6533b862fe1ef96bd12c61d2
RESEARCH PRODUCT
SIMULATIONS OF DYNAMICS AND EMISSION FROM MAGNETIZED GRB AFTERGLOWS
Dimitrios GianniosMiguel A. AloyPetar Mimicasubject
PhysicsAstrophysics::High Energy Astrophysical PhenomenaAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLight curveAfterglowMagnetic fieldInterstellar mediumMagnetizationSpace and Planetary ScienceMagnetohydrodynamicsGamma-ray burstEjectaAstrophysics::Galaxy AstrophysicsMathematical Physicsdescription
The role of magnetic fields in the GRB flow is still controversial. The afterglow emission, particularly the early phases, may provide a probe into the magnetization of the outflow. Using ultrahigh resolution relativistic MHD simulations, the interaction between radially expanding magnetized ejecta with the interstellar medium is studied. We explore the effect of the magnetic field strength of the ejecta on the afterglow structure, particularly regarding the presence and strength of a reverse shock. We compute synthetic afterglow light curves to quantify the effect of the magnetization of the flow on observed radiation.
| year | journal | country | edition | language |
|---|---|---|---|---|
| 2010-06-01 | International Journal of Modern Physics D |