Year 11 CAIE Physics: Quick Reference Handbook of Formulas & Theorems | Year 11 CAIE 物理:公式定理速查手册

📚 Year 11 CAIE Physics: Quick Reference Handbook of Formulas & Theorems | Year 11 CAIE 物理:公式定理速查手册

This handbook collates the essential formulas, theorems and principles for the CAIE IGCSE Physics (0625) syllabus – a rapid revision companion for Year 11 students. Every equation is presented with its units and a brief note on application, followed immediately by the Chinese equivalent to support bilingual learners.

本手册整理了 CAIE IGCSE 物理 (0625) 课程中的核心公式、定理与原理,是 Year 11 学生的快速复习伴侣。每个方程都配有单位和应用说明,并立即附上对应的中文解释,以便双语学习。


1. Kinematics – Motion in a Straight Line | 直线运动学

Kinematics deals with the description of motion without considering its causes. The four standard equations of uniformly accelerated motion are the backbone of this topic.

运动学只描述物体的运动,不涉及引起运动的原因。四个匀加速直线运动的基本方程是本节的核心。

v = u + at

Where v = final velocity (m/s), u = initial velocity (m/s), a = acceleration (m/s²), t = time (s).

其中 v 为末速度 (m/s),u 为初速度 (m/s),a 为加速度 (m/s²),t 为时间 (s)。

s = ut + ½at²

Here s is the displacement (m). This formula gives the distance travelled under constant acceleration.

这里 s 代表位移 (m)。该公式用于计算匀加速直线运动中的位移。

v² = u² + 2as

Useful when time is not given. Always remember that acceleration can be negative (deceleration).

在时间未知时很有用。请牢记加速度可取负值(减速)。

average speed = total distance / total time

For non-uniform motion, this defines the overall rate of movement.

对于非匀速运动,此式定义了整体的运动快慢。


2. Forces and Newton’s Laws | 力与牛顿定律

Forces govern the interaction between objects. Newton’s three laws provide the framework for understanding resultant forces and equilibrium.

力支配着物体之间的相互作用。牛顿三定律为我们理解合力与平衡提供了框架。

F = ma

Newton’s Second Law. F is the resultant force in newtons (N), m is mass in kg, a is acceleration in m/s². This vector equation means acceleration is in the direction of the net force.

牛顿第二定律。F 为合力 (N),m 为质量 (kg),a 为加速度 (m/s²)。这是一个矢量方程,加速度方向与合外力方向一致。

W = mg

Weight is the gravitational force on a mass. g is the gravitational field strength (≈ 9.8 N/kg on Earth).

重力是作用在物体上的万有引力。g 为重力场强度(地球表面约为 9.8 N/kg)。

Hooke’s Law: F = kx

Extension x (m) of a spring is directly proportional to the applied force F, up to the limit of proportionality. k is the spring constant (N/m).

弹簧的伸长量 x (m) 与外力 F 成正比,此关系在弹性限度内成立。k 为劲度系数 (N/m)。

Moment = Force × perpendicular distance from pivot

The principle of moments states that for a body in rotational equilibrium, total clockwise moment = total anticlockwise moment.

力矩 = 力 × 支点到力作用线的垂直距离。力矩原理指出,处于转动平衡的物体满足顺时针力矩之和等于逆时针力矩之和。


3. Momentum | 动量

Momentum helps analyse collisions and explosions. It is conserved in all isolated systems.

动量用于分析碰撞与爆炸过程,在任何孤立系统中动量守恒。

p = mv

Momentum p (kg·m/s) is the product of mass and velocity. It is a vector quantity.

动量 p (kg·m/s) 是质量与速度的乘积,为矢量。

F = Δp / Δt

Newton’s Second Law in terms of momentum: resultant force equals rate of change of momentum. This leads to the impulse equation.

用动量表述的牛顿第二定律:合力等于动量的变化率。由此可导出冲量方程。

Impulse = FΔt = Δ(mv)

Impulse (N·s) equals change in momentum. The area under a force–time graph gives impulse.

冲量 (N·s) 等于动量的变化量。力–时间图像下的面积表示冲量。

Conservation of momentum: m₁u₁ + m₂u₂ = m₁v₁ + m₂v₂

In the absence of external forces, total momentum before a collision equals total momentum after.

在没有外力作用时,碰撞前的总动量等于碰撞后的总动量。


4. Energy, Work and Power | 能量、功与功率

Energy can be stored or transferred. The principle of conservation of energy underpins all these calculations.

能量可以被储存或传递。能量守恒定律是所有这些计算的基础。

Work done = Fd cosθ

When a force moves an object through a displacement d in the direction of the force, work is done. In IGCSE, often θ = 0° and cosθ = 1. Unit: joule (J).

