標(biāo)題: Titlebook: Deterministic Chaos in General Relativity; David Hobill,Adrian Burd,Alan Coley Book 1994 Springer Science+Business Media New York 1994 cha [打印本頁] 作者: SCOWL 時間: 2025-3-21 17:43
書目名稱Deterministic Chaos in General Relativity影響因子(影響力)
書目名稱Deterministic Chaos in General Relativity影響因子(影響力)學(xué)科排名
書目名稱Deterministic Chaos in General Relativity網(wǎng)絡(luò)公開度
書目名稱Deterministic Chaos in General Relativity網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Deterministic Chaos in General Relativity被引頻次
書目名稱Deterministic Chaos in General Relativity被引頻次學(xué)科排名
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書目名稱Deterministic Chaos in General Relativity年度引用學(xué)科排名
書目名稱Deterministic Chaos in General Relativity讀者反饋
書目名稱Deterministic Chaos in General Relativity讀者反饋學(xué)科排名
作者: BUDGE 時間: 2025-3-21 20:19
https://doi.org/10.1007/978-3-319-10503-1en a perturbation is added to the system. By using the Melnikov method for detecting homoclinic chaos in near integrable systems, we conclude that, as one adds a time-periodic perturbation to the static black hole, a region of chaotic motion replaces the homoclinic orbit.作者: vasospasm 時間: 2025-3-22 04:22
On Defining Chaos in the Absence of Timed could be quite misleading. In particular, for any integer . > 1 we give an example of a completely integrable .-degree of freedom Hamiltonian system, with compact energy surfaces, having the property that the induced flows on almost all energy surfaces admit sensitive dependence on initial conditions.作者: 有偏見 時間: 2025-3-22 05:05
Particle Motion Around Perturbed Black Holes: The Onset of Chaosen a perturbation is added to the system. By using the Melnikov method for detecting homoclinic chaos in near integrable systems, we conclude that, as one adds a time-periodic perturbation to the static black hole, a region of chaotic motion replaces the homoclinic orbit.作者: Cardioplegia 時間: 2025-3-22 11:42
Critical Behaviour in Scalar Field Collapseack hole to spacetimes which do. The near critical regime, . ≈ .*, is characterized by a variety of non-linear phenomena including exponential sensitivity to initial conditions, scale-periodicity, and universal power-law dependence of black hole mass on parameter-space displacement |. ? .*|.作者: Ventilator 時間: 2025-3-22 13:59 作者: Ventilator 時間: 2025-3-22 18:01
Homoclinic Chaos in Relativistic Cosmologyone where the Universe may be described as a Hamiltonian dynamical system, and other where this is not possible, due to the presence of viscous matter. The overall implications of Chaos for Cosmology and General Relativity are discussed.作者: 離開就切除 時間: 2025-3-22 21:39
Classical and Quantum Chaos in Robertson-Walker Cosmologiesound the chaotic nucleus of the universe. On the quantum level we discuss particle creation, backscattering, anisotropy in the microwave background, parity violation and how all this relates to the multiple connectivity of the open spacelike slices.作者: 漸變 時間: 2025-3-23 02:51 作者: 多山 時間: 2025-3-23 06:21 作者: Obituary 時間: 2025-3-23 09:43
Medical Environment — Influences on Growtheatures, namely: (i) they allow chaos to be expressed in a gauge invariant way; (ii) they are structurally stable and (iii) in low density universes they result in radically different estimates of length scales with potentially important consequences for the interpretation of the angular variation of the background radiation.作者: 出血 時間: 2025-3-23 16:31
Book 1994prised of com- plex nonlinear systems that cannot be broken down into the behavior of their con- stituents and then reassembled to form the whole. The lack of a superposition principle in such systems has challenged researchers to use a variety of analytic and numerical methods in attempts to unders作者: 鴕鳥 時間: 2025-3-23 20:53 作者: Picks-Disease 時間: 2025-3-24 02:05
