IB Physics HL · 鼎睿学苑

Unit C.5: Doppler Effect单元 C.5:多普勒效应

The closing super-topic of Theme C "Wave behaviour". The pitch of a passing siren rises on approach and drops on recession because relative motion between source and observer compresses or stretches the wavefronts. This unit develops that idea from a qualitative picture into quantitative shift equations: the HL-only moving-source and moving-observer sound formulas, and the single low-speed light formula that underpins redshift, blueshift, the evidence for an expanding universe, radar speed guns, Doppler ultrasound, and sonar.主题 C"波的行为"的收官超主题。驶过的警笛在接近时音调升高、远离时音调降低,原因是波源与观察者之间的相对运动压缩或拉伸了波前。本单元把这一定性图像发展为定量的频移方程:HL 专属的波源运动与观察者运动声波公式,以及支撑红移、蓝移、宇宙膨胀证据、雷达测速、多普勒超声与声呐的单一低速光频移公式。

IB Physics · Theme C.5 · First Assessment 2025 Papers 1 · 2 6 Topics · SL + HL mix6 个核心专题 · SL + HL 混合

How to use this guide本指南使用说明

C.5 splits cleanly into three layers. The qualitative picture (wavefront bunching, pitch up on approach) is examinable for everyone. The explicit moving-source and moving-observer sound equations are HL only. The light shift $\frac{\Delta f}{f} \approx \frac{v}{c}$ is for everyone and drives the astrophysics applications. Marks are lost by mixing up which speed goes where and by getting the sign of the $\pm$ wrong, so the whole unit rewards drawing a clear "who is moving toward whom" diagram before reaching for a formula.C.5 清晰地分为三层。定性图像(波前堆积、接近时音调升高)人人都要考。显式的波源运动与观察者运动声波公式仅为 HL。光的频移 $\frac{\Delta f}{f} \approx \frac{v}{c}$ 人人都考,并支撑天体物理应用。失分往往来自把哪个速度放错位置,以及搞错 $\pm$ 的符号;因此本单元最看重在动笔前先画一张"谁朝谁运动"的示意图。

!
If you are cramming如果你在临阵磨枪

Approach $\Rightarrow$ higher frequency (pitch up, blueshift); recession $\Rightarrow$ lower frequency (pitch down, redshift). For sound (HL), moving source: $f' = f\frac{v}{v \pm v_s}$ (minus on approach). Moving observer: $f' = f\frac{v \pm v_o}{v}$ (plus on approach). For light at $v \ll c$: $\frac{\Delta f}{f} \approx \frac{\Delta\lambda}{\lambda} \approx \frac{v}{c}$.

接近 $\Rightarrow$ 频率升高(音调升高、蓝移);远离 $\Rightarrow$ 频率降低(音调降低、红移)。声波(HL)波源运动:$f' = f\frac{v}{v \pm v_s}$(接近取减号)。观察者运动:$f' = f\frac{v \pm v_o}{v}$(接近取加号)。光在 $v \ll c$ 时:$\frac{\Delta f}{f} \approx \frac{\Delta\lambda}{\lambda} \approx \frac{v}{c}$。

If you are going for a 7如果你目标是 7 分

Be able to derive the moving-source result from compressed wavelength $\lambda' = (v \pm v_s)/f$ and explain why moving source and moving observer give different formulas even for the same relative speed (the medium picks a rest frame for sound). Know that the light formula is symmetric in source/observer motion (no medium), and that the sign of $v$ is set by whether the separation is increasing (redshift) or decreasing (blueshift). State a sign convention every time.

能从压缩波长 $\lambda' = (v \pm v_s)/f$ 推导波源运动结果,并解释为何即使相对速度相同,波源运动与观察者运动给出不同公式(声波的介质选定了一个静止参考系)。要知道光的公式对波源/观察者运动是对称的(无介质),且 $v$ 的符号由间距是增大(红移)还是减小(蓝移)决定。每次都写明sign convention(符号约定)。

HL flagHL 标记说明 Sections C5.2 (moving source) and C5.3 (moving observer) develop the explicit Doppler equations for sound; these are HL extension content. SL students need the qualitative picture (C5.1), the light shift (C5.4), and the applications (C5.5, C5.6), but are not required to apply the moving-source / moving-observer sound formulas.C5.2(波源运动)与 C5.3(观察者运动)建立声波的显式多普勒方程;这些为 HL 扩展内容。SL 学生需要掌握定性图像(C5.1)、光的频移(C5.4)以及应用(C5.5、C5.6),但无需套用波源运动 / 观察者运动声波公式。

Wavefront Bunching and Why Pitch Shifts波前堆积与音调变化的原因 C.5 SL+HL

The core idea.
  • The Doppler effect is the change in observed frequency (and wavelength) of a wave when the source and observer move relative to one another.
  • Approach (separation decreasing): wavefronts bunch up $\Rightarrow$ shorter $\lambda$ $\Rightarrow$ higher $f$ $\Rightarrow$ higher pitch / blueshift.
  • Recession (separation increasing): wavefronts stretch out $\Rightarrow$ longer $\lambda$ $\Rightarrow$ lower $f$ $\Rightarrow$ lower pitch / redshift.
Key subtlety. The source still emits at its true frequency $f$; only the observed frequency $f'$ changes. The wave speed in the medium is unchanged — the bunching changes $\lambda$, and since $v = f\lambda$, a shorter $\lambda$ at fixed $v$ means a higher $f$.
核心思想。
  • 多普勒效应(Doppler effect)是当波源(source)与观察者(observer)相对运动时,观察到的波的频率(与波长)发生变化的现象。
  • 接近(间距减小):波前堆积 $\Rightarrow$ $\lambda$ 变短 $\Rightarrow$ $f$ 升高 $\Rightarrow$ 音调升高 / 蓝移。
  • 远离(间距增大):波前拉伸 $\Rightarrow$ $\lambda$ 变长 $\Rightarrow$ $f$ 降低 $\Rightarrow$ 音调降低 / 红移。
关键细节。波源仍以其真实频率 $f$ 发声;只有观察到的频率 $f'$ 改变。介质中的波速不变——堆积改变的是 $\lambda$,由 $v = f\lambda$,波速固定下 $\lambda$ 变短意味着 $f$ 升高。
Worked Example C5.1 (qualitative reasoning)C5.1 例题(定性推理)

An ambulance siren emits a steady tone. As it drives past a stationary listener at constant speed, describe what the listener hears, and state the frequency relative to the emitted frequency $f$ both before and after the ambulance passes.救护车警笛发出稳定音调。当它以恒定速度驶过一名静止的听者时,描述听者所听到的声音,并说明在救护车经过前后所听频率相对于发射频率 $f$ 的关系。

Identify. The relevant quantity is the line-of-sight relative motion between source and observer.

识别。关键量是波源与观察者之间沿视线方向的相对运动。

Set up. Before passing, the ambulance is approaching: separation decreases, wavefronts bunch, $\lambda$ shortens. After passing, it is receding: separation increases, wavefronts stretch, $\lambda$ lengthens.

列式。经过前,救护车正在接近:间距减小,波前堆积,$\lambda$ 变短。经过后正在远离:间距增大,波前拉伸,$\lambda$ 变长。

Execute. Before passing, $f' > f$ (higher pitch, roughly constant). After passing, $f' < f$ (lower pitch). At the exact moment of passing, the motion is momentarily perpendicular to the line of sight, so $f' \approx f$.

