{{Expert-portal|Physics}}

[[Image:Gyroskop.jpg|thumb|right|200px|This [[gyroscope]] remains upright while spinning due to its angular momentum.]]

In [[physics]], the '''angular momentum''' of an object rotating about some reference point is the measure of the extent to which the object will continue to rotate about that point unless acted upon by an external [[torque]]. In particular, if a point mass rotates about an axis, then the angular momentum with respect to a point on the axis is related to the [[mass]] of the object, the velocity and the distance of the mass to the axis. While the motion associated with linear momentum has no absolute [[frame of reference]], the [[rotation]] associated with angular momentum is sometimes spoken of as being measured relative to the [[fixed stars]].

Angular momentum is important in physics because it is a [[Conservation law|conserved]] quantity: a system's angular momentum stays constant unless an external [[torque]] acts on it. Torque is the rate at which angular momentum is transferred in or out of the system. When a rigid body rotates, its resistance to a change in its rotational motion is measured by its [[moment of inertia]]. Angular momentum is an important concept in both physics and engineering, with numerous applications. For example, the [[kinetic energy]] stored in a massive rotating object such as a [[flywheel]] is proportional to the square of the angular momentum. Conservation of angular momentum also explains many phenomena in sports and nature.

== Angular momentum in classical mechanics ==
[[Image:Torque_animation.gif|frame|right|Relationship between force (F), [[torque]] (τ), and momentum vectors (p and L) in a rotating system]]
===Definition===

Angular momentum of a particle about a given origin is defined as:

:<math>\mathbf{L}=\mathbf{r}\times\mathbf{p}</math>

where:

:<math>\mathbf{L}</math> is the angular momentum of the particle,
:<math>\mathbf{r}</math> is the position of the particle expressed as a displacement vector from the origin,
:<math>\mathbf{p}</math> is the [[Momentum|linear momentum]] of the particle, and
:<math>\times\,</math> is the vector [[cross product]].

As seen from the definition, the [[derived SI unit]]s of angular momentum are [[newton]]·[[metre]]·[[second]]s (N·m·s or kg·m²s^-1). Because of the cross product, '''L''' is a [[pseudovector]] perpendicular to both the radial vector '''r''' and the momentum vector '''p''' and it is assigned a sign by the [[right-hand rule]].

If a system consists of several particles, the total angular momentum about an origin can be obtained by adding (or integrating) all the angular momenta of the constituent particles. Angular momentum can also be calculated by multiplying the square of the displacement ''r'', the [[mass]] of the particle and the [[angular velocity]].

=== Orbital and spin angular momentum ===

It is very often convenient to consider the angular momentum of a collection of particles about their [[center of mass]], since this simplifies the mathematics considerably. The angular momentum of a collection of particles is the sum of the angular momentum of each particle:

:<math>\mathbf{L}=\sum_i \mathbf{R}_i\times m_i \mathbf{V}_i</math>

where <math>R_i</math> is the distance of particle ''i'' from the reference point, <math>m_i</math> is its mass, and <math>V_i</math> is its velocity. The center of mass is defined by:

:<math>\mathbf{R}=\frac{1}{M}\sum_i m_i \mathbf{R}_i</math>

where the total mass of all particles is given by

:<math>M=\sum_i m_i\,</math>

It follows that the velocity of the center of mass is

:<math>\mathbf{V}=\frac{1}{M}\sum_i m_i \mathbf{V}_i\,</math>

If we define <math>\mathbf{r}_i</math> as the displacement of particle ''i'' from the center of mass, and <math>\mathbf{v}_i</math> as the velocity of particle ''i'' with respect to the center of mass, then we have

:<math>\mathbf{R}_i=\mathbf{R}+\mathbf{r}_i\,</math>&nbsp;&nbsp; and &nbsp;&nbsp; <math>\mathbf{V}_i=\mathbf{V}+\mathbf{v}_i\,</math>

and also

:<math>\sum_i m_i \mathbf{r}_i=0\,</math>&nbsp;&nbsp; and &nbsp;&nbsp; <math>\sum_i m_i \mathbf{v}_i=0\,</math>

so that the total angular momentum is

:<math>\mathbf{L}=\sum_i (\mathbf{R}+\mathbf{r}_i)\times m_i (\mathbf{V}+\mathbf{v}_i) = \left(\mathbf{R}\times M\mathbf{V}\right) + \left(\sum_i \mathbf{r}_i\times m_i \mathbf{v}_i\right)</math>

The first term is just the angular momentum of the center of mass. It is the same angular momentum one would obtain if there were just one particle of mass ''M'' moving at velocity '''V''' located at the center of mass. The second term is the angular momentum that is the result of the particles spinning about their center of mass. This second term can be even further simplified if the particles form a [[rigid body]]. An analogous result is obtained for a continuous distribution of matter.

