📚 Work and Energy in A-Level Physics | A2物理：功与能量 考点精讲
In A2 Physics, the concepts of work and energy form a cornerstone for understanding mechanics, fields, and thermodynamics. This article distils the essential principles, definitions, and problem-solving strategies required for A-Level examinations, covering work done by constant and variable forces, kinetic and potential energies, the work-energy theorem, conservation of energy, power, and efficiency. Clear explanations and paired bilingual paragraphs will help you master the topic and tackle exam questions confidently.
在A2物理中，功与能量的概念是理解力学、场和热力学的基石。本文提炼了A-Level考试所必需的基本原理、定义和解题策略，涵盖恒力与变力做功、动能与势能、动能定理、能量守恒、功率和效率。清晰的双语对照讲解将帮助你掌握该主题并自信地应对考题。
1. Definition of Work | 功的定义
e force. Quantitatively, work W is the scalar product of force F and displacement s: W = F s 1 J = 1 N m. If the force is perpendicular to the displacement (θ = 90°), no work is done.
在物理学中，当一个力使物体沿力的方向发生位移时，就说该力做了功。定量地，功 W 是力 F 与位移 s 的标量积：W = F s cosθ，其中 θ 是力矢量与位移矢量之间的夹角。功的单位是焦耳（J），1 J = 1 N m。如果力与位移垂直（θ = 90°），则不做功。
2. Work Done by a Constant Force | 恒力做功
ment, cosθ = 1 and W = F d. If the force opposes motion (e.g., friction), θ = 180°, cosθ = –1, so work is negative, meaning energy is taken away from the object.
当恒力作用于沿直线运动的物体时，做功可简单表示为 W = F d cosθ，其中 d 是位移大小。若力与位移平行，则 cosθ = 1，W = F d。若力阻碍运动（如摩擦力），θ = 180°，cosθ = –1，做功为负，意味着能量从物体中移走。
3. Work Done by a Varying Force | 变力做功
k done between two points is given by the integral W = ∫ F dx, or the area under the force–displacement graph. For a spring obeying Hooke' od is essential for non-constant forces such as those in gravitational or electric fields.
如果力随位置变化，两点间所做的功由积分 W = ∫ F dx 给出，或者等于力–位移图下的面积。对于遵守胡克定律（F = kx）的弹簧，将其从0拉伸至x所做的功为 W = ½ k x²。这种方法对于非恒力（如引力场或电场中的力）至关重要。
4. Kinetic Energy and the Work-Energy Theorem | 动能与动能定理
theorem states that the net work done on an object equals its change in kinetic energy: Wnet = ΔEₖ = ½ m vf² – ½ m vi². This principle is powerful for solving problems involving acceleration, deceleration, and friction without needing to calculate acceleration directly.
动能（Eₖ）是物体由于运动而具有的能量，定义为 Eₖ = ½ m v²。动能定理指出，物体所受合力做的净功等于其动能的变化量：Wnet = ΔEₖ = ½ m vf² – ½ m vi²。这一原理在求解涉及加速、减速和摩擦力的问题时非常有效，无需直接计算加速度。
5. Gravitational Potential Energy | 重力势能
Gravitational potential energy (Eₚ) arises from an object's position in a gravitational field. Near the Earth' a radial field, the potential energy of two masses M and m separated by distance r is U = – potential energy is the negative of the work done by gravity, and it is path-independent.
重力势能（Eₚ）源于物体在引力场中的位置。在地球表面附近，对于高度变化h，ΔEₚ = m g h。更一般地，在径向场中，两个质量M和m相距r时的势能为 U = –G M m / r。势能的变化等于重力做功的负值，且与路径无关。
6. Elastic Potential Energy | 弹性势能
ic potential energy is stored in deformed objects like springs. For a spring obeying Hooke' uilibrium is Eₑ = ½ k x². This assumes no energy is lost as heat. The area under the force– ph yields the same expression and is crucial for calculating energy stored before release.
