標題: Titlebook: Black Hole Physics; Basic Concepts and N Valeri P. Frolov,Igor D. Novikov Book 1998 Springer Science+Business Media Dordrecht 1998 Gravity. [打印本頁] 作者: 正當理由 時間: 2025-3-21 17:14
書目名稱Black Hole Physics影響因子(影響力)
書目名稱Black Hole Physics影響因子(影響力)學科排名
書目名稱Black Hole Physics網絡公開度
書目名稱Black Hole Physics網絡公開度學科排名
書目名稱Black Hole Physics被引頻次
書目名稱Black Hole Physics被引頻次學科排名
書目名稱Black Hole Physics年度引用
書目名稱Black Hole Physics年度引用學科排名
書目名稱Black Hole Physics讀者反饋
書目名稱Black Hole Physics讀者反饋學科排名
作者: ULCER 時間: 2025-3-21 22:28 作者: Corroborate 時間: 2025-3-22 02:11
Lehrbuch der darstellenden Geometrieack hole (of a given mass .) is determined unambiguously by its electric charge . and rotation parameter .. If the charged black hole does not rotate, its electromagnetic field reduces to the radial electric field of the charge . and is static. Any multipoles higher than the monopole are absent.作者: 外來 時間: 2025-3-22 05:06 作者: grotto 時間: 2025-3-22 11:41
Die Ellipse: Konjugierte Durchmessersehnentional radiation. This radiation interacts with the spacetime curvature. While part of it escapes to infinity, another part is backscattered and absorbed by the resulting black hole. In the end all deviations from the Kerr-Newman field decay to zero.作者: Duodenitis 時間: 2025-3-22 16:00 作者: infinite 時間: 2025-3-22 18:22 作者: 一小塊 時間: 2025-3-22 22:45 作者: 上漲 時間: 2025-3-23 04:16
The Interior of a Black Holetional radiation. This radiation interacts with the spacetime curvature. While part of it escapes to infinity, another part is backscattered and absorbed by the resulting black hole. In the end all deviations from the Kerr-Newman field decay to zero.作者: 粗糙 時間: 2025-3-23 08:46
Book 1998putative objects whose gravitational fields are so strong that no physical bodies or signals can break free of their pull and escape. The proof that black holes do exist, and an analysis of their properties, would have a significance going far beyond astrophysics. Indeed, what is involved is not jus作者: entail 時間: 2025-3-23 11:37 作者: 繼而發(fā)生 時間: 2025-3-23 16:53
Quantum Physics of Black Holesnditions). In quantum theory, negative energy density may arise in a region of space because an external field applied to the vacuum may either increase or reduce the local energy density of zero point fluctuations. It is this phenomenon, known as ., that is to be expected to play an important role in the neighborhood of black holes.作者: 眼界 時間: 2025-3-23 20:29
Die Durchdringungslinien von Vielflachenr to answer these questions, the definition must first of all be extended to the general case of non-stationary spacetime. This generalization is obvious. It is reasonable to define the . in general as the region of spacetime from which no information-carrying signals are allowed to escape to a distant observer.作者: 使人入神 時間: 2025-3-24 01:34
Die Durchdringungslinien von Vielflacheniscussed two examples of such processes; namely, the Penrose process (Section 6.2.3) and superradiance (Section 4.8.2). In this section, we establish some general restrictions on the possible efficiency of this kind of process.作者: insipid 時間: 2025-3-24 04:26
Darstellende Geometrie der Fl?chenkrümmunge and the singularity arises. No causal signal can propagate through the throat from one asymptotically flat region (R.) to the other one (.). This property is directly connected with the non-trivial causal structure of spacetime in the presence of a black hole作者: 單獨 時間: 2025-3-24 08:18
General Properties of Black Holesr to answer these questions, the definition must first of all be extended to the general case of non-stationary spacetime. This generalization is obvious. It is reasonable to define the . in general as the region of spacetime from which no information-carrying signals are allowed to escape to a distant observer.作者: entrance 時間: 2025-3-24 11:17 作者: 使虛弱 時間: 2025-3-24 17:49
Black Holes, Wormholes, and Time Machinese and the singularity arises. No causal signal can propagate through the throat from one asymptotically flat region (R.) to the other one (.). This property is directly connected with the non-trivial causal structure of spacetime in the presence of a black hole作者: Measured 時間: 2025-3-24 20:45 作者: HERTZ 時間: 2025-3-25 00:37 作者: 同謀 時間: 2025-3-25 07:02 作者: CHOP 時間: 2025-3-25 11:02 作者: 斥責 時間: 2025-3-25 13:19
Kurven, Kegel und Zylinder zweiter Ordnungherically symmetric. The . (spacetime with spherical three-dimensional space) is described in every textbook on general relativity [see, e.g., Landau and Lifshitz (1975), Misner, Thorne, and Wheeler (1973)]. Therefore, here we will only reproduce the necessary results. Mathematical details connected作者: 撫慰 時間: 2025-3-25 17:53 作者: Atmosphere 時間: 2025-3-25 20:11
Die Durchdringungslinien von Vielflachens. Both Schwarzschild and Kerr spacetimes are stationary and possess certain symmetries. A study of geodesies (corresponding to the motion of test particles and light rays) and wave fields in these metrics enabled us to describe a number of interesting and important features of physical effects in t作者: DOLT 時間: 2025-3-26 01:31
Die Durchdringungslinien von Vielflachenlyzing the efficiency of energy extraction from black holes. Recall that although a black hole is by definition a region of no escape for material bodies and light rays, situations are possible in which energy can be extracted via certain physical processes. We will see later that this energy is ext作者: 朦朧 時間: 2025-3-26 05:56