=== Fixed axis of rotation ===

For many applications where one is only concerned about rotation around one axis, it is sufficient to discard the pseudovector nature of angular momentum, and treat it like a scalar where it is positive when it corresponds to a counter-clockwise rotations, and negative clockwise. To do this, just take the definition of the cross product and discard the unit vector, so that angular momentum becomes:

:<math>L = |\mathbf{r}||\mathbf{p}|\sin \theta_{r,p}</math>

where '''&theta;_r,p''' is the angle between '''r''' and '''p''' measured from '''r''' to '''p'''; an important distinction because without it, the sign of the cross product would be meaningless. From the above, it is possible to reformulate the definition to either of the following:

:<math>L = \pm|\mathbf{p}||\mathbf{r}_{\perp}|</math>

where '''r'''_&perp; is called the ''[[lever]] arm distance'' to '''p'''.

The easiest way to conceptualize this is to consider the lever arm distance to be the distance from the origin to the line that '''p''' travels along. With this definition, it is necessary to consider the direction of '''p''' (pointed clockwise or counter-clockwise) to figure out the sign of L. Equivalently:

:<math>L = \pm|\mathbf{r}||\mathbf{p}_{\perp}|</math>

where '''p'''_&perp; is the component of '''p''' that is perpendicular to '''r'''. As above, the sign is decided based on the sense of rotation.

For an object with a fixed mass that is rotating about a fixed symmetry axis,
the angular momentum is expressed as the product of the [[moment of inertia]] of the object and its angular
velocity vector:

:<math>\mathbf{L}= I \mathbf{\omega} </math>

where
:<math>I\,</math> is the [[moment of inertia]] of the object (in general, a [[tensor]] quantity)
:<math>\mathbf{\omega}</math> is the [[angular velocity]].

===Conservation of angular momentum===<!-- This section is linked from [[Conservation law]] -->
[[Image:PrecessionOfATop.svg|thumb|right|250px|The [[torque]] caused by the two opposing forces '''F'''_g and -'''F'''_g causes a change in the angular momentum '''L''' in the direction of that torque (since torque is the time derivative of angular momentum). This causes the top to [[precess]].]]

In a closed system angular momentum is constant. This conservation law mathematically follows from continuous directional symmetry of space (no direction in space is any different from any other direction). See [[Noether's theorem]].

The time derivative of angular momentum is called [[torque]]:

:<math>\tau = \frac{\mathrm{d}\mathbf{L}}{\mathrm{d}t} = \mathbf{r} \times \frac{\mathrm{d}\mathbf{p}}{\mathrm{d}t} = \mathbf{r} \times \mathbf{F} </math>

So requiring the system to be "closed" here is mathematically equivalent to zero external torque acting on the system:

:<math>\mathbf{L}_{\mathrm{system}} = \mathrm{constant} \leftrightarrow \sum \tau_{\mathrm{ext}} = 0 </math>

where <math>\tau_{ext}</math> is any torque applied to the system of particles.

In orbits, the angular momentum is distributed between the spin of the planet itself and the angular momentum of its orbit:

:<math>\mathbf{L}_{\mathrm{total}} = \mathbf{L}_{\mathrm{spin}} + \mathbf{L}_{\mathrm{orbit}}
</math>;

If a planet is found to rotate slower than expected, then astronomers suspect that the planet is accompanied by a satellite, because the total angular momentum is shared between the planet and its satellite in order to be conserved.

The conservation of angular momentum is used extensively in analyzing what is called ''central force motion''. If the net force on some body is directed always toward some fixed point, the ''center'', then there is no torque on the body with respect to the center, and so the angular momentum of the body about the center is constant. Constant angular momentum is extremely useful when dealing with the [[orbit]]s of [[planet]]s and [[satellite]]s, and also when analyzing the [[Bohr model]] of the [[atom]].