Complement Component (3b/4b) Receptor 1 (,),one where the Universe may be described as a Hamiltonian dynamical system, and other where this is not possible, due to the presence of viscous matter. The overall implications of Chaos for Cosmology and General Relativity are discussed.作者: 可能性 時間: 2025-3-24 03:08 作者: debble 時間: 2025-3-24 07:10 作者: 輕率的你 時間: 2025-3-24 10:50
Deterministic Chaos in General Relativity978-1-4757-9993-4Series ISSN 0258-1221 作者: Anal-Canal 時間: 2025-3-24 14:59
https://doi.org/10.1007/978-3-319-23995-8erence for these proceedings. The qualitative behaviour of both linear and non-linear autonomous differential equations is discussed. Particular attention is given to Liapunov stability theory, periodic orbits, limit sets, structural stability, and bifurcation theory, leading up to higher order systems and chaos.作者: Infelicity 時間: 2025-3-24 21:06 作者: 亂砍 時間: 2025-3-25 02:43
https://doi.org/10.1007/978-3-319-10503-1r a brief survey of available models, the relativistic kinematics and dynamics of cosmological models is developed. The “standard” (Friedman-Lema?tre-Robertson-Walker) models are described, then the Bianchi models, and finally some inhomogeneous cosmologies.作者: IDEAS 時間: 2025-3-25 04:28 作者: flammable 時間: 2025-3-25 07:58
https://doi.org/10.1007/978-3-030-43699-5This paper gives a short exposition of the use of normal form theory and reduction to study Hamiltonian systems which are perturbations of the harmonic oscillator..作者: CLASH 時間: 2025-3-25 15:32
Transformation of , ProtoplastsWe describe a method for proving the non-integrability of an analytic Hamiltonian system which does not appeal to the existence of chaotic motion.作者: 平 時間: 2025-3-25 17:25 作者: hypnotic 時間: 2025-3-25 23:57 作者: 遺留之物 時間: 2025-3-26 01:10 作者: Ccu106 時間: 2025-3-26 07:33 作者: Lethargic 時間: 2025-3-26 08:52 作者: 廢墟 時間: 2025-3-26 13:15 作者: Cumbersome 時間: 2025-3-26 20:17 作者: 講個故事逗他 時間: 2025-3-26 23:03 作者: cunning 時間: 2025-3-27 04:50
Shigeyuki Kawai Ph.D.,Kousaku Murata Ph.D.nate either at the black holes .. and .. (types (I) and (II)), or at infinity (type (III)). The limits of these three types of orbits are Cantor sets, defined by the unstable periodic orbits, that form a set of measure zero. In the case of particles with elliptic energy there are some stable periodi作者: 顯微鏡 時間: 2025-3-27 06:30 作者: 最初 時間: 2025-3-27 11:54
Anastomosis and Heterokaryon Formationtive mesh-refinement algorithm in conjunction with finite-difference techniques, I have studied the non-linear evolution of parameterized initial configurations .(., 0; .), where a critical parameter value, . = .*, generically demarcates the transition from spacetimes which do not contain a final bl作者: 方便 時間: 2025-3-27 13:52
https://doi.org/10.1007/978-3-319-10503-1r a brief survey of available models, the relativistic kinematics and dynamics of cosmological models is developed. The “standard” (Friedman-Lema?tre-Robertson-Walker) models are described, then the Bianchi models, and finally some inhomogeneous cosmologies.作者: Narrative 時間: 2025-3-27 20:12
Complement Component (3b/4b) Receptor 1 (,),hod for the detection of this kind of behavior. We describe in some detail two concrete manifestations of Homoclinic Chaos in relativistic Cosmology, one where the Universe may be described as a Hamiltonian dynamical system, and other where this is not possible, due to the presence of viscous matter作者: 我悲傷 時間: 2025-3-28 00:12
Medical Environment — Influences on Growth We find the mixing to be less pronounced than some of the claims made previously, nevertheless in low density universes the mechanism can give rise to appreciable mixing and result in a reduction in the measured cmwbr anisotropy on a range of angular scales. These models also have other important f作者: 強所 時間: 2025-3-28 02:51 作者: cluster 時間: 2025-3-28 10:18
Methods in Human Growth Geneticsgeneities of the distribution of galaxies by means of the Tolman solution of Einstein’s field equations for spherically symmetric dust in comoving coordinates. Such model is based on earlier works developed by L. Pietronero and J. R. Wertz on Newtonian cosmology, and the main points of these models 作者: 擁擠前 時間: 2025-3-28 11:01
