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A pendulum is a body suspended from a fixed support so that it swings freely back and forth under the influence of gravity. When a pendulum is displaced sideways from its resting, equilibrium position, it is subject to a restoring force due to gravity that will accelerate it back towards the equilibrium position. When released, the restoring force acting on the pendulum's mass causes it to oscillate about the equilibrium position, swinging it back and forth. The mathematics of pendulums are in general quite complicated. Simplifying assumptions can be made, which in the case of a simple pendulum allow the equations of motion to be solved analytically for small-angle oscillations.

Simple gravity pendulum

A simple gravity pendulum^[1] is an idealized mathematical model of a real pendulum.^[2][3][4] This is a weight (or bob) on the end of a massless cord suspended from a pivot, without friction. Since in this model there is no frictional energy loss, when given an initial displacement it will swing back and forth at a constant amplitude. The model is based on these assumptions:

• The rod or cord on which the bob swings is massless, inextensible and always remains taut.
• The bob is a point mass.
• Motion occurs only in two dimensions, i.e. the bob does not trace an ellipse but an arc.
• The motion does not lose energy to friction or air resistance.
• The gravitational field is uniform.
• The support does not move.

The differential equation which represents the motion of a simple pendulum is

$${\displaystyle {\frac {d^{2}\theta }{dt^{2))}+{\frac {g}{\ell ))\sin \theta =0}$$

(Eq. 1)

where g is the magnitude of the gravitational field, ℓ is the length of the rod or cord, and θ is the angle from the vertical to the pendulum.

"Force" derivation of (Eq. 1)

Consider Figure 1 on the right, which shows the forces acting on a simple pendulum. Note that the path of the pendulum sweeps out an arc of a circle. The angle θ is measured in radians, and this is crucial for this formula. The blue arrow is the gravitational force acting on the bob, and the violet arrows are that same force resolved into components parallel and perpendicular to the bob's instantaneous motion. The direction of the bob's instantaneous velocity always points along the red axis, which is considered the tangential axis because its direction is always tangent to the circle. Consider Newton's second law,

$${\displaystyle F=ma}$$

where F is the sum of forces on the object, m is mass, and a is the acceleration. Because we are only concerned with changes in speed, and because the bob is forced to stay in a circular path, we apply Newton's equation to the tangential axis only. The short violet arrow represents the component of the gravitational force in the tangential axis, and trigonometry can be used to determine its magnitude. Thus,

$${\displaystyle {\begin{aligned}F&=-mg\sin \theta =ma,\qquad {\text{so))\\a&=-g\sin \theta ,\end{aligned))}$$

where g is the acceleration due to gravity near the surface of the earth. The negative sign on the right hand side implies that θ and a always point in opposite directions. This makes sense because when a pendulum swings further to the left, we would expect it to accelerate back toward the right.

This linear acceleration a along the red axis can be related to the change in angle θ by the arc length formulas; s is arc length:

$${\displaystyle {\begin{aligned}s&=\ell \theta ,\\v&={\frac {ds}{dt))=\ell {\frac {d\theta }{dt)),\\a&={\frac {d^{2}s}{dt^{2))}=\ell {\frac {d^{2}\theta }{dt^{2))},\end{aligned))}$$

thus:

$${\displaystyle {\begin{aligned}\ell {\frac {d^{2}\theta }{dt^{2))}&=-g\sin \theta ,\\{\frac {d^{2}\theta }{dt^{2))}+{\frac {g}{\ell ))\sin \theta &=0.\end{aligned))}$$

"Torque" derivation of (Eq. 1)

Equation (1) can be obtained using two definitions for torque.

$${\displaystyle {\boldsymbol {\tau ))=\mathbf {r} \times \mathbf {F} ={\frac {d\mathbf {L} }{dt)).}$$

First start by defining the torque on the pendulum bob using the force due to gravity.

$${\displaystyle {\boldsymbol {\tau ))=\mathbf {l} \times \mathbf {F} _{\mathrm {g} },}$$

where l is the length vector of the pendulum and F_g is the force due to gravity.

For now just consider the magnitude of the torque on the pendulum.

$${\displaystyle |{\boldsymbol {\tau ))|=-mg\ell \sin \theta ,}$$

where m is the mass of the pendulum, g is the acceleration due to gravity, l is the length of the pendulum, and θ is the angle between the length vector and the force due to gravity.

