The University of Southampton
University of Southampton Institutional Repository

The traditional approximation in general relativity

The traditional approximation in general relativity
The traditional approximation in general relativity
We discuss the generalization of the so-called traditional approximation, well known in geophysics, to general relativity. We show that the approximation is applicable for rotating relativistic stars, provided that one focuses on relatively thin radial shells. This means that the framework can be used to study waves in neutron star oceans. We demonstrate that, once the effects of the relativistic frame-dragging are accounted for, the angular problem reduces to Laplace's tidal equation. We derive the dispersion relation for various classes of waves in a neutron star ocean and show that the combined effects of the frame-dragging and the gravitational redshift typically lower the frequency of a mode by about 20 per cent.
1365-2966
1349-1358
Maniopoulou, Asimina
ada812b5-349a-4070-813d-6c535fa86c09
Andersson, Nils
2dd6d1ee-cefd-478a-b1ac-e6feedafe304
Maniopoulou, Asimina
ada812b5-349a-4070-813d-6c535fa86c09
Andersson, Nils
2dd6d1ee-cefd-478a-b1ac-e6feedafe304

Maniopoulou, Asimina and Andersson, Nils (2004) The traditional approximation in general relativity. Monthly Notices of the Royal Astronomical Society, 351, 1349-1358. (doi:10.1111/j.1365-2966.2004.07872.x).

Record type: Article

Abstract

We discuss the generalization of the so-called traditional approximation, well known in geophysics, to general relativity. We show that the approximation is applicable for rotating relativistic stars, provided that one focuses on relatively thin radial shells. This means that the framework can be used to study waves in neutron star oceans. We demonstrate that, once the effects of the relativistic frame-dragging are accounted for, the angular problem reduces to Laplace's tidal equation. We derive the dispersion relation for various classes of waves in a neutron star ocean and show that the combined effects of the frame-dragging and the gravitational redshift typically lower the frequency of a mode by about 20 per cent.

This record has no associated files available for download.

More information

Published date: 2004

Identifiers

Local EPrints ID: 29460
URI: http://eprints.soton.ac.uk/id/eprint/29460
ISSN: 1365-2966
PURE UUID: 8777f2be-bb04-4362-a209-fb40f50fde63
ORCID for Nils Andersson: ORCID iD orcid.org/0000-0001-8550-3843

Catalogue record

Date deposited: 11 May 2006
Last modified: 16 Mar 2024 03:02

Export record

Altmetrics

Contributors

Author: Asimina Maniopoulou
Author: Nils Andersson ORCID iD

Download statistics

Downloads from ePrints over the past year. Other digital versions may also be available to download e.g. from the publisher's website.

View more statistics

Atom RSS 1.0 RSS 2.0

Contact ePrints Soton: eprints@soton.ac.uk

ePrints Soton supports OAI 2.0 with a base URL of http://eprints.soton.ac.uk/cgi/oai2

This repository has been built using EPrints software, developed at the University of Southampton, but available to everyone to use.

We use cookies to ensure that we give you the best experience on our website. If you continue without changing your settings, we will assume that you are happy to receive cookies on the University of Southampton website.

×