Andreas Reisenegger

Pontificia Universidad Católica de Chile — Chile

Physics and Astronomy · Physical Sciences

33h-index3.5kcitations172works2.42yr avg
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Research Topics

Pulsars and Gravitational Waves Research(80), Astrophysics and Cosmic Phenomena(36), High-pressure geophysics and materials(31), Stellar, planetary, and galactic studies(26), Gamma-ray bursts and supernovae(26)

Publications139 total

Three-dimensional numerical simulations of neutron star cores in the two-fluid MHD approximation: simple configurations
arXiv (Cornell University)·2025Open Access
Neutron star heating vs. HST observations
arXiv (Cornell University)·2025Open Access
Magnetothermal evolution of neutron star cores in the weak-coupling regime: Implications of ambipolar diffusion for the quiescent x-ray luminosity of magnetars
Physical review. D/Physical review. D.·2025
Validating and improving two-fluid simulations of the magnetic field evolution in neutron star cores
Astronomy and Astrophysics·2025· 1 citedOpen Access
Magnetothermal evolution of neutron star cores in the `weak-coupling' regime: implications of ambipolar diffusion for the quiescent X-ray luminosity of magnetars
arXiv (Cornell University)·2025Open Access
HESS J1745−290 spectrum explained by a transition in the diffusion regime of PeV cosmic rays in the Sgr A* accretion flow
Astronomy and Astrophysics·2024· 3 citedOpen Access
HESS J1745$-$290 spectrum explained by a transition in the diffusion regime of PeV cosmic rays in the Sgr A* accretion flow
arXiv (Cornell University)·2024Open Access
Magnetothermal evolution in the cores of adolescent neutron stars: The Grad–Shafranov equilibrium is never reached in the ‘strong-coupling’ regime
Monthly Notices of the Royal Astronomical Society·2023· 4 citedOpen Access
Magneto-thermal evolution in the cores of adolescent neutron stars: The Grad-Shafranov equilibrium is never reached in the 'strong-coupling' regime
arXiv (Cornell University)·2023Open Access
Stability of axially symmetric magnetic fields in stars
Monthly Notices of the Royal Astronomical Society·2022· 10 cited
Stability of axially symmetric magnetic fields in stars
arXiv (Cornell University)·2022Open Access
Evolution of random initial magnetic fields in stably stratified and barotropic stars
Monthly Notices of the Royal Astronomical Society·2022Open Access
Evolution of random initial magnetic fields in stably stratified and barotropic stars
arXiv (Cornell University)·2021· 23 citedOpen Access
Revisiting neutron starquakes caused by spin-down
Astronomy and Astrophysics·2021· 13 citedOpen Access
The search for high altitude sites in South America for the SWGO detector
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021)·2021· 9 citedOpen Access
Very-High-Energy γ-rays From the Galactic Center Generated by Cosmic Rays
2021
Neutron starquakes caused by spin-down
Bulletin of the American Physical Society·2021
Magneto-thermal evolution of neutron star cores in the "strong-coupling regime"
43rd COSPAR Scientific Assembly. Held 28 January - 4 February·2021
Constraining the equation of state of dense nuclear matter using thermal emission of neutron stars
Journal of Physics Conference Series·2020· 1 citedOpen Access
Two-fluid simulations of the magnetic field evolution in neutron star cores in the weak-coupling regime
Monthly Notices of the Royal Astronomical Society·2020· 22 citedOpen Access
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Frequent Co-authors

H. Quintana(7), J. A. Valdivia(7), Rolando Dünner(5), Sébastien Guillot(5), N. Langer(4), Peter Goldreich(3), E. R. Carrasco(3), H. Muriel(3), C. J. Ragone(3), L. Fossati(3), N. Castro(3), T. Morel(3), M. Briquet(3), T. A. Carroll(3), S. Hubrig(3), M. F. Nieva(3), L. M. Oskinova(3), N. Przybilla(3), F. R. N. Schneider(3), M. Schöller(3)