Next rewrite the angular momentum.

$${\displaystyle \mathbf {L} =\mathbf {r} \times \mathbf {p} =m\mathbf {r} \times ({\boldsymbol {\omega ))\times \mathbf {r} ).}$$

Again just consider the magnitude of the angular momentum.

$${\displaystyle |\mathbf {L} |=mr^{2}\omega =m\ell ^{2}{\frac {d\theta }{dt)).}$$

and its time derivative

$${\displaystyle {\frac {d}{dt))|\mathbf {L} |=m\ell ^{2}{\frac {d^{2}\theta }{dt^{2))},}$$

According to τ = dL/dt, we can get by comparing the magnitudes

$${\displaystyle -mg\ell \sin \theta =m\ell ^{2}{\frac {d^{2}\theta }{dt^{2))},}$$

thus:

$${\displaystyle {\frac {d^{2}\theta }{dt^{2))}+{\frac {g}{\ell ))\sin \theta =0,}$$

which is the same result as obtained through force analysis.

"Energy" derivation of (Eq. 1)

It can also be obtained via the conservation of mechanical energy principle: any object falling a vertical distance ${\displaystyle h}$ would acquire kinetic energy equal to that which it lost to the fall. In other words, gravitational potential energy is converted into kinetic energy. Change in potential energy is given by

$${\displaystyle \Delta U=mgh.}$$

The change in kinetic energy (body started from rest) is given by

$${\displaystyle \Delta K={\tfrac {1}{2))mv^{2}.}$$

Since no energy is lost, the gain in one must be equal to the loss in the other

$${\displaystyle {\tfrac {1}{2))mv^{2}=mgh.}$$

The change in velocity for a given change in height can be expressed as

$${\displaystyle v={\sqrt {2gh)).}$$

Using the arc length formula above, this equation can be rewritten in terms of dθ/dt:

$${\displaystyle {\begin{aligned}v=\ell {\frac {d\theta }{dt))&={\sqrt {2gh)),\quad {\text{so))\\{\frac {d\theta }{dt))&={\frac {\sqrt {2gh)){\ell )),\end{aligned))}$$

where h is the vertical distance the pendulum fell. Look at Figure 2, which presents the trigonometry of a simple pendulum. If the pendulum starts its swing from some initial angle θ₀, then y₀, the vertical distance from the screw, is given by

$${\displaystyle y_{0}=\ell \cos \theta _{0}.}$$

Similarly, for y₁, we have

$${\displaystyle y_{1}=\ell \cos \theta .}$$

Then h is the difference of the two

$${\displaystyle h=\ell \left(\cos \theta -\cos \theta _{0}\right).}$$

In terms of dθ/dt gives

$${\displaystyle {\frac {d\theta }{dt))={\sqrt ((\frac {2g}{\ell ))(\cos \theta -\cos \theta _{0}))).}$$

(Eq. 2)

This equation is known as the first integral of motion, it gives the velocity in terms of the location and includes an integration constant related to the initial displacement (θ₀). We can differentiate, by applying the chain rule, with respect to time to get the acceleration

$${\displaystyle {\begin{aligned}{\frac {d}{dt)){\frac {d\theta }{dt))&={\frac {d}{dt)){\sqrt ((\frac {2g}{\ell ))\left(\cos \theta -\cos \theta _{0}\right))),\\{\frac {d^{2}\theta }{dt^{2))}&={\frac {1}{2)){\frac {-{\frac {2g}{\ell ))\sin \theta }{\sqrt ((\frac {2g}{\ell ))(\cos \theta -\cos \theta _{0})))}{\frac {d\theta }{dt))\\&={\frac {1}{2)){\frac {-{\frac {2g}{\ell ))\sin \theta }{\sqrt ((\frac {2g}{\ell ))(\cos \theta -\cos \theta _{0})))}{\sqrt ((\frac {2g}{\ell ))(\cos \theta -\cos \theta _{0})))=-{\frac {g}{\ell ))\sin \theta ,\\{\frac {d^{2}\theta }{dt^{2))}&+{\frac {g}{\ell ))\sin \theta =0,\end{aligned))}$$

which is the same result as obtained through force analysis.

Small-angle approximation

The differential equation given above is not easily solved, and there is no solution that can be written in terms of elementary functions. However, adding a restriction to the size of the oscillation's amplitude gives a form whose solution can be easily obtained. If it is assumed that the angle is much less than 1 radian (often cited as less than 0.1 radians, about 6°), or

$${\displaystyle \theta \ll 1,}$$

$${\displaystyle \sin \theta \approx \theta ,}$$

$${\displaystyle {\frac {d^{2}\theta }{dt^{2))}+{\frac {g}{\ell ))\theta =0.}$$

The error due to the approximation is of order θ³ (from the Taylor expansion for sin θ).

