Light 17939 225890741 2008-07-15T21:51:42Z Startstop123 6817648 Reverted edits by [[Special:Contributions/72.130.116.135|72.130.116.135]] ([[User talk:72.130.116.135|talk]]) to last version by Ijustam {{refimprove|date=May 2007}} {{other}} [[Image:PrismAndLight.jpg|thumb|300px|A beam of white light (entering upwards from the right) is dispersed into its constituent colors by its passage through a [[triangular prism (optics)|prism]]. The fainter beam of white light exiting to the upper right has been reflected (without dispersion) off the first surface of the prism.]] '''Light''', or '''visible light''', is [[electromagnetic radiation]] of a [[wavelength]] that is [[Visible spectrum|visible]] to the [[human eye]] (about 400–700 [[nanometre|nm]]). In a [[Science|scientific]] context, the word ''light'' is sometimes used to refer to the entire [[electromagnetic spectrum]]. Moreover, in [[optics]], the term "visible light" refers to electromagnetic radiation with wavelengths of ~300 nm ([[ultraviolet|near UV]]) through ~1400 nm ([[infrared|near infrared]]). <ref>{{cite web | url = http://www.lightsources.org/cms/?pid=1000166 | title = What Is a Light Source?}}</ref> Light is composed of [[elementary particles]] called [[photons]]. Three primary properties of light are: * [[Intensity (physics)|Intensity]]; * [[Frequency]] or [[wavelength]] and; * [[Polarization]]. Light can exhibit properties of both [[wave]]s and [[Particle physics|particles]]. This property is referred to as [[wave–particle duality]]. The study of light, known as [[optics]], is an important research area in modern [[physics]]. ==Speed of light== {{main|Speed of light}} The speed of light in a [[vacuum]] is exactly 299,792,458 [[Metre per second|m/s]] (about 186,282.397 miles per second). The speed of light depends upon the medium in which it is traveling, and the speed will be lower in a transparent medium. Although commonly called the "velocity of light", technically the word ''[[velocity]]'' is a [[vector (spatial)|vector]] quantity, having both magnitude and direction. ''Speed'' refers only to the magnitude of the velocity vector. This fixed definition of the speed of light is a result of the modern attempt, in physics, to define the [[metre|basic unit of length]] in terms of the speed of light, rather than defining the speed of light in terms of a length. Different physicists have attempted to measure the speed of light throughout history. [[Galileo Galilei|Galileo]] attempted to measure the speed of light in the seventeenth century. A good early experiment to measure the speed of light was conducted by [[Ole Rømer]], a Danish physicist, in 1676. Using a telescope, Ole observed the motions of [[Jupiter]] and one of its [[natural satellite|moon]]s, [[Io (moon)|Io]]. Noting discrepancies in the apparent period of Io's orbit, Rømer calculated that light takes about 18 minutes to traverse the diameter of Earth's orbit. Unfortunately, this was not a value that was known at that time. If Ole had known the diameter of the Earth's orbit, he would have calculated a speed of 227,000,000&nbsp;m/s. Another, more accurate, measurement of the speed of light was performed in Europe by [[Hippolyte Fizeau]] in 1849. Fizeau directed a beam of light at a mirror several kilometers away. A rotating cog wheel was placed in the path of the light beam as it traveled from the source, to the mirror and then returned to its origin. Fizeau found that at a certain rate of rotation, the beam would pass through one gap in the wheel on the way out and the next gap on the way back. Knowing the distance to the mirror, the number of teeth on the wheel, and the rate of rotation, Fizeau was able to calculate the speed of light as 313,000,000&nbsp;m/s. [[Léon Foucault]] used an experiment which used rotating mirrors to obtain a value of 298,000,000&nbsp;m/s in 1862. [[Albert Abraham Michelson|Albert A. Michelson]] conducted experiments on the speed of light from 1877 until his death in 1931. He refined Foucault's methods in 1926 using improved rotating [[mirror]]s to measure the [[time]] it took light to make a round trip from Mt. Wilson to Mt. San Antonio in [[California]]. The precise measurements yielded a speed of 299,796,000&nbsp;m/s. Some scientists were able to bring light to a complete