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Looking at the Physics of What a Quark Star-Black Hole Binary Would Create in Terms of GW Signals and New Physics
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作者 Andrew Beckwith 《Journal of High Energy Physics, Gravitation and Cosmology》 2021年第4期1255-1263,共9页
A quark star, black hole pairing as a would-be Gravitational wave generator is brought up. Quark stars are, anyway, likely to be black holes, above a certain mass limit, whereas a quark star in itself obey thermodynam... A quark star, black hole pairing as a would-be Gravitational wave generator is brought up. Quark stars are, anyway, likely to be black holes, above a certain mass limit, whereas a quark star in itself obey thermodynamic “laws” which in certain ways differ from the traditional black hole models. We list some of the probable consequences of such a binary, and make predictions as to certain GW phenomenon which will have observational consequences. <i>i.e.</i>, a GW “change in energy” from a black hole—Quark star pair would likely be within 90% of that of comparatively massed black hole—black hole binary pair. The electromagnetic “profile” of the two cases would differ dramatically, and we conclude our inquiry with an open question if a generalized uncertainty principle could play a role in comparing the 7<sup>th</sup> and 8<sup>th</sup> equations of our presentation. 展开更多
关键词 GW Signals Quark star-black Hole Binary New Physics
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Why the Central Monster in M87 Should Be a Massive DEO Rather than a SMBH?
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作者 Ahmad A. Hujeirat Mauritz Wicker 《Journal of Modern Physics》 2024年第5期537-549,共13页
In this paper, we show that massive envelopes made of highly compressed normal matter surrounding dark objects (DEOs) can curve the surrounding spacetime and make the systems observationally indistinguishable from the... In this paper, we show that massive envelopes made of highly compressed normal matter surrounding dark objects (DEOs) can curve the surrounding spacetime and make the systems observationally indistinguishable from their massive black hole counterparts. DEOs are new astrophysical objects that are made up of entropy-free incompressible supranuclear dense superfluid (SuSu-matter), embedded in flat spacetimes and invisible to outside observers, practically trapped in false vacua. Based on highly accurate numerical modelling of the internal structures of pulsars and massive neutron stars, and in combination with using a large variety of EOSs, we show that the mass range of DEOs is practically unbounded from above: it spans those of massive neutron stars, stellar and even supermassive black holes: thanks to the universal maximum density of normal matter, , beyond which normal matter converts into SuSu-matter. We apply the scenario to the Crab and Vela pulsars, the massive magnetar PSR J0740 6620, the presumably massive NS formed in GW170817, and the SMBHs in Sgr A* and M87*. Our numerical results also reveal that DEO-Envelope systems not only mimic massive BHs nicely but also indicate that massive DEOs can hide vast amounts of matter capable of turning our universe into a SuSu-matter-dominated one, essentially trapped in false vacua. 展开更多
关键词 General Relativity Big Bang Black Holes QSOS Neutron Stars QCD Condensed Matter INCOMPRESSIBILITY SUPERFLUIDITY Super-Conductivity
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Evidence for False Vacuum States inside the Cores of Massive Pulsars and the Ramification on the Measurements of Their True Masses
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作者 Ahmad A. Hujeirat Mauritz M. Wicker 《Journal of Modern Physics》 2023年第11期1409-1425,共17页
Based on the theory and observations of glitching pulsars, we show that the ultra-cold supranuclear dense matter inside the cores of massive pulsars should condensate in vacua, as predicated by non-perturbative QCD. T... Based on the theory and observations of glitching pulsars, we show that the ultra-cold supranuclear dense matter inside the cores of massive pulsars should condensate in vacua, as predicated by non-perturbative QCD. The trapped matter here forms false vacuums embedded in flat spacetimes and completely disconnected from the outside world. Although the vacuum expectation value here vanishes, the masses and sizes of these incompressible superfluid cores are set to grow with cosmic times, in accord with the Onsager-Feynman superfluidity analysis. We apply our scenario to several well-studied pulsars, namely the Crab, Vela, PSR J0740+6620 and find that the trapped mass-contents in their cores read {0.15,0.55,0.64}, implying that their true masses are {1.55,2.35,2.72} , respectively. Based thereon, we conclude that: 1) The true masses of massive pulsars and neutron stars are much higher than detected by direct observations and, therefore, are unbounded from above, 2) The remnant of the merger event in GW170817 should be a massive NS harbouring a core with 1.66  . 展开更多
