標(biāo)題: Titlebook: Black Holes: A Laboratory for Testing Strong Gravity; Cosimo Bambi Textbook 2017 Springer Nature Singapore Pte Ltd. 2017 textbook black ho [打印本頁(yè)] 作者: 領(lǐng)口 時(shí)間: 2025-3-21 17:12
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書目名稱Black Holes: A Laboratory for Testing Strong Gravity影響因子(影響力)學(xué)科排名
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書目名稱Black Holes: A Laboratory for Testing Strong Gravity讀者反饋
書目名稱Black Holes: A Laboratory for Testing Strong Gravity讀者反饋學(xué)科排名
作者: –FER 時(shí)間: 2025-3-21 22:16
https://doi.org/10.1007/978-3-476-02758-0in a stationary and axisymmetric spacetime and in the Kerr metric in particular. Last, the chapter discusses possible deviations from the Kerr background due to the presence of an accretion disk or of a non-vanishing electric charge of the central black hole.作者: IVORY 時(shí)間: 2025-3-22 00:58 作者: Fretful 時(shí)間: 2025-3-22 05:57 作者: Cumulus 時(shí)間: 2025-3-22 11:52
Non-Kerr Spacetimesmetric. In the bottom-up approach, we consider instead a phenomenological parameterization of the metric, which ideally should be able to describe the spacetime of any possible black hole in any possible gravity theory.作者: 模范 時(shí)間: 2025-3-22 16:22 作者: Acclaim 時(shí)間: 2025-3-22 20:24
Textbook 2017gion around these objects with electromagnetic radiation. More importantly, it provides the basic tools for writing an astrophysical code and testing the Kerr paradigm. Astrophysical black holes are an ideal laboratory for testing strong gravity. According to general relativity, the spacetime geomet作者: fulmination 時(shí)間: 2025-3-22 23:29
https://doi.org/10.1007/978-3-476-02758-0holes, pointing out its assumptions. It also describes the transfer function for thin accretion disks and how the transfer function can be calculated in a stationary and axisymmetric spacetime and in the Kerr metric in particular. Last, the chapter discusses possible deviations from the Kerr backgro作者: 是突襲 時(shí)間: 2025-3-23 02:54
Ausgleichung nach Tschebyscheff,lity of imaging astrophysical black holes is mainly motivated by the special situation of SgrA., because it is widely thought that sub-mm VLBI facilities will be soon able to image this black hole and detect its shadow.作者: 小故事 時(shí)間: 2025-3-23 07:48 作者: Optic-Disk 時(shí)間: 2025-3-23 11:58 作者: 失誤 時(shí)間: 2025-3-23 15:35 作者: 特別容易碎 時(shí)間: 2025-3-23 19:28
Lehrbuch der inneren Medizin in vier TeilenThe chapter reviews the geodesic motion of massless and massive particles in stationary, axisymmetric, and asymptotically flat spacetimes and in the particular case of the Kerr metric.作者: 強(qiáng)行引入 時(shí)間: 2025-3-23 23:21 作者: nocturia 時(shí)間: 2025-3-24 05:43
Lehrbuch der klinischen AkupunkturThe chapter briefly reviews X-ray missions and gravitational wave experiments.作者: CHURL 時(shí)間: 2025-3-24 06:52
https://doi.org/10.1007/978-3-476-02758-0The chapter reviews the continuum-fitting method, namely the technique to fit the thermal spectrum of a geometrically thin and optically thick accretion disk of a black hole to probe the metric close to the compact object.作者: 嚴(yán)厲譴責(zé) 時(shí)間: 2025-3-24 12:43
https://doi.org/10.1007/978-3-0348-5928-8X-ray reflection spectroscopy is the study of the reflection spectrum of a thin accretion disk. The reflection spectrum has some emission lines and the most prominent one is usually the iron K. line. The reflection spectrum is generated in the inner part of the accretion disk and it can be employed to probe the metric close to the black hole.作者: PACK 時(shí)間: 2025-3-24 14:54 作者: 惡心 時(shí)間: 2025-3-24 22:20
Ausgleichung nach Tschebyscheff,The chapter briefly reviews gravitational waves from black hole coalescences, gravitational waves from extreme-mass ratio inspirals, and quasi-normal modes from black holes.作者: 大雨 時(shí)間: 2025-3-25 00:58
https://doi.org/10.1007/978-3-642-50728-1The chapter briefly reviews current attempts to test the Kerr metric around astrophysical black holes with the continuum-fitting method, X-ray reflection spectroscopy, and quasi-periodic oscilations.作者: Induction 時(shí)間: 2025-3-25 05:40
Erforderliche ZeichenmaterialienThe chapter briefly reviews current/future attempts to test the Kerr metric around astrophysical black holes with SgrA., precise measurements in the weak gravitational field of black holes, and with gravitational waves.作者: Pigeon 時(shí)間: 2025-3-25 07:55 作者: Frisky 時(shí)間: 2025-3-25 13:25 作者: Antimicrobial 時(shí)間: 2025-3-25 18:46
Motion Around Black HolesThe chapter reviews the geodesic motion of massless and massive particles in stationary, axisymmetric, and asymptotically flat spacetimes and in the particular case of the Kerr metric.作者: 有花 時(shí)間: 2025-3-25 21:24
Astrophysical Black HolesThe chapter reviews the astrophysical observations of stellar-mass black holes, intermediate mass black holes, supermassive black holes, the observations supporting the idea that these objects are indeed black holes, and the spectral state classification.作者: 躺下殘殺 時(shí)間: 2025-3-26 02:52 作者: ANA 時(shí)間: 2025-3-26 05:55
