dc.contributor | Universidade Estadual Paulista (Unesp) | |
dc.date.accessioned | 2019-10-06T16:47:44Z | |
dc.date.accessioned | 2022-12-19T18:57:28Z | |
dc.date.available | 2019-10-06T16:47:44Z | |
dc.date.available | 2022-12-19T18:57:28Z | |
dc.date.created | 2019-10-06T16:47:44Z | |
dc.date.issued | 2019-08-26 | |
dc.identifier | Physical Review D, v. 100, n. 4, 2019. | |
dc.identifier | 2470-0029 | |
dc.identifier | 2470-0010 | |
dc.identifier | http://hdl.handle.net/11449/189656 | |
dc.identifier | 10.1103/PhysRevD.100.045021 | |
dc.identifier | 2-s2.0-85072216819 | |
dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/5370694 | |
dc.description.abstract | I present a general relativistic model with a compactified second time coordinate that a priori allows for causal, yet faster than light travel in the background of a Friedmann-Lemaître-Robertson-Walker geometry, by local modification of a higher dimensional background geometry, specifically with respect to the radius of the compactified time coordinate. The modification can be induced via the fields of the model. I show that one cannot convert (as possible in special relativistic models, or simple general relativistic models) the superluminality into closed timelike loops violating causality, due to a novel combination of factors, at least for vmax≤2. The physics of the second time is constrained by postulates derived from reasonable physical assumptions. I comment on the possibility of experimental implications of the model. | |
dc.language | eng | |
dc.relation | Physical Review D | |
dc.rights | Acesso aberto | |
dc.source | Scopus | |
dc.title | Causal faster-than-light travel from a localized second time coordinate | |
dc.type | Artículos de revistas | |