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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Main Authors: Christian J. Krüger, Kostas D. Kokkotas, Praveen Manoharan, Sebastian H. Völkel
Format: Article
Language:English
Published: Frontiers Media S.A. 2021-09-01
Series:Frontiers in Astronomy and Space Sciences
Subjects:
Online Access:https://www.frontiersin.org/articles/10.3389/fspas.2021.736918/full
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spelling 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
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AT praveenmanoharan fastrotatingneutronstarsoscillationsandinstabilities
AT sebastianhvolkel fastrotatingneutronstarsoscillationsandinstabilities
AT sebastianhvolkel fastrotatingneutronstarsoscillationsandinstabilities
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