On the Photon Mass

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著名的人英语作文三年级

著名的人英语作文三年级

Title: The World's Greatest Scientist - AlbertEinsteinAlbert Einstein, a renowned German-born theoretical physicist, is widely recognized as one of the most influential and celebrated scientists of all time. Born in 1879 in Ulm, Germany, Einstein's journey to fame and recognition began at a young age, when he developed a deep interest in mathematics and physics. His groundbreaking theories and equations have revolutionized the field of physics and continue to influence scientific research worldwide.One of Einstein's most famous contributions to science is his Theory of Relativity, which was introduced in his paper "On the Electrodynamics of Moving Bodies" in 1905. This theory proposed that space and time are not absolute, but are relative to the observer's frame of reference. It also introduced the famous equation E=mc², which states that energy and mass are equivalent and can be converted into each other. This theory has had profound implications in various fields, including atomic energy and cosmology.Apart from his Theory of Relativity, Einstein also made significant contributions to the field of quantum mechanics. His work on the photoelectric effect led to the development of the photon theory, which explained the behavior of light as particles. This theory won him the Nobel Prize inPhysics in 1921.Einstein's legacy is not just in his scientific contributions, but also in his impact on society and culture. His ideas about relativity and the nature of the universe have influenced philosophers, artists, and writers alike. His quotes and sayings, such as "Imagination is more important than knowledge" and "The most beautiful thing we can experience is the mysterious. It is the source of all true art and science," have inspired generations to pursue knowledge and explore the unknown.In conclusion, Albert Einstein's life and work are a testament to the power of the human mind and the impact one individual can have on the world. His theories andequations have revolutionized physics and continue to influence scientific research, while his impact on societyand culture is immeasurable. Einstein's legacy will forever be remembered and celebrated.**中文翻译****标题:世界最伟大的科学家——阿尔伯特·爱因斯坦** 阿尔伯特·爱因斯坦,这位著名的德国裔理论物理学家,被广泛认为是历史上最有影响力和最受推崇的科学家之一。

光电子学与光子学讲义-Chapter0-perface讲课教案

光电子学与光子学讲义-Chapter0-perface讲课教案
1980s: 量子阱半导体材料(QW激光器) 光电器件更新换代
1990s: 稀土掺杂光纤(掺铒光纤放大器) 光通信技术的革命
期待新一代光电功能材料的突破 !!!
五.光电子学发展方向与趋势
➢ 量子化(材料的量子结构化)---
采用量子阱、应变量子阱、超晶格、 量子线、量子点等人构改性的材料
➢ 集成化(器件的集成化) ---
一. 光电子学的发展进程
1973年 法国 召开了光子学国际会议 The term “LA PHOTONIQUE” was coined by a French physicist to describe the use of photons in ways analogous to the use of electrons.
❖电

-e
0
❖自

l(h)/2
l(h)
三. 光子学与电子学
光子具有的优异特性: • 光子具有极高的信息容量和效率
• 光子具有极快的响应能力 • 光子系统具有极强的互连能力与并行能力 • 光子具有极大的存储能力
四.光电子学、光子学相关学术领域
• 光电子学物理基础研究
• 激光物理学 • 信息光电子学 • 生物光子学及激光医学 • 微光机电集成系统(MEMS) • 光电子武器 • 微波光子学 • 有机光子学与材料 • 光化学与分子动力学 • 能源 ……
支撑技术:
晶体外延生长工艺 --- MBE, MOCVD, CBE
细微加工工艺 --- 电子束光刻, 反应离子刻蚀(RIE)
聚焦离子束注入与刻蚀,
纳米级图形超微细加工 等
五.光电子学发展方向与趋势
集成化是器件发展水平的标志
集成光发射器:LD+EA Mod.,LD +Driver (HBT)

物理专业英语词汇

物理专业英语词汇

物理专业英语词汇摘要:物理学是一门研究自然界最基本的规律和现象的科学,它涉及到许多专业的英语词汇。

本文根据物理学的不同分支,整理了一些常用的物理专业英语词汇,并用表格的形式展示了它们的中英文对照。

本文旨在帮助物理专业的学习者和爱好者掌握一些基本的物理术语,以便于阅读和交流。

1. 基础物理词汇基础物理词汇是指一些在物理学中普遍使用的概念和量,它们是物理学的基本语言。

以下是一些基础物理词汇的中英文对照表:中文英文物理physics物质matter能量energy力force重力gravity摩擦力friction拉力traction质量mass惯性inertia加速度acceleration力矩torque静止at rest相对relative动能kinetic energy势能potential energy功work动量momentum角动量angular momentum能量守恒energy conservation保守力conserved force振动vibration振幅amplitude波wave驻波standing wave震荡oscillation相干波coherent wave干涉interference衍射diffraction轨道orbit速度velocity速率speed大小magnitude方向direction水平horizontal竖直vertical相互垂直perpendicular坐标coordinate直角坐标系Cartesian coordinate system极坐标系polar coordinate system2. 电学和磁学词汇电学和磁学是研究电荷、电流、电场、磁场等现象和规律的物理学分支,它们与光学、热学、原子物理等有着密切的联系。

以下是一些电学和磁学词汇的中英文对照表:中文英文电子electron电荷charge电流current电场electric field电通量electric flux电势electric potential导体conductor电介质dielectric绝缘体insulator电阻resistor电阻率resistivity电容capacitor3. 物理专业英语词汇物理专业英语词汇是指在物理学的学习和研究中经常使用的一些专业术语,它们涵盖了物理学的各个分支和领域,如力学、电磁学、光学、热学、量子力学等。

物理中英文词汇

物理中英文词汇

物理中英文词汇力 force牛顿(力的单位) Newton重力 gravity重心 center of gravity弹力 elastic force摩擦力 friction force滑动摩擦 sliding friction静摩擦因数 static friction factor动摩擦因数 dynamic friction factor力的合成 composition of forces力的分解 resolution of forces机械运动 mechanical motion参考系 reference frame质点 mass point直线运动 rectilinear motion位移 displacement速度 velocity速率 speed平均速度 average velocity平均速率 average speed瞬时速度 instantaneous velocity加速度 acceleration自由落体 freely falling body重力加速度 acceleration due to gravity 运动学 kinematics动丸学 dynamics牛顿第一定律 Newton first law惯性 inertia牛顿第二定律 Newton second law牛顿第三定律 Newton third law超重 overweight失重 weightlessness惯性系 inertial system非惯性系 non-inertial system惯性力 inertial force平衡状态 equilibrium state力矩 moment of force曲线运动 curvilinear motion圆周运动 circular motion周期 period频率 frequency 向心力 centripetal force向心加速度 centripetal acceleration万有引力 universal gravitation万有引力定律 law of universal gravitation 引力常量 gravitational constant第一宇宙速度 first cosmic velocity第二宇宙速度 second cosmic velocity第三宇宙速度 third cosmic velocity功 work焦耳(功的单位) joule功率 power瓦特(功率的单位) watt能 energy动能 kinetic energy动能定理 theorem of kinetic energy势能 potential energy重力势能 gravitational potential energy 弹性势能 elastic potential energy机械能 mechanical energy机械能守恒定律 law of conservation of mechanical energy冲量 impulse动量 momentum动量定理 theorem of momentum动量守恒定律 law of conservation of momentum反冲 recoil振动 vibration简谐运动 simple harmonic motion振幅 amplitude赫兹(频率的单位) hertz单摆 simple pendulum阻尼振动 damped vibration受迫振动 forced vibration驱动力 driving force共振 resonance波 wave介质 medium横波 transverse wave纵波 longitudinal wave波长 wavelength波的反射 reflection of wave波的折射 refraction of wave波的衍射 diffraction of wave波的干涉 interference of waves驻波 standing wave多普勒效应 Doppler effect超声波 supersonic wave次声波 infrasonic wave声呐 sonar阿伏加德罗常数 Avogadro constant 布朗运动 Brown motion热运动 thermal motion热力学能 thermodynamic energy内能 internal energy热力学第一定律 first law of thermodynamics能量守恒定律 law of conservation of energy热力学第二定律 Second law of thermodynamics各向同性 isotropy各向异性 anisotropy单晶体 single crystal多晶体 poly-crystal表面张力 surface tension毛细现象 capillarity液晶 liquid crystal温度 temperature体积 vo1ume压强 pressure帕斯卡(压强的单位) Pascal玻意耳定律 Boyle law查理定律 Charles law摩尔气体常量 mo1ar gas constant 克拉珀龙方程 Clapeyron equation 等温过程 isothermal process等温线 isotherm等容过程 isochoric process等容线 isochore等压过程 isobaric process等压线 isobar湿度 humidity混沌 chaos分形 fractal 电荷 electric charge电荷量 quantity of electricity正电荷 positive charge负电荷 negative charge库仑定律 Coulomb law静电感应 electrostatic induction感应电荷 induced charge元电荷 elementary charge电荷守恒定律 law of conservation of charge库仑(电荷的单位) coulomb电场 electric field电场力 electric field force电场强度 electric field strength电场线 electric field line导体 conductor静电平衡 electrostatic equilibrium静电屏蔽 electrostatic screening电势 electric potential电势差/电压 electric potential difference 伏特(电压的单位) volt电势能 electric potential energy等势面 equi-potential surface电容 capacitance电容器 capacitor充电 charging放电 discharging法拉(电容的单位) farad电流 electric current安培(电流的单位) ampere直流 direct current恒定电流 steady current电阻 resistance欧姆(电阻的单位) ohm电阻率 resistivity半导体 semiconductor超导体 superconductor电功率 electric power电动势 electromotive force -(e.m.f.) 磁性 magnetism磁场 magnetic field磁感线 magnetic induction line安培定则 Ampere rule安培力 Ampere force磁感应强度 magnetic induction左手定则 left-hand rule洛伦兹力 Lorentz force加速器 accelerator磁通量 magnetic flux电磁感应 electromagnetic induction感应电流 induction current感应电动势 induction electromotive force 电磁感应定律 law of electromagnetic induction楞次定律 Lenz law右手定则 right-hand rule自感 self-induction交流 alternating current瞬时值 instantaneous value峰值 peak value有效值 effective value电感 inductance变压器 transformer电能 electric energy电磁振荡 electromagnetic oscillation电磁场 electromagnetic field电磁波 electromagnetic wave雷达 radar射弹 抛射物 Projectile抛射体运动 Projectile motion射程 Range速度的水平(垂直)分力 Horizontal (Vertical) components of velocity电场 Superposition of Electric Fields线圈 Coil相干波源 Coherent wave source光斑 Speckle光栅衍射 Diffraction gratings光子 Photon电子 Electron光电效应 The photoelectric effect电离能 Ionization energy线放射(吸收)光谱 Line emission (absorption) spectrum荧光 Fluorescence质量筐 Mass defect结合能 Binding energy衰变 Decay 抛物线轨迹 Parabolic path量, 大小 Magnitude毕达哥拉斯 (580? -500?BC, 古希腊哲学家, 数学家) ,勾股定理 Pythagoras维度 Dimension电学 Electricity磁学 Magnetism光 Light物质,介质 Matter原子 Atom原子核 Nuclei公式 Formula常量 Constant互相垂直的矢量 Mutually perpendicular vectors标量 Scalar回旋加速器 Cyclotron裂变 Fission聚变 Fusion电烙铁 Electric soldering iron安培计 Ampere meter伏特计 Voltmeter电压 Voltage电源 Power pack电池 Battery指南针 Compass硬橡胶 Ebonite螺线管 Solenoid传音学 Acoustics导电体 Conductor绝缘体 Insulator合力 Net force法向力 Normal force铁屑 Iron filings验电器 Electroscope量角器 Protractor对地同步 (静止) 的 Geostationary半径 Radius光谱仪 Spectrometer (spectrograph, spectroscopic instrument)分光镜 Spectroscope等速圆周运动 Uniform circular motion 偏振(极化) Polarization。

