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Remark on the quasilocal calculation of tidal heating: Energy transfer through the quasilocal surface

  • In this paper, using the quasilocal formalism of Brown and York, the flow of energy through a closed surface containing a gravitating physical system is calculated in a way that augments earlier results on the subject by Booth and Creighton. To this end, by performing a variation of the total gravitational Hamiltonian (bulk plus boundary part), it is shown that associated tidal heating and deformation effects generally are larger than expected. This is because the aforementioned variation leads to previously unrecognized correction terms, including a bulk-to-boundary inflow term that does not appear in the original calculation of the time derivative of the Brown-York energy and leads to corrective extensions of Einstein’s quadrupole formula in the large sphere limit.

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Metadaten
Author:Albert Huber
Parent Title (English):American Physical Society - Physical Review D
Document Type:Article
Language:English
Completed Date:2022/01/04
Responsibility for metadata:Fachhochschule Technikum Wien
Release Date:2022/02/02
GND Keyword:cosmology; fields; gravitation
Volume:105
Issue:2
Publish on Website:1
Open Access:1
Reviewed:1
Department:Department Angewandte Mathematik und Physik
Research Focus:Sonstiges
Projects:Import
Studienjahr:2021/2022