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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

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发表于 2025-3-21 16:28:14 | 显示全部楼层 |阅读模式
书目名称Matter in the Universe
编辑Ph. Jetzer,K. Pretzl,R. Steiger
视频video
丛书名称Space Sciences Series of ISSI
图书封面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
描述This volume, the fourteenth in the Space Sciences Series of ISS/, is dedicated to the matter in the universe, which was the topic of a workshop organized 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 matter in the universe. Due to the importance of the field and the rapid developments which are taking place ISSI decided to organize a workshop on matter in the universe and invited nine convenors, John Ellis, Johannes Geiss, Philippe Jetzer, Heinrich Leutwyler, Klaus Pretzl, Rafael Rebolo, Norbert Straumann, Gustav Andreas Tammann and Rudolf von Steiger, who formulated the aims and goals of the meeting. The work­ shop was organized such as to have only 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
出版日期Book 2002
关键词Big Bang; Cosmology; Dark matter; Gravity; Relativistic jet; Universe; astrophysics
版次1
doihttps://doi.org/10.1007/978-94-017-2215-5
isbn_softcover978-90-481-6038-9
isbn_ebook978-94-017-2215-5Series ISSN 1385-7525
issn_series 1385-7525
copyrightSpringer Science+Business Media B.V. 2002
The information of publication is updating

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发表于 2025-3-21 22:14:56 | 显示全部楼层
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.
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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.
发表于 2025-3-22 23:39:48 | 显示全部楼层
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
发表于 2025-3-23 03:06:29 | 显示全部楼层
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.
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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.
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