標(biāo)題: Titlebook: Handbook of Gravitational Wave Astronomy; Cosimo Bambi,Stavros Katsanevas,Konstantinos D. Ko Reference work 2022 Springer Nature Singapore [打印本頁] 作者: fathom 時(shí)間: 2025-3-21 18:28
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: Ingrained 時(shí)間: 2025-3-21 23:58 作者: HARP 時(shí)間: 2025-3-22 01:18 作者: 地名表 時(shí)間: 2025-3-22 08:15 作者: grounded 時(shí)間: 2025-3-22 10:35 作者: Dna262 時(shí)間: 2025-3-22 14:22 作者: 白楊魚 時(shí)間: 2025-3-22 21:07
http://image.papertrans.cn/h/image/421400.jpg作者: Deduct 時(shí)間: 2025-3-22 23:46 作者: palliate 時(shí)間: 2025-3-23 04:37 作者: 徹底明白 時(shí)間: 2025-3-23 07:21 作者: 禍害隱伏 時(shí)間: 2025-3-23 10:22 作者: eucalyptus 時(shí)間: 2025-3-23 16:26
Third-Generation Gravitational-Wave Observatories mergers in the universe – including some with incredible precision, and of mapping the stellar evolution of the universe. These projects are currently in the design stage and are expected to start operations around the mid-2030s. The concepts are slightly different but have many technical similarities.作者: 使害羞 時(shí)間: 2025-3-23 22:05
Binary Neutron Starsnal are important for the latter. I also present current observational capabilities and estimates for future detections and comment on the detectability of equations of state that include deconfined quark matter and possibly phase transitions.作者: 使閉塞 時(shí)間: 2025-3-23 23:50
Isolated Neutron Starsutron star interiors. In this article, we will review current theoretical models for continuous gravitational wave emission, and observational constraints, both electromagnetic and gravitational. Finally, we will discuss future observational possibilities.作者: SLAY 時(shí)間: 2025-3-24 04:55
Dynamical Formation of MergingStellar-Mass Binary Black Holesons on the characteristics of these merging binaries such as their gravitational wave frequency, eccentricity, mass, and spins to identify these gravitational wave source populations in merger catalogs. For dynamical merger pathways, we show that GW source catalogs carry information on the escape velocity of the host environment.作者: PON 時(shí)間: 2025-3-24 09:02 作者: 新陳代謝 時(shí)間: 2025-3-24 12:22
r researchers.Covers both experimental techniques and theoreThis handbook provides an updated comprehensive description of gravitational wave astronomy. In the first part, it reviews gravitational wave experiments, from ground and space based laser interferometers to pulsar timing arrays and indirec作者: 行為 時(shí)間: 2025-3-24 16:37 作者: Exposure 時(shí)間: 2025-3-24 22:50 作者: jealousy 時(shí)間: 2025-3-25 01:35
Francois Foucarttesting 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: preservative 時(shí)間: 2025-3-25 04:07
Livia Conti,Benjamin R. B. Saliwanchikies and DIBR-based view synthesis approaches, are reviewed. Conversion artifacts and evaluation of conversion quality are discussed, and the advantages and disadvantages of the different methods are elaborated. Furthermore, practical implementations for the conversion from monoscopic to stereoscopic and multi-view video are drawn.作者: 柔美流暢 時(shí)間: 2025-3-25 10:52
Harald Lück,Joshua Smith,Michele Punturoies and DIBR-based view synthesis approaches, are reviewed. Conversion artifacts and evaluation of conversion quality are discussed, and the advantages and disadvantages of the different methods are elaborated. Furthermore, practical implementations for the conversion from monoscopic to stereoscopic and multi-view video are drawn.作者: 使入迷 時(shí)間: 2025-3-25 11:51 作者: 使成波狀 時(shí)間: 2025-3-25 18:10 作者: Picks-Disease 時(shí)間: 2025-3-25 20:59
Brynmor Haskell,Kai Schwenzern 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: Brittle 時(shí)間: 2025-3-26 03:33 作者: MIR 時(shí)間: 2025-3-26 06:49 作者: extinguish 時(shí)間: 2025-3-26 10:21
Quantum Sensors with Matter Waves for GW Observationce detectors and detail their main noise sources. We describe the different projects undertaken worldwide to realize large-scale demonstrators and push further the current limitations. We finally give the roadmap for achieving the instrumental sensitivity required to seize the scientific opportunities offered by this new research domain.作者: Paradox 時(shí)間: 2025-3-26 14:01
Research and Development for Third-Generation Gravitational Wave Detectors-generation detectors will expand our view of the gravitational wave universe to cosmic distances. This chapter will discuss the technological research and development required to build these third-generation detectors.作者: 琺瑯 時(shí)間: 2025-3-26 20:50
ion for easy identification of unknown targets. Full indexes by catalog numbers and names allow searches for specific objects.978-1-4419-9418-9978-1-4419-9419-6Series ISSN 1431-9756 Series E-ISSN 2197-6562 作者: 勉強(qiáng) 時(shí)間: 2025-3-27 00:24 作者: Coronary-Spasm 時(shí)間: 2025-3-27 04:28 作者: 戰(zhàn)勝 時(shí)間: 2025-3-27 06:49