standstill by passing it through a [[Bose-Einstein Condensate]] of the element rubidium. == Refraction == Note, ''n'' = 1 in a vacuum and ''n'' > 1 in a transparent medium, where n is the [[index of refraction]]. When a beam of light crosses the boundary between a vacuum and another medium, or between two different mediums, the wavelength of the light changes, but the frequency remains constant. If the beam of light is not [[orthogonality|orthogonal]] to the boundary, the change in wavelength results in a change in the direction of the beam. This change of direction is known as refraction. The refraction quality of [[lens (optics)|lens]]es is frequently used to manipulate light in order to change the apparent size of images. [[Magnifying glass]]es, [[Glasses|spectacles]], [[contact lens]]es, [[microscope]]s and [[refracting telescope]]s are all examples of this manipulation. ==Optics== {{main|Optics}} The study of light and the interaction of light and [[matter]] is termed [[optics]]. The observation and study of [[optical phenomenon|optical phenomena]] such as [[rainbow]]s and the [[Aurora (astronomy)|aurora borealis]] offer many clues as to the nature of light as well as much enjoyment. ==Light sources==<!-- This section is linked from [[Source]] --> {{seealso|List of light sources}} [[Image:Cloud in the sunlight.jpg|thumb|250px|A [[cloud]] illuminated by [[sunlight]]]] There are [[List of light sources|many sources of light]]. The most common light sources are thermal: a body at a given [[temperature]] emits a characteristic spectrum of [[black-body]] radiation. Examples include [[sunlight]] (the radiation emitted by the [[chromosphere]] of the [[Sun]] at around 6,000&nbsp;[[kelvin|K]] peaks in the visible region of the electromagnetic spectrum), [[incandescent light bulb]]s (which emit only around 10% of their energy as visible light and the remainder as infrared), and glowing solid particles in [[fire|flames]]. The peak of the blackbody spectrum is in the infrared for relatively cool objects like human beings. As the temperature increases, the peak shifts to shorter wavelengths, producing first a red glow, then a white one, and finally a blue color as the peak moves out of the visible part of the spectrum and into the ultraviolet. These colors can be seen when metal is [[heat]]ed to "red hot" or "white hot". The blue color is most commonly seen in a [[natural gas|gas]] flame or a [[weld]]er's torch. Atoms emit and absorb light at characteristic energies. This produces "[[emission line]]s" in the spectrum of each atom. [[Emission (electromagnetic radiation)|Emission]] can be [[spontaneous emission|spontaneous]], as in [[light-emitting diode]]s, [[gas discharge]] lamps (such as [[neon lamp]]s and [[neon sign]]s, [[mercury-vapor lamp]]s, etc.), and flames (light from the hot gas itself&mdash;so, for example, [[sodium]] in a gas flame emits characteristic yellow light). Emission can also be [[stimulated emission|stimulated]], as in a [[laser]] or a microwave [[maser]]. Acceleration of a free charged particle, such as an [[electron]], can produce visible radiation: [[cyclotron radiation]], [[synchrotron radiation]], and [[bremsstrahlung]] radiation are all examples of this. Particles moving through a medium faster than the speed of light in that medium can produce visible [[Cherenkov radiation]]. Certain chemicals produce visible radiation by [[chemoluminescence]]. In living things, this process is called [[bioluminescence]]. For example, [[firefly|fireflies]] produce light by this means, and boats moving through water can disturb plankton which produce a glowing wake. Certain substances produce light when they are illuminated by more energetic radiation, a process known as [[fluorescence]]. This is used in [[Fluorescent lamp|fluorescent light]]s. Some substances emit light slowly after excitation by more energetic radiation. This is known as [[phosphorescence]]. Phosphorescent materials can also be excited by bombarding them with subatomic particles. [[Cathodoluminescence]] is one example of this. This mechanism is used in [[cathode ray tube]] [[television]]s. Certain other mechanisms can produce light: *[[scintillation (physics)|scintillation]] *[[electroluminescence]] *[[sonoluminescence]] *[[triboluminescence]] *[[Cherenkov