Let the starting angle be θ₀. If it is assumed that the pendulum is released with zero angular velocity, the solution becomes

The motion is simple harmonic motion where θ₀ is the amplitude of the oscillation (that is, the maximum angle between the rod of the pendulum and the vertical). The corresponding approximate period of the motion is then

which is known as Christiaan Huygens's law for the period. Note that under the small-angle approximation, the period is independent of the amplitude θ₀; this is the property of isochronism that Galileo discovered.

Rule of thumb for pendulum length

$${\displaystyle T_{0}=2\pi {\sqrt {\frac {\ell }{g))))$$

$${\displaystyle \ell ={\frac {g}{\pi ^{2))}{\frac {T_{0}^{2)){4)).}$$

If SI units are used (i.e. measure in metres and seconds), and assuming the measurement is taking place on the Earth's surface, then g ≈ 9.81 m/s², and g/π² ≈ 1 m/s² (0.994 is the approximation to 3 decimal places).

Therefore, relatively reasonable approximations for the length and period are:

$${\displaystyle {\begin{aligned}\ell &\approx {\frac {T_{0}^{2)){4)),\\T_{0}&\approx 2{\sqrt {\ell ))\end{aligned))}$$

Arbitrary-amplitude period

For amplitudes beyond the small angle approximation, one can compute the exact period by first inverting the equation for the angular velocity obtained from the energy method (Eq. 2),

$${\displaystyle {\frac {dt}{d\theta ))={\sqrt {\frac {\ell }{2g))}{\frac {1}{\sqrt {\cos \theta -\cos \theta _{0))))}$$

$${\displaystyle T=t(\theta _{0}\rightarrow 0\rightarrow -\theta _{0}\rightarrow 0\rightarrow \theta _{0}),}$$

$${\displaystyle T=2t(\theta _{0}\rightarrow 0\rightarrow -\theta _{0}),}$$

$${\displaystyle T=4t(\theta _{0}\rightarrow 0),}$$

$${\displaystyle T=4{\sqrt {\frac {\ell }{2g))}\int _{0}^{\theta _{0)){\frac {d\theta }{\sqrt {\cos \theta -\cos \theta _{0)))).}$$

Note that this integral diverges as θ₀ approaches the vertical

$${\displaystyle \lim _{\theta _{0}\to \pi }T=\infty ,}$$

This integral can be rewritten in terms of elliptic integrals as

$${\displaystyle T=4{\sqrt {\frac {\ell }{g))}F\left({\frac {\pi }{2)),\sin {\frac {\theta _{0)){2))\right)}$$

$${\displaystyle F(\varphi ,k)=\int _{0}^{\varphi }{\frac {du}{\sqrt {1-k^{2}\sin ^{2}u))}\,.}$$

Or more concisely by the substitution

$${\displaystyle \sin {u}={\frac {\sin {\frac {\theta }{2))}{\sin {\frac {\theta _{0)){2))))}$$

Here K is the complete elliptic integral of the first kind defined by

$${\displaystyle K(k)=F\left({\frac {\pi }{2)),k\right)=\int _{0}^{\frac {\pi }{2)){\frac {du}{\sqrt {1-k^{2}\sin ^{2}u))}\,.}$$

For comparison of the approximation to the full solution, consider the period of a pendulum of length 1 m on Earth (g = 9.80665 m/s²) at initial angle 10 degrees is

$${\displaystyle 4{\sqrt {\frac {1{\text{ m))}{g))}\ K\left(\sin {\frac {10^{\circ )){2))\right)\approx 2.0102{\text{ s)).}$$

$${\displaystyle 2\pi {\sqrt {\frac {1{\text{ m))}{g))}\approx 2.0064{\text{ s)).}$$

The difference between the two values, less than 0.2%, is much less than that caused by the variation of g with geographical location.

From here there are many ways to proceed to calculate the elliptic integral.