关键词 Numerical Relativity PULSARS MAGNETARS Neutrons Stars Black Holes Quantum Vacuum QCD Condensed Matter INCOMPRESSIBILITY SUPERFLUIDITY Super-Conductivity
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Why the Energy Density of the Universe Is Lower and Upper-Bounded? Relaxing the Need for the Cosmological Constant
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作者 Ahmad A. Hujeirat 《Journal of Modern Physics》 CAS 2023年第6期790-801,共12页
Recently, it was argued that the energy density of the supranuclear dense matter inside the cores of massive neutron stars must have reached the , beyond which supranuclear dense matter becomes incompressible entropy-... Recently, it was argued that the energy density of the supranuclear dense matter inside the cores of massive neutron stars must have reached the , beyond which supranuclear dense matter becomes incompressible entropy-free gluon-quark superfluid. As this matter is also confined and embedded in flat spacetime, it is Lorentz invariant and could be treated as vacuum. The lower bound of matter in the universe may be derived using the following observational constraints: 1) The average energy density of the observable universe is erg/cc, 2) The observable universe is remarkably flat, and 3) the Hubble constant is a slowly decreasing function of cosmic time. Based thereon, I argue that the energy density in nature should be bounded from below by the average density of our vast and flat parent universe, , which is, in turn, comparable to the vacuum energy density , and amounts to erg/cc. When the total energy density is measured relative to , then both GR and Newtonian field equations may consistently model the gravitational potential of the parent universe without invoking cosmological constants. Relying on the recently proposed unicentric model of the observable universe, UNIMOUN, the big bang must have warped the initially flat spacetime into a curved one, though the expansion of the fireball doomed the excited energy state to diffuse out and return back to the ground energy state that governs the flat spacetime of our vast parent universe. 展开更多
关键词 General Relativity Big Bang Black Holes QSOS Neutron Stars QCD Condensed Matter INCOMPRESSIBILITY SUPERFLUIDITY Super-Conductivity
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Foundation of the Unicentric Model of the Observable Universe—UNIMOUN
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作者 Ahmad A. Hujeirat 《Journal of Modern Physics》 CAS 2023年第4期415-431,共17页
In view of the growing difficulties of ΛCDM-cosmologies to compete with recent highly accurate cosmological observations, I propose the alternative model: the Unicentric Model of the Observable UNiverse (UNIMOUN). Th... In view of the growing difficulties of ΛCDM-cosmologies to compete with recent highly accurate cosmological observations, I propose the alternative model: the Unicentric Model of the Observable UNiverse (UNIMOUN). The model relies on employing a new time-dependent -metric for the GR field equations, which enables reversible phase transitions between normal compressible fluids and incompressible quantum superfluids, necessary for studying the cosmic evolution of the observable universe. The main properties of UNIMOUN read: 1) The observable universe was born in a flat spacetime environment, which is a tiny fraction of our infinitely large and flat parent universe, 2) Our big bang (BB) happened to occur in our neighbourhood, thereby endowing the universe the observed homogeneity and isotropy, 3) The energy density in the universe is upper-bounded by the universal critical density , beyond which matter becomes purely incompressible, rendering formation of physical singulareties, and in particular black holes, impossible, 4) Big bangs are neither singular events nor invoked by external forces, but rather, they are common self-sustaining events in our parent universe, 5) The progenitors of BBs are created through the merger of cosmically dead and inactive neutron stars and/or through “supermassive black holes” that are currently observed at the centres of most massive galaxies, 6) The progenitors are made up of purely incompressible entropy-free superconducting gluon- quark superfluids with (SuSu-matter), which endows these giant objects measurable sizes, 7) Spacetimes embedding SuSu-matter are conformally flat. It is shown that UNIMOUN is capable of dealing with or providing answers to several fundamental open questions in astrophysics and cosmology without invoking inflation, dark matter or dark energy. 展开更多
