OSCILLATIONS AND WAVES CYU 13

Q13: Doppler Effect on Intensity

Physics Problem: Intensity & Doppler Effect

Question 13

A point source emits sound isotropically at constant power $P$. Sound travels with velocity $c$. Find the expression for intensity $I$ at a distance $r$ when:
(a) Detector moves with $v_d$ towards stationary source.
(b) Source moves with $v_s$ towards stationary detector.
(c) Both move towards each other with $v_s$ and $v_d$.

S’ (at t=0) S (now) v_s Detector v_d R = ct (Emission Distance) r (Current Distance) v_s t

Solution

The intensity of sound $I$ is defined as the energy received per unit area per unit time. It can be expressed as: $$ I = u \cdot v_{rel} $$ Where:
• $u$ is the Energy Density (Joules/m³) at the detector’s location.
• $v_{rel}$ is the speed of the wave relative to the detector (rate of interception).

Part (a): Source Stationary, Detector Moving ($v_d$)

1. Energy Density ($u$):
For a stationary source, energy spreads spherically. At distance $r$: $$ u = \frac{I_{static}}{c} = \frac{P}{4\pi r^2 c} $$ 2. Relative Speed ($v_{rel}$):
The detector moves towards the source against the wave direction. $$ v_{rel} = c + v_d $$ 3. Intensity ($I$):
$$ I_a = u \cdot (c + v_d) = \frac{P}{4\pi r^2 c}(c + v_d) $$ $$ I_a = \frac{P}{4\pi r^2} \left( 1 + \frac{v_d}{c} \right) $$

Part (b): Source Moving ($v_s$), Detector Stationary

1. Geometry of Emission:
Let $t$ be the time taken for the wave to travel from emission point to detector.
• Radius of wavefront: $R = c t$.
• Distance source moved: $d = v_s t$.
• Current distance (given): $r = R – d = (c – v_s)t$.
From this, we find the “Emission Radius” $R$ in terms of current distance $r$: $$ t = \frac{r}{c – v_s} \implies R = c \left( \frac{r}{c – v_s} \right) = \frac{r}{1 – v_s/c} $$ 2. Energy Density ($u$):
The energy $P$ is spread over a sphere of radius $R$ (not $r$). Additionally, the “shell” of energy is compressed by the Doppler factor $(1 – v_s/c)$. The derivation leads to: $$ u = \frac{P (1 – v_s/c)}{4\pi r^2 c} $$ *(Why? Because $u \propto \frac{1}{R^2} \times \text{Compression}$. The $1/R^2$ term dominates the increase from compression.)* 3. Intensity ($I$):
Detector is stationary, so $v_{rel} = c$. $$ I_b = u \cdot c = \frac{P (1 – v_s/c)}{4\pi r^2 c} \cdot c $$ $$ I_b = \frac{P}{4\pi r^2} \left( 1 – \frac{v_s}{c} \right) $$

Part (c): Both Moving Towards Each Other

We combine the effects found in (a) and (b).
1. The moving source establishes an energy density field $u$ described in part (b).
2. The moving detector intercepts this field with relative velocity $v_{rel}$ described in part (a). $$ I_c = u_{source\_moving} \cdot (c + v_d) $$ $$ I_c = \left[ \frac{P}{4\pi r^2 c} \left( 1 – \frac{v_s}{c} \right) \right] \cdot (c + v_d) $$ $$ I_c = \frac{P}{4\pi r^2} \left( 1 – \frac{v_s}{c} \right) \left( 1 + \frac{v_d}{c} \right) $$

(a) $ I = \frac{P}{4\pi r^2} \left( 1 + \frac{v_d}{c} \right) $

(b) $ I = \frac{P}{4\pi r^2} \left( 1 – \frac{v_s}{c} \right) $

(c) $ I = \frac{P}{4\pi r^2} \left( 1 + \frac{v_d}{c} \right) \left( 1 – \frac{v_s}{c} \right) $