Asymptotic structure of the Pauli-Fierz theory in four spacetime dimensions

被引:9
作者
Fuentealba, Oscar [1 ,2 ]
Henneaux, Marc [1 ,2 ,3 ]
Majumdar, Sucheta [1 ,2 ]
Matulich, Javier [1 ,2 ]
Troessaert, Cedric [1 ,2 ,4 ]
机构
[1] Univ Libre Bruxelles, ULB Campus Plaine CP231, B-1050 Brussels, Belgium
[2] Int Solvay Inst, ULB Campus Plaine CP231, B-1050 Brussels, Belgium
[3] Coll France, 11 Pl Marcelin Berthelot, F-75005 Paris, France
[4] Haute Ecole Robert Schuman, Rue Fontaine Mures 13b, B-6800 Libramont, Belgium
关键词
global symmetries; spacetime symmetries; classical theories of gravity; GENERAL-RELATIVITY; GRAVITATIONAL WAVES; SPATIAL INFINITY; SYMMETRIES; EQUATIONS; DYNAMICS; FIELDS; GAUGE;
D O I
10.1088/1361-6382/abbe6e
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The asymptotic structure of the Pauli-Fierz theory at spatial infinity is investigated in four spacetime dimensions. Boundary conditions on the massless spin-2 field that are invariant under an infinite-dimensional group of non-trivial 'improper' gauge symmetries are given. The compatibility of these boundary conditions with invariance of the theory under Lorentz boosts is a subtle issue which is investigated in depth and leads to the identification of the improper gauge symmetries with the pure BMS supertranslations. It is also shown how rigid Poincare transformations and improper gauge symmetries of the free Pauli-Fierz theory merge into the full BMS group as one switches on the gravitational coupling. Contrary to the massless spin-1 case, where invariance under boosts is implemented differently and where important differences between the free and the interacting cases have been exhibited recently, the free Pauli-Fierz theory and general relativity show very similar behaviors at spatial infinity.
引用
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页数:42
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