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Existence of Black Neutron Star
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作者 Trivedi Rajesh 《International Journal of Astronomy and Astrophysics》 2015年第1期11-14,共4页
A sufficiently large star will collapse to form a Black Hole Singularity due to Gravitational Pressure beyond Neutron Degeneracy. A Black Hole exhibits extremely strong Gravitational attraction that no particle or ele... A sufficiently large star will collapse to form a Black Hole Singularity due to Gravitational Pressure beyond Neutron Degeneracy. A Black Hole exhibits extremely strong Gravitational attraction that no particle or electromagnetic radiation can escape from it. The boundary of the region from which no escape is possible is called Event Horizon. In this work it is proposed that there exists a Neutron star smaller than Event Horizon, which is termed as Black Neutron Star. Furthermore an alternative method is proposed to ascertain the maximum permissible mass limit of the Neutron Star and the minimum mass limit of the naturally occurring gravitationally collapsed Black hole. 展开更多
关键词 neutron star black HOLE GRAVITATIONAL
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Neutron star mass-radius relation with gravitational field shielding by a scalar field
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作者 Bo-Jun Zhang Tian-Xi Zhang +1 位作者 Padmaja Guggilla Mostafa Dokhanian 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2013年第5期571-578,共8页
The currently well-developed models for equations of state (EoSs) have been severely impacted by recent measurements of neutron stars with a small radius and/or large mass. To explain these measurements, the theory ... The currently well-developed models for equations of state (EoSs) have been severely impacted by recent measurements of neutron stars with a small radius and/or large mass. To explain these measurements, the theory of gravitational field shielding by a scalar field is applied. This theory was recently developed in accor- dance with the five-dimensional (5D) fully covariant Kaluza-Klein (KK) theory that has successfully unified Einstein's general relativity and Maxwell's electromagnetic theory. It is shown that a massive, compact neutron star can generate a strong scalar field, which can significantly shield or reduce its gravitational field, thus making it more massive and more compact. The mass-radius relation developed under this type of modified gravity can be consistent with these recent measurements of neutron stars. In addition, the effect of gravitational field shielding helps explain why the supernova explosions of some very massive stars (e.g.9 40 MQ as measured recently) actually formed neutron stars rather than black holes as expected. The EoS models, ruled out by measurements of small radius and/or large mass neutron stars according to the the- ory of general relativity, can still work well in terms of the 5D fully covariant KK theory with a scalar field. 展开更多
关键词 stars: neutron -- gravitation -- black hole physics -- equation of state
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Mass Limit of Neutron Star
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作者 Jehangir Ahmad Dar 《International Journal of Astronomy and Astrophysics》 2014年第2期414-418,共5页
The mass limit of neutron star has still remained a mystery. The existing Tolman-Oppenheimer-Volkoff (TOV) equation for calculating the limit always gives different values, by introducing different assumptions and hav... The mass limit of neutron star has still remained a mystery. The existing Tolman-Oppenheimer-Volkoff (TOV) equation for calculating the limit always gives different values, by introducing different assumptions and having been predicted like 0.7 Mo, 3.2 Mo, 3.6 Mo, where Mo = 1.98 × 1030 Kg. There is a need of some better technique to adopt other than TOV relation to seek out the value. In this paper, a new relation between the mass of the collapsing star and its average density ρ′ has been derived and used to calculate the limit of neutron star. The conditions in radii between Schwarz Child’s radius and the actual radius of the collapsing star have been introduced to calculate the mass of star above which it will transform into a black hole and below it to a neutron star. A new constant, JN = 8.53707554 × 1039 N-3/2s-3Kg3 has been proposed with which if we introduce the average density of the collapsing neutron star, its mass limit can be calculated very easily. By putting the most possible mass density, which is the minimum required density for a collapsing star to transform into the black hole, it has been found that the mass limit of neutron star is quite higher than it has been assumed. The definition for black hole has also been re-defined on the basis of said radii conditions. 展开更多
