Abstract

Loop corrections to unequal-time correlation functions in Minkowski spacetime exhibit secular growth due to a breakdown of time-dependent perturbation theory. This is analogous to secular growth in equal-time correlators on time-dependent backgrounds, except that in Minkowski the divergences must not signal a real IR issue. In this paper, we calculate the late-time limit of the two-point correlator for different massless self-interacting scalar quantum field theories on a Minkowski background. We first use a late-time version of the in-in path integral starting in the vacuum of the free theory; in this limit, the calculation, including UV renormalization, reduces to that in in-out. We find linear or logarithmic growth in time, depending on whether the interaction strength is dimension-one or dimensionless, respectively. We next develop the Weisskopf-Wigner resummation method, that proceeds by demanding unitarity within a truncated Hilbert space, to calculate the resummed correlator and find that it gives an exact exponentiation of the late-time perturbative result. The resummed (unequal-time) correlator thus decays with an exponential or polynomial time-dependence, which is suggestive of ‘universal’ behavior that depends on the dimensions of the interaction strength.

Details

Title
Loop corrections in Minkowski spacetime away from equilibrium. Part I. Late-time resummations
Author
Chaykov, Spasen 1 ; Agarwal, Nishant 1 ; Bahrami, Sina 2 ; Holman, R. 3 

 University of Massachusetts, Department of Physics and Applied Physics, Lowell, USA (GRID:grid.225262.3) (ISNI:0000 0000 9620 1122) 
 The Pennsylvania State University, Institute for Gravitation and the Cosmos, University Park, USA (GRID:grid.29857.31) (ISNI:0000 0001 2097 4281) 
 Minerva University, San Francisco, USA (GRID:grid.29857.31) 
Pages
93
Publication year
2023
Publication date
Mar 2023
Publisher
Springer Nature B.V.
e-ISSN
10298479
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2784120874
Copyright
© The Author(s) 2023. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.