太阳能英语专业术语

太阳能英语专业术语

太阳能专业词汇名词解释字母AAA, Ampere的缩写, 安培a-Si:H, amorph silicon的缩写, 含氢的, 非结晶性硅.Absorption, 吸收.Absorption of the photons:光吸收;当能量大于到禁带宽度的光子入射时,太阳电池内的电子能量从价带迁导带,产生电子——空穴对的作用,称为光吸收。

Absorptions coefficien t, 吸收系数, 吸收强度.AC, 交流电.Ah, 安培小时.Acceptor, 接收者, 在半导体中可以接收一个电子.Alternating current, 交流电,简称“交流. 一般指大小和方向随时间作周期性变化的电压或电流. 它的最基本的形式是正弦电流. 我国交流电供电的标准频率规定为50赫兹。

交流电随时间变化的形式可以是多种多样的。

不同变化形式的交流电其应用范围和产生的效果也是不同的。

以正弦交流电应用最为广泛,且其他非正弦交流电一般都可以经过数学处理后,化成为正弦交流电的迭加。

AM, air mass的缩写, 空气质量.直射阳光光束透过大气层所通过的路程,以直射太阳光束从天顶到达海平面所通过的路程的倍数来表示。

当大气压力P=1.013巴,天空无云时,海平面处的大气质量为1。

amorphous silicon solar cell:非晶硅太阳电池(a—si太阳电池)用非晶硅材料及其合金制造的太阳电池称为非晶硅太阳电池,亦称无定形硅太阳电池,简称a—si太阳电池。

Angle of inclination, 倾斜角,即电池板和水平方向的夹角,0-90度之间。

Anode, 阳极, 正极.太阳能专业词汇名词解释字母BBack Surface Field, 缩写BSF, 在晶体太阳能电池板背部附加的电子层, 来提高电流值.Bandbreak, 在半导体中, 价带和导带之间的空隙,对于半导体的吸收特性有重要意义.Becquerel, Alexandre-Edmond, 法国物理学家, 在1839年发现了电池板效应.BSF, back surface field的缩写.Bypass-Diode, 与太阳能电池并联的二极管, 当一个太阳能电池被挡住, 其他太阳能电池产生的电流可以从它处通过.太阳能专业词汇名词解释字母CCadmium-Tellurid, 缩写CdTe; 位于II/VI位的半导体, 带空隙值为1,45eV, 有很好的吸收性, 应用于超薄太阳能电池板, 或者是连接半导体.Cathode, 阴极,或负极,是在电池板电解液里的带负电的电极,是电池板电解液里带电粒子和导线里导电电子的过渡点。

电荷的本质

电荷的本质

人类很早就观察到“摩擦起电”现象,并认识到电只 有正负二种,同种相斥,异种相吸。带正或负电的粒子称 为电荷。粒子所带电的量的多少称为电荷量。1785年,库 仑(C.A.Coulomb,1736~1806)以扭秤实验得出静电作用的 库仑定律[1],人类对电磁现象进入了定量研究时代。英国物 理学家卡文迪什(H.Cavandish,1731~ 1810)早在1774 年就发现了这一定律,而且结果更为精确[2],可惜没有被认 可。人们对库仑定律的精度进行了深入的研究[3-8],但是, 电荷究竟是什么?为什么电荷有两种?为什么同种电荷相 斥、异种电荷相吸?为什么符合库仑定律?这些问题都是 人们想解决,而实际探讨人却很少,至今还没有解决的问 题。
在Q1物体的右侧,要交换掉M1份正电量并且保持物体质 量不变,就要吸收 个带负电的微粒子和 中性的微粒 子,并放出 个带正电的微粒子,满足:
——(式2)
作用在带正电荷量为Q1的物体右侧的动量为 。
带正电荷量为Q1的物体受到的向右的力为:
——(式3)
由于右侧有负电荷Q2提供带负电的微粒子,而左侧没
有,因而,
放在空间内的一个负电荷,因其电质子呈缺乏状态, 要从外界吸收电质子,吸收的方式为向空间释放电质子缺 乏的微粒子,吸收电质子过剩的微粒子或中性微粒子,以 达到质量基本平衡。由于向空间发射和从空间吸收呈球对 称状态,合力也为零。
图1 异种电荷使两物体相互靠近 2.2 一个正电荷与一个负电荷
如 图 1 所 示 两 个 物 体 , 电 荷 量 分 别 为 Q1和 Q2, Q1为 正 电,Q 为负电,两中心点之间的距离为r,将它们放在各种
本文首先探讨电荷的本质,然后探讨电荷间相互作用 原理与库仑定律。 1 电现象与电荷
人类很早就观察到摩擦起电和雷电等现象,并认识到 电只有正负二种,同种相斥,异种相吸。带正或负电的基 本粒子称为电荷。

爱因斯坦做出的贡献的英文作文

爱因斯坦做出的贡献的英文作文

爱因斯坦做出的贡献的英文作文阿尔伯特·爱因斯坦,这位二十世纪最伟大的理论物理学家之一,以其深邃的洞察力、无与伦比的创造力和对宇宙奥秘的不懈探索,为人类科学知识体系做出了诸多里程碑式的贡献。

他不仅彻底颠覆了人们对时空、物质和能量的传统认知,更奠定了现代物理学的两大基石——相对论和量子力学。

(English):Albert Einstein, one of the greatest theoretical physicists of the 20th century, made numerous landmark contributions to humanity's scientific knowledge system with his profound insights, unparalleled creativity, and relentless exploration of cosmic mysteries. He not only fundamentally upended traditional notions of space, time, matter, and energy but also laid the twin cornerstones of modern physics: relativity and quantum mechanics.Paragraph 2 (中文):爱因斯坦首先在1905年提出了狭义相对论,这是对牛顿力学框架的一次革命性突破。

