Stress tensor fluctuations in de Sitter spacetime

被引:41
作者
Perez-Nadal, Guillem [1 ,2 ]
Roura, Albert [3 ]
Verdaguer, Enric [1 ,2 ]
机构
[1] Univ Barcelona, Dept Fis Fonamental, E-08028 Barcelona, Spain
[2] Univ Barcelona, Inst Ciencies Cosmos, E-08028 Barcelona, Spain
[3] Albert Einstein Inst, Max Planck Inst Gravitat Phys, D-14476 Golm, Germany
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2010年 / 05期
关键词
quantum field theory on curved space; inflation; cosmological perturbation theory; ENERGY-MOMENTUM TENSOR; SCALAR QUANTUM-FIELD; DESITTER SPACE; 2-POINT FUNCTIONS; BACK-REACTION; RENORMALIZATION; STABILITY; EQUATIONS; GRAVITY; STATES;
D O I
10.1088/1475-7516/2010/05/036
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The two-point function of the stress tensor operator of a quantum field in de Sitter spacetime is calculated for an arbitrary number of dimensions. We assume the field to be in the Bunch-Davies vacuum, and formulate our calculation in terms of de Sitter-invariant bitensors. Explicit results for free minimally coupled scalar fields with arbitrary mass are provided. We find long-range stress tensor correlations for sufficiently light fields (with mass m much smaller than the Hubble scale H), namely, the two-point function decays at large separations like an inverse power of the physical distance with an exponent proportional to m(2)/H-2. In contrast, we show that for the massless case it decays at large separations like the fourth power of the physical distance. There is thus a discontinuity in the massless limit. As a byproduct of our work, we present a novel and simple geometric interpretation of de Sitter-invariant bitensors for pairs of points which cannot be connected by geodesics
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页数:34
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