The Weyl BMS group and Einstein’s equations

Journal of High Energy Physics

Roberto Oliveri¹  Simone Speziale²  Laurent Freidel³  Daniele Pranzetti⁴ 

[1] CEICO, Institute of Physics of the Czech Academy of Sciences, Na Slovance 2, 182 21, Praha 8, Czech Republic;CPT-UMR 7332, CNRS, 13288, Marseille, France;Perimeter Institute for Theoretical Physics, 31 Caroline Street North, N2L 2Y5, Waterloo, Ontario, Canada;Perimeter Institute for Theoretical Physics, 31 Caroline Street North, N2L 2Y5, Waterloo, Ontario, Canada;Università degli Studi di Udine, via Palladio 8, I-33100, Udine, Italy;

关键词: Models of Quantum Gravity;    Space-Time Symmetries;    Classical Theories of Gravity;   

DOI  :  10.1007/JHEP07(2021)170

来源: Springer

【 摘 要 】

We propose an extension of the BMS group, which we refer to as Weyl BMS or BMSW for short, that includes super-translations, local Weyl rescalings and arbitrary diffeomorphisms of the 2d sphere metric. After generalizing the Barnich-Troessaert bracket, we show that the Noether charges of the BMSW group provide a centerless representation of the BMSW Lie algebra at every cross section of null infinity. This result is tantamount to proving that the flux-balance laws for the Noether charges imply the validity of the asymptotic Einstein’s equations at null infinity. The extension requires a holographic renormalization procedure, which we construct without any dependence on background fields. The renormalized phase space of null infinity reveals new pairs of conjugate variables. Finally, we show that BMSW group elements label the gravitational vacua.

【 授权许可】

CC BY