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Wave Mechanics: Energy in a 1D Wave (Topic)

Wave Mechanics: Energy in a 1D Wave

The previous articles developed the one-dimensional string wave equation,

|------------|
μutt-=-T-uxx-,
(1)

and its traveling-wave solutions. The string does more than move, however. A disturbance also carries mechanical energy.

For the ideal stretched string, the local mechanical energy per unit equilibrium length is

|------------------------|
|         1-  2   1-   2 |
|ℰ(x, t) = 2 μut + 2 Tu x.|
-------------------------
(2)

The first term is kinetic energy density and the second is elastic potential energy density. This expression is standard for transverse waves on an ideal stretched string and follows directly from the same small-slope model used to derive the wave equation [1235].

WM18 develops that result from the mechanics of a short string element, checks its dimensions, applies it to traveling waves and Standing Waves, and shows why wave energy scales as the square of amplitude. The next article will ask how this energy crosses a fixed position and will derive the corresponding power flow.

1 Energy is distributed along the string

A string is a continuous system. Rather than assigning one energy to one point, we describe the energy contained in a short equilibrium-length interval dx.

Write

dE =  ℰ(x,t)dx,
(3)

where has units of energy per unit length.

For an ideal string there are two mechanical contributions:

dE  = dK  + dU.
(4)

The local bookkeeping is summarized below.

PIC

Figure. A moving string element has kinetic energy through ut. A sloped element is slightly longer than its equilibrium projection dx, producing elastic potential energy through ux.

2 Kinetic energy density

Consider a short string element of equilibrium length dx. Its mass is

dm  = μ dx,
(5)

where μ is the linear mass density.

The transverse velocity of the material point at position x is

          ∂u
vu = ut = ---.
          ∂t
(6)

Therefore the kinetic energy of the element is

dK = 1-
2dmvu2 (7)
= 1-
2(μdx)ut2. (8)

Divide by dx:

|----------------------|
|𝒦(x, t) = dK-- = 1μu2 .|
-----------dx----2---t--
(9)

This expression is exact within the transverse-motion model used here: kinetic energy is controlled by the local material velocity, not by the propagation speed alone.

3 Elastic potential energy density

The potential-energy term requires the string geometry.

At a fixed time, a short displaced string element has arclength

     √ ----------
ds =   dx2 + du2.
(10)

Since

du = ux dx,
(11)

we obtain

     ∘  -------
ds =    1 + u2 dx.
             x
(12)

For the small-slope model,

|u | ≪ 1.
  x
(13)

Use the expansion

∘ -----       q-
  1 + q ≃ 1 + 2
(14)

for small q. With q = ux2,

     (     1  )
ds ≃   1 + -u2x  dx.
           2
(15)

The extra length is therefore

                1
dℓ = ds − dx ≃  -u2xdx.
                2
(16)

If the equilibrium Tension magnitude is approximately constant at T, the work required to create this additional length is

dU  = T dℓ.
(17)

Thus

dU  ≃ 1-Tu2 dx,
      2    x
(18)

and the elastic potential energy density is

|----------------------|
|         dU     1     |
|𝒰(x,t) = --- =  -T u2x.|
-----------dx----2------
(19)

The same small-slope approximation that linearized the force law in WM14 also gives this quadratic elastic-energy expression.

4 Total local energy density

Adding the kinetic and potential terms gives

|--------------------------------|
|                  1-  2   1-  2 |
ℰ (x,t) = 𝒦 + 𝒰 =  2μu t + 2T ux.|
----------------------------------
(20)

This formula contains an important physical separation:

  • ut measures how rapidly the material is moving through equilibrium space;
  • ux measures how much the string is locally tilted and therefore stretched relative to its equilibrium projection.

A point can have zero displacement while still carrying energy. Energy depends on velocity and deformation, not simply on the value of u.

5 Dimensional check

The kinetic term has dimensions

            2
[μu2 ] = kg-m--=  J-.
   t    m  s2    m
(21)

For the potential term, ux is dimensionless because both u and x have dimensions of length. Hence

             J
[T u2x] = N =  --.
             m
(22)

Both terms therefore have the required units of energy per unit length.