弹性势能储存在如弹簧之类的变形物体中。对于遵从胡克定律的弹簧，当从平衡位置拉伸或压缩x时，储存的能量为 Eₑ = ½ k x²。假设没有能量以热的形式散失。力–伸长图下的面积给出了相同的表达式，这对计算释放前储存的能量非常重要。
7. Conservation of Mechanical Energy | 机械能守恒
In an isolated system where only conservative forces (gravity, elastic) do work, the total mechanical energy Etotal that any decrease in potential energy equals an increase in kinetic energy, and vice versa. The principle allows us to equate initial and final energy totals without considering the intermediate motion, as in pendulum or roller‑coaster problems.
在只有保守力（重力、弹力）做功的孤立系统中，总机械能 Etotal = Eₖ + Eₚ 保持不变。这意味着势能的减少等于动能的增加，反之亦然。该原理使我们能够直接将初态和末态的总能相等，无需考虑中间运动过程，例如在单摆或过山车问题中。
8. Power | 功率
Power P measures the rate at which work is done or energy is transferred. The average power is Pavg = 1 J s⁻¹. Power is a scalar quantity, and when force and velocity are parallel, P = F v.
功率 P 衡量做功或能量转移的快慢。平均功率为 Pavg = W / t 或 ΔE / t，瞬时功率则为 P = F v cosθ，其中v是力作用点的速度。国际单位是瓦特（W），1 W = 1 J s⁻¹。功率是标量，当力与速度平行时，P = F v。
9. Efficiency | 效率
the total energy input, often expressed as a percentage: η = (useful output / input) × 100% friction, air resistance, or electrical resistance, so efficiency is always less than 100%. Improving efficiency reduces energy waste.
效率 η 是有用功或能量输出与总能量输入的比值，通常以百分比表示：η = (有用输出 / 输入) × 100%。在实际系统中，由于摩擦、空气阻力或电阻，总有一部分能量以热的形式耗散，因此效率总是小于100%。提高效率可以减少能量浪费。
10. Energy Dissipation and Work Against Friction | 能量耗散与克服摩擦做功
Work done against friction converts mechanical energy into thermal energy (heat), raising the temperature of the surfaces. This dissipated energy is unrecoverable for doing useful work. The magnitude of work against a constant frictional force f over distance d is Wf = f d. In energy‑ this is often included as a negative term, reducing the total mechanical energy available.
克服摩擦所做的功将机械能转化为热能（热量），使接触面温度升高。这些耗散的能量无法再用于做有用功。对于恒定的摩擦力 f，移动距离 d 所做的功为 Wf = f d。在能量守恒方程中，这常作为负项加入，使得可用总机械能减少。
11. Energy Transfer Diagrams and Sankey Diagrams | 能量转移图与桑基图
at. The efficiency is the ratio of the useful output arrow width to the input arrow width.
可视化能量转移对于理解效率至关重要。桑基图使用箭头表示能量，其宽度代表能量的多少。输入能量分为有用输出和浪费的能量。例如，在白炽灯中，电能 → 光 + 热。效率即有用输出箭头宽度与输入箭头宽度之比。
12. Problem-Solving Strategies for Work and Energy | 功与能量解题策略
t by identifying a system and all forces. Determine whether forces are conservative or non‑ conservative forces, use conservation of mechanical energy: Eₖ₁ + Eₚ₁ = Eₖ₂ + Eₚ₂. If non‑conservative forces act, apply the work-energy theorem: Wnet = ΔEₖ, where Wnet is the sum of work by all forces, or recognise that the work by non‑conservative forces equals the change in total mechanical energy. Always draw free‑ ² appropriately, remembering that work done against friction is always negative. Using energy methods often avoids complicated kinematics.
首先确定系统和所有受力，判断力是保守力还是非保守力。对于只有保守力的问题，使用机械能守恒：Eₖ₁ + Eₚ₁ = Eₖ₂ + Eₚ₂。如果存在非保守力，则应用动能定理：Wnet = ΔEₖ，其中 Wnet 是所有力做功的代数和，或者认识到非保守力所做的功等于总机械能的变化量。始终画出受力分析图，并恰当地使用 ΔEₚ = mgh 或 ½ kx²，记住克服摩擦所做的功总是负的。使用能量方法常常可以避免复杂的运动学计算。
Published by TutorHao | Physics Revision Series | aleveler.com
更多咨询请联系16621398022（同微信）
或截图后用「扫一扫 → 相册」选择本图