標(biāo)題: Titlebook: General Relativity and Gravitational Waves; Essentials of Theory Sanjeev Dhurandhar,Sanjit Mitra Textbook 2022 The Editor(s) (if applicable [打印本頁(yè)] 作者: GRASS 時(shí)間: 2025-3-21 18:20
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作者: –DOX 時(shí)間: 2025-3-22 00:10
Overview of Special Relativity,In this chapter we give a short review of Einstein’s special theory of relativity.作者: adequate-intake 時(shí)間: 2025-3-22 01:59 作者: larder 時(shí)間: 2025-3-22 07:26
Jean-Luc Brylinski,Steven Zucker the development of the algebra of tensors. We purposely do this in the familiar setting (to the student) of a Euclidean space but with curvilinear coordinates. The advantage is that we can always transform to Cartesian coordinates in which the situation is more simply described. Since the analysis 作者: 赤字 時(shí)間: 2025-3-22 11:34
https://doi.org/10.1007/978-4-431-30962-8n a tensor—because tensors are coordinate independent quantities. For this purpose, we need to define parallel transport of vectors or in general of tensors. We limit ourselves to Riemannian parallel transport which is relevant to general relativity. It is defined here in a natural way using Cartesi作者: Oscillate 時(shí)間: 2025-3-22 15:42 作者: Oscillate 時(shí)間: 2025-3-22 17:45
https://doi.org/10.1007/978-94-011-6570-9tion. Historically it was the first solution obtained to Einstein’s equations by Karl Schwarzschild in 1916. In full vacuum, this is a black hole solution with an event horizon at .. Since the primary property of the event horizon is its one way character, we discuss the concept of a one-way membran作者: 規(guī)范就好 時(shí)間: 2025-3-23 00:02
https://doi.org/10.1007/978-1-4684-7730-6use of the gravitational field of a massive object, (ii) the perihelion shift in Mercury’s orbit around the Sun—the precession of Mercury’s elliptical orbit, (iii) the gravitational red-shift and the Pound-Rebka experiment and (iv) finally, Shapiro time delay—where light or radar waves experience a 作者: Maximize 時(shí)間: 2025-3-23 03:47
Complex Numbers in Trigonometric Form, in the theory of general relativity. It is easier to see this in the weak field limit. In the strong field regime there do exist gravitational wave solutions, but we will not consider them here. This is because, astrophysically we expect the waves to be weak, the term “weak” is made more precise la作者: AORTA 時(shí)間: 2025-3-23 09:02
https://doi.org/10.1007/0-8176-4449-0in the time or Fourier domain as is required. Then we give a brief description of introductory statistics such as probability, random variables etc. so that the noisy data may be statistically characterised. We then discuss the matched filtering of signals buried in noisy data which must be extracte作者: 公理 時(shí)間: 2025-3-23 10:19 作者: 收到 時(shí)間: 2025-3-23 14:35 作者: Excise 時(shí)間: 2025-3-23 19:02
The Equivalence Principle,We describe the broad physical concepts of the weak and strong equivalence principles, that form the foundation of the general theory of relativity. We make use of some of the well known thought experiments to explain and elaborate on these concepts.作者: debris 時(shí)間: 2025-3-23 22:51 作者: gastritis 時(shí)間: 2025-3-24 04:19 作者: 使長(zhǎng)胖 時(shí)間: 2025-3-24 08:24 作者: 宣傳 時(shí)間: 2025-3-24 13:04
Textbook 2022advanced topics covered in this book is the fundamentals of gravitational wave data analysis, filling a gap in textbooks on general relativity. The topic blends smoothly with other chapters in the book not only because of the common area of research, but it uses similar differential geometric and al作者: 諂媚于人 時(shí)間: 2025-3-24 15:31
Jean-Luc Brylinski,Steven Zucker be used to raise and lower indices of tensors. This is explicitly demonstrated in an oblique Cartesian coordinate system to connect a contravariant vector with a covariant vector and regard it as the same entity (isomorphic) with contravariant and covariant components.作者: blight 時(shí)間: 2025-3-24 20:05 作者: Acetaldehyde 時(shí)間: 2025-3-25 02:05
Complex Numbers in Trigonometric Form,eed to consider only the weak field approximation and not slow motion—after all the GW, as we will show later, travel at the speed .. In order to make the weak field approximation we need to linearise Einstein’s equations. Note that since this is not the Newtonian approximation, because we allow spe作者: ensemble 時(shí)間: 2025-3-25 04:09 作者: 左右連貫 時(shí)間: 2025-3-25 09:49
Correction to: General Relativity and Gravitational Waves,作者: 打算 時(shí)間: 2025-3-25 15:22 作者: FILLY 時(shí)間: 2025-3-25 16:54