他揭示了时间和空间并非绝对不变,而是相互关联、随观察者运动状态而变化的统一四维时空。

著名的质能方程E=mc²,便是这一理论的核心成果,它表明能量(E)与质量(m)之间存在着直接等价关系,且能量的转换蕴含着巨大的潜能。

这一发现不仅为核能的开发提供了理论基础,也深刻影响了我们对宇宙起源、星体演化等宏观现象的理解。

物理单词中英对照

物理单词中英对照

物理单词中英对照1. 力(Force)在物理学中,力是使物体产生加速度的原因。

2. 质量(Mass)质量是物体所含物质的量,是衡量物体惯性大小的物理量。

3. 速度(Velocity)速度是描述物体位置变化快慢和方向的物理量。

4. 加速度(Acceleration)加速度是描述速度变化快慢的物理量。

5. 动能(Kinetic Energy)动能是物体由于运动而具有的能量。

6. 势能(Potential Energy)势能是物体由于位置关系而具有的能量。

7. 功(Work)功是力在物体上产生位移的过程,是能量转化的量度。

8. 功率(Power)功率是单位时间内做功的多少,表示能量转化速率。

9. 温度(Temperature)温度是衡量物体冷热程度的物理量。

10. 压强(Pressure)压强是单位面积上受到的力的大小。

11. 密度(Density)密度是单位体积内物质的质量。

12. 摩擦力(Friction)摩擦力是两个接触物体在相对运动时产生的阻力。

13. 重力(Gravity)重力是地球对物体产生的吸引力。

14. 电荷(Electric Charge)电荷是物质的一种基本属性,表现为物体间的电磁相互作用。

15. 电流(Electric Current)电流是电荷在单位时间内通过导体截面的量。

16. 电压(Electric Voltage)电压是推动电荷流动的电势差。

17. 电阻(Electric Resistance)电阻是导体对电流阻碍作用的物理量。

18. 磁场(Magnetic Field)磁场是描述磁力作用范围的物理量。

19. 振动(Vibration)振动是物体围绕平衡位置做周期性运动的现象。

20. 波(Wave)波是振动在介质中传播的过程。

物理单词中英对照(续)21. 频率(Frequency)频率是指单位时间内完成振动的次数,是描述波动特性的基本参数。

22. 波长(Wavelength)波长是波在一个周期内传播的距离,它与频率共同决定了波的速度。

Contents

Contents

doi:10.1016/S0304-4238(05)00179-2Scientia Horticulturae 105 (2005) 533–536VOL. 105, ISSUE 130 MAY 2005Regular papersSensitivity of root system to low temperature appears to be associated with the root hydraulic properties through aquaporin activityS.H. Lee and G.C. Chung (Gwangju, South Korea). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1Growth and productivity of potato as influenced by cultivar and reproductive growth. I. Stomatal conductance, rate of transpiration, net photosynthesis, and dry matter production and allocationT. Tekalign and P.S. Hammes (Pretoria, South Africa). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 13Growth and productivity of potato as influenced by cultivar and reproductive growth. II. Growth analysis, tuber yield and qualityT. Tekalign and P.S. Hammes (Pretoria, South Africa). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 29Identification of Olea europaea L. cultivars using inter-simple sequence repeat markersP.J. Terzopoulos (Athens, Greece), B. Kolano (Katowice, Poland), P.J. Bebeli, P.J. Kaltsikes (Athens, Greece) and I. Metzidakis (Chania, Greece). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 45Segregation patterns of several morphological characters and RAPD markers in interspecific hybrids between Dianthus giganteus and D. carthusianorumS.Y . Lee, B.W. Yae (Suwon, South Korea) and K.S. Kim (Seoul, South Korea). . . . . . . . . . . . . . . . 53Calcium translocation to fleshy fruit: its mechanism and endogenous controlM.C. Saure (Moisburg, Germany). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 65Phenotypic variation in native walnut populations of Northern AlbaniaG. Zeneli, H. Kola and M. Dida (Tirana, Albania). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 91Physiological acclimation of seashore paspalum and bermudagrass to low lightY . Jiang, R.N. Carrow (Griffin, GA, USA) and R.R. Duncan (San Antonio, TX, USA). . . . . . . . . . 101Somatic embryogenesis from floral tissues of feijoa (Feijoa sellowiana Berg)S. Stefanello (Toledo, Brazil), L.L.D. Vesco (Programa, Brazil), J.P.H.J. Ducroquet (Brazil),R.O. Nodari and M.P. Guerra (Florianópolis, Brazil). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 117Temperature effects on corm dormancy and growth of Zephyra elegans D.DonP. Yañez, H. Ohno and K. Ohkawa (Shizuoka City, Japan). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 127Short communicationsImproved technique for counting chromosomes in almondP. Martínez-Gómez, R. Sánchez-Pérez (Espinardo (Murcia), Spain), Y . Vaknin (Davis, CA, USA),F.Dicenta (Espinardo (Murcia), Spain) and T.M. Gradziel (Davis, CA, USA). . . . . . . . . . . . . . . . . 139Contents of Scientia HorticulturaeVolume 105 (2005)Growth responses and endogenous IAA and iPAs changes of litchi (Litchi chinensis Sonn.) seedlings induced by arbuscular mycorrhizal fungal inoculationQ. Yao, H.H. Zhu and J.Z. Chen (Guangzhou, China). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 145 Guide for Authors. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 153 VOL. 105, ISSUE 210 JUNE 2005 Regular papersEvaluation and modelling of greenhouse cucumber-crop transpiration under high and low radiation conditionsE. Medrano, P. Lorenzo, M.C. Sánchez-Guerrero (Almería, Spain) and J.I. Montero(Cabrils, Spain). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 163 Growth, yield, fruit quality and nutrient uptake of hydroponically cultivated zucchini squash as affected by irrigation systems and growing seasonsY. Rouphael and G. Colla (Viterbo, Italy). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 177Net CO2exchange rate of in vitro plum cultures during growth evolution at different photosynthetic pho-ton flux densityS. Morini and M. Melai (Pisa, Italy). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 197 Leaf phenolic content of pear cultivars resistant or susceptible to fire blightY. Gunen, A. Misirli and R. Gulcan (Izmir, Turkey). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 213 Influences of cold deprivation during dormancy on carbohydrate contents of vegetative and floral primordia and nearby structures of peach buds (Prunus persica L. Batch)M. Bonhomme, R. Rageau, A. Lacointe (Clermont-Ferrand, France) and M. Gendraud(Aubière, France). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 223 Inheritance and expression of fruit texture melting, non-melting and stony hard in peach T. Haji, H. Yaegaki and M. Yamaguchi (Ibaraki, Japan). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 241 Organic acid analysis and plant water status of two Aechmea cultivars grown under greenhouse condi-tions: implications on leaf qualityE. Londers, J. Ceusters, I. Vervaeke (Heverlee, Belgium), R. Deroose (Evergem, Belgium) and M.P.De Proft (Heverlee, Belgium). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 249 DNA ploidy level of colchicine-treated hops (Humulus lupulus L.)A. Koutoulis, A.T. Roy, A. Price, L. Sherriff and G. Leggett (Tasmania, Australia). . . . . . . . . . . . . 263 Nutrient solution effects on the development and yield of Anthurium andreanum Lind. in tropical soilless conditionsL. Dufour (Petit-Bourg, France) and V. Guérin (Beaucouzé, France). . . . . . . . . . . . . . . . . . . . . . . . 269 Short communicationIdentification of persimmon (Diospyros kaki) cultivars and phenetic relationships between Diospyros species by more effective RAPD analysisM. Yamagishi, S. Matsumoto, A. Nakatsuka and H. Itamura (Shimane, Japan). . . . . . . . . . . . . . . . 283 VOL. 105, ISSUE 3 4 JULY 2005 Regular papersEffects of fruit shape and plant density on seed yield and quality of squashH. Nerson (Ramat Yishay, Israel). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 293 Yield of scarlet eggplant (Solanum aethiopicum L.) as influenced by planting date of companion cowpea K. Ofori (Legon, Ghana) and D.K. Gamedoagbao (Bunso, Ghana). . . . . . . . . . . . . . . . . . . . . . . . . 305 Effective pollination period estimation in olive (Olea europaea L.): a pollen monitoring applicationF. Orlandi, B. Romano and M. Fornaciari (Perugia, Italy). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 313 Decreased anthocyanin biosynthesis in grape berries grown under elevated night temperature condition K. Mori, S. Sugaya and H. Gemma (Ibaraki, Japan). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 319 534Contents of Volume 105Contents of Volume 105535 Promotion of seed germination and subsequent seedling growth of loquat (Eriobotrya japonica, Lindl)by moist-chilling and GA3applicationsE.-R.F.A. El-Dengawy (El-Mansoura, Egypt). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 331 Arsenic as a factor affecting virus infection in tomato plants: changes in plant growth, peroxidase activ-ity and chloroplast pigmentsE. Miteva, D. Hristova (Kostinbrod, Bulgaria), V. Nenova (Sofia, Bulgaria) and S. Maneva(Kostinbrod, Bulgaria). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 343 Agrobacterium-mediated transformation of Musa acuminata cv. “Grand Nain” scalps by vacuum infiltrationP.O.M. Acereto-Escoffié, B.H. Chi-Manzanero, S. Echeverría-Echeverría, R. Grijalva, A.J. Kay,T. González-Estrada, E. Castaño and L.C. Rodríguez-Zapata (Yucatán, México). . . . . . . . . . . . . . . 359 Modeling the mass of apples by geometrical attributesA. Tabatabaeefar and A. Rajabipour (Karaj, Iran). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 373 Effects of cold storage on postharvest leaf and flower quality of potted Oriental-, Asiatic- and LA-hybrid lily cultivarsA.P. Ranwala and W.B. Miller (Ithaca, NY, USA). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 383 Enhanced thermotolerance of the vegetative part of MT-sHSP transgenic tomato lineP.C. Nautiyal (Junagadh, India), M. Shono and Y. Egawa (Okinawa, Japan). . . . . . . . . . . . . . . . . . 393 Short communicationInduction of somatic embryogenesis in lotus (Nelumbo nucifera Geartn.)S. Arunyanart (Bangkok, Thailand) and M. Chaitrayagun (Phuket, Thailand). . . . . . . . . . . . . . . . . 411 VOL. 105, ISSUE 429 JULY 2005 Regular papersAerial tubers induced in turnip (Brassica rapa L. var. rapa(L.) Hartm.) by gibberellin treatment T. Nishijima, H. Sugii, N. Fukino and T. Mochizuki (Kusawa, Japan). . . . . . . . . . . . . . . . . . . . . . . 423 Changes during the ripening of the very late season Spanish peach cultivar Calanda. Feasibility of using CIELAB coordinates as maturity indicesA. Ferrer, S. Remón, A.I. Negueruela and R. Oria (Zaragoza, Spain). . . . . . . . . . . . . . . . . . . . . . . . 435 Involvement of cell proliferation and cell enlargement in increasing the fruit size of Malus species T. Harada, W. Kurahashi (Hirosaki, Japan), M. Yanai (Rokkasho, Japan), Y. Wakasa(Tsukuba, Japan) and T. Satoh (Kuroishi, Japan). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 447 Yield, fruit quality, and tree health of ‘Allen Eureka’ lemon on seven rootstocks in Saudi ArabiaA. Al-Jaleel (Najran, Saudi Arabia), M. Zekri (LaBelle, FL, USA) and Y. Hammam(Najran, Saudi Arabia). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 457 Effect of temperature on seed and fruit development in three mango (Mangifera indica L.) cultivars N. Sukhvibul (Chiang Rai, Thailand), A.W. Whiley and M.K. Smith (Nambour, Australia). . . . . . . 467 Factors affecting tissue culture of Damask rose (Rosa damascena Mill.)Z. Jabbarzadeh and M. Khosh-Khui (Fars, Iran). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 475 Alterations in endogenous polyamines in bulbs of tuberose (Polianthes tuberosa L.) during dormancy S. Sood and P.K. Nagar (Himachal Pradesh, India). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 483 Phenological growth stages of the cherimoya tree (Annona cherimola Mill.)R. Cautín (Quillota, Chile) and M. Agustí (Valencia, Spain). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 491 The influence of exogenous ethylene on growth and photosynthesis of mustard (Brassica juncea) following defoliationN.A. Khan (Aligarh, India). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 499 Short communicationsIsolation and characterization of a new d-limonene synthase gene with a different expression pattern in Citrus unshiu MarcT. Shimada, T. Endo, H. Fujii and M. Omura (Shizuoka, Japan). . . . . . . . . . . . . . . . . . . . . . . . . . . 507536Contents of Volume 105Metabolic stability of plants regenerated from cryopreserved shoot tips of Dioscorea deltoidea– an endangered medicinal plantS. Dixit-Sharma (Bangalore, India), S. Ahuja-Ghosh (Charlottesville, V A, USA), B. Bushan Mandaland P.S. Srivastava (New Delhi, India). . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 513 Author Index Scientia Horticulturae Volume 105. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 519 Subject Index Scientia Horticulturae Volume 105. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 523 Contents of Scientia Horticulturae Volume 105. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 533。

核专业英语翻译

核专业英语翻译

核专业英语段落翻译南华大学,核科学技术学院,崔爽OUR MA TERIAL world is composed of many substances distinguished by their chemical, mechanical, and electrical properties. They are found in nature in various physical states—the familiar solid, liquid, and gas, along with the ionic “plasma.” However, the apparent diversity of kinds and forms of material is reduced by the knowledge that there are only a little more than 100 distinct chemical elements and that the chemical and physical features of substances depend merely on the strength of force bonds between atoms.We recall that this energy may be released by heating of solids, as in the wire of a light bulb; by electrical oscillations, as in radio or television transmitters; or by atomic interactions, as in the sun. The radiation can be viewed in either of two ways—as a wave or as a particle—depending on the process under study. In the wave view it is a combination of electric and magnetic vibrations moving through space. In the particle view it is a compact moving uncharged object, the photon, which is a bundle of pure energy, having mass only by virtue of its motion.A COMPLETE understanding of the microscopic structure of matter and the exact nature of the forces acting is yet to be realized. However, excellent models have been developed to predict behavior to an adequate degree of accuracy for most practical purposes. These models are descriptive or mathematical, often based on analogy with large-scale processes, on experimental data, or on advanced theory.The emission and absorption of light from incandescent hydrogen gas was first explained by Bohr with a novel model of the hydrogen atom. He assumed that the atom consists of a single electron moving at constant speed in a circular orbit about a nucleus—the proton成。

光合作用Photosynthesis

光合作用Photosynthesis

(12)
ribulose biphosphate (RuBP) 核酮糖二磷酸 [΄raibuləus bi΄fosfeit] A compound with a backbone of five carbon atoms that is required for carbon fixation in the Calvin-Benson cycle of photosynthesis.
2. However, this question is more
than just a theoretical one, since it has become necessary in recent years to construct some legal definitions of what life is and especially when it begins and ends.
From the point of view of chemistry and ener’getics力能学,动能学 , it is the opposite of cellular respiration. Whereas cellular respiration is highly exergonic放能的 and releases energy, photosynthesis requires energy and is highly endergonic吸收 能量的.
(10)
photosynthesis 光合作用 [,fəutəu´sinθsis] The synthesis of organic compounds by reduction of carbon dioxide using light energy absorbed by chlorophyll.