The conservation of angular momentum explains the angular acceleration of an ice skater as she brings her arms and legs close to the vertical axis of rotation. By bringing part of mass of her body closer to the axis she decreases her body's moment of inertia. Because angular momentum is constant in the absence of external torques, the angular velocity (rotational speed) of the skater has to increase.

The same phenomenon results in extremely fast spin of compact stars (like [[white dwarf]]s, [[neutron star]]s and [[black hole]]s) when they are formed out of much larger and slower rotating stars (indeed, decreasing the size of object 10⁴ times results in increase of its angular velocity by the factor 10⁸).

The conservation of angular momentum in Earth-Moon system results in the transfer of angular momentum from Earth to Moon (due to tidal torque Moon exerts of Earth). This in turn results in the slowing down of the rotation rate of Earth (at about 42 nsec/day), and in gradual increase of the radius of Moon's orbit (at ~4.5 cm/year rate).

== Angular momentum in relativistic mechanics ==

In modern (late [[20th century]]) theoretical physics, angular momentum is described using a different formalism. Under this formalism, angular momentum is the [[2-form]] [[Noether charge]] associated with rotational invariance (As a result, angular momentum is not conserved for general curved spacetimes, unless it happens to be asymptotically rotationally invariant). For a system of point particles without any intrinsic angular momentum, it turns out to be

:<math>\sum_i \bold{r}_i\wedge \bold{p}_i</math>

(Here, the [[wedge product]] is used.).

== Angular momentum in quantum mechanics ==

In [[quantum mechanics]], angular momentum is [[Quantization (physics)|quantized]] -- that is, it cannot vary continuously, but only in "[[quantum leap]]s" between certain allowed values. The angular momentum of a subatomic particle, due to its motion through space, is always a whole-number multiple of <math>\hbar</math> ("h-bar"), defined as [[Planck's constant]] divided by 2π. Furthermore, experiments show that most subatomic particles have a permanent, built-in angular momentum, which is not due to their motion through space. This [[spin (physics)|spin]] angular momentum comes in units of <math>\hbar/2</math>. For example, an electron standing at rest has an angular momentum of <math>\hbar/2</math>.

===Basic definition===
The classical definition of angular momentum as <math>\mathbf{L}=\mathbf{r}\times\mathbf{p}</math> depends on six numbers: <math>r_x</math>, <math>r_y</math>, <math>r_z</math>, <math>p_x</math>, <math>p_y</math>, and <math>p_z</math>. Translating this into quantum-mechanical terms, the [[uncertainty principle|Heisenberg uncertainty principle]] tells us that it is not possible for all six of these numbers to be measured simultaneously with arbitrary precision. Therefore, there are limits to what can be known or measured about a particle's angular momentum. It turns out that the best that one can do is to simultaneously measure both the angular momentum vector's magnitude and its component along one axis.

Mathematically, angular momentum in quantum mechanics is defined like [[momentum# Momentum in quantum mechanics|momentum]] - not as a quantity but as an [[operator]] on the [[wave function]]:

:<math>\mathbf{L}=\mathbf{r}\times\mathbf{p}</math>

where '''r''' and '''p''' are the position and momentum operators respectively. In particular, for a single particle with no [[electric charge]] and no [[spin (physics)|spin]], the [[angular momentum operator]] can be written in the position basis as

:<math>\mathbf{L}=-i\hbar(\mathbf{r}\times\nabla)</math>

where <math>\nabla</math> is the [[gradient]] operator, read as "del," "grad," or "nabla". This ''orbital angular momentum operator'' is the most commonly encountered form of the angular momentum operator, though not the only one. It satisfies the following '''commutation relations'''
:<math>[L_i, L_j ] = i \hbar \epsilon_{ijk} L_k</math>,

where &epsilon;_ijk is the (antisymmetric) [[Levi-Civita symbol]].
From this follows
:<math>\left[L_i, L^2 \right] = 0</math>

