標(biāo)題: Titlebook: Handbook of Gravitational Wave Astronomy; Cosimo Bambi,Stavros Katsanevas,Konstantinos D. Ko Living reference work 20200th edition Gravit [打印本頁(yè)] 作者: informed 時(shí)間: 2025-3-21 20:07
書目名稱Handbook of Gravitational Wave Astronomy影響因子(影響力)
書目名稱Handbook of Gravitational Wave Astronomy影響因子(影響力)學(xué)科排名
書目名稱Handbook of Gravitational Wave Astronomy網(wǎng)絡(luò)公開度
書目名稱Handbook of Gravitational Wave Astronomy網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Handbook of Gravitational Wave Astronomy被引頻次
書目名稱Handbook of Gravitational Wave Astronomy被引頻次學(xué)科排名
書目名稱Handbook of Gravitational Wave Astronomy年度引用
書目名稱Handbook of Gravitational Wave Astronomy年度引用學(xué)科排名
書目名稱Handbook of Gravitational Wave Astronomy讀者反饋
書目名稱Handbook of Gravitational Wave Astronomy讀者反饋學(xué)科排名
作者: nerve-sparing 時(shí)間: 2025-3-22 00:07 作者: limber 時(shí)間: 2025-3-22 01:22
Adam Pound,Barry Wardelleen used in the Bloomsbury MRCP Part I course. This approach remains a popular part of the examination system in that it provides a compact method of testing knowledge over a very wide field, particularly advantageous in a diverse subject such as medicine. .This volume is suited to those in the fina作者: 細(xì)胞學(xué) 時(shí)間: 2025-3-22 07:56
Francois Foucarteen used in the Bloomsbury MRCP Part I course. This approach remains a popular part of the examination system in that it provides a compact method of testing knowledge over a very wide field, particularly advantageous in a diverse subject such as medicine. .This volume is suited to those in the fina作者: 碎片 時(shí)間: 2025-3-22 12:34 作者: ADOPT 時(shí)間: 2025-3-22 16:36 作者: innovation 時(shí)間: 2025-3-22 19:05 作者: bifurcate 時(shí)間: 2025-3-22 22:59
Xian Chenhat have been used in the Bloomsbury MRCP Part I course. This approach remains a popular part of the examination system in that it provides a compact method of testing knowledge over a very wide field, particularly advantageous in a diverse subject such as medicine. .This volume is suited to those i作者: Herd-Immunity 時(shí)間: 2025-3-23 02:27
Bence Kocsishat have been used in the Bloomsbury MRCP Part I course. This approach remains a popular part of the examination system in that it provides a compact method of testing knowledge over a very wide field, particularly advantageous in a diverse subject such as medicine. .This volume is suited to those i作者: 水土 時(shí)間: 2025-3-23 08:55 作者: 不規(guī)則 時(shí)間: 2025-3-23 11:03 作者: 公理 時(shí)間: 2025-3-23 16:56 作者: recede 時(shí)間: 2025-3-23 20:38
Salvatore Vitale,Davide Gerosa,Will M. Farr,Stephen R. Taylormance analyst. Stochastic Petri net analysis packages are less commonly used. They have only recently emerged from the research laboratory, and are not in widespread commercial use. This paper takes a particular problem, diskless workstation configuration management, and analyses it using tools of b作者: 慷慨援助 時(shí)間: 2025-3-23 23:20 作者: 脖子 時(shí)間: 2025-3-24 02:56
Brynmor Haskell,Kai Schwenzertempting to capture performance analysis as a process and then considering how this process may be supported efficiently from the user point of view. It is argued that such a conceptual modelling approach will enable developers to minimise the load on users in making use of the wide and growing rang作者: 打火石 時(shí)間: 2025-3-24 08:11
Patrick Brady,Giovanni Losurdo,Hisaaki Shinkaiut objects in a concurrent system necessitates extending the notion of abstraction functions in order to model the system’s inherent nondeterminisitic behavior. My talk presented in detail the extensions required to reason about lock-free concurrent objects, used to build linearizable systems. It al作者: 楓樹 時(shí)間: 2025-3-24 14:42 作者: 評(píng)論者 時(shí)間: 2025-3-24 18:19
Advances in Machine and Deep Learning for Modeling and Real-Time Detection of Multi-messenger Sourcvitational waves, electromagnetic waves, neutrinos, and cosmic rays cover a wide range of wavelengths and timescales. Combining and processing these datasets that vary in volume, speed, and dimensionality requires new modes of instrument coordination, funding, and international collaboration with a 作者: 泥瓦匠 時(shí)間: 2025-3-24 19:28