Legendre polynomial solution for the elliptic integral

Given Eq. 3 and the Legendre polynomial solution for the elliptic integral:

$${\displaystyle K(k)={\frac {\pi }{2))\sum _{n=0}^{\infty }\left({\frac {(2n-1)!!}{(2n)!!))k^{n}\right)^{2))$$

$${\displaystyle {\begin{alignedat}{2}T&=2\pi {\sqrt {\frac {\ell }{g))}\left(1+\left({\frac {1}{2))\right)^{2}\sin ^{2}{\frac {\theta _{0)){2))+\left({\frac {1\cdot 3}{2\cdot 4))\right)^{2}\sin ^{4}{\frac {\theta _{0)){2))+\left({\frac {1\cdot 3\cdot 5}{2\cdot 4\cdot 6))\right)^{2}\sin ^{6}{\frac {\theta _{0)){2))+\cdots \right)\\&=2\pi {\sqrt {\frac {\ell }{g))}\cdot \sum _{n=0}^{\infty }\left(\left({\frac {(2n)!}{(2^{n}\cdot n!)^{2))}\right)^{2}\cdot \sin ^{2n}{\frac {\theta _{0)){2))\right).\end{alignedat))}$$

Figure 4 shows the relative errors using the power series. T₀ is the linear approximation, and T₂ to T₁₀ include respectively the terms up to the 2nd to the 10th powers.

Power series solution for the elliptic integral

Another formulation of the above solution can be found if the following Maclaurin series:

$${\displaystyle \sin {\frac {\theta _{0)){2))={\frac {1}{2))\theta _{0}-{\frac {1}{48))\theta _{0}^{3}+{\frac {1}{3\,840))\theta _{0}^{5}-{\frac {1}{645\,120))\theta _{0}^{7}+\cdots .}$$

$${\displaystyle T=2\pi {\sqrt {\frac {\ell }{g))}\left(1+{\frac {1}{16))\theta _{0}^{2}+{\frac {11}{3\,072))\theta _{0}^{4}+{\frac {173}{737\,280))\theta _{0}^{6}+{\frac {22\,931}{1\,321\,205\,760))\theta _{0}^{8}+{\frac {1\,319\,183}{951\,268\,147\,200))\theta _{0}^{10}+{\frac {233\,526\,463}{2\,009\,078\,326\,886\,400))\theta _{0}^{12}+\cdots \right),}$$

Arithmetic-geometric mean solution for elliptic integral

Given Eq. 3 and the arithmetic–geometric mean solution of the elliptic integral:

$${\displaystyle K(k)={\frac {\pi }{2M(1-k,1+k))),}$$

This yields an alternative and faster-converging formula for the period:^[6][7][8]

$${\displaystyle T={\frac {2\pi }{M\left(1,\cos {\frac {\theta _{0)){2))\right))){\sqrt {\frac {\ell }{g))}.}$$

The first iteration of this algorithm gives

$${\displaystyle T_{1}={\frac {2T_{0)){1+\cos {\frac {\theta _{0)){2)))).}$$

This approximation has the relative error of less than 1% for angles up to 96.11 degrees.^[6] Since ${\textstyle {\frac {1}{2))\left(1+\cos \left({\frac {\theta _{0)){2))\right)\right)=\cos ^{2}{\frac {\theta _{0)){4)),}$ the expression can be written more concisely as

$${\displaystyle T_{1}=T_{0}\sec ^{2}{\frac {\theta _{0)){4)).}$$

The second order expansion of ${\displaystyle \sec ^{2}(\theta _{0}/4)}$ reduces to ${\textstyle T\approx T_{0}\left(1+{\frac {\theta _{0}^{2)){16))\right).}$

A second iteration of this algorithm gives

$${\displaystyle T_{2}={\frac {4T_{0)){1+\cos {\frac {\theta _{0)){2))+2{\sqrt {\cos {\frac {\theta _{0)){2))))))={\frac {4T_{0)){\left(1+{\sqrt {\cos {\frac {\theta _{0)){2))))\right)^{2))}.}$$

This second approximation has a relative error of less than 1% for angles up to 163.10 degrees.^[6]

Approximate formulae for the nonlinear pendulum period

Though the exact period ${\displaystyle T}$ can be determined, for any finite amplitude ${\displaystyle \theta _{0}<\pi }$ rad, by evaluating the corresponding complete elliptic integral ${\displaystyle K(k)}$, where ${\displaystyle k\equiv \sin(\theta _{0}/2)}$, this is often avoided in applications because it is not possible to express this integral in a closed form in terms of elementary functions. This has made way for research on simple approximate formulae for the increase of the pendulum period with amplitude (useful in introductory physics labs, classical mechanics, electromagnetism, acoustics, electronics, superconductivity, etc.^[9] The approximate formulae found by different authors can be classified as follows:

