標(biāo)題: Titlebook: Einstein‘s General Theory of Relativity; With Modern Applicat ?yvind Gr?n,Sigbj?rn Hervik Textbook 2007 Springer-Verlag New York 2007 Cosmo [打印本頁] 作者: CHARY 時間: 2025-3-21 19:59
書目名稱Einstein‘s General Theory of Relativity影響因子(影響力)
書目名稱Einstein‘s General Theory of Relativity影響因子(影響力)學(xué)科排名
書目名稱Einstein‘s General Theory of Relativity網(wǎng)絡(luò)公開度
書目名稱Einstein‘s General Theory of Relativity網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Einstein‘s General Theory of Relativity被引頻次
書目名稱Einstein‘s General Theory of Relativity被引頻次學(xué)科排名
書目名稱Einstein‘s General Theory of Relativity年度引用
書目名稱Einstein‘s General Theory of Relativity年度引用學(xué)科排名
書目名稱Einstein‘s General Theory of Relativity讀者反饋
書目名稱Einstein‘s General Theory of Relativity讀者反饋學(xué)科排名
作者: extemporaneous 時間: 2025-3-21 21:10
Homogeneous and Isotropic Universe Modelsthe General Theory of Relativity, Einstein realized that this theory actually could say something about the universe and constructed a static universemodel as a solution of the relativistic field equations. The era of modern cosmology had begun, which would revolutionize our view of the universe.作者: Angioplasty 時間: 2025-3-22 03:04
Anisotropic and Inhomogeneous Universe Modelsll investigate the Bianchi type I universe model and the inhomogeneous Lema?tre-Tolman-Bondi (LTB) universe models. The Bianchi type I model is the simplest of the spatially homogeneous models which allows for anisotropy and the LTB-models are inhomogeneous universe models with spherically symmetric three-space.作者: condone 時間: 2025-3-22 05:33 作者: 能得到 時間: 2025-3-22 08:48
and are not present in other textbooks.Standard model of cos.The book introduces the general theory of relativity and includes applications to cosmology.? The book contains a thorough introduction to tensor calculus and curved manifolds.? After the necessary mathematical tools are introduced, we giv作者: 健壯 時間: 2025-3-22 16:28 作者: 健壯 時間: 2025-3-22 19:56 作者: Integrate 時間: 2025-3-22 22:01
Gek, Experimentele psychopathologieuch behaviour as we will show in this chapter. We will first start with the static solution that Einstein found and was the reason that Einstein introduced the cosmological constant in the first place.作者: probate 時間: 2025-3-23 03:40
Universe Models with Vacuum Energyuch behaviour as we will show in this chapter. We will first start with the static solution that Einstein found and was the reason that Einstein introduced the cosmological constant in the first place.作者: 網(wǎng)絡(luò)添麻煩 時間: 2025-3-23 05:33 作者: Cosmopolitan 時間: 2025-3-23 11:17 作者: 彎曲的人 時間: 2025-3-23 15:16 作者: 正面 時間: 2025-3-23 19:03
https://doi.org/10.1007/978-3-642-04907-1the General Theory of Relativity, Einstein realized that this theory actually could say something about the universe and constructed a static universemodel as a solution of the relativistic field equations. The era of modern cosmology had begun, which would revolutionize our view of the universe.作者: Commentary 時間: 2025-3-23 22:57 作者: painkillers 時間: 2025-3-24 04:38
https://doi.org/10.1007/978-0-387-69200-5Cosmology; EFE; Gravity; RMS; Relativity; SR; Special relativity; Universe; general relativity; general theor作者: Hdl348 時間: 2025-3-24 10:17
978-1-4419-2406-3Springer-Verlag New York 2007作者: 六邊形 時間: 2025-3-24 14:14
https://doi.org/10.1007/978-3-7091-0585-6To obtain a mathematical description of physical phenomena, it is advantageous to introduce a reference frame in order to keep track of the position of events in space and time. The choice of reference frame has historically depended upon the view of human beings and their position in the Universe.作者: 詳細(xì)目錄 時間: 2025-3-24 17:04
https://doi.org/10.1007/978-3-662-65801-7In this chapter we shall give a short introduction to the fundamental principles of the special theory of relativity, and deduce some of the consequences of the theory.作者: Mediocre 時間: 2025-3-24 19:17
