📚 IB Physics: 250 IA Ideas and Formula Derivation | IB物理：250个IA想法与公式推导
The IB Physics Internal Assessment (IA) is an opportunity for students to design and conduct their own experiment, analyze data, and draw conclusions. A successful IA depends on a well‑chosen topic that links clearly to syllabus concepts. This article presents a curated collection of 250 Physics IA ideas grouped by topic, and for each group it demonstrates how to derive the key formulas that will underpin the experimental investigation. Understanding the theoretical background is essential, not only to formulate a meaningful research question but also to linearize data and extract valid conclusions. Let’s explore these ideas and their formula derivations, turning curiosity into measurable scientific inquiry.
IB 物理内部评估（IA）是学生设计并开展实验、分析数据、得出结论的绝佳机会。一份成功的 IA 依赖于一个与课程概念紧密相关的选题。本文整理了 250 个物理 IA 想法并按主题分组，对每组都演示了如何推导支撑实验研究的关键公式。理解理论背景至关重要，这不仅能帮助构建有意义的研究问题，还能让数据线性化并得出有效结论。让我们一起来探索这些想法及其公式推导，把好奇心转化为可测量的科学探究。
1. Introduction to IA and Formula Derivation | IA与公式推导导论
Before diving into specific topics, it is important to recognise that every IB Physics IA must be built on a clear physical model. The derivation of the working formula – the equation that connects the independent and dependent variables – is the first major step after choosing a topic. Often, the raw theoretical relationship is nonlinear; by applying mathematical manipulations you can transform it into a straight‑line equation y = mx + c. This “linearisation” makes it possible to use graphical analysis to extract constants and validate the model. For example, a simple pendulum’s period T relates to length L by T = 2π√(L/g). Squaring both sides gives T² = (4π²/g) L, so a graph of T² versus L yields a slope that allows determination of g. We will see many such transformations throughout this guide.
在深入具体课题之前，重要的是认识到每一个 IB 物理 IA 都必须建立在清晰的物理模型之上。工作公式——即连接自变量与因变量的方程——的推导是选定主题后的首要步骤。原始的理论关系通常是非线性的；通过数学变换，可将其化为直线方程 y = mx + c。这种“线性化”使得利用图像分析来提取常数并验证模型成为可能。例如，单摆的周期 T 与摆长 L 的关系为 T = 2π√(L/g)。两边平方得到 T² = (4π²/g) L，因此作 T²‑L 图所得的斜率可用于测定 g。本指南中将看到许多类似变换。
2. Mechanics: From Simple Pendulum to Conservation of Energy | 力学：从单摆到能量守恒
Mechanics offers a vast playground for IA investigations. Consider a pendulum: the restoring force is F = -mg sin θ. For small angles, sin θ ≈ θ, so the equation of motion becomes a = -(g/L) x, giving simple harmonic motion with period T = 2π√(L/g). To find g, you can linearise as described. Another classic idea is investigating the coefficient of kinetic friction using a block sliding down an inclined plane. The net acceleration a = g(sin θ – μ cos θ). By measuring a for different incline angles and plotting a vs. sin θ, the slope yields g and the intercept reveals μ. For projectile motion, the range R = (v₀² sin 2θ)/g; verifying this relationship by varying launch angle shows a peak at 45°, and plotting R vs. sin 2θ should give a straight line. Each derivation starts from first principles like Newton’s laws or conservation of energy.
力学为 IA 探索提供了广阔天地。以单摆为例：回复力为 F = -mg sin θ。小角度下 sin θ ≈ θ，运动方程化为 a = -(g/L) x，得到简谐运动，周期 T = 2π√(L/g)。为求 g，可按前述方式线性化。另一个经典设想是研究斜面上滑块的动摩擦因数。滑块的净加速度 a = g(sin θ – μ cos θ)。通过测量不同倾角 θ 下的加速度，并作 a‑sin θ 图，斜率给出 g，截距显示出 μ。对于抛体运动，射程 R = (v₀² sin 2θ)/g；通过改变发射角验证该关系，可以看到 45° 取得最大值，而作 R‑sin 2θ 图应得到一条直线。每一推导都从牛顿定律或能量守恒等第一原理出发。
3. Thermal Physics: Newton’s Law of Cooling and Ideal Gas Equation | 热物理：牛顿冷却定律与理想气体状态方程
Thermal IA ideas often centre on heat transfer or gas behaviour. Newton’s law of cooling states that the rate of temperature change of a body is proportional to the difference between its temperature and the ambient temperature: dT/dt = -k (T – Tₐ). Solving this differential equation yields T(t) = Tₐ + (T₀ – Tₐ) e⁻ᵏᵗ. By taking natural logs, ln(T – Tₐ) = ln(T₀ – Tₐ) – k t, which is a linear form if you plot ln(T – Tₐ) against time t. The slope gives the cooling constant k. Alternatively, you can explore Boyle’s law PV = constant. For a fixed amount of gas at constant temperature, plotting P versus 1/V yields a straight line. Similarly, Charles’s law V/T = constant can be tested by measuring gas volume at different temperatures and extrapolating to absolute zero.
