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1.
随机分布烟尘团簇粒子辐射特性研究   总被引:3,自引:0,他引:3       下载免费PDF全文
类成新  吴振森 《物理学报》2010,59(8):5692-5699
基于分形理论,采用蒙特卡罗方法对随机分布的烟尘团簇粒子结构进行了仿真模拟,利用离散偶极子近似(discrete dipole approximation, DDA)方法研究了随机分布的烟尘团簇粒子的辐射特性,分析讨论了分形维数、原始微粒粒径和数量以及复折射率对随机分布烟尘团簇粒子辐射特性的影响.研究表明,在给定分形维数的情况下,烟尘团簇粒子的辐射特性取决于原始微粒粒径、数量及复折射率;原始微粒较小的团簇粒子,当分形维数较小时,吸收截面变化不明显,但当分形维数大于2时,吸收截面骤然增大,然而,对于具有比较大的原始微粒粒径、数量及复折射率的烟尘团簇粒子,吸收截面随着分形维数的增大而单调递减;随着分形维数的增大,团簇粒子的散射截面、消光截面及单次散射反照率均单调递增;从整体上来讲,团簇粒子的辐射特性与等效球形粒子的辐射特性存在着比较大的差别,并且这种差别随着分形维数的增大而减小.该工作对研究气溶胶粒子的辐射及气候效应具有重要的科学价值. 关键词: 烟尘团簇粒子 辐射特性 离散偶极子近似方法  相似文献   

2.
赵仁  张丽春  李怀繁 《物理学报》2010,59(5):2982-2986
运用Damour-Ruffini方法研究Kerr-Newman黑洞粒子的Hawking辐射.在保持时空中总能量,总角动量和总电荷守恒的条件下,考虑辐射粒子对时空的反作用后,得到黑洞辐射谱不再是严格的纯热谱.在该结论中,不但含有辐射粒子能量的影响项,而且含有辐射粒子角动量对黑洞角动量的影响项.所给表达式与用隧穿方法得到的表达式一致.满足量子力学的幺正性原理.  相似文献   

3.
杨维 《物理学报》2023,(1):43-47
由于SL(n,R)户田黑洞具有很好的数学结构,是研究黑洞物理较为理想的场所.本文主要研究其黑洞的霍金辐射,以及相关信息丢失问题.为了简单,只考虑在四维静态球对称SL(n,R)户田黑洞下,通过计算静止质量为零的粒子在事件视界附近隧穿效应来研究霍金辐射.在粒子的隧穿过程中,利用能量守恒并考虑了隧穿粒子对背景时空的反作用.获得粒子通过事件视界的隧穿概率取决于粒子出射前后黑洞熵的变化,并在此基础上讨论了其信息丢失问题,在满足一定条件下,我们的结果与RN黑洞和施瓦茨黑洞的结果一致.  相似文献   

4.
吕景发 《物理学报》1965,21(5):1049-1060
本文在各向异性介质中电磁场二次量子化的基础上,探讨做高匀速运动(超过该介质中的光速)的带电粒子辐射状况,得到了寻常波和非常波辐射强度的表达式,解释了粒子的自旋状态对辐射强度的影响。在粒子的运动方向沿晶体光轴和垂直于晶体光轴的两种情况下,对结果进行了分析。结果表明,量子方法的计算有别于经典结果,当考虑到粒子自旋时,在沿光轴这动的情况下,既辐射寻常波又辐射非常波。  相似文献   

5.
利用部分波展开法求解得到了Gauss声束入射下刚性和非刚性椭圆柱的声散射系数,推导了一般情况下的声辐射力矩表达式.在此基础上,通过一系列数值仿真详细分析了离轴距离、入射角度和束腰半径对声辐射力矩的影响.结果表明:正向与负向声辐射力矩均可以在一定条件下存在;低频情况下刚性椭圆柱比非刚性椭圆柱更容易产生较强的声辐射力矩;特定频率的入射声场可以激发出非刚性椭圆柱不同阶的共振散射模式,因而非刚性椭圆柱的声辐射力矩峰值与频率的关系更密切;增加束腰半径有利于扩大散射截面,进而增加椭圆柱的声辐射力矩.该研究结果预期可以为利用声辐射力矩实现粒子的可控旋转和流体黏度的反演提供一定的理论指导.  相似文献   