,Wahrnehmungsf?higkeit/Kreativit?t,In this chapter we are going to introduce the basic concepts necessary to grasp the geometrical significance of the metric tensor.作者: declamation 時間: 2025-3-25 01:47
https://doi.org/10.1007/978-3-662-43756-8In this chapter we shall consider some consequences of the formalism developed so far, by studying the relativistic kinematics in two types of non-inertial reference frames: the rotating reference frame and the uniformly accelerating reference frame.作者: Heresy 時間: 2025-3-25 05:30
https://doi.org/10.1007/978-3-662-28706-4In this chapter we will perform a 3+1 decomposition of the spacetime. This decomposition is very useful for various applications, in particular, we will use the 3+1 decomposition to derive a Lagrangian and Hamiltonian formalismof general relativity. We will also see howthe singularity theoremcan be described in this framework.作者: FELON 時間: 2025-3-25 10:56
Relativity Principles and GravitationTo obtain a mathematical description of physical phenomena, it is advantageous to introduce a reference frame in order to keep track of the position of events in space and time. The choice of reference frame has historically depended upon the view of human beings and their position in the Universe.作者: 清楚 時間: 2025-3-25 13:30 作者: Orchiectomy 時間: 2025-3-25 17:26 作者: 擺動 時間: 2025-3-25 23:07
Non-inertial Reference FramesIn this chapter we shall consider some consequences of the formalism developed so far, by studying the relativistic kinematics in two types of non-inertial reference frames: the rotating reference frame and the uniformly accelerating reference frame.作者: Guaff豪情痛飲 時間: 2025-3-26 03:15
Covariant Decomposition, Singularities, and Canonical CosmologyIn this chapter we will perform a 3+1 decomposition of the spacetime. This decomposition is very useful for various applications, in particular, we will use the 3+1 decomposition to derive a Lagrangian and Hamiltonian formalismof general relativity. We will also see howthe singularity theoremcan be described in this framework.作者: 離開可分裂 時間: 2025-3-26 05:43 作者: Irksome 時間: 2025-3-26 12:18 作者: Accede 時間: 2025-3-26 16:03 作者: chisel 時間: 2025-3-26 18:51
https://doi.org/10.1007/978-3-8349-6454-0d gravitational masses, was that there is no gravitational force at all. What is said to be “particle motion under the influence of the gravitational force” in Newtonian theory, is according to the general theory of relativity, free motion along geodesic curves in a curved space-time.作者: 偽善 時間: 2025-3-26 22:49
Markus Hoffmann,Thorsten S. Richterhe gravitational field moves slowly compared to the velocity of light. In the case of mass distributions of limited extension the field is weak at distances much larger than the Schwarzschild radius of the mass (see Chapter 10). At such distances the absolute value of the gravitational potential is 作者: Hemoptysis 時間: 2025-3-27 02:41 作者: 其他 時間: 2025-3-27 06:37 作者: 暖昧關(guān)系 時間: 2025-3-27 11:16
Gek, Experimentele psychopathologieevelopments in the last decades that have given new life to the cosmological constant. Firstly, the idea of . gave cosmology a whole new view upon the first split second of our universe. A key ingredient in the inflationary model is the behaviour of models that have a cosmological constant-like beha作者: flaunt 時間: 2025-3-27 14:16
Medien professionell einsetzen,teresting models of our universe. Actually, one of the main goals of cosmology today is to . the isotropy and homogeneity the universe has and in order to explain a certain property of the universe one has to consider sufficiently generalmodels that need not have this property. In this chapter we wi作者: atopic-rhinitis 時間: 2025-3-27 18:28 作者: DEFER 時間: 2025-3-28 00:19
