Conservation of
asymptotic charges
from \(\mathscr I^-\) to \(\mathscr I^+\)
APS 2018, Columbus, OH
Charges and fluxes on \(\mathscr I\)
\((M, g)\) conformal completion of \((\hat M, \hat g)\); \(g_{ab} = \Omega^2 \hat g_{ab}\)
For any function \(\alpha(\mathbb S^2)\) on \(\mathscr I^-\) or \(\mathscr I^+\)
- charges: \(\mathcal Q [\alpha, S] = \int\limits_S \alpha F_{ab} l^a n^b \)
- conservation law: \(\mathcal Q [\alpha, S_2] - \mathcal Q [\alpha, S_1] = \mathcal F[\alpha]\)
full symmetry group \(\alpha_- \otimes \alpha_+\)
Global conservation (?)
- \(\lim\limits_{\to i^0}\alpha_-(\mathbb S^2) = \lim\limits_{\to i^0}\alpha_+( - \mathbb S^2) \)
- total \(\mathcal F[\alpha_-] = \) total \(\mathcal F[\alpha_+]\)
Constrains allowed classical scattering
Quantum S-matrix, information loss (?)
Global conservation (known results)
(not a complete list)- Bondi \(4\)-momentum in full GR. Ashtekar, Magnon-Ashtekar [1979]
- Angular momentum in stationary spacetimes full GR. Ashtekar, Streubel [1979]
- all charges on Minkowski background: EM Campiglia, Eyheralde [2017] and linearised gravity Troessaert [2017]
all charges on general spacetimes?
\(i^0\) is a funny place!
at \(i^0\):
- \(\nabla_a\Omega = 0\); \(\nabla_a \nabla_b\Omega = 2 g_{ab}\) (cannot use Bondi frame)
- if \(charge \neq 0\): \(\Omega F_{ab}\) is direction-dependent
- if \(mass \neq 0\): \(\partial_a g_{bc}\) is direction-dependent
Very low differential structure
Blowup \(i^0\) — space of directions: \(\mathscr C\)
\(\mathscr C\): cylinder of directions in \(Ti^0\)
\(\mathscr N^\pm\): spheres of null directions
- direction-dependent “electric field”: \(\mathbf E_a\)
- Maxwell equations: equations for \(\mathbf E_a\) on \(\mathscr C\)
- symmetries: \(\alpha(\mathscr C)\)
- charges: \(\mathcal Q_0[\alpha, S] = \int\limits_S \alpha \mathbf E_a \mathbf u^a \)
Null regularity & matching at \(\mathscr N^\pm\)
Assume regularity of fields and symmetries at \(\mathscr N^\pm\)
- Limits from \(\mathscr I^{\pm}\) \(=\) limits to \(\mathscr N^\pm\) on \(\mathscr C\)
- \(\implies\) charges from \(\mathscr I^\pm\) \(=\) charges on \(\mathscr C\) at \(\mathscr N^\pm\)
regular symmetry group \(\alpha(\mathscr C)\): \(\alpha_\pm(\mathbb S^2) = \alpha(\mathscr C)\vert_{\mathscr N^\pm}\)
Totally fluxless symmetries on \(\mathscr C\) and conservation
- Maxwell equations \(\implies\) (rescaled) \(\mathbf E_a \mathbf u^a\) evolves antipodally from \(\mathscr N^-\) to \(\mathscr N^+\)
- demand total flux \(\mathcal F[\alpha; \mathscr C] = 0 \iff \alpha\vert_{\mathscr N^-} \equiv \alpha\vert_{\mathscr N^+}\) antipodally
Totally fluxless symmetries on \(\mathscr C\) match antipodally i.e. \(\lim\limits_{\to i^0}\alpha_-(\mathbb S^2) = \lim\limits_{\to i^0}\alpha_+(- \mathbb S^2) \) and \(\mathcal F[\alpha_-] = \mathcal F[\alpha_+]\)
Summary
EM on general asymp. flat spacetimes
- \(\lim\limits_{\to i^0}\alpha_-(\mathbb S^2) = \lim\limits_{\to i^0}\alpha_+(- \mathbb S^2) \)
- \(\mathcal F[\alpha_-] = \mathcal F[{\alpha_+}]\)
uses
- Blowup of \(i^0\) to cylinder \(\mathscr C\)
- regularity of fields and symmetries in null directions
- Maxwell equations; totally fluxless symmetries