小学上册B卷英语上册试卷

小学上册B卷英语上册试卷

小学上册英语上册试卷英语试题一、综合题(本题有100小题,每小题1分,共100分.每小题不选、错误,均不给分)1.My grandma taught me how to knit. Now I can make ________ (围巾) for my dolls.2.The __________ (水体) is essential for life.3.What do we call a collection of stars?A. GalaxyB. UniverseC. PlanetD. Solar System4.The __________ was a major event in the history of the United States. (民权运动)5. A _____ (植物品种) can become endangered.6. A _______ (小斑马) has unique stripes.7.My friend is very _______ (形容词) when it comes to art. 她的作品都很 _______ (形容词).8.What is the opposite of empty?A. FullB. LightC. HeavyD. DarkA9.What is the name of the region in the center of a black hole?A. SingularityB. Event HorizonC. Accretion DiskD. Photon Sphere10. A solid has a definite _______ and volume.11.My teacher is very __________ (鼓励).12.What do we call a group of stars forming a pattern?A. GalaxyB. ConstellationC. ClusterD. NebulaB13.I want to _______ (去旅行)到不同的地方。

物理专业英语翻译

物理专业英语翻译

第一章Our material world(物质世界) is composed of many substances distinguished(区别) by their chemical, mechanical, and electrical properties(特性). They are found in nature in various physical states(物理状态)---the familiar solid, liquid, and gas, along with(连同) the ionic "plasma "(等离子体) However, the apparent diversity(多样性) of kinds and forms of material is reduced by the knowledge that there are only a little over 100 distinct chemical elements(元素) and that the chemical and physical features of substances depend merely on the strength of force bonds(结合) between atoms. 我们的物质世界(物质世界)是由许多物质(以区别区别被其化工、机械、、电气性能(特性)。

他们是在大自然中找到的材料在不同的物理状态(物理状态)——而且熟悉的固体、液体和气体,随着(连同)离子“等离子体”(等离子体)然而,明显的多样性(多样性)各类形式的资料将减少知识只有一个小超过100种特定的化学元素(元素),化学和物理特征的物质的力量仅仅看力债券(结合)之间的原子。

In turn(依次), the distinctions between the elements of nature arise from(起于) the number and arrangement of basic particles(基本粒子)—electrons(电子), protons(质子), and neutrons(中子). At both the atomic and nuclear levels, the structure of elements is determined by internal forces and energy(内力和内能).1.1 FORCES AND ENERGY(力和能量)反过来(依次),区别自然元素(源自起于)电话号码和安排基本粒子)-electrons基本粒子(电子),质子((质子),和中子(中子)。

Wave-particleduality

Wave-particleduality

1. Wave Particle Dualitya. Write the relationship for the kinetic energy and momentum for particle moving at speeds much slower than the speed of light.b. Find the wavelength of an electron in an x -ray machine having a kinetic energy 10 keV.c. Write the relationship for the kinetic energy and momentum for a particle moving at speeds which are on the order of the speed of light.d. Write the relationship for the kinetic energy and momentum for a photon.e . The maximum energy of an x -ray photon produced by a 10 keV electron is 10 keV. Find the wavelength of such an x -ray photon.2. Schroedinger’s EquationA completely free beam of electrons is moving in the +x direction with a kinetic energy of 10 keV. a. Write the Schroedinger equation for a particle moving in the x direction. b. Show that the wave function in a. is a solution to the Schroedinger equation.3. Schroedinger’s EquationAn electron is confined to move freely in a one dimensional box of length L =1.0 nm having infinite potential walls.a. Write the space part wave function for the ground state, and draw it in the upper left provided axes.b. Write the space part probability density and draw it in the lower left provided axes.c. Draw the wave function and probability density for the same situation but for the case where the height of the potential walls is finite.d. Which state, a. or c., has the lower energy. Explain in one sentence.4. In momentum space (k -space) the separation of states is given by Δk x =Δk y =Δk z =π/L .a. Find the number of states in a volume V =L 3 with momentum less than k and kinetic energy less than E .b. Find the Fermi energy for neutrons in a neutron star having 5×1057neutrons with radius 10 km.c. Find the total zero-point kinetic energy of the neutrons at temperature T =0 K.ψx ψxP x P x1. R elativityA s tar i s e mitting l ight i n t he p ositive x d irection. T he w avelength o f t he l ight i s 400 n m.a. (5 p t) W hat i s t he p eriod Δt i n n s o f o ne o scillation o f l ight i n t he s tar’s f ixed reference f rame.Assuming t he w ave t urns o n a t t=0b. (5 p t) H ow f ar d oes i t g o i n t =100 n s i n t he s tar’s f ixed f rame?c. (5 p t) W rite t he 4-­‐vector f or t he s pace-­‐time p osition a fter a t ime 100 n s.d. (5 p t) O btain t he s pace-­‐time i nvariant i nterval t hat t he l ight t ravels i n 100 n s. Suppose t he s tar m oves a way f rom t he e arth i n t he p ositive x d irection w ith a v elocity 0.8c.e. (5 p t) W hat i s t he p eriod Δ′t i n n s o f o ne o scillation o f l ight i n t he e arth’s m oving r eference f rame?f. (5 p t) H ow f ar d oes t he l ight t ravel a fter o ne o scillation a s s een b y t he e arth.f. (5 p t) W rite t he 4-­‐vector f or t he s pace-­‐time p osition a fter a t ime ′t corresponding t o one o scillation a s s een f rom t he e arth’s r eference f rame.g. (5 p t) O btain t he s pace-­‐time i nvariant i nterval i n t he e arth’s f rame t hat t he l ight travels i n 100 n s2.) B ohr m odel.According t o t he B ohr m odel o f t he h ydrogen a tom, a n e lectron i n t he g round s tateorbits a t a r adius o f a bout 0.5 A o. S uppose t he e lectron i s r eplaced b y a m uon( mµc2=105 MeV) t o f orm a m uonic a tom.a. (10 p t) W hat i s t he r adius o f o rbit f or t he m uonic a tom i n i ts g round s tate?b. (10 p t) W hat a re t he e nergies o f t he g round a nd f irst a nd f irst e xcited s tates?c. (10 p t) W hat i s t he w avelength c orresponding t o t he t ransition b etween t he f irst exciteds tate a nd t he g round s tate?3.)Schroedinger e quation.A s imple h armonic o scillator (SHO) h as a m ass m a nd s pring c onstant K. T he p otential e nergy is 1/2Kx2.a. (10 p t) W rite t he S chroedinger e quation f or t he s pace p art o f t he S HO.b. (10 p t) T he w ave f unction f or t he g round s tate h as t he f orm Ae bx2. B y d irects ubstitution s how t his i s a s olution, a nd t hereby f inding t he c onstant b i n t erms o f m a nd Kc. (10 p t) W rite t he p robability d istribution f or t he g round s tate, a nd c arefullyg raph i t.d. (10 p t) W rite a n i ntegral w hichwould b e u sed t o o btain t he n ormalizing c onstantA.You d o n ot n eed t o s olve t his i ntegral)4.)Schroedinger E q. i n 3 d imensions.Consider a t hree d imensional c ubic p otential w ell w ith r igid (infinite) w alls, h avingsides o f d imension L x = L y = L z = L=0.1 n m.a. (5 p t) W rite t he S chroedinger e quation f or a p article w ithin t he w ell.b. (5 p t) W rite t he q uantum c onditions o n k x , k y a nd k z.c. (5 p t) O btain t he q uantum c ondition o n t he w ave n umber k2.d. (5 p t) O btain t he q uantum c ondition o n t he a llowed e nergies E.e. (5 p t) W rite t he g round s tate s olution Ψ(x,y,z)to t he S chroedingere quationf or a p article w ithin t he w ell.f. (5 p t) W rite t he p robability d ensity f or a p article w ithin t he w ell i n t he g roundstate.g. (5 p t) O btain t he n umerical r esult o n t he a llowed e nergies E i n u nits o f e V.h. (5 p t) O btain t he n umber o f e lectrons w hich c an b e a ccommodated a t e ach o ft he l owest 3 e nergy l evels. T ake i nto a ccount t hat d ifferent c ombinations o fq uantum n umbers c an h ave t he s ame e nergy, a nd t hat t wo e lectrons,c orresponding t o s pin u p a nd d own c an f it i ntoe ach c ombination of s patialq uantum n umbers.2006 Exam. 21. A b aby s eal i n t he p acific o cean h as a b ody t emperature o f 310 K. I f t he m ean temperature o f t he w ater i s 287 K a t w hat r ate w ill t he s eal l ose e nergy b y r adiating p hotons? (σ=5.7×10−8 W⋅m-2⋅K-4)2. W ave p article d uality.Compare t he w avelength a nd f requency o f a p hoton a nd e lectron, e ach w ith k ineticenergy 10 K eV.3. B ohr m odel.a. U se t he B ohr m odel o f t he a tom t o e stimate t he e nergy l evels o f p ositronium, i n w hich a n electron o rbits a p ositron.b. T he i onization e nergy (binding e nergy) o f a n e lectron i n h ydrogen i s 13.6 e V.What i s t he i onization e nergy o f p ositronium?4. P article i n a b ox.Approximate a n a tomic n ucleus a s a n i nfinite c ubical b ox o f s ide L=2 f m, w here1 f m = 10-­‐15 m, i n w hich t he n ucleons m ove f reely.a. O btain a n e xpression f or t he w avelength o f t he g round, o r l owest l ying e nergy s tate.b. W hat i s t he k inetic e nergy o f a n eutron i n t he g round s tate o f t his a tom. T he r estenergy o f a n eutron i s m c2=939 M eV.5. S imple h armonic o scillator.A n a pproximate r epresentation o f t he i nteraction b etween t wo a toms i n a d iatomicm olecule i s a s pring l ike f orce F=-­Kx w ith o scillator f requency ω=. T ake t he f orcec onstant t o b e 8×103 e V/nm2 = 1000 N/m, a nd t he m ass of e ach a tom a round t o b e5×10−27kg(mc2=4.69 G eV). T he w ave f unction f or t he g round s tate o f a s imple h armonic o scillatori s ψ0(x)=mωπ⎛⎝⎜⎞⎠⎟1/4e−mω2x2.a. W hat i s t he e nergy o f t he g round s tate?b. F ind t he w ave f unction i n m omentum s pace b y p erforming a F ourier t ransformation.6. D ensity o f s tates a nd F ermi e nergy.a. F ind t he a verage e nergy o f a n e lectron i n a w hite d warf s tar o f r adius 10,000 k mcontaining 2×1057 n ucleons, h alf o f w hich a re p rotons. T he d ensity o f s tates d istribution i sdNdE=E1/2.b. F rom t he r esults i n p art a, c omment o n w hether i t i s a pproporiate t o u se n on-­‐relativistickinematics.Other p roblems f rom p revious e xams:1. A f ree e lectron h as k inetic e nergy 1000 e V. I t m oves i n t he x-­y p lane i n a d irection w hichmakes a n a ngle 30 d eg. r elative t o t he x a xis.a. F ind i ts m omentum p, w avelength λ a nd w ave n umber k.b. W rite t he w ave f unction Ψ(x,y,z,t) i n s ymbols (not n umerical v alues) i n C artesiancoordinates.c. W rite t he p robability d ensity P(x,y,z).d. W hat c an y ou s ay a bout t he u ncertainty i n t he e lectron’s p osition.Approximate a n ucleus c onsisting o f f ree n ucleons i n a s pherical r igid w all p otential w ith radius R=4 f m. F or t he i sotope 17O:a. W hat a re t he q uantum n umbers o f e ach o f t he n eutrons a nd p rotons?b. W hat a re t he e nergies o f e ach o f t he n eutrons a nd p rotons i n t he i sotope 17O?2. a. W rite t he w ave f unction f or a f ree p article m oving i n 3-­‐dimensional C artesiancoordinates.b. T he r elativistic v ersion o f t he S chroedinger e quation i s c alled t he K lein-­‐Gordon e quation.Using E2=p2c2+m2c4, c onstruct t he K lein-­‐Gordon e quation b y e xpressing t he e nergy a nd momentum i n t erms o f d ifferential o perators.c. S how t hat t he w ave f unction i n p art a. i s a s olution t o t he K lein-­‐Gordon w ave f unction t hatwas c onstructed i n p art c.3.) C onsider a n e lectron w hich m oves f reely i n a 2 d imensional i nfinite s quare w ell o f s ide a . a. W rite t he S chroedinger e quation f or t his c ase. b. W hat a re t he a llowed v alues o fk x and k yc. W hat a re t he a llowed e nergy l evels?d. I f a =10Angstroms, w hat i s t he l owest e nergy.e. W rite t he w ave f unction f or t his s tate.4.) T he t hree p rimary t erms w hich d etermine t he b inding e nergy o f a n ucleusare v olume , s urface a nd C oulomb , E V , E S , E C e nergies.a. W hat i s t he R a nd Z d ependence o f e ach, w here R i s t he n uclear r adius a nd Z t he a tomic number.Also i ndicate t he s ign o f e ach. i E V ∝ii E S ∝iii E C ∝b. W hat i s t he A a nd Z d ependence o f e ach, w here A i s t he n umber o f n ucleons. A lso i ndicate the s ign o f e ach. i E V /A ∝ii E S /A ∝iii E C /A ∝c. D raw t he m agnitude o f e ach a s a f unction o f A , a s w ell a s t he s um o f e ach. B e s ure t o c learly fill i n t he e nergy s cale i n t he v ertical a xis a nd t he n umber o f n ucleons i n the h orizontal a xis a t t he p osition o f t he t ic m arks.5.) I n t he b lank s paces p rovided i n t he t able, f ill i n t he p roperties o f t he p article s hown, a s w ell a s t he energy s cales a nd q uark m akeup w here a ppropriate.6.Draw a g raph f or t he s hape o f t he n ucleon-­‐nucleon a ttractive p otential e nergy, i ndicating the a pproximate r ange a nd d epth.particl e Charge Rest m ass energy Units o f energy QuarkFlavor c ontent p +1 .93 GeV uud nπ−.139 π+ e 0.511 ν γ W 89 g7. a . 92238U c aptures a n eutron, f ollowed b y a symmetric f ission i nto 2 u nbound n eutrons a nd3892Sr a nd 54140Xe . O btain t he d ifference i n t he b inding e nergy b etween t he i nitial 92238U and t he f inal 3892Sr a nd 54140Xe n uclides, a nd t herefore t he e nergy r eleased.b . C alculate t he k inetic e nergyd ue t o t he e lectrostatic r epulsion b etween t he 3892Sr a nd 54140Xe w hen t hey a re s till t ouching, a nd s how t hat i t i s t he s ame o rder a s y our a nswerin p art a . a bove. (note:r =r 0A 1/3with r 0≈1.2fm.)8.Fill i n t he t able b elow:9. a . T he m ajor s ource o f e nergy p roduction i n t he s un i s t he p roton-­‐proton c ycle. Trace t he s teps o f t he p -­p c ycle a s w e d iscussed i n c lass.b . I f t he f inal r esult i s t he f usion o f 4 p rotons i nto 4He ,c alculate t he t otal e nergy r eleased in t he c ycle.10. D raw a F eynman d iagram f or e ach o f t he f ollowing p rocesses, a nd i dentify t he e xchanged quantum:a. e -­ +µ+♑e -­ +µ+via t he e lectromagnetic i nteraction. b. e -­ +µ+♑e + +µ-­ v ia t he w eak i nteraction.c. u +u →s +s v ia t he s trong i nteraction.6. F rom t he i nformation o n s pin, b aryon n umber a nd s trangeness g iven i n t he t ablebelow, f ill i n t he q uark f lavor c ontent a nd d ecay i nteraction o f e ach o f t he f ollowing h adrons.Decay interact we。

