【24h】

Pulsars: Gigantic nuclei

机译:脉冲星:巨大核

获取原文
获取原文并翻译 | 示例
           

摘要

What is the real nature of pulsars? This is essentially a question of the fundamental strong interaction between quarks at low-energy scale and hence of the non-perturbative quantum chromo-dynamics, the solution of which would certainly be meaningful for us to understand one of the seven millennium prize problems (i.e., "Yang-Mills Theory") named by the Clay Mathematical Institute. After a historical note, it is argued here that a pulsar is very similar to an extremely big nucleus, but is a little bit different from the gigantic nucleus speculated 80 years ago by L. Landau. The paper demonstrates the similarity between pulsars and gigantic nuclei from both points of view: the different manifestations of compact stars and the general behavior of the strong interaction.
机译:脉冲星的真正本质是什么?这本质上是一个问题,即低能级夸克之间基本的强相互作用,因此是非微扰量子色动力学的问题,对于我们理解七个千年奖问题之一(即,“杨米尔斯理论”)由克莱数学研究所命名。根据历史记载,这里有人说脉冲星与一个非常大的原子核非常相似,但是与80年前L.Landau推测的巨大原子核有些不同。本文从两种观点证明了脉冲星和巨大核之间的相似之处:紧密恒星的不同表现形式和强相互作用的一般行为。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号