求解。经过前,$f' > f$(音调偏高、大致恒定)。经过后,$f' < f$(音调偏低)。在恰好经过的瞬间,运动暂时垂直于视线,故 $f' \approx f$。

Evaluate. The listener hears a sudden drop in pitch as the ambulance passes — not a continuous rise. The pitch is high-then-low, with the change concentrated near passing.

评估。听者在救护车经过时听到音调骤降——不是连续升高。音调是先高后低,变化集中在经过附近。

Going deeper: it is the line-of-sight component that matters深入:起作用的是视线方向分量

The Doppler shift depends only on the component of relative velocity along the line joining source and observer (the radial component). A source moving in a circle around the observer at constant radius produces no shift, because its radial velocity is always zero even though its speed is large.

多普勒频移只取决于相对速度沿波源与观察者连线方向(径向)的分量。绕观察者做等半径圆周运动的波源产生频移,因为其径向速度始终为零,尽管速率很大。

This is why an aircraft flying tangentially overhead shows the strongest pitch drop just as it crosses directly above you: that is when the radial velocity swings fastest from $+v$ (approaching) through $0$ to $-v$ (receding).

这就是为何切向飞过头顶的飞机在它恰好越过你正上方时音调降得最明显:此刻径向速度从 $+v$(接近)经 $0$ 最快地摆到 $-v$(远离)。

A car horn sounds as the car drives toward a stationary pedestrian at constant speed. Compared with the emitted frequency $f$, the pedestrian hears:汽车朝静止行人匀速行驶时鸣笛。与发射频率 $f$ 相比,行人听到的频率:
C5.1 · Q1
A lower frequency, because the sound spreads out较低,因为声音扩散
A higher frequency, because the wavefronts bunch up较高,因为波前堆积
Exactly $f$, since the car emits at $f$恰为 $f$,因为车以 $f$ 发声
A higher frequency only because the sound is louder较高,仅因为声音更响
Approach means decreasing separation, so each successive wavefront is emitted closer to the observer than the last. The wavefronts bunch, $\lambda$ shortens, and since $v = f\lambda$ at fixed wave speed, $f'$ rises.接近意味着间距减小,于是每个相继的波前比前一个更靠近观察者。波前堆积,$\lambda$ 变短,由波速固定下 $v = f\lambda$,故 $f'$ 升高。
Loudness (amplitude) and pitch (frequency) are independent. On approach the wavefronts bunch, shortening $\lambda$ and raising $f'$ above $f$.响度(振幅)与音调(频率)相互独立。接近时波前堆积,$\lambda$ 变短,$f'$ 高于 $f$。
A whistle is whirled in a horizontal circle on a string. A listener stands far away in the plane of the circle. The listener hears:哨子系在绳上做水平圆周运动。一名听者远站在圆所在平面内。听者听到:
C5.1 · Q2
A steadily rising pitch持续升高的音调
A constant pitch above the emitted one高于发射音调的恒定音调
No change at all, since the whistle never gets closer完全不变,因为哨子从不靠近
A pitch that rises and falls once per revolution每转一圈起伏一次的音调
Over each revolution the whistle moves toward the listener for half the circle (radial velocity toward, blueshift, pitch up) and away for the other half (recession, redshift, pitch down). The pitch oscillates once per revolution.每转一圈,哨子有半圈朝听者运动(径向速度向内、蓝移、音调升高),另半圈远离(远离、红移、音调降低)。音调每圈起伏一次。
Only the radial (line-of-sight) component of velocity Doppler-shifts the sound. It swings from toward to away each revolution, so the pitch rises and falls once per turn.只有径向(视线方向)速度分量产生多普勒频移。它每圈在朝向与远离之间往复,故音调每圈起伏一次。

Moving Source, Stationary Observer波源运动、观察者静止 HL C.5 HL

The data-booklet equation HL. For a source of true frequency $f$ moving at speed $v_s$ through a medium in which the wave speed is $v$, a stationary observer hears f' = f v / (v ± v_s): $$ f' = f\,\frac{v}{v \pm v_s}. $$ Sign rule. Use the minus sign when the source moves toward the observer (denominator smaller $\Rightarrow$ $f' > f$, blueshift). Use plus when the source moves away ($f' < f$, redshift). Why. The source chases its own wavefronts, so the emitted wavelength ahead is compressed to $\lambda' = (v \pm v_s)/f$.
数据手册公式 HL对于真实频率为 $f$、以速率 $v_s$ 在波速为 $v$ 的介质中运动的波源,静止观察者听到 f' = f v / (v ± v_s): $$ f' = f\,\frac{v}{v \pm v_s}. $$ 符号规则。当波源观察者运动时取减号(分母变小 $\Rightarrow$ $f' > f$,蓝移)。当波源远离时取加号($f' < f$,红移)。 原因。波源追赶自己的波前,故前方发出的波长被压缩为 $\lambda' = (v \pm v_s)/f$。
Worked Example C5.2 (moving source)C5.2 例题(波源运动)

A train sounds a $400\ \mathrm{Hz}$ whistle and moves toward a stationary observer at $30\ \mathrm{m\,s^{-1}}$. The speed of sound is $340\ \mathrm{m\,s^{-1}}$. Find the frequency the observer hears, then the frequency after the train has passed and is receding at the same speed.火车鸣 $400\ \mathrm{Hz}$ 汽笛,以 $30\ \mathrm{m\,s^{-1}}$ 朝静止观察者运动。声速为 $340\ \mathrm{m\,s^{-1}}$。求观察者听到的频率,以及火车经过后以同速远离时的频率。

Identify. Source moving, observer stationary $\Rightarrow$ use the HL moving-source equation f' = f v / (v ± v_s).

识别。波源运动、观察者静止 $\Rightarrow$ 用 HL 波源运动公式 f' = f v / (v ± v_s)

Approaching (minus sign).

接近(取减号)。

$$ f' = 400 \times \frac{340}{340 - 30} = 400 \times \frac{340}{310} \approx 439\ \mathrm{Hz}. $$

Receding (plus sign).

远离(取加号)。

$$ f' = 400 \times \frac{340}{340 + 30} = 400 \times \frac{340}{370} \approx 368\ \mathrm{Hz}. $$

Evaluate. The observer hears the pitch jump from about $439\ \mathrm{Hz}$ to about $368\ \mathrm{Hz}$ as the train passes — a drop of roughly $71\ \mathrm{Hz}$. Note the shifts are not symmetric: the rise on approach ($+39$) exceeds the fall on recession ($-32$), a hallmark of the moving-source case.

评估。火车经过时观察者听到音调由约 $439\ \mathrm{Hz}$ 跳到约 $368\ \mathrm{Hz}$——下降约 $71\ \mathrm{Hz}$。注意频移并不对称:接近时升高($+39$)大于远离时降低($-32$),这是波源运动情形的特征。

Going deeper: deriving $f' = f v/(v - v_s)$ from compressed wavefronts深入:由压缩波前推导 $f' = f v/(v - v_s)$

In one period $T = 1/f$ the source emits one wavefront and itself advances a distance $v_s T$ toward the observer. The next wavefront is emitted from that advanced position. So ahead of the source, successive wavefronts are separated not by $\lambda = vT$ but by

在一个周期 $T = 1/f$ 内,波源发出一个波前,自身朝观察者前进 $v_s T$。下一个波前从前进后的位置发出。因此在波源前方,相继波前的间距不再是 $\lambda = vT$,而是

$$ \lambda' = vT - v_s T = (v - v_s)\,T = \frac{v - v_s}{f}. $$

The observer still measures the wave travelling at speed $v$, so the frequency received is

观察者测得的波速仍为 $v$,故接收频率为

$$ f' = \frac{v}{\lambda'} = \frac{v}{(v - v_s)/f} = f\,\frac{v}{v - v_s}. $$

Replacing $v_s \to -v_s$ for a receding source gives the $+$ version. This derivation shows clearly that what changes is the wavelength, not the wave speed in the medium.

