標(biāo)題: Titlebook: Astronomy, Cosmology and Fundamental Physics; Proceedings of the E Peter A. Shaver,Luigi DiLella,Alvaro Giménez Conference proceedings 2003 [打印本頁(yè)] 作者: HAND 時(shí)間: 2025-3-21 17:23
書目名稱Astronomy, Cosmology and Fundamental Physics影響因子(影響力)
書目名稱Astronomy, Cosmology and Fundamental Physics影響因子(影響力)學(xué)科排名
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書目名稱Astronomy, Cosmology and Fundamental Physics被引頻次
書目名稱Astronomy, Cosmology and Fundamental Physics被引頻次學(xué)科排名
書目名稱Astronomy, Cosmology and Fundamental Physics年度引用
書目名稱Astronomy, Cosmology and Fundamental Physics年度引用學(xué)科排名
書目名稱Astronomy, Cosmology and Fundamental Physics讀者反饋
書目名稱Astronomy, Cosmology and Fundamental Physics讀者反饋學(xué)科排名
作者: 粗野 時(shí)間: 2025-3-22 00:02
Cosmological Weak Lensing,We present the current status of cosmic shear studies and their implications on cosmological models. Theoretical expectations and observational results are discussed in the framework of standard cosmology and CDM scenarios. The potentials of the next generation cosmic shear surveys are discussed.作者: RAG 時(shí)間: 2025-3-22 04:00
Cosmic Microwave Background Fluctuations,smological model, these structures result from acoustic oscillations of the primeval plasma at recombination (.). In the framework of the Hot Big Bang theory with the inflation hypothesis, the statistical properties of the image of the CMB allow us to measure most of the cosmological parameters.作者: 氣候 時(shí)間: 2025-3-22 04:48
The State of the Universe: Cosmological Parameters 2002,o measure cosmological parameters has increased tremendously, while at the same time, we have been surprised beyond our wildest dreams by the results. I review here recent measurements of the expansion rate, geometry, age, matter content, and equation of state of the universe, and discuss the implications for our understanding of cosmology.作者: ALB 時(shí)間: 2025-3-22 10:12
The Standard Model of Particle Physics: Status and Low-Energy Tests,. An overview of the present experimental status is presented. The main topics discussed are the muon anomalous magnetic moment, the asymptotic freedom of strong interactions, the lepton universality of gauge couplings, the quark flavour structure and CP violation.作者: stress-response 時(shí)間: 2025-3-22 14:56
Astroparticle Physics with the L3+C Detector, years 1999 and 2000. Thanks to the unique properties of this detector, research topics relevant to various current problems in cosmic ray muon and astroparticle physics can be studied. The status of the data analysis on different subjects is presented.作者: 耕種 時(shí)間: 2025-3-22 20:30 作者: arboretum 時(shí)間: 2025-3-22 23:16 作者: DAMN 時(shí)間: 2025-3-23 05:22 作者: 欲望 時(shí)間: 2025-3-23 05:37
ESO Astrophysics Symposiahttp://image.papertrans.cn/b/image/163661.jpg作者: MAL 時(shí)間: 2025-3-23 12:10 作者: 我不重要 時(shí)間: 2025-3-23 14:19 作者: 瘋狂 時(shí)間: 2025-3-23 20:17 作者: strain 時(shí)間: 2025-3-24 01:51
Julia Naskrent,Ann-Kristin Blocktribute differently to the evolution of the scale parameter it is possible to disentangle their importance as a function of time. Type Ia Supernovae are the only distance indicator available over a large enough range of the universal history. All other observations are based either on the assumption作者: Morbid 時(shí)間: 2025-3-24 04:24
Marke als Mittel im Kampf um Anerkennungurvey of X-ray selected clusters of galaxies we determine statistical properties of the galaxy cluster population, their spatial correlation, and the density fluctuation power spectrum of the cosmic matter distribution on large scales up to about 1 Gpc. Comparing these results with predictions of co作者: 硬化 時(shí)間: 2025-3-24 08:52
