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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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期刊全稱Astronomy, Cosmology and Fundamental Physics
期刊簡稱Proceedings of the T
影響因子2023Michele Caffo,Roberto Fanti,Alvio Renzini
視頻videohttp://file.papertrans.cn/164/163660/163660.mp4
學科分類Astrophysics and Space Science Library
圖書封面Titlebook: Astronomy, Cosmology and Fundamental Physics; Proceedings of the T Michele Caffo,Roberto Fanti,Alvio Renzini Conference proceedings 1989 Kl
影響因子In the development of Fundamental Physics on one side, and of Astronomy/Cosmology on the other side, periods of parallell, relatively independent progress seem to alternate with others of intense interaction and mutual influence. To this latter case belong the very beginnings of Modern Physics, with Galileo and Newton. There is now a widespread feeling that another of such flourishing periods may have started some ten years ago, with the advent of Unified Theories and the introduction of Inflationary Cosmologies. The interaction between the two disciplines has become tighter ever since, spurring studies of e. g. astronomical and particle Dark Matter candidates, Superstrings and Cosmic Strings, phase transitions in the Early Universe, etc. etc. Then the recent birth of Neutrino Astronomy has added further flavor to this splendid conjunction. It was indeed with the clear perception of this trend that six years ago CERN and ESO decided to jointly organize a series of symposia focusing on the interactions between Astronomy, Cosmology, and Fundamental Physics, to be held about every two years. The aim of these meetings is to bring together astronomers, cosmologists, and particle physici
Pindex Conference proceedings 1989
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Julia Naskrent,Ann-Kristin Blockf assessing Ω from mass to light ratios give zero dark matter content to voids. Since much of the universe is empty, Ω could be much greater than the optical assessment of 0.1 < Ω < 0.3. The IRAS high Ω is explained as a biassing of IRAS galaxies away from high density regions.
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Dark Matter in Astronomyf assessing Ω from mass to light ratios give zero dark matter content to voids. Since much of the universe is empty, Ω could be much greater than the optical assessment of 0.1 < Ω < 0.3. The IRAS high Ω is explained as a biassing of IRAS galaxies away from high density regions.
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https://doi.org/10.1007/978-981-33-6244-4bility 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.
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Cosmological Parameters of the Universeesent epoch. Present data favor H. ≈ 60–80 km/sec/Mpc and Ω. ≈ 0.1–0.2. Within observational errors, these values are consistent with T. ~ 15 Gyr and Λ. = 0, but the low value of Ω. appears incompatible with the inflation paradigm of the early Big Bang.
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