Fast Rotating Neutron Stars: Oscillations and Instabilities
In this review article, we present the main results from our most recent research concerning the oscillations of fast rotating neutron stars. We derive a set of time evolution equations for the investigation of non-axisymmetric oscillations of rapidly rotating compact objects in full general relativ...
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2021-09-01
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doaj-ab5d988d74624686a8646124cb0bb24a2021-09-28T04:29:45ZengFrontiers Media S.A.Frontiers in Astronomy and Space Sciences2296-987X2021-09-01810.3389/fspas.2021.736918736918Fast Rotating Neutron Stars: Oscillations and InstabilitiesChristian J. Krüger0Kostas D. Kokkotas1Praveen Manoharan2Sebastian H. Völkel3Sebastian H. Völkel4Theoretical Astrophysics, IAAT, University of Tübingen, Tübingen, GermanyTheoretical Astrophysics, IAAT, University of Tübingen, Tübingen, GermanyTheoretical Astrophysics, IAAT, University of Tübingen, Tübingen, GermanySISSA, INFN Sezione di Trieste, Trieste, ItalyIFPU, Trieste, ItalyIn this review article, we present the main results from our most recent research concerning the oscillations of fast rotating neutron stars. We derive a set of time evolution equations for the investigation of non-axisymmetric oscillations of rapidly rotating compact objects in full general relativity, taking into account the contribution of a dynamic spacetime. Using our code, which features high accuracy at comparably low computational expense, we are able to extract the frequencies of non-axisymmetric modes of compact objects with rotation rates up to the Kepler limit. We propose various universal relations combining bulk properties of isolated neutron stars as well as of binary systems before and after merger; these relations are independent of the true equation of state and may serve as a valuable tool for gravitational wave asteroseismology. We also present an introductory example using a Bayesian analysis.https://www.frontiersin.org/articles/10.3389/fspas.2021.736918/fullneutron starequation of statestarsrotationstarsBayesiah analysis |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Christian J. Krüger Kostas D. Kokkotas Praveen Manoharan Sebastian H. Völkel Sebastian H. Völkel |
spellingShingle |
Christian J. Krüger Kostas D. Kokkotas Praveen Manoharan Sebastian H. Völkel Sebastian H. Völkel Fast Rotating Neutron Stars: Oscillations and Instabilities Frontiers in Astronomy and Space Sciences neutron star equation of state stars rotation stars Bayesiah analysis |
author_facet |
Christian J. Krüger Kostas D. Kokkotas Praveen Manoharan Sebastian H. Völkel Sebastian H. Völkel |
author_sort |
Christian J. Krüger |
title |
Fast Rotating Neutron Stars: Oscillations and Instabilities |
title_short |
Fast Rotating Neutron Stars: Oscillations and Instabilities |
title_full |
Fast Rotating Neutron Stars: Oscillations and Instabilities |
title_fullStr |
Fast Rotating Neutron Stars: Oscillations and Instabilities |
title_full_unstemmed |
Fast Rotating Neutron Stars: Oscillations and Instabilities |
title_sort |
fast rotating neutron stars: oscillations and instabilities |
publisher |
Frontiers Media S.A. |
series |
Frontiers in Astronomy and Space Sciences |
issn |
2296-987X |
publishDate |
2021-09-01 |
description |
In this review article, we present the main results from our most recent research concerning the oscillations of fast rotating neutron stars. We derive a set of time evolution equations for the investigation of non-axisymmetric oscillations of rapidly rotating compact objects in full general relativity, taking into account the contribution of a dynamic spacetime. Using our code, which features high accuracy at comparably low computational expense, we are able to extract the frequencies of non-axisymmetric modes of compact objects with rotation rates up to the Kepler limit. We propose various universal relations combining bulk properties of isolated neutron stars as well as of binary systems before and after merger; these relations are independent of the true equation of state and may serve as a valuable tool for gravitational wave asteroseismology. We also present an introductory example using a Bayesian analysis. |
topic |
neutron star equation of state stars rotation stars Bayesiah analysis |
url |
https://www.frontiersin.org/articles/10.3389/fspas.2021.736918/full |
work_keys_str_mv |
AT christianjkruger fastrotatingneutronstarsoscillationsandinstabilities AT kostasdkokkotas fastrotatingneutronstarsoscillationsandinstabilities AT praveenmanoharan fastrotatingneutronstarsoscillationsandinstabilities AT sebastianhvolkel fastrotatingneutronstarsoscillationsandinstabilities AT sebastianhvolkel fastrotatingneutronstarsoscillationsandinstabilities |
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