Mass attenuation coefficient(质量衰减系数)

Mass attenuation coefficient(质量衰减系数)

Tables of X-Ray Mass Attenuation Coefficientsand Mass Energy-Absorption Coefficientsfrom 1 keV to 20 MeV forElements Z = 1 to 92and 48 Additional Substances of DosimetricInterest*J. H. Hubbell+ and S. M. SeltzerRadiation and Biomolecular Physics Division, PML, NIST© 1989, 1990, 1996 copyright by the U.S. Secretary of Commerce on behalf of the United States of America. All rights reserved. NIST reserves the right to charge for these data in the future.AbstractTables and graphs of the photon mass attenuation coefficient μ/ρ and the mass energy-absorption coefficient μen/ρ are presented for all of the elements Z = 1 to 92, and for 48 compounds and mixtures of radiological interest. The tables cover energies of thephoton (x-ray, gamma ray, bremsstrahlung) from 1 keV to 20 MeV. The μ/ρ values are taken from the current photon interaction database at the National Institute of Standards and Technology, and the μen/ρ values are based on the new calculations by Seltzer described in Radiation Research 136, 147 (1993). These tables of μ/ρ and μen/ρreplace and extend the tables given by Hubbell in the International Journal of Applied Radiation andIsotopes 33, 1269 (1982).Note on NIST X-ray Attenuation DatabasesTable of Contents1.Introduction2.X-Ray Mass Attenuation CoefficientsTable 1. Material constants for elemental media.Table 2. Material constants and composition for compounds and mixtures.Values of the mass attenuation coefficient and the mass energy-absorptioncoefficient as a function of photon energy, for:Table 3.[Data] elemental media.Table 4.[Data] compounds and mixtures.3.The Mass Energy-Absorption Coefficient4.Summary5.ReferencesX-Ray Mass Attenuation Coefficients1. IntroductionThe present compilation is an extension of the recent calculationsof Seltzer (1993), and is intended to replace the values of μ/ρ and μen/ρ given in Hubbell (1982) which have been widely used as reference data in radiation shielding and dosimetry computations. The present tables differ from those in Hubbell (1982) in the following respects:1.Instead of providing results for only 40 selected elements with atomicnumbers spanning Z = 1 to 92, now all 92 elements are included.2.Instead of using a common energy grid from 1 keV to 20 MeV,without photoelectric absorption edges (K, L1, etc.), now all edgeenergies are included and identified, and values of μ/ρ and μen/ρ aregiven just above and below each edge to facilitate accurateinterpolation.3.Somewhat different values for the atomic photoeffect cross sectionhave been used for Z = 2 to 54. The 1982 compilation was based onthe application of renormalization factors given by Scofield (1973) tohis calculated values of the cross section. Although Scofield (1973)calculated the cross sections for all Z≥ 2, he gave renormalizationfactors only for 2 ≤Z≤ 54. An evaluation by Saloman et al. (1988)compared the Scofield theoretical values with the measured-valuedatabase, and concluded that overall agreement was better withoutthis renormalization. The present work therefore uses the"un-renormalized" Scofield (1973) theoretical values of thephotoeffect cross section for all elements Z≥ 2. The analytical resultsused for Z = 1 are the same as those used in the 1982 compilation.4.For compounds and mixtures, values for μ/ρ can be obtained bysimple additivity, i.e., combining values for the elements according to their proportions by weight. To the extent that values for μen/ρ areaffected by the radiative losses (bremsstrahlung production,annihilation in flight, etc.) suffered during the course of slowingdown in the medium by the electrons and positrons that have been setin motion, simple additivity is no longer adequate. The 1982compilation ignored such matrix effects (they tend to be small atphoton energies below 20 MeV); in the present tables they have beentaken into account.A narrow beam of monoenergetic photons with an incident intensity I o, penetrating a layer of material with mass thickness x and density ρ, emerges with intensity I given by the exponential attenuation law(eq 1)Equation (1) can be rewritten as(eq 2)from which μ/ρ can be obtained from measured values of I o, I and x.Note that the mass thickness is defined as the mass per unit area, and is obtained by multiplying the thickness t by the density ρ, i.e., x = ρt.The various experimental arrangements and techniques from which μ/ρ can be obtained, particularly in the crystallographic photon energy/wavelength regime, have recently been examined and assessed by Creagh andHubbell (1987, 1990) as part of the International Union of Crystallography (IUCr) X-Ray Attenuation Project. This has led to new tables of μ/ρ in the 1992 International Tables for Crystallography (Creagh and Hubbell, 1992). The current status of μ/ρ measurements has also been reviewed recentlyby Gerward (1993), and an updated bibliography of measured data is available in Hubbell(1994).Present tabulations of μ/ρ rely heavily on theoretical values for the total cross section per atom, σtot, which is related to μ/ρ according to(eq 3) In (eq 3), u (= 1.660 540 2 × 10-24 g Cohen and Taylor 1986) is the atomic mass unit (1/12 of the mass of an atom of the nuclide 12C), A is the relative atomic mass of the target element, and σtot is the total cross section for an interaction by the photon, frequently given in units of b/atom (barns/atom), where b = 10-24 cm2.The attenuation coefficient, photon interaction cross sections and related quantities are functions of the photon energy. Explicit indication of this functional dependence has been omitted to improve readability.The total cross section can be written as the sum over contributions from the principal photon interactions,(eq 4) where σpe is the atomic photoeffect cross section, σcoh and σincoh are the coherent (Rayleigh) and the incoherent (Compton) scattering cross sections, respectively, σpair and σtrip are the cross sections for electron-positron production in the fields of the nucleus and of the atomic electrons, respectively, and σph.n. is the photonuclear cross section.Photonuclear absorption of the photon by the atomic nucleus results most usually in the ejection of one or more neutrons and/or protons. This interaction can contribute as much as 5 % to 10 % to the total photon interaction cross section in a fairly narrow energy region usually occurring somewhere between 5 MeV and 40 MeV, depending on where the giant resonance of the target nuclide falls (see, e.g., Hayward, 1970; Fuller and Hayward,1976; and Dietrich and Berman, 1988; also the illustrative tablesin Hubbell, 1969, 1982). The effects of this interaction can be observed in measurements of the total attenuation coefficient (see, e.g., Gimm and Hubbell, 1978). However, this cross section has not been included in previous tabulations because of the difficulties due to (a) the irregular dependence of both the magnitude and resonance-shape of the cross section as a function of both Z and A; (b) the gaps in the available information, much of which is for separated isotopes or targets otherwise differing from natural isotopic mixtures; and (c) the lack of theoretical modelsfor σph.n. comparable to those available for calculations of the other cross sections of interest. The practice of omitting the contribution of the photonuclear cross section in tables of the mass attenuation coefficient has been continued in this work, along with the neglect of other less-probable photon-atom interactions, such as nuclear-resonance scattering andDelbrück scattering.Our results for the elements are given in Table 3 for elements Z = 1 to 92 and photon energies 1 keV to 20 MeV, and have been calculated according to(eq 5) Values for the relative atomic mass A of the target elements were taken from Martin (1988) and can be extracted from the values of Z/A givenin Table 1;values for the individual contributing cross sections are those found in the current NIST database (see Berger and Hubbell, 1987), as outlined below.Atomic photoeffect. For photon energies from 1 keV to 1.5 MeV, values of the photoelectric cross section, σpe, are those calculated by Scofield (1973), based on his solution of the Dirac equation for the orbital electrons moving in a static Hartree-Slater central potential. No renormalization was performed using those factors given by Scofield for the elements with Z = 2 to 54 to convert to values expected from a relativistic Hartree-Fock model. This represents a break with the practice by Hubbell (1977, 1982)and Hubbell et al. (1980) in which this renormalization had been done.Electron-positron pair and triplet production cross sections. Cross sections for the production of electron-positron pairs (e-, e+) in the field of the atomic nucleus, σpair, and for the production of triplets (2e-, e+) in the field of the atomic electrons, σtrip, are taken from the compilation of Hubbell etal. (1980). Their synthesis combined the use of formulas from Bethe-Heitler theory with various other theoretical models to take into account screening, Coulomb, and radiative corrections. Different combinations were used in the near-threshold, intermediate and high-energy regions to obtain the best possible agreement with experimental cross sections (Gimm and Hubbell, 1978).Mixtures and compounds. Values of the mass attenuation coefficient, μ/ρ,for the 48 mixtures and compounds (assumed homogeneous) are givenin Table 4,and were obtained according to simple additivity:(eq 6)X-Ray Mass Attenuation Coefficients3. The Mass Energy-Absorption Coefficient, μen/ρThe methods used to calculate the mass energy-absorption coefficient, μen/ρ, are described perhaps more clearly through the use of an intermediate quantity, the mass energy-transfer coefficient, μtr/ρ.The mass energy-transfer coefficient,μtr/ρ, when multiplied by the photon energy fluence ψ (ψ = ΦE, where Φ is the photon fluence and E the photon energy), gives the dosimetric quantity kerma. As discussed in depthby Carlsson (1985), kerma has been defined (ICRU Report 33, 1980) as (and is an acronym for) the sum of the k inetic e nergies of all those primary charged particles r eleased by uncharged particles (here photons) perunit ma ss. Thusμtr/ρ takes into account the escape only of secondary photon radiations produced at the initial photon-atom interaction site, plus, by convention, the quanta of radiation from the annihilation of positrons (assumed to have come to rest) originating in the initial pair- andtriplet-production interactions.Hence μtr/ρ is defined as(eq 7) In (eq 7), coherent scattering has been omitted because of the negligible energy transfer associated with it, and the factors f represent the average fractions of the photon energy E that is transferred to kinetic energy of charged particles in the remaining types of interactions. Theseenergy-transfer fractions are given by(eq 8) where X is the average energy of fluorescence radiation (characteristicx rays) emitted per absorbed photon;(eq 9) where is the average energy of the Compton-scattered photon;(eq 10)where mc2 is the rest energy of the electron; and(eq 11)The fluorescence energy X in (eq 8), (eq 9), and ( 11) depends on the distribution of atomic-electron vacancies produced in the process under consideration and is in general evaluated differently for photoelectric absorption, incoherent scattering, and triplet production. Moreover, X isassumed to include the emission of "cascade" fluorescence x rays associated with the complete atomic relaxation process initiated by the primary vacancy, the significance of which has been pointed out by Carlsson (1971). As only the characteristics of the target atom are involved in calculating μtr/ρ, the mass energy-transfer coefficient for homogeneous mixtures and compounds can be obtained in a manner analogous to that for μ/ρ:(eq 12)The mass energy-absorption coefficient involves the further emission of radiation produced by the charged particles in traveling through the medium, and is defined as(eq 13) The factor g in (eq. 13) represents the average fraction of the kinetic energy of secondary charged particles (produced in all the types of interactions) that is subsequently lost in radiative (photon-emitting) energy-loss processes as the particles slow to rest in the medium. The evaluation of g is accomplished by integrating the cross section for the radiative process of interest over the differential tracklength distribution established by the particles in the course of slowing down. In the continuous-slowing-down approximation, the tracklength distribution is replaced by the reciprocal of the electron or positron total stopping power of the medium. Even assuming Bragg additivity for the stopping power (that now appears in the denominator of the integral), simple additivity for μen/ρ or - as suggested by Attix (1984) - for g is formally incorrect. When the numerical values of g are relatively small, the errors in μen/ρ incurred by using simple additivity schemes are usually small, a consequence partially mitigating the use additivity, particularly for photon energies below 20 MeV. However, additivity has not been used in the present work.For the values of μen/ρ given in Table 3 and Table 4, the evaluationof g takes into explicit account (a) the emission of bremsstrahlung,(b) positron annihilation in flight, (c) fluorescence emission as a result of electron- and positron-impact ionization, and (d) the effects on these processes of energy-loss straggling and knock-on electron production as the secondary particles slow down (i.e., of going beyond thecontinuous-slowing-down approximation). This scheme thus goes beyond that of ICRU Report 33 (1980) which, perhaps by oversight, formally includes only (a) above, and of previous work, which usually includes (a) and (b).For the calculation of g, the radiative (bremsstrahlung) stopping powers used are based on the results by Seltzer and Berger (1985, 1986) and Kim et al.