Since,
:<math>L_x = -i\hbar (y {\partial\over \partial z} - z {\partial\over \partial y})</math>
:<math>L_y = -i\hbar (z {\partial\over \partial x} - x {\partial\over \partial z})</math>
:<math>L_z = -i\hbar (x {\partial\over \partial y} - y {\partial\over \partial x})</math>

it follows, for example,
:<math>\begin{align}
\left[L_x,L_y\right] & = -\hbar^2 \left( (y {\partial \over \partial z} - z {\partial\over \partial y})(z {\partial\over \partial x} - x {\partial\over \partial z}) - (z {\partial\over \partial x} - x {\partial\over \partial z})(y {\partial \over \partial z} - z {\partial\over \partial y})\right) \\
& = -\hbar^2 \left( y {\partial\over \partial x} - x {\partial\over \partial y}\right) = i \hbar L_z. \\
\end{align}</math>

===Addition of quantized angular momenta===
{{details|Clebsch-Gordan coefficients}}
Given a quantized total angular momentum <math>\overrightarrow{j}</math> which is the sum of two individual quantized angular momenta <math>\overrightarrow{l_1}</math> and <math>\overrightarrow{l_2}</math>,

:<math>\overrightarrow{j} = \overrightarrow{l_1} + \overrightarrow{l_2}</math>

the [[quantum number]] <math>j</math> associated with its magnitude can range from <math>|l_1 - l_2|</math> to <math>l_1 + l_2</math> in integer steps
where <math>l_1</math> and <math>l_2</math> are quantum numbers corresponding to the magnitudes of the individual angular momenta.
^^

===Angular momentum as a generator of rotations===
If <math>\phi</math> is the angle around a specific axis, for example the azimuthal angle around the z axis, then the angular momentum along this axis is the [[Noether's theorem|generator]] of rotations around this axis:
:<math>L_z = -i\hbar {\partial\over \partial \phi}.</math>

The [[eigenfunction]]s of L_z are therefore <math>e^{i m_l \phi}</math>, and since <math>\phi</math> has a period of <math>2\pi</math>, m_l must be an integer.

For a particle with a [[Spin (physics)|spin]] '''S''', this takes into account only the angular dependence of the location of the particle, for example its orbit in an atom. It is therefore known as [[orbital angular momentum]]. However, when one rotates the system, one also changes the [[Spin (physics)|spin]]. Therefore the [[total angular momentum]], which is the full [[Noether's theorem|generator]] of rotations, [[Azimuthal_quantum_number#Total_angular_momentum_of_an_electron_in_the_atom|is]]
<math>J_i = L_i + S_i</math>
Being an angular momentum, '''J''' satisfies the same commutation relations as L, as will explained below. namely
:<math>[J_i, J_j ] = i \hbar \epsilon_{ijk} J_k</math>
from which follows
:<math>\left[J_i, J^2 \right] = 0.</math>

Acting with J on the [[wavefunction]] <math>\psi</math> of a particle generates a rotation:
<math>e^{i \phi J_z} \psi</math> is the [[wavefunction]] <math>\psi</math> rotated around the z axis by an angle <math>\phi</math>. For an infinitesmal rotation by an angle <math>d\phi</math>, the rotated [[wavefunction]] is <math>\psi+ i d\phi J_z \psi</math>. This is similarly true for rotations around any axis.

In a charged particle the momentum [[Momentum#Momentum_in_electromagnetism|gets a contribution from the electromagnetic field]], and the angular momenta '''L''' and '''J''' change accordingly.

If the [[Hamiltonian (quantum mechanics)|Hamiltonian]] is invariant under rotations, as in spherically symmetric problems, then according to [[Noether's theorem]], it [[commutator|commutes]] with the [[total angular momentum]]. So the total angular momentum is a [[conserved quantity]]
:<math>\left[J_i, H \right] = 0</math>

Since angular momentum is the generator of rotations, its commutation relations follow the commutation relations of the generators of the three-dimensional [[rotation group]] [[Orthogonal group|SO(3)]]. This is why '''J''' always satisfies these commutation relations. In '''d''' dimensions, the angular momentum will satisfy the same commutation relations as the generators of the '''d'''-dimensional rotation group [[Orthogonal group|SO(d)]].

[[SO(3)]] has the same [[Lie algebra]] (i.e. the same commutation relations) as [[SU(2)]]. Generators of [[SU(2)]] can have half-integer [[eigenvalues]], and so can m<math>j</math>. Indeed for [[fermion]]s the [[Spin (physics)|spin]] '''S''' and [[total angular momentum]] '''J''' are half-integer. In fact this is the most general case: j and m<math>j</math> are either integers or half-integers.

