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Spin-star environment assisted entanglement generation in weakly coupled bipartite systems
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作者 王艮芳 吕建美 王林成 《Chinese Physics B》 SCIE EI CAS CSCD 2014年第5期107-112,共6页
We study the entanglement evolution in a weakly coupled bipartite system with a large energy level difference under the influence of spin-star environments. The subsystems can be coupled to a pure state or a thermal e... We study the entanglement evolution in a weakly coupled bipartite system with a large energy level difference under the influence of spin-star environments. The subsystems can be coupled to a pure state or a thermal equilibrium state spin-star environment. Our results show that, in the case of the coupling strength being less than the energy level difference of the subsystems (weakly coupled), the spin-star environment can always be used to assist the entanglement generation of the bipartite system. 展开更多
关键词 ENTANGLEMENT spin-star environment weakly coupled system
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夸克物质中的超子整体极化与矢量介子自旋排列 被引量:4
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作者 阮丽娟 许长补 杨驰 《物理学报》 SCIE EI CAS CSCD 北大核心 2023年第11期13-18,共6页
相对论重离子对撞机RHIC上超子整体极化和矢量介子自旋排列的实验发现证实了近20年前提出的理论.该理论预言和实验测量开辟了一种从自旋这个新的自由度来研究高能重离子碰撞中产生的高温高密核物质特性的新途径.本文简略回顾了整体极化... 相对论重离子对撞机RHIC上超子整体极化和矢量介子自旋排列的实验发现证实了近20年前提出的理论.该理论预言和实验测量开辟了一种从自旋这个新的自由度来研究高能重离子碰撞中产生的高温高密核物质特性的新途径.本文简略回顾了整体极化理论提出和实验发现,总结了现有大科学装置上的相关测量进展,以及国际上现有的多种理论解释.同时,简要介绍了STAR探测器近期升级所带来的物理机遇. 展开更多
关键词 相对论重离子对撞机 螺线管径迹谱仪 超子整体极化 矢量介子自旋排列
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功能磁共振成像在胶质瘤精确诊断中的研究 被引量:3
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作者 王巍 孙鹏 +4 位作者 刘妍姝 李露露 刘志兰 张原理 张毓婧 《实用肿瘤学杂志》 CAS 2017年第6期524-527,共4页
目的应用多种功能磁共振成像对胶质瘤进行评估,术前对脑胶质瘤进行较精准的诊断。方法收集35例经病理诊断证实的胶质瘤患者,均行常规磁共振成像(Magnetic resonance imaging,MRI)及功能MRI检查,对体素内不相干运动扩散加权成像(Intravox... 目的应用多种功能磁共振成像对胶质瘤进行评估,术前对脑胶质瘤进行较精准的诊断。方法收集35例经病理诊断证实的胶质瘤患者,均行常规磁共振成像(Magnetic resonance imaging,MRI)及功能MRI检查,对体素内不相干运动扩散加权成像(Intravoxel incoherent motion diffusion weighted imaging,IVIM-DWI)中快速扩散系数(D*)、慢扩散系数(D)、灌注分数(f)和分布扩散系数(DDC)的值进行统计学分析。结果高级别胶质瘤患者病灶侧IVIM的D、D*、DDC值较对侧正常脑白质增高(D:0.71±0.05×10^(-3)mm^2/s vs.0.14±0.03×10^(-3)mm^2/s;D*:0.06±0.04 mm^2/s vs.0.03±0.02 mm^2/s;DDC:1.29±0.33×10^(-3)mm^2/s vs.0.43±0.14×10^(-3)mm^2/s)、f值较对侧正常脑白质降低(f:0.41±0.11vs.0.51±0.05),差异均具有统计学意义(P<0.05)。结论多种磁共振功能成像序列协同分析胶质瘤,可以避免肿瘤的异质性,显著提高了磁共振检查对高级别脑胶质瘤实性部分的识别能力及精确性。 展开更多
关键词 胶质瘤 磁共振成像 体素内不相干运动 三维增强梯度回波T2*血管成像序列 动脉自旋标记灌注成像
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挠率探测物理的判据