热学 IA 构想常围绕热传递或气体行为。牛顿冷却定律指出，物体的温度变化率正比于其温度与环境温度之差：dT/dt = -k (T – Tₐ)。解此微分方程得 T(t) = Tₐ + (T₀ – Tₐ) e⁻ᵏᵗ。取自然对数后，ln(T – Tₐ) = ln(T₀ – Tₐ) – k t，若作 ln(T – Tₐ) 对时间 t 的图，便可得到线性形式，斜率为冷却常数 k。另一方案是探究玻意耳定律 PV = 常量。对一定量气体保持恒温，作 P‑1/V 图可得直线。类似地，查理定律 V/T = 常量可通过测量不同温度下气体体积并外推到绝对零度来检验。
4. Waves: Standing Wave Patterns and Doppler Shift | 波：驻波图案与多普勒频移
Investigations on waves are both visual and mathematically rich. A classic IA involves standing waves on a string fixed at both ends. The wavelength λ of the nth harmonic is λ = 2L/n, and the wave speed v = f λ. Combining with v = √(T/μ) (where T is tension, μ linear density) yields f = (n/2L)√(T/μ). If you vary tension and measure frequency for a fixed harmonic, a graph of f² versus T gives a straight line, and the slope allows μ to be found. For sound waves in a resonant tube (closed at one end), the resonant lengths obey L = (2n-1)λ/4, so by plotting L against 1/f you can determine the speed of sound. Doppler shift for a moving source f’ = f (v / (v – uₛ)) can be tested using a smartphone app to measure frequency shift of a moving buzzer; the derived formula can be linearised by plotting 1/f’ against uₛ to extract the speed of sound v.
波的研究可视化效果好且蕴含丰富数学。经典的 IA 实验是研究两端固定的弦上的驻波。第 n 次谐波的波长 λ = 2L/n，波速 v = f λ。结合 v = √(T/μ)（T 为张力，μ 为线密度）得 f = (n/2L)√(T/μ)。若改变张力并测量固定谐波的频率，作 f²‑T 图可得直线，由其斜率可求出 μ。对一端封闭的共鸣管，共振长度满足 L = (2n-1)λ/4，因此作 L 对 1/f 图可测定声速。对于运动声源的多普勒效应 f’ = f (v / (v – uₛ))，可利用智能手机 App 测量移动蜂鸣器的频率变化，通过作 1/f’ 对 uₛ 的图来线性化，从而提取声速 v。
5. Electricity: Ohm’s Law, Kirchhoff’s Rules and RC Circuits | 电学：欧姆定律、基尔霍夫定律与 RC 电路
Electric circuits offer endless IA possibilities. A simple resistance investigation can verify Ohm’s law V = IR and the rules for series and parallel resistors. For a nichrome wire, resistance R = ρ L / A, where ρ is resistivity. Varying L and measuring R, a plot of R vs. L yields ρ from the slope. More advanced is the discharge of a capacitor through a resistor: the voltage across the capacitor obeys V(t) = V₀ e⁻ᵗ/ᴿᶜ. Taking natural logs gives ln V = ln V₀ – (1/RC) t, a straight line with slope -1/RC. Alternatively, charging a capacitor follows V = V₀ (1 – e⁻ᵗ/ᴿᶜ), which can be rearranged as ln(V₀ – V) = ln V₀ – t/RC. In internal resistance experiments, the terminal voltage V = ε – I r, so a graph of V vs. I gives the EMF ε as intercept and internal resistance r as the magnitude of the slope.
