PIRSA:11050006

Electron star holography

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

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

          @misc{ pirsa_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},
            year = {2011},
            month = {may},
            note = {PIRSA:11050006 see, \url{https://pirsa.org}}
          }

Sean Hartnoll

Stanford University

Talk number
PIRSA:11050006
Collection
Talk Type
Subject
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.