English   español  
Please use this identifier to cite or link to this item: http://hdl.handle.net/10261/162453
Share/Impact:
Statistics
logo share SHARE logo core CORE   Add this article to your Mendeley library MendeleyBASE

Visualizar otros formatos: MARC | Dublin Core | RDF | ORE | MODS | METS | DIDL
Exportar a otros formatos:

Title

Stability of Schwarzschild singularity in non-local gravity

AuthorsCalcagni, Gianluca ; Modesto, Leonardo
Issue Date12-Sep-2017
PublisherElsevier
CitationPhysics Letters B, 773: 596-600 (2017)
AbstractIn a previous work, it was shown that all Ricci-flat spacetimes are exact solutions for a large class of non-local gravitational theories. Here we prove that, for a subclass of non-local theories, the Schwarzschild singularity is stable under linear perturbations. Thus, non-locality may be not enough to cure all the singularities of general relativity. Finally, we show that the Schwarzschild solution can be generated by the gravitational collapse of a thin shell of radiation.
Description5 pags. -- Open Access funded by Creative Commons Atribution Licence 4.0
Publisher version (URL)https://doi.org/10.1016/j.physletb.2017.09.018
URIhttp://hdl.handle.net/10261/162453
Identifiersdoi: 10.1016/j.physletb.2017.09.018
issn: 1873-2445
Appears in Collections:(CFMAC-IEM) Artículos
Files in This Item:
File Description SizeFormat 
Stability of Schwarzschild.pdf232,81 kBAdobe PDFThumbnail
View/Open
Show full item record
Review this work
 

Related articles:


WARNING: Items in Digital.CSIC are protected by copyright, with all rights reserved, unless otherwise indicated.