极早期宇宙

  • 网络very early universe
极早期宇宙极早期宇宙
  1. 目前观测到的重子光子数比10~(-9)可能是由极早期宇宙中的超重玻色子的衰变产生的,在这种衰变中C及CP是破坏的。

    The observed baryon-to-photon ratio of 10-9 could be produced by the decays of superheavy bosons in the very early universe if C and CP are violated in its actions .

  2. 极早期宇宙的研究中若干问题浅析

    Some Remarks on the Research of the Very Early Universe