標(biāo)題: Titlebook: Black Holes, Gravitational Radiation and the Universe; Essays in Honor of C Bala R. Iyer,Biplab Bhawal Book 1999 Springer Science+Business [打印本頁(yè)] 作者: Gratification 時(shí)間: 2025-3-21 19:25
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書目名稱Black Holes, Gravitational Radiation and the Universe讀者反饋學(xué)科排名
作者: Lipoma 時(shí)間: 2025-3-21 21:25 作者: Champion 時(shí)間: 2025-3-22 03:07 作者: 多樣 時(shí)間: 2025-3-22 06:58
Notes on Black Hole Fluctuations and Back-Reaction,n as a manifestation of a fluctuction-dissipation relation was first proposed by Candelas and Sciama [3, 4]. Even though, as we will soon see, the fluctuations in the thought of these earlier authors are not the correct ones and the relations proposed were not really addressing the back-reaction of 作者: Suggestions 時(shí)間: 2025-3-22 09:43 作者: 信條 時(shí)間: 2025-3-22 13:49
Micro-Structure of Black Holes and String Theory,didates in binary systems and there is also evidence that the matter of galaxies is belched in ‘a(chǎn)ctive galactic nuclei’ which are black holes with a million times the solar mass. Why do black holes occur? The standard answer is gravitational collapse and the existence of black hole solutions in gene作者: ALERT 時(shí)間: 2025-3-22 19:05
Quantum Geometry and Black Holes,rature and a multiple of the area of its event horizon should be identified with its thermodynamic entropy [1]. In this reasoning, he had to use not only general relativity but also quantum mechanics. Indeed, without recourse to the Planck’s constant, ?, the identification is impossible because even作者: 杠桿支點(diǎn) 時(shí)間: 2025-3-22 23:06
Black Holes, Global Monopole Charge and Quasi-Local Energy,n: can we get the same solutions from a slightly different and more general equation, which is not the derivative of the original equation? The answer is yes. Take the case of the Schwarzshild solution. It is the unique spherically symmetric solution of the Einstein vacuum equation, .. = 0. It can a作者: 半球 時(shí)間: 2025-3-23 02:54
Kinematical Consequences of Inertial Forces in General Relativity,on is an indicator of the characteristic of a body that determines its motion. Whereas according to Newton’s law of motion, a body’s state of rest or of uniform motion does in no way characterise its inertia, any change in this state depends upon its inertia. As the change of state can be recorded o作者: affluent 時(shí)間: 2025-3-23 09:25
Neutron Stars and Relativistic Gravity,tic gravity can be understood as the warping of space-time near any object that has mass. Consider the following examples. In Newtonian gravity, a planet orbits around a star in an ellipse. In relativistic gravity the orbit is not a closed curve; it is approximately an ellipse, whose major axis prec作者: DAMN 時(shí)間: 2025-3-23 12:07 作者: 姑姑在炫耀 時(shí)間: 2025-3-23 17:55 作者: 推遲 時(shí)間: 2025-3-23 19:10 作者: Influx 時(shí)間: 2025-3-24 02:15 作者: delta-waves 時(shí)間: 2025-3-24 06:23
Fundamental Theories of Physicshttp://image.papertrans.cn/b/image/188948.jpg作者: Scintigraphy 時(shí)間: 2025-3-24 06:34
https://doi.org/10.1007/978-94-017-0934-7Accretion; Cosmology; Gravity; Relativity; Universe; astrophysics; general relativity; mathematical physics作者: acclimate 時(shí)間: 2025-3-24 13:37
978-90-481-5121-9Springer Science+Business Media Dordrecht 1999作者: exceptional 時(shí)間: 2025-3-24 15:30
Die Insuffizienz des Gef?sssystemsI wish to express my deep gratitude to C. V. Vishveshwara for his encouragement. It is a great honour to be his student. It is also a pleasure to write this article in honor of him.作者: 流動(dòng)性 時(shí)間: 2025-3-24 20:06
Die nerv?sen Kreislaufst?rungenIt is well known that, contrary to what happens in prerelativistic physics, there is no general exact solution in general relativity to the problem of two extended charged bodies in equilibrium under the combined action of the gravito-electromagnetic forces due to their masses and charges.作者: 碎片 時(shí)間: 2025-3-25 02:47 作者: myalgia 時(shí)間: 2025-3-25 04:15
Analysis of the Equilibrium of a Charged Test Particle in the Kerr-Newman Black Hole,It is well known that, contrary to what happens in prerelativistic physics, there is no general exact solution in general relativity to the problem of two extended charged bodies in equilibrium under the combined action of the gravito-electromagnetic forces due to their masses and charges.作者: 歡騰 時(shí)間: 2025-3-25 10:54
Astrophysical Evidence for Black Hole Event Horizons,und each other under the influence of their mutual gravitational attraction, black holes with masses of order several solar masses . ~ 5 – 20M.) are thought to exist as the dead remnant of the initially more massive of the two stars.作者: Condense 時(shí)間: 2025-3-25 14:13
Black Holes, Gravitational Radiation and the Universe978-94-017-0934-7Series ISSN 0168-1222 Series E-ISSN 2365-6425 作者: 暴露他抗議 時(shí)間: 2025-3-25 16:57
Theodor Heinrich Schiebler,Walter Schmidtund each other under the influence of their mutual gravitational attraction, black holes with masses of order several solar masses . ~ 5 – 20M.) are thought to exist as the dead remnant of the initially more massive of the two stars.作者: 有毒 時(shí)間: 2025-3-25 20:56
