Magnetorotation-induced pulsar recoils

H. Sawai, K. Kotake, S. Yamada

Research output: Contribution to journalArticle

Abstract

We propose a new mechanism for pulsar kicks, which is magnetohydrodynamically-induced kick. We carry out two-dimensional numerical simulations on the core-collapse of a massive star with differential rotation and initially large magnetic fields which have equatorially asymmetric dipole-like configuration. As a result of the computations, we get transient large kick velocities which are up to 500 km/s. However, these large velocities are soon damped since surrounding matter prevent proto-neutron-stars from moving away and finally no substantial kicks are produced. This may be a crucial problem for all pulsar kick computations.

Original languageEnglish
Pages (from-to)151-152
Number of pages2
JournalJournal of Physics: Conference Series
Volume31
Issue number1
DOIs
Publication statusPublished - 2006 Mar 22

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Fingerprint Dive into the research topics of 'Magnetorotation-induced pulsar recoils'. Together they form a unique fingerprint.

  • Cite this