• ‘Not so large-angle’ formulae, i.e. those yielding good estimates for amplitudes below ${\displaystyle \pi /2}$ rad (a natural limit for a bob on the end of a flexible string), though the deviation with respect to the exact period increases monotonically with amplitude, being unsuitable for amplitudes near to ${\displaystyle \pi }$ rad. One of the simplest formulae found in literature is the following one by Lima (2006): ${\textstyle T\approx -\,T_{0}\,{\frac {\ln {a)){1-a))}$, where ${\displaystyle a\equiv \cos {(\theta _{0}/2)))$.^[10]
• ‘Very large-angle’ formulae, i.e. those which approximate the exact period asymptotically for amplitudes near to ${\displaystyle \pi }$rad, with an error that increases monotonically for smaller amplitudes (i.e., unsuitable for small amplitudes). One of the better such formulae is that by Cromer, namely:^[11] ${\textstyle T\approx {\frac {2}{\pi ))\,T_{0}\,\ln {(4/a)))$.

Of course, the increase of ${\displaystyle T}$ with amplitude is more apparent when ${\displaystyle \pi /2<\theta _{0}<\pi }$, as has been observed in many experiments using either a rigid rod or a disc.^[12] As accurate timers and sensors are currently available even in introductory physics labs, the experimental errors found in ‘very large-angle’ experiments are already small enough for a comparison with the exact period and a very good agreement between theory and experiments in which friction is negligible has been found. Since this activity has been encouraged by many instructors, a simple approximate formula for the pendulum period valid for all possible amplitudes, to which experimental data could be compared, was sought. In 2008, Lima derived a weighted-average formula with this characteristic:^[9]

$${\displaystyle T\approx {\frac {r\,a^{2}\,T_{\text{Lima))+k^{2}\,T_{\text{Cromer))}{r\,a^{2}+k^{2))},}$$

${\displaystyle r=7.17}$

${\displaystyle \theta _{0}=95^{\circ ))$

Arbitrary-amplitude angular displacement

The Fourier series expansion of ${\displaystyle \theta (t)}$ is given by^[13][14]

$${\displaystyle \theta (t)=8\sum _{n\geq 1{\text{ odd))}{\frac {(-1)^{\left\lfloor {n/2}\right\rfloor )){n)){\frac {q^{n/2)){1+q^{n))}\cos(n\omega t)}$$

where ${\displaystyle q}$ is the elliptic nome, ${\displaystyle q=\exp \left({-\pi K{\bigl (}{\sqrt {\textstyle 1-k^{2))}{\bigr )}{\big /}K(k)}\right),}$ ${\displaystyle k=\sin(\theta _{0}/2),}$ and ${\displaystyle \omega =2\pi /T}$ the angular frequency.

If one defines

$${\displaystyle \varepsilon ={\frac {1}{2))\cdot {\frac {1-{\sqrt {\cos(\theta _{0}/2)))}{1+{\sqrt {\cos(\theta _{0}/2)))))}$$

${\displaystyle q}$

$${\displaystyle q=\varepsilon +2\varepsilon ^{5}+15\varepsilon ^{9}+150\varepsilon ^{13}+1707\varepsilon ^{17}+20910\varepsilon ^{21}+\cdots }$$

${\displaystyle \theta _{0}<\pi }$

${\displaystyle \varepsilon <{\tfrac {1}{2))}$

Equivalently, the angle can be given in terms of the Jacobi elliptic function ${\displaystyle \operatorname {cd} }$ with modulus ${\displaystyle k}$^[15]

$${\displaystyle \theta (t)=2\arcsin \left(k\operatorname {cd} \left({\sqrt {\frac {g}{\ell ))}t;k\right)\right),\quad k=\sin {\frac {\theta _{0)){2)).}$$

For small ${\displaystyle x}$, ${\displaystyle \sin x\approx x}$, ${\displaystyle \arcsin x\approx x}$ and ${\displaystyle \operatorname {cd} (t;0)=\cos t}$, so the solution is well-approximated by the solution given in Pendulum (mechanics)#Small-angle approximation.

Examples

The animations below depict the motion of a simple (frictionless) pendulum with increasing amounts of initial displacement of the bob, or equivalently increasing initial velocity. The small graph above each pendulum is the corresponding phase plane diagram; the horizontal axis is displacement and the vertical axis is velocity. With a large enough initial velocity the pendulum does not oscillate back and forth but rotates completely around the pivot.

• 
  Initial angle of 0°, a stable equilibrium
• 
  Initial angle of 45°
• 
  Initial angle of 90°
• 
  Initial angle of 135°
• 
  Initial angle of 170°
• 
  Initial angle of 180°, unstable equilibrium
• 
  Pendulum with just barely enough energy for a full swing
• 
  Pendulum with enough energy for a full swing

Damped, driven pendulum

The above discussion focuses on a pendulum bob only acted upon by the force of gravity. Here we instead suppose a damping force, e.g. air resistance, as well as a sinusoidal driving force acts on the body. This system is a damped, driven oscillator, and is chaotic.

