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Titlebook: Astronomy, Cosmology and Fundamental Physics; Proceedings of the T Michele Caffo,Roberto Fanti,Alvio Renzini Conference proceedings 1989 Kl

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11#
發(fā)表于 2025-3-23 09:45:48 | 只看該作者
Results from the FREJUS Experimentbility is described and lifetime limits are given for various decay modes with a charged lepton or an anti-neutrino in the final state. Neutrino and muon data have been also analyzed to search for a signal coming from the supernova SN1987A, yielding a negative answer.
12#
發(fā)表于 2025-3-23 17:08:27 | 只看該作者
Probing the Universe with Rich Clusters of Galaxies as Giant Gravitational Telescopesith the Canada France Hawa? telescope which prove that the cluster A370 acts on the background galaxies as a giant gravitational telescope. This observational advance will probably open a new stage in the study of gravitational lenses and their implications in cosmology.
13#
發(fā)表于 2025-3-23 18:15:00 | 只看該作者
https://doi.org/10.1007/978-981-33-6244-4s, a few lines of which are quoted above. The crucial clue in the solution of this mystery was the . of an event; the dog did . bark. It was in effect a null experiment--the value of the incident lay in what did not happen. Holmes correctly deduced that because the dog did not bark, the intruder must have been its owner.
14#
發(fā)表于 2025-3-24 00:19:02 | 只看該作者
The Cosmic Microwave Background Radiation and the Dog in the Nights, a few lines of which are quoted above. The crucial clue in the solution of this mystery was the . of an event; the dog did . bark. It was in effect a null experiment--the value of the incident lay in what did not happen. Holmes correctly deduced that because the dog did not bark, the intruder must have been its owner.
15#
發(fā)表于 2025-3-24 03:00:30 | 只看該作者
16#
發(fā)表于 2025-3-24 08:01:01 | 只看該作者
17#
發(fā)表于 2025-3-24 11:25:27 | 只看該作者
Recent Results from the ,,,, Colliders TRISTAN and CESR
18#
發(fā)表于 2025-3-24 15:48:41 | 只看該作者
Lithium -7 as a cosmological observablee comparison between the present calculations and the cosmic abundances suggest that the contrast R between the phases is unlikely to be larger than ten. This result is in agreement with the best estimate of the critical temperature of the phase transition (180 MeV
19#
發(fā)表于 2025-3-24 20:40:46 | 只看該作者
20#
發(fā)表于 2025-3-25 02:30:18 | 只看該作者
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