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  2. Spin angular momentum of light - Wikipedia

    en.wikipedia.org/wiki/Spin_angular_momentum_of_light

    The general expression for the spin angular momentum is [1] =, where is the speed of light in free space and is the conjugate canonical momentum of the vector potential.The general expression for the orbital angular momentum of light is =, where = {,,,} denotes four indices of the spacetime and Einstein's summation convention has been applied.

  3. Quantization of the electromagnetic field - Wikipedia

    en.wikipedia.org/wiki/Quantization_of_the...

    The photon having non-zero linear momentum, one could imagine that it has a non-vanishing rest mass m 0, which is its mass at zero speed. However, we will now show that this is not the case: m 0 = 0. Since the photon propagates with the speed of light, special relativity is called for. The relativistic expressions for energy and momentum ...

  4. Photodisintegration - Wikipedia

    en.wikipedia.org/wiki/Photodisintegration

    In explosions of very large stars (250 or more solar masses), photodisintegration is a major factor in the supernova event. As the star reaches the end of its life, it reaches temperatures and pressures where photodisintegration's energy-absorbing effects temporarily reduce pressure and temperature within the star's core.

  5. Photon - Wikipedia

    en.wikipedia.org/wiki/Photon

    According to VMD, the photon is a superposition of the pure electromagnetic photon, which interacts only with electric charges, and vector mesons, which mediate the residual nuclear force. [108] However, if experimentally probed at very short distances, the intrinsic structure of the photon appears to have as components a charge-neutral flux of ...

  6. Photon structure function - Wikipedia

    en.wikipedia.org/wiki/Photon_structure_function

    Photons with high photon energy can transform in quantum mechanics to lepton and quark pairs, the latter fragmented subsequently to jets of hadrons, i.e. protons, pions, etc.At high energies E the lifetime t of such quantum fluctuations of mass M becomes nearly macroscopic: t ≈ E/M 2; this amounts to flight lengths as large as one micrometer for electron pairs in a 100 GeV photon beam, while ...

  7. Radiation pressure - Wikipedia

    en.wikipedia.org/wiki/Radiation_pressure

    The radiation pressure again can be seen as the transfer of each photon's momentum to the opaque surface, plus the momentum due to a (possible) recoil photon for a (partially) reflecting surface. Since an incident wave of irradiance I f over an area A has a power of I f A , this implies a flux of I f / E p photons per second per unit area ...

  8. Neutrino theory of light - Wikipedia

    en.wikipedia.org/wiki/Neutrino_theory_of_light

    The neutrino theory of light is the proposal that the photon is a composite particle formed of a neutrino–antineutrino pair.It is based on the idea that emission and absorption of a photon corresponds to the creation and annihilation of a particle–antiparticle pair.

  9. Recombination (cosmology) - Wikipedia

    en.wikipedia.org/wiki/Recombination_(cosmology)

    Shortly after recombination, the photon mean free path became larger than the Hubble length, and photons traveled freely without interacting with matter. [16] For this reason, recombination is closely associated with the last scattering surface, which is the name for the last time at which the photons in the cosmic microwave background ...