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The Science reports of the Tohoku University. Seventh series: (Geography). Tohoku Daigaku最新文献

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Study of Deep Inelastic Scattering of Polarized Electrons off Polarized Deuterons 极化氘核对极化电子的深度非弹性散射研究
M. Kuriki
This thesis describes a 29GeV electron - nucleon scattering experiment carried out at Stanford Linear Accelerator Center (SLAC). Highly polarized electrons are scattered off a polarized ND{sub 3} target. Scattered electrons are detected by two spectrometers located in End Station A (ESA) at angles of 4.5{degrees} and 7{degrees} with respect to the beam axis. We have measured the spin structure function g{sub 1} of deuteron over the range of 0.029 < x < 0.8 and 1. 0 < Q{sup 2} < 12.0(GeV/c){sup 2}. This integral indicates a discrepancy of more than three standard deviations from the prediction of the Ellis-Jaffe sum rule, 0.068{+-}0.005 at Q{sup 2} = 3.0(GeV/c){sup 2} while our result of g{sub 1}{sup d} in good agreement with SMC results. Combined with g{sub 1} of the proton, the measurement of {integral}{sub 0}{sup 1}(g{sub 1}{sup d}-g{sub 1}{sup n}) is 0.169{+-}0.008. We also obtained the strong coupling constant at Q{sup 2} = 3.0(GeV/c){sup 2} to be 0.417{sub -0.110}{sup +0.086}, using the power correction for the sum rule up to third order of {alpha}{sub s}. This result is in agreement with the strong coupling constant {alpha}{sub s}(Q{sup 2}) = 3.0(GeV/c{sup 2}) obtained from various experiments. Using our deuteron results and the axial vector couplings of hyperon decays, the total quark polarization along the nucleon spin is found to be 0.286{+-}.055, implying that quarks carry only 30% of the nucleon spin. The strange sea quark polarization is also determined to be -0.101 {+-} .023. These measurements are in agreement with other experiments and provide the world`s most precise measurement of these quark polarizations. 80 refs., 151 figs., 23 tabs.
本文描述了在斯坦福直线加速器中心(SLAC)进行的29GeV电子-核子散射实验。高极化电子从极化ND{sub 3}目标上散射出去。位于终端站A (ESA)的两台光谱仪以相对于束流轴的4.5度和7度角探测散射电子。我们测量了氘核的自旋结构函数g{sub 1}在0.029 < x < 0.8和1的范围内。0 < Q{sup 2} < 12.0(GeV/c){sup 2}。该积分表明与Ellis-Jaffe和规则的预测有三个标准差以上的差异,在Q{sup 2} = 3.0(GeV/c){sup 2}时0.068{+-}0.005,而我们的g{sub 1}{sup d}的结果与SMC的结果很好地一致。结合质子的g{sub 1},{积分}{sub 0}{sup 1}(g{sub 1}{sup d}-g{sub 1}{sup n})的测量值为0.169{+-}0.008。我们还得到了Q{sup 2} = 3.0(GeV/c){sup 2}处的强耦合常数为0.417{sub -0.110}{sup +0.086},使用了对求和规则的功率校正,直到{alpha}{sub s}的三阶。这一结果与各种实验得到的强耦合常数{alpha}{sub s}(Q{sup 2}) = 3.0(GeV/c{sup 2})是一致的。利用我们的氘核结果和超子衰变的轴向矢量耦合,发现沿核子自旋的总夸克极化为0.286{+-}。055,这意味着夸克只携带30%的核子自旋。奇异海夸克极化也被确定为-0.101{+-}.023。这些测量结果与其他实验一致,并提供了世界上最精确的夸克极化测量。参80。, 151个无花果。, 23页。
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引用次数: 1
Quantum Group Symmetries in Models of Elementary Particle Physics(Abstracts of Doctral Dissertations) 基本粒子物理模型中的量子群对称性(学位论文摘要)
U. Carow-Watamura
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引用次数: 2
Fractal Analysis of X-ray Emission from Centaurus X-3 Observed with Ginga(Proceedings of the Workshop on the Hydrodynamic Study of Accretion Disks and Pulsating Stars) 半人马座X-3 x射线辐射的分形分析(吸积盘与脉动星流体动力学研究研讨会论文集)
R. Kanetake
X‐ray time series data from the 4.8‐second binary pulsar Cen X‐3 observed with Ginga are analyzed. We study the fractal dimension of x‐ray intensity of the total 1.7∼37 keV energy band. The fractal dimensions of the temporal behavior on time scales ≥4.8 seconds are comparatively large. It implies that the source varies with small size perturbations compared with the scale of the system. The effect of noise on the fractal dimension is estimated briefly. It is mentioned that there exists a low dimensional motion with the time scale of 500 s.
