共查询到20条相似文献,搜索用时 12 毫秒
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A magnetized Iron CALorimeter (ICAL) detector at the India-based neutrino observatory (INO) is used to study neutrino oscillation sensitivity using atmospheric muon neutrino source. The ICAL detector will be able to detect muon tracks and hadron showers produced by neutrino interactions with the iron target. We have performed precision measurement analysis for the atmospheric neutrino oscillation parameters with the muon neutrino events, generated by Monte Carlo NUANCE event generator. A marginalized χ2 analysis based on reconstructed neutrino energy and muon zenith angle binning scheme has been performed to determine the sensitivity for the atmospheric neutrino mixing parameters, \(\sin ^{2}\theta _{23}\) and \(| {\Delta } m^{2}_{23}|\). 相似文献
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从光谱位相相干电场重构法(SPIDER)的原理出发,实现了算法、讨论时间延迟、光谱剪切量、滤波窗口宽度、色散量等几个方面的优化选取。当展宽器色散和脉冲宽度一定时,脉冲对的时间延迟存在一个最佳取值范围。相对光谱剪切量在5%~15%间,滤波窗口宽度为/3,重构出的位相误差最小。对干涉图取平均来减小噪声的影响。用SPIDER算法还原了脉冲的电场和位相信息,由SPIDER测量的脉冲宽度为17.7 fs。同时为了比较,用自相关法测量了同一脉冲,由自相关曲线可估算出脉冲宽度为16.8 fs,与SPIDER 的误差比为5.1%,说明了实验的有效性。 相似文献
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康普顿探测器可以获得脉冲X射线照射量随时间变化的波形,探测器特性主要由收集体、介质和金属外壳的材料、尺寸决定。针对神龙一号加速器产生的X射线的能谱结构,应用蒙特卡罗模拟方法,进行探测器结构尺寸设计,获得最佳的有机玻璃介质厚度为30 mm。探测器灵敏度系数随X光能量变化的曲线表明其能量响应较差,分析与计算结果表明在收集体前加低Z金属可有效改善能量响应特性并提高灵敏度系数。计算得到用于测量神龙一号加速器的X射线照射量的康普顿探测器的灵敏度系数为6.86×1011(C/kg)-1。 相似文献
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康普顿探测器可以获得脉冲X射线照射量随时间变化的波形,探测器特性主要由收集体、介质和金属外壳的材料、尺寸决定。针对神龙一号加速器产生的X射线的能谱结构,应用蒙特卡罗模拟方法,进行探测器结构尺寸设计,获得最佳的有机玻璃介质厚度为30 mm。探测器灵敏度系数随X光能量变化的曲线表明其能量响应较差,分析与计算结果表明在收集体前加低Z金属可有效改善能量响应特性并提高灵敏度系数。计算得到用于测量神龙一号加速器的X射线照射量的康普顿探测器的灵敏度系数为6.86×1011 (C/kg)-1。 相似文献
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H. Tanimoto S. Nasu F. E. Fujita I. Sakamoto A. Tanoue 《Hyperfine Interactions》1988,42(1-4):1009-1012
Conversion electron Mössbauer spectroscopy (CEMS) was applied to study the behaviour of119Sn atoms implanted into Ni at the accelerating energy of 100–400KeV and doses of 5×1015–5×1016 ions/cm2 at room temperature. All CEMS spectra were measured at room temperature and successfully analyzed by two components. The energy and dose dependence of CEMS spectra were well explained by the depth distribution of119Sn atoms. 相似文献
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《Nuclear Physics B - Proceedings Supplements》1999,70(1-3)
The upward-going muon flux (Eμ > 1 GeV) has been measured with the underground detector MACRO at LNGS. The total number of measured events is compatible at the 8% c.l. with the expected one. Moreover, the zenith angular distribution of the measured flux does not match the expectation showing a deficit in the vertical direction where the apparatus performance is best known. Assuming an oscillation hypothesis with parameters in the range recently suggested to solve the atmospheric neutrino problem, the agreement increases, but not significantly. The results of an indirect dark matter search for a signal of WIMPs from the core of the Sun and of the Earth are given. Neutrino astronomy with MACRO is giving interesting results regarding possible high energy neutrino emission from pointlike sources and coincidences of neutrino events with γ-ray bursts. 相似文献
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Gobinda Majumder 《Pramana》2004,62(3):587-590
Semileptonic decays ofB →X
u
lv have great importance both from theoretical and experimental point of view, as they are useful for extracting the magnitude
ofV
ub, one of the tiniest elements of CKM matrix. Similarly measurement ofB √ Ds×u can be used to calculateV
ub The Belle Collaboration has measured these branching ratios and extractedV
ub for various theoretical models. 相似文献
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Aaltonen T Álvarez González B Amerio S Amidei D Anastassov A Annovi A Antos J Apollinari G Appel JA Arisawa T Artikov A Asaadi J Ashmanskas W Auerbach B Aurisano A Azfar F Badgett W Bae T Barbaro-Galtieri A Barnes VE Barnett BA Barria P Bartos P Bauce M Bedeschi F Beecher D Behari S Bellettini G Bellinger J Benjamin D Beretvas A Bhatti A Binkley M Bisello D Bizjak I Bland KR Blumenfeld B Bocci A Bodek A Bortoletto D Boudreau J Boveia A Brigliadori L Bromberg C Brucken E Budagov J Budd HS 《Physical review letters》2012,108(15):151803
We have measured the W-boson mass M(W) using data corresponding to 2.2 fb(-1) of integrated luminosity collected in pp collisions at sqrt[s] = 1.96 TeV with the CDF II detector at the Fermilab Tevatron collider. Samples consisting of 470,126 W → eν candidates and 624,708 W → μν candidates yield the measurement M(W) = 80,387 ± 12(stat.) ± 15(syst.) = 80,387 ± 19 MeV/c2. This is the most precise measurement of the W-boson mass to date and significantly exceeds the precision of all previous measurements combined. 相似文献
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G. Marre M. Carras B. Vinter V. Berger 《Physica E: Low-dimensional Systems and Nanostructures》2004,20(3-4):515