Equation (1) can be written as

$${\displaystyle ml^{2}{\frac {d^{2}\theta }{dt^{2))}=-mgl\sin \theta }$$

(see the Torque derivation of Equation (1) above).

We can now add a damping term and a forcing term to the right hand side to get

$${\displaystyle ml^{2}{\frac {d^{2}\theta }{dt^{2))}=-mgl\sin \theta -b{\frac {d\theta }{dt))+a\cos(\Omega t)}$$

where we have assumed the damping couple to be proportional to the angular velocity (this is true for low-speed air resistance, see also Drag (physics)). ${\displaystyle a}$ and ${\displaystyle b}$ are constants defining the amplitude of forcing and the degree of damping respectively. ${\textstyle \Omega }$ is the angular frequency of the driving oscillations.

We can now simplify by dividing through by ${\textstyle ml^{2))$ and redefining the constants appropriately to obtain

$${\displaystyle {\frac {d^{2}\theta }{dt^{2))}+B{\frac {d\theta }{dt))+{\frac {g}{l)){\sin \theta }=A\cos(\Omega t).}$$

This equation exhibits chaotic behaviour. The exact motion of this pendulum can only be found numerically and is highly dependent on initial conditions, e.g. the initial velocity and the starting amplitude. However, the small angle approximation outlined above can still be used under the required conditions to give an approximate analytical solution.

Compound pendulum

A compound pendulum (or physical pendulum) is one where the rod is not massless, and may have extended size; that is, an arbitrarily shaped rigid body swinging by a pivot ${\displaystyle O}$. In this case the pendulum's period depends on its moment of inertia ${\displaystyle I_{O))$ around the pivot point.

The equation of torque gives:

$${\displaystyle \tau =I\alpha }$$

${\displaystyle \alpha }$

${\displaystyle \tau }$

The torque is generated by gravity so: ${\displaystyle \tau =-mgr_{\mathrm {CM} }\sin \theta }$ where:

• ${\displaystyle m}$ is the total mass of the ridig body (rod and bob)
• ${\displaystyle r_{\mathrm {CM} ))$ is the distance from the pivot point to the system's center of mass
• ${\displaystyle \theta }$ is the angle from the vertical

Hence, under the small-angle approximation, ${\displaystyle \sin \theta \approx \theta }$,

$${\displaystyle \alpha ={\ddot {\theta ))\approx -{\frac {mgr_{\mathrm {CM} )){I_{O))}\theta }$$

${\displaystyle I_{O))$

${\displaystyle O}$

The expression for ${\displaystyle \alpha }$ is of the same form as the conventional simple pendulum and gives a period of^[2]

$${\displaystyle T=2\pi {\sqrt {\frac {I_{O)){mgr_{\mathrm {CM} ))))}$$

And a frequency of

$${\displaystyle f={\frac {1}{T))={\frac {1}{2\pi )){\sqrt {\frac {mgr_{\mathrm {CM} )){I_{O))))}$$

If the initial angle is taken into consideration (for large amplitudes), then the expression for ${\displaystyle \alpha }$ becomes:

$${\displaystyle \alpha ={\ddot {\theta ))=-{\frac {mgr_{\mathrm {CM} )){I_{O))}\sin \theta }$$

$${\displaystyle T=4\operatorname {K} \left(\sin ^{2}{\frac {\theta _{\mathrm {max} )){2))\right){\sqrt {\frac {I_{O)){mgr_{\mathrm {CM} ))))}$$

${\displaystyle \theta _{\mathrm {max} ))$

${\displaystyle \operatorname {K} (k)}$

An important concept is the equivalent length, ${\displaystyle \ell ^{\mathrm {eq} ))$, the length of a simple pendulums that has the same angular frequency ${\displaystyle \omega _{0))$ as the compound pendulum: ${\displaystyle {\omega _{0))^{2}={\frac {g}{\ell ^{\mathrm {eq} ))}={\frac {mgr_{\mathrm {CM} )){I_{O))}\implies \ell ^{\mathrm {eq} }={\frac {I_{O)){gr_{\mathrm {CM} ))))$

Consider the following cases:

• The simple pendulum is the special case where all the mass is located at the bob swinging at a distance ${\displaystyle \ell }$ from the pivot. Thus, ${\displaystyle r_{\mathrm {CM} }=\ell }$ and ${\displaystyle I_{O}=m\ell ^{2))$, so the expression reduces to: ${\displaystyle {\omega _{0))^{2}={\frac {mgr_{\mathrm {CM} )){I_{O))}={\frac {mg\ell }{m\ell ^{2))}={\frac {g}{\ell ))}$ . Notice ${\displaystyle \ell ^{\mathrm {eq} }=\ell }$, as expected (the definition of equivalent length).
• A homogeneous rod of mass ${\displaystyle m}$ and length ${\displaystyle \ell }$ swinging from its end has ${\displaystyle r_{\mathrm {CM} }={\frac {1}{2))\ell }$ and ${\displaystyle I_{O}={\frac {1}{3))m\ell ^{2))$, so the expression reduces to: ${\displaystyle {\omega _{0))^{2}={\frac {mgr_{\mathrm {CM} )){I_{O))}={\frac {mg\,{\frac {1}{2))\ell }((\frac {1}{3))m\ell ^{2))}={\frac {g}((\frac {2}{3))\ell ))}$ . Notice ${\displaystyle \ell ^{\mathrm {eq} }={\frac {2}{3))\ell }$, a homogeneous rod oscilates as if it were a simple pendulum of two-thirds its length.
• A heavy simple pendulum: combination of a homogeneous rod of mass ${\displaystyle m_{\mathrm {rod} ))$ and length ${\displaystyle \ell }$ swinging from its end, and a bob ${\displaystyle m_{\mathrm {bob} ))$ at the other end. Then the system has a total mass of ${\displaystyle m_{\mathrm {bob} }+m_{\mathrm {rod} ))$, and the other parameters being ${\displaystyle r_{\mathrm {CM} }={\frac {m_{\mathrm {bob} }+m_{\mathrm {rod} )){m_{\mathrm {bob} }+2m_{\mathrm {rod} ))}\ell }$ and ${\displaystyle I_{O}=m_{\mathrm {bob} }\ell ^{2}+{\frac {1}{3))m_{\mathrm {rod} }\ell ^{2))$, so the expression reduces to:

${\displaystyle {\omega _{0))^{2}={\frac {mgr_{\mathrm {CM} )){I_{O))}={\frac {(m_{\mathrm {bob} }+m_{\mathrm {rod} })g\,{\frac {m_{\mathrm {bob} }+m_{\mathrm {rod} )){m_{\mathrm {bob} }+2m_{\mathrm {rod} ))}\ell }{m_{\mathrm {bob} }\ell ^{2}+{\frac {1}{3))m_{\mathrm {rod} }\ell ^{2))}={\frac {g}{\ell )){\frac {(m_{\mathrm {bob} }+m_{\mathrm {rod} })^{2)){(m_{\mathrm {bob} }+2m_{\mathrm {rod} })\left(m_{\mathrm {bob} }+{\frac {1}{3))m_{\mathrm {rod} }\right)))={\frac {g}{\ell )){\frac {\left(1+{\frac {m_{\mathrm {rod} )){m_{\mathrm {bob} ))}\right)^{2)){\left(1+2{\frac {m_{\mathrm {rod} )){m_{\mathrm {bob} ))}\right)\left(1+{\frac {1}{3)){\frac {m_{\mathrm {rod} )){m_{\mathrm {bob} ))}\right)))}$. Notice this formula can be particularized into the two previous cases studied before just by considering the mass of the rod or the bob to be zero respectively. Also notice that the formula does not depend on both the mass of the bob and the rod, but on their ratio, ${\displaystyle {\frac {m_{\mathrm {rod} )){m_{\mathrm {bob} ))))$. An approximation can be made for ${\displaystyle {\frac {m_{\mathrm {rod} )){m_{\mathrm {bob} ))}\ll 1}$: ${\displaystyle {\omega _{0))^{2}\approx {\frac {g}{\ell )){\frac {1}{1+{\frac {1}{3)){\frac {m_{\mathrm {rod} )){m_{\mathrm {bob} ))))}\approx {\frac {g}{\ell ))\left(1-{\frac {1}{3)){\frac {m_{\mathrm {rod} )){m_{\mathrm {bob} ))}+\cdots \right)}$

Notice how similar it is to the angular frequency in a spring-mass system with effective mass, and how Rayleigh's value appears.