(1986), and are very slightly different from the values used in ICRU Report 37 (1984). The collision stopping powers, evaluated according to the prescriptions in ICRU Report 37 (1984), include departures from simple Bragg additivity due to chemical-binding, phase, and density effects, as reflected in the choice of the mean excitation energy I and density ρ for the medium. These departures from Bragg additivity for the stopping power of the matrix can result in discernable differences in the massenergy-absorption coefficient, such as between those for water vapor and liquid.Further details of the calculations are given in Seltzer (1993) and will not be repeated here. Instead, a summary of expressions used for the calculationof g is given below. The formulas include the integration over the initial particle spectra, and have been generalized to include mixtures and compounds.Photoelectric Absorption. The radiative losses for the photoelectrons have been evaluated according to(eq 14) where μpe/ρ is the total photoeffect mass attenuation coefficient for an incident photon of energy E in the medium, (μpe/ρ)n,i is the corresponding coefficient for the n th atomic electron subshell of the i th elemental constituent, B n,i is the binding energy of that subshell, and(eq 15)is the total radiative yield. The total radiative yield has been evaluated as the sum of two components. The bremsstrahlung yield,Y b(T), is the mean fraction of the initial kinetic energy T of an electron (or positron) that is converted to bremsstrahlung energy as the particle slows down to rest; and the x-ray energy yield,Y x(T), usually very much smaller than Y b(T), is the mean fraction of the initial kinetic energy converted to fluorescence emission due to ionization by the electron (or positron) in the course of slowing down. The very small radiative losses for the associated Auger electrons have been neglected.Incoherent (Compton) Scattering. For incoherent scattering(eq 16) where S(q,Z i) is the incoherent scattering factor, taken from the compilation of Hubbell et al. (1975), dσKN/d E′ is the Klein-Nishina cross section differential in the Compton-scattered photon energy E′,E min = E/(1 +2E/mc2) is the minimum energy of the scattered photon (corresponding to 180° scattering), and Y(T) is the total radiative yield.Pair and Triplet production. The radiative losses from electrons and positrons created in the pair and triplet processes, including the effects of positron annihilation in flight, have been evaluated according to:(eq 17) where P pair,i(T+)d T+ is the probability that the positron from apair-production interaction with the i th constituent atom will have a kinetic energy between T+ and T+ + d T+, Y-(T-) and Y+(T+) are the total radiation yields for the electrons and positrons, respectively, and η(T+) is the correction for positron annihilation in flight. Pair spectra have been evaluated using Bethe-Heitler theory in conjunction with screening and Coulomb corrections. The annihilation-in-flight correction has been derived on the basis outlined in Berger (1961), and has been evaluated using thetwo-quanta annihilation-in-flight cross section of Bethe (1935) plus estimates for the one-quantum annihilation-in-flight cross section. Computation of g trip proceeds similarly, but using the threshold for triplet production of 4 mc2 instead of 2 mc2 in (eq 17), and usingthe Wheeler-Lamb(1939) expressions for the screening corrections to the triplet spectra.Abstract|Introduction|Mass Atten. Coef.|Mass Energy-Absorp.Coef. |Summary|ReferencesX-Ray Mass Attenuation Coefficients4. SummaryValues of the mass attenuation coefficient, μ/ρ, and the massenergy-absorption coefficient, μen/ρ, for photon energies 1 keV to 20 MeV, including all absorption edges, are given for all elements Z = 1 to 92in Table 3 and for 48 compounds and mixtures of radiological interestin Table 4. Graphs ofμ/ρ and μen/ρ are presented for all materials included in Tables 3 and 4. Table 1 lists the values of Z/A, the mean excitation energy I, and the density used in the calculations of μen/ρ for Table 3; Table 2 gives similar information used to obtain results for Table 4, including the fractions by weight w i of the constituent elements assumed for each material.X-Ray Mass Attenuation Coefficients5. ReferencesAllison, J.W. (1961), Gamma-Radiation Absorption Coefficients of Various Materials Allowing for Bremsstrahlung and other Secondary Radiations, Austral. J. Phys. 14, 443-461.Attix, F.H. (1984), Energy-Absorption Coefficients for γ-Rays in Compounds and Mixtures, Phys. Med. Biol. 29, 869-871.Bethe, H.A. (1935), On the annihilation radiation of positrons. Proc. R. Soc. London150, 129-141.Bearden, J.A. and Burr, A.F. (1967), Reevaluation of X-Ray Atomic Energy Levels, Rev. Mod. Phys. 39, 125-142.Berger, M.J. and Hubbell, J.H. (1987), XCOM: Photon Cross Sections on a Personal Computer, NBSIR 87-3597.Berger, R.T. (1961), The X- or Gamma-Ray Energy Absorption or Transfer Coefficient: Tabulations and Discussion, Rad. Res. 15, 1-29.Brown, R.T. (1970a), Coherent and Incoherent X-Ray Scattering by Bound Electrons. I. Helium Isoelectronic Sequence, Phys Rev. A 1, 1342-1347.Brown, R.T. (1970b), Coherent and Incoherent X-Ray Scattering by Bound Electrons. II. Three-and Four-Electron Atoms, Phys. Rev. A 2, 614-620.Brown, R.T. (1971), Atomic Form Factor for Neutral Carbon, J. Chem. Phys. 55, 353-355.Brown, R.T. (1972), Incoherent-Scattering Function for Atomic Carbon, Phys. Rev. A 5, 2141-2144.Brown, R.T. (1974), Coherent and Incoherent X-Ray Scattering by Bound Electrons. III. Five-Electron Atoms, Phys. Rev. A 10, 438-439. Carlsson, G.A. (1971), A Criticism of Existing Tabulations of Mass Energy Transfer and Mass Energy Absorption Coefficients, HealthPhys. 20, 653-655.Carlsson, G.A. (1985), Theoretical Basis for Dosimetry, Chap. 1 in The Dosimetry of Ionizing Radiation, Vol. 1, K.R. Kase, B.E. Bäjrngard and F.H. Attix, eds. (Academic Press, Orlando), 1-75.Cohen, E.R. and Taylor, B.N. (1986), The 1986 Adjustment of the Fundamental Physical Constants, CODATA Bulletin 63 (values republished most recently in Physics Today, August 1997, BG7-BG11).Creagh, D.C. and Hubbell, J.H. (1987), Problems Associated with the Measurement of X-Ray Attenuation Coefficients. I. Silicon. Report on the International Union of Crystallography X-Ray Attenuation Project, Acta Cryst. A 43, 102-112.Creagh, D.C. and Hubbell, J.H. (1990), Problems Associated with the Measurement of X-Ray Attenuation Coefficients. II. Carbon. Report on the International Union of Crystallography X-Ray Attenuation Project, Acta Cryst. A 46, 402-408.Creagh, D.C. and Hubbell, J.H. (1992), X-Ray Absorption (or Attenuation) Coefficients, Sec. 4.2.4. in International Tables forCrystallography, Vol. C,A.J.C. Wilson, ed. (Kluwer Academic Publishers, Dordrecht), 189-206.Cromer, D.T. and Mann, J.B. (1967), Compton Scattering Factors for Spherically Symmetric Free Atoms, J. Chem. Phys. 47, 1892-1983.Cromer, D.T. (1969), Compton Scattering Factors for Aspherical Free Atoms, J. Chem. Phys. 50, 4857-4859.Cromer, D.T. and Waber, J.T. (1974), Atomic Scattering Factors for X-Rays, Sec. 2.2. in International Tables for X-Ray Crystallography, Vol. 4 (Kynoch Press, Birmingham), 71-147.Cullen, D.E., Chen, M.H., Hubbell, J.H., Perkins, S.T., Plechaty, E.F., Rathkopf, J.A. and Scofield, J.H. (1989), Tables and Graphs ofPhoton-Interaction Cross Sections from 10 eV to 100 GeV Derived from the LLNL Evaluated Photon Data Library (EPDL), Part A: Z = 1 to 50; PartB: Z = 51 to 100, Lawrence Livermore National Laboratory ReportUCRL-50400, Vol. 6, Rev. 4.Cunningham, J.R. and Johns, H.E. (1980), Calculation of the Average Energy Absorbed in Photon Interactions, Med. Phys. 7, 51-54.Del Grande, N.K. (1986), Measured 1 to 40 keV Photoabsorption Cross Sections for: Fe, Ni, Sn, Ta, Pt, Au, Pb, U, Proc. SPIE 691 (X-Ray Imaging II), 2-10.Del Grande, N.K. (1990), L Shell Photoabsorption Spectroscopy for Solid Metals: Ti, V, Cr, Fe, Ni, Cu, Physica Scripta 41, 110-114.Deslattes, R.D. (1969), Estimates of X-Ray Attenuation Coefficients for the Elements and Their Compounds, Acta Cryst. A 25, 89-93.Dietrich, S.S. and Berman, B.L. (1988), Atlas of Photoneutron Cross Sections Obtained with Monoenergetic Photons, At. Data Nucl. Data Tables 38, 199-338.Doyle, P.A. and Turner, P.S. (1968), Relativistic Hartree-Fock X-Ray and Electron Scattering Factors, Acta Cryst. A 24, 390-397.Evans, R.D. (1968), X-Ray and γ-Ray Interactions, Chap. 3 in Radiation Dosimetry, Vol. 1, F. H. Attix and W. C, Roesch, eds. (Academic Press, New York), 93-155.Faessler, A. (1955), Röntgenspektrum und Bindungszustand, Sec. 1508in Landolt-Börnstein Zahlenwerte und Funktionen aus Physik, Chemie, Astronomie, Geophysik und Technik, A. Eucken, ed. (Springer, Berlin), 769-868.Fuller, E.G. and Hayward, E. (1976), Photonuclear Reactions (Dowden, Hutchinson & Ross, Stroudsburg, Pennsylvania).Gerward, L. (1993), X-Ray Attenuation Coefficients: Current State of Knowledge and Availability. Radiat. Phys. Chem. 41, 783-789.Gimm, H.A. and Hubbell, J.H. (1978), Total Photon Absorption Cross Section Measurements, Theoretical Analysis and Evaluations for Energies above 10 MeV, NBS Techn. Note 968.Hayward, E. (1970), Photonuclear Reactions, NBS Monograph 118.Higgins, P.D., Attix, F.H., Hubbell, J.H., Seltzer, S.M., Berger, M.J. and Sibata, C.H. (1992), Mass Energy-Transfer and Mass Energy-Absorption Coefficients, Including In-Flight Positron Annihilation for Photon Energies 1 keV to 100 MeV, NISTIR 4812.Hubbell, J.H. and Berger, M.J. (1968), Sec. 4.1: Attenuation Coefficients, Energy Absorption Coefficients, and Related Quantities. and Sec. 4.2: Photon Atomic Cross Sections, in Engineering Compendium on Radiation Shielding, Vol. 1, R.G. Jaeger, ed. (Springer, Berlin), 167-202.Hubbell, J.H. (1969), Photon Cross Sections, Attenuation Coefficients, and Energy Absorption Coefficients from 10 keV to 100 GeV, NSRDS-NBS 29.Hubbell, J.H., McMaster, W.H., Del Grande, N.K. and Mallett, J.H. (1974), X-Ray Cross Sections and Attenuation Coefficients, Sec. 2.1.in International Tables for X-Ray Crystallography, Vol. 4, J.A. Ibers and W.C. Hamilton, eds. (Kynoch Press, Birmingham), 47-70.Hubbell, J.H., Veigele, Wm.J., Briggs, E.A., Brown, R.T., Cromer, D.T. and Howerton, R.J. (1975), Atomic Form Factors, Incoherent Scattering Functions, and Photon Scattering Cross Sections, J. Phys. Chem. Ref.Data 4, 471-538; erratum in 6, 615-616 (1977).Hubbell, J.H. (1977), Photon Mass Attenuation and MassEnergy-Absorption Coefficients for H, C, N, O, Ar, and Seven Mixtures from 0.1 keV to 20 MeV, Rad. Res. 70, 58-81.Hubbell, J.H. and Øverbø, I. (1979), Relativistic Atomic Form Factors and Photon Coherent Scattering Cross Sections, J. Phys. Chem. Ref.Data 8, 69-105.Hubbell, J.H., Gimm, H.A. and Øverbø, I. (1980), Pair, Triplet, and Total Atomic Cross Sections (and Mass Attenuation Coefficients) for 1 MeV-100 GeV Photons in Elements Z = 1 to 100, J. Phys, Chem. Ref.Data 9, 1023-1147.Hubbell, J.H. (1982), Photon Mass Attenuation and Energy-Absorption Coefficients from 1 keV to 20 MeV, Int. J. Appl. Radiat.Isot. 33, 1269-1290.Hubbell, J.H. (1994), Bibliography of Photon Total Cross Section (Attenuation Coefficient) Measurements 10 eV to 13.5 GeV, 1907-1993, NISTIR 5437.ICRU (1980), Radiation Quantities and Units, Report 33 of the International Commission on Radiation Units and Measurements (Bethesda, MD).ICRU (1984), Stopping Powers for Electrons and Positrons, Report 37 of the International Commission on Radiation Units and Measurements (Bethesda, MD).ICRU (1989), Tissue Substitutes in Radiation Dosimetry and Measurement, Report 44 of the International Commission on Radiation Units and Measurements (Bethesda, MD).Johns, H.E. and Cunningham, J.R. (1983), The Physics of Radiology, 4th Ed. (Thomas, Springfield, Ill.)Kim, L., Pratt, R.H., Seltzer, S.M. and Berger, M.J. (1986), Ratio of Positron to Electron Bremsstrahlung Energy Loss: An Approximate Scaling Law, Phys. Rev. A 33, 3002-3009.Klein, O. and Nishina, Y. (1929), Über die Streuung von Strahlung durch freie Elektronen nach der neuen relativistischen Quantendynamik von Dirac, Z. Physik 52, 853-868.Lytle, F.W. (1963), X-Ray Absorption Fine-Structure Investigations at Cryogenic Temperatures, in Developments in Applied Spectroscopy, Vol. 2 (Plenum, New York), 285-296.Lytle, F.W., Greegor, R.B., Sandstrom, D.R., Marques, E.C., Wong, J., Spiro, C.L., Huffman, G.P. and Huggins, F.E. (1984), Measurement of Soft X-Ray Absorption Spectra with a Fluorescent Ion Chamber Detector, Nucl. Instr. Meth. 226, 542-548.Martin, R.L. (1988), Atomic Weights of the Elements 1987, Pure and Appl. Chem 60, 841-854.Mork, K.J. (1971), Radiative Corrections. II. Compton Effect, Phys. Rev.A 4, 917-927.Øverbø, I. (1977), Atomic Form Factors for Large Momentum Transfers, Nuovo Cim. B 40, 330-338.Øverbø, I. (1978), Large-q Form Factors for Light Atoms, Phys.Scripta 17, 547-548.Pirenne, M.H. (1946), The Diffraction of X-Rays and Electrons by Free Molecules (Cambridge Univ. Press, London), 12-28.Plechaty, E.F., Cullen, D.E. and Howerton, R.J. (1978), Tables and Graphs of Photon-Interaction Cross Sections from 0.1 keV to 100 MeV Derived from the LLNL Evaluated-Nuclear-Data Library, Lawrence Livermore National Laboratory Report UCRL-5400, Vol. 6, Rev. 2.Pratt, R.H. (1960), Atomic Photoelectric Effect at High Energies, Phys. Rev. 117, 1017-1028.Ribberfors, R. and Carlsson, G.A. (1985), Compton Component of the Mass-Energy Absorption Coefficient: Corrections Due to the Energy Broadening of Compton-Scattered Photons, Rad. Res. 101, 47-59.。

