The Internal Spin Angular Momentum of an Asymptotically Flat Spacetime
Andrew Randono, David Sloan

TL;DR
This paper explores how internal spin of a spinor field is represented in the gravitational field at infinity in asymptotically flat spacetimes, leading to a spin-enlarged Poincaré symmetry and new conserved charges.
Contribution
It introduces a modified asymptotic symmetry group incorporating internal spin, and constructs boundary integrals for total angular momentum including spin contributions.
Findings
Internal spin is encoded in the asymptotic tetrad.
A new conserved charge related to gauge transformations is identified.
The phase space becomes finite with appropriate boundary conditions.
Abstract
In this paper we investigate the manner in which the internal spin angular momentum of a spinor field is encoded in the gravitational field at asymptotic infinity. The inclusion of internal spin requires us to re-analyze our notion of asymptotic flatness. In particular, the Poincar\'{e} symmetry at asymptotic infinity must replaced by a spin-enlarged Poincar\'{e} symmetry. Likewise, the generators of the asymptotic symmetry group must be supplemented to account for the internal spin. In the Hamiltonian framework of first order Einstein-Cartan gravity, the extra generator comes from the boundary term of the Gauss constraint in the asymptotically flat context. With the additional term, we establish the relations among the Noether charges of a Dirac field, the Komar integral, and the asymptotic ADM-like geometric integral. We show that by imposing mild restraints on the generating…
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