Gawiser1, Silk

  • 1E. Gawiser is at the Department of Physics, University of California at Berkeley, Berkeley, CA 94720, USA. E-mail: gawiser@astron. berkeley.edu. J. Silk is at the Departments of Physics and Astronomy and the Center for Particle Astrophysics, Univ.

Science (New York, N.Y.)
|June 5, 1998
PubMed
まとめ

宇宙マイクロ波の背景放射と銀河の分布データは,一般的な宇宙学モデルに挑戦しています. しかし,冷たい + 熱いダークマターモデルは観測と一致しており,大規模なニュートリノが重要な宇宙物質を構成する可能性があることを示唆しています.

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