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Simultaneous solution of Kompaneets equation and Radiative Transfer equation in the photon energy range 1 - 125 KeV

机译:Kompaneets方程和辐射传输的同时求解   光子能量范围为1 - 125 KeV的方程

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摘要

Radiative transfer equation in plane parallel geometry and Kompaneetsequation is solved simultaneously to obtain theoretical spectrum of 1-125 KeVphoton energy range. Diffuse radiation field is calculated usingtime-independent radiative transfer equation in plane parallel geometry, whichis developed using discrete space theory (DST) of radiative transfer in ahomogeneous medium for different optical depths. We assumed free-free emissionand absorption and emission due to electron gas to be operating in the medium.The three terms $n, n^2$ and $\displaystyle \bigg({\frac {\partial n}{\partialx_k}}\bigg)$ where $n$ is photon phase density and $\displaystyle x_k=\bigg({\frac {h \nu} {k T_e}} \bigg) $, in Kompaneets equation and those due tofree-free emission are utilized to calculate the change in the photon phasedensity in a hot electron gas. Two types of incident radiation are considered:(1) isotropic radiation with the modified black body radiation $I^{MB}$ [1] and(2) anisotropic radiation which is angle dependent. The emergent radiation at$\tau=0$ and reflected radiation $\tau=\tau_{max}$ are calculated by using thediffuse radiation from the medium. The emergent and reflected radiation containthe free-free emission and emission from the hot electron gas. Kompaneetsequation gives the changes in photon phase densities in different types ofmedia. Although the initial spectrum is angle dependent, the Kompaneetsequation gives a spectrum which is angle independent after several Comptonscattering times.
机译:同时求解平面平行几何中的辐射传递方程和Kompaneets方程,获得1-125 KeVphoton能级范围的理论光谱。在平面平行几何中,使用与时间无关的辐射传递方程来计算扩散辐射场,该方程是使用离散空间理论(DST)在不均匀介质中针对不同光学深度的辐射传递来开发的。我们假定介质中存在自由电子的自由发射和吸收以及由于电子气体的发射。这三个术语$ n,n ^ 2 $和$ \ displaystyle \ bigg({\ frac {\ partial n} {\ partialx_k}} \ bigg)$,其中$ n $是光子相位密度,$ \ displaystyle x_k = \ bigg({\ frac {h \ nu} {k T_e}} \ bigg)$,在Kompaneets方程中以及由于自由发射引起的用于计算热电子气中光子相密度的变化。考虑了两种类型的入射辐射:(1)具有修改后的黑体辐射$ I ^ {MB} $ [1]的各向同性辐射;以及(2)与角度相关的各向异性辐射。通过使用来自介质的漫射辐射来计算出radiationtau = 0处的出射辐射和tau = tau_max的反射辐射。出射和反射的辐射包含自由发射和热电子气发射。 Kompaneets方程给出了不同类型介质中光子相密度的变化。尽管初始光谱是与角度相关的,但在几次康普顿散射时间后,Kompaneets方程给出的光谱与角度无关。

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