Physical interpretation of the imaginary period

The Jacobian elliptic function that expresses the position of a pendulum as a function of time is a doubly periodic function with a real period and an imaginary period. The real period is, of course, the time it takes the pendulum to go through one full cycle. Paul Appell pointed out a physical interpretation of the imaginary period:^[16] if θ₀ is the maximum angle of one pendulum and 180° − θ₀ is the maximum angle of another, then the real period of each is the magnitude of the imaginary period of the other.

Coupled pendula

Coupled pendulums can affect each other's motion, either through a direction connection (such as a spring connecting the bobs) or through motions in a supporting structure (such as a tabletop). The equations of motion for two identical simple pendulums coupled by a spring connecting the bobs can be obtained using Lagrangian mechanics.

The kinetic energy of the system is:

$${\displaystyle E_{\text{K))={\frac {1}{2))mL^{2}\left({\dot {\theta ))_{1}^{2}+{\dot {\theta ))_{2}^{2}\right)}$$

${\displaystyle m}$

${\displaystyle L}$

${\displaystyle \theta _{1))$

${\displaystyle \theta _{2))$

The potential energy of the system is:

$${\displaystyle E_{\text{p))=mgL(2-\cos \theta _{1}-\cos \theta _{2})+{\frac {1}{2))kL^{2}(\theta _{2}-\theta _{1})^{2))$$

where ${\displaystyle g}$ is the gravitational acceleration, and ${\displaystyle k}$ is the spring constant. The displacement ${\displaystyle L(\theta _{2}-\theta _{1})}$ of the spring from its equilibrium position assumes the small angle approximation.

The Lagrangian is then

$${\displaystyle {\mathcal {L))={\frac {1}{2))mL^{2}\left({\dot {\theta ))_{1}^{2}+{\dot {\theta ))_{2}^{2}\right)-mgL(2-\cos \theta _{1}-\cos \theta _{2})-{\frac {1}{2))kL^{2}(\theta _{2}-\theta _{1})^{2))$$

$${\displaystyle {\begin{aligned}{\ddot {\theta ))_{1}+{\frac {g}{L))\sin \theta _{1}+{\frac {k}{m))(\theta _{1}-\theta _{2})&=0\\{\ddot {\theta ))_{2}+{\frac {g}{L))\sin \theta _{2}-{\frac {k}{m))(\theta _{1}-\theta _{2})&=0\end{aligned))}$$

Adding and subtracting these two equations in turn, and applying the small angle approximation, gives two harmonic oscillator equations in the variables ${\displaystyle \theta _{1}+\theta _{2))$ and ${\displaystyle \theta _{1}-\theta _{2))$:

$${\displaystyle {\begin{aligned}{\ddot {\theta ))_{1}+{\ddot {\theta ))_{2}+{\frac {g}{L))(\theta _{1}+\theta _{2})&=0\\{\ddot {\theta ))_{1}-{\ddot {\theta ))_{2}+\left({\frac {g}{L))+2{\frac {k}{m))\right)(\theta _{1}-\theta _{2})&=0\end{aligned))}$$

$${\displaystyle {\begin{aligned}\theta _{1}+\theta _{2}&=A\cos(\omega _{1}t+\alpha )\\\theta _{1}-\theta _{2}&=B\cos(\omega _{2}t+\beta )\end{aligned))}$$

$${\displaystyle {\begin{aligned}\omega _{1}&={\sqrt {\frac {g}{L))}\\\omega _{2}&={\sqrt ((\frac {g}{L))+2{\frac {k}{m))))\end{aligned))}$$

and ${\displaystyle A}$, ${\displaystyle B}$, ${\displaystyle \alpha }$, ${\displaystyle \beta }$ are constants of integration.

Expressing the solutions in terms of ${\displaystyle \theta _{1))$ and ${\displaystyle \theta _{2))$ alone:

$${\displaystyle {\begin{aligned}\theta _{1}&={\frac {1}{2))A\cos(\omega _{1}t+\alpha )+{\frac {1}{2))B\cos(\omega _{2}t+\beta )\\\theta _{2}&={\frac {1}{2))A\cos(\omega _{1}t+\alpha )-{\frac {1}{2))B\cos(\omega _{2}t+\beta )\end{aligned))}$$

If the bobs are not given an initial push, then the condition ${\displaystyle {\dot {\theta ))_{1}(0)={\dot {\theta ))_{2}(0)=0}$ requires ${\displaystyle \alpha =\beta =0}$, which gives (after some rearranging):

$${\displaystyle {\begin{aligned}A&=\theta _{1}(0)+\theta _{2}(0)\\B&=\theta _{1}(0)-\theta _{2}(0)\end{aligned))}$$