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黑洞自旋、喷流及基本面研究

发布时间:2018-06-08 05:12

  本文选题:射电类星体 + 黑洞自旋 ; 参考:《云南师范大学》2016年硕士论文


【摘要】:本文对黑洞自旋射电噪类星体黑洞的质量和自旋与喷流能量的相关性,Blazar黑洞自旋能量与红移的相关性,射电类星体黑洞自旋与射电噪的相关性,黑洞吸积率与喷流能量的相关性,RLQ与XRB的基本面关系特性等一系列问题进行了主要的研究。第一章,主要简单的介绍了活动星系核的一些基本特性,例如活动星系核的分类和统一模型;活动星系核中心黑洞质量及自旋的计算方法;第二章,喷流的形成与黑洞吸积之间存在很大的关系,分析黑洞吸积率与喷流能量的相关性有助于我们对研究黑洞内部结构以及喷流形成原因的研究。本章我们具体探讨黑洞吸积率与喷流能量之间的相关性。为研究黑洞自旋与喷流的关系提供理论基础。第三章,我们主要研究了Blazar黑洞的自旋能量与红移之间的关系。黑洞喷流的产生与黑洞自旋密有着很大的关系。研究黑洞自旋和喷流之间的相关性对研究喷流的形成以及产生机制有着重要的意义。通过数据分析所得结果如下:(1)Blazar黑洞自旋在三种不同磁场条件下(B=BEDD,B=104G,B∝j)均与红移存在线性相关,在爱丁顿磁场条件下尤其明显(B=BEDD);(2)FR II射电星系(RG),FR II射电噪类星体(RLQ),核占优星系(CD)三种样本的黑洞自旋能量与红移的相关系数存在一定的差异;(3)黑洞自旋能量与红移的强相关性说明,黑洞自旋能量在一定程度上反映出黑洞并合与吸积的信息;第四章,我们研究了射电类星体黑洞自旋与射电噪之间的关系。结果如下:(1)陡谱射电星类星体自旋在三种磁场条件下都存在(B=BEDD,B=104G,B∝j)均与射电噪存在明显的相关性;(2)陡谱射电星类星体与射电噪之间的相关性并不受相对论聚束效应的影响;(3)平谱射电类星体与射电噪之间不存在相关性,这说明黑洞自旋与射电噪之间的相关性与射电类星体的具体类型有一定的联系;(4)陡谱射电星类星体的黑洞自旋和射电噪之间的强相关性表明,黑洞的自旋能量在某种程度上能反映出陡谱射电类星体射电噪度的信息。这个研究结果与其他人提出的理论相符。第五章,黑洞喷流的产生和黑洞的自旋之间有着很大的关系。黑洞自旋以及喷流之间的相关性对喷流的形成以及产生机制的研究有着重要的意义。本文中我们具体关注射电类星体黑洞质量、自旋与其自身的喷流能量的相关性,以通过验证前人的理论来探讨运用新的黑洞自旋计算方法的可行性及可靠性。所得结论如下:(1)首先我们验证了射电类星体黑洞质量与其喷流能量确实存在相关性与其他人所得的结果相同;(2)通过大数据统计,我们发现射电类星体黑洞自旋与喷流能量之间存在线性相关;(3)陡谱射电类星体所得到的自旋数据与平谱射电类星体存在一定的差异。(4)研究结果进一步表明了喷流能量很可能像黑洞质量一样能够对黑洞的自旋能量的大小产生影响。黑洞喷流的形成很可能是黑洞质量与黑洞自旋共同作用的结果。研究结果与先前其他人提出的理论猜想一致。第六章,我们RLQ与XRB的基本面关系。在很多低/硬态X射线双星系统中(XRB),射电和X射线之间都存在较好的相关关系。DongAi-Jun以Saikia都通过研究得出了射电静类星体(RQQ)也存在着这一关系,并且其关系式与低/硬态X射线双星的基本关系有着一定的相似度。分析结果表明:(1)255个射电噪类星体(RLQ)的黑洞质量与X射线和射电光度之间以及射电光度爱丁顿比率和X射线爱丁顿比率之间均存在相关性,这与DongAi-Jun等运用亮硬态黑洞双星和射电噪类星体所得出的基本关系式有一定的相似性但仍然存在一定差异;(2)低/硬态X射线双星与射电噪类星体的基本关系式可统一logLR0.998.logLX0.592.logMBH6.56.;(3)研究结果进一步证明了由X射线和射电光度都与质量所构成的黑洞活动基本关系式具有高度的统一性,不仅可用于描述于低/硬态X射线双星系统和射电静类星体,同样可作用于射电噪类星样体。
[Abstract]:The correlation between spin and jet energy, the correlation between spin energy and red shift of Blazar black hole, the correlation between black hole spin and radio noise, the correlation of the black hole accretion rate and the jet energy, the relationship between the black hole accretion rate and the jet energy, the relationship between the RLQ and the base surface of the XRB are mainly discussed in this paper. The first chapter briefly introduces some basic characteristics of active galactic nuclei, such as the classification and unified model of active galactic nuclei, the method of calculating the mass and spin of the black hole in the center of active galactic nuclei; the second chapter, there is a great relationship between the formation of the jet and the accretion of the black hole, and the correlation between the accretion rate of the black hole and the energy of the jet. In this chapter, we discuss the correlation between the black hole accretion rate and the jet energy. In this chapter, we provide a theoretical basis for the study of the relationship between the spin and jet flow of black holes. In the third chapter, we mainly study the relationship between the spin energy and the red shift of the Blazar black hole. The formation of the spins of the black hole has a great relationship with the spin density of the black hole. It is important to study the correlation between the spin and the jet of the black hole to study the formation and mechanism of the jet. The results of the data analysis are as follows: (1) the spin of the Blazar black hole is linear with the red shift in the three different magnetic fields (B=104G, B, J). Correlation, especially in the Eddington magnetic field (B=BEDD); (2) FR II radio galaxy (RG), FR II radio noise quasar (RLQ), and nuclear dominant Galaxy (CD), the correlation coefficient between the spin energy and the red shift of the black hole is different. (3) the strong correlation between the black hole self spin energy and the red shift indicates that the spin energy of the black hole is to a certain extent. In