Geometrical quantum time in the U(1)3 model of Euclidean quantum gravity

被引:0
作者
Bakhoda, Sepideh [1 ]
Ma, Yongge [1 ]
机构
[1] Beijing Normal Univ, Sch Phys & Astron, Key Lab Multiscale Spin Phys, Minist Educ, Beijing 100875, Peoples R China
基金
中国国家自然科学基金;
关键词
loop quantum gravity; Hamiltonian constraint; time problem; SPIN DYNAMICS QSD; COMPLETE OBSERVABLES; ASHTEKAR VARIABLES; SPACE; QUANTIZATION; REAL;
D O I
10.1088/1572-9494/ad972b
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Loop quantum gravity faces challenges in constructing a well-defined Hamiltonian constraint and understanding the quantum notion of time. In this paper these issues are studied by quantizing the U(1)3 model, a simplified system exhibiting features similar to general relativity. By isolating a holonomy component within the Hamiltonian constraint, a discrete relative time evolution equation for quantum states is obtained. Then, a Shr & ouml;dinger-like equation is derived in the continuum limit. Thus, the physical states solving this Shr & ouml;dinger-like equation can be written out. The emergence of the time parameter and its corresponding quantum operator are analyzed. It indicates the notion of a geometrical quantum time for quantum gravity.
引用
收藏
页数:14
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