Compton drag as a mechanism for very high linear polarization in gamma-ray bursts

The recent claim by Coburn & Boggs to have detected a very high degree of linear polarization in the prompt emission of GRB 021206 has stimulated interest in how much polarization could arise in gamma-ray bursts (GRBs) from synchrotron emission. Alternatively, as Shaviv & Dar have shown, GRB polarization could be produced by inverse Compton scattering in the point-source limit. We discuss polarization from a fireball that upscatters a soft radiation field. We show that, after the proper angular integration, the residual polarization can be large, in some cases approaching the point-source limit. We discuss the probability of realizing the geometrical conditions in which a large polarization is obtained showing that, for a particularly bright burst such as GRB 021206, the detection of polarization at the first attempt in the Compton drag scenario is not unlikely.

[1]  Eli Waxman,et al.  Astronomy: New direction for γ-rays , 2003, Nature.

[2]  Arnon Dar,et al.  Gamma Ray Bursts from Minijets , 1994 .

[3]  Gruzinov,et al.  Strongly Polarized Optical Afterglows of Gamma-Ray Bursts , 1999, The Astrophysical journal.

[4]  R. Laing A model for the magnetic-field structure in extended radio sources , 1980 .

[5]  G. Rybicki,et al.  Radiative processes in astrophysics , 1979 .

[6]  M. Feroci,et al.  Intrinsic spectra and energetics of BeppoSAX Gamma-Ray Bursts with known redshifts , 2002, astro-ph/0205230.

[7]  M. Rees,et al.  Compton-dragged Gamma-Ray Bursts Associated with Supernovae , 1999, The Astrophysical journal.

[8]  S. R. Kulkarni,et al.  BEAMING IN GAMMA-RAY BURSTS: EVIDENCE FOR A STANDARD ENERGY RESERVOIR , 2001 .

[9]  Davide Lazzati,et al.  Polarization light curves and position angle variation of beamed gamma-ray bursts , 1999, astro-ph/9906471.

[10]  Re'em Sari,et al.  Linear Polarization and Proper Motion in the Afterglow of Beamed Gamma-Ray Bursts , 1999, astro-ph/9906503.

[11]  N. Shaviv,et al.  Fireballs in dense stellar regions as an explanation of gamma-ray bursts , 1995, astro-ph/9503105.

[12]  B. Garilli,et al.  Inverse Compton scattering of ambient radiation by a cold relativistic jet - A source of beamed, polarized continuum in blazars? , 1987 .

[13]  Amotz Shemi Gamma-ray bursts from interaction of relativistic flows with radiation fields , 1994, astro-ph/9404047.

[14]  David Eichler,et al.  Polarization of Gamma-Ray Bursts via Scattering off a Relativistic Sheath , 2003 .

[15]  B. Paczyński,et al.  Bursts of gamma rays from Compton scattering at cosmological distances , 1991 .

[16]  Jonathan Granot,et al.  LINEAR POLARIZATION IN GAMMA-RAY BURSTS: THE CASE FOR AN ORDERED MAGNETIC FIELD , 2003 .

[17]  T. Piran,et al.  Implications of the -ray polarization of GRB 021206 , 2003, astro-ph/0307290.

[18]  Abraham Loeb,et al.  Generation of Magnetic Fields in the Relativistic Shock of Gamma-Ray Burst Sources , 1999, astro-ph/9904363.

[19]  C. I. O. Technology.,et al.  Polarization of Prompt Gamma-Ray Burst Emission: Evidence for Electromagnetically Dominated Outflow , 2003, astro-ph/0305410.

[20]  M. Rees,et al.  Compton dragged gamma‐ray bursts: the spectrum , 2000, astro-ph/0002049.

[21]  S. Boggs,et al.  Polarization of the prompt γ-ray emission from the γ-ray burst of 6 December 2002 , 2003, Nature.