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星期三, 二月 20, 2008

Belmont 2008 一个模拟高能辐射过程的程序

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好像还没成熟,值得期待完整的程序。

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文章信息:

· arXiv e-print (arXiv:0802.2661)
· References in the Article
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Title:
A new code for radiation processes in high energy plasmas
Authors:
Belmont, R.; Malzac, J.; Marcowith, A.
Publication:
eprint arXiv:0802.2661
Publication Date:
02/2008
Origin:
ARXIV
Keywords:
Astrophysics
Comment:
Poster at the international workshop 'Simbol-X: the hard X-ray universe in focus' held in Bologna, 14-16 May 2007. To appear in Memorie della SAIt, 2 pages, 1 figure
Bibliographic Code:
2008arXiv0802.2661B

Abstract

Extreme objects such as X-ray binaries, AGN, or $\gamma$-ray bursters harbor high energy plasmas whose properties are not well understood yet. Not only are they responsible of the hard X- and $\gamma$-ray emission we observe but also they have a strong influence on the main dynamics and energetics of these objects themselves. Here we present a new kinetic code that solves the evolution equations for particles and photons around compact objects. It produces spectra that will be compared with observations from Simbol-X to constrain the radiation and acceleration processes in these objects.
Bibtex entry for this abstract Preferred format for this abstract (see Preferences)

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