Publicação: Massive vector fields in Kerr-Newman and Kerr-Sen black hole spacetimes
dc.contributor.author | Cayuso, Ramiro | |
dc.contributor.author | Dias, Oscar J.C. | |
dc.contributor.author | Gray, Finnian | |
dc.contributor.author | Kubizňák, David | |
dc.contributor.author | Margalit, Aoibheann | |
dc.contributor.author | Santos, Jorge E. | |
dc.contributor.author | Souza, Renato Gomes [UNESP] | |
dc.contributor.author | Thiele, Leander | |
dc.contributor.institution | Perimeter Institute | |
dc.contributor.institution | University of Waterloo | |
dc.contributor.institution | University of Southampton | |
dc.contributor.institution | Centre for Mathematical Sciences | |
dc.contributor.institution | Institute for Advanced Study | |
dc.contributor.institution | Universidade Estadual Paulista (Unesp) | |
dc.date.accessioned | 2020-12-12T02:03:41Z | |
dc.date.available | 2020-12-12T02:03:41Z | |
dc.date.issued | 2020-04-01 | |
dc.description.abstract | The superradiant instability modes of ultralight massive vector bosons are studied for weakly charged rotating black holes in Einstein-Maxwell gravity (the Kerr- Newman solution) and low-energy heterotic string theory (the Kerr-Sen black hole). We show that in both these cases, the corresponding massive vector (Proca) equations can be fully separated, exploiting the hidden symmetry present in these spacetimes. The resultant ordinary differential equations are solved numerically to find the most unstable modes of the Proca field in the two backgrounds and compared to the vacuum (Kerr black hole) case. | en |
dc.description.affiliation | Perimeter Institute, 31 Caroline Street North | |
dc.description.affiliation | Department of Physics and Astronomy University of Waterloo | |
dc.description.affiliation | STAG research centre and Mathematical Sciences Highfield Campus University of Southampton | |
dc.description.affiliation | DAMTP Centre for Mathematical Sciences, Wilberforce Road | |
dc.description.affiliation | Institute for Advanced Study | |
dc.description.affiliation | ICTP South American Institute for Fundamental Research IFT-UNESP | |
dc.description.affiliationUnesp | ICTP South American Institute for Fundamental Research IFT-UNESP | |
dc.identifier | http://dx.doi.org/10.1007/JHEP04(2020)159 | |
dc.identifier.citation | Journal of High Energy Physics, v. 2020, n. 4, 2020. | |
dc.identifier.doi | 10.1007/JHEP04(2020)159 | |
dc.identifier.issn | 1029-8479 | |
dc.identifier.issn | 1126-6708 | |
dc.identifier.scopus | 2-s2.0-85083833824 | |
dc.identifier.uri | http://hdl.handle.net/11449/200326 | |
dc.language.iso | eng | |
dc.relation.ispartof | Journal of High Energy Physics | |
dc.source | Scopus | |
dc.subject | Black Holes | |
dc.subject | Black Holes in String Theory | |
dc.title | Massive vector fields in Kerr-Newman and Kerr-Sen black hole spacetimes | en |
dc.type | Artigo | |
dspace.entity.type | Publication | |
unesp.campus | Universidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulo | pt |