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相关论文: Models for Nonthermal Photon Spectra

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The ultimate goal of the observation of nonthermal emission from astrophysical sources is to understand the underlying particle acceleration and evolution processes, and few tools are publicly available to infer the particle distribution…

高能天体物理现象 · 物理学 2015-09-14 Víctor Zabalza

In this paper we complete the set of diagnostic tools for synchrotron emitting sources presented by Del Zanna et al. (Astron. Astrophys. 453, 621, 2006) with the computation of inverse Compton radiation from the same relativistic particles.…

天体物理学 · 物理学 2009-11-13 D. Volpi , L. Del Zanna , E. Amato , N. Bucciantini

In this paper we review the possible radiation mechanisms for the observed non-thermal emission in clusters of galaxies, with a primary focus on the radio and hard X-ray emission. We show that the difficulty with the non-thermal,…

天体物理学 · 物理学 2009-11-13 V. Petrosian , Y. Rephaeli , A. Bykov

In a hybrid thermal-nonthermal plasma, we find that the dominant emission and absorption mechanisms are synchrotron by nonthermal electrons and bremsstrahlung by thermal electrons. These two processes significantly change the spectrum from…

天体物理学 · 物理学 2009-10-30 D. Lin , E. P. Liang

Interactions between photons and electrons are ubiquitous in astrophysics. Photons can be down scattered (Compton scattering) or up scattered (inverse Compton scattering) by moving electrons. Inverse Compton scattering, in particular, is an…

高能天体物理现象 · 物理学 2023-04-05 Anderson C. M. Lai , Kenny C. Y. Ng

The observational signature of supernova remnants (SNRs) is very complex, in terms of both their geometrical shape and their spectral properties, dominated by non-thermal synchrotron and inverse-Compton scattering. We propose a…

太阳与恒星天体物理 · 物理学 2014-11-14 M. Obergaulinger , J. Ma. Chimeno , P. Mimica , M. A. Aloy , A. Iyudin

We study the X-ray spectra of tenuous, two-temperature accretion flows using a model involving an exact, Monte Carlo computation of the global Comptonization effect as well as general relativistic description of both the flow structure and…

高能天体物理现象 · 物理学 2015-06-23 Andrzej Niedzwiecki , Agnieszka Stepnik , Fu-Guo Xie

Massive stars in binary systems have long been regarded as potential sources of high-energy gamma rays.The emission is principally thought to arise in the region where the stellar winds collide and accelerate relativistic particles which…

高能天体物理现象 · 物理学 2015-06-19 K. Reitberger , R. Kissmann , A. Reimer , O. Reimer

Using Monte Carlo methods to simulate the inverse Compton scattering of soft photons, we model the spectrum of the Galactic black hole candidate Cyg X-1, which shows evidence of a nonthermal tail extending beyond a few hundred keV. We…

天体物理学 · 物理学 2009-10-30 A. Crider , E. P. Liang , I. A. Smith , D. Lin , M. Kusunose

We study the emission and absorption spectra due to various photon and pair processes in a non-equilibrium pair plasma containing a significant density of photons. We present here some preliminary results from Monte-Carlo simulations. These…

天体物理学 · 物理学 2007-05-23 Ravi P. Pilla , Jacob Shaham

Hard, non-thermal, persistent pulsed X-ray emission extending between 10 keV and $\sim 150$ keV has been observed in nearly ten magnetars. For inner-magnetospheric models of such emission, resonant inverse Compton scattering of soft thermal…

高能天体物理现象 · 物理学 2018-02-28 Zorawar Wadiasingh , Matthew G. Baring , Peter L. Gonthier , Alice K. Harding

We consider a relativistically moving blob consisting of an isotropic electron distribution that Compton-scatters photons from an external isotropic radiation field. We compute the resulting beaming pattern, i.e. the distribution of the…

高能天体物理现象 · 物理学 2011-07-27 Anne Hutter , Felix Spanier

We treat the non-relativistic Compton scattering process in which an incoming photon scatters from an N-electron many-body state to yield an outgoing photon and a recoil electron, without invoking the commonly used frameworks of either the…

强关联电子 · 物理学 2007-10-11 I. G. Kaplan , B. Barbiellini , A. Bansil

We investigate the phenomenology of nonlinear Compton scattering of polarised photons by unpolarised electrons in plane-wave backgrounds. The energy and angular spectra of polarised photons are calculated for linearly- and…

高能物理 - 唯象学 · 物理学 2020-08-19 B. King , S. Tang

The beaming pattern of radiation emitted by a relativistically moving source like jets in microquasars, AGN and GRBs, is a key issue for understanding of acceleration and radiation processes in these objects. In this paper we introduce a…

高能天体物理现象 · 物理学 2018-05-30 S. R. Kelner , E. Lefa , F. M. Rieger , F. A. Aharonian

We present our software to compute gamma-ray emission from inverse-Compton scattering by cosmic-ray leptons in the heliosphere, as well as in the photospheres of stars. It includes a formulation of modulation in the heliosphere, but it can…

太阳与恒星天体物理 · 物理学 2015-06-15 Elena Orlando , Andrew W. Strong

The non-thermal spectra of jetted active galactic nuclei show a variety of shapes in their low- and high energy components. In some of the brightest Fermi-LAT blazars, prominent spectral breaks at a few GeV have been regularly detected,…

高能天体物理现象 · 物理学 2016-04-20 Lars Hunger , Anita Reimer

We study the blackbody properties and the thermodynamic equilibrium quantities of a photon gas in the framework of nonlinear electrodynamics. In this vein, we take into account the photon propagation in a uniform external magnetic field in…

统计力学 · 物理学 2023-08-23 I. Soares , R. Turcati , S. B. Duarte

The spectral properties of a hybrid steady thermal-nonthermal isotropic plasma are studied. The involved emission mechanisms are thermal bremsstrahlung, nonthermal bremsstrahlung, cyclotron and nonthermal synchrotron. Formulas are derived…

天体物理学 · 物理学 2007-05-23 D. Lin , E. P. Liang

We investigate roles of the bulk comptonization process in the propagation of thermal photons emitted at the shock breakout of a supernova explosion. We use a hydrodynamical model based on a self-similar solution for the shock breakout. The…

高能天体物理现象 · 物理学 2015-05-19 Akihiro Suzuki , Toshikazu Shigeyama
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