T
Taner Akgün
Researcher at Pontifical Catholic University of Chile
Publications - 4
Citations - 234
Taner Akgün is an academic researcher from Pontifical Catholic University of Chile. The author has contributed to research in topics: Magnetic field & Magnetic energy. The author has an hindex of 3, co-authored 4 publications receiving 201 citations. Previous affiliations of Taner Akgün include Barcelona Supercomputing Center.
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Stability of magnetic fields in non-barotropic stars: an analytic treatment
TL;DR: In this paper, the authors provide an explicit expression for a plausible equilibrium structure of an axially symmetric magnetic field with both poloidal and toroidal components of adjustable strengths, in a non-barotropic static fluid star, and study its stability using the energy principle.
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Gravitational wave emission from a magnetically deformed non-barotropic neutron star
TL;DR: In this paper, the mass quadrupole moment was calculated by perturbing a zeroth-order hydrostatic equilibrium by an axisymmetric magnetic field with a linked poloidal-toroidal structure.
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Revisiting the Flowers-Ruderman instability of magnetic stars
TL;DR: In this article, the authors considered the effect of adding a toroidal field by studying the potential energy perturbation when the rotation is not done along a sharp cut, but with a continuous displacement field that switches the direction of rotation across a region of small but finite width.
Journal ArticleDOI
Revisiting the Flowers-Ruderman instability of magnetic stars
TL;DR: In this article, the authors considered the effect of adding a toroidal field by studying the potential energy perturbation when the rotation is not done along a sharp cut, but with a continuous displacement field that switches the direction of rotation across a region of small but finite width.