標題: Titlebook: Current Trends in Relativistic Astrophysics; Theoretical, Numeric Leonardo Fernández-Jambrina,Luis Manuel González-R Book 2003 Springer-Ver [打印本頁] 作者: fungus 時間: 2025-3-21 17:54
書目名稱Current Trends in Relativistic Astrophysics影響因子(影響力)
書目名稱Current Trends in Relativistic Astrophysics影響因子(影響力)學科排名
書目名稱Current Trends in Relativistic Astrophysics網(wǎng)絡公開度
書目名稱Current Trends in Relativistic Astrophysics網(wǎng)絡公開度學科排名
書目名稱Current Trends in Relativistic Astrophysics被引頻次
書目名稱Current Trends in Relativistic Astrophysics被引頻次學科排名
書目名稱Current Trends in Relativistic Astrophysics年度引用
書目名稱Current Trends in Relativistic Astrophysics年度引用學科排名
書目名稱Current Trends in Relativistic Astrophysics讀者反饋
書目名稱Current Trends in Relativistic Astrophysics讀者反饋學科排名
作者: 開玩笑 時間: 2025-3-21 23:18 作者: 植物茂盛 時間: 2025-3-22 03:33
https://doi.org/10.1007/978-3-658-39635-0pulsars, active galactic nuclei and gamma-ray bursts are some of the observed processes that are the object of this discipline. On the other hand, the intriguing features of black holes, singularities and hypotheses like the no-hair conjecture and cosmic censorship have been discussed for decades. P作者: 責任 時間: 2025-3-22 05:30 作者: NEXUS 時間: 2025-3-22 08:49
Harris C. M. Tiddens,Andrea Isermann-Kühnd polar. Their equations decouple and reduce to Schr?dinger wave equations. Special attention is paid to quasi-normal modes for black holes and how they can be excited, since gravitational waves are emitted at their frequencies and they appear in many dynamical processes.作者: Indurate 時間: 2025-3-22 14:10 作者: Indurate 時間: 2025-3-22 20:59 作者: Blanch 時間: 2025-3-23 01:17
https://doi.org/10.1007/978-3-658-40576-2otion of unresolved steep gradients without creating spurious oscillations. I will show how these techniques have been extended to relativistic hydrodynamics, making it possible to explore some challenging astrophysical scenarios. I will review recent literature concerning the main properties of dif作者: 小卒 時間: 2025-3-23 02:49
https://doi.org/10.1007/978-3-658-40584-7 3+1 formalism and with the evolution equations written as a FOFCH (first-order flux conservative hyperbolic) system, advanced numerical methods from CFD (Computational Fluid Dynamics) have been successfully applied. A flux limiter mechanism has been implemented in order to deal with steep gradients作者: 聯(lián)邦 時間: 2025-3-23 07:35
https://doi.org/10.1007/978-3-658-40584-7spond naturally to the spacetime dynamics. We show that the combination of excision and gauge conditions we use is able to drive highly distorted, rotating black holes to an almost static state at late times, with well behaved metric functions, without the need for any special initial conditions or 作者: 輕快帶來危險 時間: 2025-3-23 09:41
https://doi.org/10.1007/978-3-658-40584-7pactification and a reformulation of the Einstein equations in terms of rescaled variables, the so-called “conformal field equations” developed by Friedrich. These equations allow to include “infinity” on a finite grid, solving regular equations, whose solutions give rise to solutions of the Einstei作者: maverick 時間: 2025-3-23 16:40
Michael Burawoys Public Sociology the related gravitational wave emission. The black holes are modelled by two Dirac delta functions in conformally related d-dimensional euclidean space. The limit from the Einstein field equations in (d+1)-dimensional spacetime is applied to achieve well- defined mathematical expressions in 4-dimen作者: 離開真充足 時間: 2025-3-23 20:34
https://doi.org/10.1007/978-3-658-40979-1al concepts involved in interferometric and acoustic (Weber bar) GW antennas. In particular, the type of signal the GW deposits in the detector in each case will be assessed, as well as its intensity and deconvolution. Brief reference will also be made to detector sensitivity characterisation, inclu作者: Aspiration 時間: 2025-3-24 00:00
Pers?nlichkeiten aus der Politikntz transformation we show that the symmetric part satisfies the dominant energy condition (up to sign) and can be written as a sum of at most . superenergy tensors of simple forms determined by its null eigenvectors. By studying relations between eigenvectors of the symmetric and anti-symmetric par作者: Indicative 時間: 2025-3-24 03:44
Pers?nlichkeiten aus Gesellschaft und Kulturcircularity conditions that can be considered for the Yang-Mills field in a stationary axisymmetric SU(2) Einstein-Yang-Mills theory imply in fact that the field is of embedded Abelian type, or else that the metric is not asymptotically flat.作者: Flat-Feet 時間: 2025-3-24 10:19