the fourth chapter, we study the relationship between the spin and radio noise of a radio quasar black hole. The results are as follows: (1) there is a significant correlation between the quasar spin in the three kinds of magnetic fields (B=BEDD, B=104G, B J); (2) the quasar and radio noise of the steepest radio stars. The correlation is not influenced by the relativistic bunching effect; (3) there is no correlation between the plane radio quasars and the radio noise, which shows that the correlation between the black hole spin and the radio noise is related to the specific types of the radio quasars; (4) the strong correlation table between the spin and the radio noise of the steepar quasars. It is clear that the spin energy of the black hole can reflect the radio noise of the steepest radio quasars to some extent. The result of this study is in accordance with the theory proposed by other people. In the fifth chapter, there is a great relationship between the production of black hole jet and the spin of the black hole. The spin and the correlation between the black hole and the jet flow are formed and produced. The study of the mechanism is of great significance. In this paper, we pay close attention to the correlation between the mass of the black hole of the radio quasar and its own jet energy, so as to verify the feasibility and reliability of the new method of spin calculation using the new black hole by verifying the predecessors' Theory. The conclusions are as follows: (1) first we verified the radio quasar black. The correlation between the mass of the cavity and the energy of the jet is the same as that of other people. (2) we found that there is a linear correlation between the spin and the jet energy of the radio quasar. (3) there is a certain difference between the spin data obtained by the steepest radio quasars and the flat spectral radio quasars. (4) the results of the study are advanced. One step shows that the jet energy is likely to affect the size of the spin energy of a black hole like the mass of a black hole. The formation of the black hole jet is likely to be the result of the joint effect of the mass of the black hole and the spin of the black hole. The results are in accordance with the previous theoretical conjectures. The sixth chapter, the fundamental relation between our RLQ and XRB. In the multi low / hard X ray binary system (XRB), there is a good correlation between radio and X rays..DongAi-Jun has been found to have this relationship with Saikia through the study of Saikia, and its relation has a certain similarity with the basic system of low / hard X ray binary stars. The analysis results show that: (1) 255 There is a correlation between the mass of the black hole of the radio noise quasar (RLQ) and the X ray and the radio luminosity, the radio photometric Eddington ratio and the Eddington ratio of X ray, which is similar to the basic relationship between the black black black hole double star and the radio noise quasar, but still has certain differences; (2) The basic relationship between the low / hard X ray binary stars and the radio noise quasars can be unified logLR0.998.logLX0.592.logMBH6.56.. (3) the result of the study further proves that the basic relation of the black hole activity, which is composed of X ray and radio luminosity, is highly unified, and can be used not only to describe the low / hard X ray double star system and to shoot it. The electrostatic quasar also acts on the radio noise star like body.
【学位授予单位】:云南师范大学
【学位级别】:硕士
【学位授予年份】:2016
【分类号】:P145.8

【参考文献】

相关期刊论文 前4条

1 张旭;张雄;;黑洞吸积率与喷流能量相关性讨论[J];天文研究与技术;2016年01期

2 张旭;张皓晶;张雄;;射电噪类星体黑洞的质量和自旋与喷流能量的相关性[J];天文学报;2015年05期

3 张旭;张雄;;Blazar黑洞自旋能量与红移相关性研究[J];天文研究与技术;2015年03期

4 张旭;张雄;;射电类星体黑洞自旋与射电噪相关性研究[J];天文研究与技术;2015年04期



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