General relativity;
Quantum gravity;
Three-dimensional gravity;
Teichmuller geometry;
Wilson loops;
COSMOLOGICAL CONSTANT;
D O I:
10.1007/s10714-010-0981-9
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We review the geometrical properties of vacuum spacetimes in (2+1)-gravity with vanishing cosmological constant. We explain how these spacetimes are characterised as quotients of their universal cover by holonomies. We explain how this description can be used to clarify the geometrical interpretation of the fundamental physical variables of the theory, holonomies and Wilson loops. In particular, we discuss the role of Wilson loop observables as the generators of the two fundamental transformations that change the geometry of (2+1)-spacetimes, grafting and earthquake. We explain how these variables can be determined from realistic measurements by an observer in the spacetime.
机构:
Penn State Univ, Ctr Gravitat Phys & Geometry, Dept Phys, University Pk, PA 16802 USAPenn State Univ, Ctr Gravitat Phys & Geometry, Dept Phys, University Pk, PA 16802 USA
Ashtekar, Abhay
Dreyer, Olaf
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机构:
Penn State Univ, Ctr Gravitat Phys & Geometry, Dept Phys, University Pk, PA 16802 USA
Perimeter Inst Theoret Phys, Waterloo, ON N2J 2W9, CanadaPenn State Univ, Ctr Gravitat Phys & Geometry, Dept Phys, University Pk, PA 16802 USA
Dreyer, Olaf
Wisniewski, Jacek
论文数: 0引用数: 0
h-index: 0
机构:
Penn State Univ, Ctr Gravitat Phys & Geometry, Dept Phys, University Pk, PA 16802 USAPenn State Univ, Ctr Gravitat Phys & Geometry, Dept Phys, University Pk, PA 16802 USA