Schwinger effect and backreaction in de Sitter spacetime

被引:24
|
作者
Stahl, Clement [1 ,2 ,3 ,4 ,5 ]
Xue, She-Sheng [1 ,2 ]
机构
[1] ICRANet, Piazzale Republ 10, I-65122 Pescara, Italy
[2] Univ Roma La Sapienza, Dipartimento Fis, Piazzale Aldo Moro 5, I-00185 Rome, Italy
[3] Univ Nice Sophia Antipolis, 28 Ave Valrose, F-06103 Nice 2, France
[4] KTH Royal Inst Technol, NORDITA, Roslagstullsbacken 23, SE-10691 Stockholm, Sweden
[5] Stockholm Univ, Roslagstullsbacken 23, SE-10691 Stockholm, Sweden
关键词
MAGNETIC-FIELDS; PAIR PRODUCTION;
D O I
10.1016/j.physletb.2016.07.011
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider the particle-antiparticle pairs produced by both a strong electric field and de Sitter curvature. We investigate in 1 + 1 D the backreaction of the pairs on the electromagnetic field. To do so we describe the canonical quantization of an electromagnetic field in de Sitter space and add in the Einstein-Maxwell equation the fermionic current induced by the pairs. After solving this equation, we find that the electric field gets either damped or unaffected depending on the value of the pair mass and the gauge coupling. No enhancement of the electromagnetic field to support a magnetogenesis scenario is found. The physical picture is that the Schwinger pairs locally created screen the production and amplification of the electromagnetic field. However, if one considers light bosons created by the Schwinger mechanism, we report a solution to the Einstein-Maxwell equation with an enhancement of the electromagnetic field. This solution could be a new path to primordial magnetogenesis. (C) 2016 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY license.
引用
收藏
页码:288 / 292
页数:5
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