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作者 张承民 《河北工业大学学报》 CAS 1993年第3期39-42,共4页
挠率的两个源被研究—宏观转动和排列自旋。在狄拉克粒子作为直接对挠率探测者的情况下,挠率自旋效应受到背景的强烈影响,这些背景是磁自旋作用,转动自旋作用和引力自旋作用。增加挠率等价于增加背景本身,首次给出的挠率探测判据是,除... 挠率的两个源被研究—宏观转动和排列自旋。在狄拉克粒子作为直接对挠率探测者的情况下,挠率自旋效应受到背景的强烈影响,这些背景是磁自旋作用,转动自旋作用和引力自旋作用。增加挠率等价于增加背景本身,首次给出的挠率探测判据是,除了中子星,在任何星内或星外实验,都没有希望给出挠率的直接甚至间接证据。有希望的挠率证据一定是在致密星体上的间接和积累结果。宏观转动粒子作为挠率间接探测者在目前进行的任何实验都不能给出挠率的迹像。 展开更多
关键词 引力理论 规范引力 挠率 自旋粒子 星体
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一种基于连续星图观测的自旋姿态估计方法 被引量:3
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作者 宁晓琳 白鑫贝 姜丽伟 《中国空间科学技术》 CSCD 北大核心 2013年第6期49-57,共9页
传统的利用地球敏感器和太阳敏感器作为测量仪器的自旋卫星姿态确定方法存在系统误差和安装误差等,从而导致自旋姿态确定误差较大的问题,文章提出了一种利用星敏感器获取的连续星图估计卫星自旋姿态参数的新方法。该方法以卫星的自旋轴... 传统的利用地球敏感器和太阳敏感器作为测量仪器的自旋卫星姿态确定方法存在系统误差和安装误差等,从而导致自旋姿态确定误差较大的问题,文章提出了一种利用星敏感器获取的连续星图估计卫星自旋姿态参数的新方法。该方法以卫星的自旋轴和旋转角速度作为状态变量,通过星敏感器连续跟踪拍摄的恒星的成像位置作为观测量,利用无迹卡尔曼滤波估计出卫星的自旋姿态参数。仿真结果表明,在星敏感器的精度为3″时,该方法的自旋轴估计精度为0.344 8″,自旋角速度估计精度为10-4(°)/s数量级。 展开更多
关键词 自旋卫星 星图观测 无迹卡尔曼滤波 星敏感器 姿态估计
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估算有中子星作伴星的黑洞质量
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作者 王学明 谢光中 张有宏 《云南天文台台刊》 CSCD 1995年第2期48-53,共6页
在本文中,我们讨论了由中子星和黑洞构成的密近双星系统的引力效应。首先,我们清楚地解释了引力辐射存在引起的轨道圆化,并估算了圆化的时间尺度。求解了围绕史瓦西黑洞作圆轨道运动的矢量进动方程,得到了一个精确解。由进动周期和... 在本文中,我们讨论了由中子星和黑洞构成的密近双星系统的引力效应。首先,我们清楚地解释了引力辐射存在引起的轨道圆化,并估算了圆化的时间尺度。求解了围绕史瓦西黑洞作圆轨道运动的矢量进动方程,得到了一个精确解。由进动周期和中心黑洞的质量的关系,我们得到了估算中子星伴随的黑洞质量的方法。随后我们讨论了以中子星脉冲信号随自旋进动变化来寻找黑洞的方法。 展开更多
关键词 密近双星 黑洞 中子星 自旋进动 引力辐射
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不同压强条件下环锭旋流喷嘴内部流场模拟
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作者 初曦 邱华 《纺织学报》 EI CAS CSCD 北大核心 2020年第9期33-38,共6页
为探究在不同环锭旋流喷嘴气道入口压强条件下喷嘴内部的流场分布规律,借助STAR-CCM+与ANSYS CFX流体分析软件建立旋流喷嘴模型并进行数值模拟分析,得到在纺纱过程中旋流喷嘴内部气流的速度和压力分布云图。结果表明:空气通入气道入口... 为探究在不同环锭旋流喷嘴气道入口压强条件下喷嘴内部的流场分布规律,借助STAR-CCM+与ANSYS CFX流体分析软件建立旋流喷嘴模型并进行数值模拟分析,得到在纺纱过程中旋流喷嘴内部气流的速度和压力分布云图。结果表明:空气通入气道入口的流动机制遵循涡流效应,以旋流状向纱道两端流出,向两侧流出的旋流可对纱线进行轻微解捻和毛羽的进一步贴服;喷嘴内部流场对比示意图表明入口压强对纱线受力的分布并无影响,但气流压强波动幅度随入口压强的增大而增大,波动幅度越大越利于毛羽的包裹,对纤维束的包裹作用也更强烈,但过大的气流压强会造成更多纤维的流失。 展开更多
关键词 旋流喷嘴 数值模拟 毛羽 气流场 STAR-CCM+ 纺纱
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A key factor to the spin parameter of uniformly rotating compact stars: crust structure
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作者 Bin Qi Nai-Bo Zhang +2 位作者 Bao-Yuan Sun Shou-Yu Wang Jian-Hua Gao 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2016年第4期63-70,共8页
