Pulsar-driven Jets in Supernovae, Gamma-Ray Bursts, and the Universe
Abstract
The bipolarity of Supernova 1987A can be understood through its very early light curve observed from the CTIO 0.4-m telescope and IUE FES, and following speckle observations of the `Mystery Spot' by two groups. These indicate a highly directional beam/jet of light/particles, with initial collimation factors in excess of 10,000 and velocities in excess of 0.95 c, as an impulsive event of up to 1e-5 solar masses interacting with circumstellar material. These can be produced by a model proposed in 1972, by Bolotovskii and Ginzburg, which employs pulsar emission from polarization currents induced/(modulated faster than c) beyond the pulsar light cylinder by the periodic electromagnetic field (supraluminally induced polarization currents -- SLIP). SLIP accounts for the disruption of progenitors in supernova explosions and their anomalous dimming at cosmological distances, jets from Sco X-1 and SS 433, the lack/presence of intermittent pulsations from the high/low luminosity low mass X-ray binaries, long/short gamma-ray bursts and predicts that their afterglows are the pulsed optical/near infrared emission associated with these pulsars. SLIP may also account for the TeV e+/e- results from PAMELA and ATIC, the WMAP `Haze'/Fermi `Bubbles', and the r-process. SLIP jets from SNe of the first stars may allow galaxies to form without dark matter, and explain the peculiar, non-gravitational motions observed from pairs of distant galaxies by GALEX.
Keywords
Cite
@article{arxiv.1205.5107,
title = {Pulsar-driven Jets in Supernovae, Gamma-Ray Bursts, and the Universe},
author = {John Middleditch},
journal= {arXiv preprint arXiv:1205.5107},
year = {2015}
}
Comments
This article has been published in the open source journal, Advances in Astronomy: http://www.hindawi.com/journals/aa/2012/898907 This arXiv version is out of date. arXiv admin note: substantial text overlap with arXiv:0909.2604 (Note: but less so by v2, Also Brook Sandford in Ackn. -JM)