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NUMERICAL STUDIES OF COSMIC-RAY INJECTION AND ACCELERATION

机译:宇宙射线注入与加速的数值研究

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A numerical scheme that incorporates a thermal leakage injection model into a combined gasdynamics and cosmic-ray (CR) diffusion-convection code has been developed. The hydro/CR code can follow in a very cost-effective way the evolution of CR-modified planar quasi-parallel shocks by adopting subzone shock tracking and multilevel adaptive mesh refinement techniques. An additional conservative quantity, S = P_g/ρ~(γg-1), is introduced to follow the adiabatic compression accurately in the precursor region, especially in front of strong, highly modified shocks. The "thermal leakage" injection model is based on the nonlinear interactions of the suprathermal particles with self-generated MHD waves in quasi-parallel shocks. The particle injection is followed numerically by filtering the diffusive flux of suprathermal particles across the shock to the upstream region according to a velocity-dependent transparency function that controls the fraction of leaking particles. This function is determined by a single parameter, e, which should depend on the strength of postshock wave turbulence but is modeled as a constant parameter in our simulations. We have studied CR injection and acceleration efficiencies during the evolution of CR-modified planar shocks for a wide range of initial shock Mach numbers, M_0, assuming a Bohm-like diffusion coefficient. For expected values of e the injection process is very efficient when the subshock is strong, leading to fast and significant modification of the shock structure. As the CR pressure increases, the subshock weakens and the injection rate decreases accordingly so that the subshock does not disappear. Although some fraction of the particles injected early in the evolution continue to be accelerated to ever higher energies, the postshock CR pressure reaches an approximate time-asymptotic value because of a balance between fresh injection/acceleration and advec-tion/diffusion of the CR particles away from the shock. In the strong shock limit of M_0 approx> 30, the injection and acceleration processes are largely independent of the initial shock Mach number for a given ε, while they are sensitively dependent on M_0 for M_0 < 30. We conclude that the injection rates in strong parallel shocks are sufficient to lead to rapid nonlinear modifications to the shock structures and that self-consistent injection and time-dependent simulations are crucial to understanding the nonlinear evolution of CR-modified shocks.
机译:已经开发了一种将热泄漏注入模型结合到组合的气体动力学和宇宙射线(CR)扩散对流代码中的数值方案。通过采用分区冲击追踪和多级自适应网格细化技术,hydro / CR代码可以非常经济高效地跟踪CR修改的平面准平行冲击的演变。引入了一个额外的保守量S = P_g /ρ〜(γg-1),以精确地跟随前体区域中的绝热压缩,尤其是在强烈的高度变化的冲击之前。 “热泄漏”注入模型基于准平行冲击中超热粒子与自生MHD波的非线性相互作用。在数值上进行粒子注入之后,根据速度相关的透明度函数(控制泄漏粒子的比例),过滤穿过冲击波到上游区域的超热粒子的扩散通量。该函数由单个参数e决定,该参数应取决于震后波湍流的强度,但在我们的模拟中被建模为恒定参数。我们已经研究了CR修饰的平面激波在各种初始激波马赫数M_0的演变过程中的CR注入和加速效率,并假设其具有类似Bohm的扩散系数。对于e的期望值,当子冲击很强时,喷射过程非常有效,从而导致冲击结构的快速显着改变。随着CR压力的增加,子冲击会减弱,喷射速率也会相应降低,因此子冲击不会消失。尽管在演化的早期注入的粒子中有一部分会继续加速到更高的能量,但是由于CR粒子的新鲜注入/加速与对流/扩散之间的平衡,震后的CR压力达到了近似的时间渐近值。远离震惊。在M_0大约> 30的强冲击极限下,对于给定的ε,注入和加速过程很大程度上与初始冲击马赫数无关,而对于M_0 <30而言,它们敏感地取决于M_0。平行冲击足以导致对冲击结构进行快速的非线性修改,而自洽的注入和时间相关的模拟对于理解CR修改的冲击的非线性演变至关重要。

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