Published 2002 | Version public
Book Section - Chapter

To the Lighthouse

  • 1. ROR icon California Institute of Technology

Abstract

The extreme hypothesis that essentially all types of ultrarelativistic outflow - specifically AGN jets, pulsar wind nebulae and GRB - are electromagnetic, rather than gas dynamical, phenomena is considered. Electromagnetic flows are naturally anisotropic and self-collimating so as to produce jet-like features. The relativistic force-free description of these flows, which is simpler than the relativistic MHD description, is explained. It is suggested that the magnetic field associated with AGN jets and GRB is quite extensively distributed in latitüde, without necessarily increasing by much the total power. It is also proposed that the observed emission from these sources traces out regions of high current density where global instabilities drive a turbulence spectrum that is ultimately responsible for the particle acceleration and the synchrotron, inverse Compton and synchro-Compton emission. The direct extraction of spin energy from a black hole is re-examined and an electromagnetic model of GRB explosions is developed. It is also suggested that some GRB "lighthouses" be identified with accretion-induced collapse of a neutron star to form a black hole in a binary system.

Additional Information

© 2002 Springer-Verlag Berlin Heidelberg. First Online 08 October 2003. I thank the organisers of this workshop for their hospitality and patience and Mitch Begelman, Paolo Coppi, Arieh Konigl, Amir Levinson, Max Lyutikov, Chris McKee, David Payne, Martin Rees and Roman Znajek for their collaboration. Brian Punsly and Maurice van Putten are also thanked for stimulating debates on some of the issues raised here. Support under NASA grant 5-2837 is gratefully acknowledged.

Additional details

Identifiers

Eprint ID
96212
DOI
10.1007/10856495_59
Resolver ID
CaltechAUTHORS:20190607-141641546

Related works

Describes
10.1007/10856495_59 (DOI)

Funding

NASA
5-2837

Dates

Created
2019-06-07
Created from EPrint's datestamp field
Updated
2021-11-16
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
TAPIR
Series Name
ESO Astrophysics Symposia