关键词 General Relativity: Big Bang Black Holes QSOS Neutron Stars QCD Condensed Matter INCOMPRESSIBILITY SUPERFLUIDITY Super-Conductivity
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Hubble Tension versus the Cosmic Evolution of Hubble Parameter in the Unicentric Model of the Observable Universe
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作者 Ahmad Hujeirat 《Journal of Modern Physics》 CAS 2023年第3期183-197,共15页
Recently, a unicentric model of the observable universe (UNIMOUN) was proposed. Accordingly, big bangs are common events in our infinitely large, flat, homogeneous and isotropic parent universe. Their progenitors are ... Recently, a unicentric model of the observable universe (UNIMOUN) was proposed. Accordingly, big bangs are common events in our infinitely large, flat, homogeneous and isotropic parent universe. Their progenitors are clusters of cosmically dead and massive neutron stars that merged after reaching the ultimate lowest quantum energy state, where the matter is in an incompressible superconducting gluon-quark superfluid state and zero-entropy, hence granting the resulting progenitors measurable sizes and immunity to collapsing into black holes. Our big bang happened to occur in our neighbourhood, thereby enduing the universe, the observed homogeneity and isotropy. As the enclosed mass of the progenitor was finite, the dynamically expanding curved spacetimes embedded the fireball started flattening to finally diffuse into the flat spacetime of the parent universe. By means of general relativistic numerical hydrodynamical calculations, we use the H-metric to follow the time-evolution of the spacetime embedding the progenitor during the hadronization and the immediately following epochs. Based thereon, we find that the kinetic energy of newly created normal matter increases with distance in a self-similar manner, imitating thereby outflows of nearly non-interacting particles. On cosmic time scales, this behaviour yields a Hubble parameter, H(t), which decreases slowly with the distance from the big bang event. Given the sensitivity of the data of the Cosmic Microwave Background (CMB) from Planck to the underlying cosmological model, we conclude that UNIMOUN is a viable alternative to ΛCMD-cosmologies. 展开更多
关键词 General Relativity: Big Bang Black Holes QUASARS Neutron Stars Quantum Chromodynamics Condensed Matter INCOMPRESSIBILITY SUPERFLUIDITY Super-Conductivity
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伽玛射线暴及其余辉研究进展 被引量:3
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作者 徐明 黄永锋 《天文学进展》 CSCD 北大核心 2012年第1期17-34,共18页
伽玛射线暴是一种来自宇宙空间随机方向的短时间内伽玛射线突然增亮的现象。伽玛射线暴虽然早在1967年就由Vela卫星观测到,但直到1997年人们才通过余辉观测确定其寄主星系,并通过寄主星系的红移最终确定了伽玛射线暴的宇宙学起源。对伽... 伽玛射线暴是一种来自宇宙空间随机方向的短时间内伽玛射线突然增亮的现象。伽玛射线暴虽然早在1967年就由Vela卫星观测到,但直到1997年人们才通过余辉观测确定其寄主星系,并通过寄主星系的红移最终确定了伽玛射线暴的宇宙学起源。对伽玛射线暴研究概况进行了评述:详细介绍了伽玛射线暴及其余辉的观测进展,特别是近期Swift卫星和Fermi卫星带来的新发现;系统描述了伽玛射线暴标准火球模型、伽玛射线暴余辉物理(相对论性外流与暴周环境介质的相互作用过程、辐射产生机制等)及伽玛射线暴的前身星等。也对伽玛射线暴的未来研究进行了展望。 展开更多
关键词 辐射机制 伽玛射线暴 中子星 黑洞
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GRB 130427A/SN 2013cq与伽玛射线暴-超新星成协 被引量:1
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作者 王善钦 戴子高 吴雪峰 《天文学进展》 CSCD 北大核心 2014年第4期481-515,共35页
从1998年4月初步确认GRB 980425/SN 1998bw成协,至2013年9月确认GRB130831A/SN 2013fu成协,共有11对伽玛暴与超新星成协事件通过光谱学方法得到确认。对伽玛暴-超新星成协的详细研究大大深化了人们对伽玛暴与Ic型超新星的认识,并推进了... 从1998年4月初步确认GRB 980425/SN 1998bw成协,至2013年9月确认GRB130831A/SN 2013fu成协,共有11对伽玛暴与超新星成协事件通过光谱学方法得到确认。对伽玛暴-超新星成协的详细研究大大深化了人们对伽玛暴与Ic型超新星的认识,并推进了人们对大质量恒星演化、死亡以及爆发机制的研究:对它们的多波段余辉的性质以及超新星光谱的观测与分析间接地揭示出伽玛暴-超新星中心引擎的性质。这些事件中,GRB 130427A/SN 2013cq具有特殊的重要性:它是近距离宇宙中唯一的高能、高亮度的伽玛暴,它的GeV辐射挑战了当前的伽玛暴辐射机制,伴随它的明亮光学闪提供了爆炸本性的有用线索,伴随它的SN 2013cq是伽玛暴成协的超新星中动能最大的超新星之一,对伴随它的中微子探测的零结果也对伽玛暴的瞬时辐射模型给出了有用的限制。总结了GRB 130427A/SN 2013cq的重要观测结果,这对于探索伽玛暴-超新星成协的本质及伽玛暴瞬时辐射和余辉的细节性质有非常重要的研究价值。 展开更多
关键词 伽玛射线暴 超新星 中子星 黑洞
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Kinnersley时空中的粒子辐射特征 被引量:2
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作者 杨树政 林理彬 《广西师范大学学报(自然科学版)》 CAS 2000年第3期24-26,共3页
恒星内部依次进行着核反应 ,促使恒星不断地演化 ,恒星演化到晚期的归宿将成为白矮星或中子星或黑洞 .对于 Kinnersley黑洞而言 ,加速度是导致非热辐射粒子的主要原因 ;Kinnersley时空中的 Dirac能级分布与极角 θ有关 .