6 Pure traveling waves have equal kinetic and potential densities

Consider a right-moving traveling profile

u(x,t) = F (x − ct).
(23)

Let

ξ = x − ct.
(24)

Then

ux =  F′(ξ)
(25)

and

u =  − cF′(ξ).
 t
(26)

The kinetic energy density becomes

𝒦 =  1μc2[F ′(ξ)]2.
     2
(27)

For the ideal string,

 2   T-
c =  μ ,
(28)

so

   2
μc  =  T.
(29)

Therefore

     1
𝒦 =  -T [F ′(ξ )]2.
     2
(30)

But

𝒰  = 1-Tu2x = 1T [F ′(ξ)]2.
     2        2
(31)

Hence

|------|
𝒦--=-𝒰--
(32)

for every point of a pure right-moving wave. The same proof holds for a pure left-moving wave G(x + ct).

The total energy density of a pure traveling wave can therefore be written as

|--------------------------------------|
|ℰ =  T[F ′(x − ct)]2 = μc2[F ′(x − ct)]2. |
---------------------------------------
(33)

A pulse example is shown below.

PIC

Figure. For a Gaussian pure traveling pulse, with normalized coordinate ζ = (x ct)∕σ, the kinetic and elastic potential energy densities are equal point by point. The energy density depends on the square of the pulse slope, so a smooth pulse can have zero energy density exactly at its displacement maximum.

7 Why the center of a smooth pulse can have zero energy density

This result can initially seem surprising. Consider a smooth pulse at its maximum. At the exact peak,

  ′
F  = 0.
(34)

For a shape-preserving traveling pulse,

       ′
ux = F  = 0
(35)

and

          ′
ut = − cF  = 0.
(36)

Therefore both local energy-density terms vanish at the exact pulse peak.

The pulse still carries finite total energy because energy is distributed over the regions where the profile changes. Large displacement alone is not the same as large local wave energy.

8 Sinusoidal traveling wave

Consider

u(x,t) = A cos(kx − ωt + ϕ).
(37)

Define

𝜃 =  kx − ωt + ϕ.
(38)

Then

ut = A ω sin 𝜃
(39)

and

ux = − Ak sin𝜃.
(40)

The kinetic energy density is

     1    2 2   2
𝒦  = --μA ω  sin 𝜃.
     2
(41)

The potential energy density is

𝒰  = 1T A2k2 sin2𝜃.
     2
(42)

The ideal-string dispersion relation is

ω =  ck
(43)

with

 2   T-
c =  μ .
(44)

Thus

T k2 = μω2,
(45)

so again

|-------|
|𝒦 =  𝒰 .
--------
(46)

The total energy density is

|----------------------------------|
|ℰ(x,t) = μA2 ω2 sin2(kx −  ωt + ϕ).|
-----------------------------------
(47)

PIC

Figure. The displacement varies as cos 𝜃, while the energy density varies as sin 2𝜃. Energy density is nonnegative and repeats twice during one displacement phase cycle.

9 Average energy density of a sinusoidal traveling wave

Over one full phase cycle,

⟨   2  ⟩   1
 sin 𝜃  =  -.
           2
(48)

Therefore

|------1--------|
⟨ℰ ⟩ = -μA2 ω2. |
-------2---------
(49)

The average kinetic and average potential contributions are each half of this:

|----------------------|
|             1-  2  2 |
|⟨𝒦 ⟩ = ⟨𝒰 ⟩ = 4μA ω  .|
-----------------------
(50)

The energy contained in one wavelength, averaged over the sinusoidal phase pattern, is

E   = ⟨ℰ⟩λ.
  λ
(51)

Hence

|----------------|
|      1         |
|E λ = -μA2 ω2λ. |
-------2---------
(52)

This result agrees with standard treatments of sinusoidal mechanical waves [3].

10 Energy scales as amplitude squared and frequency squared

For fixed μ, the average sinusoidal energy density obeys

        2 2
⟨ℰ⟩ ∝ A  ω .
(53)

Therefore:

  • doubling the amplitude multiplies average energy density by 4;
  • tripling the angular frequency at fixed amplitude multiplies it by 9;
  • changing the sign of the displacement amplitude does not change the energy.