Lehrbuch der darstellenden Geometrieo observation by distant observers. At first glance, black hole electrodynamics is quite trivial. Indeed, the electromagnetic field of a stationary black hole (of a given mass .) is determined unambiguously by its electric charge . and rotation parameter .. If the charged black hole does not rotate,作者: 處理 時間: 2025-3-26 10:11 作者: Ingredient 時間: 2025-3-26 16:21
Lehrbuch der darstellenden Geometrieare, indeed, insignificant for black holes of about a solar mass (and greater). However, for a small-mass (primordial) black hole these effects cannot be ignored; in fact, they qualitatively change the black hole’s evolution. They are also likely to become important for those regions inside a black 作者: BUCK 時間: 2025-3-26 20:12
Die Ellipse: Konjugierte Durchmessersehnen drawing the inevitable conclusion that the particle flux to infinity which carries away positive energy is accompanied by a flux of negative energy across the horizon into the black hole. This would be impossible in classical theory, with ordinary physical assumptions satisfied (energy dominance co作者: liposuction 時間: 2025-3-27 00:05 作者: Mhc-Molecule 時間: 2025-3-27 01:57
Die Ellipse: Konjugierte Durchmessersehnentles down very quickly to the unique stationary state — a Kerr-Newman black hole. Dynamical deviations from this state produce the emission of gravitational radiation. This radiation interacts with the spacetime curvature. While part of it escapes to infinity, another part is backscattered and absor作者: 戲法 時間: 2025-3-27 07:44 作者: glucagon 時間: 2025-3-27 13:19 作者: 平項山 時間: 2025-3-27 17:37
Rotating Black Holeshole when the radius of the collapsing body becomes less than the gravitational radius. Suppose the collapsing body deviates considerably from spherical symmetry and/or its angular momentum and electromagnetic field are large. Will a black hole form? If it does, what will its properties be?作者: Nebulizer 時間: 2025-3-27 21:26 作者: 結束 時間: 2025-3-28 00:37
Ultimate Fate of Black and White Holeshe book certainly is not a complete theory and requires modifications because of quantum effects. Quantum effects become dominant at Planck scales, and quantum gravity is required there. In this section we comment on some of the problems of black hole physics that require quantum gravity for their solutions.作者: STING 時間: 2025-3-28 04:22
Fundamental Theories of Physicshttp://image.papertrans.cn/b/image/188946.jpg作者: PLAYS 時間: 2025-3-28 06:54
Black Hole Physics978-94-011-5139-9Series ISSN 0168-1222 Series E-ISSN 2365-6425 作者: 中國紀念碑 時間: 2025-3-28 14:14 作者: 針葉 時間: 2025-3-28 18:35 作者: maverick 時間: 2025-3-28 21:10 作者: Osteons 時間: 2025-3-28 23:49 作者: mighty 時間: 2025-3-29 05:42
Lehrbuch der darstellenden GeometrieThis chapter is devoted to problems involving perturbed black holes. We describe the evolution of physical fields in the exterior of Schwarzschild and Kerr black holes. As we shall see, an understanding of wave propagation in black hole geometries opens the door to studies of:作者: 高度 時間: 2025-3-29 11:14
https://doi.org/10.1007/978-3-662-43020-0As a result of the lightlike nature of the event horizon enclosing the black hole, the horizon acts as a one-way membrane. Particles and radiation can cross the event horizon from outside and enter the black hole, but escape is forbidden for both particles and radiation. Hence, processes involving black holes are essentially irreversible.作者: stress-test 時間: 2025-3-29 11:35
https://doi.org/10.1007/978-3-662-43020-0Hawking’s discovery of thermal radiation from black holes was a complete surprise to most specialists, even though quite a few indications of a close relationship between black hole physics and thermodynamics had emerged before this discovery.作者: URN 時間: 2025-3-29 18:35 作者: apiary 時間: 2025-3-29 20:13 作者: artless 時間: 2025-3-30 00:17
Stationary Black HolesAs a result of the lightlike nature of the event horizon enclosing the black hole, the horizon acts as a one-way membrane. Particles and radiation can cross the event horizon from outside and enter the black hole, but escape is forbidden for both particles and radiation. Hence, processes involving black holes are essentially irreversible.作者: 不愿 時間: 2025-3-30 04:29
Thermodynamics and Statistical Mechanics of Black HolesHawking’s discovery of thermal radiation from black holes was a complete surprise to most specialists, even though quite a few indications of a close relationship between black hole physics and thermodynamics had emerged before this discovery.作者: anagen 時間: 2025-3-30 10:33 作者: 子女 時間: 2025-3-30 13:05
Rotating Black Holeshole when the radius of the collapsing body becomes less than the gravitational radius. Suppose the collapsing body deviates considerably from spherical symmetry and/or its angular momentum and electromagnetic field are large. Will a black hole form? If it does, what will its properties be?作者: 爭吵加 時間: 2025-3-30 18:24 作者: 擁擠前 時間: 2025-3-30 22:26
Physical Effects in the Gravitational Field of a Black Holelyzing the efficiency of energy extraction from black holes. Recall that although a black hole is by definition a region of no escape for material bodies and light rays, situations are possible in which energy can be extracted via certain physical processes. We will see later that this energy is ext作者: Anticoagulant 時間: 2025-3-31 04:18 作者: Painstaking 時間: 2025-3-31 07:10 作者: Ornithologist 時間: 2025-3-31 11:09