Psychologische Klassifizierung,hapter. We know that in physics and mathematics, integration and differentiation are important, if not essential, operations that appear in almost all physical theories. In this chapter we will explore differentiation on curved manifolds and reveal several interesting properties.作者: Benign 時間: 2025-3-28 02:04 作者: perjury 時間: 2025-3-28 10:02 作者: modest 時間: 2025-3-28 10:45
Differentiation, Connections, and Integrationhapter. We know that in physics and mathematics, integration and differentiation are important, if not essential, operations that appear in almost all physical theories. In this chapter we will explore differentiation on curved manifolds and reveal several interesting properties.作者: aviator 時間: 2025-3-28 15:36
Einstein’s Field Equationsd gravitational masses, was that there is no gravitational force at all. What is said to be “particle motion under the influence of the gravitational force” in Newtonian theory, is according to the general theory of relativity, free motion along geodesic curves in a curved space-time.作者: outer-ear 時間: 2025-3-28 20:30 作者: mechanical 時間: 2025-3-29 02:33 作者: 閃光你我 時間: 2025-3-29 06:39
Vectors, Tensors, and Formsformalism will be used to give a mathematical formulation of the fundamental principles of the general theory of relativity. It will also be employed to give an invariant formulation of Maxwell’s equations so that the equations can be applied with reference to an arbitrary basis in curved spacetime.作者: 絆住 時間: 2025-3-29 07:30 作者: 顛簸地移動 時間: 2025-3-29 12:06
Curvature It is easy to visualize curves and surfaces in three-dimensional space but it is difficult to grasp visually what curvature means in three-dimensional space, or worse still, in four-dimensional space-time. However the curvature of such spacesmay be discussed using the lower dimensional analogues of作者: 中和 時間: 2025-3-29 16:35 作者: Cardiac 時間: 2025-3-29 22:25
The Linear Field Approximationhe gravitational field moves slowly compared to the velocity of light. In the case of mass distributions of limited extension the field is weak at distances much larger than the Schwarzschild radius of the mass (see Chapter 10). At such distances the absolute value of the gravitational potential is 作者: antedate 時間: 2025-3-30 02:59
The Schwarzschild Solution and Black Holesn to these equations. The solution is due to the astronomer Karl Schwarzschild, and in his honour the solution is referred to as the .. This solution represents a spacetime outside a non-rotating black hole. The Kerr solution representing spacetime outside a rotating black hole will also be deduced.作者: concentrate 時間: 2025-3-30 04:42
Homogeneous and Isotropic Universe Modelsvitation, involves attraction between celestial bodies. However, very little is said of the evolution of the universe itself. The universe was believed to be static, and its evolution was beyond any physical theory. But after the year 1917, things were different. Within two years after the birth of 作者: DRAFT 時間: 2025-3-30 09:31
Universe Models with Vacuum Energyevelopments in the last decades that have given new life to the cosmological constant. Firstly, the idea of . gave cosmology a whole new view upon the first split second of our universe. A key ingredient in the inflationary model is the behaviour of models that have a cosmological constant-like beha作者: 在駕駛 時間: 2025-3-30 12:35
Anisotropic and Inhomogeneous Universe Modelsteresting models of our universe. Actually, one of the main goals of cosmology today is to . the isotropy and homogeneity the universe has and in order to explain a certain property of the universe one has to consider sufficiently generalmodels that need not have this property. In this chapter we wi作者: Enrage 時間: 2025-3-30 19:59
d to the coming decades of Public Health - what are the next steps to primary prevention and health promotion...This must-have reference work is designed for practitioners, students, theorists, and researchers working in psychology, sociology, social work, nursing and medicine within the realm of Public Health. .
