Thermal correlator at null infinity

A bstract We study the thermal Carrollian correlators at null infinity in the real-time formalism. We derive the Feynman rules to calculate these correlators in the position space. We compute the bulk-to-bulk, bulk-to-boundary and boundary-to-boundary propagators for massless scalar theory. Due to the doubling of the fields degrees of freedom, the number of each propagator is quadrupled. The bulk-to-boundary propagators have the form of (extended) Bose-Einstein distribution in the position space. Utilizing the contour integral of the propagators, we can transform the Feynman rules to momentum space. Interestingly, while the external lines and amplitudes in momentum space depend on the contour, Carrollian correlators in position space are independent of it. We show how to compute four-point correlators at finite temperature. The tree level correlators can be written as the summation of Barnes zeta functions and reduce to the ones in the zero temperature limit.

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Publication Details

Journal
Journal of High Energy Physics
Published
2025-10-15
DOI
https://doi.org/10.1007/jhep10(2025)127
Citations
1
Primary Topic
Black Holes and Theoretical Physics
Type
article
Field-Weighted Citation Impact
1.87

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article

Thermal correlator at null infinity

Jiang Long, Hong-Yang Xiao
1 citations
Journal of High Energy Physics
Black Holes and Theoretical Physics
1.87
article

Thermal correlator at null infinity

Jiang Long, Hong-Yang Xiao
article en
1 citations

Abstract

A bstract We study the thermal Carrollian correlators at null infinity in the real-time formalism. We derive the Feynman rules to calculate these correlators in the position space. We compute the bulk-to-bulk, bulk-to-boundary and boundary-to-boundary propagators for massless scalar theory. Due to the doubling of the fields degrees of freedom, the number of each propagator is quadrupled. The bulk-to-boundary propagators have the form of (extended) Bose-Einstein distribution in the position space. Utilizing the contour integral of the propagators, we can transform the Feynman rules to momentum space. Interestingly, while the external lines and amplitudes in momentum space depend on the contour, Carrollian correlators in position space are independent of it. We show how to compute four-point correlators at finite temperature. The tree level correlators can be written as the summation of Barnes zeta functions and reduce to the ones in the zero temperature limit.

Journal of High Energy PhysicsVol. 2025(10)
Huazhong University of Science and Technology (CN)
National Natural Science Foundation of China, Fundamental Research Funds for the Central Universities
Openalex Percentile: Top 11%
Black Holes and Theoretical Physics
1.87
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Thermal correlator at null infinity — Jiang Long, Hong-Yang Xiao · Journal of High Energy Physics (2025) | TGRS Research Map | TGRS