Secular growths and their relation to equilibrium states in perturbative QFT
Stefano Galanda, Nicola Pinamonti, Leonardo Sangaletti

TL;DR
This paper investigates conditions under which secular growths in perturbative quantum field theory can be avoided, demonstrating that spatially compact interactions and suitable background states prevent these growths, especially in thermal equilibrium.
Contribution
It shows that secular effects can be avoided in perturbative QFT with compact spatial support of interactions and specific background states, extending previous results to more general states.
Findings
Secular growths are avoided with compact spatial support of interactions.
Thermalisation ensures no secular effects in the large time limit.
Results apply to scalar and Dirac fields in external electromagnetic potentials.
Abstract
In the perturbative treatment of interacting quantum field theories, if the interaction Lagrangian changes adiabatically in a finite interval of time, secular growths may appear in the truncated perturbative series also when the interaction Lagrangian density is returned to be constant. If this happens, the perturbative approach does not furnish reliable results in the evaluation of scattering amplitudes or expectation values. In this paper we show that these effects can be avoided for adiabatically switched-on interactions, if the spatial support of the interaction is compact and if the background state is suitably chosen. We start considering equilibrium background states and show that, when thermalisation occurs (interaction Lagrangian of spatial compact support), secular effects are avoided. Furthermore, no secular effects pop up if the limit where the Lagrangian is supported…
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Taxonomy
TopicsQuantum Electrodynamics and Casimir Effect · Cold Atom Physics and Bose-Einstein Condensates · Quantum, superfluid, helium dynamics
