pith. sign in

arxiv: 1710.00373 · v1 · pith:TIIUBN2Unew · submitted 2017-10-01 · 🌌 astro-ph.HE

Cooling waves in pair plasma

classification 🌌 astro-ph.HE
keywords coolingpairtemperaturemuchplasmawaveapproxbelow
0
0 comments X
read the original abstract

We consider structure and emission properties of a pair plasma fireball that cools due to radiation. At temperatures $T \geq 0.5 m_e c^2$ the cooling takes a form of clearly defined cooling wave, whereby the temperature and pair density experience a sharp drop within a narrow region. The surface temperature, corresponding to the location where the optical depth to infinity reaches unity, never falls much below $0.1 m_e c^2 \approx 50$ keV. The propagation velocity of the cooling wave is much smaller than the speed of light and decreases with increasing bulk temperature.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.