小学下册B卷英语第2单元寒假试卷

小学下册B卷英语第2单元寒假试卷

小学下册英语第2单元寒假试卷英语试题一、综合题(本题有100小题,每小题1分,共100分.每小题不选、错误,均不给分)1.My grandmother has a __________ house. (舒适的)2.I think everyone should have a mentor to guide them in __________.3.I love the sound of ______ (水滴) on the roof.4.What do we call a large amount of snow that falls quickly?A. ShowerB. BlizzardC. DrizzleD. Storm5.What is the name of the boundary beyond which no light can escape a black hole?A. Event HorizonB. SingularityC. Photon SphereD. Accretion Disk6.I think learning is very ________ (重要).7.The chemical formula for sulfuric acid is __________.8.The _____ (mountain) is snowy.9.What is the name of the fictional character who flies with Peter Pan?A. CinderellaB. Tinker BellC. Snow WhiteD. ArielB10. A ______ is a positively charged particle in the nucleus of an atom.11.My ______ is a great cook and loves to bake.12.What do you call the person who repairs cars?A. DoctorB. MechanicC. TeacherD. ChefB13.The concept of ecological sustainability promotes practices that support ______ health.14.The country known for its fashion is ________ (以时尚闻名的国家是________).15.What is the first month of the year?A. JanuaryB. FebruaryC. MarchD. AprilA16. A base can neutralize an ______.17.My ________ (外甥) likes to play soccer after school.18. A __________ (科学探索) expands our understanding of the natural world.19.What do we call a person who studies the human mind?A. PsychologistB. SociologistC. AnthropologistD. Biologist20.I have a favorite ______ (玩具), a teddy bear that I sleep with every night.21. A tornado is a fast-moving ______.22.The ________ (交通枢纽) connects different regions.23.Which instrument has keys and makes music?A. GuitarB. ViolinC. PianoD. DrumC24.__________ is the substance that dissolves in a solution.25.The tree is home to many ______.26.What do you call the place where you play sports?A. SchoolB. FieldC. GymD. ClassroomC27.The ice cream truck is _______ (coming) down the street.28.I have a toy _______ that dances and sings my favorite tunes.29.I like to go ______ (滑雪) with my friends during winter break.30.The boiling point of water is higher at _____ altitudes.31.My brother likes to _____ video games. (play)32.I love to paint my toy ____ in bright colors. (玩具名称)33.The _____ (rain) nourishes the soil.34.The teacher helps students develop _____ (技能).35.The _______ of a sound can be measured in decibels.36. d States was formed after declaring independence from ________ (英国). The Ural37._____ (vineyards) produce grapes for wine.38.My friends are _______ (支持我的).39.The goldfish is often kept in _______ (家庭) aquariums.40.My cousin is a ______. She loves to create art.41.What is 6 x 7?A. 42B. 36C. 48D. 54A42.We built a ________ out of blocks.43.My friend is very ________.44.What is the freezing point of water?A. 0 degrees CelsiusB. 100 degrees CelsiusC. 32 degrees FahrenheitD. Both A and CD45.Every morning, I write in my _______ (日记). It helps me organize my _______ (思想).46.The ____ has a soft voice and is heard in the morning.47.The ____ is a curious animal that enjoys exploring new places.48.My ________ (玩具名称) can float on water.49.The crow is known for its ________________ (智慧).50.I have a special ________ that reminds me of home.51.What is the main language spoken in Spain?A. FrenchB. GermanC. SpanishD. Italian52.Understanding a plant's ______ helps in its proper care. (了解植物的需求有助于正确照顾它。

