Simulations of cosmic-ray feedback by active galactic nuclei in galaxy clusters   总被引：1，自引：0，他引：1  

Debora Sijacki  Christoph Pfrommer  Volker Springel  Torsten A. Enßlin 《Monthly notices of the Royal Astronomical Society》2008,387(4):1403-1415

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Properties of vertically self-gravitating accretion discs with a dissipative corona     

Fazeleh Khajenabi  Peter Duffy 《Monthly notices of the Royal Astronomical Society》2008,388(4):1843-1852

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Dissipative accretion flows around a rotating black hole     

Santabrata Das  Sandip K. Chakrabarti 《Monthly notices of the Royal Astronomical Society》2008,389(1):371-378

We study the dynamical structure of a cooling dominated rotating accretion flow around a spinning black hole. We show that non-linear phenomena such as shock waves can be studied in terms of only three flow parameters, namely the specific energy     , the specific angular momentum (λ) and the accretion rate     of the flow. We present all possible accretion solutions. We find that a significant region of the parameter space in the     plane allows global accretion shock solutions. The effective area of the parameter space for which the Rankine–Hugoniot shocks are possible is maximum when the flow is dissipation-free. It decreases with the increase of cooling effects and finally disappears when the cooling is high enough. We show that shock forms further away when the black hole is rotating compared to the solution around a Schwarzschild black hole with identical flow parameters at a large distance. However, in a normalized sense, the flow parameters for which the shocks form around the rotating black holes are produced shocks closer to the black hole. The location of the shock is also dictated by the cooling efficiency in that higher the accretion rate     , the closer is the shock location. We believe that some of the high-frequency quasi-periodic oscillations may be due to the flows with higher accretion rate around the rotating black holes.  相似文献   

Calculation of the Intensity Ratio and Intrinsic Redshift Ratio of the Cerenkov Iron K_α and K_β Lines and Its Possible Application in the Study of AGNs     

Dang-bo Liu  Lei Chen  Jun-han You 《Chinese Astronomy and Astrophysics》2008

We have pointed out that, when thermal relativistic electrons with an isotropic velocity distribution move through a region of dense gas or impinge upon its surface, the Cerenkov effect will produce a particular kind of atomic or ionic emission line, which we have called the “Cerenkov line-like radiation”. This prediction for the optical wavebands has been verified by laboratory experiments. In this paper, we extend this line-like radiation theory to the X-ray waveband and give the basic formulae for calculating the intensity ratio and intrinsic redshift ratio of the Cerenkov iron K_α and K_β lines, for different ionization orders of iron. Potential application of this calculated result may be found in the study of AGNs. The recent observations of NGC3783 show that besides the iron K_α line at ∼6.4 keV, there is also a very strong iron Kβ line at ∼7.0 keV, and that the ratio of equivalent widths between the two is anomalous: EWK_α/EWK_β ≈ 3.43. It is difficult to explain this by the conventional mechanism of “photoelectric absorption-fluorescence emission”. We suggest that the mechanism of Cerenkov line-like radiation can provides a way of solving this puzzle. Besides, we expect that the calculated intrinsic redshift ratio of Cerenkov iron K_α and K_β lines could be tested in future observations. If our suggestion is further supported by observations, then our view on the physical environment around the central massive black hole of an AGN will be greatly modified: the activity becomes more energetic and violent, and the gas, much denser than previously thought.  相似文献   

考虑间歇充填和浓度效应的充填体长期强度试验研究     

曹帅  宋卫东  薛改利 《岩土力学》2018,39(Z1):341-347

为探究不同充填间隔时间(FTS)和料浆浓度对胶结充填体长期强度影响机制,配制70%、72%、75%三个浓度、充填间隔时间为12、24、36、48 h的两分层胶结充填体试件,开展单轴抗压强度(UCS)试验并探究其力学特性及其破坏形式。试验结果表明,（1）胶结充填体峰值抗压强度随充填间隔时间增大而呈递减趋势,充填间隔时间一定时胶结充填体抗压强度随料浆浓度增大而增大,且峰值抗压强度与充填间隔时间呈多项式函数规律;（2）胶结充填体试件加载过程中表现为压密阶段、线弹性阶段、裂纹扩展阶段和破坏发展4个阶段,随充填间隔时间延长,胶结充填体的破坏形式可能表现为张拉破坏–拉剪破坏过渡–拉剪混合破坏的损伤模式。研究结论能够为后期充填体强度设计和稳定性控制提供有益参考。  相似文献   