6.
 为开发回旋超辐射在毫米波和亚毫米波超辐射高功率微波源中的优势,采用3维PIC粒子模拟对回旋超辐射的工作特性进行了分析,并在此基础上优化设计了器件结构及工作参数范围。模拟表明,微波峰值功率与电子束脉宽在一定范围内成平方关系,符合超辐射的典型特征。初步实验在210 kV, 250 A的电子束参数下获得了6 MW的微波峰值功率输出,工作频率37.2 GHz,模式为TE01,与粒子模拟的结果基本一致。  相似文献   

7.
设计了一种基于超辐射机理的X波段相对论返波管结构, 利用全电磁2.5维粒子模拟程序对返波管中的超辐射机理进行了粒子模拟研究. 模拟表明: 在束430kV、束流4kA, 脉宽3.1ns的电子束驱动下,实现了峰值功率1.5GW、频率10GHz、脉宽500ps的亚纳秒微波脉冲输出, 峰值功率转换效率达到87.2%;在超辐射机理作用下, 微波峰值功率与电子束脉宽在一定的范围内成平方关系.  相似文献   

8.
赵仁  张丽春  胡双启 《物理学报》2006,55(8):3902-3905
运用量子统计的方法,直接求解Schwarzschild时空背景下玻色场和费米场的配分函数,得到熵的积分表达式.按照最近的研究结果,认为黑洞的Hawking辐射过程是隧道效应过程,在考虑黑洞隧道效应产生过程中黑洞能量发生变化的基础上,给出积分的下限为黑洞的视界位置.由此得到黑洞熵的主要项为视界面积的1/4.不存在使人疑惑的紫外截断因子,并且由此可得黑洞辐射粒子的能量与辐射温度成正比的结论. 关键词: 黑洞熵 量子统计 隧道效应 反作用  相似文献   

9.
吴济民 《中国物理 C》1993,17(2):146-151
利用我们曾经解析求得的电子、正电子分布函数的表达式,我们求得了e+e对撞过程中辐射因子的严格的解析表达式.这一级数表达式可以很快地收敛到所要求的精度.本文也给出了与现有的近似结果的比较.本文结果十分有益于精确计算e+e对撞过程中的辐射修正.  相似文献   

10.
基于Thomas-Fermi半经典近似研究了谐振子势阱约束下任意维理想玻色气体的玻色-爱因斯坦凝聚(BEC).导出了玻色气体的BEC转变温度、基态粒子占据比例、内能和热容量等物理量的解析表达式,讨论了空间维度和谐振子势阱的影响.以二维和三维玻色系统为例,数值计算了上述热力学量,并与解析结果进行了对比,二者获得了较好的吻合.  相似文献   

11.
Thermal radiation of electrically charged fermions from a rotating black hole with electric and magnetic charges in de Sitter space is considered. The tunneling probabilities for outgoing and incoming particles are obtained and the Hawking temperature is calculated. The relation for the classical action for the particles in the black hole’s background is also found.  相似文献   

12.
We study Hawking radiation of charged fermions as a tunneling process from charged regular black holes, i.e., the Bardeen and ABGB black holes. For this purpose, we apply the semiclassical WKB approximation to the general covariant Dirac equation for charged particles and evaluate the tunneling probabilities. We recover the Hawking temperature corresponding to these charged regular black holes. Further, we consider the back-reaction effects of the emitted spin particles from black holes and calculate their corresponding quantum corrections to the radiation spectrum. We find that this radiation spectrum is not purely thermal due to the energy and charge conservation but has some corrections. In the absence of charge, e = 0, our results are consistent with those already present in the literature.  相似文献   

13.
Physical limits on the amount of information carried by bandlimited waveforms radiated in one and three dimensions are considered. It is shown that the entropy of radiation can achieve the Bekenstein bound using a “burst” of energy, whose density vanishes as the radiating system expands. In comparison, black body radiation of infinite bandwidth achieves the same entropy scaling, that is proportional to the volume of the space, but requires an energy density that remains constant as the system expands. Rather than following the standard statistical physics approach of counting the number of eigenstates of the Hamiltonian of the quantum wave field, our derivation first considers an optimal subspace approximation, and then determines the number of bits that are required to represent any waveform in the space spanned by this representation with a minimum quantized energy error. This favors a geometric interpretation where the complexity of state counting is replaced by the one of determining the minimum cardinality covering of the signal space by high-dimensional balls, or boxes, whose size is lower bounded by quantum constraints. All derivations are given for both deterministic and stochastic settings.  相似文献   

