Abstract

We discuss the Hamiltonian dynamics of general relativity with real connection variables on a null foliation, and use the Newman-Penrose formalism to shed light on the geometric meaning of the various constraints. We identify the equivalent of Sachs’ constraint-free initial data as projections of connection components related to null rotations, i.e. the translational part of the ISO(2) group stabilising the internal null direction soldered to the hypersurface. A pair of second-class constraints reduces these connection components to the shear of a null geodesic congruence, thus establishing equivalence with the second-order formalism, which we show in details at the level of symplectic potentials. A special feature of the first-order formulation is that Sachs’ propagating equations for the shear, away from the initial hypersurface, are turned into tertiary constraints; their role is to preserve the relation between connection and shear under retarded time evolution. The conversion of wave-like propagating equations into constraints is possible thanks to an algebraic Bianchi identity; the same one that allows one to describe the radiative data at future null infinity in terms of a shear of a (non-geodesic) asymptotic null vector field in the physical spacetime. Finally, we compute the modification to the spin coefficients and the null congruence in the presence of torsion.

Highlights

  • Null foliations play an important role in general relativity

  • We discuss the Hamiltonian dynamics of general relativity with real connection variables on a null foliation, and use the Newman-Penrose formalism to shed light on the geometric meaning of the various constraints

  • We identify the equivalent of Sachs’ constraint-free initial data as projections of connection components related to null rotations, i.e. the translational part of the ISO(2) group stabilising the internal null direction soldered to the hypersurface

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Summary

Introduction

Null foliations play an important role in general relativity Among their special features, they admit a gauge-fixing for which the Einstein’s equations can be integrated hierarchically, and constraint-free initial data identified, as shown by Sachs [1]; and provide a framework for the description of gravitational radiation from isolated systems and of conserved charges, starting from the seminal work of Sachs, of Bondi, van der Burg and Metzner ( BMS), Newman and Penrose (NP), Geroch and Ashtekar [2,3,4,5,6,7,8,9,10,11,12] (see [13,14,15] and reference therein).

Sachs’ free data and metric Hamiltonian structure
Bondi gauge and Sachs constraint-free initial data
Hamiltonian structure
Tetrad and foliation
Constraint structure
Newman-Penrose tetrad
The affine null congruence
Torsionlessness of the affine null congruence
Tertiary constraints as the propagating equations
E mambΥab
Bondi gauge
Equivalence of symplectic potentials
Conclusions
A Spin coefficients
C Tetrad transformations and gauge fixings
EA1 0 EAM
Adapting a NP tetrad
The Bondi gauge and Newman-Unti tetrad
E Mappings to the χ-tetrad
Areal r and Sachs’ metric coefficients
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