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originally posted by: Arbitrageur
originally posted by: spy66
Will a photon change property/wavelength as soon as it hits an object and reflects of it and moves on until the photon hits an other abject?
Light is one reason to why we can observe motion compared to stationary Objects.
Light is also the main Source we use to observe changes in matter.
Light is also Our main Source of time.
originally posted by: dragonridr
originally posted by: spy66
Will a photon change property/wavelength as soon as it hits an object and reflects of it and moves on until the photon hits an other abject?
Light is one reason to why we can observe motion compared to stationary Objects.
Light is also the main Source we use to observe changes in matter.
Light is also Our main Source of time.
Would it surprise you if i told you a photon doesnt reflect off an object? It is a copy of the EM field that we see as reflected light.
Do you mean change in direction? If that's not what you mean, what kind of change are you talking about? I'm not seeing any wavelength (color) changes in this photograph in the reflection, are you?
A photon would still change right?
originally posted by: Arbitrageur
a reply to: spy66
Do you mean change in direction? If that's not what you mean, what kind of change are you talking about? I'm not seeing any wavelength (color) changes in this photograph in the reflection, are you?
A photon would still change right?
There are only a handful of videos of Richard Feynman's lectures. Four are from his university of Auckland lectures and one of them is on reflection of light. He describes the problems with classical wave theory, and classical particle theory and how they both fell short of explaining specific reflection behavior for centuries since Newton, so it's not the simplest topic. Then he describes how we can model what happens in reflection, though he admits it's not an intuitive model, like the rest of quantum mechanics.
QED: Fits of Reflection and Transmission -- Quantum Behaviour -- Richard Feynman (2/4)
Compton scattering is an inelastic scattering of a photon by a quasi-free charged particle, usually an electron. It results in a decrease in energy (increase in wavelength) of the photon (which may be an X-ray or gamma ray photon), called the Compton effect. Part of the energy of the photon is transferred to the recoiling electron. Inverse Compton scattering also exists, in which a charged particle transfers part of its energy to a photon.
The concept we disagreed with was your idea that a single photon would expand in all directions. It doesn't.
We need to draw a distinction between the photon itself, and the wavefunction of the photon. To say the wavefunction spreads out is correct, but the photon itself does not spread out.
originally posted by: Astyanax
a reply to: Arbitrageur
The concept we disagreed with was your idea that a single photon would expand in all directions. It doesn't.
That's not strictly true.
The photon wavefunction gives nonzero probability values for position at all locations; it isn't until the photon is detected that we can say which direction it went.
Let me repeat for emphasis:
experiments confirm that the photon is not a short pulse of electromagnetic radiation; it does not spread out as it propagates
Do we teach this in graduate school? Yes. As dragonridr said we teach graduate students the Copenhagen interpretation as if it's true without much emphasis on alternative interpretations (That I'm aware of).
originally posted by: Astyanax
There's no photon till it's detected. Until then, there's only a wavefunction.
So if this interpretation is correct, there is a photon before it's detected, and the wavefunction is guiding it.
The de Broglie–Bohm theory of quantum mechanics is a theory by Louis de Broglie and extended later by David Bohm to include measurements. Particles, which always have positions, are guided by the wavefunction. The wavefunction evolves according to the Schrödinger wave equation, and the wavefunction never collapses. The theory takes place in a single space-time, is non-local, and is deterministic. The simultaneous determination of a particle's position and velocity is subject to the usual uncertainty principle constraint. The theory is considered to be a hidden variable theory, and by embracing non-locality it satisfies Bell's inequality. The measurement problem is resolved, since the particles have definite positions at all times.
originally posted by: spy66
a reply to: dragonridr
I have another question:
A photon can not have mass, if it did it would not travel With the exact speed of light c in a vacuum.
A photon has no electrical charge and is therefor stable. That means it is a constant from E.
Can you explain to me how, or at what time in the light cone time frame a photon gets its spin?
Would the photon have a spin already in the past light cone, or would the photon recieve the spin and vector from the Object it interacts With before it becomes the New light cone?
Or does the photon spin just change vector constantly at the speed of light "as it interects with With the motion and electrical charge of a particle"?
- What i mean is: From the past light cone a Photon brings With it a vector and spin, and when it interact With a particle it changes vector and momentom and becomes the New light cone.
Is this true?
If it true, the photons does change both its momentom and vector when it interacts With a particle.
The light cone i am refering to: "The past light cone E is the future light cone inverted at the constant speed of light".
In deBroglie-Bohm, the photon you detected on earth from 12 billion years ago was traveling in the direction of where the Earth would eventually be now, for the 12 billion years. You can't say there was no photon before the observation, because in the DeBroglie-Bohm interpretation there was, and there is no wave-function collapse upon observation as there is in the Copenhagen interpretation.
originally posted by: Astyanax
The same problem arises in the de Broglie-Bohm interpretation. 'The 'photon is always somewhere, but where is it? How do you tell it apart from all the others emitted by the source?
So let's say .01 light seconds before you detect the photon, it was .01 light seconds away from your detector according to deBroglie-Bohm. Maybe you didn't know where it was then, but you know now where it was then and it wasn't equally likely to have been 80 billion light years away, as the Copenhagen interpretation of wave function collapse might suggest.