Quantum phase transition of infrared radiation

Fuente: arXiv
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Autori principali: Biadasiewicz, Bartosz, Dybalski, Wojciech
Natura: Preprint
Pubblicazione: 2024
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author Biadasiewicz, Bartosz
Dybalski, Wojciech
author_facet Biadasiewicz, Bartosz
Dybalski, Wojciech
contents We describe a phase transition of infrared radiation, driven by quantum fluctuations, which takes place at the boundary of (the conformal diagram of) Minkowski spacetime. Specifically, we consider a family of states interpolating between the vacuum and the Kraus-Polley-Reents infravacuum. A state from this family can be imagined as a static source emitting flashes of infrared radiation in distant past. The flashes are in suitable squeezed states and the time intervals between them are controlled by a certain parameter r. For r<0 the states are lightcone normal, thus physically indistinguishable from local excitations of the vacuum. They suffer from the usual infrared problems such as disintegration of the Bloch-Nordsieck S-matrix and rotational symmetry breaking by soft photon clouds. However, for r>0 lightcone normality breaks down, the S-matrix is stabilized by the Kraus-Polley-Reents mechanism and the rotational symmetry is restored. We interpret these two situations as ordered (r<0) and disordered (r>0) phase of infrared radiation, and show that they can be distinguished by asymptotic fluctuations of the fields. We also determine the singular behaviour of some S-matrix elements near the critical point r=0.
format Preprint
id arxiv_https___arxiv_org_abs_2406_00203
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Quantum phase transition of infrared radiation
Biadasiewicz, Bartosz
Dybalski, Wojciech
High Energy Physics - Theory
Quantum Gases
Statistical Mechanics
Mathematical Physics
We describe a phase transition of infrared radiation, driven by quantum fluctuations, which takes place at the boundary of (the conformal diagram of) Minkowski spacetime. Specifically, we consider a family of states interpolating between the vacuum and the Kraus-Polley-Reents infravacuum. A state from this family can be imagined as a static source emitting flashes of infrared radiation in distant past. The flashes are in suitable squeezed states and the time intervals between them are controlled by a certain parameter r. For r<0 the states are lightcone normal, thus physically indistinguishable from local excitations of the vacuum. They suffer from the usual infrared problems such as disintegration of the Bloch-Nordsieck S-matrix and rotational symmetry breaking by soft photon clouds. However, for r>0 lightcone normality breaks down, the S-matrix is stabilized by the Kraus-Polley-Reents mechanism and the rotational symmetry is restored. We interpret these two situations as ordered (r<0) and disordered (r>0) phase of infrared radiation, and show that they can be distinguished by asymptotic fluctuations of the fields. We also determine the singular behaviour of some S-matrix elements near the critical point r=0.
title Quantum phase transition of infrared radiation
topic High Energy Physics - Theory
Quantum Gases
Statistical Mechanics
Mathematical Physics
url https://arxiv.org/abs/2406.00203