Temperatures of renormalizable quantum field theories in curved spacetime

被引:2
|
作者
Lynch, Morgan H. [1 ,2 ,3 ]
Afshordi, Niayesh [2 ,4 ]
机构
[1] Technion Israel Inst Technol, Dept Elect Engn, IL-32000 Haifa, Israel
[2] Perimeter Inst Theoret Phys, 31 Caroline St North, Waterloo, ON N2J 2Y5, Canada
[3] Univ Wisconsin, Leonard E Parker Ctr Gravitat Cosmol & Astrophys, POB 413, Milwaukee, WI 53201 USA
[4] Univ Waterloo, Dept Phys & Astron, Waterloo, ON N2L 3G1, Canada
关键词
Unruh effect; Hawking effect; Unruh-DeWitt detector; Hadamard form; TENSOR; STATES; TIME;
D O I
10.1088/1361-6382/aae792
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper we compute the temperature registered by an Unruh-DeWitt detector coupled to a Hadamard renormalizable quantum field in an arbitrary state, moving along an accelerated trajectory in a curved spacetime. For a massless and conformally invariant field, the generalized expression for the temperature is given by the quadratic sum of the 4-acceleration, Raychaudhuri scalar, and renormalized field polarization. We can further find a novel constraint on the renormalized quantum field polarization in relativistic systems that are in global thermal equilibrium.
引用
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页数:9
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