activity
20182026
most cited3d gravity in Bondi-Weyl gauge: charges, corners, and integrability

37 citations · 102 across the 8 of their papers we have counts for

collaborators
Showing hep-thShow all

12 papers · 1 filter

hep-th20243 cited

Field-dependent diffeomorphisms and the transformation of surface charges between gauges

Luca Ciambelli, Marc Geiller

When studying gauge theories in the presence of boundaries, local symmetry transformations are typically classified as gauge or physical depending on whether the associated charges…

hep-th2024

Celestial charges and the subleading structure of asymptotically-flat spacetimes

Marc Geiller

We study the subleading structure of asymptotically-flat spacetimes and its relationship to the loop algebra of higher spin charges. We do so using both the Bondi-Sa…

hep-th202430 cited

The partial Bondi gauge: Gauge fixings and asymptotic charges

Marc Geiller, Céline Zwikel

In the companion paper [SciPost Phys. 13, 108 (2022), arXiv:2205.11401 [hep-th]] we have studied the solution space at null infinity for gravity in the partial Bondi gauge. This pa…

hep-th2023

Minimal massive supergravity and new theories of massive gravity

Nihat Sadik Deger, Marc Geiller, Jan Rosseel +1

We present an action for minimal massive gravity (MMG) in three dimensions in terms of a dreibein and an independent spin connection. Furthermore, the construction provides an acti…

hep-th2023

Radiative Asymptotic Symmetries of 3D Einstein-Maxwell Theory

Jorrit Bosma, Marc Geiller, Sucheta Majumdar +1

We study the null asymptotic structure of Einstein-Maxwell theory in three-dimensional (3D) spacetimes. Although devoid of bulk gravitational degrees of freedom, the system admits…

hep-th202137 cited

3d gravity in Bondi-Weyl gauge: charges, corners, and integrability

Marc Geiller, Christophe Goeller, Céline Zwikel

We introduce a new gauge and solution space for three-dimensional gravity. As its name Bondi-Weyl suggests, it leads to non-trivial Weyl charges, and uses Bondi-like coordinates to…