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<rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:dc="http://purl.org/dc/elements/1.1/"><rdf:Description rdf:about="https://dk.um.si/IzpisGradiva.php?id=81528"><dc:title>Conformal symmetries for extremal black holes with general asymptotic scalars in STU supergravity</dc:title><dc:creator>Cvetič,	Mirjam	(Avtor)
	</dc:creator><dc:creator>Pope,	Christopher N.	(Avtor)
	</dc:creator><dc:creator>Saha,	Aritra	(Avtor)
	</dc:creator><dc:subject>black holes</dc:subject><dc:subject>extended supersymmetry</dc:subject><dc:subject>supergravity models</dc:subject><dc:subject>string theory</dc:subject><dc:description>We present a construction of the most general BPS black holes of STU supergravity (N = 2 supersymmetric D = 4 supergravity coupled to three vector supermultiplets) with arbitrary asymptotic values of the scalar fields. These solutions are obtained by acting with a subset of the global symmetry generators on STU BPS black holes with zero values of the asymptotic scalars, both in the U-duality and the heterotic frame. The solutions are parameterized by fourteen parameters: four electric and four magnetic charges, and the asymptotic values of the six scalar fields. We also present BPS black hole solutions of a consistently truncated STU supergravity, which are parameterized by two electric and two magnetic charges and two scalar fields. These latter solutions are significantly simplified, and are very suitable for further explicit studies. We also explore a conformal inversion symmetry of the Couch-Torrence type, which maps any member of the fourteen-parameter family of BPS black holes to another member of the family. Furthermore, these solutions are expected to be valuable in the studies of various swampland conjectures in the moduli space of string compactifications.</dc:description><dc:publisher>SISSA</dc:publisher><dc:date>2021</dc:date><dc:date>2022-04-08 14:56:48</dc:date><dc:type>Znanstveno delo</dc:type><dc:identifier>81528</dc:identifier><dc:language>sl</dc:language></rdf:Description></rdf:RDF>
