Charged black hole with string cloud deformation: Entanglement and chaos

We perform a holographic analysis of several quantum information-theoretic observables—entanglement entropy (EE), mutual information (MI), entanglement wedge cross section (EWCS), butterfly velocity ( <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"> <a:msub> <a:mi>v</a:mi> <a:mi>B</a:mi> </a:msub> </a:math> ), and thermo mutual information (TMI)—in the background of charged anti–de Sitter (AdS) black hole deformed by a homogeneous string cloud. This configuration is dual to a large <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"> <c:msub> <c:mi mathvariant="script">N</c:mi> <c:mi>c</c:mi> </c:msub> </c:math> strongly coupled field theory at finite temperature and finite chemical potential, in presence of quark-cloud. We study how the entanglement structure and chaotic dynamics in the boundary theory are affected by the charge and backreaction. In our observation we find that both EE and EWCS increase monotonically with charge and backreaction, indicating enhanced correlations due to additional degrees of freedom. On the other hand MI and TMI show a more intricate dependence: backreaction tends to strengthen correlations, while increasing charge suppresses entanglement and makes the system more susceptible to scrambling. The analysis of the butterfly velocity <f:math xmlns:f="http://www.w3.org/1998/Math/MathML" display="inline"> <f:msub> <f:mi>v</f:mi> <f:mi>B</f:mi> </f:msub> </f:math> indicates that the presence of charge and the backreaction suppress the chaotic behavior of the system by. Furthermore, TMI exhibits a sharp transition under shockwave perturbations, with interboundary entanglement being entirely disrupted beyond a critical shock strength, which decreases with increasing charge.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-10-07
DOI
https://doi.org/10.1103/vxnt-zf5j
Citations
1
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
1.87
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article

Charged black hole with string cloud deformation: Entanglement and chaos

Shagun Kaushal, Himanshu Parihar, Arpit Maurya, Sanjay Pant
1 citations
Physical review. D/Physical review. D.
Black Holes and Theoretical Physics
1.87
article

Charged black hole with string cloud deformation: Entanglement and chaos

Shagun Kaushal, Himanshu Parihar, Arpit Maurya, Sanjay Pant
article en
1 citations

Abstract

We perform a holographic analysis of several quantum information-theoretic observables—entanglement entropy (EE), mutual information (MI), entanglement wedge cross section (EWCS), butterfly velocity ( <a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"> <a:msub> <a:mi>v</a:mi> <a:mi>B</a:mi> </a:msub> </a:math> ), and thermo mutual information (TMI)—in the background of charged anti–de Sitter (AdS) black hole deformed by a homogeneous string cloud. This configuration is dual to a large <c:math xmlns:c="http://www.w3.org/1998/Math/MathML" display="inline"> <c:msub> <c:mi mathvariant="script">N</c:mi> <c:mi>c</c:mi> </c:msub> </c:math> strongly coupled field theory at finite temperature and finite chemical potential, in presence of quark-cloud. We study how the entanglement structure and chaotic dynamics in the boundary theory are affected by the charge and backreaction. In our observation we find that both EE and EWCS increase monotonically with charge and backreaction, indicating enhanced correlations due to additional degrees of freedom. On the other hand MI and TMI show a more intricate dependence: backreaction tends to strengthen correlations, while increasing charge suppresses entanglement and makes the system more susceptible to scrambling. The analysis of the butterfly velocity <f:math xmlns:f="http://www.w3.org/1998/Math/MathML" display="inline"> <f:msub> <f:mi>v</f:mi> <f:mi>B</f:mi> </f:msub> </f:math> indicates that the presence of charge and the backreaction suppress the chaotic behavior of the system by. Furthermore, TMI exhibits a sharp transition under shockwave perturbations, with interboundary entanglement being entirely disrupted beyond a critical shock strength, which decreases with increasing charge.

Physical review. D/Physical review. D.Vol. 112(8)
Indian Institute of Technology Ropar (IN), National Tsing Hua University (TW), National Center for Theoretical Sciences (TW), National Center for Theoretical Sciences, Physics Division, Graphic Era University (IN), Indian Institute of Technology Delhi (IN), Vellore Institute of Technology University (IN)
Openalex Percentile: Top 11%
Black Holes and Theoretical Physics
1.87
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