We study the dimensionless spin parameter j ≡ cJ/(GM2) of different kinds of uniformly rotating compact stars, including traditional neutron stars, hyperonic neutron stars and hybrid stars, based on relativistic me... We study the dimensionless spin parameter j ≡ cJ/(GM2) of different kinds of uniformly rotating compact stars, including traditional neutron stars, hyperonic neutron stars and hybrid stars, based on relativistic mean field theory and the MIT bag model. It is found that j ~ 0.7, which had been suggested in traditional neutron stars, is sustained for hyperonic neutron stars and hybrid stars with M 〉 0.5 MG. Not the interior but rather the crust structure of the stars is a key factor to determine jmax for three kinds of selected compact stars. Furthermore, a universal formula j = 0.63(f/fK) -- 0.42(f/fK)2 + 0.48(f/fK)z is suggested to determine the spin parameter at any rotational frequency f smaller than the Keplerian frequency fK. 展开更多
关键词 stars: neutron -- stars: rotation -- spin parameter-- equation of state -- methods: numerical
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Star Grain Regression Analysis under Spin Effect and Chamber Pressure Effect 被引量:1
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作者 SOE Hlaing Tun 《Computer Aided Drafting,Design and Manufacturing》 2010年第2期54-58,共5页
The angular acceleration due to the spin effect increases the burning rate of solid propellant and changes the motor performance by increasing the operating pressure and decreasing the burning time. So it is important... The angular acceleration due to the spin effect increases the burning rate of solid propellant and changes the motor performance by increasing the operating pressure and decreasing the burning time. So it is important to know the grain regression taken place in the solid propellant rocket motor in the acceleration field. This study represents the grain regression analysis of two-dimensional axis-symmetric star grain configuration of the solid propellant rocket motor with spin induced acceleration effect and pressure effect on burn rate using geometrical and numerical analysis. While the rocket is spinning, the burn rates on each point of the propellant surface are different with its radial distance, acceleration vector angle and surface slope. With the different burn rates on the propellant surface, we analyze the propellant surface perimeter and port area, and these results are compared with those of constant burn rate and burn rate affected by the chamber pressure. 展开更多
关键词 star grain regression grain design spin effect chamber pressure effect
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有挠引力理论对SN1987A中微子两次信号的解释
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作者 陈方培 宋黎明 《大连理工大学学报》 CAS CSCD 北大核心 1994年第1期23-30,共8页
用有挠引力理论的粒子运动方程探讨了SN1987A中微子的运动,得出中微子可沿两条路径经历不同的时间到达地球的结论,对所观察到的中微子两次信号作出了比较合理的解释.
