Mar 17 – 19, 2026
Politecnico di Torino
Europe/Rome timezone

Holographic thermal propagator from modularity

Not scheduled
30m
Room Buzano, at DISMA, 3rd floor (Politecnico di Torino)

Room Buzano, at DISMA, 3rd floor

Politecnico di Torino

Corso Duca degli Abruzzi, 24, 10129 Torino (TO), Italy
Contributed Talks Contributed Talk

Description

We revisit the low-temperature thermal propagator of a holographic conformal field theory in four spacetime dimensions by exploiting its connection to the Nekrasov–Shatashvili (NS) limit of the $\Omega$-deformed $\mathcal{N}=2$ supersymmetric $SU(2)$ Yang–Mills theory with $N_f=4$ hypermultiplets. In the regime of vanishing energy, the low-temperature expansion corresponds to a large adjoint vacuum expectation value expansion. In this limit, we show that a second expansion in instanton numbers organizes into quasi-modular forms, which can be resummed into closed-form expressions in terms of Eisenstein series. The resulting thermal propagator series in positive powers of small temperatures exhibits clear signs of being asymptotic. Our method—combining modular properties, $q$-recursion techniques, and the NS prepotential—provides a systematic and computationally efficient framework for analyzing retarded Green's functions of holographic black branes in the low-temperature limit.

Author

Katarina Trailović (Institute Jožef Stefan)

Co-author

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