Total yield of electron-positron pairs produced from vacuum in strong electromagnetic fields: Validity of the locally constant field approximation

Publikation: Beitrag in FachzeitschriftForschungsartikelBeigetragenBegutachtung

Beitragende

  • D. G. Sevostyanov - , St. Petersburg State University (Autor:in)
  • I. A. Aleksandrov - , St. Petersburg State University (Autor:in)
  • Günter Plunien - , Professur für Theoretische Quantenoptik (Autor:in)
  • V.M. Shabaev - , St. Petersburg State University (Autor:in)

Abstract

The widely used locally constant field approximation (LCFA) can be utilized in order to derive a simple closed-form expression for the total number of particles produced in the presence of a strong electromagnetic field of a general spatiotemporal configuration. A usual justification for this approximate approach is the requirement that the external field vary slowly in space and time. In this investigation, we examine the validity of the LCFA by comparing its predictions to the results obtained by means of exact nonperturbative numerical techniques. To benchmark the LCFA in the regime of small field amplitudes and low frequencies, we employ a semiclassical approach. As a reference, we consider a standing electromagnetic wave oscillating both in time and space as well as two spatially uniform field configurations: Sauter pulse and oscillating electric field. Performing a thorough numerical analysis, we identify the domain of the field parameters where the approximation is well justified. In particular, it is demonstrated that the Keldysh parameter itself is not a relevant quantity governing the accuracy of the LCFA. It is also found that for field amplitudes close to the Schwinger critical value, the LCFA may overestimate the particle yield. We discuss how this effect is related to the Pauli exclusion principle and quantum interference.

Details

OriginalspracheEnglisch
Aufsatznummer076014
Seiten (von - bis)1
Seitenumfang15
FachzeitschriftPhysical Review: D, covering particles, fields, gravitation, and cosmology
Jahrgang2021
Ausgabenummer104
PublikationsstatusVeröffentlicht - 14 Okt. 2021
Peer-Review-StatusJa

Externe IDs

Scopus 85117386930

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Bibliotheksschlagworte