The neutrino mass hierarchy at reactor experiments now that θ13 is large

被引：18

作者：

Ciuffoli, Emilio ^{[1
]}

Evslin, Jarah ^{[1
]}

Zhang, Xinmin ^{[1
,2
]}

机构：

[1] Chinese Acad Sci, IHEP, TPCSF, Beijing 100049, Peoples R China

[2] Chinese Acad Sci, IHEP, Div Theoret Phys, Beijing 100049, Peoples R China

来源：

JOURNAL OF HIGH ENERGY PHYSICS | 2013年 / 03期

关键词：

Neutrino Detectors and Telescopes;

D O I：

10.1007/JHEP03(2013)016

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：

Now that theta(13) is known to be large, a medium baseline reactor experiment can observe the fine structure of the electron antineutrino survival probability curve, approximately periodic oscillations in L/E with period 4 pi/vertical bar Delta M-31(2)vertical bar. The periodicity with respect to L/E is broken by 2-3 oscillations which, in the case of the normal (inverted) hierarchy, shift the first 16 oscillations nearly 1% higher (lower) and move the next 16 lower (higher). The energy of each peak determines a particular combination of the mass differences, for example cos(2)(theta(12))vertical bar Delta M-31(2)vertical bar + sin(2)(theta(12))vertical bar Delta M-32(2)vertical bar for all peaks visible at baselines under 40 km. Comparing these combinations with each other or with NO nu A results one can in principle determine the mass hierarchy. Alternately, as the Fourier transforms of the 1-3 and 2-3 oscillation probabilities are out of phase by the 1-2 oscillation probability, near the maximum of the 1-2 oscillation the complex phase of the total survival probability can be used to determine the hierarchy. Two interference effects make this task difficult. First, kilometer distances between the reactors reduce the amplitudes of peaks below about 4MeV. Second, even reactors 100 or more kilometers away significantly obscure the 1-2 oscillation maximum, which also complicates a measurement of the solar mixing angle with a single detector.

引用

页数：31

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