关键词 引力规范理论 超新星 有挠引力
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Pivotal Role of Spin in Celestial Body Motion Mechanics: Prelude to a Spinning Universe
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作者 Puthalath Koroth Raghuprasad 《Journal of High Energy Physics, Gravitation and Cosmology》 2021年第1期98-122,共25页
This is the final article in our series dealing with the interplay of spin and gravity that leads to the generation, and continuation of celestial body motions in the universe. In our prior studies we focused on such ... This is the final article in our series dealing with the interplay of spin and gravity that leads to the generation, and continuation of celestial body motions in the universe. In our prior studies we focused on such interactions in the elementary particles, and in the celestial bodies in the solar system. Foremost among the findings was that, along with gravity, matter at all levels exhibits axial spin. We further noted that all freestanding bodies outside our solar system, including the largest such units, the stars and galaxies also spin on their axes. Also, the axial rotation speed of planets in our solar system has a linear positive relationship to their masses, thus hinting at its fundamental and autonomous nature. We have reported that this relationship between the size of the body and its axial rotation speed extends to the stars and even the galaxies. Next, all congregations of matter spin on their axes in the counterclockwise direction;all satellites orbit their mother bodies also in the counterclockwise direction, <i>i.e.</i>: in our solar system, with only rare exceptions, the satellite bodies follow the mother bodies’ axial rotation. This relationship exists also in the case of the rings of planets, the asteroids and the Kuiper belt bodies, as well as the stars and their galaxies. We also noted the intricate involvements between spin and gravity in the exquisite phenomena of synchronous and negative rotations of planets and some satellites;we have explained in detail how these two phenomena occur. The closest large moons of the gas and ice giants and the earth’s moon exhibit synchronous rotation. In this paper we present evidence that these synchronously rotating satellite bodies’ <b>axial rotation speed</b> is closely related to the size and the axial rotation speeds of their respective mother bodies. In the satellites that follow a non-synchronous rotation (most of the planets and their satellites) the satellites’ own rotation speed usually dominates. In all these rotational/orbital motions, we believe, the axial rotation and gravity collaborate with the resultant centrifugal force, which prevents the satellite bodies from crashing into the mother bodies. We have inferred from the above observations that the axial spin is a fundamental property of matter, akin to gravity, electromagnetism, and strong and weak nuclear forces. This inherent property of matter to spin on its axis is what initiates all celestial body motions and makes such motions perpetual. The lateral motions of stars within the galaxies, are also influenced by the sizes of the stars;the larger the star, the faster it moves radially. Similarly, the larger the spiral galaxy, the faster it rotates on its axis. We extrapolate from these observations that the axial rotational speeds of galaxies affect their motion in space as well, that this is circumferential, and we predict this will also be in the counterclockwise direction. This lateral movement of the galaxies will give the appearance of the whole universe spinning on its axis. 展开更多
关键词 Axial Rotation Centrifugal Force Counterclockwise Gravity Neutron Stars Proto-Planetary Disk SPIN
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Predicting neutron star spins from twin kHz QPOs 被引量:1
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作者 SHI ChangSheng Department of Astronomy,Nanjing University,Nanjing 210093,China College of Material Science and Chemical Engineering,Hainan University,Hainan 570228,China 《Science China(Physics,Mechanics & Astronomy)》 SCIE EI CAS 2010年第S1期247-248,共2页
We briefly review the proposed relations between the frequencies of twin kilohertz quasi-periodic oscillations(kHz QPOs) and the spin frequencies in neutron star low-mass X-ray binaries(NSLMXBs).To test the validity o... We briefly review the proposed relations between the frequencies of twin kilohertz quasi-periodic oscillations(kHz QPOs) and the spin frequencies in neutron star low-mass X-ray binaries(NSLMXBs).To test the validity of the proposed models,we estimate the spin frequencies under these theoretical relations and compare them with the measured ones.It seems that magnetohydrodynamic(MHD) oscillations are more promising to account for the kHz QPOs. 展开更多
关键词 WIN KHZ QPOs SPIN neutron stars LMXBs
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