radiation]] When the concept of light is intended to include very-high-energy photons (gamma rays), additional generation mechanisms include: *[[radioactive decay]] *particle–[[antiparticle]] annihilation ==Theories about light== ===Indian theories=== In [[Science and technology in ancient India|ancient India]], the philosophical schools of [[Samkhya]] and [[Vaisheshika]], from around the [[6th century BC|6th]]&ndash;5th century BC, developed theories on light. According to the Samkhya school, light is one of the five fundamental "subtle" elements (''tanmatra'') out of which emerge the gross elements. The [[atomism|atomicity]] of these elements is not specifically mentioned and it appears that they were actually taken to be continuous. On the other hand, the Vaisheshika school gives an [[atomic theory]] of the physical world on the non-atomic ground of [[Aether (classical element)|ether]], space and time. (See ''[[Atomism#Indian atomism|Indian atomism]]''.) The basic [[atom]]s are those of earth (''prthivı''), water (''apas''), fire (''tejas''), and air (''vayu''), that should not be confused with the ordinary meaning of these terms. These atoms are taken to form binary molecules that combine further to form larger molecules. Motion is defined in terms of the movement of the physical atoms and it appears that it is taken to be non-instantaneous. Light rays are taken to be a stream of high velocity of ''tejas'' (fire) atoms. The particles of light can exhibit different characteristics depending on the speed and the arrangements of the ''tejas'' atoms. Around the first century BC, the ''[[Vishnu Purana]]'' correctly refers to [[sunlight]] as the "the seven rays of the sun". Later in 499, [[Aryabhata]], who proposed a [[heliocentrism|heliocentric]] [[solar system]] of [[gravitation]] in his ''[[Aryabhatiya]]'', wrote that the planets and the [[Moon]] do not have their own light but reflect the light of the [[Sun]]. The Indian [[Buddhist]]s, such as [[Dignāga]] in the 5th century and [[Dharmakirti]] in the 7th century, developed a type of [[atomism]] that is a philosophy about reality being composed of atomic entities that are momentary flashes of light or energy. They viewed light as being an atomic entity equivalent to energy, similar to the modern concept of [[photon]]s, though they also viewed all matter as being composed of these light/energy particles. ===Greek and Hellenistic theories=== {{main|Emission theory (vision)}} In the fifth century BC, [[Empedocles]] postulated that everything was composed of [[four elements]]; fire, air, earth and water. He believed that [[Aphrodite]] made the human eye out of the four elements and that she lit the fire in the eye which shone out from the eye making sight possible. If this were true, then one could see during the night just as well as during the day, so Empedocles postulated an interaction between rays from the eyes and rays from a source such as the sun. In about 300 BC, [[Euclid]] wrote ''Optica'', in which he studied the properties of light. Euclid postulated that light travelled in straight lines and he described the laws of reflection and studied them mathematically. He questioned that sight is the result of a beam from the eye, for he asks how one sees the stars immediately, if one closes one's eyes, then opens them at night. Of course if the beam from the eye travels infinitely fast this is not a problem. In 55 BC, [[Lucretius]], a Roman who carried on the ideas of earlier Greek [[atomism|atomists]], wrote: "''The light & heat of the sun; these are composed of minute atoms which, when they are shoved off, lose no time in shooting right across the interspace of air in the direction imparted by the shove.''" - ''On the nature of the Universe'' Despite being similar to later particle theories, Lucretius's views were not generally accepted and light was still theorized as emanating from the eye. [[Ptolemy]] (c. 2nd century) wrote about the [[refraction]] of light, and developed a theory of vision that objects are seen by rays of light emanating from the eyes. ===Optical theory=== {{main|Book of Optics|Islamic physics}} The [[Islamic science|Muslim scientist]], [[Ibn al-Haytham]] (965-1040), known as ''Alhacen'' or ''Alhazen'' in the West, in his ''[[Book of Optics]]'' (1021), developed a broad theory that explained [[Visual perception|vision]], using [[geometry]] and [[anatomy]], which stated that each point on an illuminated area or object radiates light rays in every direction, but that only one ray from each point, which strikes the eye perpendicularly, can be seen. The other rays strike at different angles and are not seen. He described the [[pinhole camera]] and invented the [[camera obscura]], which produces an inverted image, and used it as an example to support his argument.