Nationale Feiertage und Feste der Türkeion for the shortest path in the bulk for a 1+4 cosmological metric. The time cost and the redshifts for photons and gravitons after travelling their respective path are compared. We consider some numerical solutions of the shortest path equation, and show that there is no shortest path in the bulk f作者: 拱形大橋 時間: 2025-3-24 11:02 作者: intimate 時間: 2025-3-24 18:32 作者: 自由職業(yè)者 時間: 2025-3-24 22:31
Hans-Werner Wahl,Clemens Tesch-R?mer an anisotropic scalar field and two perfect fluids representing dust and isotropic radiation. Based on this solution, we construct a cosmological model that respects the evolution of the scale factor predicted in standard cosmology.作者: 出生 時間: 2025-3-25 00:48
https://doi.org/10.1007/978-3-658-41465-8ers and the degree of polarization. The evolution equations for Stokes parameters on a curved space-time are obtained using the parallel transport of the polarization vector along a null geodesic. The interest of these equations in Astrophysics and Relativistic Cosmology is outlined.作者: SPALL 時間: 2025-3-25 04:03
Hermann Brandenburg,Volker Fenchel causal future directed vectors. These diffeomorphisms, called proper causal relations, contain as a subset the well known group of conformal relations which can be characterized as those diffeomorphisms such that both the transformation itself and its inverse are proper causal relations. It turns o作者: 聯(lián)邦 時間: 2025-3-25 10:38
https://doi.org/10.1007/3-540-36973-2Accretion; Cosmology; Gravity; Lorentz transformation; astrophysics; black holes; numerical relativity; rel作者: 休息 時間: 2025-3-25 13:08
978-3-662-14420-6Springer-Verlag Berlin Heidelberg 2003作者: Hyperalgesia 時間: 2025-3-25 17:09
Black Hole Thermodynamicsof their horizon area. The brick wall model and an operational approach are discussed. An attempt to understand at the microlevel how the quantum black hole acquires its thermal properties is included. The chapter concludes with some remarks on the extension of these techniques to describing the dynamical process of black hole evaporation.作者: 樣式 時間: 2025-3-25 23:16
Perturbations of Black Holesd polar. Their equations decouple and reduce to Schr?dinger wave equations. Special attention is paid to quasi-normal modes for black holes and how they can be excited, since gravitational waves are emitted at their frequencies and they appear in many dynamical processes.作者: 噱頭 時間: 2025-3-26 01:37 作者: 多嘴多舌 時間: 2025-3-26 04:17 作者: Inveterate 時間: 2025-3-26 08:52 作者: Rct393 時間: 2025-3-26 13:44 作者: Flawless 時間: 2025-3-26 16:48
Lorentzian Comments on Stokes Parametersers and the degree of polarization. The evolution equations for Stokes parameters on a curved space-time are obtained using the parallel transport of the polarization vector along a null geodesic. The interest of these equations in Astrophysics and Relativistic Cosmology is outlined.作者: Mnemonics 時間: 2025-3-26 21:32
Current Trends in Relativistic Astrophysics978-3-540-36973-8Series ISSN 0075-8450 Series E-ISSN 1616-6361 作者: Noisome 時間: 2025-3-27 02:32 作者: Wernickes-area 時間: 2025-3-27 05:57 作者: omnibus 時間: 2025-3-27 10:31 作者: anniversary 時間: 2025-3-27 17:24 作者: 女歌星 時間: 2025-3-27 19:48
https://doi.org/10.1007/978-3-658-41465-8d order equation for two functions. From the solutions of those equations the Ernst potential can be foundb y quadrature. As an application we give a new class of solutions in spherical coordinates which generalize the Tomimatsu-Sato solutions.作者: persistence 時間: 2025-3-27 23:18
Hans-Werner Wahl,Clemens Tesch-R?mer an anisotropic scalar field and two perfect fluids representing dust and isotropic radiation. Based on this solution, we construct a cosmological model that respects the evolution of the scale factor predicted in standard cosmology.作者: conifer 時間: 2025-3-28 03:27
https://doi.org/10.1007/978-3-658-41465-8ers and the degree of polarization. The evolution equations for Stokes parameters on a curved space-time are obtained using the parallel transport of the polarization vector along a null geodesic. The interest of these equations in Astrophysics and Relativistic Cosmology is outlined.作者: 博愛家 時間: 2025-3-28 09:09 作者: sphincter 時間: 2025-3-28 10:36
Lecture Notes in Physicshttp://image.papertrans.cn/d/image/241470.jpg作者: 迷住 時間: 2025-3-28 14:39
0075-8450 ich was to provide a modern introduction to specific aspects of the field for young researchers, as well as for nonspecialists from related areas. Particular emphasis is placed on the theory of black holes and evolution, relativistic stars and jet hydrodynamics, as well as the production and detecti作者: canvass 時間: 2025-3-28 20:17
https://doi.org/10.1007/978-3-658-39635-0 intriguing features of black holes, singularities and hypotheses like the no-hair conjecture and cosmic censorship have been discussed for decades. Perturbative and numerical approaches are mandatory to tackle most of these issues.作者: DNR215 時間: 2025-3-29 01:58
