Chiral perturbation theory for GR

被引:0
作者
Kirill Krasnov
Yuri Shtanov
机构
[1] University of Nottingham,School of Mathematical Sciences
[2] Bogolyubov Institute for Theoretical Physics,undefined
[3] Astronomical Observatory,undefined
[4] Taras Shevchenko National University of Kiev,undefined
来源
Journal of High Energy Physics | / 2020卷
关键词
Classical Theories of Gravity; Scattering Amplitudes;
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摘要
We describe a new perturbation theory for General Relativity, with the chiral first-order Einstein-Cartan action as the starting point. Our main result is a new gauge-fixing procedure that eliminates the connection-to-connection propagator. All other known first-order formalisms have this propagator non-zero, which significantly increases the combinatorial complexity of any perturbative calculation. In contrast, in the absence of the connection-to-connection propagator, our formalism leads to an effective description in which only the metric (or tetrad) propagates, there are only cubic and quartic vertices, but some vertex legs are special in that they cannot be connected by the propagator. The new formalism is the gravity analog of the well-known and powerful chiral description of Yang-Mills theory.
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共 17 条
[1]  
Cheung C(2017) = 8 JHEP 09 002-undefined
[2]  
Remmen GN(2017) = 2 Class. Quant. Grav. 34 095001-undefined
[3]  
Krasnov K(2015) = 4 Phys. Rev. D 92 065012-undefined
[4]  
Cofano M(1993)undefined Phys. Rev. D 47 2504-undefined
[5]  
Fu C-H(2015)undefined JHEP 03 118-undefined
[6]  
Krasnov K(2013)undefined JHEP 11 040-undefined
[7]  
Siegel W(2015)undefined JHEP 03 120-undefined
[8]  
Delfino G(1986)undefined Nucl. Phys. B 266 709-undefined
[9]  
Krasnov K(undefined)undefined undefined undefined undefined-undefined
[10]  
Scarinci C(undefined)undefined undefined undefined undefined-undefined