θ parameter in loop quantum gravity: Effects on quantum geometry and black hole entropy

被引:7
|
作者
Rezende, Danilo Jimenez [1 ]
Perez, Alejandro [1 ]
机构
[1] CNRS Marseille Luminy, Ctr Phys Theor, F-13288 Marseille, France
来源
PHYSICAL REVIEW D | 2008年 / 78卷 / 08期
关键词
D O I
10.1103/PhysRevD.78.084025
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The precise analog of the theta-quantization ambiguity of Yang-Mills theory exists for the real SU(2) connection formulation of general relativity. As in the former case theta labels representations of large gauge transformations, which are superselection sectors in loop quantum gravity. We show that unless theta=0, the (kinematical) geometric operators such as area and volume are not well defined on spin network states. More precisely the intersection of their domain with the dense set Cyl in the kinematical Hilbert space H of loop quantum gravity is empty. The absence of a well-defined notion of area operator acting on spin network states seems at first in conflict with the expected finite black hole entropy. However, we show that the black hole (isolated) horizon area-which in contrast to kinematical area is a (Dirac) physical observable-is indeed well defined, and quantized so that the black hole entropy is proportional to the area. The effect of theta is negligible in the semiclassical limit where proportionality to area holds.
引用
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页数:7
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