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Fast Rotating Neutron Stars: Oscillations and Instabilities [PDF]

open access: yesFrontiers in Astronomy and Space Sciences, 2021
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 ...
C. Krüger   +3 more
semanticscholar   +1 more source

Radial oscillations of dark matter admixed neutron stars [PDF]

open access: yesPhysical Review D, 2022
Within the relativistic mean-field model, we investigate the properties of dark matter (DM) admixed neutron stars, considering non-rotating objects made of isotropic matter.
Pinku Routaray   +5 more
semanticscholar   +1 more source

Oscillations of highly magnetized non-rotating neutron stars [PDF]

open access: yesCommunications Physics, 2022
Highly magnetized neutron stars are promising candidates to explain some of the most peculiar astronomical phenomena, for instance, fast radio bursts, gamma-ray bursts, and superluminous supernovae. Pulsations of these highly magnetized neutron stars are
Man Yin Leung   +3 more
semanticscholar   +1 more source

Radial Oscillations of Quark Stars Admixed with Dark Matter [PDF]

open access: yesUniverse, 2021
We investigated compact stars consisting of cold quark matter and fermionic dark matter treated as two admixed fluids. We computed the stellar structures and fundamental radial oscillation frequencies of different masses of the dark fermion in the cases ...
J. C. Jim'enez, E. Fraga
semanticscholar   +1 more source

g -mode oscillations in hybrid stars: A tale of two sounds [PDF]

open access: yes, 2021
We study the principal core g-mode oscillation in hybrid stars containing quark matter and find that they have an unusually large frequency range (≈ 200 600 Hz) compared to ordinary neutron stars or self-bound quark stars of the same mass.
P. Jaikumar   +3 more
semanticscholar   +1 more source

Boson stars and their radial oscillations [PDF]

open access: yes, 2021
We review the derivation of the pulsations equations for spherically symmetric boson stars and then make a thorough study of the radial oscillation frequencies for the fundamental and first excited modes.
B. Kain
semanticscholar   +1 more source

Radial oscillations and stability of compact stars in f(R, T) = R+ 2β T gravity [PDF]

open access: yesJournal of Cosmology and Astroparticle Physics, 2020
We examine the static structure configurations and radial stability of compact stars within the context of f(R, T) gravity, with R and T standing for the Ricci scalar and trace of the energy-momentum tensor, respectively.
Juan M.Z. Pretel   +3 more
semanticscholar   +1 more source

Asteroseismology: Radial oscillations of neutron stars with realistic equation of state [PDF]

open access: yesPhysical Review D, 2020
We study radial oscillations of non-rotating neutron stars (NSs) in four-dimensional General Relativity. The interior of the NS was modelled within a recently proposed multicomponent realistic equation of state (EoS) with the induced surface tension (IST)
V. Sagun, G. Panotopoulos, Ilídio Lopes
semanticscholar   +1 more source

Oscillations of Rapidly Rotating Stars [PDF]

open access: yesInternational Astronomical Union Colloquium, 2000
AbstractWe present numerical simulations of gravito-inertial waves propagating in radiative zones of rapidly rotating stars. A first model, using the Boussinesq approximation, allows us to study the oscillations of a quasi-incompressible stratified fluid embedded in a rapidly rotating sphere or spherical shell. In a second step, we investigate the case
Dintrans, Boris, Rieutord, Michel
openaire   +2 more sources

Reliable description of the radial oscillations of compact stars [PDF]

open access: yesPhysical Review D, 2020
We develop a numerical algorithm for the solution of the Sturm-Liouville differential equation governing the stationary radial oscillations of nonrotating compact stars.
F. D. Clemente   +2 more
semanticscholar   +1 more source

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