The intrinsic properties of particles, such as charge , mass , and spin , are determined by this gauge symmetry. The photon concept has led to momentous advances in experimental and theoretical physics, including lasers , Bose—Einstein condensation , quantum field theory , and the probabilistic interpretation of quantum mechanics. It has been applied to photochemistry , high-resolution microscopy , and measurements of molecular distances. Recently, photons have been studied as elements of quantum computers , and for applications in optical imaging and optical communication such as quantum cryptography.
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The word quanta singular quantum, Latin for how much was used before to mean particles or amounts of different quantities , including electricity. In , the German physicist Max Planck was studying black-body radiation, and specifically the Ultraviolet Catastrophe : he suggested that the experimental observations would be explained if the energy carried by electromagnetic waves could only be released in "packets" of energy. In his article  in Annalen der Physik he called these packets "energy elements".
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In , Albert Einstein published a paper in which he proposed that many light-related phenomena—including black-body radiation and the photoelectric effect —would be better explained by modelling electromagnetic waves as consisting of spatially localized, discrete wave-packets. Arthur Compton used photon in , referring to Gilbert N. Lewis , who coined the term in a letter to Nature on December 18, Although Wolfers's and Lewis's theories were contradicted by many experiments and never accepted, the new name was adopted very soon by most physicists after Compton used it.
This symbol for the photon probably derives from gamma rays , which were discovered in by Paul Villard ,   named by Ernest Rutherford in , and shown to be a form of electromagnetic radiation in by Rutherford and Edward Andrade. A photon is massless , [c] has no electric charge ,   and is a stable particle. A photon has two possible polarization states. A photon's wave vector may not be zero and can be represented either as a spatial 3-vector or as a relativistic four-vector ; in the latter case it belongs to the light cone pictured.
Different signs of the four-vector denote different circular polarizations , but in the 3-vector representation one should account for the polarization state separately; it actually is a spin quantum number. In both cases the space of possible wave vectors is three-dimensional.
The photon is the gauge boson for electromagnetism ,  : 29—30 and therefore all other quantum numbers of the photon such as lepton number , baryon number , and flavour quantum numbers are zero. Photons are emitted in many natural processes.
For example, when a charge is accelerated it emits synchrotron radiation. During a molecular , atomic or nuclear transition to a lower energy level , photons of various energy will be emitted, ranging from radio waves to gamma rays. Photons can also be emitted when a particle and its corresponding antiparticle are annihilated for example, electron—positron annihilation. Since p points in the direction of the photon's propagation, the magnitude of the momentum is.
The photon also carries a quantity called spin angular momentum that does not depend on its frequency.
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These two possible helicities, called right-handed and left-handed, correspond to the two possible circular polarization states of the photon. To illustrate the significance of these formulae, the annihilation of a particle with its antiparticle in free space must result in the creation of at least two photons for the following reason.
In the center of momentum frame , the colliding antiparticles have no net momentum, whereas a single photon always has momentum since, as we have seen, it is determined by the photon's frequency or wavelength, which cannot be zero. Hence, conservation of momentum or equivalently, translational invariance requires that at least two photons are created, with zero net momentum.
However, it is possible if the system interacts with another particle or field for the annihilation to produce one photon, as when a positron annihilates with a bound atomic electron, it is possible for only one photon to be emitted, as the nuclear Coulomb field breaks translational symmetry. Seen another way, the photon can be considered as its own antiparticle thus an "antiphoton" is simply a normal photon.
The reverse process, pair production , is the dominant mechanism by which high-energy photons such as gamma rays lose energy while passing through matter. The classical formulae for the energy and momentum of electromagnetic radiation can be re-expressed in terms of photon events. For example, the pressure of electromagnetic radiation on an object derives from the transfer of photon momentum per unit time and unit area to that object, since pressure is force per unit area and force is the change in momentum per unit time.
Each photon carries two distinct and independent forms of angular momentum of light. The light orbital angular momentum of a particular photon can be any integer N , including zero. Current commonly accepted physical theories imply or assume the photon to be strictly massless. If the photon is not a strictly massless particle, it would not move at the exact speed of light, c , in vacuum. Its speed would be lower and depend on its frequency. Relativity would be unaffected by this; the so-called speed of light, c , would then not be the actual speed at which light moves, but a constant of nature which is the upper bound on speed that any object could theoretically attain in spacetime.