小学上册第二次英语第六单元测验试卷

小学上册第二次英语第六单元测验试卷

小学上册英语第六单元测验试卷考试时间:80分钟(总分:100)B卷一、综合题(共计100题共100分)1. 选择题:What is the name of the process by which plants release oxygen?A. PhotosynthesisB. RespirationC. DigestionD. Fermentation答案: A2. 选择题:What is the capital of the Central African Republic?A. BanguiB. BouarC. BerberatiD. Bambari答案:A3. 听力题:She is a ______. She teaches us science.4. 填空题:The stars are ________ (璀璨).5. 填空题:The _____ (thyme) plant is aromatic and useful.6. 填空题:A _____ is a narrow strip of land connecting two larger land areas.7. 填空题:The _______ (Age of Exploration) led to the discovery of new lands and trade routes.8. 填空题:The first person to win the Nobel Prize in Physics was _______. (亨利·贝克勒尔)I enjoy _______ (cooking) new recipes.10. 选择题:What is the name of the famous turtle in the children's book?A. FranklinB. GaryC. TimmyD. Oliver11. 选择题:What do we call the tool used to cut paper?A. KnifeB. ScissorsC. RulerD. Glue12. 选择题:What is the main ingredient in a smoothie?A. MilkB. YogurtC. FruitD. Ice答案:C13. 填空题:I made a ________ out of clay.14. 填空题:The ______ (自然) is full of surprises.15. 填空题:My dad enjoys __________ (木工).16. 填空题:The teacher, ______ (老师), motivates us to learn.17. 填空题:The ______ (小鸭子) swims in the pond. It quacks and looks for its ______ (妈妈).18. 填空题:The owl has excellent ______ (夜视能力).19. 填空题:My teacher teaches us . (我的老师教我们。

初三英语物理概念单选题30题

初三英语物理概念单选题30题

初三英语物理概念单选题30题1. When you push a heavy box, the force you apply is called _____.A. gravitational forceB. frictional forceC. applied forceD. magnetic force答案:C。

本题考查力的概念。

选项A 重力是物体由于地球吸引而受到的力;选项B 摩擦力是阻碍物体相对运动的力;选项C 施加的力,符合推重箱子时所用力的描述;选项D 磁力是与磁体相关的力。

2. Energy can be transformed from one form to another. Which of the following is an example of converting electrical energy to light energy?A. A fan runningB. A battery chargingC. A bulb lighting upD. A car engine working答案:C。

本题考查能量转化。

选项A 风扇运行是电能转化为机械能;选项B 电池充电是电能转化为化学能;选项C 灯泡亮起是电能转化为光能;选项D 汽车发动机工作是内能转化为机械能。

3. If an object is at rest on a table, the force acting on it is _____.A. only gravitational forceB. only normal forceC. both gravitational force and normal forceD. no force at all答案:C。

物体静止在桌子上,受到竖直向下的重力和桌子对它竖直向上的支持力,支持力也叫弹力,在这种情况下称为法向力(normal force)。

4. Which of the following has the greatest amount of potential energy?A. A ball at the top of a hillB. A car moving at high speedC. A bird flying in the skyD. A person sitting on a chair答案:A。

小学上册第九次英语第五单元寒假试卷

小学上册第九次英语第五单元寒假试卷

小学上册英语第五单元寒假试卷英语试题一、综合题(本题有100小题,每小题1分,共100分.每小题不选、错误,均不给分)1.What do you call a collection of books?A. LibraryB. ShelfC. ArchiveD. Bookstore2.Mixtures can be homogeneous or _____.3.The cat is ________ on the sofa.4.The ________ (生态恢复计划) aims to revive habitats.5.My brother’s name is ____.6.What is the opposite of "hot"?A. WarmB. ColdC. CoolD. ChillyB7.The _______ of sound can vary in different spaces and environments.8.My friend is __________ (非常有帮助).9.What do you call a person who plays music?A. ArtistB. MusicianC. ActorD. AuthorB10.The ________ (绿色空间) enhances urban areas.11. are great at ______ (攀爬). Squirrel12. A __________ can form when rivers deposit sediment.13.The _____ (狮子) is known for its majestic mane.14.What is 4 x 3?A. 10B. 12C. 14D. 16B15.The __________ (灌溉) system is important for farms.16.The ________ (hologram) is a D image.17.The rabbit eats ______ (草) and vegetables.18.I put my _______ (shoes) by the door.19. A __________ (植物的生命周期) includes several stages.20.What is 25 + 25?A. 40B. 45C. 50D. 5521.The __________ (历史的声音) echoes through time.22.The main gas involved in photosynthesis is ______.23.The _______ (小青蛙) croaks by the pond.24.The invention of ________ has revolutionized entertainment.25.The __________ is changing quickly, so I should grab my coat. (天气)26.What is the term for a baby fox?A. KitB. CubC. PupD. CalfA27.I enjoy spending time with my ______.28.Planting native species can support local ______. (种植本地物种可以支持当地生态系统。

光电学部分答案-刘旭版

光电学部分答案-刘旭版
作业11a过长度为d的自由空间光线角度不变位置改变近轴光线作业11b薄透镜厚度d0yz面上为焦距为f的薄透镜作业11312beamidentificationbytwowidths
光电子学作业 参考答案
作业1
Fundamentals of Photonics (括号内为中文教材上题目 的位置):
• 1.4-1 • 1.4-4 • 3.1-2 (P41-2) • 3.1-3 (P41-3) • 3.2-1 (P41-4)
可列式求解:
作业1
(a)过长度为d的自由空间,光线角度不变,位置改变
(近轴光线
)
作业1
(b)薄透镜厚度d 0, y-z面上为焦距为f的薄透镜
作业1
3.1-2 Beam Identification by Two Widths. A Gaussian beam of wavelength =10.6 pm (emitted by a CO2 laser) has widths W1=1.699mm and W2=3.38mm at two points separated by a distance d=10 cm. Determine the location of the waist and the waist radius.
作业2
复参数q表达形式:
界面传输矩阵为: q参数满足ABCD法则:
则: 又 发散角
故: 为:
作业2
9.1-1 Resonance Frequencies of a Resonator with an Etalon.
(a) Determine the spacing between adjacent resonance frequencies in a resonator constructed of two parallel planar mirrors separated by a distance d=15 cm in air (n=1). (b) A transparent plate of thickness d1=2.5 cm and refractive index n=1.5 is placed inside the resonator and is tilted slightly to prevent light reflected from the plate from reaching the mirrors. Determine the spacing between the resonance frequencies of the resonator.
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4 m2 γc h2 ν 2 1/2
(3)
We would like to point out that (3) indicates that higher frequency radiation has a velocity greater than lower frequency radiation reaching one thousandth of a second earlier. This is a very subtle and minute effect and is best tested in for example, the observation of high energy gamma rays, which we receive from deep outer space. It is quite remarkable that we may already have witnessed this effect- higher frequency components of gamma rays in cosmic rays do indeed seem to reach earlier than their lower frequency counterparts [6]. The GLAST satellite of NASA to be launched later in 2007 may be able to throw more light on these high energy Gamma rays. 5. Another consequence of the non zero photon mass is that the usual Coulomb potential goes over into a Yukawa potential with a range equal to the Compton length of the photon which in fact is ∼ 1028 cms which again is the radius of the universe. So the effect will be very small indeed but in principle this would lead to, for example a shift in the fine structure energy levels that could be observed. Let us introduce the Yukawa potential, V (r ) = αe−µr /r (4)
both of which are at rest in the same inertial reference frame. If Lorentz Invariance was strictly valid, then such a force would not have existed. The conclusion was that there was such a Lorentz violation at an energy threshold of 10−9 eV , corresponding to a low energy regime. It may be pointed out that this threshold is in fact above that in a massive photon with the mass suggested above. 4. With a non zero photon mass we would have, for radiation
1 πd GL 32
4
Φ 2 w w −u
k
1 (w 4
− u)2 nhIln
× sin(ΘA )
(1)
in which ΘA is on the angle between Aambient and Earth’s rotation axis. As can be seen from (1) the torque vanishes if the photon does not have a mass. Alternatively this could happen if the cosmic ambience vector potential were accidentally aligned with the earth’s axis of rotation. Such an accident was of course ruled out. The experiment with values substituted into (1) suggested that the photon mass is less than 10−52 gms. 3. Mignani and co-workers have performed experiments which demonstrate, surprisingly a violation of Lorentz Invariance in the low energy regime [5]. In fact this is exactly what we would expect with the photon mass suggested above. This experiment was first performed in 1998 and then repeated in 1999 with improved sensitivity. Both gave the same result. The experiment attempted to detect a DC voltage across a conductor induced by the steady magnetic field of a coil. Such a voltage would be a signature of a violation of Lorentz Invariance, as it would indicate a non zero Lorentz force between the magnetic field generated by a stationary current and a charge, 2
1
Introduction
Generally the mass of the photon is taken to be zero. What is not so well known is the fact that a photon with a non zero mass does not contradict established theory, though experiments have provided upper limits to such a mass. These upper limits have become more and more stringent and presently a good estimate seems to be 10−57 gms. The author’s work has shown that, on theoretical grounds, the photon should have a mass ∼ 10−65 gms [1], which is below the experimental limit. We will come back to the theoretical framework which suggests the above photon mass, but before that we will discuss some experimental tests which can confirm the above results. Indeed it must be mentioned that already experiments suggest a non vanishing photon mass.
2 2 −1/2 /c ] E = hν = mν c2 [1 − vγ
(2)
From (2) one would have a dispersive group velocity for waves of frequency ν given by (Cf. also ref.[2]) vγ = c 1 −
arXiv:0706.3319v1 [physics.gen-ph] 22 Jun 2007
On the Photon Mass
B.G. Sidharth∗ Frankfurt Institute of Advanced Studies Max Von Laue Strasse 1, D-60438, Frankfurt am Main, Germany ∗ Permanent Address: International Institute for Applicable Mathematics & Information Sciences Hyderabad (India) & Udine (Italy) B.M. Birla Science Centre, Adarsh Nagar, Hyderabad - 500 063 (India)
1ห้องสมุดไป่ตู้
2
Experiments and Results
1. Laboratory tests have suggested that Maxwell’s displacement current is a real phenomenon [2, 3], which leads to the fact that vacuum contains a dissipative mechanism or friction, which again leads to a non zero photon mass. This was achieved by Bartlete and Corle by using squids which enable them to directly measure the magnetic field inside a thin circular parallel plate capacitor, as it was being charged. 2. We now briefly describe an experiment which so far has yielded limits [4], in agreement with other experimental limits. In this experiment, described by Lakes an influence of large cosmic magnetic vector fields on massive photons can be measured in the laboratory via the energy density of µγ A2 , where µγ is the Compton wavelength of the photon. A modified Cavendish balance was used for this purpose. A toroid of electrical steel was wound with a current carrying wire and supported by water floatation. Stability and a restoring torque was provided by a tungsten wire. A fine copper wire provided an electrical return path. Further a magnetic shield of MU metal was added to try and eliminate noise due to magnetic field fluctuations. The operative relation is given by µ2 γ |Aambient | =
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