Principal Investigators: Kostas Kokkotas, Ralph Neuhaeuser
Magnetars are neutron stars with a magnetic field greatly
exceeding B > 10^14 G. Sporadic "giant flares" are believed
to be associated with starquakes caused by the rearrangement
of the huge magnetic field. During these giant flares huge
amounts of energy are released in only a few seconds (gamma
and x-rays) and in addition, it is expected that gravitational
waves should be generated. The plan is to simulate the magnetar
dynamics in order to reveal the actual strength of the emitted
gravitational waves, while in addition a Bayesian approach will
be used for the detection of as yet unnoticed high frequency
oscillations of magnetars.
| Kostas Kokkotas | Professor, PI 2010 | ||
| Ralph Neuhaeuser | Professor, PI 2010 | ||
| Markus Hohle | Postdoc, 2011 | ||
| Antonella Colaiuda | Postdoc, 2011 | ||
| Sam Lander | Postdoc, 2011 | ||
| Ludwig Trepl | PhD Student, 2010 | ||
| Janos Schmidt | PhD Student, 2011 |
[1]
Stratification, superfluidity and magnetar QPOs
A. Passamonti, S. K. Lander,
arXiv:1210.2969 (MNRAS submitted)
[2]
Motion of charged particles and quasinormal modes around the magnetically and tidally deformed black hole
R. A. Konoplya, Yu-Chun Liu,
arXiv:1205.5311v1
[3]
Are there any stable magnetic fields in barotropic stars?
S. K. Lander, D. I. Jones,
arXiv:1202.2339 (MNRAS submitted)
[4]
Coupled polar-axial magnetar oscillations
A. Colaiuda, K.D. Kokkotas,
MNRAS in press
[5]
Hydromagnetic equilibrium in non-barotropic multifluid neutron stars
K. Glampedakis, N. Andersson, S.K. Lander,
MNRAS 2012, 420, 1263
[6]
Magnetic neutron star equilibria with stratification and type-II superconductivity
S.K.Lander, N. Andersson, K. Glampedakis,
MNRAS 2012, 419, 732
[7]
Are gravitational waves from giant magnetar flares observable?
B. Zink, P.D. Lasky, K.D. Kokkotas,
Phys. Rev. D 2012, 85, 024030
[8]
Gravitational Waves and Hydromagnetic Instabilities in Rotating Magnetized Neutron Stars
P. Lasky, B. Zink, K.D. Kokkotas,
Phys. Rev. D (2012)
[9]
Magnetars oscillations in the presence of a crust
A. Colaiuda, K.D. Kokkotas,
MNRAS 2011, 414, 3014
[10]
Magnetohydrodynamics of superfluid and superconducting neutron star cores
K. Glampedakis, N. Andersson, L. Samuelsson,
MNRAS 2011, 410, 805
[11]
Ambipolar diffusion in superfluid neutron stars
K. Glampedakis, D.I. Jones, L. Samuelsson,
MNRAS 2011, 413, 2021
[12]
Magneto-rotational neutron star evolution: the role of core vortex pinning
K. Glampedakis, N. Andersson,
ApJ 2011, 740, 35
[13]
Bayesian timing analysis of giant flare of SGR 1806-20 by RXTE PCA
V. V. Hambaryan, R. Neuhaeuser, K. D. Kokkotas,
Astronomy and Astrophysics 528, 45
[14]
Hydromagnetic instabilities in relativistic neutron stars
P.D. Lasky, B. Zink, K.D. Kokkotas, K. Glampedakis,
ApJ 2011, 735, 20L
[15]
HORIZON: Accelerated General Relativistic Magnetohydrodynamics
B. Zink,
arXiv:1102.5202
[16]
Magnetized Neutron Stars
A. Colaiuda,
PhDThesis, Eberhard-Karls-University of Tübingen (2011)
[17]
Particle Motion around Black Holes immersed in a Magnetic Field
Liu, Yu-Chun,
Diploma Thesis, Master Thesis, Eberhard-Karls-University of Tübingen (2011)