https://doi.org/10.1007/978-3-658-19668-4e cooling universe - described by just a few parameters - to a very messy hot one - the realm of radiative, hydrodynamic and star formation processes. In popular cold dark matter cosmological scenarios, stars and quasars may have first appeared in significant numbers around a redshift of 10 or so, a作者: Additive 時(shí)間: 2025-3-24 12:24 作者: 鴿子 時(shí)間: 2025-3-24 16:35 作者: Fantasy 時(shí)間: 2025-3-24 23:04 作者: 蚊子 時(shí)間: 2025-3-25 01:35 作者: 咆哮 時(shí)間: 2025-3-25 04:34 作者: 盟軍 時(shí)間: 2025-3-25 08:06 作者: 無(wú)禮回復(fù) 時(shí)間: 2025-3-25 11:54 作者: Slit-Lamp 時(shí)間: 2025-3-25 18:37 作者: 明智的人 時(shí)間: 2025-3-25 22:07 作者: Dysarthria 時(shí)間: 2025-3-26 03:28 作者: WITH 時(shí)間: 2025-3-26 07:05
Holger J. Schmidt,Carsten Baumgarthand mass composition of cosmic rays are reviewed. The enigma set by the existence of ultra high-energy cosmic rays remains and ideas proposed to explain it are discussed. Progress with the construction of the Pierre Auger Observatory and plans for the EUSO space instrument are outlined.作者: ablate 時(shí)間: 2025-3-26 10:02 作者: 彎腰 時(shí)間: 2025-3-26 15:28
https://doi.org/10.1007/978-3-658-39568-1ime. In the soft (0.5-2 keV) band more than 90% of the XRB flux has been resolved using 1.4 Msec observations with ROSAT [17] and recently 1-2 Msec Chandra observations [29,4] and 100 ksec observations with XMM-Newton [18]. In the harder (2-10 keV) band a similar fraction of the background has been 作者: 幻影 時(shí)間: 2025-3-26 18:16
Astronomy, Cosmology and Fundamental Physics978-3-540-44851-8Series ISSN 1431-2433 Series E-ISSN 1611-6143 作者: 杠桿支點(diǎn) 時(shí)間: 2025-3-27 00:07 作者: generic 時(shí)間: 2025-3-27 02:17 作者: PAC 時(shí)間: 2025-3-27 07:43
Marc Herz,Julius Arnegger,Marius Mayer. An overview of the present experimental status is presented. The main topics discussed are the muon anomalous magnetic moment, the asymptotic freedom of strong interactions, the lepton universality of gauge couplings, the quark flavour structure and CP violation.作者: 混合物 時(shí)間: 2025-3-27 13:12 作者: 食品室 時(shí)間: 2025-3-27 15:40
Holger J. Schmidt,Carsten Baumgarthfetime can provide significant progress in exploring the range of variability suggested by QSO data. We also discuss the effects of a time varying . on stellar structure and evolution. We find that radioactive dating of ancient stars can offer a new observational window.作者: 伙伴 時(shí)間: 2025-3-27 21:41 作者: affluent 時(shí)間: 2025-3-28 00:28 作者: 北京人起源 時(shí)間: 2025-3-28 05:06
First Light and the Reionization of the Universe,tages depends on the power-spectrum of density fluctuations on small scales and on a complex network of poorly understood ‘feedback’ mechanisms, and is one of the missing links in galaxy formation and evolution studies.作者: FLORA 時(shí)間: 2025-3-28 09:40
Gamma-Ray Bursts: The Most Powerful Cosmic Explosions,explosions in the Earth’s atmosphere or in space. To check for possible radioactivity produced by explosions on the backside of the Moon, the Vela satellites had very wide orbits extending halfway to the Moon. There were always several of them orbiting the Earth at any given time. In 1967 they detec作者: panorama 時(shí)間: 2025-3-28 12:48 作者: 盡管 時(shí)間: 2025-3-28 18:37 作者: Common-Migraine 時(shí)間: 2025-3-28 22:18 作者: 全神貫注于 時(shí)間: 2025-3-29 01:13 作者: 集合 時(shí)間: 2025-3-29 05:49 作者: forthy 時(shí)間: 2025-3-29 09:39
