The spectroscopy of solar sterile neutrinos

被引：3
作者：
Lopes, Ildio [1 ,2 ,3 ]
机构：
[1] UL, Ctr Astrofis & Gravitacao CENTRA, IST, Dept Fis, Av Rovisco Pais 1, P-1049001 Lisbon, Portugal
[2] CNRS, Inst Astrophys Paris, UMR 7095, 98 Bis Bd Arago, F-75014 Paris, France
[3] Sorbonne Univ, UPMC, 98 Bis Bd Arago, F-75014 Paris, France
来源：
EUROPEAN PHYSICAL JOURNAL C | 2018年 / 78卷 / 04期
关键词：
OSCILLATIONS;
D O I：
10.1140/epjc/s10052-018-5770-8
中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
摘要：
We predict the sterile neutrino spectrum of some of the key solar nuclear reactions and discuss the possibility of these being observed by the next generation of solar neutrino experiments. By using an up-to-date standard solar model with good agreement with current helioseismology and solar neutrino flux data sets, we found that from solar neutrino fluxes arriving on Earth only 3-4% correspond to the sterile neutrino. The most intense solar sources of sterile neutrinos are the pp and (7) Be nuclear reactions with a total flux of 2.2 x 10(9) and 1.8 x 10(8) cm(2)s(-1), followed by the (13) N and (15) O nuclear reactions with a total flux of 1.9 x 10(7) and 1.7 x 10(7) cm(2) s(-1). Moreover, we compute the sterile neutrino spectra of the nuclear proton-proton nuclear reactions - pp, hep and B-8 and the carbon-nitrogen-oxygen - (13) N, (15) O and (17) F and the spectral lines of (7) Be.
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页数：10
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