<ref>[http://inventors.about.com/library/inventors/blphotography.htm History of Photography and the Camera]</ref> This contradicted Ptolemy's theory of vision that objects are seen by rays of light emanating from the eyes. Alhacen held light rays to be streams of minute [[Photon|energy particles]]<ref name=Rashed>{{Citation |last=Rashed |first=Roshdi |year=2007 |title=The Celestial Kinematics of Ibn al-Haytham |journal=Arabic Sciences and Philosophy |volume=17 |pages=7–55 [19] |publisher=[[Cambridge University Press]] }}: {{quote|"In his optics ‘‘the smallest parts of light’’, as he calls them, retain only properties that can be treated by geometry and verified by experiment; they lack all sensible qualities except energy."}}</ref> that travelled at a [[Speed of light|finite speed]].<ref name=MacTutor>{{MacTutor|id=Al-Haytham|title=Abu Ali al-Hasan ibn al-Haytham}}</ref><ref name=MacKay>{{citation|title=Scientific Method, Statistical Method and the Speed of Light|first1=R. J.|last1=MacKay|first2=R. W.|last2=Oldford|journal=Statistical Science|volume=15|issue=3|date=August 2000|pages=254-78}}</ref><ref name=Hamarneh>Sami Hamarneh (March 1972). Review of Hakim Mohammed Said, ''Ibn al-Haitham'', ''[[Isis (journal)|Isis]]'' '''63''' (1), p. 119.</ref> He improved [[Ptolemy]]'s theory of the refraction of light, and went on to discover the laws of refraction. He also carried out the first experiments on the dispersion of light into its constituent colors. His major work ''Kitab al-Manazir'' (''Book of Optics'') was translated into [[Latin]] in the [[Middle Ages]], as well his book dealing with the colors of sunset. He dealt at length with the theory of various physical phenomena like shadows, eclipses, the rainbow. He also attempted to explain [[binocular vision]], and gave a correct explanation of the apparent increase in size of the sun and the moon when near the horizon, known as the [[moon illusion]]. Because of his extensive experimental research on optics, Ibn al-Haytham is considered the "father of modern [[optics]]".<ref>R. L. Verma (1969). ''Al-Hazen: father of modern optics''.</ref> Ibn al-Haytham also correctly argued that we see objects because the sun's rays of light, which he believed to be streams of tiny energy particles<ref name=Rashed/> travelling in straight lines, are reflected from objects into our eyes.<ref name=MacTutor/> He understood that light must travel at a large but finite velocity,<ref name=MacTutor/><ref name=MacKay/><ref name=Hamarneh/> and that refraction is caused by the velocity being different in different substances.<ref name=MacTutor/> He also studied spherical and parabolic mirrors, and understood how refraction by a lens will allow images to be focused and magnification to take place. He understood mathematically why a spherical mirror produces aberration. [[Avicenna]] (980-1037) agreed that the speed of light is finite, as he "observed that if the perception of light is due to the emission of some sort of particles by a luminous source, the speed of light must be finite."<ref>[[George Sarton]], ''Introduction to the History of Science'', Vol. 1, p. 710.</ref> [[Abū Rayhān al-Bīrūnī]] (973-1048) also agreed that light has a finite speed, and he was the first to discover that the speed of light is much faster than the [[speed of sound]].<ref name=Biruni>{{MacTutor|id=Al-Biruni|title=Al-Biruni}}</ref> In the late 13th and early 14th centuries, [[Qutb al-Din al-Shirazi]] (1236-1311) and his student [[Kamāl al-Dīn al-Fārisī]] (1260-1320) continued the work of Ibn al-Haytham, and they were the first to give the correct explanations for the [[rainbow]] phenomenon.