<div class="csl-bib-body">
<div class="csl-entry">Leuthner, M. (2021). <i>Hamiltonian surface charges in 3d Einstein gravity</i> [Diploma Thesis, Technische Universität Wien]. reposiTUm. https://doi.org/10.34726/hss.2021.95104</div>
</div>
-
dc.identifier.uri
https://doi.org/10.34726/hss.2021.95104
-
dc.identifier.uri
http://hdl.handle.net/20.500.12708/18945
-
dc.description.abstract
Hamiltonian surface charges are introduced in terms of the covariant phase space formalism, then they are computed for Einstein gravity in three spacetime dimensions. In general, this gives a different result depending on whether one uses the second-order (metric) or first-order (Cartan or Chern-Simons) formulation. This is studied explicitly for three different spacetime examples, only in one of which the difference between formalisms becomes apparent.
en
dc.language
English
-
dc.language.iso
en
-
dc.rights.uri
http://rightsstatements.org/vocab/InC/1.0/
-
dc.subject
three-dimensional gravity
en
dc.subject
Chern-Simons
en
dc.subject
covariant phase space
en
dc.subject
asymptotic symmetries
en
dc.subject
surface charges
en
dc.title
Hamiltonian surface charges in 3d Einstein gravity