电路为 IA 提供了无穷可能。基本的电阻探究可验证欧姆定律 V = IR 以及串并联电阻规则。对镍铬合金丝，电阻 R = ρ L / A，其中 ρ 为电阻率。改变 L 测量 R，作 R‑L 图，斜率可求 ρ。更进阶的是电容器通过电阻放电：电容两端电压遵循 V(t) = V₀ e⁻ᵗ/ᴿᶜ。取自然对数得 ln V = ln V₀ – (1/RC) t，为一直线，斜率为 -1/RC。电容器充电过程满足 V = V₀ (1 – e⁻ᵗ/ᴿᶜ)，可改写为 ln(V₀ – V) = ln V₀ – t/RC。在测量电源内阻的实验中，端电压 V = ε – I r，因此作 V‑I 图，纵截距为电动势 ε，斜率的绝对值为内阻 r。
6. Magnetism and Electromagnetic Induction | 磁学与电磁感应
Magnetism investigations often involve the force on a current‑carrying wire in a magnetic field, given by F = B I L sin θ. By placing a magnet on a balance and varying current I through a wire segment, you can measure the change in apparent weight and thus the force. A plot of F vs. I yields a straight line whose slope equals B L sin θ, which can be used to determine B. Faraday’s law of induction ε = -N dΦ/dt can be investigated by dropping a magnet through a coil. The induced EMF peak is proportional to the speed of the magnet. More precisely, the flux change depends on the magnet’s strength and coil geometry. A square‑wave relationship emerges when analysing the time‑dependence; plotting peak EMF against the velocity at entry, which is controlled by drop height, gives a linear relation that confirms the law. Eddy current braking can also be studied: a magnet sliding down an aluminium ramp experiences a drag force proportional to velocity, leading to a terminal velocity.
磁学的探究常涉及载流导线在磁场中的受力，由 F = B I L sin θ 给出。将磁铁置于电子天平上，改变导线中的电流 I，可测量表观重量变化即力。作 F‑I 图得一直线，斜率为 B L sin θ，可用于确定 B。法拉第感应定律 ε = -N dΦ/dt 可通过使磁铁穿过线圈来研究。感应电动势峰值与磁铁速度成正比。更精确地说，磁通变化取决于磁铁强度与线圈几何。分析时间依赖关系会呈现方波特征；绘制峰值电动势对进入速度（由下落高度控制）的图，可得线性关系，验证该定律。还可研究涡流制动：磁铁沿铝质斜面下滑受到与速度成正比的阻力，从而出现收尾速度。
7. Optics: Interference, Diffraction and Snell’s Law | 光学：干涉、衍射与斯涅尔定律
Double‑slit interference is a favourite IA: the fringe spacing Δy = λ D / d, where D is the slit‑to‑screen distance and d is slit separation. By varying D and measuring Δy, a graph of Δy vs. D produces a straight line with slope λ/d, so with known d, λ can be found. For single‑slit diffraction, the width of the central maximum w = 2λ D / a. Plotting w vs. D again allows the wavelength to be determined. Refraction experiments using Snell’s law n₁ sin θ₁ = n₂ sin θ₂ can be used to determine the refractive index of a liquid or glass block. A graph of sin θ₁ versus sin θ₂ yields a straight line through origin whose slope is n₂/n₁. More creative ideas involve measuring the focal length of a lens using the lens equation 1/f = 1/u + 1/v and linearising by plotting 1/v vs. 1/u, or investigating Malus’s law I = I₀ cos²θ for polarisers.