Technically, this is because the [[universal cover]] of SO(3) is [[isomorphic]] [[SU(2)]], and the [[Representation theory of SU(2)|representation]]s of the latter are fully known. '''J_i''' span the [[Lie algebra]] and '''J²''' is the [[Casimir invariant]], and it can be shown that if the [[eigenvalues]] of '''J_z''' and '''J²''' are m_j and j(j+1) then m_j and j are both integer multiples of one-half. j is non-negative and m_j takes values between -j and j.

===Relation to [[spherical harmonics]]===
Angular momentum operators usually occur when solving a problem with [[spherical symmetry]] in [[spherical coordinates]]. Then, the angular momentum in space representation is:
:: <math>L^2 = -\frac{\hbar^2}{\sin\theta}\frac{\partial}{\partial \theta}\left( \sin\theta \frac{\partial}{\partial \theta}\right) - \frac{\hbar^2}{\sin^2\theta}\frac{\partial^2}{\partial \phi^2} </math>
When solving to find [[eigenstate]]s of this operator, we obtain the following
:: <math> L^2 | l, m \rang = {\hbar}^2 l(l+1) | l, m \rang </math>
:: <math> L_z | l, m \rang = \hbar m | l, m \rang </math>
where
::<math> \lang \theta , \phi | l, m \rang = Y_{l,m}(\theta,\phi)</math>
are the [[spherical harmonic]]s.

==Angular momentum in electrodynamics==
When describing the motion of a charged particle in the presence of an [[electromagnetic field]], the "kinetic momentum" ''p'' is not [[gauge invariant]]. As a consequence, the canonical angular momentum <math> \mathbf{L} = \mathbf{r} \times \mathbf{p} </math> is not gauge invariant either. Instead, the momentum that is physical, the so-called [[canonical momentum]], is

:<math> \mathbf{p} -\frac {e \mathbf{A} }{c}</math>

where <math>e</math> is the [[electric charge]], ''c'' the [[speed of light]] and ''A'' the [[vector potential]]. Thus, for example, the [[Hamiltonian (quantum mechanics)|Hamiltonian]] of a charged particle of mass ''m'' in an electromagnetic field is then

:<math> H =\frac{1}{2m} \left( \mathbf{p} -\frac {e \mathbf{A} }{c}\right)^2 + e\phi</math>

where <math>\phi</math> is the [[scalar potential]]. This is the Hamiltonian that gives the [[Lorentz force law]]. The gauge-invariant angular momentum, or "kinetic angular momentum" is given by

:<math>K= \mathbf{r} \times \left( \mathbf{p} -\frac {e \mathbf{A} }{c}\right)</math>

The interplay with quantum mechanics is discussed further in the article on [[canonical commutation relation]]s.

== See also ==

* [[Moment of Inertia]]
* [[Angular momentum coupling]]
* [[Areal velocity]]
* [[Control moment gyroscope]]
* [[Rotational energy]]
* [[Rigid rotor]]
* [[Yrast]]
* [[Noether's theorem]]

==External links==

*[http://www.lightandmatter.com/html_books/2cl/ch05/ch05.html Conservation of Angular Momentum] - a chapter from an online textbook

*[http://www.hakenberg.de/diffgeo/collision_resolution.htm Angular Momentum in a Collision Process] - derivation of the three dimensional case

==References==
* E. U. Condon and G. H. Shortley, ''The Theory of Atomic Spectra'', (1935) Cambridge at the University Press, ISBN 0-521-09209-4 ''See chapter 3''.
* Edmonds, A.R., ''Angular Momentum in Quantum Mechanics'', (1957) Princeton University Press, ISBN 0-691-07912-9.
*{{cite book | author=Serway, Raymond A.; Jewett, John W. | title=Physics for Scientists and Engineers (6th ed.) | publisher=Brooks/Cole | year=2004 | id=ISBN 0-534-40842-7}}
*{{cite book | author=Tipler, Paul | title=Physics for Scientists and Engineers: Mechanics, Oscillations and Waves, Thermodynamics (5th ed.) | publisher=W. H. Freeman | year=2004 | id=ISBN 0-7167-0809-4}}

[[Category:Fundamental physics concepts]]
[[Category:Physical quantity]]
[[Category:Rotational symmetry]]
[[Category:Conservation laws]]

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