Lehrbuch der drahtlosen Telegraphie will review the progress made using this method in solving various systems of equations in black hole space-time backgrounds. The equations of important physical interest that we shall discuss consist primarily of the linear perturbation equations for various fields. In particular: Maxwell’s equati作者: Admonish 時(shí)間: 2025-3-26 00:34 作者: CEDE 時(shí)間: 2025-3-26 07:56
https://doi.org/10.1007/978-3-662-42404-9gularities [1]. In particular, if a sufficiently large amount of mass is contained in a sufficiently small region, trapped surfaces must form [2] or future light cone reconvergence should occur [3], in which case gravitational collapse to a singularity must result. One of the key outstanding issues 作者: promote 時(shí)間: 2025-3-26 10:43
Lehrbuch der empirischen Forschungn as a manifestation of a fluctuction-dissipation relation was first proposed by Candelas and Sciama [3, 4]. Even though, as we will soon see, the fluctuations in the thought of these earlier authors are not the correct ones and the relations proposed were not really addressing the back-reaction of 作者: Arthropathy 時(shí)間: 2025-3-26 14:42 作者: 完全 時(shí)間: 2025-3-26 19:31 作者: 巧思 時(shí)間: 2025-3-26 21:15 作者: 無(wú)意 時(shí)間: 2025-3-27 02:49 作者: 健忘癥 時(shí)間: 2025-3-27 08:19
https://doi.org/10.1007/978-3-642-91723-3on is an indicator of the characteristic of a body that determines its motion. Whereas according to Newton’s law of motion, a body’s state of rest or of uniform motion does in no way characterise its inertia, any change in this state depends upon its inertia. As the change of state can be recorded o作者: angina-pectoris 時(shí)間: 2025-3-27 10:37 作者: GRACE 時(shí)間: 2025-3-27 17:21 作者: 軌道 時(shí)間: 2025-3-27 19:29 作者: 變形詞 時(shí)間: 2025-3-27 22:12
Allgemeine Anatomie des Nervensystemsbinary systems and (2) as supermassive black holes in the nuclei of active galaxies and quasars. A black hole most vividly manifests itself when it accretes matter from a companion star or the surroundings. As the matter moves under the spell of the black hole’s gravity, it heats up to high temperat作者: 使服水土 時(shí)間: 2025-3-28 06:05
Theodor Heinrich Schiebler,Walter Schmidtsive bodies residing in their centres. X-ray binaries, active galactic nuclei, extragalactic double radio sources displaying relativistic jets and other such interesting phenomena are some examples for which an important part of the gravitational energy associated with the inflow of matter is radiat作者: 廣告 時(shí)間: 2025-3-28 09:20 作者: Fibrillation 時(shí)間: 2025-3-28 10:31 作者: 誓言 時(shí)間: 2025-3-28 17:11
Black Holes, Global Monopole Charge and Quasi-Local Energy,lace equation but not its first integral? We shall show that the two sets of equations are dual of each other in a certain sense [2]. In the former case the unique solution is the Schwarzschild black hole while the dual set provides a black hole with a global monopole charge [3]. The latter solution作者: 高談闊論 時(shí)間: 2025-3-28 21:51 作者: VOC 時(shí)間: 2025-3-28 23:25 作者: congenial 時(shí)間: 2025-3-29 03:42 作者: 迅速成長(zhǎng) 時(shí)間: 2025-3-29 08:45 作者: 我沒(méi)有命令 時(shí)間: 2025-3-29 13:45
Lehrbuch der empirischen Forschungh formalisms [7] for the establishment of a quantum statistical field theory in curved spacetime (for a review, see [8, 9]). It was found that the back-reaction of quantum fields (through processes like particle creation) on a classical background spacetime can be described by an Einstein-Langevin e作者: Impugn 時(shí)間: 2025-3-29 18:22 作者: Digitalis 時(shí)間: 2025-3-29 20:00 作者: Subjugate 時(shí)間: 2025-3-30 00:15
Theodor Heinrich Schiebler,Walter Schmidt gravity a gyroscope in free fall does not naturally precess, while it does in relativistic gravity. This is supposed to be due to an additional gravitational torque felt by the gyroscope. It is difficult to observe such effects in our solar system, where the gravitational field is relatively weak. 作者: BIDE 時(shí)間: 2025-3-30 07:22
Lehrbuch der gesamten Anatomie des Menschene per year concentrates on accretion disk phenomena (for a recent one, see Abramowicz et al. 1997a), and entire texts (e.g., Frank et al. 1992), monographs (e.g., Chakrabarti 1990a), and many far more extensive reviews than this current effort (substantial recent ones include Chakrabarti 1996a; Lin 作者: aggressor 時(shí)間: 2025-3-30 10:53
Black Holes, Gravitational Radiation and the UniverseEssays in Honor of C作者: sulcus 時(shí)間: 2025-3-30 15:13 作者: insurrection 時(shí)間: 2025-3-30 17:01 作者: 炸壞 時(shí)間: 2025-3-30 22:48
Lehrbuch der drahtlosen Telegraphieons, Dirac’s equation and the Weyl neutrino equation and the gravitational perturbation equations. We will also discuss generalised Hertz potentials, the Rarita-Schwinger equation and the properties of Teukolsky functions.作者: 移植 時(shí)間: 2025-3-31 02:23
Lehrbuch der drahtlosen Telegraphie background geometry. Under this assumption a scattering theory can be constructed and conservation laws governing the generation and propagation of the energy flux can be found, but with relevant differences between stars and black holes.作者: Offensive 時(shí)間: 2025-3-31 05:46 作者: embolus 時(shí)間: 2025-3-31 09:49 作者: 極大的痛苦 時(shí)間: 2025-3-31 15:22