对远离的波源用 $v_s \to -v_s$ 即得 $+$ 形式。该推导清楚表明:改变的是波长,而非介质中的波速。

HL A siren of frequency $1000\ \mathrm{Hz}$ approaches a stationary observer at $34\ \mathrm{m\,s^{-1}}$ ($v_{\text{sound}} = 340\ \mathrm{m\,s^{-1}}$). Observed frequency:HL $1000\ \mathrm{Hz}$ 警笛以 $34\ \mathrm{m\,s^{-1}}$ 接近静止观察者($v_{\text{声}} = 340\ \mathrm{m\,s^{-1}}$)。观察到的频率:
C5.2 · Q1
$1111\ \mathrm{Hz}$
$900\ \mathrm{Hz}$
$1100\ \mathrm{Hz}$
$1034\ \mathrm{Hz}$
Moving source approaching $\Rightarrow$ minus sign: $f' = 1000 \times \frac{340}{340 - 34} = 1000 \times \frac{340}{306} \approx 1111\ \mathrm{Hz}$.波源接近 $\Rightarrow$ 取减号:$f' = 1000 \times \frac{340}{340 - 34} = 1000 \times \frac{340}{306} \approx 1111\ \mathrm{Hz}$。
Use $f' = f v/(v - v_s)$ with the minus sign for approach. Putting $v_s$ in the numerator or adding it instead are the common traps.用 $f' = f v/(v - v_s)$,接近取减号。把 $v_s$ 放到分子或改成加法是常见陷阱。
HL Why is the pitch increase on approach larger than the pitch decrease on recession for a moving source at the same speed?HL 为何同速波源接近时音调升高量大于远离时降低量?
C5.2 · Q2
The sound is louder on approach接近时声音更响
The wave speed increases on approach接近时波速增大
$v_s$ appears in the denominator, so $-v_s$ and $+v_s$ shift $f'$ by unequal amounts$v_s$ 在分母,故 $-v_s$ 与 $+v_s$ 对 $f'$ 的改变量不相等
The frequency emitted by the source changes波源发射的频率改变
Because $f' = f v/(v \pm v_s)$ has $v_s$ in the denominator, the function is nonlinear: $\frac{v}{v - v_s}$ rises faster than $\frac{v}{v + v_s}$ falls. The relation is not symmetric in $v_s$, unlike the moving-observer case.由于 $f' = f v/(v \pm v_s)$ 中 $v_s$ 在分母,函数是非线性的:$\frac{v}{v - v_s}$ 升高得比 $\frac{v}{v + v_s}$ 降低得快。该关系对 $v_s$ 不对称,与观察者运动情形不同。
Wave speed and emitted frequency are both unchanged. The asymmetry comes purely from $v_s$ sitting in the denominator of $f' = f v/(v \pm v_s)$.波速与发射频率都不变。不对称纯粹源于 $v_s$ 位于 $f' = f v/(v \pm v_s)$ 的分母。

Moving Observer, Stationary Source观察者运动、波源静止 HL C.5 HL

The data-booklet equation HL. For an observer moving at speed $v_o$ through the medium toward (or away from) a stationary source of frequency $f$, with wave speed $v$, the observed frequency is f' = f (v ± v_o) / v: $$ f' = f\,\frac{v \pm v_o}{v}. $$ Sign rule. Use plus when the observer moves toward the source ($f' > f$); use minus when moving away ($f' < f$). Combined case. Source and observer both moving: $$ f' = f\,\frac{v \pm v_o}{v \pm v_s}. $$ Pick each sign so that approach raises $f'$.
数据手册公式 HL观察者以速率 $v_o$ 在介质中朝(或离)频率为 $f$ 的静止波源运动,波速为 $v$,则观察频率为 f' = f (v ± v_o) / v: $$ f' = f\,\frac{v \pm v_o}{v}. $$ 符号规则。观察者波源运动取加号($f' > f$);远离减号($f' < f$)。 组合情形。波源与观察者都运动: $$ f' = f\,\frac{v \pm v_o}{v \pm v_s}. $$ 取号原则:接近使 $f'$ 升高。
Worked Example C5.3 (moving observer, then combined)C5.3 例题(观察者运动,再组合)

A stationary loudspeaker emits a $500\ \mathrm{Hz}$ tone. A cyclist rides toward it at $10\ \mathrm{m\,s^{-1}}$ ($v_{\text{sound}} = 340\ \mathrm{m\,s^{-1}}$). (a) Find the frequency the cyclist hears. (b) Now suppose the speaker is itself carried toward the cyclist at $10\ \mathrm{m\,s^{-1}}$ while the cyclist still rides toward it at $10\ \mathrm{m\,s^{-1}}$; find the new frequency.静止扬声器发出 $500\ \mathrm{Hz}$ 音调。骑车者以 $10\ \mathrm{m\,s^{-1}}$ 朝它骑行($v_{\text{声}} = 340\ \mathrm{m\,s^{-1}}$)。(a) 求骑车者听到的频率。(b) 若扬声器本身也以 $10\ \mathrm{m\,s^{-1}}$ 朝骑车者运动,而骑车者仍以 $10\ \mathrm{m\,s^{-1}}$ 朝它骑行,求新频率。

Identify (a). Observer moving toward stationary source $\Rightarrow$ f' = f (v + v_o)/v with the plus sign.

识别 (a)。观察者朝静止波源运动 $\Rightarrow$ f' = f (v + v_o)/v,取加号。

$$ f' = 500 \times \frac{340 + 10}{340} = 500 \times \frac{350}{340} \approx 515\ \mathrm{Hz}. $$

Identify (b). Both moving toward each other $\Rightarrow$ combined formula, plus on top (observer approaches), minus on bottom (source approaches).

识别 (b)。两者相向运动 $\Rightarrow$ 组合公式,分子取加号(观察者接近),分母取减号(波源接近)。

$$ f' = 500 \times \frac{340 + 10}{340 - 10} = 500 \times \frac{350}{330} \approx 530\ \mathrm{Hz}. $$

Evaluate. Even though both speeds are $10\ \mathrm{m\,s^{-1}}$, the moving-observer shift ($+15\ \mathrm{Hz}$) and the moving-source contribution differ slightly because the formulas are different. Sound, unlike light, is not symmetric in which body moves: the medium defines a rest frame.