This square-law behavior is one of the most important recurring features of wave physics. Similar quadratic energy measures will appear later for acoustic, electromagnetic, and quantum-wave contexts, although the detailed physical meaning of the field variables changes.

11 A general two-direction field

WM16 showed that a sufficiently smooth whole-line solution can be written as

u(x,t) = F (x − ct) + G (x + ct).
(54)

Let

ξ = x − ct,    η = x + ct.
(55)

Then

ux =  F′(ξ) + G′(η)
(56)

and

u  = − cF ′(ξ) + cG ′(η).
  t
(57)

Use T = μc2. The total energy density is

= 1-
2μc2[F+ G]2 + 1-
2T[F+ G]2 (58)
= T-
 2[F+ G]2 + T-
2[F+ G]2. (59)

Expanding the squares, the cross terms cancel:

|--------------------------|
|ℰ = T [F ′(ξ)]2 + T[G ′(η)]2.|
---------------------------
(60)

This is a useful result. The displacement fields interfere linearly, but in the ideal string model the total mechanical energy density separates into the sum of the directional component energy densities.

The kinetic and potential parts individually need not be equal when both directions are present.

12 Standing waves exchange kinetic and potential energy

A standing wave can be written

u (x,t) = B sin(kx )cos(ωt),
(61)

with fixed ends chosen so that

    nπ
k = ---.
     L
(62)

The derivatives are

ut = − B ω sin(kx )sin(ωt)
(63)

and

ux = Bk cos(kx )cos(ωt).
(64)

Thus

     1
𝒦 =  -μB2 ω2 sin2(kx) sin2(ωt)
     2
(65)

and

𝒰 = 1-TB2k2  cos2(kx )cos2(ωt).
    2
(66)

Unlike a single traveling wave, these two densities are not generally equal point by point.

Integrating over a normal-mode length 0 x L gives

K (t) = 1μB2 ω2L  sin2(ωt)
        4
(67)

and

       1-   2 2     2
U(t) = 4 μB  ω L cos (ωt).
(68)

Therefore

|--------------1---------|
E  = K  + U =  -μB2 ω2L, |
---------------4----------
(69)

which is constant in the ideal lossless model.

PIC

Figure. For one ideal standing-wave normal mode, total energy is constant while the integrated kinetic and elastic potential energies exchange periodically.

13 Worked Example 1: Local energy density from measured slope and velocity

A string has

μ = 0.020kg/m,      T =  80N.
(70)

At one event (x,t), suppose

ut = 1.5 m/s
(71)

and

ux = 0.080.
(72)

Find the kinetic, potential, and total energy densities.

Solution

The kinetic density is

𝒦 = 1
--
2μut2 (73)
= 1-
2(0.020)(1.5)2 (74)
= 0.0225 J/m. (75)

The potential density is

𝒰 = 1-
2Tux2 (76)
= 1-
2(80)(0.080)2 (77)
= 0.256 J/m. (78)

Therefore

|----------------------------|
ℰ-=--0.2785J/m--≃--0.279-J/m.--
(79)

The kinetic and potential densities are not equal here. Equality is guaranteed point by point only for a pure traveling wave moving at the string wave speed.

14 Worked Example 2: Sinusoidal average energy density and energy per wavelength

A sinusoidal traveling wave has

A =  4.0 mm,      f = 50 Hz,
(80)

on a string with

μ = 0.012kg/m,      T =  75N.
(81)

Find the wave speed, wavelength, average energy density, and average energy contained in one wavelength.