关键词 black Hole neutron star SCHWARZ Child’s Radius Relation DEGENERACY Pressure Event HORIZON FCC and HCP LATTICES and TOV Equation
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On the Ultimate Fate of Massive Neutron Stars in an Ever Expanding Universe
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作者 Ahmad A. Hujeirat 《Journal of Modern Physics》 2018年第1期51-69,共19页
General theory of relativity predicts the central densities of massive neutron stars (-MANs) to be much larger than the nuclear density. In the absence of energy production, the lifetimes of MANs should be shorter tha... General theory of relativity predicts the central densities of massive neutron stars (-MANs) to be much larger than the nuclear density. In the absence of energy production, the lifetimes of MANs should be shorter that their low-mass counterparts. Yet neither black holes nor neutron stars, whose masses are between two and five solar masses have ever been observed. Also, it is not clear what happened to the old MANs that were created through the collapse of first generation of stars shortly after the Big Bang. In this article, it is argued that MANs must end as completely invisible objects, whose cores are made of incompressible quark-gluon-superfluids and that their effective masses must have doubled through the injection of dark energy by a universal scalar field at the background of supranuclear density. It turns out that recent glitch observations of pulsars and young neutron star systems and data from particle collisions at the LHC and RHIC are in line with the present scenario. 展开更多
关键词 Relativity: General black Hole Physics neutron stars SUPERFLUIDITY QCD DARK Energy DARK Matter
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The Remnant of GW170817: A Trapped Neutron Star with a Massive Incompressible Superfluid Core
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作者 Ahmad A. Hujeirat Ravi Samtaney 《Journal of Modern Physics》 2020年第11期1785-1798,共14页
Our bimetric spacetime model of glitching pulsars is applied to the remnant of GW170817. Accordingly, pulsars are born with embryonic incompressible superconducting gluon-quark superfluid cores (SuSu-matter) that are ... Our bimetric spacetime model of glitching pulsars is applied to the remnant of GW170817. Accordingly, pulsars are born with embryonic incompressible superconducting gluon-quark superfluid cores (SuSu-matter) that are embedded in Minkowski spacetime, whereas the ambient compressible and dissipative media (CDM) are imbedded in curved spacetime. As pulsars cool down, the equilibrium between both spacetime is altered, thereby triggering the well-observed glitch phenomena. Based thereon and assuming all neutron stars (<em>NSs</em>) to be born with the same initial mass of <img src="Edit_4d2d9e5f-812f-41d7-9422-5cfb3fc10997.bmp" alt="" />, we argue that the remnant of GW170817 should be a relatively faint <em>NS</em> with a massive central core made of SuSu-matter. The effective mass and radius of the remnant are predicted to be <img src="Edit_6702e3a8-abff-41f9-a45b-a2bc1e6c61b0.bmp" alt="" /> and <span style="white-space:nowrap;"><em>R</em><sub><em>rem</em></sub>=10.764 Km</span>, whereas the mass of the enclosed SuSu-core is <img src="Edit_6fe43fca-e33b-45a6-b846-bd7a09d4b8dd.bmp" alt="" />. Here, about 1/2<em>M</em><sub><em>core</em></sub> is an energy enhancement triggered by the phase transition of the gluon-quark-plasma from the microscopic into macroscopic scale. The current compactness of the remnant is <img src="Edit_38ced5f8-6f72-44d8-a3c9-89c2eaf73e0e.bmp" alt="" />, but predicted to increase as the CDM and cools down, rendering the remnant an invisible dark energy object, and therefore to an excellent black hole candidate. 展开更多
关键词 Relativity: Numerical General black Hole Physics MAGNETARS neutron stars Pulsars SUPERFLUIDITY Superconductivity GLUONS QUARKS Plasmas QCD