致密砂岩多期裂缝形成机制及定量表征研究进展     

孙志勇  陈开远  冯建伟  隋淑玲 《地质力学学报》2017,23(2):272-279

致密砂岩油气是重要的非常规资源,裂缝作为主要渗流通道,其本身分布规律的复杂性以及多期发育和多期充填的特征,直接影响着裂缝预测的精度,目前尚缺乏一套全面解决构造裂缝定量预测的系统方法。因此,需要深入探讨多期裂缝的识别、充填过程和形成—叠加演化机制,建立合理的裂缝表征模型,以定量预测裂缝参数分布范围。在大量文献调研的基础上,本文认为致密储层裂缝研究主要涉及三个关键方向:通过野外露头和岩心观察,分析裂缝发育特征,结合构造演化和流体包裹体分析,确定裂缝发育期次;通过热液充填模拟实验和岩石力学实验,揭示裂缝充填机制,及其在多期应力作用下裂缝的萌生、扩展和叠加过程;采用实验统计方法,基于能量守恒定理和最大应变能密度理论,建立考虑裂缝差异充填的各向异性强度破裂准则,建立裂缝参数的定量表征模型。最终,本文形成和完善了致密砂岩多期裂缝演化及量化表征的理论体系,为此类油气田的勘探开发提供重要科学依据。  相似文献   

砂砾石大坝填筑碾压的相关试验与研究          下载免费PDF全文

张朋辉  韩赛超  李晓帅  张小东 《探矿工程》2017,44(5):72-77

针对南疆砂砾石填筑大坝进行碾压试验,验证坝体填筑设计压实标准的合理性、检验22 t自行式振动碾的适用性及其性能的可靠性。本试验主要采用室内相对密度试验、现场的碾压测定出碾压遍数、碾压沉降及相应密实度及其他试验参数,通过试验参数列表、试验参数包络线图与设计标准值的比较,得出最佳砂砾石填筑方案,同时也确定大坝填筑时的施工碾压控制参数,从而确保了工程质量。  相似文献   

巨厚砂砾层裸孔钻进施工技术          下载免费PDF全文

殷宝兵  黄留新  张瑞琼 《探矿工程》2017,44(9):26-31

在江苏沿海地区进行城市地质及水文地质等区域性地质调查,主要的野外工作手段就是全孔取心岩心钻探,但江苏沿海地区沉积层厚度300～500 m不等,最深处800 m之多。在如此之深的巨厚沉积层中钻探取心、且取心率要求之高在江苏乃至全国没有先例。结合某钻孔的施工实例,从钻探设备的选择、施工工艺的确定、泥浆控制技术等方面入手,全面总结了江苏沿海地区巨厚砂砾层全孔取心施工技术,对类似钻探项目的实施具有很好的借鉴作用。  相似文献   

ADM6-4H井四开水平段钻井液技术          下载免费PDF全文

刘春明 《探矿工程》2017,44(8):51-54

ADM6-4H井是AHDEB油田使用常规随钻测量仪器（MWD）和螺杆动力钻具组合完成的一口水平段长度1500 m、最大水平位移1915.17 m的6 in小井眼大位移水平井,也是AHDEB油田目前水平位移最大的一口水平井。该井四开水平段钻进使用聚磺混油钻井液体系,在携砂、井眼稳定和润滑减阻等方面效果突出。四开水平段钻速快,钻进扭矩小,钻井液性能稳定,无井壁失稳,无漏失,无卡钻,无托压,其经验技术值得借鉴。  相似文献   

山东平邑石膏矿矿难大口径救援钻孔施工技术          下载免费PDF全文

杨涛  杜兵建 《探矿工程》2017,44(5):19-23

2015年“12.25”平邑矿难钻孔救援是我国首例通过钻孔救生的成功案例。由于地层不断坍塌变形,导致了复杂地层条件的产生,给救援钻孔的施工带来极大困难。针对这一特殊情况,采用空气反循环钻井工艺技术,处理钻孔事故时采用气举反循环工艺技术。总结了大口径钻孔施工经验,对今后施工大口径救援钻孔提出有待改进的问题和建议。  相似文献