评估。尽管两速率都是 $10\ \mathrm{m\,s^{-1}}$,观察者运动的频移($+15\ \mathrm{Hz}$)与波源运动的贡献略有不同,因为公式不同。声波(不同于光)对"谁运动"不对称:介质定义了一个静止参考系。

Going deeper: why moving observer adds, moving source divides深入:为何观察者运动是相加、波源运动是相除

A moving observer does not change the wavelength in the medium — the wavefronts are still spaced by $\lambda = v/f$. What changes is the rate at which the observer sweeps through them. Moving toward the source at $v_o$, the observer meets wavefronts at the relative speed $v + v_o$, so

运动的观察者不改变介质中的波长——波前间距仍为 $\lambda = v/f$。改变的是观察者掠过波前的速率。以 $v_o$ 朝波源运动时,观察者以相对速度 $v + v_o$ 遇到波前,故

$$ f' = \frac{v + v_o}{\lambda} = \frac{v + v_o}{v/f} = f\,\frac{v + v_o}{v}. $$

A moving source instead changes $\lambda$ itself (Section C5.2), which is why $v_s$ enters in the denominator. Same relative speed, different physics — and the two formulas only coincide to first order in $v/v_{\text{sound}}$.

而运动的波源改变的是 $\lambda$ 本身(见 C5.2),这就是 $v_s$ 进入分母的原因。相同相对速度、不同物理——两个公式仅在 $v/v_{\text{声}}$ 的一阶近似下一致。

HL A listener runs away from a stationary $660\ \mathrm{Hz}$ siren at $20\ \mathrm{m\,s^{-1}}$ ($v_{\text{sound}} = 340\ \mathrm{m\,s^{-1}}$). The frequency heard is:HL 听者以 $20\ \mathrm{m\,s^{-1}}$ 远离静止的 $660\ \mathrm{Hz}$ 警笛($v_{\text{声}} = 340\ \mathrm{m\,s^{-1}}$)。听到的频率:
C5.3 · Q1
$700\ \mathrm{Hz}$
$621\ \mathrm{Hz}$
$660\ \mathrm{Hz}$
$640\ \mathrm{Hz}$
Observer moving away $\Rightarrow$ minus sign: $f' = 660 \times \frac{340 - 20}{340} = 660 \times \frac{320}{340} \approx 621\ \mathrm{Hz}$.观察者远离 $\Rightarrow$ 取减号:$f' = 660 \times \frac{340 - 20}{340} = 660 \times \frac{320}{340} \approx 621\ \mathrm{Hz}$。
Moving observer uses $f' = f(v \pm v_o)/v$; receding takes the minus sign in the numerator, so $f' < f$.观察者运动用 $f' = f(v \pm v_o)/v$;远离时分子取减号,故 $f' < f$。
HL A source and observer both move directly toward each other at the same speed $u$ through still air. Compared with the source-only-moving case (observer at rest), the combined observed frequency is:HL 波源与观察者在静止空气中以相同速率 $u$ 相向运动。与仅波源运动(观察者静止)相比,组合观察频率:
C5.3 · Q2
Exactly the same完全相同
Lower更低
Higher更高
Cannot be compared without numbers无数据无法比较
Combined: $f' = f\frac{v + u}{v - u}$. Source-only: $f' = f\frac{v}{v - u}$. Since $v + u > v$, the combined result is higher — the observer's own approach adds further blueshift on top of the source's.组合:$f' = f\frac{v + u}{v - u}$。仅波源:$f' = f\frac{v}{v - u}$。由于 $v + u > v$,组合结果更高——观察者自身的接近在波源蓝移之上叠加了更多蓝移。
Combined $f' = f\frac{v+u}{v-u}$ vs source-only $f\frac{v}{v-u}$: the extra $+u$ in the numerator makes the combined frequency higher.组合 $f' = f\frac{v+u}{v-u}$ 对比仅波源 $f\frac{v}{v-u}$:分子多出的 $+u$ 使组合频率更高。

Doppler Shift for Electromagnetic Waves电磁波的多普勒频移 C.5 SL+HL

The low-speed light equation. For a source and observer with relative speed $v \ll c$ along the line of sight, the data booklet gives Δf / f ≈ Δλ / λ ≈ v / c: $$ \frac{\Delta f}{f} \approx \frac{\Delta\lambda}{\lambda} \approx \frac{v}{c}. $$ What is symmetric. Light needs no medium, so only the relative velocity matters — moving source and moving observer give the same shift. There is one formula, not two. Signs. Recession (separation increasing) $\Rightarrow$ $\lambda$ increases (redshift). Approach $\Rightarrow$ $\lambda$ decreases (blueshift). $\Delta\lambda = \lambda_{\text{obs}} - \lambda_{\text{rest}}$.
低速光公式。当波源与观察者沿视线方向的相对速率 $v \ll c$ 时,数据手册给出 Δf / f ≈ Δλ / λ ≈ v / c: $$ \frac{\Delta f}{f} \approx \frac{\Delta\lambda}{\lambda} \approx \frac{v}{c}. $$ 对称之处。光不需要介质,故只有相对速度起作用——波源运动与观察者运动给出相同频移。只有一个公式,而非两个。 符号。远离(间距增大)$\Rightarrow$ $\lambda$ 增大(红移)。接近 $\Rightarrow$ $\lambda$ 减小(蓝移)。$\Delta\lambda = \lambda_{\text{obs}} - \lambda_{\text{rest}}$。
Worked Example C5.4 (spectral line shift)C5.4 例题(谱线频移)

A hydrogen line with rest wavelength $656.3\ \mathrm{nm}$ is observed from a distant galaxy at $658.5\ \mathrm{nm}$. Taking $c = 3.00\times10^{8}\ \mathrm{m\,s^{-1}}$, find the radial speed of the galaxy and state whether it is approaching or receding.某谱线静止波长 $656.3\ \mathrm{nm}$ 的氢线,从遥远星系观测为 $658.5\ \mathrm{nm}$。取 $c = 3.00\times10^{8}\ \mathrm{m\,s^{-1}}$,求该星系的径向速度,并说明是接近还是远离。

Identify. Light source, small shift $\Rightarrow$ use Δλ/λ ≈ v/c.

识别。光源、小频移 $\Rightarrow$ 用 Δλ/λ ≈ v/c

Compute the shift. $\Delta\lambda = 658.5 - 656.3 = 2.2\ \mathrm{nm}$. The wavelength has increased, so this is a redshift (recession).

计算频移。$\Delta\lambda = 658.5 - 656.3 = 2.2\ \mathrm{nm}$。波长增大,故为红移(远离)。

$$ v \approx c\,\frac{\Delta\lambda}{\lambda} = (3.00\times10^{8}) \times \frac{2.2}{656.3} \approx 1.0\times10^{6}\ \mathrm{m\,s^{-1}}. $$

Evaluate. The galaxy recedes at about $1.0\times10^{6}\ \mathrm{m\,s^{-1}}$, roughly $0.3\%$ of $c$. Since $v \ll c$, the low-speed approximation is well justified.

评估。星系以约 $1.0\times10^{6}\ \mathrm{m\,s^{-1}}$ 远离,约为 $c$ 的 $0.3\%$。由于 $v \ll c$,低速近似完全成立。

Going deeper: why $\Delta f/f$ and $\Delta\lambda/\lambda$ have opposite signs but equal magnitude深入:为何 $\Delta f/f$ 与 $\Delta\lambda/\lambda$ 符号相反但大小相等

For light in vacuum $c = f\lambda$ is fixed, so $f\lambda = \text{const}$. Differentiating, $\lambda\,\Delta f + f\,\Delta\lambda \approx 0$, hence

真空中光满足 $c = f\lambda$ 恒定,即 $f\lambda = \text{常数}$。微分得 $\lambda\,\Delta f + f\,\Delta\lambda \approx 0$,于是

$$ \frac{\Delta f}{f} \approx -\frac{\Delta\lambda}{\lambda}. $$

The magnitudes match (both $\approx v/c$), but a redshift means $\Delta\lambda > 0$ and $\Delta f < 0$. The data-booklet line $\frac{\Delta f}{f} \approx \frac{\Delta\lambda}{\lambda} \approx \frac{v}{c}$ is a magnitude statement; in problems you decide red vs blue from the physical direction of motion. This formula is the non-relativistic limit — for $v$ comparable to $c$ the full relativistic Doppler formula is needed, but the IB course stays at $v \ll c$.

