標題: Titlebook: General Relativity, Cosmology and Astrophysics; Perspectives 100 yea Ji?í Bi?ák,Tomá? Ledvinka Book 2014 Springer International Publishing [打印本頁] 作者: 萬圣節(jié) 時間: 2025-3-21 19:06
書目名稱General Relativity, Cosmology and Astrophysics影響因子(影響力)
書目名稱General Relativity, Cosmology and Astrophysics影響因子(影響力)學科排名
書目名稱General Relativity, Cosmology and Astrophysics網(wǎng)絡(luò)公開度
書目名稱General Relativity, Cosmology and Astrophysics網(wǎng)絡(luò)公開度學科排名
書目名稱General Relativity, Cosmology and Astrophysics被引頻次
書目名稱General Relativity, Cosmology and Astrophysics被引頻次學科排名
書目名稱General Relativity, Cosmology and Astrophysics年度引用
書目名稱General Relativity, Cosmology and Astrophysics年度引用學科排名
書目名稱General Relativity, Cosmology and Astrophysics讀者反饋
書目名稱General Relativity, Cosmology and Astrophysics讀者反饋學科排名
作者: 笨拙的我 時間: 2025-3-21 21:52
https://doi.org/10.1007/978-3-319-06349-2Anti-de Sitter Spacetime; Black Branes; Black Holes; Cosmological Models; Ergosphere; Loop Quantum Gravit作者: Celiac-Plexus 時間: 2025-3-22 02:49 作者: Indicative 時間: 2025-3-22 07:53
Jeannette Den Ouden,Fred Janssen then the target of different observers: a suitable algorithm to compare among their measurements should necessarily be developed, either formally or operationally. This is the task of what we call “theory of measurement,” which we discuss here in the framework of general relativity.作者: 耐寒 時間: 2025-3-22 09:37
Susan Gair,Tamar Hager,Omri Herzogndard, single-field slow-roll inflation, and the curvature and tensor perturbations produced from it, we discuss possible sources of nonlinear, non-Gaussian perturbations in other models of inflation. Then we describe the so-called . formalism, which is a powerful tool for evaluating nonlinear curvature perturbations on super Hubble scales.作者: 大猩猩 時間: 2025-3-22 16:25 作者: 大猩猩 時間: 2025-3-22 20:20
Observers, Observables and Measurements in General Relativity then the target of different observers: a suitable algorithm to compare among their measurements should necessarily be developed, either formally or operationally. This is the task of what we call “theory of measurement,” which we discuss here in the framework of general relativity.作者: Constitution 時間: 2025-3-22 22:00
Inflation and Birth of Cosmological Perturbationsndard, single-field slow-roll inflation, and the curvature and tensor perturbations produced from it, we discuss possible sources of nonlinear, non-Gaussian perturbations in other models of inflation. Then we describe the so-called . formalism, which is a powerful tool for evaluating nonlinear curvature perturbations on super Hubble scales.作者: Stress-Fracture 時間: 2025-3-23 03:58 作者: jocular 時間: 2025-3-23 05:55
Higher-Dimensional Black HolesThis article reviews black hole solutions of higher-dimensional General Relativity. The focus is on stationary vacuum solutions and recent work on instabilities of such solutions.作者: Priapism 時間: 2025-3-23 12:40
978-3-319-38034-6Springer International Publishing Switzerland 2014作者: Femish 時間: 2025-3-23 17:42 作者: ALIBI 時間: 2025-3-23 21:51 作者: Valves 時間: 2025-3-23 23:52
Stefan C. Müller,Peter J. Plath,Armin Fuchs1912, discuss Einstein’s papers on gravitation from that period and emphasize which new concepts and ideas he introduced. I also want to indicate how the main themes that preoccupied him then, the principle of equivalence, bending of light, gravitational redshift and frame dragging effects, are aliv作者: ENNUI 時間: 2025-3-24 03:33
Jeannette Den Ouden,Fred Janssen then the target of different observers: a suitable algorithm to compare among their measurements should necessarily be developed, either formally or operationally. This is the task of what we call “theory of measurement,” which we discuss here in the framework of general relativity.作者: 生氣地 時間: 2025-3-24 09:31 作者: cyanosis 時間: 2025-3-24 14:21 作者: concentrate 時間: 2025-3-24 15:23
Complexity in New Product Development, the problem lends itself to a perturbative treatment, wherein corrections to the geodesic motion of the smaller object (due to radiation reaction, internal structure, etc.) are accounted for order by order in ., using the language of an effective .. The prospect for observing gravitational waves f作者: 糾纏 時間: 2025-3-24 22:46 作者: PRISE 時間: 2025-3-25 02:30