A study of the optimization of the detectivity of a mid-infrared double heterostructure photovoltaic detector is proposed. Simple approximate analytic expressions for the dark current are compared with full numerical calculations, and provide a physical insight into the mechanisms dominating the dark current. The analysis is performed step by step, from a simple p–n junction to the full double heterostructure. The influence of temperature, barrier band gap energy in a double heterostructure, doping density in the active region, on diffusion and generation–recombination mechanisms is analyzed. It is finally shown how the performances of a double heterostructure photovoltaic detector can be improved by controlled doping of the active region. 相似文献
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The relation for the sensitivity of the pneumatic detector based on the analysis of the thermal, pneumatic and optical parts of the instrument is derived. From this relation the optimum diameter of the flexible mirror and the optimum gas pressure in the detector cell are calculated.List of symbols used
B
brightness [sb]
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C
thermal capacity of absorbing membrane [cal cm–2 grad–1]
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c
specific heat of gas in cell [cal g–1 grad–1]
-
D
diameter of grid [cm]
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d
diameter of flexible mirror [cm]
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E
illumination [ph]
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F
2
area of light spot [cm2]
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F
3
area of flexible mirror [cm2]
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f,f
1
focal distance [cm]
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f
0
chopping frequency of infra-red radiation [sec–1]
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h
depth of cell [cm]
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k
radiation cooling constant [cal cm–2 sec–1 grad–1]
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k
0
reflectivity of flexible mirror
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k
1,k
2,k
3,k
4
constants
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L
total length of edge of half of grid [cm]
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l
distance between lens and flexible mirror [cm]
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M, N
constants
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m
refractive power of flexible mirror [cm–1]
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n
number of grammolecules of gas in cell
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P
radiative power [cal sec–1]
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p,p
0,p
pressure, atmospheric pressure, change in pressure [dyne cm–2]
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R
gas constant [erg grad–1]
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r
coordinate
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r
0
radius of flexible mirror [cm]
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r
1,r
2
radii of beam of rays [cm]
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t
tension of flexible mirror [dyne cm–1]
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, T, T
f
absolute temperature and its change [grad]
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V, V
volume and increase in volume [cm3]
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v
coordinate
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v
0
maximum height of deflection of flexible mirror [cm]
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x, x
distance of object and image from focal planes [cm]
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,
angles
-
specific weight of gas at pressure of 1 atm. [g cm–3]
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absorption coefficient of infra-red radiation
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thermal conductivity of gas [cal cm–1 sec–1 grad–1]
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v
number of lines of grid per 1 cm [cm–1]
-
radius of light spot on grid [cm]
- T
time constant [sec]
-
0,
1,
2,
3
light flux and its change [lm] 相似文献
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We investigate the advantages of using two independent, linear detectors for continuous quantum measurement. For single-shot measurement, the detection process may be quantum limited if the detectors are twins. For weak continuous measurement, cross correlations allow a violation of the Korotkov-Averin bound for the detector's signal-to-noise ratio. The joint weak measurement of noncommuting observables is also investigated, and we find the cross correlation changes sign as a function of frequency, reflecting a crossover from incoherent relaxation to coherent, out of phase oscillations. Our results are applied to a double quantum-dot charge qubit, simultaneously measured by two quantum point contacts. 相似文献
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This paper discusses the influence of the finite pulse-time effect simultaneously acting with the effect of heat source capacity, the effect of thermometer heat capacity and the effect of inertia of measuring apparatus on the accuracy of a pulse method. Further on, the relations for the maximal and effective temperature of a sample are derived. The above effects are examined separately, which allows setting some useful criterions for neglecting these effects. The results of numerical calculations are presented also graphically. 相似文献
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