Continuum-Fitting MethodThe chapter reviews the continuum-fitting method, namely the technique to fit the thermal spectrum of a geometrically thin and optically thick accretion disk of a black hole to probe the metric close to the compact object.作者: BAIL 時(shí)間: 2025-3-26 12:00
X-Ray Reflection SpectroscopyX-ray reflection spectroscopy is the study of the reflection spectrum of a thin accretion disk. The reflection spectrum has some emission lines and the most prominent one is usually the iron K. line. The reflection spectrum is generated in the inner part of the accretion disk and it can be employed to probe the metric close to the black hole.作者: Gum-Disease 時(shí)間: 2025-3-26 16:41 作者: ineptitude 時(shí)間: 2025-3-26 17:44
Gravitational WavesThe chapter briefly reviews gravitational waves from black hole coalescences, gravitational waves from extreme-mass ratio inspirals, and quasi-normal modes from black holes.作者: 是比賽 時(shí)間: 2025-3-27 00:02
Testing the Kerr Paradigm with X-Ray ObservationsThe chapter briefly reviews current attempts to test the Kerr metric around astrophysical black holes with the continuum-fitting method, X-ray reflection spectroscopy, and quasi-periodic oscilations.作者: PHONE 時(shí)間: 2025-3-27 02:10
Tests with Other ApproachesThe chapter briefly reviews current/future attempts to test the Kerr metric around astrophysical black holes with SgrA., precise measurements in the weak gravitational field of black holes, and with gravitational waves.作者: heart-murmur 時(shí)間: 2025-3-27 06:51
Cosimo BambiProvides the mathematical tools to compute some key-features in the X-ray spectrum of black holes.Contains calculations and analytical details in the appendix.Offers exercises and examples for student作者: 核心 時(shí)間: 2025-3-27 11:45 作者: NATAL 時(shí)間: 2025-3-27 16:18
https://doi.org/10.1007/978-981-10-4524-0textbook black holes; Continuum-Fitting Method; Iron Line Method; Quasi-Periodic Oscillations; Kerr Para作者: 圍裙 時(shí)間: 2025-3-27 18:45
978-981-13-5158-7Springer Nature Singapore Pte Ltd. 2017作者: GULF 時(shí)間: 2025-3-28 00:54 作者: 步履蹣跚 時(shí)間: 2025-3-28 03:14 作者: 莊嚴(yán) 時(shí)間: 2025-3-28 09:37
Thin Accretion Disksholes, pointing out its assumptions. It also describes the transfer function for thin accretion disks and how the transfer function can be calculated in a stationary and axisymmetric spacetime and in the Kerr metric in particular. Last, the chapter discusses possible deviations from the Kerr backgro作者: 產(chǎn)生 時(shí)間: 2025-3-28 10:37
Imaging Black Holeslity of imaging astrophysical black holes is mainly motivated by the special situation of SgrA., because it is widely thought that sub-mm VLBI facilities will be soon able to image this black hole and detect its shadow.作者: 考得 時(shí)間: 2025-3-28 16:23
Non-Kerr Spacetimesnon-Kerr black hole solution from a certain alternative theory of gravity and we check whether it can better explain observational data than the Kerr metric. In the bottom-up approach, we consider instead a phenomenological parameterization of the metric, which ideally should be able to describe the作者: 宣傳 時(shí)間: 2025-3-28 22:20
Black Holes: A Laboratory for Testing Strong Gravity作者: 慢慢沖刷 時(shí)間: 2025-3-29 02:00
Black Holes: A Laboratory for Testing Strong Gravity978-981-10-4524-0作者: justify 時(shí)間: 2025-3-29 04:26 作者: 治愈 時(shí)間: 2025-3-29 07:31
Legal and Administrative Services through Electronic Commercehitecture and the workflow that defines the interactions and interchange of information among actors. With these elements we have implemented an electronic commerce application inside the TRADE project . that demonstrates how these services can be offered in an electronic manner.作者: 過份好問 時(shí)間: 2025-3-29 11:35
https://doi.org/10.1007/978-3-031-79943-3r system is able to generate “fast” and “precise” versions of PSO and, among all the possible configurations which lie between the fastest and the most precise, the ones that give the best trade-offs between precision and speed.作者: 獨(dú)白 時(shí)間: 2025-3-29 17:33 作者: 巨頭 時(shí)間: 2025-3-29 20:55 作者: CYN 時(shí)間: 2025-3-30 00:47 作者: 共同給與 時(shí)間: 2025-3-30 08:01 作者: upstart 時(shí)間: 2025-3-30 10:03
Great Beginnings and Strong Endingsocesses and the Indian monsoon intensity. The forcing functions of this connection are however, a matter of academic debate. A comprehensive understanding of the Arctic is therefore of special importance for a monsoon-dependent agrarian economy like India.作者: 仔細(xì)閱讀 時(shí)間: 2025-3-30 15:24 作者: 信條 時(shí)間: 2025-3-30 17:49
Characteristics of Cytomegalovirustil Wildy . (1960) introduced the negative staining technique to electron microscopy. They found that herpes simplex virus did not have the spherical shape thought, up to 1960, to be common to many viruses. In sections prepared by negative staining, the naked virus particle or capsid was shown to be
