Superluminal censorship

DOI10.1016/S0920-5632(00)00782-9zbMath1273.83125arXivgr-qc/9810026OpenAlexW3037847640WikidataQ56048240 ScholiaQ56048240MaRDI QIDQ373107

Matt Visser, Stefano Liberati, Bruce A. Bassett

Publication date: 21 October 2013

Published in: Nuclear Physics. B. Proceedings Supplements (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9810026

Mathematics Subject Classification ID

Space-time singularities, cosmic censorship, etc. (83C75)

Related Items (21)

Time evolution after double trace deformation ⋮ Subluminal Galilean genesis ⋮ Relativistic charged spheres: compact stars, compactness and stable configurations ⋮ Does the Gauss–Bonnet term stabilize wormholes? ⋮ Ghost conditions for Gauss-Bonnet cosmologies ⋮ On causality conditions in de Sitter spacetime ⋮ Constraints on gravitation from causality and quantum consistency ⋮ Warp drive aerodynamics ⋮ Yukawa–Casimir wormholes in 4-D Einstein Gauss–Bonnet gravity ⋮ Superluminal travel made possible (in two dimensions) ⋮ General relativity from causality ⋮ Vaidya spacetimes, black-bounces, and traversable wormholes ⋮ Introducing physical warp drives ⋮ Breaking the warp barrier: hyper-fast solitons in Einstein–Maxwell-plasma theory ⋮ Conformal rigidity from focusing ⋮ Simple analytic model of wormhole formation ⋮ More on gravitational memory ⋮ Closed timelike curves and ‘effective’ superluminal travel with naked line singularities ⋮ Black-bounce to traversable wormhole ⋮ Faster than light photons in gravitational fields. II: Dispersion and vacuum polarisation ⋮ Challenges for emergent gravity

Cites Work

• The unphysical nature of `warp drive'
• Superluminal Travel Requires Negative Energies
• Wormholes in spacetime and their use for interstellar travel: A tool for teaching general relativity
• No warp drive
• Caustics of compensated spherical lens models
• The distortion of the area distance-redshift relation in inhomogeneous isotropic universes
• General Relativity
• Traversable wormholes from massless conformally coupled scalar fields

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