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Hamiltonian Analysis of 4-dimensional Spacetime in Bondi-like Coordinates

Chao-Guang Huang, Shi-Bei Kong

TL;DR

The authors develop a Hamiltonian formulation of 4D gravity on a null Bondi-like foliation using a coframe/connection (Palatini) approach, and perform a full Dirac constraint analysis. By decomposing $SO(1,3)$ into $SO(1,1)\oplus SO(2)\oplus T^{\pm}(2)$, they obtain a null coframe with two null and two spacelike directions, derive 32 primary and 14 secondary constraints (46 total), and show that 6 are first class while 40 are second class, yielding 2 local gravitational degrees of freedom. The torsion-free conditions appear as consistency requirements, and the integrability conditions reduce to Ricci identities, with the equations of motion for the canonical variables fully displayed. The results provide a concrete Hamiltonian framework for gravity in Bondi-like coordinates, potentially connecting to BF-type formulations and pure-connection dynamics in constrained null geometries. Overall, the work advances canonical gravity on null surfaces and clarifies the constraint structure and physical content of 4D Bondi-like spacetimes.

Abstract

We discuss the Hamiltonian formulation of gravity in 4-dimensional spacetime under Bondi-like coordinates ${v, r, x^a, a=2, 3}$. In Bondi-like coordinates, the 3-dimensional hypersurface is a null hypersurface and the evolution direction is the advanced time $v$. The internal symmetry group $SO(1,3)$ of the 4-dimensional spacetime is decomposed into $SO(1,1)$, $SO(2)$, and $T^\pm(2)$, whose Lie algebra $so(1,3)$ is decomposed into $so(1,1)$, $so(2)$, $t^\pm(2)$ correspondingly. The $SO(1,1)$ symmetry is very obvious in this kind of decomposition, which is very useful in $so(1,1)$ BF theory. General relativity can be reformulated as the 4-dimensional coframe $(e^I_μ)$ and connection $(ω^{IJ}_μ)$ dynamics of gravity based on this kind of decomposition in the Bondi-like coordinate system. The coframe consists of 2 null 1-forms $e^-$, $e^+$ and 2 spacelike 1-forms $e^2$, $e^3$. The Palatini action is used. The Hamiltonian analysis is conducted by the Dirac's methods. The consistency analysis of constraints has been done completely. There are 2 scalar constraints and one 2-dimensional vector constraint. The torsion-free conditions are acquired from the consistency conditions of the primary constraints about $π^μ_{IJ}$. The consistency conditions of the primary constraints $π^0_{IJ}=0$ can be reformulated as Gauss constraints. The conditions of the Lagrange multipliers have been acquired. The Poisson brackets among the constraints have been calculated. There are 46 constraints including 6 first class constraints $π^0_{IJ}=0$ and 40 second class constraints. The local physical degrees of freedom is 2. The integrability conditions of Lagrange multipliers $n_0$, $l_0$, and $e^A_0$ are Ricci identities. The equations of motion of the canonical variables have also been shown.

Hamiltonian Analysis of 4-dimensional Spacetime in Bondi-like Coordinates

TL;DR

The authors develop a Hamiltonian formulation of 4D gravity on a null Bondi-like foliation using a coframe/connection (Palatini) approach, and perform a full Dirac constraint analysis. By decomposing into , they obtain a null coframe with two null and two spacelike directions, derive 32 primary and 14 secondary constraints (46 total), and show that 6 are first class while 40 are second class, yielding 2 local gravitational degrees of freedom. The torsion-free conditions appear as consistency requirements, and the integrability conditions reduce to Ricci identities, with the equations of motion for the canonical variables fully displayed. The results provide a concrete Hamiltonian framework for gravity in Bondi-like coordinates, potentially connecting to BF-type formulations and pure-connection dynamics in constrained null geometries. Overall, the work advances canonical gravity on null surfaces and clarifies the constraint structure and physical content of 4D Bondi-like spacetimes.

Abstract

We discuss the Hamiltonian formulation of gravity in 4-dimensional spacetime under Bondi-like coordinates . In Bondi-like coordinates, the 3-dimensional hypersurface is a null hypersurface and the evolution direction is the advanced time . The internal symmetry group of the 4-dimensional spacetime is decomposed into , , and , whose Lie algebra is decomposed into , , correspondingly. The symmetry is very obvious in this kind of decomposition, which is very useful in BF theory. General relativity can be reformulated as the 4-dimensional coframe and connection dynamics of gravity based on this kind of decomposition in the Bondi-like coordinate system. The coframe consists of 2 null 1-forms , and 2 spacelike 1-forms , . The Palatini action is used. The Hamiltonian analysis is conducted by the Dirac's methods. The consistency analysis of constraints has been done completely. There are 2 scalar constraints and one 2-dimensional vector constraint. The torsion-free conditions are acquired from the consistency conditions of the primary constraints about . The consistency conditions of the primary constraints can be reformulated as Gauss constraints. The conditions of the Lagrange multipliers have been acquired. The Poisson brackets among the constraints have been calculated. There are 46 constraints including 6 first class constraints and 40 second class constraints. The local physical degrees of freedom is 2. The integrability conditions of Lagrange multipliers , , and are Ricci identities. The equations of motion of the canonical variables have also been shown.

Paper Structure

This paper contains 26 sections, 80 equations.