<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/CINECAstyle.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-09-23T17:47:03Z</responseDate><request verb="GetRecord" identifier="oai:iris.unica.it:11584/266452" metadataPrefix="oai_dc">https://iris.unica.it/oai/request</request><GetRecord><record><header><identifier>oai:iris.unica.it:11584/266452</identifier><datestamp>2022-10-15T12:12:07Z</datestamp><setSpec>com_11584_207615</setSpec><setSpec>com_11584_111066</setSpec><setSpec>col_11584_265854</setSpec></header><metadata><oai_dc:dc xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:doc="http://www.lyncode.com/xoai" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:dc="http://purl.org/dc/elements/1.1/" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
<dc:title>Black brane solutions of Einstein-scalar-Maxwell gravity&#xd;
and their holographic applications</dc:title>
<dc:creator>SERRA, MATTEO</dc:creator>
<dc:subject>ads/cft correspondence</dc:subject>
<dc:subject>black branes</dc:subject>
<dc:subject>buchi neri</dc:subject>
<dc:subject>corrispondenza ads/cft</dc:subject>
<dc:subject>holography</dc:subject>
<dc:subject>olografia</dc:subject>
<dc:subject>Settore FIS/02 - Fisica Teorica, Modelli e Metodi Matematici</dc:subject>
<dc:description>Black hole solutions of Einstein (and Einstein-Maxwell) gravity coupled to scalar fields have acquired a growing interest and importance in recent years.&#xd;
This interest is motivated both by more \classical" issues, as the problem of the uniqueness of classical black holes solutions (and related \no-hair" theorems), and mainly by recent applications of the AdS/CFT correspondence,&#xd;
an holographic duality which allows to describe, starting from a gravitational theory, strongly coupled quantum field theories.&#xd;
In this thesis, we treat this topic both from a pure gravitational point of view and from the holographic perspective. In particular, we propose a general method for exactly solving, in some cases, the field equations of&#xd;
Einstein-scalar-Maxwell gravity, and present some new analytical and numerical solutions (we mainly focus on black brane solutions, i.e. solutions with a planar event horizon). Moreover, we discuss hyperscaling violation,&#xd;
a particular scaling behavior of free energy and entropy (as functions of the temperature), typical of some phase transitions of real condensed matter systems.&#xd;
Hyperscaling violation can be described, via AdS/CFT, starting from a gravitational solution with a particular symmetry.&#xd;
Finally, we perform some interesting results about the mass spectrum and stability of black brane solutions in a wide class of gravitational models.&#xd;
In particular, the thermodynamics of some solutions of these models provides important information about the possible existence of physicallyrelevant phase transitions in the dual field theories.</dc:description>
<dc:date>2014-04-16</dc:date>
<dc:type>info:eu-repo/semantics/doctoralThesis</dc:type>
<dc:identifier>http://hdl.handle.net/11584/266452</dc:identifier>
<dc:language>eng</dc:language>
<dc:relation>numberofpages:203</dc:relation>
<dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
<dc:publisher>Università degli Studi di Cagliari</dc:publisher>
<dc:rights>license:Non specificato</dc:rights>
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