Session X3: Magnetars

1:30 PM–3:18 PM, Tuesday, April 25, 2006
Hyatt Regency Dallas - Landmark C

Sponsoring Unit: DAP
Chair: David Palmer, Los Alamos National Laboratory

Abstract ID: BAPS.2006.APR.X3.3

Abstract: X3.00003 : Solar physics of magnetars

2:42 PM–3:18 PM

Preview Abstract

Author:

  Maxim Lyutikov
    (UBC)

Two closely related types of neutron stars -- Anomalous X-ray Pulsars and Soft Gamma Ray Repeaters, commonly called magnetars -- posses magnetic field exceeding quantum critical fields. Dissipation of these fields powers persistent and bursting emission and produces occasionally giant flares. Using analogies with the Sun, I will describe magnetospheric structure of magnetars, the way magnetic dissipation can proceed in the relativistically strong regime and how giant flares, analogues of coronal mass ejections, may develop. Finally, I will discuss how the observed non-thermal spectra can be formed through resonant cyclotron scattering of surfaces radiation.

To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2006.APR.X3.3