当力使物体沿力的方向移动一段位移 d 时,力做功。在 IGCSE 中,通常 θ = 0°,cosθ = 1。单位:焦耳 (J)。

Kinetic Energy: KE = ½mv²

Energy of a moving object.

物体由于运动而具有的能量。

Gravitational Potential Energy: GPE = mgh

Energy stored due to an object’s height h above a reference level.

物体因被举高 h 而储存的能量。

Efficiency = (useful energy output / total energy input) × 100%

Efficiency can also be calculated from power: (useful power output / total power input) × 100%.

效率也可用功率计算:(有用输出功率 / 输入总功率)× 100%。

Power = work done / time taken = energy transferred / time

Power P is measured in watts (W). 1 W = 1 J/s.

功率 P 的单位是瓦特 (W)。1 W = 1 J/s。


5. Pressure and Density | 压强与密度

Pressure is the force exerted per unit area. Density links mass and volume, and appears frequently in fluid statics.

压强是单位面积上受到的压力。密度将质量与体积联系起来,在流体静力学中经常出现。

Pressure p = F / A

Unit: pascal (Pa); 1 Pa = 1 N/m². The same force produces a higher pressure when the area is smaller.

单位:帕斯卡 (Pa);1 Pa = 1 N/m²。相同作用力下,受力面积越小,压强越大。

Pressure in a liquid: p = ρgh

ρ = density (kg/m³), g = gravitational field strength, h = depth (m). This pressure acts equally in all directions at a given depth.

ρ 为液体密度 (kg/m³),g 为重力场强度,h 为深度 (m)。在同一深度,液体向各个方向的压强相等。

Density ρ = m / V

Mass per unit volume. Units: kg/m³ or g/cm³.

单位体积的质量。单位:kg/m³ 或 g/cm³。


6. Thermal Physics | 热物理学

Temperature, heat and the behaviour of gases are governed by simple yet powerful relationships. Absolute temperature (kelvin) must be used in gas law calculations.

温度、热量和气体行为受一些简单而强大的关系支配。使用气体定律计算时必须采用绝对温度(开尔文)。

Specific heat capacity: Q = mcΔθ

Q is the thermal energy (J), m mass (kg), c specific heat capacity (J/(kg·°C) or J/(kg·K)), Δθ temperature change.

Q 为热量 (J),m 为质量 (kg),c 为比热容 (J/(kg·°C) 或 J/(kg·K)),Δθ 为温度变化。

Specific latent heat: Q = mL

During a change of state (melting/freezing, boiling/condensation), temperature stays constant. L is latent heat (J/kg).

在物态变化(熔化/凝固、沸腾/液化)过程中,温度保持不变。L 为潜热 (J/kg)。

Boyle’s Law: p₁V₁ = p₂V₁ (constant T)

For a fixed mass of gas at constant temperature, pressure and volume are inversely proportional.

对于一定质量的气体,在温度不变时,压强与体积成反比。

Charles’ Law: V₁/T₁ = V₂/T₂ (constant p)

Volume is directly proportional to absolute temperature when pressure is constant.

在压强不变时,体积与绝对温度成正比。

Pressure Law: p₁/T₁ = p₂/T₂ (constant V)

Pressure is directly proportional to absolute temperature at fixed volume.

在体积不变时,压强与绝对温度成正比。

Combined gas equation: pV/T = constant

For a fixed mass of gas, (p₁V₁)/T₁ = (p₂V₂)/T₂. Remember T must be in kelvin (K = °C + 273).

对于一定质量的气体,(p₁V₁)/T₁ = (p₂V₂)/T₂。注意温度单位必须为开尔文 (K = °C + 273)。


7. Wave Properties | 波的性质

Waves transfer energy without transferring matter. The universal wave equation links speed, frequency and wavelength.

波传递能量而不传递物质。通用波动方程将波速、频率和波长联系起来。

v = fλ

Wave speed v (m/s) = frequency f (Hz) × wavelength λ (m). This holds for all types of waves.

波速 v (m/s) = 频率 f (Hz) × 波长 λ (m)。此式适用于所有类型的波。

Frequency f = 1/T

The period T is the time for one complete oscillation (s).

周期 T 是完成一次全振动所需的时间 (s)。

For reflection, the angle of incidence equals the angle of reflection. Refraction obeys Snell’s law: n₁ sin i = n₂ sin r, but in IGCSE the qualitative relationships and critical angle calculations are key.

对于反射,入射角等于反射角。折射遵循斯涅尔定律:n₁ sin i = n₂ sin r,但 IGCSE 重点考察定性关系以及临界角的计算。

Critical angle: sin c = 1/n

n is the refractive index of the medium when light travels from the medium to air. Total internal reflection occurs when the angle of incidence exceeds the critical angle.

n 为光从该介质射向空气时的折射率。当入射角大于临界角时,发生全内反射。


8. Light and Lenses | 光与透镜

Lenses form real or virtual images. The magnification equation is essential for ray diagram verification.