Solution

First convert the amplitude:

A = 0.0040 m.
(82)

The wave speed is

c = ∘ ---
  T-
   μ (83)
= ∘ ------
  --75--
  0.012 (84)
= 79.1 m/s. (85)

The wavelength is

λ = c-
f (86)
= 79.1
----
 50 (87)
= 1.58 m. (88)

The angular frequency is

ω =  2πf =  314.2rad/s.
(89)

The average energy density is

⟨ℰ⟩ = 1-
2μA2ω2 (90)
= 1-
2(0.012)(0.0040)2(314.2)2 (91)
9.47 × 103 J/m. (92)

Thus

|------------------|
|⟨ℰ⟩ ≃ 9.47 mJ/m.  |
-------------------
(93)

The energy per wavelength is

Eλ = ⟨ℰ⟩λ (94)
= (9.47 × 103)(1.58) (95)
1.50 × 102 J. (96)

Therefore

|--------------|
|Eλ ≃ 0.0150 J.|
----------------
(97)

15 Worked Example 3: Total energy of a Gaussian traveling pulse

Consider the right-moving pulse

               [          2]
u(x,t) = A exp  − (x-−-ct)-  .
                     2σ2
(98)

Let

A =  1.0cm,     σ =  0.080 m,      T = 60 N.
(99)

Find the total mechanical energy of the pulse.

Solution

Let

z = x −  ct.
(100)

Then

              (   z2 )
F (z) = A exp   − --2-
                  2σ
(101)

and

                 (     2 )
F ′(z) = − Az- exp  − -z--  .
          σ2         2σ2
(102)

For a pure traveling wave,

ℰ = T [F ′(z )]2.
(103)

Hence

           2 2    (    2)
         A--z-        z--
ℰ(z ) = T σ4  exp   − σ2   .
(104)

The total energy is

     ∫ ∞
E  =      ℰ(z)dz.
      −∞
(105)

Using

∫ ∞       2 2      √ π-
    z2e −z∕σ dz =  ----σ3,
 −∞                 2
(106)

we obtain

E = T A2
---4-
 σ√ π-
----
 2σ3 (107)
=      √--
T-A2--π-
   2σ . (108)

Now use

A  = 0.010m.
(109)

Then

E = (60 )(0.010)2√ π-
---------------
   2(0.080) (110)
6.65 × 102 J. (111)

Therefore

|--------------|
-E-≃--0.0665J.-|
(112)

The result scales as A2 and inversely with the pulse width parameter σ: for the same peak displacement, a sharper pulse has larger slopes and therefore more energy.

16 Worked Example 4: Amplitude and frequency scaling

Wave 1 and wave 2 travel on the same string. Suppose

A2 =  2A1
(113)

and

ω2 = 3ω1.
(114)

Find the ratio of their average sinusoidal energy densities.

Solution

Since

       1   2 2
⟨ℰ ⟩ = -μA  ω ,
       2
(115)

and both waves are on the same string,

⟨ℰ ⟩
--2-
⟨ℰ1⟩ = A2 ω2
--22-22
A 1ω1 (116)
= (2)2(3)2 (117)
= 36. (118)

Thus

|--------------|
-⟨ℰ2⟩ =-36⟨ℰ1⟩.|
(119)

The square-law scaling compounds rapidly when both amplitude and frequency increase.

17 Worked Example 5: Energy exchange in a standing mode

A fixed-fixed string normal mode is

u(x,t) = B sin(kx)cos(ωt )
(120)

with

B =  6.0mm,      μ =  0.015 kg/m,      f = 30 Hz,     L =  1.0 m.
(121)

Find the total mode energy, and find the integrated kinetic and potential energies when

ωt = π-.
     6
(122)

Solution

Convert the amplitude:

B = 0.0060 m.
(123)

The angular frequency is

ω =  2πf =  188.5rad/s.
(124)

The constant total mode energy is

E = 1-
4μB2ω2L (125)
= 1
--
4(0.015)(0.0060)2(188.5)2(1.0) (126)
4.80 × 103 J. (127)

Therefore

|-------------|
E--≃-4.80mJ.---
(128)

At ωt = π∕6,

   2( π)    1
sin   -- =  --
      6     4
(129)

and

    (  )
cos2 π-  =  3.
      6     4
(130)

Hence

K  = 1-E ≃  1.20 mJ
     4
(131)

and

     3-
U =  4E  ≃ 3.60 mJ.
(132)

So

|-------------------------------|
K  ≃ 1.20 mJ,     U  ≃ 3.60mJ.  |
---------------------------------
(133)

Their sum remains the same total mechanical energy.

