Instability of charged massive scalar fields in bound states around Kerr–Sen black holes

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dc.contributor.author Siahaan, Haryanto Mangaratua
dc.date.accessioned 2017-12-14T08:29:05Z
dc.date.available 2017-12-14T08:29:05Z
dc.date.issued 2015
dc.identifier.issn 1793-6594
dc.identifier.uri http://hdl.handle.net/123456789/4616
dc.description International Journal of Modern Physics D; 2015
dc.description.abstract In this paper, we show the instability of a charged massive scalar field in bound states around Kerr–Sen black holes. By matching the near and far region solutions of the radial part in the corresponding Klein–Gordon equation, one can show that the frequency of bound state scalar fields contains an imaginary component which gives rise to an amplification factor for the fields. Hence, the unstable modes for a charged and massive scalar perturbation in Kerr–Sen background can be shown. en_US
dc.description.uri https://www.worldscientific.com/doi/pdf/10.1142/S0218271815501023
dc.language.iso en en_US
dc.publisher World Scientific Publishing Company en_US
dc.relation.ispartofseries International Journal of Modern Physics D;2015
dc.subject INSTABILITY en_US
dc.subject CHARGED MASSIVE SCALARS en_US
dc.subject BOUND STATES en_US
dc.subject Kerr–Sen BLACK HOLES en_US
dc.title Instability of charged massive scalar fields in bound states around Kerr–Sen black holes en_US
dc.type Journal Articles en_US


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