两者大小相等(都约 $v/c$),但红移意味着 $\Delta\lambda > 0$ 而 $\Delta f < 0$。数据手册的 $\frac{\Delta f}{f} \approx \frac{\Delta\lambda}{\lambda} \approx \frac{v}{c}$ 是大小关系式;解题时由运动的物理方向判断红/蓝。该公式是非相对论极限——当 $v$ 接近 $c$ 时需用完整的相对论多普勒公式,但 IB 课程停留在 $v \ll c$。

A spectral line of rest wavelength $500\ \mathrm{nm}$ is seen at $500.1\ \mathrm{nm}$. The source's radial speed ($c = 3.0\times10^{8}\ \mathrm{m\,s^{-1}}$) is about:静止波长 $500\ \mathrm{nm}$ 的谱线被观测为 $500.1\ \mathrm{nm}$。波源径向速率($c = 3.0\times10^{8}\ \mathrm{m\,s^{-1}}$)约为:
C5.4 · Q1
$6.0\times10^{3}\ \mathrm{m\,s^{-1}}$
$6.0\times10^{5}\ \mathrm{m\,s^{-1}}$
$3.0\times10^{8}\ \mathrm{m\,s^{-1}}$
$6.0\times10^{4}\ \mathrm{m\,s^{-1}}$
$\Delta\lambda = 0.1\ \mathrm{nm}$. $v \approx c\,\Delta\lambda/\lambda = (3.0\times10^{8})(0.1/500) = (3.0\times10^{8})(2\times10^{-4}) = 6.0\times10^{4}\ \mathrm{m\,s^{-1}}$.$\Delta\lambda = 0.1\ \mathrm{nm}$。$v \approx c\,\Delta\lambda/\lambda = (3.0\times10^{8})(0.1/500) = 6.0\times10^{4}\ \mathrm{m\,s^{-1}}$。
Use $v \approx c\,\Delta\lambda/\lambda$. Here $\Delta\lambda/\lambda = 0.1/500 = 2\times10^{-4}$, so $v = 2\times10^{-4} c = 6.0\times10^{4}\ \mathrm{m\,s^{-1}}$.用 $v \approx c\,\Delta\lambda/\lambda$。此处 $\Delta\lambda/\lambda = 0.1/500 = 2\times10^{-4}$,故 $v = 2\times10^{-4} c = 6.0\times10^{4}\ \mathrm{m\,s^{-1}}$。
Unlike sound, the light Doppler shift depends only on the relative velocity of source and observer because:与声波不同,光的多普勒频移只取决于波源与观察者的相对速度,因为:
C5.4 · Q2
Light needs no medium, so there is no preferred rest frame to break the symmetry光不需要介质,故无优先静止参考系来破坏对称性
Light travels faster than sound光比声音传播得快
Light has no wavelength光没有波长
Observers cannot move at light speed观察者不能以光速运动
Sound's two formulas differ because air provides a rest frame: "source moving" and "observer moving" are physically distinct relative to the air. Light propagates in vacuum with no medium, so only the relative velocity is defined, and one symmetric formula results.声波两个公式不同是因为空气提供了静止参考系:"波源运动"与"观察者运动"相对空气在物理上不同。光在真空中传播无介质,故只定义相对速度,给出一个对称公式。
The key is the absence of a medium. With no rest frame, only relative velocity is meaningful, so moving source and moving observer cannot be distinguished.关键在于没有介质。没有静止参考系,只有相对速度有意义,故波源运动与观察者运动无法区分。

Astronomical Evidence for an Expanding Universe宇宙膨胀的天文证据 C.5 SL+HL

Definitions.
  • Redshift: observed $\lambda$ longer than rest $\lambda$ ($\Delta\lambda > 0$) $\Rightarrow$ source receding.
  • Blueshift: observed $\lambda$ shorter than rest $\lambda$ ($\Delta\lambda < 0$) $\Rightarrow$ source approaching.
The galactic evidence. Spectral lines from almost all distant galaxies are redshifted, and (Hubble) the more distant the galaxy, the greater the redshift $\Rightarrow$ the faster it recedes. This is the central observational pillar of an expanding universe. Caution. Cosmological redshift is strictly due to the expansion of space itself; the recession-speed reading via $v \approx c\,\Delta\lambda/\lambda$ is a good model only for nearby galaxies with $v \ll c$.
定义。
  • 红移(redshift):观测 $\lambda$ 长于静止 $\lambda$($\Delta\lambda > 0$)$\Rightarrow$ 波源远离。
  • 蓝移(blueshift):观测 $\lambda$ 短于静止 $\lambda$($\Delta\lambda < 0$)$\Rightarrow$ 波源接近。
星系证据。几乎所有遥远星系的谱线都红移,且(哈勃)星系越远红移越大 $\Rightarrow$ 退行越快。这是宇宙膨胀的核心观测支柱。 注意。宇宙学红移严格来说源于空间本身的膨胀;用 $v \approx c\,\Delta\lambda/\lambda$ 读取退行速度仅对 $v \ll c$ 的邻近星系是好模型。
Worked Example C5.5 (galactic redshift)C5.5 例题(星系红移)

A calcium line of rest wavelength $393.4\ \mathrm{nm}$ appears redshifted to $401.2\ \mathrm{nm}$ in a galaxy's spectrum. (a) Find the recession speed. (b) State what this, together with similar measurements at many distances, is evidence for.某星系光谱中静止波长 $393.4\ \mathrm{nm}$ 的钙线红移至 $401.2\ \mathrm{nm}$。(a) 求退行速度。(b) 说明这一结果连同许多不同距离上的类似测量能作为什么证据。

Identify. Redshift of a light source $\Rightarrow$ v ≈ c Δλ/λ.

识别。光源红移 $\Rightarrow$ v ≈ c Δλ/λ

Shift. $\Delta\lambda = 401.2 - 393.4 = 7.8\ \mathrm{nm}$, positive $\Rightarrow$ recession.

频移。$\Delta\lambda = 401.2 - 393.4 = 7.8\ \mathrm{nm}$,为正 $\Rightarrow$ 远离。

$$ v \approx c\,\frac{\Delta\lambda}{\lambda} = (3.00\times10^{8}) \times \frac{7.8}{393.4} \approx 5.9\times10^{6}\ \mathrm{m\,s^{-1}}. $$

Interpret (b). The galaxy recedes at about $5.9\times10^{6}\ \mathrm{m\,s^{-1}}$ ($\sim 2\%$ of $c$). The systematic redshift of distant galaxies, growing with distance, is direct evidence that the universe is expanding (the Big Bang picture).

解读 (b)。星系以约 $5.9\times10^{6}\ \mathrm{m\,s^{-1}}$ 退行(约 $c$ 的 $2\%$)。遥远星系普遍红移且随距离增大,是宇宙正在膨胀(大爆炸图景)的直接证据。

Going deeper: why we still see blueshift sometimes深入:为何有时仍能看到蓝移

Not everything is redshifted. The Andromeda galaxy, our nearest large neighbour, is blueshifted: its local gravitational pull toward the Milky Way exceeds the cosmological recession at such close range, so it is actually approaching us. Cosmological redshift only dominates for galaxies far enough that the expansion of space outruns local "peculiar" velocities.

