Addendum to "Neutrinos in the Cosmos": Neutrino Halos as the 25% Dark Matter

被引:0
作者
Hwang, W-Y. Pauchy [1 ,2 ]
机构
[1] Natl Taiwan Univ, Asia Pacific Org Cosmol & Particle Astrophys, Inst Astrophys, Ctr Theoret Sci, Taipei 106, Taiwan
[2] Natl Taiwan Univ, Dept Phys, Taipei 106, Taiwan
来源
UNIVERSE-TAIPEI | 2016年 / 4卷 / 01期
关键词
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We propose to detect the presence of the Fermi-Dirac sphere of the neutrino halo of the Earth (or, of the Venus). The reaction v(Solar/UHE)+(nu) over bar (free) -> epsilon(-) + epsilon(+) has the threshold at 10(13) eV for a free neutrino of mass 0.058 eV. But a neutrino halo, as attached to a visual ordinary-matter macroscopic object, such as the Earth, the Venus, the Sun, and the stars, which accounts for five times in weight the dark-matter cosmic background neutrinos (CBv's), should have a Fermi-Dirac sphere with the fermi surface energy as high as 200 TeV. This aspect offers the possibility to detect the existence of the Fermi-Dirac sphere of a neutrino halo. We suspect that a couple of PeV neutrinos already detected at IceCube might come from the Fermi-Dirac sphere of the neutrino halo of the Earth.
引用
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页码:7 / 11
页数:5
相关论文
共 5 条
[1]  
Halzen Francis, 2014, CERN COURIER, P30
[2]  
Hwang W-Y. Pauchy, 2015, ARXIV13044705V2
[3]  
Hwang W-Y. Pauchy, 2015, ARXIV12095488V4
[4]  
Hwang W-Y. Pauchy, 2015, NEUTRINOS COSMOS PRO
[5]  
Hwang W-Y. Pauchy, 2016, ARXIV10121082V4