[SEMINARI] Termination of the magnetorotational instability....
Enric Marco
Enric.Marco en uv.es
Lun Feb 2 14:23:54 CET 2015
Title: Termination of the magnetorotational instability via the
parasitic Kelvin-Helmholtz instability in core-collapse supernovae.
Speaker: Tomasz Rembiasz (MPA, Garching)
Data: Dimecres 4 de Febrer a les 12:30 hores en el seminari.
Abstract:
Magnetorotational instability (MRI) is one of the most promising agents
significantly amplifying magnetic fields in (resulting from
rapidly rotating progenitors) core-collapse supernovae (CC-SNe).
The initial phase of the MRI (of the exponential growth) is well understood,
however its exact termination mechanism remains unknown.
In this talk, we present our newest results clearly indicating
that the MRI, given CC-SN conditions, is terminated by the parasitic
Kelvin-Helmholtz instability.
This allows us to set the limit on the maximum magnetic field amplification
by the MRI.
http://celeste.uv.es/daa/seminari.php.UTF8?id=1090
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Dr. Enric Marco
Departament d'Astronomia i Astrofísica
Facultat de Física
Universitat de València
C/ Dr. Moliner, 50
46100 Burjassot, Spain
Phone: (34)-96-354-3069
Fax:(34)-96-354-3084
enric.marco en uv.es
www.uv.es/marco
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