并非一切都红移。仙女座星系是离我们最近的大邻居,呈蓝移:在如此近的距离上,它朝银河系的局部引力吸引超过宇宙学退行,故它实际上正在接近我们。宇宙学红移只在足够远、空间膨胀超过局部"本动"速度的星系上占主导。

In a binary star system, the two stars alternately approach and recede as they orbit, so their spectral lines shift back and forth periodically — a Doppler signature used to detect unseen companions, including exoplanets.

在双星系统中,两颗恒星随轨道运动交替接近与远离,其谱线周期性来回移动——这一多普勒特征被用来探测看不见的伴星,包括系外行星。

The spectral lines of a distant galaxy are all shifted toward longer wavelengths. This tells us the galaxy is:某遥远星系的谱线全部向更长波长移动。这说明该星系:
C5.5 · Q1
Approaching (blueshift)接近(蓝移)
Receding (redshift)远离(红移)
Stationary relative to us相对我们静止
Hotter than the Sun比太阳热
Longer observed wavelength means $\Delta\lambda > 0$: a redshift, which corresponds to recession. The systematic redshift of distant galaxies is the evidence for cosmic expansion.观测波长变长意味着 $\Delta\lambda > 0$:红移,对应远离。遥远星系普遍红移是宇宙膨胀的证据。
Longer wavelength = redshift = recession. Blueshift (shorter $\lambda$) would mean approach. Temperature is a separate property.波长变长 = 红移 = 远离。蓝移($\lambda$ 变短)才是接近。温度是另一个性质。
A binary star's spectral line oscillates periodically between slight redshift and slight blueshift. The best explanation is:一颗双星的谱线在轻微红移与轻微蓝移之间周期性振荡。最佳解释是:
C5.5 · Q2
The star is heating and cooling恒星在加热和冷却
The universe expands then contracts宇宙先膨胀后收缩
Orbital motion alternately moves the star toward then away from us轨道运动使恒星交替朝我们再远离
The star's true frequency changes with time恒星真实频率随时间改变
As the star orbits the common centre of mass, its radial velocity toward us reverses each half-period: approach (blueshift) then recede (redshift). The period of the line oscillation equals the orbital period — this is how spectroscopic binaries and many exoplanets are found.恒星绕共同质心运动时,其朝我们的径向速度每半周期反向:接近(蓝移)再远离(红移)。谱线振荡周期等于轨道周期——这正是发现分光双星与许多系外行星的方法。
A periodic back-and-forth shift signals periodic radial motion: orbital motion. Temperature and intrinsic frequency changes do not produce a clean periodic Doppler oscillation.周期性来回移动表明周期性径向运动:轨道运动。温度与固有频率变化不会产生干净的周期性多普勒振荡。

Radar Speed Guns, Doppler Ultrasound and Sonar雷达测速枪、多普勒超声与声呐 C.5 SL+HL

The double-shift trick. Most practical Doppler devices reflect a wave off a moving target. The target first acts as a moving observer (receives a shifted wave), then re-emits as a moving source (shifts it again). The two shifts add, so the round-trip fractional shift is twice the one-way value: $$ \frac{\Delta f}{f} \approx \frac{2v}{c}\ (\text{radar}), \qquad \frac{\Delta f}{f} \approx \frac{2v}{v_{\text{sound}}}\ (\text{ultrasound / sonar}). $$ Three workhorses. Radar speed gun: microwaves bounce off a car, $\Delta f$ gives speed. Doppler ultrasound: sound reflects off moving red blood cells to map blood-flow speed. Sonar: a moving ship or shoal of fish Doppler-shifts the returned ping.
双重频移技巧。多数实用多普勒装置都让波从运动目标反射。目标先充当运动的观察者(接收频移波),再作为运动的波源重新发射(再次频移)。两次频移相加,故往返的相对频移是单程值的两倍: $$ \frac{\Delta f}{f} \approx \frac{2v}{c}\ (\text{雷达}), \qquad \frac{\Delta f}{f} \approx \frac{2v}{v_{\text{声}}}\ (\text{超声 / 声呐}). $$ 三大典型应用。雷达测速枪:微波从车上反射,$\Delta f$ 给出速度。多普勒超声:声波从运动的红细胞反射以测血流速度。声呐:运动的船或鱼群使返回的脉冲发生多普勒频移。
Worked Example C5.6 (radar speed gun)C5.6 例题(雷达测速枪)

A police radar gun emits microwaves of frequency $24.0\ \mathrm{GHz}$ at a car driving directly toward it. The reflected beam returns shifted up by $4.0\ \mathrm{kHz}$. Taking $c = 3.0\times10^{8}\ \mathrm{m\,s^{-1}}$, find the car's speed.警用雷达枪向迎面驶来的汽车发射 $24.0\ \mathrm{GHz}$ 微波。反射波返回时频率升高 $4.0\ \mathrm{kHz}$。取 $c = 3.0\times10^{8}\ \mathrm{m\,s^{-1}}$,求车速。

Identify. Reflection off a moving target $\Rightarrow$ double shift: $\Delta f / f \approx 2v/c$.

识别。波从运动目标反射 $\Rightarrow$ 双重频移:$\Delta f / f \approx 2v/c$。

Rearrange for $v$.

解出 $v$。

$$ v \approx \frac{c\,\Delta f}{2 f} = \frac{(3.0\times10^{8})(4.0\times10^{3})}{2 \times (24.0\times10^{9})}. $$ $$ v \approx \frac{1.2\times10^{12}}{4.8\times10^{10}} = 25\ \mathrm{m\,s^{-1}} \approx 90\ \mathrm{km\,h^{-1}}. $$

Evaluate. The car travels at about $25\ \mathrm{m\,s^{-1}}$. Forgetting the factor of $2$ (treating it as a one-way shift) would double the reported speed — a classic exam trap.

评估。车速约 $25\ \mathrm{m\,s^{-1}}$。漏掉因子 $2$(当作单程频移)会使报出的速度翻倍——典型考试陷阱。

Going deeper: Doppler ultrasound and the cosine factor深入:多普勒超声与余弦因子

In medical Doppler ultrasound, a probe sends sound (typically a few $\mathrm{MHz}$) into tissue; it reflects off red blood cells moving at speed $v$ and returns shifted by $\Delta f \approx \frac{2 f v \cos\theta}{v_{\text{sound}}}$, where $\theta$ is the angle between the beam and the flow direction. The $\cos\theta$ appears because only the component of blood velocity along the beam Doppler-shifts the echo.

在医学多普勒超声中,探头向组织发出声波(通常几 $\mathrm{MHz}$);它从以速率 $v$ 运动的红细胞反射,返回时频移 $\Delta f \approx \frac{2 f v \cos\theta}{v_{\text{声}}}$,其中 $\theta$ 是声束与血流方向的夹角。出现 $\cos\theta$ 是因为只有沿声束方向的血流速度分量才产生多普勒频移。

Clinicians measure $\Delta f$, know $f$, $v_{\text{sound}}$ in tissue, and $\theta$, and solve for blood-flow speed $v$ — for example to detect a narrowed artery, where flow speeds up. This is the same physics as the radar gun, just with sound in tissue instead of microwaves in air.