Binary Neutron Stars,emit. After a general introduction to the formation of these systems and to the dynamics of mergers and after some comments on the state of the art of numerical simulations thereof, I descend into some details about how to link gravitational-wave measurements with the equation of state of neutron st作者: 小蟲 時(shí)間: 2025-3-25 03:11 作者: 世俗 時(shí)間: 2025-3-25 06:18
Black Hole-Neutron Star Mergers,tiple binary black hole and binary neutron star systems have been detected, and while we are still waiting for the first confirmed observation of a mixed black hole-neutron star (BHNS) merger, a number of candidate events have been announced over the last observing run of the LIGO-Virgo Collaboratio作者: 擋泥板 時(shí)間: 2025-3-25 10:43
Black-Hole Superradiance: Searching for Ultralight Bosons with Gravitational Waves,ce. This phenomenon is ubiquitous in many physical systems and also occurs for spinning black holes and stars, with far-reaching consequences for gravitational-wave astronomy and searches for new physics with astrophysical compact objects. In particular, ultralight bosonic fields (predicted in a var作者: 換話題 時(shí)間: 2025-3-25 15:38
CMB Experiments and Gravitational Waves,sistencies in observations of the universe, including the thermal equilibrium of the CMB at otherwise super-horizon scales, and the observed spatial flatness of the universe. Inflation would expand space by at least 60 e-folds in 10. s in order to explain the observed flatness and homogeneity of the作者: 故意釣到白楊 時(shí)間: 2025-3-25 18:39 作者: STERN 時(shí)間: 2025-3-25 21:52 作者: DOSE 時(shí)間: 2025-3-26 00:27 作者: 驚惶 時(shí)間: 2025-3-26 05:23
Effective Field Theory Methods to Model Compact Binaries,gravitational wave detections from compact binary coalescences will demand even more accurate description of the source dynamics as the sensitivity of detectors increases over years. The analytic modeling of classical gravitational dynamics has been enriched over the last decade of powerful methods 作者: Antagonist 時(shí)間: 2025-3-26 08:34 作者: dagger 時(shí)間: 2025-3-26 16:21
Emission of Gravitational Radiation in Scalar-Tensor and f(R)-Theories,heories of gravity in the strong field regime. Such tests rely sensitively on the phase evolution of the gravitational waves, which is controlled by the energy momentum carried by such waves out of the system. The weak-field limit of alternative metric theories shows new aspects of gravitation which作者: Bumptious 時(shí)間: 2025-3-26 19:38 作者: BUST 時(shí)間: 2025-3-26 23:05
Formation Channels of Single and Binary Stellar-Mass Black Holes, and merger rates. In this review, we discuss the main formation channels of BBHs from stellar evolution and dynamics. Uncertainties on massive star evolution (e.g., stellar winds, rotation, overshooting, and nuclear reaction rates), core-collapse supernovae, and pair instability still hamper our co作者: tattle 時(shí)間: 2025-3-27 02:05 作者: disparage 時(shí)間: 2025-3-27 09:22
Inferring the Properties of a Population of Compact Binaries in Presence of Selection Effects,: do all sources come from the same underlying population, or several populations are required? What are the properties of these populations? As the detection of gravitational waves is becoming routine and the size of the event catalog increases, finer and finer details of the astrophysical distribu作者: 向下 時(shí)間: 2025-3-27 09:44 作者: 蜿蜒而流 時(shí)間: 2025-3-27 15:08
Isolated Neutron Stars,observations is, however, a challenging endeavor, as the radiation is only emitted by the outermost layers and is scattered by the interstellar medium. Gravitational waves, on the other hand, while challenging to detect, interact weakly with matter and are likely to carry a clean imprint of the high作者: Galactogogue 時(shí)間: 2025-3-27 17:50 作者: DRILL 時(shí)間: 2025-3-28 00:56
LISA and the Galactic Population of Compact Binaries,ible to the space-based gravitational wave detector LISA. A few tens of thousands of these systems will be individually resolvable in frequency space, while the remainder will contribute to a confusion-limited foreground at frequencies below about 1 mHz. In addition to the close white dwarf binaries作者: 爆炸 時(shí)間: 2025-3-28 02:51
Living reference work 20200th editionnts, from ground and space based laser interferometers to pulsar timing arrays and indirect detection from the cosmic microwave background. In the second part, it discusses a number of astrophysical and cosmological gravitational wave sources, including black holes, neutron stars, possible more exot作者: 慌張 時(shí)間: 2025-3-28 08:07 作者: Indecisive 時(shí)間: 2025-3-28 13:00 作者: indigenous 時(shí)間: 2025-3-28 17:00 作者: Tonometry 時(shí)間: 2025-3-28 22:22