https://doi.org/10.1007/978-3-031-30727-0ble MOTS play an interesting role in a number of geometric inequalities involving physical parameters such as area, mass, charge or, in the axially symmetric case, angular momentum. Some of those inequalities are global in nature while others are local, with interesting relationships between them. I作者: Flu表流動 時間: 2025-3-25 05:54 作者: 拔出 時間: 2025-3-25 11:34 作者: 悅耳 時間: 2025-3-25 14:23 作者: PAGAN 時間: 2025-3-25 19:23
Sebastian Bachmann,Simon Fechnern. We demonstrate that these properties are connected with and generated by a special geometrical object, the Principal Conformal Killing-Yano tensor (PCKYT). The most general solution, describing such black holes, Kerr-NUT-ADS metric, admits this structure. Moreover a solution of the Einstein Equat作者: 外露 時間: 2025-3-25 23:41 作者: 背書 時間: 2025-3-26 03:14 作者: 身體萌芽 時間: 2025-3-26 06:32
https://doi.org/10.1007/978-3-322-87005-6ting for the observed inhomogeneities in the cosmic microwave background already illustrates this point to a certain extent because the paradigm is based on quantum field theory on the curved cosmological space-times. However, this analysis excludes the Planck era because the background space-time s作者: FRET 時間: 2025-3-26 11:28
0168-1222 Classical General Relativity, (iii) Cosmology and Quantum Gravity, and (iv) Numerical Relativity and Relativistic Astrophysics..978-3-319-38034-6978-3-319-06349-2Series ISSN 0168-1222 Series E-ISSN 2365-6425 作者: hemophilia 時間: 2025-3-26 16:05
Gravitational Self-Force: Orbital Mechanics Beyond Geodesic Motionic effects of the self-force, including the . correction to the precession rate of the periastron. I will highlight the way in which such calculations allow us to make a fruitful contact with other approaches to the two-body problem.作者: 哀求 時間: 2025-3-26 17:09
Dynamic and Thermodynamic Stability of Black Holes and Black Branesar momentum. However, we prove that all black branes corresponding to thermodynamically unstable black holes are dynamically unstable, as conjectured by Gubser and Mitra. We also prove that positivity of . is equivalent to the satisfaction of a “l(fā)ocal Penrose inequality,” thus showing that satisfact作者: nepotism 時間: 2025-3-26 21:06
Loop Quantum Gravity and the Planck Regime of Cosmology relation involving the scalar and tensor power spectra and a new source for non-Gaussianities. The genesis of the large scale structure of the universe can be traced back to quantum gravity fluctuations in the Planck regime. This report provides a bird’s eye view of these developments for the gener作者: 典型 時間: 2025-3-27 01:59
Book 2014ext 100 years. .The content is divided into four broad parts: (i) Gravity and Prague, (ii) Classical General Relativity, (iii) Cosmology and Quantum Gravity, and (iv) Numerical Relativity and Relativistic Astrophysics..作者: 抗生素 時間: 2025-3-27 07:13
Complexity in New Product Developmentic effects of the self-force, including the . correction to the precession rate of the periastron. I will highlight the way in which such calculations allow us to make a fruitful contact with other approaches to the two-body problem.作者: 割讓 時間: 2025-3-27 09:48 作者: 溺愛 時間: 2025-3-27 16:36 作者: 思考而得 時間: 2025-3-27 18:16
Hamiltonian Formalism for Spinning Black Holes in General Relativityst-Newtonian Hamiltonians are given in explicit analytic forms. A next-to-leading order in spin generalization is presented, others are mentioned. Comparisons between the Hamiltonian formalisms by ADM, Dirac, and Schwinger are made.作者: Popcorn 時間: 2025-3-27 22:44
Stability of Marginally Outer Trapped Surfaces and Geometric Inequalitiesmmetric case, angular momentum. Some of those inequalities are global in nature while others are local, with interesting relationships between them. In this lecture the notion of stable MOTS will be reviewed and some of the geometric inequalities involving stable MOTS will be described.作者: 路標 時間: 2025-3-28 03:03
Stationary Black-Hole Binaries: A Non-existence Proofroperties, we present a non-existence proof for the equilibrium configuration in question. From a mathematical point of view, this result is a further example for the efficiency of the inverse (“scattering”) method in non-linear theories.作者: 重畫只能放棄 時間: 2025-3-28 10:07