临床上测出 $\Delta f$,已知 $f$、组织中 $v_{\text{声}}$ 与 $\theta$,即可解出血流速度 $v$——例如检测变窄的动脉(此处血流加速)。这与雷达枪是同样的物理,只是把空气中的微波换成组织中的声波。

A radar gun measures a fractional frequency shift $\Delta f/f$ on the reflected beam. The target's speed toward the gun is best estimated by:雷达枪测得反射波相对频移 $\Delta f/f$。目标朝雷达的速度最佳估计为:
C5.6 · Q1
$v \approx c\,\Delta f / f$
$v \approx 2 c\,\Delta f / f$
$v \approx \tfrac{1}{2} c\,\Delta f / f$
$v \approx c\,f / \Delta f$
Reflection gives a double shift $\Delta f/f \approx 2v/c$. Solving for $v$: $v \approx \tfrac{1}{2} c\,\Delta f/f$. The factor of one-half undoes the round-trip doubling.反射给出双重频移 $\Delta f/f \approx 2v/c$。解出 $v$:$v \approx \tfrac{1}{2} c\,\Delta f/f$。这个二分之一抵消了往返的加倍。
A reflected beam is shifted twice (target as observer, then as source), so $\Delta f/f \approx 2v/c$ and hence $v \approx \tfrac{1}{2} c\,\Delta f/f$.反射波被频移两次(目标先作观察者、再作波源),故 $\Delta f/f \approx 2v/c$,于是 $v \approx \tfrac{1}{2} c\,\Delta f/f$。
In Doppler ultrasound of blood flow, the returned echo from red blood cells moving toward the probe is:在血流多普勒超声中,朝探头运动的红细胞返回的回波:
C5.6 · Q2
Higher in frequency than the emitted ultrasound频率高于发射的超声
Lower in frequency than the emitted ultrasound频率低于发射的超声
Identical in frequency, only louder频率相同,只是更响
Converted to microwaves转化为微波
Cells approaching the probe act as a moving observer then a moving source, both raising the frequency. The echo returns blueshifted (higher $f$). Measuring $\Delta f$ gives the flow speed.朝探头运动的细胞先作运动观察者、再作运动波源,两者都使频率升高。回波返回时蓝移($f$ 更高)。测 $\Delta f$ 即得血流速度。
Approach raises frequency. The reflecting cells double-shift the echo upward, so the returned ultrasound has a higher frequency than emitted.接近使频率升高。反射的细胞使回波双重上移,故返回超声频率高于发射。

Exam Strategy and Common Pitfalls考试策略与常见陷阱

Get the sign right (every paper)取对符号(每张试卷)
  • Decide "approach or recede" first, then force the sign to match. Approach must give $f' > f$; recede must give $f' < f$. Check your $\pm$ against this before computing.
  • 先判断"接近还是远离",再让符号匹配。接近必须给出 $f' > f$;远离必须给出 $f' < f$。计算前先用此核对你的 $\pm$。
  • For sound, $v_s$ lives in the denominator and $v_o$ in the numerator. Putting them in the wrong place is the single most common C.5 error.
  • 声波中 $v_s$ 在分母、$v_o$ 在分子。放错位置是 C.5 最常见的单一错误。
Sound vs light HL声波与光 HL
  • The explicit $f' = f v/(v \pm v_s)$ and $f' = f(v \pm v_o)/v$ are HL and apply to sound only. SL questions stay qualitative for sound.
  • 显式的 $f' = f v/(v \pm v_s)$ 与 $f' = f(v \pm v_o)/v$ 属 HL,仅适用于声波。SL 对声波只考定性。
  • For light, never split into "source vs observer"; use the single $\Delta f/f \approx v/c$ with the relative speed.
  • 对光绝不区分"波源还是观察者";直接用单一的 $\Delta f/f \approx v/c$ 配相对速度。
Reflected-wave problems (factor of 2)反射波问题(因子 2)
  • Any "bounce off a moving target" device (radar, ultrasound, sonar) doubles the shift: $\Delta f/f \approx 2v/c$ or $2v/v_{\text{sound}}$.
  • 任何"从运动目标反射"的装置(雷达、超声、声呐)都使频移加倍:$\Delta f/f \approx 2v/c$ 或 $2v/v_{\text{声}}$。
  • Read the question: a one-way shift (a passing star) has no factor of 2; a reflected echo does.
  • 看清题意:单程频移(驶过的恒星)没有因子 2;反射回波有。
Units and approximations单位与近似
  • Keep wavelengths in consistent units; $\Delta\lambda/\lambda$ is dimensionless, so $\mathrm{nm}$ cancels $\mathrm{nm}$. Carry $c$ in $\mathrm{m\,s^{-1}}$.
  • 波长保持单位一致;$\Delta\lambda/\lambda$ 无量纲,$\mathrm{nm}$ 与 $\mathrm{nm}$ 相消。$c$ 用 $\mathrm{m\,s^{-1}}$。
  • The light formula is the $v \ll c$ limit. If a question gives $v$ near $c$, flag that the simple formula is only approximate.
  • 光公式是 $v \ll c$ 极限。若题目给出接近 $c$ 的 $v$,要指出简单公式只是近似。

Flashcards闪卡

0 / 12 flipped已翻 0 / 12
Doppler effect definition?多普勒效应定义?
Change in observed frequency/wavelength due to relative motion of source and observer.因波源与观察者相对运动引起的观察频率/波长变化。
Approach $\Rightarrow$ pitch?接近 $\Rightarrow$ 音调?
Higher $f$, shorter $\lambda$ (blueshift); wavefronts bunch.$f$ 升高、$\lambda$ 变短(蓝移);波前堆积。
Recession $\Rightarrow$ pitch?远离 $\Rightarrow$ 音调?
Lower $f$, longer $\lambda$ (redshift); wavefronts stretch.$f$ 降低、$\lambda$ 变长(红移);波前拉伸。
Moving source, sound? HL声波波源运动?HL
$$f' = f\,\frac{v}{v \pm v_s}$$Minus on approach.接近取减号。
Moving observer, sound? HL声波观察者运动?HL
$$f' = f\,\frac{v \pm v_o}{v}$$Plus on approach.接近取加号。
Combined source + observer? HL波源与观察者均运动?HL
$$f' = f\,\frac{v \pm v_o}{v \pm v_s}$$
Light Doppler, $v \ll c$?光多普勒,$v \ll c$?
$$\frac{\Delta f}{f} \approx \frac{\Delta\lambda}{\lambda} \approx \frac{v}{c}$$
Why one formula for light?光为何只有一个公式?
No medium $\Rightarrow$ no rest frame $\Rightarrow$ only relative velocity matters.无介质 $\Rightarrow$ 无静止参考系 $\Rightarrow$ 只有相对速度起作用。
Redshift means?红移意味着?
$\lambda$ increased ($\Delta\lambda > 0$); source receding.$\lambda$ 增大($\Delta\lambda > 0$);波源远离。
Galaxy redshift evidence for?星系红移是什么证据?
An expanding universe; more distant $\Rightarrow$ greater redshift.宇宙膨胀;越远 $\Rightarrow$ 红移越大。
Reflected-wave shift (radar)?反射波频移(雷达)?
$$\frac{\Delta f}{f} \approx \frac{2v}{c}$$Double shift on a bounce.反射使频移加倍。
Doppler ultrasound measures?多普勒超声测量?
Blood-flow speed from echo off moving red cells.由运动红细胞回波测血流速度。

