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Orbital angular momentum of light

Orbital angular momentum of light is a astronomy topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand Orbital angular momentum of light rather than just read about it. In short: The orbital angular momentum of light (OAM) is the component of angular momentum of a light beam that is dependent on the field spatial distribution, and not on the polarization. OAM can be split into two types.

Orbital angular momentum of light — main illustration
Orbital angular momentum of light — illustration

Key takeaways

  • Orbital angular momentum of light belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect Orbital angular momentum of light to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Orbital angular momentum of light from memory before moving on to harder problems.

Reference excerpt

The orbital angular momentum of light (OAM) is the component of angular momentum of a light beam that is dependent on the field spatial distribution, and not on the polarization. OAM can be split into two types. The internal OAM is an origin-independent angular momentum of a light beam that can be associated with a helical or twisted wavefront. The external OAM is the origin-dependent angular momentum that can be obtained as cross product of the light beam position (center of the beam) and its total linear momentum. While widely used in laser optics, there is no unique decomposition of spin and orbital angular momentum of light.

Concept

A beam of light carries a linear momentum P {\displaystyle \mathbf {P} } , and hence it can be also attributed an external angular momentum L e = r × P {\displaystyle \mathbf {L} _{e}=\mathbf {r} \times \mathbf {P} } . This external angular momentum depends on the choice of the origin of the coordinate system. If one chooses the origin at the beam axis and the beam is cylindrically symmetric (at least in its momentum distribution), the external angular momentum will vanish. The external angular momentum is a form of OAM, because it is unrelated to polarization and depends on the spatial distribution of the optical field (E). A more interesting example of OAM is the internal OAM appearing when a paraxial light beam is in a so-called "helical mode". Helical modes of the electromagnetic field are characterized by a wavefront that is shaped as a helix, with an optical vortex in the center, at the beam axis (see figure). If the phase varies around the axis of such a wave, it carries orbital angular momentum. In the figure to the right, the first column shows the beam wavefront shape. The second column is the optical phase distribution in a beam cross-section, shown in false colors. The third column is the light intensity distribution in a beam cross-section (with a dark vortex core at the center). The helical modes are characterized by an integer number m {\displaystyle m} , positive or negative. If m = 0 {\displaystyle m=0} , the mode is not helical and the wavefronts are multiple disconnected surfaces, for example, a sequence of parallel planes (from which the name "plane wave"). If m = ± 1 {\displaystyle m=\pm 1} , the handedness determined by the sign of m {\displaystyle m} , the wavefront is shaped as a single helical surface, with a step length equal to the wavelength λ {\displaystyle \lambda } . If | m | ⩾ 2 {\displaystyle |m|\geqslant 2} , the wavefront is composed of | m | {\displaystyle |m|} distinct but intertwined helices, with the step length of each helix surface equal to | m | λ {\displaystyle |m|\lambda } , and a handedness given by the sign of m {\displaystyle m} . The integer m {\displaystyle m} is also the so-called "topological charge" of the optical vortex. Light beams that are in a helical mode carry nonzero OAM. As an example, any Laguerre-Gaussian mode with rotational mode number l ≠ 0 {\displaystyle l\neq 0} has such a helical wavefront.

Formulation The classical expression of the orbital angular momentum is the following:

L = ϵ 0 ∑ i = x , y , z ∫ ( E i ( r × ∇ ) A i ) d 3 r , {\displaystyle \mathbf {L} =\epsilon _{0}\sum _{i=x,y,z}\int \left(E^{i}\left(\mathbf {r} \times {\boldsymbol {\nabla }}\right)A^{i}\right)d^{3}\mathbf {r} ,}

where E {\displaystyle \mathbf {E} } and A {\displaystyle \mathbf {A} } are the electric field and the vector potential, respectively, ϵ 0 {\displaystyle \epsilon _{0}} is the vacuum permittivity and we are using SI units. The i {\displaystyle i} -superscripted symbols denote the cartesian components of the corresponding vectors. For a monochromatic wave this expression can be transformed into the following one:

… excerpt ends here. Continue reading the full article.

Illustrations

Orbital angular momentum of light: Different columns show the beam helical structures, phase fronts, and corresponding intensity distributions.
Different columns show the beam helical structures, phase fronts, and corresponding intensity distributions.
Orbital angular momentum of light: A light beam with a given orbital angular momentum (OAM) can be generated by letting a standard Gaussian beam impinge on a display of a spatial light modulator (SLM). If the phase profile on SLM is flat, the SLM works effectively as a mirror. If the phase has a helical profile, the resulting beam is a Laguerre-Gaussian (LG) beam with a well-defined OAM. In real applications, there is a non-negligible admixture in the reflected beam in the form of a Gaussian beam. One can get rid of it by superposing the helical phase on the SLM with a diffraction grating.
A light beam with a given orbital angular momentum (OAM) can be generated by letting a standard Gaussian beam impinge on a display of a spatial light modulator (SLM). If the phase profile on SLM is flat, the SLM works effectively as a mirror. If the phase has a helical profile, the resulting beam is a Laguerre-Gaussian (LG) beam with a well-defined OAM. In real applications, there is a non-negligible admixture in the reflected beam in the form of a Gaussian beam. One can get rid of it by superposing the helical phase on the SLM with a diffraction grating.

Worked examples

Example 1 — a first encounter with Orbital angular momentum of light

Start with the simplest possible case. Write down what Orbital angular momentum of light claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In astronomy, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to Orbital angular momentum of light before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about Orbital angular momentum of light ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of Orbital angular momentum of light

In research
Orbital angular momentum of light appears in astronomy research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses Orbital angular momentum of light in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
Orbital angular momentum of light is common in secondary-school and first-year university syllabi. It links to neighbouring topics Angular momentum of light, Light, Orbital angular momentum of waves, so understanding it makes those chapters shorter.
In everyday life
Look for Orbital angular momentum of light outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.
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How to study Orbital angular momentum of light in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Orbital angular momentum of light means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain Orbital angular momentum of light out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Orbital angular momentum of light in simple terms?

The orbital angular momentum of light (OAM) is the component of angular momentum of a light beam that is dependent on the field spatial distribution, and not on the polarization. OAM can be split into two types.

Why does Orbital angular momentum of light matter?

Because it connects several astronomy ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study Orbital angular momentum of light?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on Orbital angular momentum of light.

Tags

  • Angular momentum of light
  • Light
  • Orbital angular momentum of waves

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