14.
郑利娟  程天海  吴俣 《物理学报》2017,66(16):169201-169201
黑碳气溶胶是当前气溶胶辐射强迫评估中最不确定的因子.本文通过构建黑碳的微物理模型,分别模拟了新鲜状态的黑碳气溶胶和混合生长(老化)后被硫酸盐包裹的黑碳气溶胶,利用叠加T矩阵方法计算获得了具有团簇形态和多成分混合的黑碳气溶胶红外吸收特性,通过大气辐射传输模型模拟了黑碳气溶胶的长波辐射强迫,分析了典型理化参数的敏感性.发现黑碳混合生长可以显著增强其大气层顶的长波辐射强迫,最高可达3倍.而且,包裹黑碳的硫酸盐半径越大,将明显增强大气层顶的黑碳长波辐射强迫.这些发现将有助于降低黑碳气溶胶气候效应评估的不确定性.  相似文献   

15.
Using Damour-Ruffini method, Hawking radiation of rotating black strings is studied. Under the condition that the total energy, total angular momentum and total charge are conservative, the transition probability from initial state (energy M+ω, charge Q+e and angular momentum J+m) to final state (energy M, charge Q and angular momentum J) for black strings is derived considering the reaction of radiation particles to spacetime. That is, the probability that black strings radiate particles with energy ω, charge e and angular momentum m is obtained. The real spectrum is not a strictly pure thermal spectrum. Our result is consistent with Parikh and Wilczek’s result. It satisfies the unitary principle of quantum mechanics. However, in our result there are not only the term that denotes effect of energy and charge of radiation particles but also the term that denotes effect of radiation particles angular momentum on rotating black strings angular momentum. We provide a new way for investigating radiation of black strings.  相似文献   

16.
Recent research shows that the WKB approximation and the Hamilton-Jacobi method has been succeed in studying the tunneling radiation of vector particles. In view of this, our main aim in this letter is to study the Proca equation and the vector particles tunneling radiation in the 4-dimensional and 5-dimensional black holes. And finally, the results here show that the temperature of vector particle is the same as Dirac particle’s and other particle’s.  相似文献   

17.
The nonthermal radiation of a Kerr black hole is considered as the tunneling of particles being produced through an effective Dirac gap. In the leading semiclassical approximation, this approach is also applicable to bosons. Our semiclassical results for photons and gravitons are consistent with those obtained previously. For neutrinos, the result of our complete quantum-mechanical calculation is about twice as large as the previous one.  相似文献   

18.
According to Parikh's recent work, Hawking radiation is viewed as a tunneling process and the barrier is created just by the outgoing particle itself. In this paper, we extend Parikh's work to the case of massive particles' tunneling, and calculate the emission rate at which massive particles tunnel across the event horizon of an arbitrarily dimensional Schwarzschild black hole. The result is also consistent with an underlying unitary theory and takes the same functional form as that of massless particles. Moreover, our result also shows that Hawking radiation is an intrinstic property of the black hole.  相似文献   

19.
In the difference formulation for the transport of thermally emitted photons the photon intensity is defined relative to a reference field, the black body at the local material temperature. This choice of reference field combines the separate emission and absorption terms that nearly cancel, thereby removing the dominant cause of noise in the Monte Carlo solution of thick systems, but introduces time and space derivative source terms that cannot be determined until the end of the time step. The space derivative source term can also lead to noise induced crashes under certain conditions where the real physical photon intensity differs strongly from a black body at the local material temperature.In this paper, we consider a difference formulation relative to the material temperature at the beginning of the time step, or in cases where an alternative temperature better describes the radiation field, that temperature. The result is a method where iterative solution of the material energy equation is efficient and noise induced crashes are avoided. We couple our generalized reference field scheme with an ad hoc interpolation of the space derivative source, resulting in an algorithm that produces the correct flux between zones as the physical system approaches the thick limit.  相似文献   

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