Spectral evolution of non-thermal electron distributions in intense radiation fields
From MaRDI portal
Publication:5437458
DOI10.1051/0004-6361:20078298zbMATH Open1130.85316arXiv0708.1516OpenAlexW2124619345WikidataQ68664742 ScholiaQ68664742MaRDI QIDQ5437458
Author name not available (Why is that?)
Publication date: 21 January 2008
Published in: (Search for Journal in Brave)
Abstract: (abridged) Models of many astrophysical gamma-ray sources assume they contain a homogeneous distribution of electrons that are injected as a power-law in energy and evolve by interacting with radiation fields, magnetic fields and particles in the source and by escaping. This problem is particularly complicated if the radiation fields have higher energy density than the magnetic field and are sufficiently energetic that inverse Compton scattering is not limited to the Thomson regime. We present a simple, time-dependent, semi-analytical solution of the electron kinetic equation that treats both continuous and impulsive injection, cooling via synchrotron and inverse Compton radiation, (taking into account Klein-Nishina effects) and energy dependent particle escape. The kinetic equation for an arbitrary, time-dependent source function is solved by the method of Laplace transformations. Using an approximate expression for the energy loss rate that takes into account synchrotron and inverse Compton losses including Klein-Nishina effects for scattering off an isotropic photon field with either a power-law or black-body distribution, we find explicit expressions for the cooling time and escape probability of individual electrons. This enables the full, time-dependent solution to be reduced to a single quadrature. From the electron distribution, we then construct the time-dependent, multi-wavelength emission spectrum. We compare our solutions with several limiting cases and discuss the general appearance and temporal behaviour of spectral features (i.e., cooling breaks, bumps etc.). As a specific example, we model the broad-band energy spectrum of the open stellar association Westerlund-2 at different times of its evolution, and compare it with observations.
Full work available at URL: https://arxiv.org/abs/0708.1516
No records found.
No records found.
This page was built for publication: Spectral evolution of non-thermal electron distributions in intense radiation fields
Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q5437458)
