Momentum of a Massless Particle
Most recent answer: 10/17/2013
- Anushka (age 16)
India
I've marked this as a follow-up to ones that may answer it. The key is to pay attention to the different uses of the symbol "m", either as rest-mass or as the factor in p=mv.
"How do we know the momentum of a massless particle?" There are several ways. One is to directly measure the momentum by measuring, for example, the force exerted on a mirror by a stream of photons. Here one uses that p is conserved and also that the particle number can be determined using universal quantum relation E=hf, where E is energy, h is Planck's constant, and f is frequency. Another way is to use an argument from Maxwell's equations that requires E=pc if momentum is to be conserved. That gives a momentum density in terms of the electric and magnetic fields. It can be converted to a momentum per particle again using E=hf. Another way is to look for the missing momentum in events involving a few massive particles and a photon or two. Other ways include using the universal quantum relation |p|=h/λ, where λ is the wavelength. λ can be measured with diffraction gratings or other methods.
Mike W.
(published on 06/04/2013)
Follow-Up #1: photon mass again
- Anushka (age 16)
This is a familiar question. I've put it in the right thread.
Here's the key point to re-emphasize, once you've gone over our old answers. The "m" your teacher got, hv/c2 , is the mass that photon would contribute to the total mass of a bag of photons with zero net momentum. That inertial mass is not generally the same as the invariant (rest) mass for a single particle, but it has a great property. The sum of the inertial masses for a collection of non-interacting particles is the same as the inertial mass of the collection as a whole. That's not close to being true for the invariant masses.
Mike W.
(published on 06/21/2013)
Follow-Up #2: Does the Earth bend light?
- Jess (age 13)
Sydney, NSW, Australia
You can follow the rest of this thread to get the basic physics. Yes, the earth bends light. The maximum angle is roughly gR/c2, where g is the gravitational acceleration at the surface and R is the Earth's radius. That comes out to about 10-9 radians, so it's not a big effect. The bending as light goes near the Sun is much bigger. It was first observed in 1919, fitting the prediction of general relativity.
Mike W.
(published on 07/30/2013)
Follow-Up #3: light and gravity again
- Hinerangi (age 16)
Auckland, New Zealand
see above
(published on 08/07/2013)
Follow-Up #4: cosmic speed limit
- Chris Whyley (age 53)
Swansea United Kingdom
Maybe the earlier parts of this thread will help.
Mike W.
(published on 10/17/2013)