黑洞自旋、噴流及基本面研究
發(fā)布時間:2018-06-08 05:12
本文選題:射電類星體 + 黑洞自旋; 參考:《云南師范大學(xué)》2016年碩士論文
【摘要】:本文對黑洞自旋射電噪類星體黑洞的質(zhì)量和自旋與噴流能量的相關(guān)性,Blazar黑洞自旋能量與紅移的相關(guān)性,射電類星體黑洞自旋與射電噪的相關(guān)性,黑洞吸積率與噴流能量的相關(guān)性,RLQ與XRB的基本面關(guān)系特性等一系列問題進(jìn)行了主要的研究。第一章,主要簡單的介紹了活動星系核的一些基本特性,例如活動星系核的分類和統(tǒng)一模型;活動星系核中心黑洞質(zhì)量及自旋的計(jì)算方法;第二章,噴流的形成與黑洞吸積之間存在很大的關(guān)系,分析黑洞吸積率與噴流能量的相關(guān)性有助于我們對研究黑洞內(nèi)部結(jié)構(gòu)以及噴流形成原因的研究。本章我們具體探討黑洞吸積率與噴流能量之間的相關(guān)性。為研究黑洞自旋與噴流的關(guān)系提供理論基礎(chǔ)。第三章,我們主要研究了Blazar黑洞的自旋能量與紅移之間的關(guān)系。黑洞噴流的產(chǎn)生與黑洞自旋密有著很大的關(guān)系。研究黑洞自旋和噴流之間的相關(guān)性對研究噴流的形成以及產(chǎn)生機(jī)制有著重要的意義。通過數(shù)據(jù)分析所得結(jié)果如下:(1)Blazar黑洞自旋在三種不同磁場條件下(B=BEDD,B=104G,B∝j)均與紅移存在線性相關(guān),在愛丁頓磁場條件下尤其明顯(B=BEDD);(2)FR II射電星系(RG),FR II射電噪類星體(RLQ),核占優(yōu)星系(CD)三種樣本的黑洞自旋能量與紅移的相關(guān)系數(shù)存在一定的差異;(3)黑洞自旋能量與紅移的強(qiáng)相關(guān)性說明,黑洞自旋能量在一定程度上反映出黑洞并合與吸積的信息;第四章,我們研究了射電類星體黑洞自旋與射電噪之間的關(guān)系。結(jié)果如下:(1)陡譜射電星類星體自旋在三種磁場條件下都存在(B=BEDD,B=104G,B∝j)均與射電噪存在明顯的相關(guān)性;(2)陡譜射電星類星體與射電噪之間的相關(guān)性并不受相對論聚束效應(yīng)的影響;(3)平譜射電類星體與射電噪之間不存在相關(guān)性,這說明黑洞自旋與射電噪之間的相關(guān)性與射電類星體的具體類型有一定的聯(lián)系;(4)陡譜射電星類星體的黑洞自旋和射電噪之間的強(qiáng)相關(guān)性表明,黑洞的自旋能量在某種程度上能反映出陡譜射電類星體射電噪度的信息。這個研究結(jié)果與其他人提出的理論相符。第五章,黑洞噴流的產(chǎn)生和黑洞的自旋之間有著很大的關(guān)系。黑洞自旋以及噴流之間的相關(guān)性對噴流的形成以及產(chǎn)生機(jī)制的研究有著重要的意義。本文中我們具體關(guān)注射電類星體黑洞質(zhì)量、自旋與其自身的噴流能量的相關(guān)性,以通過驗(yàn)證前人的理論來探討運(yùn)用新的黑洞自旋計(jì)算方法的可行性及可靠性。所得結(jié)論如下:(1)首先我們驗(yàn)證了射電類星體黑洞質(zhì)量與其噴流能量確實(shí)存在相關(guān)性與其他人所得的結(jié)果相同;(2)通過大數(shù)據(jù)統(tǒng)計(jì),我們發(fā)現(xiàn)射電類星體黑洞自旋與噴流能量之間存在線性相關(guān);(3)陡譜射電類星體所得到的自旋數(shù)據(jù)與平譜射電類星體存在一定的差異。(4)研究結(jié)果進(jìn)一步表明了噴流能量很可能像黑洞質(zhì)量一樣能夠?qū)诙吹淖孕芰康拇笮‘a(chǎn)生影響。黑洞噴流的形成很可能是黑洞質(zhì)量與黑洞自旋共同作用的結(jié)果。研究結(jié)果與先前其他人提出的理論猜想一致。第六章,我們RLQ與XRB的基本面關(guān)系。在很多低/硬態(tài)X射線雙星系統(tǒng)中(XRB),射電和X射線之間都存在較好的相關(guān)關(guān)系。DongAi-Jun以Saikia都通過研究得出了射電靜類星體(RQQ)也存在著這一關(guān)系,并且其關(guān)系式與低/硬態(tài)X射線雙星的基本關(guān)系有著一定的相似度。分析結(jié)果表明:(1)255個射電噪類星體(RLQ)的黑洞質(zhì)量與X射線和射電光度之間以及射電光度愛丁頓比率和X射線愛丁頓比率之間均存在相關(guān)性,這與DongAi-Jun等運(yùn)用亮硬態(tài)黑洞雙星和射電噪類星體所得出的基本關(guān)系式有一定的相似性但仍然存在一定差異;(2)低/硬態(tài)X射線雙星與射電噪類星體的基本關(guān)系式可統(tǒng)一logLR0.998.logLX0.592.logMBH6.56.;(3)研究結(jié)果進(jìn)一步證明了由X射線和射電光度都與質(zhì)量所構(gòu)成的黑洞活動基本關(guān)系式具有高度的統(tǒng)一性,不僅可用于描述于低/硬態(tài)X射線雙星系統(tǒng)和射電靜類星體,同樣可作用于射電噪類星樣體。
[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.
【學(xué)位授予單位】:云南師范大學(xué)
【學(xué)位級別】:碩士
【學(xué)位授予年份】:2016
【分類號】:P145.8
【參考文獻(xiàn)】
相關(guān)期刊論文 前4條
1 張旭;張雄;;黑洞吸積率與噴流能量相關(guān)性討論[J];天文研究與技術(shù);2016年01期
2 張旭;張皓晶;張雄;;射電噪類星體黑洞的質(zhì)量和自旋與噴流能量的相關(guān)性[J];天文學(xué)報;2015年05期
3 張旭;張雄;;Blazar黑洞自旋能量與紅移相關(guān)性研究[J];天文研究與技術(shù);2015年03期
4 張旭;張雄;;射電類星體黑洞自旋與射電噪相關(guān)性研究[J];天文研究與技術(shù);2015年04期
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