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

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21#
發(fā)表于 2025-3-25 06:16:09 | 只看該作者
Monika Ankele,Céline Kaiser,Sophie Ledebureld theoretical models. The quintessence lagrangian is taken to be the sum of a simple exponentialpotential and a non-canonical kinetic term. This parameterization covers most variantsof quintessence and makes the naturalness conditions particularly transparent. Several “natural” scalar models lead,
22#
發(fā)表于 2025-3-25 11:00:46 | 只看該作者
Aufführen – Aufzeichnen – Anordnenhismystery, but no satisfactory solution has been found yet. The appearance of extradimensions in the framework of brane world systems seems to provide some new ideasto address this problem form a different point of view. We shall discuss some of thesenew approaches and see whether or not they lead
23#
發(fā)表于 2025-3-25 14:52:01 | 只看該作者
https://doi.org/10.1007/978-3-642-56643-1Baryon; Beta decay; Boson; Galaxy; Gravity; Neutrino; Particle Physics; astroparticles; astrophysics; cosmolo
24#
發(fā)表于 2025-3-25 18:30:42 | 只看該作者
25#
發(fā)表于 2025-3-25 21:17:34 | 只看該作者
26#
發(fā)表于 2025-3-26 01:05:46 | 只看該作者
27#
發(fā)表于 2025-3-26 08:01:33 | 只看該作者
28#
發(fā)表于 2025-3-26 11:33:57 | 只看該作者
The Distribution of Dark Matter in Galaxies: Constant-Density Dark Halos Envelop the Stellar Diskshe edge of the stellar disk, implying a constant dark halo density over the entire disk region. The structural properties of halos around normal spirals are similar to those around dwarf and low surface brightness galaxies; nevertheless they provide far more substantial evidence of the discrepancy b
29#
發(fā)表于 2025-3-26 12:40:02 | 只看該作者
30#
發(fā)表于 2025-3-26 20:26:23 | 只看該作者
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