GRB afterglows: deep Newtonian phase and its application

Details GRB afterglows: deep Newtonian phase and its application GRB afterglows: deep Newtonian phase and its application

2005-02-26

arxiv.org/abs/astro-ph/0502555v1

Nuovo Cim.C28:415-418,2005

Astronomy and Astrophysics

Astrophysics

Poster at the 4th workshop "Gamma-Ray Bursts in the Afterglow Era" (Rome, 2004), accepted for publication in the proceedings.

Scientific paper

10.1393/ncc/i2005-10141-2

Gamma-ray burst afterglows have been observed for months or even years in a few cases. It deserves noting that at such late stages, the remnants should have entered the deep Newtonian phase, during which the majority of shock-accelerated electrons will no longer be highly relativistic. To calculate the afterglows, we must assume that the electrons obey a power-law distribution according to their kinetic energy, not simply the Lorentz factor.

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