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Andreas Reisenegger

Researcher at Pontifical Catholic University of Chile

Publications -  77
Citations -  3028

Andreas Reisenegger is an academic researcher from Pontifical Catholic University of Chile. The author has contributed to research in topics: Neutron star & Pulsar. The author has an hindex of 26, co-authored 76 publications receiving 2551 citations. Previous affiliations of Andreas Reisenegger include Metropolitan University & NASA Headquarters.

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Magnetic field decay in isolated neutron stars

TL;DR: In this article, the authors investigated three mechanisms that promote the loss of magnetic flux from an isolated neutron star, including buoyant rise and dragging by superfluid neutron vectors, and found that the drift speed is proportional to the second power of the magnetic field strength.
MonographDOI

Science with the Cherenkov Telescope Array

B. S. Acharya, +580 more
TL;DR: The Cherenkov Telescope Array (CTA) as mentioned in this paper is the major global observatory for very high energy gamma-ray astronomy over the next decade and beyond, covering a huge range in photon energy from 20 GeV to 300 TeV.
Journal ArticleDOI

A new class of g-modes in neutron stars

TL;DR: In this article, the lowest-order, quadrupolar, g-modes for cold, Newtonian, neutron star models with M/M_☉ = 0.581 and M/m_⌉ = 1.405 were derived.
Journal ArticleDOI

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.
Journal ArticleDOI

Excitation of neutron star normal modes during binary inspiral

TL;DR: In this article, a compact binary inspirals due to the emission of gravitational waves, its orbital period decreases continuously down to approximately 1 ms, its value at coalescence during the last part of the inspiral, when the two stars are close together, and their tidal interactions become strong.