Titlebook: Dark Matter in Astro- and Particle Physics; Proceedings of the I H. V. Klapdor-Kleingrothaus Conference proceedings 2001 Springer-Verlag Be

exclusice

Conference proceedings 2001alks in this book emphasize the experimental and theoretical status and perspectives of the ongoing search for dark matter, and the future potential of the field into the next millennium, stressing in particular the interplay between astro- and particle physics.

infarct

headway

極深

Decibel

Contribution to Dark Matter from Extragalactic Dustent models of the composition of the ISM..I present a few examples of these recent observations. Cold dust is found to follow the large-scale HI warps (NGC 4565) and even to trace interactions (NGC 4631).

會議

換話題

Self-Interacting Cold Dark Matter Halosed data on the rotation curves of dwarf galaxies. However, subsequently, core collapse leads to an even steeper central density cusp. In order to explain the observed dark matter rotation curves by weak interaction, the cross section must be in a narrow range around......

儲備

Can Quintessence Be Natural?ameterization covers most variantsof quintessence and makes the naturalness conditions particularly transparent. Several “natural” scalar models lead, for the present cosmological era, to a large fraction ofhomogeneous dark energy density and an acceleration of the scale factor as suggestedby observation.

暴發(fā)戶

使厭惡

https://doi.org/10.1007/978-3-642-79389-97) of the density is in the form of cosmological term or “dark (vacuum) energy”. The density of the matter is 0.3 – 0.4 (including hot and cold dark matter and luminous matter), the upper limit of the density of the hot dark matter is 0.05, all in units of the critical cosmological density.