请输入您要查询的百科知识:

 

词条 Quark epoch
释义

  1. See also

  2. References

{{Physical cosmology}}

In physical cosmology the Quark epoch was the period in the evolution of the early universe when the fundamental interactions of gravitation, electromagnetism, the strong interaction and the weak interaction had taken their present forms, but the temperature of the universe was still too high to allow quarks to bind together to form hadrons. The quark epoch began approximately 10−12 seconds after the Big Bang, when the preceding electroweak epoch ended as the electroweak interaction separated into the weak interaction and electromagnetism. During the quark epoch the universe was filled with a dense, hot quark–gluon plasma, containing quarks, leptons and their antiparticles. Collisions between particles were too energetic to allow quarks to combine into mesons or baryons. The quark epoch ended when the universe was about 10−6 seconds old, when the average energy of particle interactions had fallen below the binding energy of hadrons. The following period, when quarks became confined within hadrons, is known as the hadron epoch.

See also

  • Chronology of the universe
  • Cosmogony

References

  • {{cite book | last = Allday | first = Jonathan | title = Quarks, Leptons and the Big Bang | publisher = | edition = Second | date = 2002 | isbn = 978-0-7503-0806-9 }}
  • Physics 175: Stars and Galazies - The Big Bang, Matter and Energy{{dead link|date=July 2016 |bot=InternetArchiveBot |fix-attempted=yes }}; Ithaca College, New York
{{Big Bang timeline}}{{Cosmology-stub}}

2 : Big Bang|Physical cosmology

随便看

 

开放百科全书收录14589846条英语、德语、日语等多语种百科知识,基本涵盖了大多数领域的百科知识,是一部内容自由、开放的电子版国际百科全书。

 

Copyright © 2023 OENC.NET All Rights Reserved
京ICP备2021023879号 更新时间:2024/9/23 5:34:10