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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Hippocampus

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.

秘傳

pulse-pressure

制定法律

Entreaty

ABIDE

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.

卡死偷電

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

一起

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.