Light's orbital angular momentum

In summary, the article discusses the possible existence of orbital angular momentum in light, but does not provide evidence to support this claim. There are several different modes for Gaussian beams called Laguerre-Gaussian modes, which exist in classical and quantum mechanics, but the article does not mention whether these modes exist in free space or only in a resonator. Furthermore, the article does not mention the no-hair theorem, which states that there are no other structures that uniquely characterize a black hole.
  • #1
Khashishi
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I read this article, and I'm confused about several things.
http://scitation.aip.org/content/aip/magazine/physicstoday/article/57/5/10.1063/1.1768672

Apparently, light can have orbital angular momentum as well as spin. But I don't see how this is possible, at least in vacuum. Is this in vacuum or a waveguide? (It wasn't too clear in the article or first reference) To have orbital momentum, one has to orbit around something. What is light orbiting around? The article says the center of the beam, but there's nothing there, right?

I see there are various modes for Gaussian beams called Laguerre-Gaussian modes. Do these exist in free space or only in some kind of laser resonator?
 
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  • #2
It can have "orbital" angular momentum in vacuum. You don't need an orbit, in a similar way a massive object can have angular momentum without rotating or orbiting, if its flight direction does not point towards/away from the origin of the coordinate system.
 
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  • #3
I thought of that, but that would mean that the light beam must be diverging/converging quite rapidly. Is this the case for this kind of beam?
 
  • #4
I don't have access to the article here. Orbital angular momentum is a common thing in nuclear transitions, for example.
 
  • #5
I've to read the article first, to say anything about it, but for sure it's highly misleading to talk about orbital and spin angular momentum for a relativistic (classical or quantum) field and particularly for the electromagnetic field, which is a massless vector field, because there is no gauge invariant way to define this split of the total angular momentum (which is of course well defined) for the electromagnetic field.

The correct mathematical treatment is well known as "multipole expansion" in classical electrodynamics. For QED the corresponding mode decomposition of the electromagnetic field operator is the use of simultaneous single-photon eigenstates for energy, and total angular momentum (quantum numbers ##\ell## and ##m## as in the multipole expansion). For a very thorough treatment of this, see

Landau/Lifshitz Vol. 4 (Quantum Electrodynamics).
 
  • #6
Just a layman here, but let me take a stab.

A collapsing star gravitates and has angular momentum. If it becomes a black hole, it still gravitates and has the same angular momentum. But we do not know (and can not know) if the stuff inside the BH has rest mass or if it has all been converted to radiation. But we need not know, because it has the same gravity and angular momentum either way.

By that reasoning, I say light must have angular momentum. Whether that qualifies as "orbital angular momentum" is a different question.
 
  • #7
Of course, light (i.e., the electromagnetic field) has angular momentum. That's well known since the 19th century. It's only impossible to make sense of a split into orbital and spin parts of angular momentum. Only total angular momentum has a physical meaning.

A black hole is defined uniquely by its conserved bulk properties (invariant mass, angular momentum, electric charge). There are (within classical Einstein-Maxwell theory) no other structures characterizing a black hole. This is known as Wheeler's "no-hair theorem".
 

1. What is light's orbital angular momentum?

Light's orbital angular momentum refers to the angular momentum carried by a beam of light as it travels through space. It is a property of light that is related to its spin and direction of motion.

2. How is light's orbital angular momentum measured?

Light's orbital angular momentum is measured using interferometers, which are devices that can detect tiny changes in the phase of light as it travels through space. The phase changes are related to the beam's angular momentum.

3. What is the significance of light's orbital angular momentum?

Light's orbital angular momentum has many practical applications, such as in optical communication and manipulation of small particles. It also plays a role in fundamental physics, as it is related to the behavior of light at the quantum level.

4. Can light's orbital angular momentum be changed?

Yes, light's orbital angular momentum can be changed by altering the properties of the light beam, such as its polarization or spatial profile. This can be done using specialized optical components.

5. How does light's orbital angular momentum affect its interaction with matter?

Light's orbital angular momentum can affect its interaction with matter in various ways, such as influencing the direction and intensity of its absorption, scattering, and emission. This property is used in fields such as spectroscopy and quantum optics.

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