M.Sc. Theses

  Theses supervised in the M.Sc. program "Computational Physics" by members of our section.
  Maria Andrea: Numerical models of magnetospheres for strongly magnetized neutron stars (N. Stergioulas) 
  Maria Manolopoulou: Galaxy Cluster Rotation (E. Plionis) English version:
Konstantinos Palapanidis: Equilibrium Models of Strongly Magnetized Neutron Stars (N. Stergioulas) English version: 
Christos VourellisModels of black hole disks with self-gravity and non-constant angular momentum (N. Stergioulas) 
  Eleni Graikou Timing of the Triple Pulsar System PSR J1623-2631 using TEMPO2 (N. Stergioulas, J.H. Seiradakis, K. Lazaridis) en   gr (summary) 
  Gkratsia Tantilian Simulating the Gravitational Field on a Non-rotating Neutron Star on GPUs (K. Kokkotas, N. Stergioulas) gr  en   presentation 
Panagiotis Iosif:  The CFC approximation in uniformly and differentially rotating relativistic stars (N. Stergioulas) gr   en (summary) 
  Panagiotis Antoniadis: The IDO Method and its Implementation in CUDA C (N. Stergioulas)  (additionaly, download numerical codes here).
Vasileios FrogakisAlfvén quasi-periodic oscillation in neutron stars and numerical solution of magnetohydrodynamic equations (N. Stergioulas) 
Petros Kalogeras: Theoretical and numerical consideration of the baroclinic instability (N. Stergioulas) 
  Χρήστος Παναγιωτακόπουλος: Μελέτη Συστημάτων Lotcka-Volterra (E. Μελετλίδου) 
  Magdalini Anastasiou: Study of neutron stars single and integrated pulses (N. Stergioulas) 

Nikolaos Tsakiris: A Vacuum Tracking Method for Oscillating Stars (N. Stergioulas) 

Dimitrios Voukantzis: Simulations of Compact Binary Systems in the Ellipsoidal Approximation (N. Stergioulas)    
  Vasileios Tziampazlis: Three-Dimensional Simulations of Rotational Modes in Relativistic Stars  (N. Stergioulas)        
Λουκάς Σκαρπαλέζος: Χαοτική Κίνηση (Ε. Μελετλίδου) 
Οδυσσέας Μααΐτα Τζαμάλ: Μοντελοποίηση του Ομογενούς Μαρκοβιανού Συστήματος ως Ελαστικό Μέσο   (Ε. Μελετλίδου) 
  Georgios Askolidis: Three-Dimensional Visualization of Simulations in Numerical Relativity (N. Stergioulas)  
Eythimios Kotsialos: Numerical Solution of Ordinary Differential Equations Using Power Series Methods and Applications to the General Three-Body Problem (G. Voyatzis)