole spacetimes
- Semiclassical wormholes
- Self sustained traversable wormholes and the equation of state
- Analitical approximation of for a massive scalar field in static spherically symmetric spacetimes