Tensor Algebra, be used to raise and lower indices of tensors. This is explicitly demonstrated in an oblique Cartesian coordinate system to connect a contravariant vector with a covariant vector and regard it as the same entity (isomorphic) with contravariant and covariant components.作者: Palpate 時(shí)間: 2025-3-25 21:51 作者: degradation 時(shí)間: 2025-3-26 02:02 作者: interlude 時(shí)間: 2025-3-26 06:06
Gravitational Wave Data Analysis,posed in a differential geometric framework. We show how a metric can be defined on the signal manifold and can be used to place templates in the parameter space in an efficient way. The Fisher information matrix and the Rao-Cramer bound are discussed in the context of estimation of errors in parame作者: lymphoma 時(shí)間: 2025-3-26 12:24
Textbook 2022irst time. Both authors have been teaching the course in various forms for a few decades and have designed the book as a one stop book at basic level including derivations and exercises...A spectacular prediction of general relativity is gravitational waves. Gravitational waves were first detected b作者: 并排上下 時(shí)間: 2025-3-26 14:41 作者: PALSY 時(shí)間: 2025-3-26 19:08
,Einstein’s Equations,portant cases such as dust and perfect fluid. The chapter ends with the Newtonian limit of Einstein’s equations in the low velocity, weak field limit, where it is shown that Einstein’s gravity goes over to Newtonian gravity. When obtaining this limit the constant . relating the two sides of Einstein’s equations is determined.作者: custody 時(shí)間: 2025-3-26 23:11 作者: Palliation 時(shí)間: 2025-3-27 04:08
The Geometry of Curved Spaces and Tensor Calculus,e laws of special relativity are valid. We further describe geodesics as special curves in a curved spacetime. We show how the deviation of neighbouring geodesics can be used to measure the curvature of a spacetime. Further, the Ricci tensor and scalar curvature are defined from which the Einstein tensor is built.作者: ureter 時(shí)間: 2025-3-27 05:21
2198-7882 s for researchers entering the field.Is the first introducto.This book serves as a textbook for senior undergraduate students who are learning the subject of general relativity and gravitational waves for the first time. Both authors have been teaching the course in various forms for a few decades a作者: 格子架 時(shí)間: 2025-3-27 12:14 作者: 動(dòng)機(jī) 時(shí)間: 2025-3-27 16:39 作者: 恃強(qiáng)凌弱 時(shí)間: 2025-3-27 21:43 作者: keloid 時(shí)間: 2025-3-27 23:16 作者: Introduction 時(shí)間: 2025-3-28 06:00
The Geometry of Curved Spaces and Tensor Calculus,n a tensor—because tensors are coordinate independent quantities. For this purpose, we need to define parallel transport of vectors or in general of tensors. We limit ourselves to Riemannian parallel transport which is relevant to general relativity. It is defined here in a natural way using Cartesi作者: Hallowed 時(shí)間: 2025-3-28 08:58 作者: Aqueous-Humor 時(shí)間: 2025-3-28 11:23
Schwarzschild Solution and Black Holes,tion. Historically it was the first solution obtained to Einstein’s equations by Karl Schwarzschild in 1916. In full vacuum, this is a black hole solution with an event horizon at .. Since the primary property of the event horizon is its one way character, we discuss the concept of a one-way membran作者: CRATE 時(shí)間: 2025-3-28 17:30 作者: dendrites 時(shí)間: 2025-3-28 21:21 作者: 脆弱么 時(shí)間: 2025-3-29 01:40
Gravitational Wave Data Analysis,in the time or Fourier domain as is required. Then we give a brief description of introductory statistics such as probability, random variables etc. so that the noisy data may be statistically characterised. We then discuss the matched filtering of signals buried in noisy data which must be extracte作者: eulogize 時(shí)間: 2025-3-29 04:14
Morphologische Untersuchungen an der Eihautiedene Frage, ob die aus dem Fruchtwasser isolierbaren Phospholipide in der fetalen Lunge oder im Amnionepithel gebildet werden oder an beiden Stellen. Sie k?nnten durch Exozytose aus dem Amnionepithel in das Fruchtwasser abgegeben werden (Schmidt et al. 1982).作者: 旋轉(zhuǎn)一周 時(shí)間: 2025-3-29 08:07 作者: Misnomer 時(shí)間: 2025-3-29 11:36
?- nis in der nahen Zukunft aussehen wird. Welche Sachfragen werden die bila- ralen Beziehungen pr?gen? Was verbindet und was trennt die beiden L?nder mit Blick auf die heute schon absehbaren politischen Entwicklungen? Haben W- schau und Berlin überhaupt gemeinsame Interessen in der europ?ischen und作者: 討好美人 時(shí)間: 2025-3-29 16:30
Selbst- und Fremdzuschreibungen im Kontext von Europa978-3-531-92412-0作者: carotid-bruit 時(shí)間: 2025-3-29 21:39
by incorporating a heritage studies lens to reveal the maki.This book examines heritage-led regeneration and decision-making processes in Tokyo’s urban centres of Nihonbashi and Marunouchi. Detailing some of the city’s most prominent and recent redevelopment projects, Jiewon Song recognizes key ins
