Black-hole ejecta by frame-dragging along the axis of rotation

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dc.creatorvan Putten, Maurice H. P. M.
dc.date2004-09-02
dc.date.accessioned2026-07-07T02:14:27Z
dc.date.available2026-07-07T02:14:27Z
dc.descriptionAn energy $E=ωJ$ is derived for gravitational spin-orbit coupling by frame-dragging $ω$ acting on angular momentum $J$. This interaction defines a no-boundary mechanism for linear acceleration of magnetized matter along the axis of rotation of black holes. We explain GRB030329/SN2003dh by centered nucleation of a high-mass black hole with rapid rotation, producing baryon-poor ejecta by gravitational spin-orbit coupling. The duration of the burst is attributed to spin-down in the emission of gravitational-waves by a surrounding non-axisymmetric torus.
dc.identifierhttps://arxiv.org/abs/astro-ph/0409062
dc.identifierhttp://arxiv.org/abs/astro-ph/0409062
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8116
dc.subjectAstrophysics
dc.titleBlack-hole ejecta by frame-dragging along the axis of rotation
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