Unit C.5 Practice Quiz单元 C.5 练习测验

As a fire engine drives past a stationary observer at constant speed, the observer hears the siren's pitch:消防车以恒定速度驶过静止观察者时,观察者听到警笛音调:
Q1
Rise continuously throughout全程持续升高
Stay high while approaching, then drop as it passes and recedes接近时偏高,经过并远离时降低
Fall continuously throughout全程持续降低
Stay exactly constant完全恒定
Approaching $\Rightarrow$ $f' > f$ (constant-ish high pitch); at passing the radial speed is zero ($f' \approx f$); receding $\Rightarrow$ $f' < f$. The listener hears a high tone then a sudden drop.接近 $\Rightarrow$ $f' > f$(大致偏高);经过时径向速度为零($f' \approx f$);远离 $\Rightarrow$ $f' < f$。听者先听高音再骤降。
The pitch is high (constant) on approach and low on recession, with the change concentrated at passing — not a continuous slide.音调在接近时偏高(恒定)、远离时偏低,变化集中在经过——不是连续滑变。
HL A $300\ \mathrm{Hz}$ source recedes from a stationary observer at $20\ \mathrm{m\,s^{-1}}$ ($v_{\text{sound}} = 340\ \mathrm{m\,s^{-1}}$). The observed frequency is:HL $300\ \mathrm{Hz}$ 波源以 $20\ \mathrm{m\,s^{-1}}$ 远离静止观察者($v_{\text{声}} = 340\ \mathrm{m\,s^{-1}}$)。观察频率:
Q2
$319\ \mathrm{Hz}$
$300\ \mathrm{Hz}$
$283\ \mathrm{Hz}$
$280\ \mathrm{Hz}$
Moving source receding $\Rightarrow$ plus sign: $f' = 300 \times \frac{340}{340 + 20} = 300 \times \frac{340}{360} \approx 283\ \mathrm{Hz}$.波源远离 $\Rightarrow$ 取加号:$f' = 300 \times \frac{340}{340 + 20} = 300 \times \frac{340}{360} \approx 283\ \mathrm{Hz}$。
Source receding uses $f' = f v/(v + v_s)$ with the plus sign, giving $f' < f$. Keep $v_s$ in the denominator.波源远离用 $f' = f v/(v + v_s)$,取加号,$f' < f$。$v_s$ 保持在分母。
A galaxy's $486.1\ \mathrm{nm}$ line is observed at $492.0\ \mathrm{nm}$. Its recession speed ($c = 3.0\times10^{8}\ \mathrm{m\,s^{-1}}$) is about:某星系 $486.1\ \mathrm{nm}$ 谱线被观测为 $492.0\ \mathrm{nm}$。退行速度($c = 3.0\times10^{8}\ \mathrm{m\,s^{-1}}$)约为:
Q3
$3.6\times10^{6}\ \mathrm{m\,s^{-1}}$
$3.6\times10^{7}\ \mathrm{m\,s^{-1}}$
$5.9\ \mathrm{m\,s^{-1}}$
$1.2\times10^{8}\ \mathrm{m\,s^{-1}}$
$\Delta\lambda = 492.0 - 486.1 = 5.9\ \mathrm{nm}$. $v \approx c\,\Delta\lambda/\lambda = (3.0\times10^{8})(5.9/486.1) \approx 3.6\times10^{6}\ \mathrm{m\,s^{-1}}$.$\Delta\lambda = 492.0 - 486.1 = 5.9\ \mathrm{nm}$。$v \approx c\,\Delta\lambda/\lambda = (3.0\times10^{8})(5.9/486.1) \approx 3.6\times10^{6}\ \mathrm{m\,s^{-1}}$。
Compute $\Delta\lambda/\lambda = 5.9/486.1 \approx 0.0121$, then $v \approx 0.0121 c \approx 3.6\times10^{6}\ \mathrm{m\,s^{-1}}$. Watch the power of ten.先算 $\Delta\lambda/\lambda = 5.9/486.1 \approx 0.0121$,再 $v \approx 0.0121 c \approx 3.6\times10^{6}\ \mathrm{m\,s^{-1}}$。注意数量级。
A sonar pulse of $40\ \mathrm{kHz}$ reflects off a submarine approaching at $10\ \mathrm{m\,s^{-1}}$ ($v_{\text{sound in water}} = 1500\ \mathrm{m\,s^{-1}}$). The frequency shift of the returned pulse is about:$40\ \mathrm{kHz}$ 声呐脉冲从以 $10\ \mathrm{m\,s^{-1}}$ 接近的潜艇反射(水中 $v_{\text{声}} = 1500\ \mathrm{m\,s^{-1}}$)。返回脉冲频移约为:
Q4
$130\ \mathrm{Hz}$
$0\ \mathrm{Hz}$
$270\ \mathrm{Hz}$
$530\ \mathrm{Hz}$
Reflection $\Rightarrow$ double shift: $\Delta f \approx f \cdot 2v/v_{\text{sound}} = (40\,000)\cdot\frac{2(10)}{1500} = 40\,000 \times 0.01333 \approx 530\ \mathrm{Hz}$.反射 $\Rightarrow$ 双重频移:$\Delta f \approx f \cdot 2v/v_{\text{声}} = (40\,000)\cdot\frac{2(10)}{1500} \approx 530\ \mathrm{Hz}$。
Use the factor of 2 for a reflected pulse: $\Delta f \approx 2 f v/v_{\text{sound}}$. Omitting the 2 halves the answer to $\approx 270\ \mathrm{Hz}$.反射脉冲用因子 2:$\Delta f \approx 2 f v/v_{\text{声}}$。漏掉 2 会得一半 $\approx 270\ \mathrm{Hz}$。
Which observation is the strongest single piece of evidence that the universe is expanding?哪一项观测是宇宙膨胀最有力的单一证据?
Q5
Stars twinkle at night夜晚星星闪烁
The Sun's spectrum has dark lines太阳光谱有暗线
Distant galaxies are systematically redshifted, more so the farther they are遥远星系系统性红移,越远红移越大
The Andromeda galaxy is blueshifted仙女座星系蓝移
The systematic redshift of distant galaxies — growing with distance — shows they recede ever faster, the signature of an expanding universe. Andromeda's blueshift is a local exception (it is gravitationally bound nearby), not evidence against expansion.遥远星系普遍红移且随距离增大,表明它们退行越来越快,这是宇宙膨胀的特征。仙女座蓝移是局部例外(引力束缚的近邻),并非反对膨胀的证据。
The key evidence is the distance-dependent redshift of galaxies. Twinkling (atmosphere), solar absorption lines, and one nearby blueshift are unrelated to cosmic expansion.关键证据是星系随距离增大的红移。闪烁(大气)、太阳吸收线与一个近邻蓝移都与宇宙膨胀无关。

Readiness Checklist备考清单

Tick each item when you can do it cold, without notes, on your first attempt.

每一条都要"裸做"做对(不看笔记、一次过)才打勾。

0 / 11 mastered已掌握 0 / 11

IB Paper-Style PracticeIB 试卷风格练习

C.5 Practice and Solutions are on the roadmap, to ship under Practice Questions/Unit_C5_*.html with the bilingual built-in pattern.

C.5 配套 Practice 与 Solutions 在排期,上线后位于 Practice Questions/Unit_C5_*.html