J. C. van Wieringen,Machteld J. Roedece, imperfect fluid Bianchi models with ‘dimensionless’ equations of state are shown to have self-similar asymptotic solutions. Conversely, it is also shown that if the spacetime is self-similar, then the resulting equations of state must be of this same ‘dimensionless’ form. The conditions under wh作者: crucial 時間: 2025-3-28 17:20 作者: 精美食品 時間: 2025-3-28 22:32 作者: 注意到 時間: 2025-3-28 23:23
978-1-4757-9995-8Springer Science+Business Media New York 1994作者: 我說不重要 時間: 2025-3-29 04:12 作者: 陰險 時間: 2025-3-29 07:53
A Short Course on Chaotic Hamiltonian Systemsamilton’s equations, as would be encountered in elementary mechanics courses, is assumed. The treatment of geodesic flows in Section 3 is somewhat in the spirit of symplectic mechanics, but classical notation is emphasized. The presentation is rigorous only in Section 1, which is quite elementary. References for further study are provided.作者: GROUP 時間: 2025-3-29 14:23
Relativistic Cosmologiesr a brief survey of available models, the relativistic kinematics and dynamics of cosmological models is developed. The “standard” (Friedman-Lema?tre-Robertson-Walker) models are described, then the Bianchi models, and finally some inhomogeneous cosmologies.作者: STEER 時間: 2025-3-29 16:13
0258-1221 struction of exact solutions to the Einstein equations. However, most of those solutions are nonphysical and of those that do have a physical significance, many978-1-4757-9995-8978-1-4757-9993-4Series ISSN 0258-1221 作者: 樹木心 時間: 2025-3-29 21:58
Chaos in the Case of Two Fixed Black Holesall into the corresponding black hole. For certain values of the parameters one or both satellite orbits may not exist. Then the separation of the type (I) and/or type (II) orbits is done by some almost hyperbolic orbits. In the Newtonian case the satellite orbits around .. and .. never exist (excep作者: Connotation 時間: 2025-3-30 00:19
Relativistic Fractal Cosmologiese density with the distance as a power law (the de Vaucouleurs’ density power law), the fractal dimension within the range 1 ≤ . ≤ 2, and the present range of uncertainty for the Hubble constant. The spatially homogeneous Friedmann model is discussed as a special case of the Tolman solution, and it 作者: 彎曲的人 時間: 2025-3-30 07:01 作者: 厭煩 時間: 2025-3-30 09:55
Methods in Human Growth Geneticse density with the distance as a power law (the de Vaucouleurs’ density power law), the fractal dimension within the range 1 ≤ . ≤ 2, and the present range of uncertainty for the Hubble constant. The spatially homogeneous Friedmann model is discussed as a special case of the Tolman solution, and it 作者: Ardent 時間: 2025-3-30 15:30 作者: 表狀態(tài) 時間: 2025-3-30 18:44
Introduction to Dynamical Systemserence for these proceedings. The qualitative behaviour of both linear and non-linear autonomous differential equations is discussed. Particular attention is given to Liapunov stability theory, periodic orbits, limit sets, structural stability, and bifurcation theory, leading up to higher order syst作者: Infinitesimal 時間: 2025-3-30 21:05 作者: escalate 時間: 2025-3-31 01:46
On Defining Chaos in the Absence of Timee of initial values. Using the recent discovery that the sensitivity hypothesis is a logical consequence of the other two conditions we formulate a time-and-metric independent concept of chaos for foliations which implies the usual definition when the leaves are the orbits of a flow on a manifold. S作者: Radiculopathy 時間: 2025-3-31 08:32
Chaos in the Case of Two Fixed Black Holesnate either at the black holes .. and .. (types (I) and (II)), or at infinity (type (III)). The limits of these three types of orbits are Cantor sets, defined by the unstable periodic orbits, that form a set of measure zero. In the case of particles with elliptic energy there are some stable periodi作者: Metamorphosis 時間: 2025-3-31 11:40 作者: CREST 時間: 2025-3-31 16:09 作者: 幸福愉悅感 時間: 2025-3-31 19:46 作者: 無能力之人 時間: 2025-4-1 00:07
