共查询到19条相似文献,搜索用时 46 毫秒
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吴义根 陈国明 陈和生 张守宇 唐孝威 童国梁 M.Bocciolini C.Civinini R.D''alessandro M.Meschini M.Pieri P.Spillantini 王贻芳 H.Hofer P.LeCoultre B.Spiess J.Ulbricht 《中国物理 C》1991,15(10):865-874
本文介绍子配有BGO(锗酸铋)晶体阵列的L3铀强子量能器性能的模拟测试.对L3强子量能器以及测试实验作了简要介绍,并给出了该量能器对4—20GeV能量范围的π介子的能量分辨率、e/π响应比、角分辨、能量分辨率随入射π介子方向的变化以及强子穿透率等实验结果. 相似文献
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We present some physics possibilities with an iron calorimeter detector (ICAL) and a status report on the feasibility study
to construct such a detector at a future possible India-based Neutrino Observatory (INO). This talk was given at the workshop
on high energy physics phenomenology, WHEPP-8, in Jan. 2004, at IIT Bombay. 相似文献
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2015年诺贝尔物理学奖授予了发现中微子振荡也就是中微子有质量的实验。这个发现是至今为止,粒子物理标准模型——这一得到广泛实验验证的理论中唯一指明存在新物理的明显证据。文章将介绍中微子振荡发现以后主要的中微子实验物理目标、采用的探测技术、实验状况及其未来展望。 相似文献
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We present a simple but general treatment of neutrino oscillations in the framework of quantum mechanics, using plane waves and intuitive wave packet principles when necessary. We attempt to clarify some confusing statements that have recently appeared in the literature. 相似文献
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We examine the effects of mixing induced non-diagonal light-heavy neutrino weak neutral currents on the amplitude for the
process
(with a=e, μ or τ). By imposing constraint that the amplitude should not exceed the perturbative unitarity limit at high energy
, we obtain bounds on light-heavy neutrino mixing parameter sin2
where
is the mixing angle. In the case of one heavy neutrino (mass mξ) or mass degenerate heavy neutrinos, for Λ=1 TeV, no bound is obtained for mξ<0.50 TeV. However, sin2
≤3.8 × 10−6 for mξ=5 TeV and sin
≤6.0 × 10−8 for mξ=10 TeV. For Λ=∞, no constraint is obtained for mξ<0.99 TeV and sin2
≤3.8 × 10−2 (for mξ=5 TeV) and sin2
≤9.6 × 10−3 (for mξ=10 TeV). 相似文献
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Atsuto Suzuki 《Proceedings of the Japan Academy. Series B, Physical and biological sciences》2007,83(2):27-38
KamLAND measured the e’s flux from distant nuclear reactors, and found fewer events than expected from standard assumptions about e propagation at the 99.998% confidence level (C.L.). The observed energy spectrum disagrees with the expected spectral shape at 99.6% C.L., and prefers the distortion from neutrino oscillation effects. A two-flavor oscillation analysis of the data from KamLAND and solar neutrino experiments with CPT invariance, yields
eV2 and
. All solutions to the solar neutrino problem except for the large mixing angle (LMA) region are excluded. KamLAND succeeded in detecting geoneutrinos produced by the decays of 238U and 232Th within the Earth. The total observed number of 4.5 to 54.2, assuming a Th/U mass concentration ratio of 3.9 is consistent with 19 predicted by geophysical models. This detection allows better estimation of the abundances and distributions of radioactive elements in the Earth, and of the Earth’s overall heat budget. 相似文献
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利用最新的WMAP观测数据推导出电子、Muon和Tau中微子的运动学有效质量的一般上限:e2+μ2+τ2=m12+m22+m32<0.5eV2,或α<0.71eV(其中α=e,μ,τ)。考虑现有中微子振荡的实验数据,进一步得到e<0.24eV以及μ≈τ<0.24eV. 因此有效质量μ和τ太小而无法被探测. 相似文献
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Takaaki Kajita 《Proceedings of the Japan Academy. Series B, Physical and biological sciences》2010,86(4):303-321
Neutrino oscillation was discovered through studies of neutrinos produced by cosmic-ray interactions in the atmosphere. These neutrinos are called atmospheric neutrinos. They are produced as decay products in hadronic showers resulting from collisions of cosmic rays with nuclei in the atmosphere. Electron-neutrinos and muon-neutrinos are produced mainly by the decay chain of charged pions to muons to electrons. Atmospheric neutrino experiments observed zenith-angle and energy dependent deficit of muon-neutrino events. Neutrino oscillations between muon-neutrinos and tau-neutrinos explain these data well. Neutrino oscillations imply that neutrinos have small but non-zero masses. The small neutrino masses have profound implications to our understanding of elementary particle physics and the Universe. This article discusses the experimental discovery of neutrino oscillations. 相似文献
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Sandip Pakvasa 《Pramana》2004,62(2):347-358
The current status of neutrino anomalies is summarized; the KamLAND experiment is described and the recent results of KamLAND
presented. 相似文献