標(biāo)題: Titlebook: Black Holes: Theory and Observation; Proceedings of the 1 Friedrich W. Hehl,Claus Kiefer,Ralph J.K. Metzler Conference proceedings 1998 Spr [打印本頁] 作者: damped 時(shí)間: 2025-3-21 19:55
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作者: 諂媚于人 時(shí)間: 2025-3-21 22:47 作者: apropos 時(shí)間: 2025-3-22 03:20
Lehrbuch der pharmazeutischen Biologieitters up to energies of at least several GeV. They show a highly variable nonthermal emission component. The assumption of isotropic emission together with the observed vaxiability would lead to a high radiation density in a small emission region. At least for some sources, the derived compactness 作者: ingenue 時(shí)間: 2025-3-22 08:27
Digitale Bildentstehung und -verarbeitungal PGG model is demonstrated in vacuum, and the structure of the black hole type solutions of the quadratic models with and without matter is analyzed in detail. Finally, the integrability of the general dilaton gravity model is established by recasting 作者: Arthropathy 時(shí)間: 2025-3-22 09:11
Black Holes: A General Introduction,, provide a powerful analytical tool able to examine macroscopic and microscopic properties of the universe. This introductory article presents in a pictorial way the basic concepts of black hole‘s theory, as well as a description of the astronomical sites where black holes are suspected to lie, namely binary X-ray sources and galactic nuclei.作者: Obligatory 時(shí)間: 2025-3-22 15:09 作者: 依法逮捕 時(shí)間: 2025-3-22 19:30
Black Hole Hair: A Review,ymptotic infinity) has received renewed attention in the last few years due, in part, to the unexpected discovery of such solutions in various theories. In the present work, we give a brief review of these developments emphasising in the point of view of the authors.作者: GRILL 時(shí)間: 2025-3-22 22:48 作者: 孵卵器 時(shí)間: 2025-3-23 04:26 作者: 羅盤 時(shí)間: 2025-3-23 09:22
Gedanken Experiments in Black Hole Thermodynamics,d mysterious connections, such as the relation between black hole area and entropy. Idealized experiments, using accelerated mirrors, descending boxes and massive shells, can help to provide intuitive understanding and operational definitions of these concepts.作者: Adenoma 時(shí)間: 2025-3-23 09:44
Friedrich W. Hehl,Claus Kiefer,Ralph J.K. MetzlerThis book brings together theory and observations in a unique way.作者: 蹣跚 時(shí)間: 2025-3-23 14:29 作者: Allure 時(shí)間: 2025-3-23 21:52
Lehrbuch der pharmazeutischen Biologie, provide a powerful analytical tool able to examine macroscopic and microscopic properties of the universe. This introductory article presents in a pictorial way the basic concepts of black hole‘s theory, as well as a description of the astronomical sites where black holes are suspected to lie, nam作者: Abrade 時(shí)間: 2025-3-24 00:03
Lehrbuch der pharmazeutischen Biologie process the gravitational energy is converted into electromagnetic radiation. Before the launch of the Compton Gamma-Ray Observatory (CGRO) only four AGNs had been reported to emit detectable gamma-rays. Now, after roughly six years in orbit, the different CGRO experiments have discovered about 90 作者: 協(xié)迫 時(shí)間: 2025-3-24 02:58 作者: antenna 時(shí)間: 2025-3-24 08:08 作者: 過份好問 時(shí)間: 2025-3-24 12:04 作者: Mutter 時(shí)間: 2025-3-24 17:17 作者: fiscal 時(shí)間: 2025-3-24 20:04
Lehrbuch der psychoanalytische Therapieall the reduction of the Einstein-Maxwell action in the presence of a Killing field. The resulting coset structure of the field equations gives rise to the Mazur identity, being the key to the uniqueness proof for the Kerr-Newman metric.作者: reaching 時(shí)間: 2025-3-25 01:26 作者: 到婚嫁年齡 時(shí)間: 2025-3-25 04:04 作者: 敵意 時(shí)間: 2025-3-25 07:37
Krankengeschichten und Behandlungsberichte,tic field, aligned along the Debever-Penrose directions of the Weyl tensor of Petrov type D. Among them, because of their interpretation as black holes, the Reissner-Nordstr?m static solution and the Kerr-Newman stationary axisymmetric solution are singled out.作者: Malleable 時(shí)間: 2025-3-25 12:49 作者: exclamation 時(shí)間: 2025-3-25 18:59
Lehrbuch der psychoanalytischen Therapie in numerical black hole simulations, I discuss a series of calculations from axisymmetry to full 3D that can be seen as stepping stones to simulations of the full 3D coalescence of two black holes. In particular, I emphasize the interplay between perturbation theory and numerical simulation that bu作者: 贊美者 時(shí)間: 2025-3-25 20:07 作者: chondromalacia 時(shí)間: 2025-3-26 00:11 作者: Offstage 時(shí)間: 2025-3-26 05:34
Qualit?tssicherung und Konstanzprüfungeneral relativistic irreversible thermodynamics and derive a universal parameter thermodynamics for rotating fluids ("rotating bodies"). To extend the procedure to black holes, the black hole limit of the rigidly rotating disk of dust solution is discussed. It then turns out that the first law of bl作者: Condyle 時(shí)間: 2025-3-26 11:10 作者: cruise 時(shí)間: 2025-3-26 14:26
E. A. Zimmer,Marianne Zimmer-Brossy effects on the geometry near the inner (Cauchy) horizon because of a diverging blueshift. Determining the inner structure of the hole is really an evolutionary problem with precisely known initial data. The evolution can in principle be followed to within Planck distances of the singularity at the 作者: Conjuction 時(shí)間: 2025-3-26 17:29