Environmental Noise in Gravitational-Wave Interferometersaths, 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: 揭穿真相 時(shí)間: 2025-3-27 10:14 作者: miscreant 時(shí)間: 2025-3-27 15:42 作者: 有毒 時(shí)間: 2025-3-27 17:52
ods to calculate gravitational waveforms. The fourth and last part of the book covers techniques employed in gravitational wave astronomy data analysis. This book represents both a valuable resource for graduate students and an important reference for researchers in gravitational wave astronomy.978-981-16-4306-4作者: exclusice 時(shí)間: 2025-3-28 00:04
is better reflects what one really sees – oftentimes barely – in the eyepiece. Even my circumspect observations in their edited form exude more certitude than is warranted, for in order not to be tiresome I deleted countless qualifiers (“about,” “more or less,” “apparently,” “might be,” “probably,” 作者: Forehead-Lift 時(shí)間: 2025-3-28 03:18 作者: 領(lǐng)先 時(shí)間: 2025-3-28 10:15
Fiodor Sorrentino,Jean-Pierre Zendring so central both to psychology and to connectionist modelling, it is one area about which everyone in the field has their own strong views, and the diversity and quality of the presentations and, just as importantly, the discussion which followed them, certainly attested to this.978-3-540-76208-9978-1-4471-1546-5Series ISSN 1431-6854 作者: obligation 時(shí)間: 2025-3-28 12:58 作者: 莎草 時(shí)間: 2025-3-28 17:31 作者: synchronous 時(shí)間: 2025-3-28 20:05 作者: 亞當(dāng)心理陰影 時(shí)間: 2025-3-29 00:58 作者: fluffy 時(shí)間: 2025-3-29 06:36 作者: medium 時(shí)間: 2025-3-29 09:02
Introduction to Gravitational Wave Astronomyers in this handbook. It starts with a brief historical review of the development of GW astronomy, from Einstein’s prediction of GWs in 1916 to the first direct detection in 2015. It presents the theory of linearized perturbations about Minkowski spacetime of Einstein’s equations and shows how gauge作者: 大暴雨 時(shí)間: 2025-3-29 13:50
Terrestrial Laser Interferometersrview of the history of how these laser interferometers prevailed as the most promising technology in the search for gravitational waves. We describe their working principles and their limitations and provide examples of some of the most important technologies that enabled their construction. We int作者: textile 時(shí)間: 2025-3-29 16:18 作者: ostrish 時(shí)間: 2025-3-29 22:10
Pulsar Timing Array Experimentscs. Pulsar timing arrays (PTAs) use sets of extremely well-timed pulsars as a galaxy-scale detector with arms extending between Earth and each pulsar in the array. These challenging experiments look for correlated deviations in the pulsars’ timing that are caused by low-frequency gravitational waves作者: 線 時(shí)間: 2025-3-30 00:26
Quantum Sensors with Matter Waves for GW Observationility of specific atomic energy levels makes atom interferometers and clocks ideal candidates to extend the frequency window for the observation of gravitational waves in the mid-frequency band, ranging from 10 mHz to 10 Hz. We present the geometry and functioning of this new class of ground and spa作者: BORE 時(shí)間: 2025-3-30 06:30 作者: 粗糙 時(shí)間: 2025-3-30 09:44
Third-Generation Gravitational-Wave Observatoriesored. A greatly more sensitive third generation of observatories is currently being planned: The Einstein Telescope in Europe and Cosmic Explorer in the USA. The Einstein Telescope is envisaged as an underground observatory in the shape of an equilateral triangle with a side length of 10 km located 作者: 平靜生活 時(shí)間: 2025-3-30 14:12
Research and Development for Third-Generation Gravitational Wave Detectorss were from instruments of the second generation of detectors – the first generation of kilometer-scale ground based detectors operated as planned, but did not conclusively observe gravitational waves. The second-generation detectors (Advanced LIGO and Advanced Virgo) opened the field, and the third作者: 斷言 時(shí)間: 2025-3-30 18:24 作者: 謊言 時(shí)間: 2025-3-30 22:27 作者: 不愛防注射 時(shí)間: 2025-3-31 02:07 作者: 哀求 時(shí)間: 2025-3-31 05:30 作者: 秘密會(huì)議 時(shí)間: 2025-3-31 09:37
Isolated Neutron Starsobservations 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: Kidney-Failure 時(shí)間: 2025-3-31 16:20
-Process Nucleosynthesis from Compact Binary Mergersing at high speed in space. Being matter coming from the violent disruption of a neutron star, these ejecta are initially very dense, hot, and extremely rich in neutrons. The few available protons form heavy nuclei (“seeds”) that absorb the more abundant free neutrons, increasing their size. The neu作者: 除草劑 時(shí)間: 2025-3-31 20:08 作者: 休息 時(shí)間: 2025-4-1 01:31
