標(biāo)題: Titlebook: Matter in the Universe; Ph. Jetzer,K. Pretzl,R. Steiger Book 2002 Springer Science+Business Media B.V. 2002 Big Bang.Cosmology.Dark matter [打印本頁(yè)] 作者: 服裝 時(shí)間: 2025-3-21 16:28
書(shū)目名稱(chēng)Matter in the Universe影響因子(影響力)
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書(shū)目名稱(chēng)Matter in the Universe讀者反饋學(xué)科排名
作者: Hippocampus 時(shí)間: 2025-3-21 22:14
Dark Matter from Weak Gravitational Lensingiverse at all scales. Put into the perspective of this conference, the most illustrative new results concern clusters of galaxies and cosmic shear. In the following I focus on these two topics and discuss the present status of cosmological applications of weak lensing.作者: 秘傳 時(shí)間: 2025-3-22 02:48 作者: pulse-pressure 時(shí)間: 2025-3-22 04:54 作者: 制定法律 時(shí)間: 2025-3-22 09:26 作者: Entreaty 時(shí)間: 2025-3-22 13:56 作者: ABIDE 時(shí)間: 2025-3-22 19:37
Clouds and Diffuse Baryonic Dark Matterlo. Basically, cosmic-ray protons in the galactic halo scatter on the clouds clumped into dark clusters, giving rise to a .-ray flux. An analysis of EGRET data has led to the discovery of a statistically significant diffuse .-ray emission from the galactic halo, which turns out to be in remarkably good agreement with our prediction.作者: 卡死偷電 時(shí)間: 2025-3-22 23:39
Book 2002zed by ISSI from 19 to 22 March 2001 in Bern. The aim of the meeting was to gather ac- tive researchers from various fields (cosmology, astrophysics, nuclear and particle physics as well as space science) to asses the exciting new developments in the search for abundant and yet unknown forms of matt作者: 一起 時(shí)間: 2025-3-23 03:06
Cosmic Microwave Background Anisotropy Observationsleosynthesis are the first results emerging from the current CMB data. Future experiments on ground (mainly interferometers), in balloons and from space (MAP and Planck missions) have the potential to constrain more than 10 cosmological parameters with high precision.作者: 裝入膠囊 時(shí)間: 2025-3-23 06:56
Mass Distribution in Our Galaxyive, near-maximal disk in our ～ ..,Sbc spiral galaxy. While the outer rotation curve and global mass distribution are not as readily measured as in similar spiral galaxies, the dark halo mass estimated from satellite velocities is consistent with a flat rotation curve continuing on from the luminous mass distribution.作者: GOAT 時(shí)間: 2025-3-23 13:01
Quantum Field Theoretic Description of Matter in the Universeos within a supernova plasma will be discussed. Then the possible presence of quark matter in a neutron star core and finally the interaction of light with the Cosmic Microwave Background will be considered.作者: Arbitrary 時(shí)間: 2025-3-23 15:07
D. Reimersn is a hindrance to the implementation of a fast recovery of patients. It’s mandatory for nurses to implement the ICU-AW prevention through an active collaboration in early patients’ positioning, progressive mobilization, and active collaboration during physiotherapy interventions. The only contrain作者: Individual 時(shí)間: 2025-3-23 21:38 作者: Suggestions 時(shí)間: 2025-3-23 23:36 作者: 殺死 時(shí)間: 2025-3-24 04:43 作者: Aspirin 時(shí)間: 2025-3-24 08:05
M. H. Thomaprovided in prison and throughout the Criminal Justice System and are therefore at a disadvantage compared to the general population. This chapter will commence with definitions of intellectual disabilities and the changes in these definitions due to changing legislation and policy, which is partial作者: 有危險(xiǎn) 時(shí)間: 2025-3-24 11:05 作者: 獨(dú)白 時(shí)間: 2025-3-24 17:08
Cosmic Microwave Background Anisotropy Observations CMB, achieved about 10 years ago, boosted a large number of ground-based and balloon-borne experiments that have delineated the CMB angular power spectrum up to spherical harmonic multipole ? ~ 1000. A wealth of information on cosmological parameters is being revealed by these measurements. Very re作者: Jubilation 時(shí)間: 2025-3-24 20:07 作者: intelligible 時(shí)間: 2025-3-25 01:44 作者: FLIP 時(shí)間: 2025-3-25 06:08 作者: Grandstand 時(shí)間: 2025-3-25 09:11 作者: 險(xiǎn)代理人 時(shí)間: 2025-3-25 14:06
Clouds and Diffuse Baryonic Dark Matteroud suggest that at most about 20% of the halo dark matter is in form of MACHOs (Massive Astrophysical Compact Halo Objects). The dark matter could also, at least partially, be made of cold molecular clouds (mainly H.). We proposed a model for baryonic dark matter, according to which dark clusters o作者: CLOUT 時(shí)間: 2025-3-25 16:29
Mass Distribution in Our Galaxylo. A new luminosity model consistent with the COBE NIR data and the apparent magnitude distributions of bulge clump giant stars has bulge/bar length of (? 3.5 kpc, axis ratios of 1:(0.3–0.4):0.3, and short disk scale-length (? 2.1 kpc). Gas-dynamical flows in the potential of this model with consta作者: 原來(lái) 時(shí)間: 2025-3-25 20:09 作者: 時(shí)間等 時(shí)間: 2025-3-26 00:18 作者: obsession 時(shí)間: 2025-3-26 07:50