18 Worked Example 6: Energy density of simultaneous right- and left-moving components

At one event, suppose a two-direction solution has

F′ = 0.10,    G ′ = − 0.040,    T =  50N.
(134)

Find the total energy density. Also find the kinetic and potential parts separately.

Solution

For the two-family solution,

ℰ =  T[(F ′)2 + (G′)2].
(135)

Therefore

= 50[(0.10)2 + (0.040)2] (136)
= 50(0.0116) (137)
= 0.580 J/m . (138)

For the kinetic part,

          ′    ′
ut = c(− F +  G ).
(139)

Using μc2 = T,

𝒦 = T
--
2(F+ G)2 (140)
= 50-
 2(0.10 0.040)2 (141)
= 25(0.0196) (142)
= 0.490 J/m . (143)

For the potential part,

𝒰 = T-
2(F+ G)2 (144)
= 25(0.10 0.040)2 (145)
= 25(0.0036) (146)
= 0.0900 J/m . (147)

As a check,

0.490 + 0.0900 = 0.580 J/m.
(148)

The kinetic and potential densities are not equal because this field contains both propagation directions at once.

19 Common mistakes

  • Mistake: treating displacement amplitude itself as energy. Energy depends on squared velocity and squared slope.
  • Mistake: using the propagation speed c in place of the material velocity ut in the kinetic energy.
  • Mistake: assuming 𝒦 = 𝒰 for every wave field. Pointwise equality holds for a pure traveling wave, not for an arbitrary superposition or standing wave.
  • Mistake: forgetting that ux is dimensionless for transverse displacement u measured in meters against coordinate x measured in meters.
  • Mistake: assuming the displacement maximum of a pulse must also be the local energy-density maximum. For a smooth pure traveling pulse, the exact displacement peak can have zero slope and zero transverse velocity.
  • Mistake: applying the ideal-string energy density outside the small-slope, constant-tension model without checking whether the approximations remain valid.

20 What WM18 establishes

The ideal one-dimensional string contains mechanical energy with local density

|------------------|
|    1-  2   1-  2 |
ℰ =  2μu t + 2T ux.|
--------------------
(149)

For a pure traveling wave,

|------|
𝒦  = 𝒰 |
--------
(150)

and, for a sinusoidal traveling wave,

|---------------|
|      1        |
⟨ℰ ⟩ = -μA2 ω2. |
-------2---------
(151)

The next question is no longer how much energy is locally present, but how rapidly that energy passes a fixed position. That leads naturally to wave power and energy flux.

References

References

[1]   A. P. French, Vibrations and Waves, M.I.T. Introductory Physics Series, W. W. Norton & Company, 1971.

[2]   Frank S. Crawford, Jr., Waves, Berkeley Physics Course, Volume 3, McGraw-Hill, 1968.

[3]   William Moebs, Samuel J. Ling, and Jeff Sanny, University Physics, Volume 1, OpenStax, 2016, Section 16.4, “Energy and Power of a Wave.”

[4]   Howard Georgi, The Physics of Waves, Benjamin/Cummings, 1992, continuum and traveling-wave chapters; also distributed through MIT OpenCourseWare 8.03SC.

[5]   Massachusetts Institute of Technology, 8.03SC Physics III: Vibrations and Waves, Fall 2016, Problem Set 5 and Lecture 10 materials on traveling waves and string energy, MIT OpenCourseWare.


"Wave Mechanics: Energy in a 1D Wave" is owned by bloftin.
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Keywords:  wave mechanics, wave energy, energy density, kinetic energy density, elastic potential energy density, stretched string, traveling wave, standing wave, linear mass density, tension, amplitude squared, frequency squared

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example of Wave Mechanics: Energy in a 1D Wave (Example) by bloftin

Cross-references: flux, parameter, WM16, field, relation, deformation, formula, WM14, force, work, magnitude, Tension, speed, velocity, mass, system, power, position, square, Standing Waves, mechanics, waves, kinetic energy, equilibrium, energy, wave equation
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This is version 1 of Wave Mechanics: Energy in a 1D Wave, born on 2026-09-12.
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Classification:
Physics Classification46.40.Cd (Mechanical wave propagation (including diffraction, scattering, and)
 46.40.-f (Vibrations and mechanical waves )
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