Instability of Anti-de Sitter Spacetimemation for a large class of initial data arbitrarily close to the AdS solution. We conjecture that this instability is triggered by a resonant mode mixing which gives rise to diffusion of energy from low to high frequencies.作者: Muscularis 時間: 2025-3-28 13:54 作者: dry-eye 時間: 2025-3-28 18:38 作者: 努力趕上 時間: 2025-3-28 19:56
Some Links Between General Relativity and Other Parts of Physicses is of course an old one, but recently, because of advances in technology, these questions have become more topical. In this talk I will illustrate this theme by examples drawn from optics, acoustics, liquid crystals, graphene and the currently popular topic of cloaking.作者: DEFER 時間: 2025-3-28 23:29
Black Holes, Hidden Symmetry and Complete Integrability: Brief Reviewions with (or without) a cosmological constant which possesses PCKYT is the Kerr-NUT-ADS metric. This object (PCKYT) is responsible for such remarkable properties of higher dimensional rotating black holes as: (i) complete integrability of geodesic equations and (ii) complete separation of variables of the important field equations.作者: thrombosis 時間: 2025-3-29 03:11
https://doi.org/10.1007/978-3-030-79084-4l world of the last vestiges of the purely geometrical Ptolemaic world view; and the precise formulation of Mach’s principle required to place GR correctly in the line of conceptual and technical evolution that began with the ancient Greek astronomers.作者: 命令變成大炮 時間: 2025-3-29 08:12 作者: 向下五度才偏 時間: 2025-3-29 11:35 作者: Choreography 時間: 2025-3-29 16:19 作者: 裹住 時間: 2025-3-29 20:39
The General Relativistic Two Body Problem and the Effective One Body Formalismlf-Force (GSF) computations, the EOB formalism is likely to provide an efficient way of computing the very many accurate template waveforms that are needed for Gravitational Wave (GW) data analysis purposes.作者: 財主 時間: 2025-3-30 00:34
Cosmological Models and Stability start by comparing the role of the equivalence principle to that of the principles used in cosmology. I will then briefly describe the standard model of cosmology to give a perspective on some mathematical problems and conjectures on cosmological models, which are discussed in the later part of this paper.作者: ESPY 時間: 2025-3-30 07:58 作者: cluster 時間: 2025-3-30 09:35
0168-1222 0 years after Einstein in Prague.Includes historical notes o.The articles included in this Volume represent a broad and highly qualified view on the present state of general relativity, quantum gravity, and their cosmological and astrophysical implications. As such, it may serve as a valuable source作者: 嗎啡 時間: 2025-3-30 15:57 作者: Benzodiazepines 時間: 2025-3-30 16:44 作者: 表被動 時間: 2025-3-30 23:55
Why Does Nobody Know Anything Anymore?,roperties, we present a non-existence proof for the equilibrium configuration in question. From a mathematical point of view, this result is a further example for the efficiency of the inverse (“scattering”) method in non-linear theories.作者: 口味 時間: 2025-3-31 03:04 作者: Infantry 時間: 2025-3-31 08:40 作者: Resign 時間: 2025-3-31 12:02
Einstein in Prague: Relativity Then and Now1912, discuss Einstein’s papers on gravitation from that period and emphasize which new concepts and ideas he introduced. I also want to indicate how the main themes that preoccupied him then, the principle of equivalence, bending of light, gravitational redshift and frame dragging effects, are aliv作者: 假 時間: 2025-3-31 15:56
Observers, Observables and Measurements in General Relativity then the target of different observers: a suitable algorithm to compare among their measurements should necessarily be developed, either formally or operationally. This is the task of what we call “theory of measurement,” which we discuss here in the framework of general relativity.作者: 揮舞 時間: 2025-3-31 17:52
Some Links Between General Relativity and Other Parts of Physicste physics courses, it is natural to ask: how can its basic concepts and techniques be used to illuminate areas of physics which have no connection with gravity? Another way of asking this question is: are the analogues situations to those occurring in General Relativity? The search for such analogu