<ref name=Biruni /> ===The 'plenum'=== [[René Descartes]] (1596-1650) held that light was a disturbance of the ''plenum'', the continuous substance of which the universe was composed. In 1637 he published a theory of the [[refraction]] of light that assumed, incorrectly, that light travelled faster in a denser medium than in a less dense medium. Descartes arrived at this conclusion by analogy with the behaviour of [[sound]] waves. Although Descartes was incorrect about the relative speeds, he was correct in assuming that light behaved like a wave and in concluding that refraction could be explained by the speed of light in different media. As a result, Descartes' theory is often regarded as the forerunner of the wave theory of light. ===Particle theory=== [[Ibn al-Haytham]] (Alhazen) (965-1040) proposed a particle theory of light in his ''[[Book of Optics]]'' (1021). He held light rays to be streams of minute [[Photon|energy particles]]<ref name=Rashed/> that travel in straight lines at a [[Speed of light|finite speed]].<ref name=MacTutor/><ref name=MacKay/><ref name=Hamarneh/> He states in his optics that "the smallest parts of light," as he calls them, "retain only properties that can be treated by geometry and verified by experiment; they lack all sensible qualities except energy."<ref name=Rashed/> [[Pierre Gassendi]] (1592-1655), an atomist, proposed a particle theory of light which was published posthumously in the 1660s. [[Isaac Newton]] studied Gassendi's work at an early age, and preferred his view to Descartes' theory of the ''plenum''. He stated in his ''Hypothesis of Light'' of 1675 that light was composed of corpuscles (particles of matter) which were emitted in all directions from a source. One of Newton's arguments against the wave nature of light was that waves were known to bend around obstacles, while light travelled only in straight lines. He did, however, explain the phenomenon of the [[diffraction]] of light (which had been observed by [[Francesco Grimaldi]]) by allowing that a light particle could create a localised wave in the [[Aether (classical element)|aether]]. Newton's theory could be used to predict the [[Reflection (physics)|reflection]] of light, but could only explain [[refraction]] by incorrectly assuming that light accelerated upon entering a denser [[Medium (optics)|medium]] because the [[gravity|gravitational]] pull was greater. Newton published the final version of his theory in his ''[[Opticks]]'' of 1704. His reputation helped the [[particle theory of light]] to hold sway during the 18th century. The particle theory of light led [[Laplace]] to argue that a body could be so massive that light could not escape from it. In other words it would become what is now called a black hole. Laplace withdrew his suggestion when the wave theory of light was firmly established. A translation of his essay appears in ''The large scale structure of space-time,'' by [[Stephen Hawking]] and [[George F. R. Ellis]]. ===Wave theory=== In the 1660s, [[Robert Hooke]] published a [[wave]] theory of light. [[Christiaan Huygens]] worked out his own wave theory of light in 1678, and published it in his ''Treatise on light'' in 1690. He proposed that light was emitted in all directions as a series of waves in a medium called the ''[[Luminiferous ether]]''. As waves are not affected by gravity, it was assumed that they slowed down upon entering a denser medium. [[Image:Young Diffraction.png|right|thumb|200px|Thomas Young's sketch of the two-slit experiment showing the [[diffraction]] of light. Young's experiments supported the theory that light consists of waves.]] The wave theory predicted that light waves could interfere with each other like [[sound]] waves (as noted around 1800 by [[Thomas Young (scientist)|Thomas Young]]), and that light could be [[polarization|polarized]]. Young showed by means of a [[double-slit experiment|diffraction experiment]] that light behaved as waves. He also proposed that different [[color]]s were caused by different [[wavelength]]s of light, and explained color vision in terms of three-colored receptors in the eye. Another supporter of the wave theory was [[Leonhard Euler]]. He argued in ''Nova theoria lucis et colorum'' (1746) that [[diffraction]] could more easily be explained by a wave theory. Later, [[Augustin-Jean Fresnel]] independently worked out his own wave theory of light, and presented it to the [[Académie des Sciences]] in 1817. [[Simeon Poisson|Simeon Denis Poisson]] added to Fresnel's mathematical work to produce a convincing argument in favour of the wave theory, helping to overturn Newton's corpuscular theory. The weakness of the wave theory was that light waves, like sound waves, would need a medium for transmission. A hypothetical substance called the [[luminiferous aether]] was proposed, but its existence was cast into strong doubt in the late nineteenth century by the [[Michelson-Morley experiment]]. Newton's corpuscular theory implied that light would travel faster in a denser medium, while the wave theory of Huygens and others implied the opposite. At that time, the [[speed of light]] could not be measured accurately enough to decide which theory was correct. The first to make a sufficiently accurate measurement was [[Léon Foucault]], in 1850. His result supported the wave theory, and the classical particle theory was finally abandoned. ===Electromagnetic theory=== [[Image:light-wave.svg|360px|thumb|A [[Polarization|linearly-polarized]] light wave frozen in time and showing the two oscillating components of light; an [[electric field]] and a [[magnetic field]] perpendicular to each other and to the direction of motion (a [[transverse wave]]).]] In 1845, [[Michael Faraday]] discovered that the angle of polarization of a beam of light as it passed through a polarizing material could be altered by a [[magnetic]] field, an effect now known as [[Faraday rotation]]. This was the first evidence that light was related to [[electromagnetism]]. Faraday proposed in 1847 that light was a high-frequency electromagnetic vibration, which could propagate even in the absence of a medium such as the ether. Faraday's work inspired [[James Clerk Maxwell]] to study electromagnetic radiation and light. Maxwell discovered that self-propagating electromagnetic waves would travel through space at a constant speed, which happened to be equal to the previously measured speed of light. From this, Maxwell concluded that light was a form of electromagnetic radiation: he first stated this result in 1862 in ''On Physical Lines of Force''. In 1873, he published ''[[A Treatise on Electricity and Magnetism]]'', which contained a full mathematical description of the behaviour of electric and magnetic fields, still known as [[Maxwell's equations]]. Soon after, [[Heinrich Hertz]] confirmed Maxwell's theory experimentally by generating and detecting [[radio]] waves in the laboratory, and demonstrating that these waves behaved exactly like visible light, exhibiting properties such as reflection, refraction, diffraction, and interference. Maxwell's theory and Hertz's experiments led directly to the development of modern radio, radar, television, electromagnetic imaging, and wireless communications. ===The special theory of relativity=== The wave theory was wildly successful in explaining nearly all optical and electromagnetic phenomena, and was a great triumph of nineteenth century physics. By the late nineteenth century, however, a handful of experimental anomalies remained that could not be explained by or were in direct conflict with the wave theory. One of these anomalies involved a controversy over the speed of light. The constant speed of light predicted by Maxwell's equations and confirmed by the Michelson-Morley experiment contradicted the mechanical laws of motion that had been unchallenged since the time of [[Galileo Galilei|Galileo]], which stated that all speeds were relative to the speed of the observer. In 1905, [[Albert Einstein]] resolved this paradox by revising the Galilean model of space and time <!