Dark Quark ‘Stars’: Do They Matter for ΩMatter?and antileptons 2) a shell of hadrons in particular ., ., Λ and Σ. and leptons or antileptons and 3) a shell of hydrogen in the superfluid phase. If the superfluid hydrogen phase goes over into the electromagnetic plasma phase at densities well below one atom (10 fm)., as is usually assumed, the hyd作者: 消息靈通 時(shí)間: 2025-3-26 10:39
978-90-481-6038-9Springer Science+Business Media B.V. 2002作者: Infant 時(shí)間: 2025-3-26 13:05 作者: 過(guò)度 時(shí)間: 2025-3-26 17:29 作者: BOLT 時(shí)間: 2025-3-26 21:00 作者: 過(guò)份 時(shí)間: 2025-3-27 04:10
Weak and Strong Lensing StatisticsAfter a brief introduction to gravitational lensing theory, a rough overview of the types of gravitational lensing statistics that have been performed so far will be given. I shall then concentrate on recent results of galaxy-galaxy lensing, which indicate that galactic halos extend much further than can be probed via rotation of stars and gas.作者: 拾落穗 時(shí)間: 2025-3-27 09:00 作者: ALOFT 時(shí)間: 2025-3-27 13:13 作者: 總 時(shí)間: 2025-3-27 14:20
AxionsAxions are one of the few particle-physics candidates for dark matter which are well motivated independently of their possible cosmological role. A brief review is given of the theoretical motivation for axions, their possible role in cosmology, the existing astrophysical limits, and the status of experimental searches.作者: Vasoconstrictor 時(shí)間: 2025-3-27 21:14
Space Sciences Series of ISSIhttp://image.papertrans.cn/m/image/627809.jpg作者: cortisol 時(shí)間: 2025-3-28 00:36 作者: cathartic 時(shí)間: 2025-3-28 02:36
Book 2002only plenary sessions with typically half- hour presentations and ample time for discussions. The last day was devoted to conclusions and future objectives. The knowledge of the amount and nature of matter present in the universe is undoubtedly one of the most relevant topics oftoday‘s astrophysics 作者: 滴注 時(shí)間: 2025-3-28 08:29 作者: 業(yè)余愛(ài)好者 時(shí)間: 2025-3-28 12:28 作者: MIR 時(shí)間: 2025-3-28 16:12
y during CPR. Aspects such as visiting hours, number of visitors, and dressing procedures will also be examined, with a particular focus on the levels of infections. We will argue that patients, their families, and healthcare professionals can benefit from open visiting policies. ICUs should become 作者: 圍巾 時(shí)間: 2025-3-28 20:09 作者: 吸氣 時(shí)間: 2025-3-28 23:43 作者: 的闡明 時(shí)間: 2025-3-29 04:11 作者: 憤世嫉俗者 時(shí)間: 2025-3-29 08:02 作者: Guileless 時(shí)間: 2025-3-29 13:08 作者: 節(jié)約 時(shí)間: 2025-3-29 18:03 作者: 發(fā)起 時(shí)間: 2025-3-29 21:21
1860-4862 : .In this book, an international team of highly qualified experts treats important topics in "Acoustic Echo and Noise Control" and report the latest developments. Methods for enhancing the quality of transmitted speech signals are gaining growing attention in universities and in industrial developm作者: 和音 時(shí)間: 2025-3-30 03:52 作者: 調(diào)味品 時(shí)間: 2025-3-30 04:50
Maximum Drift Velocity in Semiconductors,lyze the ballistic transit of electrons injected at high initial velocity into a semiconductor (Sec. 3.4). The material in this chapter is essential to understanding the physics of transistor operation that will be developed in subsequent chapters and to evaluating possibilities for achieving maximum transistor operating speed.作者: COMMA 時(shí)間: 2025-3-30 08:56
The Theory of Complex Formal Organization,es, mitochondria, Golgi apparatus and rough ER which was dilated considerably. Radioimmunoassay indicated a significant decrease in hormone levels of plasma TSH, PRL and LH after colchicine and vinblastine treatment. When such drug-injected rats were further stimulated with hypothalamic releasing ho作者: Insensate 時(shí)間: 2025-3-30 13:21 作者: Semblance 時(shí)間: 2025-3-30 17:24 作者: 晚來(lái)的提名 時(shí)間: 2025-3-30 20:56
Joost Augusteijn,Patrick Dassen,Maartje Janseamming and be able to apply these concepts and techniques to your next cloud application developments.??..What You‘ll Learn..·???????? Start programming with Ballerina?..·???????? Gain the basics978-1-4842-5138-6978-1-4842-5139-3作者: 放氣 時(shí)間: 2025-3-31 04:15
Following the Emergence of Unpredictable Uses? New Stakes and Tasks for a Social Scientific Understa作者: 連接 時(shí)間: 2025-3-31 07:11
Book 2014This unique book provides a rare insight into the debilitating impact of regimes that fail to respond to the complex and gender specific needs of women behind bars. Exploring the marginalization, mental health and experiences of women in prison, it specifically focuses on the legacy of women‘s imprisonment in Northern Ireland.作者: 省略 時(shí)間: 2025-3-31 11:13
