Evanescent gravitons in Warped Anti-de Sitter space
Paste one version of a text here.Besides black holes, the phase space of three-dimensional massive gravity about Warped-Anti de Sitter (WAdS) space contains solutions that decay exponentially in time. They describe evanescent graviton configurations that, while governed by a wave equation with non-v...
| Authors: | ; |
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| Format: | Article |
| Status: | Published version |
| Publication date: | 2016 |
| Country: | Argentina |
| Institution: | Consejo Nacional de Investigaciones Científicas y Técnicas |
| Repository: | CONICET Digital (CONICET) |
| Language: | English |
| OAI Identifier: | oai:ri.conicet.gov.ar:11336/46652 |
| Online Access: | http://hdl.handle.net/11336/46652 |
| Access Level: | Open access |
| Keyword: | Ads/Cft Black Holes https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| Summary: | Paste one version of a text here.Besides black holes, the phase space of three-dimensional massive gravity about Warped-Anti de Sitter (WAdS) space contains solutions that decay exponentially in time. They describe evanescent graviton configurations that, while governed by a wave equation with non-vanishing effective mass, do not carry net gravitational energy. Explicit examples of such solutions have been found in the case of Topologically Massive Gravity; here, we generalize them to a much more general ghost-free massive deformation, with the difference being that the decay rate gets corrected due to the presence of higher-order terms. |
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