• Thumbnail for Chronology of the universe
    or more photons as they transition to a low energy state. This release of photons is known as photon decoupling. Some of these decoupled photons are captured...
    138 KB (13,925 words) - 00:44, 3 August 2024
  • challenge. Single photon sources exhibit antibunching. As photons are emitted one at a time, the probability of seeing two photons at the same time for...
    26 KB (3,164 words) - 16:17, 6 December 2023
  • Thumbnail for Radiation pressure
    field or in terms of the momenta of photons, particles of light. The interaction of electromagnetic waves or photons with matter may involve an exchange...
    40 KB (5,289 words) - 15:21, 14 July 2024
  • Thumbnail for Huygens–Fresnel principle
    pattern: in dark areas, no photons are landing, and in bright areas, many photons are landing. The set of possible photon paths is consistent with Richard...
    24 KB (3,052 words) - 06:29, 25 July 2024
  • the normal is I photons/(s·m2·sr) and the number of photons per second emitted into the vertical wedge is I dΩ dA. The number of photons per second emitted...
    9 KB (1,266 words) - 01:50, 2 March 2024
  • Thumbnail for Universe
    Universe (section Photons)
    atoms. As a result, photons no longer interacted frequently with matter and the universe became transparent. The highly redshifted photons from this period...
    158 KB (16,428 words) - 09:28, 30 July 2024
  • produced a pair of entangled photons by implementing the process of parametric down-conversion. In order to ensure that the two photons cannot be distinguished...
    84 KB (10,921 words) - 17:13, 28 June 2024
  • \rangle } polarized light, half of the photons are absorbed in both cases. This may make it seem like half of the photons are in state | R ⟩ {\displaystyle...
    36 KB (5,245 words) - 19:07, 29 June 2024
  • Thumbnail for Gravitational redshift
    shift in older literature) is the phenomenon that electromagnetic waves or photons travelling out of a gravitational well lose energy. This loss of energy...
    43 KB (5,976 words) - 20:21, 2 August 2024
  • Thumbnail for Reionization
    provided the photons that reionized the IGM. To ionize neutral hydrogen, an energy larger than 13.6 eV is required, which corresponds to photons with a wavelength...
    50 KB (5,729 words) - 05:08, 12 August 2024
  • Thumbnail for Black hole
    feature any singularities. The photon sphere is a spherical boundary where photons that move on tangents to that sphere would be trapped in a non-stable...
    164 KB (18,501 words) - 04:51, 26 July 2024
  • Thumbnail for Electron
    Electron (category CS1 German-language sources (de))
    be explained by the formation of virtual photons in the electric field generated by the electron. These photons can heuristically be thought of as causing...
    153 KB (15,428 words) - 05:58, 22 July 2024
  • Introduction to quantum mechanics (category CS1 German-language sources (de))
    called photons, and predicts its spectral energies (corresponding to pure colors), and the intensities of its light beams. A single photon is a quantum...
    66 KB (7,480 words) - 07:18, 3 July 2024
  • Thumbnail for Integrating sphere
    calculated. This number is the average number of times a photon is scattered in the sphere, before it is absorbed in the coating or escapes through a...
    19 KB (1,923 words) - 04:27, 26 February 2024
  • Thumbnail for Interstellar medium
    of photons, but often such photons can penetrate throughout the neutral phase and only get absorbed in the outer layers of molecular clouds. Photons with...
    60 KB (7,343 words) - 22:10, 1 August 2024
  • Thumbnail for Stefan–Boltzmann law
    Stefan–Boltzmann law (category CS1 German-language sources (de))
    5205 × 10 15 photons ⋅ s − 1 ⋅ m − 2 ⋅ K − 3 ) ⋅ T 3 {\displaystyle N_{\mathrm {phot} }=\left({1.5205\times 10^{15}}\;{\textrm {photons}}{\cdot }{\textrm...
    38 KB (5,480 words) - 13:36, 4 July 2024
  • Thumbnail for Elementary particle
    particles exist in the visible universe (not including dark matter), mostly photons and other massless force carriers. The Standard Model of particle physics...
    35 KB (3,434 words) - 04:52, 26 July 2024
  • Thumbnail for Future of an expanding universe
    will grow at an increasing rate. Redshift will stretch ancient ambient photons (including gamma rays) to undetectably long wavelengths and low energies...
    51 KB (5,565 words) - 23:45, 8 August 2024
  • Thumbnail for Atom
    be modified through bombardment by high energy subatomic particles or photons. If this modifies the number of protons in a nucleus, the atom changes...
    125 KB (12,755 words) - 12:29, 26 July 2024
  • Thumbnail for Photonic crystal
    1070/QE1975v004n07ABEH009654. Ohtaka, K (1979). "Energy band of photons and low-energy photon diffraction". Physical Review B. 19 (10): 5057–67. Bibcode:1979PhRvB...
    61 KB (7,088 words) - 22:07, 18 May 2024
  • Thumbnail for Ray tracing (graphics)
    some length. Photon mapping is another method that uses both light-based and eye-based ray tracing; in an initial pass, energetic photons are traced along...
    60 KB (7,573 words) - 16:29, 17 July 2024
  • fuel-free relativistic propulsion of large masses via recycled boomerang photons". arXiv:1903.03423 [gr-qc]. Michio Kaku (March 15, 2011). "Physics of the...
    23 KB (1,683 words) - 11:50, 19 July 2024
  • Thumbnail for Planck's law
    Planck's law (category CS1 German-language sources (de))
    interactions (between photons and other particles or even, at sufficiently high temperatures, between the photons themselves) will cause the photon energy distribution...
    141 KB (18,060 words) - 01:42, 9 June 2024
  • Thumbnail for Sievert
    07 mm in the ICRU sphere phantom. Examples of low penetrating radiation are alpha particles, beta particles and low-energy photons. This dose quantity...
    68 KB (6,614 words) - 04:41, 29 June 2024
  • levels of light photons into electrons, amplify those electrons, and then convert the electrons back into photons of light. Photons from a low-light...
    26 KB (3,779 words) - 15:25, 12 December 2023
  • Thumbnail for Redshift
    energy is known as a "redshifting", as photons in the visible spectrum would appear more red. Similarly, photons falling into a gravitational field become...
    86 KB (9,205 words) - 14:38, 29 July 2024
  • Thumbnail for Cosmic ray
    Cosmic ray (category CS1 German-language sources (de))
    further interaction. Others decay into photons, subsequently producing electromagnetic cascades. Hence, next to photons, electrons and positrons usually dominate...
    96 KB (10,538 words) - 10:08, 24 July 2024
  • here, as any observer observing the speed of photons in their region will find the speed of those photons to be c, while the speed at which we observe...
    17 KB (2,404 words) - 19:41, 18 June 2024
  • Thumbnail for Speed of light
    Speed of light (category CS1 German-language sources (de))
    fundamental excitations (or quanta) of the electromagnetic field, called photons. In QED, photons are massless particles and thus, according to special relativity...
    145 KB (15,359 words) - 18:03, 8 August 2024
  • Thumbnail for Observable universe
    reported that extragalactic background light (EBL) amounted to 4×1084 photons. As the universe's expansion is accelerating, all currently observable...
    65 KB (6,730 words) - 23:06, 8 August 2024