本文分析了用Ginga观测到的4.8秒双星脉冲星Cen X - 3的X射线时间序列数据。我们研究了1.7 ~ 37 keV总能带x射线强度的分形维数。时间尺度≥4.8秒时,时间行为的分形维数较大。这意味着与系统的尺度相比,源随着小尺度的扰动而变化。简要估计了噪声对分形维数的影响。文中提到存在一个时间尺度为500s的低维运动。
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引用次数: 0
Origin of Far-Infrared Emission in Seyfert and Starburst Galaxies(Abstracts of Doctral Dissertations) 塞弗特星系和星暴星系远红外辐射的起源(论文摘要)
H. Mouri
To study the origin of far-IR emission in starburst nuclei (SBNs) and active galactic nuclei (AGNs), the 25-60 μm spectral index [α(25, 60)] has been compared with the intensity ratios of [O I] λ6300 to Hα ([O I]/Hα) and H 2 υ=1-0 S(1) 2.12 μm to Brγ [S(1)/Brγ] for 48 galaxies (16 SBNs, 27 AGNs, and five LINERs).
为了研究星暴核(SBNs)和活动星系核(AGNs)远红外辐射的来源,对48个星系(16个SBNs, 27个AGNs和5个LINERs)的25-60 μm光谱指数[α(25,60)]与[O I] λ6300 /Hα ([O I]/Hα)和h2 υ=1-0 S(1) 2.12 μm /Brγ [S(1)/Brγ]的强度比进行了比较。
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引用次数: 29
STRUCTURE AND PHYSICS OF COOL GIANT MOLECULAR COMPLEXES(Proceedings of Japan-France Seminar on Chemical Evolution of Galaxies with Active Star Formation) 冷巨分子复合物的结构和物理(日法活跃恒星形成星系化学演化研讨会论文集)
E. Falgarone, M. Pérault
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引用次数: 19
Thermal instability of hydrogen-burning shells in very massive stars. 大质量恒星中氢燃烧壳的热不稳定性。
Yasuo Tanaka, N. Arimoto, M. Takeuti
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引用次数: 2
Post-war seasonal labor migration from the rural areas in Japan. 战后日本农村地区的季节性劳动力迁移。
K K Oshiro
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引用次数: 0
Recent population change in the Japanese metropolis: the flight from the inner city. 日本大都市最近的人口变化:内城人口外流。
D H Kornhauser
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引用次数: 0
Pollen analysis of peat on a sand bar in eastern Hokkaido. 北海道东部沙洲泥炭的花粉分析。
K. Sohma, Kazuo Ishizuka
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引用次数: 2
Formation Process of M3 Milch-Cow-Keeping Region in Northeastern Part of Kitakami Mountainland - Agricultural Geographic Description of Two Milch-Cow-Keeping Regions(2) 北上山地东北部M3奶牛区形成过程——两个奶牛区农业地理描述(2)
Ken-ichi Tanabe
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引用次数: 1
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The Science reports of the Tohoku University. Seventh series: (Geography). Tohoku Daigaku
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