-- [[Isaac Newton|Newton's]] [[Newton's laws of motion|laws of motion]] --> to account for the constancy of the speed of light. Einstein formulated his ideas in his [[special theory of relativity]], which radically altered humankind's understanding of [[Space#Physical spaces|space]] and [[time]]. Einstein also demonstrated a previously unknown fundamental [[mass-energy equivalence|equivalence]] between [[energy]] and [[mass]] with his famous equation :<math>E = mc^2 \, </math> where ''E'' is energy, ''m'' is rest mass, and ''c'' is the [[speed of light]]. ===Particle theory revisited=== Another experimental anomaly was the [[photoelectric effect]], by which light striking a metal surface ejected electrons from the surface, causing an [[electric current]] to flow across an applied [[voltage]]. Experimental measurements demonstrated that the energy of individual ejected electrons was proportional to the ''[[frequency]]'', rather than the ''[[intensity]]'', of the light. Furthermore, below a certain minimum frequency, which depended on the particular metal, no current would flow regardless of the intensity. These observations clearly contradicted the wave theory, and for years physicists tried in vain to find an explanation. In 1905, Einstein solved this puzzle as well, this time by resurrecting the particle theory of light to explain the observed effect. Because of the preponderance of evidence in favor of the wave theory, however, Einstein's ideas were met initially by great skepticism among established physicists. But eventually Einstein's explanation of the photoelectric effect would triumph, and it ultimately formed the basis for [[wave–particle duality]] and much of [[quantum mechanics]]. ===Quantum theory=== A third anomaly that arose in the late 19th century involved a contradiction between the wave theory of light and measurements of the electromagnetic spectrum emitted by thermal radiators, or so-called [[black body|black bodies]]. Physicists struggled with this problem, which later became known as the [[ultraviolet catastrophe]], unsuccessfully for many years. In 1900, [[Max Planck]] developed a new theory of [[Planck's law of black-body radiation|black-body radiation]] that explained the observed spectrum correctly. Planck's theory was based on the idea that black bodies emit light (and other electromagnetic radiation) only as discrete bundles or packets of [[energy]]. These packets were called [[quantum|quanta]], and the particle of light was given the name [[photon]], to correspond with other particles being described around this time, such as the [[electron]] and [[proton]]. A photon has an energy, ''E'', proportional to its frequency, ''f'', by :<math>E = hf = \frac{hc}{\lambda} \,\! </math> where ''h'' is [[Planck's constant]], <math>\lambda</math> is the wavelength and ''c'' is the [[speed of light]]. Likewise, the momentum ''p'' of a photon is also proportional to its frequency and inversely proportional to its wavelength: :<math>p = { E \over c } = { hf \over c } = { h \over \lambda }. </math> As it originally stood, this theory did not explain the simultaneous wave- and particle-like natures of light, though Planck would later work on theories that did. In 1918, Planck received the [[Nobel Prize in Physics]] for his part in the founding of quantum theory. ===Wave–particle duality=== The modern theory that explains the nature of light includes the notion of [[wave–particle duality]], described by [[Albert Einstein]] in the early 1900s, based on his study of the [[photoelectric effect]] and Planck's results. Einstein asserted that the energy of a photon is proportional to its [[frequency]]. More generally, the theory states that everything has both a particle nature and a wave nature, and various experiments can be done to bring out one or the other. The particle nature is more easily discerned if an object has a large mass, and it was not until a bold proposition by [[Louis de Broglie]] in 1924 that the scientific community realized that [[electrons]] also exhibited wave–particle duality. The wave nature of electrons was experimentally demonstrated by Davission and Germer in 1927. Einstein received the Nobel Prize in 1921 for his work with the wave–particle duality on photons (especially explaining the photoelectric effect thereby), and de Broglie followed in 1929 for his extension to other particles. ===Quantum electrodynamics=== The quantum mechanical theory of light and electromagnetic radiation continued to evolve through the 1920s and 1930's, and culminated with the development during the 1940s of the theory of [[quantum electrodynamics]], or QED. This so-called [[quantum field theory]] is among the most comprehensive and experimentally successful theories ever formulated to explain a set of natural phenomena. QED was developed primarily by physicists [[Richard Feynman]], [[Freeman Dyson]], [[Julian Schwinger]], and [[Shin-Ichiro