Phantom scalar field counterpart to Curzon-Chazy spacetime
arXiv:2112.11738 · doi:10.1088/1361-6382/ac8267
Abstract
We derive and analyze phantom scalar field counterpart to Curzon-Chazy spacetime. Such solution contains wormhole throat while the region inside the throat behaves like a one-directional time machine. We describe its conformal structure and non-scalar singularity hidden inside the wormhole. We examine the results provided by different definitions of mass of spacetime to understand their value in the presence of phantom matter. The electromagnetic generalization of this spacetime is as well briefly considered.
References in corpus (15)
- The Gravitational Hamiltonian, Action, Entropy, and Surface Terms
- The phantom menaced: constraints on low-energy effective ghosts
- Black-bounce to traversable wormhole
- The null energy condition in dynamic wormholes
- Dynamic wormholes
- Light's Bending Angle due to Black Holes: From the Photon Sphere to Infinity
- Weyl metrics and wormholes
- Gravitational energy in stationary spacetimes
- Robinson-Trautman solution with scalar hair
- Properties of Robinson--Trautman solution with scalar hair
- Scalar Hairy Black Holes in the presence of Nonlinear Electrodynamics
- Brown-York Energy and Radial Geodesics
- Nonsymmetric Dynamical Thin-Shell Wormhole in Robinson--Trautman Class
- Higher-dimensional Buchdahl and Janis-Robinson-Winicour transformations in the Einstein-Maxwell system with a massless scalar field
- Quantum fate of timelike naked singularity with scalar hair