R?ntgenologische StandardprojektionenWe investigate the possible gravitational redshift values for boson stars with a self-interaction, studying a wide range of possible masses. We find a limiting value of . for stable boson star configurations. We can rule out the direct observability of boson stars. X-ray spectroscopy is perhaps the most interesting possibility.作者: Conduit 時(shí)間: 2025-3-26 23:09 作者: 運(yùn)氣 時(shí)間: 2025-3-27 01:17
Black Holes: Theory and Observation978-3-540-49535-2Series ISSN 0075-8450 Series E-ISSN 1616-6361 作者: 翻布尋找 時(shí)間: 2025-3-27 08:10 作者: Optometrist 時(shí)間: 2025-3-27 13:22 作者: 面包屑 時(shí)間: 2025-3-27 15:54 作者: 調(diào)味品 時(shí)間: 2025-3-27 21:39 作者: Decongestant 時(shí)間: 2025-3-27 23:38 作者: 字形刻痕 時(shí)間: 2025-3-28 04:04
Digitale Bildentstehung und -verarbeitungd mysterious connections, such as the relation between black hole area and entropy. Idealized experiments, using accelerated mirrors, descending boxes and massive shells, can help to provide intuitive understanding and operational definitions of these concepts.作者: osteoclasts 時(shí)間: 2025-3-28 09:47
https://doi.org/10.1007/b13593astrophysics; black hole; black holes; dynamics; general relativity; physics; quantum theory; relativity; th作者: Cantankerous 時(shí)間: 2025-3-28 11:08 作者: STELL 時(shí)間: 2025-3-28 15:50 作者: committed 時(shí)間: 2025-3-28 19:11 作者: 粗語 時(shí)間: 2025-3-29 00:32
https://doi.org/10.1007/978-3-642-60958-9 of the line in MCG-6-30-15, where the line profile shows strong indications that a Kerr black hole is present in the object. Finally, we show how future X-ray missions will help in deepening our understanding of the emission of broad iron lines from AGN.作者: Bouquet 時(shí)間: 2025-3-29 03:55
Lehrbuch der psychoanalytischen Therapiegeometric optics). Wave "optics" is discussed and the limitations of the standard theory in this regime are pointed out. A nonlocal theory of accelerated observers is briefly described that is consistent with observation and excludes the possibility of existence of a fundamental scalar field in nature.作者: 消息靈通 時(shí)間: 2025-3-29 08:16 作者: 消散 時(shí)間: 2025-3-29 13:32
Measurement Theory and General Relativity,geometric optics). Wave "optics" is discussed and the limitations of the standard theory in this regime are pointed out. A nonlocal theory of accelerated observers is briefly described that is consistent with observation and excludes the possibility of existence of a fundamental scalar field in nature.作者: hemoglobin 時(shí)間: 2025-3-29 17:07
0075-8450 f a panel discussion the participants of the school address the existence of black holes consenting that it has by now been verified with certainty.978-3-662-14175-5978-3-540-49535-2Series ISSN 0075-8450 Series E-ISSN 1616-6361 作者: 有危險(xiǎn) 時(shí)間: 2025-3-29 20:45
Lehrbuch der pharmazeutischen Biologiemass is very likely enclosed within less than 8 light minutes which corresponds to 15 Schwarzschild radii of a million solar mass black hole. Accepting these arguments one must conclude that a massive black hole is located at the core of the Milky Way.作者: Vo2-Max 時(shí)間: 2025-3-30 03:17
Lehrbuch der psychoanalytische Therapielectric conductivity, etc.) of a fictitious membrane. This procedure is completely adequate as long as one is not interested in fine details very close to the horizon. The details of this boundary layer are, however, completely irrelevant for astrophysical applications. The following points will be discussedin detail:作者: 一個(gè)攪動(dòng)不安 時(shí)間: 2025-3-30 05:44
First Conclusive Evidence for a Massive Black Hole in the Center of the Milky Way,mass is very likely enclosed within less than 8 light minutes which corresponds to 15 Schwarzschild radii of a million solar mass black hole. Accepting these arguments one must conclude that a massive black hole is located at the core of the Milky Way.作者: intrigue 時(shí)間: 2025-3-30 09:24 作者: eulogize 時(shí)間: 2025-3-30 14:52 作者: preservative 時(shí)間: 2025-3-30 17:25
,Local Version of the Area Theorem (on a Question by G. ’t Hooft),. to the future of .. Suppose there is a black hole at time . whose area is smaller than any black hole area at time .. Then all null generators of the future event horizon intersecting the surface of this black hole must have past end points between . and .Below we will explain and justify this statement in a more precise fashion.作者: legislate 時(shí)間: 2025-3-30 21:56 作者: expansive 時(shí)間: 2025-3-31 04:42
N-haltige Verbindungen au?er Alkaloide soft state transition, quasi-periodic oscillations, power-law spectral slope in soft states, almost constancy of power-law slopes in both hard and soft states, pattern of the rise and fall of intensities in X-ray novae and processes and rates of mass outflow could be easily understood using the advective disk model which includes this barrier.作者: STELL 時(shí)間: 2025-3-31 06:57 作者: 思想 時(shí)間: 2025-3-31 09:18 作者: 含糊 時(shí)間: 2025-3-31 16:53
E. A. Zimmer,Marianne Zimmer-Brossyolutionary problem with precisely known initial data. The evolution can in principle be followed to within Planck distances of the singularity at the inner horizon, using only well-established physical laws (the Einstein field equations). This lecture reviews recent progress in this area, highlighting outstanding problems and gaps.作者: aspersion 時(shí)間: 2025-3-31 19:37 作者: indignant 時(shí)間: 2025-4-1 00:43 作者: 無能力 時(shí)間: 2025-4-1 04:48
