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Exercises · 14.10

Q.For the travelling harmonic wave
[!FORMULA] y(x,t)=2.0cos⁡2π(10t−0.0080 x+0.35)y(x, t) = 2.0 \cos 2\pi(10t - 0.0080\,x + 0.35)
where xx and yy are in cm and tt in s. Calculate the phase difference between oscillatory motion of two points separated by a distance of

(a) 4 m4\ \text{m},
(b) 0.5 m0.5\ \text{m},
(c) λ/2\lambda/2,
(d) 3λ/43\lambda/4
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The phase difference between two points on a travelling wave depends on their spatial separation and the wave's wavelength. We extract the wave number from the given equation to find the wavelength, then calculate the phase difference for each specified separation using Δϕ=2πλΔx\Delta\phi = \frac{2\pi}{\lambda} \Delta x. The phase differences are 6.4π6.4\pi, 0.8π0.8\pi, π\pi, and 3π/23\pi/2 radians for the respective separations.

A travelling harmonic wave describes how a disturbance propagates through a medium. The "phase" of the wave at a particular point in space and time tells us about the stage of its oscillation. For a travelling wave, the phase changes as you move along the direction of propagation (xx) and also as time (tt) progresses.

When we talk about the phase difference between two points, we are usually interested in how much one point "leads" or "lags" the other in its oscillatory motion at the same instant in time. This spatial phase difference is directly proportional to the distance separating the two points. If two points are separated by one full wavelength (λ\lambda), they are in phase, meaning their phase difference is 2π2\pi radians. If they are separated by half a wavelength (λ/2\lambda/2), they are exactly out of phase, with a phase difference of π\pi radians.

The general form of a travelling harmonic wave is often written as:

y(x,t)=Acos⁡(ωt−kx+ϕ0)y(x, t) = A \cos(\omega t - kx + \phi_0)

where:

  • AA is the amplitude.
  • ω\omega is the angular frequency (2πf2\pi f, where ff is the frequency).
  • kk is the wave number (2π/λ2\pi/\lambda, where λ\lambda is the wavelength).
  • ϕ0\phi_0 is the initial phase constant.

The argument of the cosine function, (ωt−kx+ϕ0)(\omega t - kx + \phi_0), is the phase of the wave at position xx and time tt.

For two points, x1x_1 and x2x_2, at the same time tt, their phases are:

ϕ1=ωt−kx1+ϕ0\phi_1 = \omega t - kx_1 + \phi_0

ϕ2=ωt−kx2+ϕ0\phi_2 = \omega t - kx_2 + \phi_0

The phase difference, Δϕ\Delta\phi, is then:

Δϕ=ϕ2−ϕ1=(ωt−kx2+ϕ0)−(ωt−kx1+ϕ0)\Delta\phi = \phi_2 - \phi_1 = (\omega t - kx_2 + \phi_0) - (\omega t - kx_1 + \phi_0)

Δϕ=−k(x2−x1)=−kΔx\Delta\phi = -k(x_2 - x_1) = -k \Delta x

The magnitude of the phase difference is ∣kΔx∣|k \Delta x|. Since we are typically interested in the magnitude of the phase difference, we use:

The phase difference Δϕ\Delta\phi between two points separated by a distance Δx\Delta x on a travelling wave is given by:

Δϕ=kΔx=2πλΔx\Delta\phi = k \Delta x = \frac{2\pi}{\lambda} \Delta x

where kk is the wave number and λ\lambda is the wavelength.

Let's apply this to the given problem.

  1. Extract wave parameters from the given equation. The given wave equation is y(x,t)=2.0cos⁡2π(10t−0.0080 x+0.35)y(x, t) = 2.0 \cos 2\pi(10t - 0.0080\,x + 0.35). To match it with the standard form y(x,t)=Acos⁡(ωt−kx+ϕ0)y(x, t) = A \cos(\omega t - kx + \phi_0), we first distribute the 2π2\pi inside the cosine argument:

y(x,t)=2.0cos⁡(2π⋅10t−2π⋅0.0080 x+2π⋅0.35)y(x, t) = 2.0 \cos (2\pi \cdot 10t - 2\pi \cdot 0.0080\,x + 2\pi \cdot 0.35)

y(x,t)=2.0cos⁡(20πt−0.016πx+0.7π)y(x, t) = 2.0 \cos (20\pi t - 0.016\pi x + 0.7\pi)

By comparing this with the standard form, we can identify the wave number $k$:
$k = 0.016\pi$.
The units for $x$ are in cm, so the units for $k$ are $\text{rad/cm}$.

2. Calculate the wavelength (λ\lambda).

The wave number kk is related to the wavelength λ\lambda by the formula k=2πλk = \frac{2\pi}{\lambda}.

We can rearrange this to find λ\lambda:

λ=2πk\lambda = \frac{2\pi}{k}

Substitute the value of $k$:

λ=2π0.016π cm−1=20.016 cm\lambda = \frac{2\pi}{0.016\pi \text{ cm}^{-1}} = \frac{2}{0.016} \text{ cm}

λ=200016 cm=125 cm\lambda = \frac{2000}{16} \text{ cm} = 125 \text{ cm}

It's often useful to work in meters for consistency, especially since some given distances are in meters.
$$\lambda = 125 \text{ cm} = 1.25 \text{ m}$$ …

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