Conférence
Notice
Langue :
Anglais
Crédits
Fanny Bastien (Réalisation), Thomas Backdahl (Intervention)
Conditions d'utilisation
CC BY-NC-ND 4.0
DOI : 10.60527/mfmx-5312
Citer cette ressource :
Thomas Backdahl. I_Fourier. (2014, 4 juillet). Thomas Backdahl - Symmetry operators, conserved currents and energy momentum tensors , in 2014. [Vidéo]. Canal-U. https://doi.org/10.60527/mfmx-5312. (Consultée le 17 mai 2024)

Thomas Backdahl - Symmetry operators, conserved currents and energy momentum tensors

Réalisation : 4 juillet 2014 - Mise en ligne : 9 juin 2016
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Descriptif

Conserved quantities, for example energy and momentum, play a fundamental role in the analysis of dynamics of particles and fields. For field equations, one manifestation of conserved quantities in a broad sense is the existence of symmetry operators, i.e. linear differential operators which take solutions to solutions. A well known example of a symmetry operator for the scalar wave equation is provided by the Lie derivative along a Killing vector field. It is important to note that other kinds of objects can generate symmetry operators. For waves in the Kerr spacetime there is a symmetry operator associated with Carter's constant. This symmetry, which is "hidden" in the sense that it arises from a Killing spinor, satisfying a generalization of the Killing vector equation, rather than a Killing vector, was an essential ingredient in a proof of decay of scalar waves on the Kerr background by Andersson and Blue. In this talk we will consider what conditions on a spacetime are necessary for existence of symmetry operators for the conformal wave equation, the Dirac Weyl equation, and the Maxwell equation, i.e. for massless test fields of spins 0, 1/2 and 1. We will investigate how the conditions for the symmetry operators for the different field equations are related, and how they are related to existence of conserved currents. Furthermore, these tools lead to the construction of a new energy momentum tensor for a Maxwell field on a Kerr background. This will provide a powerful tool for the study of decay of Maxwell fields on the Kerr spacetime.

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