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超高能宇宙射线、宇宙学常数与θ真空

Ultrahigh energy cosmic rays, cosmological constant, and theta vacua.

作者信息

Jaikumar Prashanth, Mazumdar Anupam

机构信息

Physics Department, McGill University, Montréal, 3600, Québec, Canada H3A 2T8.

出版信息

Phys Rev Lett. 2003 May 16;90(19):191301. doi: 10.1103/PhysRevLett.90.191301. Epub 2003 May 15.

Abstract

We propose that the origin of ultrahigh energy cosmic rays beyond the Greisen-Zatsepin-Kuzmin cutoff and the origin of small cosmological constant can both be explained by vacuum tunneling effects in a theory with degenerate vacua and fermionic doublets. By considering the possibility of tunneling from a particular winding number state, accompanied by violation of some global quantum number of fermions, the small value of the vacuum dark energy and the production of high energy cosmic rays are shown to be related. We predict that the energy of such cosmic rays should be at least 5x10(14) GeV.

摘要

我们提出,超出格列森-扎采平-库兹明截断的超高能宇宙射线的起源以及小宇宙学常数的起源,都可以在一个具有简并真空和费米子双重态的理论中,通过真空隧穿效应来解释。通过考虑从特定缠绕数态隧穿的可能性,伴随着某些费米子全局量子数的违反,真空暗能量的小值与高能宇宙射线的产生被证明是相关的。我们预测,此类宇宙射线的能量应至少为5×10¹⁴ GeV。

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