https://doi.org/10.1007/978-3-658-39776-0lisionless particles, each with angular momentum). Using linear perturbation theory we show that in the former case there are still critical phenomena, explicitly predictingthe associated scalingla ws. We show that, on the contrary, critical phenomena are not generic for Vlasov matter.作者: absorbed 時間: 2025-3-29 05:48
https://doi.org/10.1007/978-3-658-40979-1h case will be assessed, as well as its intensity and deconvolution. Brief reference will also be made to detector sensitivity characterisation, including very summary data on current state of the art of GW detectors.作者: 是限制 時間: 2025-3-29 09:32
Pers?nlichkeiten aus der Politikenergy tensors of simple forms determined by its null eigenvectors. By studying relations between eigenvectors of the symmetric and anti-symmetric parts, a complete classification of all conformal Lorentz transformation in any dimension is then obtained according to the null eigenvectors of the anti-symmetric parts.作者: fabricate 時間: 2025-3-29 13:48
Nationale Feiertage und Feste der Türkeiespective path are compared. We consider some numerical solutions of the shortest path equation, and show that there is no shortest path in the bulk for the Randall-Sundrum vacuum brane solution, the linear cosmological solution of Binétruy, et. al. for ω = —1,—2/3, and for some expanding brane universes.作者: Ophthalmoscope 時間: 2025-3-29 19:02 作者: 螢火蟲 時間: 2025-3-29 20:48
Relativistic Astrophysics intriguing features of black holes, singularities and hypotheses like the no-hair conjecture and cosmic censorship have been discussed for decades. Perturbative and numerical approaches are mandatory to tackle most of these issues.作者: 閃光東本 時間: 2025-3-30 03:48
Critical Phenomena in Gravitational Collapse: The Role of Angular Momentumlisionless particles, each with angular momentum). Using linear perturbation theory we show that in the former case there are still critical phenomena, explicitly predictingthe associated scalingla ws. We show that, on the contrary, critical phenomena are not generic for Vlasov matter.作者: Cumbersome 時間: 2025-3-30 04:20
The Detection of Gravitational Wavesh case will be assessed, as well as its intensity and deconvolution. Brief reference will also be made to detector sensitivity characterisation, including very summary data on current state of the art of GW detectors.作者: Ointment 時間: 2025-3-30 10:08 作者: 財政 時間: 2025-3-30 14:47 作者: 颶風 時間: 2025-3-30 19:57
Book 2003 black holes and evolution, relativistic stars and jet hydrodynamics, as well as the production and detection of gravitational waves. The book is complemented by further contributions and animation supplied on the accompanying CD-ROM.作者: keloid 時間: 2025-3-30 22:46
https://doi.org/10.1007/978-3-658-40584-7 like the ones usually associated with black hole spacetimes. As a test bed, the method has been applied to 3D metrics describing propagation of nonlinear gauge waves. Results are compared with the ones obtained with standard methods, showing a great increase in both robustness and stability of the numerical algorithm.作者: Palate 時間: 2025-3-31 04:05 作者: 吸氣 時間: 2025-3-31 07:01
?konometrie und maschinelles Lernench apparently allow superluminal travel, but are in fact flat Minkowski space-times. Therefore, to avoid these dificulties it is important to provide an appropriate definition of superluminal travel..We investigate these problems and the relationship between weak-energy-condition violation and superluminal travel.作者: 軟弱 時間: 2025-3-31 12:53
https://doi.org/10.1007/978-3-658-40584-7cy of even better resolved 2D codes. While traditional 2D codes show errors in quantities such as apparent horizon mass of over 100% by . ≈ 100., and crash by . ≈ 150., with our new techniques the same systems can be evolved for more than hundreds of .’s in full 3D with errors of only a few percent.作者: 證明無罪 時間: 2025-3-31 13:53
Gauge Conditions for Long-Term Numerical Black Hole Evolution With or Without Excisioncy of even better resolved 2D codes. While traditional 2D codes show errors in quantities such as apparent horizon mass of over 100% by . ≈ 100., and crash by . ≈ 150., with our new techniques the same systems can be evolved for more than hundreds of .’s in full 3D with errors of only a few percent.作者: Spina-Bifida 時間: 2025-3-31 18:10
https://doi.org/10.1007/978-3-658-40576-2 the second part, I will illustrate the use of HRSC methods in various astrophysical applications, where special and general relativistic hydrodynamical processes play a crucial role, such as: relativistic extragalactic jets, accretion onto compact objects, models of formation of Gamma-Ray Bursts, and stellar core collapse.作者: 壕溝 時間: 2025-4-1 00:11 作者: 行乞 時間: 2025-4-1 02:13 作者: 上流社會 時間: 2025-4-1 07:10