If a photon did have non-zero mass, there would be other effects as well. Coulomb's law would be modified and the electromagnetic field would have an extra physical degree of freedom. These effects yield more sensitive experimental probes of the photon mass than the frequency dependence of the speed of light. If Coulomb's law is not exactly valid, then that would allow the presence of an electric field to exist within a hollow conductor when it is subjected to an external electric field. This thus allows one to test Coulomb's law to very high precision. Sharper upper limits on the speed of light have been obtained in experiments designed to detect effects caused by the galactic vector potential.
Although the galactic vector potential is very large because the galactic magnetic field exists on very great length scales, only the magnetic field would be observable if the photon is massless.
Photon - Wikipedia
These sharp limits from the non-observation of the effects caused by the galactic vector potential have been shown to be model-dependent. Photons inside superconductors develop a nonzero effective rest mass ; as a result, electromagnetic forces become short-range inside superconductors. In most theories up to the eighteenth century, light was pictured as being made up of particles. The Maxwell wave theory , however, does not account for all properties of light.
The Maxwell theory predicts that the energy of a light wave depends only on its intensity , not on its frequency ; nevertheless, several independent types of experiments show that the energy imparted by light to atoms depends only on the light's frequency, not on its intensity. For example, some chemical reactions are provoked only by light of frequency higher than a certain threshold; light of frequency lower than the threshold, no matter how intense, does not initiate the reaction.
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Similarly, electrons can be ejected from a metal plate by shining light of sufficiently high frequency on it the photoelectric effect ; the energy of the ejected electron is related only to the light's frequency, not to its intensity. As shown by Albert Einstein ,   some form of energy quantization must be assumed to account for the thermal equilibrium observed between matter and electromagnetic radiation ; for this explanation of the photoelectric effect , Einstein received the Nobel Prize in physics.
Since the Maxwell theory of light allows for all possible energies of electromagnetic radiation, most physicists assumed initially that the energy quantization resulted from some unknown constraint on the matter that absorbs or emits the radiation. In , Einstein was the first to propose that energy quantization was a property of electromagnetic radiation itself. This photon momentum was observed experimentally  by Arthur Compton , for which he received the Nobel Prize in The pivotal question was then: how to unify Maxwell's wave theory of light with its experimentally observed particle nature?
Unlike Planck, Einstein entertained the possibility that there might be actual physical quanta of light—what we now call photons. He noticed that a light quantum with energy proportional to its frequency would explain a number of troubling puzzles and paradoxes, including an unpublished law by Stokes, the ultraviolet catastrophe , and the photoelectric effect.
Stokes's law said simply that the frequency of fluorescent light cannot be greater than the frequency of the light usually ultraviolet inducing it. Einstein eliminated the ultraviolet catastrophe by imagining a gas of photons behaving like a gas of electrons that he had previously considered. He was advised by a colleague to be careful how he wrote up this paper, in order to not challenge Planck, a powerful figure in physics, too directly, and indeed the warning was justified, as Planck never forgave him for writing it.
Einstein's predictions were verified experimentally in several ways in the first two decades of the 20th century, as recounted in Robert Millikan 's Nobel lecture. See, for example, the Nobel lectures of Wien ,  Planck  and Millikan. Attitudes changed over time.
In part, the change can be traced to experiments such as Compton scattering , where it was much more difficult not to ascribe quantization to light itself to explain the observed results. However, refined Compton experiments showed that energy—momentum is conserved extraordinarily well in elementary processes; and also that the jolting of the electron and the generation of a new photon in Compton scattering obey causality to within 10 ps.
Accordingly, Bohr and his co-workers gave their model "as honorable a funeral as possible". A few physicists persisted  in developing semiclassical models in which electromagnetic radiation is not quantized, but matter appears to obey the laws of quantum mechanics. Although the evidence from chemical and physical experiments for the existence of photons was overwhelming by the s, this evidence could not be considered as absolutely definitive; since it relied on the interaction of light with matter, and a sufficiently complete theory of matter could in principle account for the evidence.
Nevertheless, all semiclassical theories were refuted definitively in the s and s by photon-correlation experiments.
agendapop.cl/wp-content/business/jiraz-rastreador-de.php Photons, like all quantum objects, exhibit wave-like and particle-like properties. Their dual wave—particle nature can be difficult to visualize. The photon displays clearly wave-like phenomena such as diffraction and interference on the length scale of its wavelength.
For example, a single photon passing through a double-slit experiment exhibits interference phenomena but only if no measure was made at the slit.
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A single photon passing through a double-slit experiment lands on the screen with a probability distribution given by its interference pattern determined by Maxwell's equations.