Nikolaos Stergioulas
Nikolaos Stergioulas
Professor, Department of Physics, Aristotle University of Thessaloniki
Verified email at - Homepage
Cited by
Cited by
Design concepts for the Cherenkov Telescope Array CTA: an advanced facility for ground-based high-energy gamma-ray astronomy
CTA Consortium J. Knapp@ leeds. ac. uk http://www. cta-observatory. org, ...
Experimental Astronomy 32, 193-316, 2011
Introducing the CTA concept
BS Acharya, M Actis, T Aghajani, G Agnetta, J Aguilar, F Aharonian, ...
Astroparticle physics 43, 3-18, 2013
Black holes, gravitational waves and fundamental physics: a roadmap
L Barack, V Cardoso, S Nissanke, TP Sotiriou, A Askar, C Belczynski, ...
Classical and quantum gravity 36 (14), 143001, 2019
Neutron-star radius constraints from GW170817 and future detections
A Bauswein, O Just, HT Janka, N Stergioulas
The Astrophysical Journal Letters 850 (2), L34, 2017
Comparing models of rapidly rotating relativistic stars constructed by two numerical methods
N Stergioulas, JL Friedman
arXiv preprint astro-ph/9411032, 1994
Rotating stars in relativity
N Stergioulas
Living Reviews in Relativity 6 (1), 3, 2003
Three-dimensional relativistic simulations of rotating neutron-star collapse to a Kerr black hole
L Baiotti, I Hawke, PJ Montero, F Löffler, L Rezzolla, N Stergioulas, ...
Physical Review D—Particles, Fields, Gravitation, and Cosmology 71 (2), 024035, 2005
Prospects for fundamental physics with LISA
E Barausse, E Berti, T Hertog, SA Hughes, P Jetzer, P Pani, TP Sotiriou, ...
General Relativity and Gravitation 52, 1-33, 2020
Quantum gravity phenomenology at the dawn of the multi-messenger era—A review
A Addazi, J Alvarez-Muniz, RA Batista, G Amelino-Camelia, V Antonelli, ...
Progress in Particle and Nuclear Physics 125, 103948, 2022
On the relevance of the r-mode instability for accreting neutron stars and white dwarfs
N Andersson, KD Kokkotas, N Stergioulas
The Astrophysical Journal 516 (1), 307, 1999
Rotating relativistic stars
JL Friedman, N Stergioulas
Cambridge University Press, 2013
Towards a stable numerical evolution of strongly gravitating systems in general relativity: The conformal treatments
M Alcubierre, B Brügmann, T Dramlitsch, JA Font, P Papadopoulos, ...
Physical Review D 62 (4), 044034, 2000
The large observatory for X-ray timing (LOFT)
M Feroci, L Stella, M Van der Klis, TJL Courvoisier, M Hernanz, R Hudec, ...
Experimental Astronomy 34, 415-444, 2012
Three-dimensional numerical general relativistic hydrodynamics. II. Long-term dynamics of single relativistic stars
JA Font, T Goodale, S Iyer, M Miller, L Rezzolla, E Seidel, N Stergioulas, ...
Physical Review D 65 (8), 084024, 2002
Gravitational waves and non-axisymmetric oscillation modes in mergers of compact object binaries
N Stergioulas, A Bauswein, K Zagkouris, HT Janka
Monthly Notices of the Royal Astronomical Society 418 (1), 427-436, 2011
Torsional oscillations of relativistic stars with dipole magnetic fields
H Sotani, KD Kokkotas, N Stergioulas
Monthly Notices of the Royal Astronomical Society 375 (1), 261-277, 2007
Rotating stars in relativity
V Paschalidis, N Stergioulas
Living Reviews in Relativity 20, 1-169, 2017
Observing gravitational waves from the post-merger phase of binary neutron star coalescence
JA Clark, A Bauswein, N Stergioulas, D Shoemaker
Classical and Quantum Gravity 33 (8), 085003, 2016
Unified picture of the post-merger dynamics and gravitational wave emission in neutron star mergers
A Bauswein, N Stergioulas
Physical Review D 91 (12), 124056, 2015
Construction of highly accurate models of rotating neutron stars–comparison of three different numerical schemes
T Nozawa, N Stergioulas, E Gourgoulhon, Y Eriguchi
Astronomy and Astrophysics Supplement Series 132 (3), 431-454, 1998
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