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  2. Radiation pressure - Wikipedia

    en.wikipedia.org/wiki/Radiation_pressure

    The backward acting force of pressure exerted on the front surface is thus larger than the force of pressure acting on the back. Hence, as the resultant of the two forces, there remains a force that counteracts the motion of the plate and that increases with the velocity of the plate. We will call this resultant 'radiation friction' in brief."

  3. Planck relation - Wikipedia

    en.wikipedia.org/wiki/Planck_relation

    The Planck relation [1] [2] [3] (referred to as Planck's energy–frequency relation, [4] the Planck–Einstein relation, [5] Planck equation, [6] and Planck formula, [7] though the latter might also refer to Planck's law [8] [9]) is a fundamental equation in quantum mechanics which states that the energy E of a photon, known as photon energy, is proportional to its frequency ν: =.

  4. Photon - Wikipedia

    en.wikipedia.org/wiki/Photon

    Seen another way, the photon can be considered as its own antiparticle (thus an "antiphoton" is simply a normal photon with opposite momentum, equal polarization, and 180° out of phase). The reverse process, pair production , is the dominant mechanism by which high-energy photons such as gamma rays lose energy while passing through matter. [ 32 ]

  5. Planck constant - Wikipedia

    en.wikipedia.org/wiki/Planck_constant

    The Planck constant, or Planck's constant, denoted by , [1] is a fundamental physical constant [1] of foundational importance in quantum mechanics: a photon's energy is equal to its frequency multiplied by the Planck constant, and the wavelength of a matter wave equals the Planck constant divided by the associated particle momentum.

  6. Photon gas - Wikipedia

    en.wikipedia.org/wiki/Photon_gas

    This force will be equal to the pressure times the cross sectional area (A) of the piston. This process can be continued at a constant temperature until the photon gas is at a volume V 0. Integrating the force over the distance (x) traveled yields the total work done to create this photon gas at this volume

  7. Solar sail - Wikipedia

    en.wikipedia.org/wiki/Solar_sail

    The force imparted to a solar sail arises from the momentum of photons. The momentum of a photon or an entire flux is given by Einstein's relation: [23] [24] = / where p is the momentum, E is the energy (of the photon or flux), and c is the speed of light. Specifically, the momentum of a photon depends on its wavelength p = h/λ

  8. Photon energy - Wikipedia

    en.wikipedia.org/wiki/Photon_energy

    E is the photon's energy; λ is the photon's wavelength; c is the speed of light in vacuum; h is the Planck constant; The photon energy at 1 Hz is equal to 6.626 070 15 × 10 −34 J, which is equal to 4.135 667 697 × 10 −15 eV.

  9. Coupling constant - Wikipedia

    en.wikipedia.org/wiki/Coupling_constant

    As explained in the introduction, the coupling constant sets the magnitude of a force which behaves with distance as /. The 1 / r 2 {\displaystyle 1/r^{2}} -dependence was first explained by Faraday as the decrease of the force flux : at a point B distant by r {\displaystyle r} from the body A generating a force, this one is proportional to the ...