Formation Channels of Single and Binary Stellar-Mass Black Holes,y. Dynamical processes in dense stellar systems can trigger the formation of BHs in the mass gap and intermediate-mass BHs via hierarchical BH mergers and via multiple stellar collisions. Finally, we discuss the importance of reconstructing the cosmic evolution of BBHs.作者: motivate 時(shí)間: 2025-3-29 01:04
Gravitational Waves from Core-Collapse Supernovae,hin our galaxy, while future third-generation instruments will enable more robust and detailed observations. The rapidly rotating models that develop non-axisymmetric instabilities may be visible up to a megaparsec distance with the third-generation detectors. Finally, we discuss strategies for multi-messenger observations of supernovae.作者: 他姓手中拿著 時(shí)間: 2025-3-29 04:20 作者: frivolous 時(shí)間: 2025-3-29 11:13 作者: 串通 時(shí)間: 2025-3-29 11:48 作者: 違反 時(shí)間: 2025-3-29 19:13
Detection Landscape in the deci-Hertz Gravitational-Wave Spectrum,atom interferometry. A major focus of this chapter is toward the technology behind DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) and its scientific pathfinder mission concept B-DECIGO.作者: Expurgate 時(shí)間: 2025-3-29 19:49
Electromagnetic Counterparts of Gravitational Waves in the Hz-kHz Range,the diverse electromagnetic counterparts to gravitational wave sources detectable by current ground-based detectors, providing basic information on their properties and on the physics that governs their emission. In addition, it addresses observational and data analysis strategies to optimize their detection and characterization.作者: 先鋒派 時(shí)間: 2025-3-30 02:22
Environmental Noise in Gravitational-Wave Interferometers,aths, investigation and mitigation methods. We refer to the experience gained during the commissioning and operation of the existing gravitational-wave interferometers and the most recent documentation on the subject. We wish to share indications useful for the design and commissioning of future terrestrial gravitational-wave detectors.作者: 向前變橢圓 時(shí)間: 2025-3-30 06:33 作者: 玩忽職守 時(shí)間: 2025-3-30 08:31 作者: Processes 時(shí)間: 2025-3-30 15:17
Adam Pound,Barry Wardelltesting knowledge over a very wide field, particularly advantageous in a diverse subject such as medicine. .This volume is suited to those in the final stages of preparation for their examinations, such as the MRCP Part I, which is taken by about 3,000 doctors annually. The user will gain experience of performing under the stress of a time limit.作者: Projection 時(shí)間: 2025-3-30 20:11 作者: 語(yǔ)言學(xué) 時(shí)間: 2025-3-30 22:11
Richard Brito,Paolo Panitesting knowledge over a very wide field, particularly advantageous in a diverse subject such as medicine. .This volume is suited to those in the final stages of preparation for their examinations, such as the MRCP Part I, which is taken by about 3,000 doctors annually. The user will gain experience of performing under the stress of a time limit.作者: Afflict 時(shí)間: 2025-3-31 03:46 作者: Capture 時(shí)間: 2025-3-31 06:08
Riccardo Sturanies on a technique for using computational power for dynamically creating links, known as retrieval links. The algorithm used for creating retrieval links is described and some preliminary experiments to assess the value of this facility are discussed.作者: 貝雷帽 時(shí)間: 2025-3-31 09:18 作者: STRIA 時(shí)間: 2025-3-31 14:32
Salvatore Vitale,Davide Gerosa,Will M. Farr,Stephen R. Taylort in widespread commercial use. This paper takes a particular problem, diskless workstation configuration management, and analyses it using tools of both types. Although the theoretical limitations of both types of solution package are well known, little work has been done to compare their practical performance.作者: 民間傳說(shuō) 時(shí)間: 2025-3-31 20:38 作者: magenta 時(shí)間: 2025-4-1 00:20
Luca Baiottin the final stages of preparation for their examinations, such as the MRCP Part I, which is taken by about 3,000 doctors annually. The user will gain experience of performing under the stress of a time limit.978-3-540-19781-2978-1-4471-2005-6作者: Thyroiditis 時(shí)間: 2025-4-1 05:18