双缝干涉是热门的 IA：条纹间距 Δy = λ D / d，其中 D 为缝到屏距离，d 为缝距。改变 D 并测量 Δy，作 Δy‑D 图得一直线，斜率为 λ/d，若已知 d 可求 λ。单缝衍射中，中央亮纹宽度 w = 2λ D / a。同样作 w‑D 图可测定波长。使用斯涅尔定律 n₁ sin θ₁ = n₂ sin θ₂ 的折射实验可用于测定液体或玻璃块的折射率。作 sin θ₁ 对 sin θ₂ 的图得过原点的直线，斜率为 n₂/n₁。更具创造性的构想包括利用透镜公式 1/f = 1/u + 1/v，作 1/v‑1/u 图线性化求焦距，或者探究偏振片的马吕斯定律 I = I₀ cos²θ。
8. Nuclear Physics: Radioactive Decay and Absorption | 核物理：放射性衰变与吸收
Radioactive decay follows N = N₀ e⁻λt. The decay constant λ is related to half‑life by λ = ln 2 / T₁/₂. The activity A = λ N, so A = A₀ e⁻λt. A standard IA involves measuring the background‑corrected count rate of a short‑lived isotope and plotting ln A vs. time to obtain λ. Absorption of gamma radiation follows I = I₀ e⁻μx, where x is absorber thickness and μ is the linear attenuation coefficient. A semi‑log plot of ln I vs. x gives μ. One can then compare the measured μ with the theoretical value or investigate the dependence on energy. The inverse‑square law for gamma radiation: intensity I = k / r². By plotting I against 1/r², a straight line confirms the relationship. Combining these concepts, you might design an IA to find the half‑value thickness of different materials.
放射性衰变遵循 N = N₀ e⁻λt。衰变常量 λ 与半衰期的关系为 λ = ln 2 / T₁/₂。活度 A = λ N，因此 A = A₀ e⁻λt。典型的 IA 包括测量短寿命同位素扣除本底后的计数率，并作 ln A‑t 图求 λ。伽马辐射的吸收符合 I = I₀ e⁻μx，其中 x 为吸收体厚度，μ 为线性衰减系数。作 ln I‑x 半对数图可得 μ。随后可将实验 μ 与理论值比较或探究其能量依赖性。伽马辐射的平方反比定律：强度 I = k / r²。通过作 I‑1/r² 图可得直线，确证关系。结合这些概念，可以设计 IA 来求不同材料的半值厚度。
9. Energy and Environment: Solar Panels and Wind Power | 能源与环境：太阳能板与风能
Energy‑related IA topics are highly relevant. For a photovoltaic cell, the power output depends on the load resistance and light intensity. The maximum power point occurs when the load matches the internal resistance. A common experiment: under constant illumination, vary the external resistance R and measure voltage V and current I. Power is P = IV. A plot of P vs. R reveals the optimum resistance; linearisation is not always straightforward here, but you can analyse the I‑V characteristic to determine the fill factor. Wind turbine models: the power extracted by a turbine is P = ½ ρ A v³ Cₚ, where ρ is air density, A swept area, v wind speed, Cₚ performance coefficient. Testing with a small fan and turbine, you can measure the electrical power output for different wind speeds. Plotting P against v³ yields a straight line; the slope gives ½ ρ A Cₚ.
与能源相关的 IA 主题颇具现实意义。对于光伏电池，输出功率取决于负载电阻和光强。最大功率点出现在负载与内阻匹配时。常见实验：在恒定光照下，改变外接电阻 R，测量电压 V 和电流 I。功率 P = IV。作 P‑R 图可找出最佳电阻，虽然此处线性化不总是直接，但可通过分析 I‑V 特性来确定填充因子。风力发电机模型：涡轮机提取的功率为 P = ½ ρ A v³ Cₚ，其中 ρ 为空气密度，A 为扫风面积，v 为风速，Cₚ 为性能系数。用小风扇和发电机进行测试，可测量不同风速下的电输出功率。作 P‑v³ 图可得直线，斜率给出 ½ ρ A Cₚ。
10. Astrophysics: Inverse Square Law and Magnitudes | 天体物理：平方反比定律与星等
Astrophysics offers beautiful IA ideas using simple equipment. Stellar brightness follows the inverse square law for apparent magnitude: the difference in magnitude Δm = m₂ – m₁ = -2.5 log₁₀(F₂/F₁). If you set up a light sensor and a bulb, the illuminance E = I / d², where d is distance. Therefore E ∝ 1/d². Plotting E against 1/d² gives a straight line. Relating to magnitude, you can define a reference distance and compute apparent magnitudes to verify the distance‑modulus formula. Another idea is stellar temperature determination: using a spectrometer or colour filters, measure the relative intensity at two wavelengths. Wien’s displacement law λ_max T = constant, and the ratio of intensities follows the Planck distribution. By plotting ln(I_red/I_blue) against 1/T (with T controlled by a variable power lamp), you can extract a linear relationship. Parallax simulation: using a parallax viewer, angle p ∝ 1/d, giving a direct verification of distance measurement.
