Non-local scalar field on deSitter and its infrared behaviour

被引:3
|
作者
Narain, Gaurav [1 ]
Kajuri, Nirmalya [2 ]
机构
[1] Beihang Univ, Dept Space Sci, Beijing 100191, Peoples R China
[2] Chennai Math Inst, Siruseri 603103, Kelambakkam, India
关键词
DeSitter field theory; Non-locality; Infrared physics; Scalar field; INFLATIONARY UNIVERSE SCENARIO; SITTER SPACE; FLATNESS; DYNAMICS; HORIZON; STATES;
D O I
10.1016/j.physletb.2019.02.030
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate free non-local massless and massive scalar field on deSitter (dS) space-time. We compute the propagator for the non-local scalar field for the corresponding theories on flat and deSitter spacetimes. It is seen that for the non-local theory, the massless limit of massive propagator is smooth for both flat and deSitter. Moreover, this limit matches exactly with the massless propagator of the non-local scalar field for both flat and deSitter space-time. The propagator is seen to respect dS invariance. Furthermore, investigations of the non-local Green's function on deSitter for large time-like separation shows that the propagator has no infrared divergences. The dangerous infrared log-divergent contributions which arise is local massless theories are absent in the corresponding non-local version. Lack of infrared divergences in the propagator hints at the strong role non-localities may play in the dS infrared physics. This study suggests thatnon-locality can cure IR issues in deSitter. (c) 2019 The Authors. Published by Elsevier B.V.
引用
收藏
页码:143 / 148
页数:6
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