Global Anisotropies in Supernova Explosions and Pulsar Recoil

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dc.creatorScheck, L.
dc.creatorPlewa, T.
dc.creatorKifonidis, K.
dc.creatorJanka, H. -Th.
dc.creatorMüller, E.
dc.date2004-05-17
dc.date2004-05-18
dc.date.accessioned2026-07-25T19:20:23Z
dc.descriptionWe show by two-dimensional and first three-dimensional simulations of neutrino-driven supernova explosions that low (l=1,2) modes can dominate the flow pattern in the convective postshock region on timescales of hundreds of milliseconds after core bounce. This can lead to large global anisotropy of the supernova explosion and pulsar kicks in excess of 500 km/s.
dc.description3 pages, 2 figures, contribution to Procs. 12th Workshop on Nuclear Astrophysics, Ringberg Castle, March 22-27, 2004
dc.identifierhttps://arxiv.org/abs/astro-ph/0405311
dc.identifierhttp://arxiv.org/abs/astro-ph/0405311
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/63793
dc.subjectAstrophysics
dc.titleGlobal Anisotropies in Supernova Explosions and Pulsar Recoil
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