PIRSA:14090072

Conformal field theories at non-zero temperature: operator product expansions, Monte Carlo, and holography

APA

(2014). Conformal field theories at non-zero temperature: operator product expansions, Monte Carlo, and holography. Perimeter Institute for Theoretical Physics. https://pirsa.org/14090072

MLA

Conformal field theories at non-zero temperature: operator product expansions, Monte Carlo, and holography. Perimeter Institute for Theoretical Physics, Sep. 19, 2014, https://pirsa.org/14090072

BibTex

          @misc{ scivideos_PIRSA:14090072,
            doi = {10.48660/14090072},
            url = {https://pirsa.org/14090072},
            author = {},
            keywords = {Quantum Fields and Strings, Quantum Matter, Strong Gravity},
            language = {en},
            title = {Conformal field theories at non-zero temperature: operator product expansions, Monte Carlo, and holography},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2014},
            month = {sep},
            note = {PIRSA:14090072 see, \url{https://scivideos.org/index.php/pirsa/14090072}}
          }
          
Talk numberPIRSA:14090072
Source RepositoryPIRSA
Collection

Abstract

We discuss properties of 2-point functions in CFTs in 2+1D at finite temperature. For concreteness, we focus on those involving conserved flavour currents, in particular on the associated conductivity. At frequencies much greater than the temperature, ω >> T, the ω dependence of the conductivity can be computed from the operator product expansion (OPE) between the currents and operators which acquire a non-zero expectation value at T > 0. Such results are found to be in excellent agreement with quantum Monte Carlo studies of the O(2) Wilson-Fisher CFT. Results for the conductivity and other observables are also obtained in vector 1/N expansions. We match these large ω results to the corresponding correlators of holographic representations of the CFT: the holographic approach then allows us to extrapolate to small ω/T. Other holographic studies implicitly only used the OPE between the currents and the energy-momentum tensor, and this yields the correct leading large ω behavior for a large class of CFTs. However, for the Wilson-Fisher CFT a relevant “thermal” operator must also be considered, and then consistency with the Monte Carlo results is obtained without a previously needed ad hoc rescaling of the T value [1]. We also use the OPE to prove sum rules obeyed by the conductivity. **In collaboration with A. Katz, S. Sachdev and E. Sørensen** [1] WWK, E. Sørensen, S. Sachdev, Nat. Phys. 10, 361 (2014)