Abstract
Magnetars are surrounded by diffuse plasma in magnetic field strengths well above the quantum electrodynamic critical value. We derive equations of ''quantum force-free electrodynamics'' for this plasma using effective field theory arguments. We argue that quantum effects do not modify the large scale structure of the magnetosphere, and in particular that the spin-down rate does not deviate significantly from the classical result. We provide definite evolution equations that can be used to explore potentially important small-scale corrections, such as shock formation, which has been proposed as a mechanism for both burst and quiescent emission from magnetars.
Original language | English (US) |
---|---|
Article number | 042 |
Journal | Journal of Cosmology and Astroparticle Physics |
Volume | 2016 |
Issue number | 5 |
DOIs | |
State | Published - May 19 2016 |
Externally published | Yes |
ASJC Scopus subject areas
- Astronomy and Astrophysics