Tomonaga]]. Feynman, Schwinger, and Tomonaga shared the 1965 Nobel Prize in Physics for their contributions. == Light pressure == {{main|Radiation pressure}} Light pushes on objects in its way, just as the wind would do. This pressure is most easily explainable in particle theory: photons hit and transfer their momentum. Light pressure can cause [[asteroid]]s to spin faster,<ref>{{cite web | url = http://discovermagazine.com/2004/feb/asteroids-get-spun-by-the-sun/ | title = Asteroids Get Spun By the Sun | author = Kathy A. | work = Discover Magazine | date = 02.05.2004}}</ref> acting on their irregular shapes as on the vanes of a [[windmill]]. The possibility to make [[solar sail]]s that would accelerate spaceships in space is also under investigation<ref>{{cite web | url = http://www.nasa.gov/vision/universe/roboticexplorers/solar_sails.html | title = Solar Sails Could Send Spacecraft 'Sailing' Through Space | work = NASA | date = 08.31.2004}}</ref><ref>{{cite web | url = http://www.nasa.gov/centers/marshall/news/news/releases/2004/04-208.html | title = NASA team successfully deploys two solar sail systems | work = NASA | date = 08.9.2004}}</ref>. Although the motion of the [[Crookes radiometer]] was originally attributed to light pressure, this interpretation is incorrect; the characteristic Crookes rotation is the result of a partial vacuum.<ref>P. Lebedev, Untersuchungen über die Druckkräfte des Lichtes, Ann. Phys. 6, 433 (1901).</ref> This should not be confused with the [[Nichols radiometer]], in which the motion ''is'' directly caused by light pressure.<ref>Nichols, E.F & Hull, G.F. (1903) [http://books.google.com/books?id=8n8OAAAAIAAJ&pg=RA5-PA327&dq=torsion+balance+radiation The Pressure due to Radiation], ''The Astrophysical Journal'',Vol.17 No.5, p.315-351</ref> ==Spirituality== [[Image:Kallara Pazhyapalli Light.JPG|thumb|right|300px|Light Decoration for the feast of St.Thomas at Kallara Pazhayapalli in Kottayam, Kerala-Importance of light in religion]] The sensory perception of light plays a central role in spirituality ([[Vision (religion)|vision]], [[enlightenment]], [[darshan]], [[Tabor Light]]), and the presence of light as opposed to its absence ([[darkness]]) is a common Western metaphor of [[good and evil]], [[knowledge]] and [[ignorance]], and similar concepts. ==References== {{reflist}} ==See also== {{commons|Light}}{{wiktionary}}{{wikiquote}} <div class="references-small" style="-moz-column-count:2; column-count:2;"> *[[Automotive lighting]] *[[Ballistic photon]] *[[Color temperature]] *[[Corpuscular theory of light]] *[[Electromagnetic spectrum]] *[[Huygens' principle]] *[[Fermat's principle]] *[[International Commission on Illumination]] *[[Light beam]] - in particular about light beams visible from the side *[[Light pollution]] *[[Lighting]] *[[Photic sneeze reflex]] *[[Photometry (optics)|Photometry]] *[[Rights of Light]] *[[Spectrometry]] </div> ==External links== <!-- Please do not add links here before ensuring that they do not violate [[WP:LINKS]], [[WP:COI]] and [[WP:SPAM]] --> ''' [[Category:Light| ]] [[ar:ضوء]] [[ast:Lluz]] [[gn:Mba'erendy]] [[az:İşıq]] [[bn:আলো]] [[zh-min-nan:Kng]] [[be-x-old:Сьвятло]] [[bar:Liacht]] [[bs:Svjetlost]] [[bg:Светлина]] [[ca:Llum]] [[cs:Světlo]] [[cy:Goleuni]] [[da:Lys]] [[pdc:Licht]] [[de:Licht]] [[et:Valgus]] [[el:Φως]] [[es:Luz]] [[eo:Lumo]] [[eu:Argi]] [[fa:نور]] [[fr:Lumière]] [[ga:Solas]] [[gl:Luz]] [[gan:光]] [[ko:빛]] [[hr:Svjetlost]] [[io:Lumo]] [[bpy:লুজ]] [[id:Cahaya]] [[is:Ljós]] [[it:Luce]] [[he:אור]] [[jv:Cahya]] [[kn:ಬೆಳಕು]] [[ka:სინათლე]] [[ku:Ruhnahî (fîzîk)]] [[la:Lux]] [[lv:Gaisma]] [[lt:Šviesa]] [[li:Lèch]] [[jbo:gusni]] [[lmo:Lüs]] [[hu:Fény]] [[mk:Светлина]] [[mg:Fahazavana]] [[ml:പ്രകാശം]] [[mr:प्रकाश]] [[ms:Cahaya]] [[mn:Гэрэл]] [[nah:Tlāhuīlli]] [[nl:Licht]] [[nds-nl:Locht (straoling)]] [[new:जः]] [[ja:光]] [[nap:Luce]] [[no:Lys]] [[nn:Lys]] [[nrm:Lumyire]] [[nov:Lume]] [[oc:Lutz]] [[uz:Yorugʻlik]] [[pl:Światło]] [[pt:Luz]] [[ro:Lumină]] [[qu:Achkiy]] [[ru:Свет]] [[sq:Drita]] [[scn:Luci]] [[simple:Light]] [[sk:Svetlo]] [[sl:Svetloba]] [[sr:Светлост]] [[fi:Valo]] [[sv:Ljus]] [[ta:ஒளி]] [[te:కాంతి]] [[th:แสง]] [[vi:Ánh sáng]] [[tg:Нӯр]] [[tr:Işık]] [[uk:Світло (фізика)]] [[ur:روشنی]] [[wa:Loumire]] [[yi:ליכטיגקייט]] [[yo:Imole]] [[zh-yue:光]] [[zh:光]]