关键词 恒星 核反应 Kinnersley黑洞 非热辐射粒子
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金花梨变异单系对梨黑星病的抗性研究 被引量:2
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作者 刘遵春 廖明安 包东娥 《西北林学院学报》 CSCD 北大核心 2006年第2期108-109,共2页
对金花梨及其12个变异系进行了抗梨黑星病抗性的田间调查。结果表明,金花梨部分变异单系在抗梨黑星病方面发生了一定程度的变异,其中J4抗梨黑星病能力最强,其次为J10、J14、J5、J15。
关键词 金花梨 变异单系 梨黑星病
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黑芝麻螺旋藻复合营养饮料稳定性的研究 被引量:6
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作者 刘灵杰 韦艳萍 +7 位作者 龙肇谋 莫丽萍 陀海燕 谭栀恩 曾佩琴 罗春花 陈卫卫 傅鹏 《食品研究与开发》 CAS 北大核心 2018年第18期112-118,共7页
以黑芝麻与螺旋藻为主要原料,研究黑芝麻螺旋藻复合营养饮料的稳定性工艺。首先通过单因素试验法分别考察了蔗糖酯、蒸馏单硬脂酸甘油酯、黄原胶、海藻酸丙二醇酯、羧甲基纤维素钠等乳化剂与稳定剂对饮料的感官和稳定性的影响;在此基础... 以黑芝麻与螺旋藻为主要原料,研究黑芝麻螺旋藻复合营养饮料的稳定性工艺。首先通过单因素试验法分别考察了蔗糖酯、蒸馏单硬脂酸甘油酯、黄原胶、海藻酸丙二醇酯、羧甲基纤维素钠等乳化剂与稳定剂对饮料的感官和稳定性的影响;在此基础上,采用星点设计-效应面法优选黑芝麻螺旋藻复合营养饮料的最佳稳定性工艺条件。结果表明:蒸馏单硬脂酸甘油酯用量为0.21%,黄原胶用量为0.04%,海藻酸钠丙二醇酯用量为0.09%;与理论预测值0.850的相对标准偏差(relative standard deviation,RSD)为6.59%。所建立的数学模型具有较好的预测性,所选的工艺条件重现性较好。 展开更多
关键词 黑芝麻 螺旋藻 稳定性 星点设计-效应面法 复合营养饮料
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相对分子质量及端基改性对炭黑补强星形溶聚丁苯橡胶性能的影响 被引量:8
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作者 张帅 赵素合 吴友平 《橡胶工业》 CAS 2015年第3期140-144,共5页
研究相对分子质量及端基改性对炭黑补强星形溶聚丁苯橡胶(SSBR)各项性能的影响。结果表明,随着相对分子质量的增大,SSBR生胶和混炼胶的门尼粘度增大,拉伸强度和拉断伸长率先增大后有所减小,撕裂强度和耐磨性能改善,压缩疲劳温升及永久... 研究相对分子质量及端基改性对炭黑补强星形溶聚丁苯橡胶(SSBR)各项性能的影响。结果表明,随着相对分子质量的增大,SSBR生胶和混炼胶的门尼粘度增大,拉伸强度和拉断伸长率先增大后有所减小,撕裂强度和耐磨性能改善,压缩疲劳温升及永久变形不断减小。分子链末端经叔丁基二苯基氯硅烷改性的SSBR硫化胶的物理性能、耐磨性能和动态力学性能达到平衡,符合高性能绿色轮胎胎面胶的要求。 展开更多
关键词 星形溶聚丁苯橡胶 端基改性 炭黑 动态力学性能
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γ射线爆(GRB)研究进展及其几种模型的讨论
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作者 黄文耿 周爱芝 杨丕博 《华中师范大学学报(自然科学版)》 CAS CSCD 北大核心 2000年第2期167-170,228,共5页
观测结果表明 ,γ射线爆源空间分布是各向同性但不均匀的 ,说明γ射线爆起源于宇宙学距离 .本文介绍 γ射线爆的观测情况和分类 ,并讨论了几种当前比较流行的 γ射线爆理论模型 .