Constraining Cosmological Parameters with Observations of Galaxy Clusters,smological models we obtain tight constrains for the matter density parameter of the Universe, consistent with the combined results from observations of the microwave background anisotropies and distant type Ia supernovae.作者: Asseverate 時(shí)間: 2025-3-29 15:12
Beyond the Standard Model,nts are reviewed using benchmark scenarios to focus the discussion. The status and prospects of experiments on neutrino masses and oscillations are also reviewed, as is the possibility of observing transitions between different charged leptons.作者: Celiac-Plexus 時(shí)間: 2025-3-29 15:33 作者: 新字 時(shí)間: 2025-3-29 21:03 作者: 從容 時(shí)間: 2025-3-30 03:00
Carsten Baumgarth,Holger J. Schmidtnts are reviewed using benchmark scenarios to focus the discussion. The status and prospects of experiments on neutrino masses and oscillations are also reviewed, as is the possibility of observing transitions between different charged leptons.作者: thrombosis 時(shí)間: 2025-3-30 07:42 作者: seruting 時(shí)間: 2025-3-30 10:05
1431-2433 tes, evidence for neutrino oscillations, space experiments on fundamental physics, and discoveries of extrasolar planets. This book will be useful for researchers and graduate students who wish to have a broad overview of the current developments in these fields..978-3-642-07281-9978-3-540-44851-8Series ISSN 1431-2433 Series E-ISSN 1611-6143 作者: scrape 時(shí)間: 2025-3-30 12:28
Holger J. Schmidt,Carsten Baumgarthnts, both on the ground and in space, gives fascinating prospects also for observational cosmology and astroparticle physics. Through realistically possible further observational developments at high mountain altitudes a rapid extension of the field is to be expected.作者: 歌唱隊(duì) 時(shí)間: 2025-3-30 19:30
Charlotte Heyder,Isabelle Hillebrandteutrinos from MeV to EeV energy by a variety of mechanisms. The important conclusion is that, independently of the specific blueprint of the source, it takes a kilometer-scale neutrino observatory to detect the neutrino beam associated with the highest energy cosmic rays and gamma rays. The technology for commissioning such instruments exists.作者: 行乞 時(shí)間: 2025-3-30 23:41
Astrophysics with High Energy Gamma Rays,nts, both on the ground and in space, gives fascinating prospects also for observational cosmology and astroparticle physics. Through realistically possible further observational developments at high mountain altitudes a rapid extension of the field is to be expected.作者: 領(lǐng)帶 時(shí)間: 2025-3-31 03:38
High-Energy Neutrinos from Cosmic Rays,eutrinos from MeV to EeV energy by a variety of mechanisms. The important conclusion is that, independently of the specific blueprint of the source, it takes a kilometer-scale neutrino observatory to detect the neutrino beam associated with the highest energy cosmic rays and gamma rays. The technology for commissioning such instruments exists.作者: GEAR 時(shí)間: 2025-3-31 05:55 作者: 鎮(zhèn)痛劑 時(shí)間: 2025-3-31 11:54
Co-creation: Building brands togetherthat it requires scalar fields with extremely flat potentials or four-form fields coupled to branes with an extremely small charge. Some recent suggestions are reviewed on how such features can arise in particle physics models.作者: inhibit 時(shí)間: 2025-3-31 17:15
Nina De Cleir,Inga Schmidt-Rossicles, such as neutrinos, or other unknown particles like the axion or the supersymmetric LSP version of the Weakly Interacting Massive Particles (WIMPs)? If WIMPs are the Dark Matter in the Galaxy, how can they be detected? This paper briefly reviews the current status of some searches for this dark component of the Universe.作者: 別炫耀 時(shí)間: 2025-3-31 19:18