天体物理中的 IA 想法能用简单器材完美实现。恒星亮度遵循视亮度的平方反比定律，星等差 Δm = m₂ – m₁ = -2.5 log₁₀(F₂/F₁)。若设置光传感器与灯泡，照度 E = I / d²，d 为距离。故 E ∝ 1/d²。作 E‑1/d² 图可得直线。联系星等概念，可定义参考距离并计算视星等以验证距离模数公式。另一构想是恒星温度测定：用光谱仪或滤色片测量两波长处的相对强度。维恩位移定律 λ_max T = 定值，强度比遵循普朗克分布。作 ln(I_red/I_blue) 对 1/T（T 由可变功率灯控制）的图，可提取线性关系。视差模拟：使用视差观察器，角度 p ∝ 1/d，直接验证距离测量。
11. Advanced Tips: Linearisation and Uncertainty | 进阶建议：线性化与不确定度
No matter which IA idea you pick, you will need to handle uncertainties and turn your raw data into a well‑analysed graph. Common linearisation techniques include: taking logs of both sides for exponential or power laws (log‑log or semi‑log plots), squaring, reciprocal, or other algebraic transformations. Always propagate uncertainties into the linearised quantities. If you plot y’ = k x’ + c, where y’ = f(y, x), the uncertainty in y’ must be calculated using the rules for combining uncertainties. Many students forget this and get inconsistent error bars. Also, carefully consider the assumptions in your derivation: e.g., small angle approximation, negligible air resistance, constant temperature. Mention them in your IA and discuss how they affect your results. Finally, don’t just list 250 ideas – pick one that you genuinely find interesting and for which you can obtain reliable data.
无论你选择哪个 IA 构念，都必须处理不确定度并将原始数据转化为经过细致分析的图表。常见的线性化手法包括：对指数或幂律关系取对数（双对数或半对数图）、平方、取倒数或其他代数变换。务必将不确定度传递到线性化后的量中。如果你画出 y’ = k x’ + c，其中 y’ = f(y, x)，y’ 的不确定度必须按不确定度合成公式计算。许多学生会忘掉这一步，导致误差棒不自洽。同时，仔细考量推导中的假设，如小角度近似、空气阻力可忽略、温度恒定等。在 IA 报告中提及它们并讨论其如何影响结果。最后，不要仅仅列出 250 个想法——选择一个你真正感兴趣且能获取可靠数据的主题。
12. Conclusion and Final Thoughts | 总结与思考
This tour through 250 IB Physics IA ideas has shown how formula derivation lies at the heart of every successful investigation. From mechanics to astrophysics, the same pattern emerges: begin with a fundamental law, manipulate the equation to reveal a linear relationship between measurable quantities, and then use the gradient and intercept to extract physical constants. Remember that a good IA is not about exotic apparatus but about clear thinking and rigorous analysis. Even simple experiments can yield excellent results when you understand the underlying theory. Use this resource as a springboard, select your topic, and dedicate time to planning your experimental method. The derivation steps you practice here will serve you not only in the IA but throughout your physics journey.
这次走过 250 个 IB 物理 IA 构思的旅程展示了公式推导如何成为每一项成功探究的核心。从力学到天体物理，相同的模式反复显现：从一个基本定律出发，对方程进行变换以揭示可测量量之间的线性关系，然后利用斜率和截距提取物理常数。记住，优秀的 IA 不在于仪器的花哨，而在于清晰的思维和严谨的分析。只要理解了背后的理论，哪怕很简单的实验也能产生出色的结果。请把这份资料当作跳板，选定你的主题，并花时间精心设计实验方法。你在此练习的推导步骤不但会服务于你的 IA，也将贯穿你的整个物理学习之旅。
Published by TutorHao | Physics Revision Series | aleveler.com
更多咨询请联系16621398022（同微信）
屏轩国际教育cambridge primary/secondary checkpoint, cat4, ukiset,ukcat,igcse,alevel,PAT,STEP,MAT, ibdp,ap,ssat,sat,sat2课程辅导，国外大学本科硕士研究生博士课程论文辅导Cancel reply