透镜可成实像或虚像。放大率公式是验证光路图的重要工具。

Magnification = image height / object height = image distance / object distance

No sign convention is required in the core syllabus; use absolute distances for convex lens calculations.

核心课程中无需符号约定;凸透镜计算时使用绝对距离。

The principal focus of a converging lens is the point where rays parallel to the principal axis converge. For a diverging lens, they appear to diverge from the principal focus.

凸透镜的焦点是平行于主光轴的光线会聚的点。凹透镜的焦点是平行于主光轴的光线发散后反向延长线会聚的点。


9. Electricity and Circuits | 电与电路

Current, voltage and resistance are linked by Ohm’s law. Mastering series and parallel circuit rules is critical for problem-solving.

电流、电压和电阻由欧姆定律联系。掌握串联和并联电路的规律是解题的关键。

Ohm’s Law: V = IR

Potential difference V (V), current I (A), resistance R (Ω). Applies only when temperature remains constant.

电势差 V (V)、电流 I (A)、电阻 R (Ω)。仅在温度恒定条件下适用。

Resistance: R = V/I

The ratio of voltage to current defines resistance.

电压与电流之比定义为电阻。

Series circuits: Rₜₒₜ = R₁ + R₂ + …

Current is the same everywhere; the supply voltage divides across components.

电流处处相等;电源电压在各元件间分配。

Parallel circuits: 1/Rₜₒₜ = 1/R₁ + 1/R₂ + …

Voltage is the same across each branch; currents add up to the total current.

各支路电压相等;总电流为各支路电流之和。

Electrical power: P = IV = I²R = V²/R

Power in watts (W). The energy transferred is E = Pt = IVt.

功率单位为瓦特 (W)。消耗的电能 E = Pt = IVt。


10. Magnetism and Electromagnetism | 磁学与电磁学

Magnetic fields exert forces on moving charges and current-carrying conductors. Electromagnetic induction is the basis for generators and transformers.

磁场对运动电荷和载流导体会施加作用力。电磁感应是发电机与变压器的基础。

Motor effect force: F = BIL

F = force on a conductor (N), B = magnetic flux density (T), I = current (A), L = length of conductor in the field (m). The direction is given by Fleming’s left-hand rule.

F 为导体所受的力 (N),B 为磁通密度 (T),I 为电流 (A),L 为导体在磁场中的长度 (m)。方向由弗莱明左手定则判定。

Transformer equation: Vₚ/Vₛ = Nₚ/Nₛ

For an ideal transformer, the ratio of primary to secondary voltage equals the turns ratio. Step-up (Nₛ > Nₚ) increases voltage; step-down does the opposite.

对于理想变压器,原、副线圈电压比等于匝数比。升压变压器 (Nₛ > Nₚ) 提高电压,降压变压器则相反。

Transformer power: IₚVₚ = IₛVₛ (ideal)

Since power is conserved, a higher voltage on the secondary side means a smaller current.

由于功率守恒,副边电压升高意味着电流减小。


11. Atomic and Nuclear Physics | 原子与核物理

Radioactive decay follows a statistical law. The half-life concept and equations for nuclear reactions are fundamental.

放射性衰变遵循统计规律。半衰期的概念以及核反应方程是基础。

Alpha decay: A decreases by 4, Z decreases by 2

Example: \u00B2\u00B3\u2078U\u2082\u2082 → \u00B2\u00B3\u2074Th\u2082\u2080 + \u00B2He\u2082. The emitted alpha particle is a helium nucleus.

例如:²³⁸U₉₂ → ²³⁴Th₉₀ + ⁴He₂。发射的 α 粒子是氦原子核。

Beta-minus decay: A unchanged, Z increases by 1

A neutron becomes a proton, emitting a β⁻ particle (electron) and an antineutrino.

一个中子转变成质子,发射出一个 β⁻ 粒子(电子)和一个反中微子。

Half-life: fraction remaining = (1/2)^n, n = number of half-lives

The time taken for the activity (or number of undecayed nuclei) to fall to half its initial value is constant for a given isotope.

给定同位素的活度(或未衰变原子核数)降至初始值一半所需的时间是恒定的。

Nuclear fission and fusion

Fission is the splitting of a heavy nucleus into two lighter nuclei, releasing energy. Fusion is the joining of light nuclei to form a heavier nucleus, which powers the Sun.

裂变是一个重核分裂成两个较轻的核并释放能量。聚变是轻核结合成更重的核,为太阳提供能量。


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