关键词 Γ射线爆 中子星 银河系 宇宙学模型 超新星模型
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夸克简并压可以阻止小质量黑洞无限坍缩 被引量:1
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作者 刘发兴 刘颂豪 《广东工业大学学报》 CAS 2003年第1期20-22,共3页
根据粒子物理理论和量子简并理论,本文认为自然界存在夸克星,这是恒星演化最后阶段形成的一类产物.文章估算了夸克星的质量极限和半径.结果表明夸克星的质量分布在事件视界以内,即夸克星是黑洞,但构成这种黑洞的物质并没有坍缩到大小为... 根据粒子物理理论和量子简并理论,本文认为自然界存在夸克星,这是恒星演化最后阶段形成的一类产物.文章估算了夸克星的质量极限和半径.结果表明夸克星的质量分布在事件视界以内,即夸克星是黑洞,但构成这种黑洞的物质并没有坍缩到大小为零的一点. 展开更多
关键词 夸克简并压 黑洞 坍缩 致密星 粒子物理 量子简并 恒星演化 质量极限 夸克星
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恒星级黑洞的观测证认研究进展 被引量:1
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作者 张双南 《天文学进展》 CSCD 北大核心 2012年第1期1-16,共16页
具有不同质量的恒星在耗尽其热核能源后,最终可能会坍缩成为性质完全不同的致密天体,如白矮星、中子星或者黑洞。从20世纪30年代起,黑洞的观测及其证认一直是天体物理学的研究热点之一。首先简要地回顾了恒星级黑洞的形成及其候选天体... 具有不同质量的恒星在耗尽其热核能源后,最终可能会坍缩成为性质完全不同的致密天体,如白矮星、中子星或者黑洞。从20世纪30年代起,黑洞的观测及其证认一直是天体物理学的研究热点之一。首先简要地回顾了恒星级黑洞的形成及其候选天体的研究历史;然后介绍了如何从观测上证认恒星级黑洞:接着详细讨论了恒星级黑洞的质量和自转参数的测量方法;最后介绍恒星级黑洞观测及其证认的最新研究进展,并做出结论:目前已经有充分的证据宣告在部分吸积X射线双星中存在恒星级黑洞。 展开更多
关键词 黑洞 中子星 X射线 双星
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数值相对论简介(Ⅰ)——爱因斯坦方程 被引量:2
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作者 刘文彪 《北京师范大学学报(自然科学版)》 CAS CSCD 北大核心 2003年第2期193-197,共5页
对数值相对论中涉及的一些典型的算法进行了简单的介绍 .在广义相对论中 ,引力场是由一组极其复杂的、相互耦合的、非线性的双曲或椭圆偏微分方程决定的 .由于大规模并行计算机的运行速度和存储容量的飞速发展 ,在爱因斯坦场方程写出 8... 对数值相对论中涉及的一些典型的算法进行了简单的介绍 .在广义相对论中 ,引力场是由一组极其复杂的、相互耦合的、非线性的双曲或椭圆偏微分方程决定的 .由于大规模并行计算机的运行速度和存储容量的飞速发展 ,在爱因斯坦场方程写出 80多年以后终于有可能对在天体物理中十分令人关注的现象如黑洞或中子星的碰撞问题等 ,进行广义相对论性的三维模拟 ,进而诞生了数值相对论 . 展开更多
关键词 数值相对论 爱因斯坦方程 广义相对论 引力场 黑洞 中子星 计算方法
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天体尺度上的重大灾变事件——恒星的形成和归宿(下)
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作者 赵君亮 《自然杂志》 北大核心 2010年第5期255-259,共5页
恒星之一生,长者可达几万亿年,短则不到一千万年,期间历经多次短时标的灾变事件,而此类事件出现前后,恒星多方面性质发生了非常剧烈的、甚至是根本性的改变。对此,天文学家已经有了较为充分的认识,但尚未完全洞悉其中之众多奥秘。
