PIRSA:11050006

Electron star holography

APA

Hartnoll, S. (2011). Electron star holography. Perimeter Institute for Theoretical Physics. https://pirsa.org/11050006

MLA

Hartnoll, Sean. Electron star holography. Perimeter Institute for Theoretical Physics, May. 10, 2011, https://pirsa.org/11050006

BibTex

          @misc{ scivideos_PIRSA:11050006,
            doi = {10.48660/11050006},
            url = {https://pirsa.org/11050006},
            author = {Hartnoll, Sean},
            keywords = {Quantum Fields and Strings},
            language = {en},
            title = {Electron star holography},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2011},
            month = {may},
            note = {PIRSA:11050006 see, \url{https://scivideos.org/index.php/pirsa/11050006}}
          }
          

Sean Hartnoll Stanford University

Talk numberPIRSA:11050006
Source RepositoryPIRSA

Abstract

What is the gravity dual of a strongly interacting state of matter at zero temperature and finite charge density? The simplest candidates are extremal black holes. The presence of charged matter in the bulk can often mean that extremal black holes are not the ground state. In this talk I will discuss the physics of a class of solutions, essentially charged neutron stars, that can be thermodynamically preferred over extremal black holes.