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

LVAD360

FLIC

Status and Physics of the Fermilab TEVATRONded to create the TEVATRON. Here we describe the fixed target physics program, largely from the major runs of 800 GeV in 1985 and 1987. The first collider run of . at 1.8 TeV took place from January–May 1987. The operation and physics results of the collider will also be presented. Finally, an outli

Insatiable

Results from the FREJUS Experimentic neutrino (anti-neutrino) interactions in the detector shows that the behaviour of the apparatus is well understood. The analysis of the nucleon stability 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 m

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柏樹(shù)

Underground Physicsnos receive more attention. In fact, present experiments on ∣3∣3 decay and the new thecniques recently developed are very promising and garantee that in a near future very stringent limit on neutrinoless decay and Majoron emission will be reached and two neutrino mode observed for a few nuclei..Sola

LUCY

Probing the Universe with Rich Clusters of Galaxies as Giant Gravitational Telescopesservations at the European Observatory: the luminous Einstein arcs (or rings) in rich clusters of galaxies. We also present more recent observations with the Canada France Hawa? telescope which prove that the cluster A370 acts on the background galaxies as a giant gravitational telescope. This obser

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Dark Matter in Astronomy dark matter in the solar neighbourhood..Evidence for dark matter in the outer parts of galaxies is found both in extended rotation curves and in the relative motions of binary galaxies. The best evidence for dark matter remains the dynamics of the great clusters of galaxies, i.e. where galaxies are

ATP861

Dark Matter Candidatesf? Needless to say, the answer to this question has very important implications for the evolution of the Universe, determining both the ultimate fate and the course of structure formation. Remarkably, at this late date in the history of the Universe we still do not have a definitive answer to this s

FIR

Astrophysics and Space Science Libraryhttp://image.papertrans.cn/b/image/163660.jpg

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