关键词 行星状星云 白矮星 中子星 黑洞
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黑洞候选体X射线双星Cyg X-1硬度比周期特性研究 被引量:1
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作者 董爱军 盖宁 张福安 《天文学报》 CSCD 北大核心 2012年第5期391-401,共11页
利用离散傅里叶分析法,基于RXTE(Rossi X-ray Timing Explorer)/ASM(All-Sky Monitor,1.5~12 keV)观测数据,对黑洞候选体X射线双星Cyg X-1硬度比HR(5~12 keV/3~5 keV)(简写HR)的时变特性进行了分析,结果表明黑洞候选体X射线双星Cyg ... 利用离散傅里叶分析法,基于RXTE(Rossi X-ray Timing Explorer)/ASM(All-Sky Monitor,1.5~12 keV)观测数据,对黑洞候选体X射线双星Cyg X-1硬度比HR(5~12 keV/3~5 keV)(简写HR)的时变特性进行了分析,结果表明黑洞候选体X射线双星Cyg X-1硬度比HR存在明显的周期特性:(1)混合态(硬态+软态,本文指MJD=50087~55841期间所有的观测数据)时,HR存在T≈5.6 d、40.0 d、78.4 d、173.8 d以及400/800 d的时变周期;(2)硬态时,HR存在T≈5.6 d、33.7/67.6 d、45.3 d和165.3 d的周期特性;(3)软态时,HR出现了T≈38.5 d、48.1 d和128.3 d的周期性变化.并利用粘滞理论和Zdziarski吸积盘模型讨论了以上周期特性的物理机制. 展开更多
关键词 恒星 双星 X射线 个别 Cyg X-1 黑洞物理
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高密天体特征分析
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作者 彭望录 《陕西师范大学学报(自然科学版)》 CAS CSCD 1995年第S1期1-3,共3页
对恒星演化后期的三类高密星体(白矮星,中子星,黑洞)的基本性质和概念作了简明介绍.
关键词 白矮星 中子星 黑洞
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关于宇宙暗物质主要形态之黑洞-夸克星的新证据分析 被引量:7
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作者 张海鹏 张力 +8 位作者 罗延安 范祖辉 张鹏杰 黄明球 常丽君 孟庆义 张丹参 胡扬洋 李新兵 《山西师范大学学报(自然科学版)》 2015年第2期49-54,共6页
通过分析新近证据,进一步探讨宇宙暗物质等问题,分析认为:(1)宇宙紫外辐射超出已知辐射源4倍的发现,可能就是源于我国的、2013年初预言的约在可见光附近波段的宇宙背景辐射;彭罗斯等2010年发现的CMB偏振环等新证据,较有力地支持原始夸... 通过分析新近证据,进一步探讨宇宙暗物质等问题,分析认为:(1)宇宙紫外辐射超出已知辐射源4倍的发现,可能就是源于我国的、2013年初预言的约在可见光附近波段的宇宙背景辐射;彭罗斯等2010年发现的CMB偏振环等新证据,较有力地支持原始夸克星碰撞、重组的宇宙演化及起源模型;黑洞(暗星)-夸克星可能是宇宙暗物质的主要形态,应足以解释暗物质与可见物质的比例.以上均应深入研究;(2)76个黑洞的强大磁场的发现,客观上有力地支持了星系中心超大质量黑洞等的携1/3正负电子电荷的最基本的正、负夸克构型;(3)质能守恒定律的经典物理学意义所推论的最基本夸克的空心圈环结构,为圈量子引力奠定了较坚实的粒子物理学基础;(4)结合高频引力波产生机理(激光约束核聚变等)及探测机理,应对中微子与高频引力波(引力子)进行会师研究. 展开更多
关键词 黑洞 暗星 夸克星 圈量子引力 引力波 高频 中微子 左旋 暗物质
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