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dc.contributor.advisorSitepu, Mimpin
dc.contributor.advisorSimbolon, Tua Raja
dc.contributor.authorRahmadani, Rahmadani
dc.date.accessioned2022-12-29T04:39:34Z
dc.date.available2022-12-29T04:39:34Z
dc.date.issued2011
dc.identifier.urihttps://repositori.usu.ac.id/handle/123456789/79064
dc.description.abstractIn this final settlement discussed Reissner-Nordstrom solution which is a spherical black hole solutions resulting from the expansion of the Schwarzschild metric. Schwarzschild metric is derived from Einstein's field equations that have a black hole in accordance with the relativity and the nature termodinamikanya. Based on the nature of black holes termodinamikanya black holes are classified into cold, warm black hole and black hole supersymmetry. On the black hole supersymmetry inserted element in the context of supersymmetry N = 2 and supergravity in four dimensions.en_US
dc.language.isoiden_US
dc.publisherUniversitas Sumatera Utaraen_US
dc.titlePengaruh Temperatur dan Sifat Supersimetri Lubang Hitam Sferisen_US
dc.typeThesisen_US
dc.identifier.nimNIM060801045
dc.identifier.nidnNIDN0015117202
dc.identifier.kodeprodiKODEPRODI45201#Fisika
dc.description.pages62 Halamanen_US
dc.description.typeSkripsi Sarjanaen_US


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