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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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Stellar Rotating Black Holes 被引量:1
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作者 Ardeshir Irani 《Journal of High Energy Physics, Gravitation and Cosmology》 2022年第1期97-99,共3页
Both mass and charge are needed to create a rotating Black Hole as has been investigated in great mathematical detail by the Reissner-Nordstrom metric and the Kerr-Newman metric. It is their application to astronomica... Both mass and charge are needed to create a rotating Black Hole as has been investigated in great mathematical detail by the Reissner-Nordstrom metric and the Kerr-Newman metric. It is their application to astronomical phenomena that they have stated difficulty with because astronomical objects have no net electric charge and that is what we are exploring. While the energy in the gravitational field of the mass of a Neutron Star alone cannot create a stationary Black Hole, together with the energy in the strong magnetic field created by a rotating Neutron Star a rotating Black Hole is formed. Black Holes are the portal to the next higher spatial dimension. 展开更多
关键词 Mass CHARGE Rotating black Hole Astronomical Objects neutron star
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Quantum Neutron Unit Gravity
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作者 Donald Chakeres Vola Andrianarijaona 《Journal of High Energy Physics, Gravitation and Cosmology》 2017年第2期267-276,共10页
Quantum gravity and the transformation of a neutron star or the merger of two neutron stars into a black hole are important topics in cosmology. According to the Schwarzschild radius relationship, a black hole arises ... Quantum gravity and the transformation of a neutron star or the merger of two neutron stars into a black hole are important topics in cosmology. According to the Schwarzschild radius relationship, a black hole arises when two times of the gravitational binding energy of the gravitational system, GBE, equal the annihilation energy of its total mass. From a quantum perspective, the integer number of neutrons defines the GBE and mass in the merger of binary pure neutron stars transforming to a black hole. Therefore, one can scale all gravitational binding energy relationships by using neutron mass, energy, distance, time, or frequency equivalents. We define ?of the neutron as the binding energy, 1.4188 × 10&#872249 J, of a virtual system of two neutrons separated by the neutron Compton wavelength. The??divided by a neutron’s rest mass energy represents a fundamental, dimensionless proportionality constant, 9.4252 × 10&#872240, . The square root of , αG, which we introduce here as a coupling constant, is identical in concept to the fine structure constant found in electromagnetic physics, but for gravity. Both αG and ?inter-relate the neutron, proton, electron, Bohr radius, speed of light, Planck’s constant, GBE of the electron in hydrogen, and Planck time. This paper demonstrates a direct conceptual and computational rationale of why the neutron and its negative beta decay quantum products accurately can represent a quantum gravitational natural unit system. 展开更多
关键词 QUANTUM GRAVITY neutron black HOLES neutron starS
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The Stellar Black Hole
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作者 Kenneth Dalton 《Journal of High Energy Physics, Gravitation and Cosmology》 2018年第4期651-654,共4页
A black hole model is proposed in which a neutron star is surrounded by a neutral gas of electrons and positrons. The gas is in a completely degenerate quantum state and does not radiate. The pressure and density in t... A black hole model is proposed in which a neutron star is surrounded by a neutral gas of electrons and positrons. The gas is in a completely degenerate quantum state and does not radiate. The pressure and density in the gas are found to be much less than those in the neutron star. The radius of the black hole is far greater than the Schwarzschild radius. 展开更多
关键词 black Hole Model neutron stars DEGENERATE LEPTON Gas
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Black Holes, the Big Bang and the Habitable Universe: Are They Really Compatible?
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作者 Ahmad A. Hujeirat 《Journal of Modern Physics》 2018年第1期70-83,共14页
Astronomical observations have confirmed the existence of BHs and the occurrence of the Big Bang event to beyond any reasonable doubt. While quantum field theory and general theory of relativity predict the mass-spect... Astronomical observations have confirmed the existence of BHs and the occurrence of the Big Bang event to beyond any reasonable doubt. While quantum field theory and general theory of relativity predict the mass-spectrum of BHs to be unlimited, both theories agree that their creation is irreversible. In this article, I argue that the recently-proposed SuSu-objects (objects that are made of incompressible superconducting gluon-quark superfluids) may not only entail the required properties to be excellent BH-candidates, but also encode a hidden connection to dark matter and dark energy in cosmology. If such connection indeed exists, then the inevitable consequence would be that our universe is infinite and subject to repeated Big Bang events of the second kind, which makes the habitability of the universe certain and our cosmic relevance insignificant and meaningless. 展开更多
关键词 Relativity: General black Hole Physics neutron stars SUPERFLUIDITY QCD DARK Energy DARK Matter
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Quantum Stabilization of General-Relativistic Variable-Density Degenerate Stars
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作者 David Eric Cox Ronald L. Mallett MP Silverman 《Journal of Modern Physics》 2012年第7期561-569,共9页
Research by one of the authors suggested that the critical mass of constant-density neutron stars will be greater than eight solar masses when the majority of their neutrons group into bosons that form a Bose-Einstein... Research by one of the authors suggested that the critical mass of constant-density neutron stars will be greater than eight solar masses when the majority of their neutrons group into bosons that form a Bose-Einstein condensate, provided the bosons interact with each other and have scattering lengths on the order of a picometer. That analysis was able to use Newtonian theory for the condensate with scattering lengths on this order, but general relativity provides a more fundamental analysis. In this paper, we determine the equilibrium states of a static, spherically-symmetric variable-density mixture of a degenerate gas of noninteracting neutrons and a Bose-Einstein condensate using general relativity. We use a Klein-Gordan Lagrangian density with a Gross-Pitaevskii term for the condensate and an effective field for the neutrons. We show that a new class of compact stars can exist with masses above the Oppenheimer-Volkoff limit, provided the scattering length of the bosons is large enough. These stars have no internal singularities, obey causality, and demonstrate a quantum mechanism consistent with general relativity that could prevent collapsed stars from becoming black holes. 展开更多
关键词 Gravity General RELATIVITY neutron starS black Holes BOSE-EINSTEIN CONDENSATES Numerical Physics
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Evidence of Pulsars Metamorphism and Their Connection to Stellar Black Holes
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作者 Ahmad A. Hujeirat 《Journal of Modern Physics》 2018年第4期532-553,共22页
It is agreed that the progenitors of neutron stars (-NSs) and black holes (-BHs) should be massive stars with . Yet none of these objects have ever been found with . Moreover, numerical modelings show that NSs of reas... It is agreed that the progenitors of neutron stars (-NSs) and black holes (-BHs) should be massive stars with . Yet none of these objects have ever been found with . Moreover, numerical modelings show that NSs of reasonable masses can be obtained only if the corresponding central density is beyond the nuclear one: an unverifiable density-regime with unknown physics. Here I intend to clarify the reasons underlying the existence of this mass-gap and propose a new class of invisible ultra-compact objects: the end-stage in the cosmological evolution of pulsars and neutron stars in an ever expanding universe. The present study relies on theoretical and experimental considerations as well as on solution of the non-linear TOV equation modified to include a universal scalar field &minus;&empty;at the background of supranuclear densities. The computer-code is based on finite volume method using both the first-order Euler and fourth-order Rugge-Kutta integration methods. The inclusion of &empty;at zero-temperature is motivated by recent observations of the short-living pentaquarks at the LHC. Based on these studies, I argue that pulsars must be born with embryonic super-baryons (SBs) that form through merger of individual neutrons at their centers. The cores of SBs are made of purely incompressible superconducting gluon-quark superfluids (henceforth SuSu-fluids). Such quantum fluids have a uniform supranuclear density and governed by the critical EOSs for baryonic matter and for &empty;-induced dark energy . The incompressibility here ensures that particles communicate at the shortest possible time scale, superfluidity and superconductivity enforce SBs to spin-down promptly as dictated by the Onsager-Feynman equation and to expel vortices and magnetic flux tubes, whereas their lowest energy state grants SBs lifetimes that are comparable to those of protons. These extra-ordinary long lifetimes suggest that conglomeration of SuSu-objects would evolve over several big bang events to possibly form dark matter halos that embed the galaxies in the observable universe. Pulsars and young neutron stars should metamorphose into SuSu-objects: a procedure which is predicted to last for one Gyr or even shorter, depending on their initial compactness. Once the process is completed, then they become extraordinary compact and turn invisible. It turns out that recent observations of particle collisions at the LHC and RHIC, observations of glitching pulsars and primordial galaxies remarkably support the present scenario. 展开更多
关键词 RELATIVITY General black Hole Physics PULSARS neutron stars SUPERFLUIDITY Low Temperature and Condensed MATTER QCD DARK Energy DARK MATTER
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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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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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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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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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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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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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