Difference between revisions of "Photochemistry" - New World Encyclopedia

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[[Image:Spectre.svg|thumb|350px|Illustration of the electromagnetic spectrum. Note the visible spectrum, as well as ultraviolet and infrared regions.]]'''Photochemistry''', a sub-discipline of [[chemistry]], is the study of the interactions between [[atoms]], small [[molecules]], and light (or [[electromagnetic radiation]]).<ref>{{GoldBookRef|title=photochemistry|file=P04588}}</ref>
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{{Claimed}}
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[[Image:Spectre.svg|thumb|350px|Significant regions of the electromagnetic spectrum, with their approximate wavelengths. The bottom part of the illustration shows an expanded version of the visible spectrum.]]
  
Like most scientific disciplines, photochemistry utilizes the SI or metric measurement system. Important units and constants that show up regularly include the [[metre]] (and variants such as centimetre, millimetre, micrometre, nanometre, etc.), seconds, hertz, joules, moles, the [[gas constant]] ''R'', and the [[Boltzmann constant]]. These units and constants are also integral to the field of [[physical chemistry]].
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'''Photochemistry''', a sub-discipline of [[chemistry]], is the study of the interactions between [[atom]]s, small [[molecules]], and light (or [[electromagnetic radiation]]).<ref>{{GoldBookRef|title=photochemistry|file=P04588}}</ref> The chemical reactions that take place through these interactions are known as '''photochemical reactions'''. The main pillars of photochemistry are photochemical reactions in organic chemistry, UV/VIS (ultraviolet/visible) spectroscopy, and [[photosynthesis]] in biochemistry.
  
The first law of photochemistry, known as the [[Grotthuss-Draper law]] (for chemists [[Theodor Grotthuss]] and [[John W. Draper]]), states that light must be absorbed by a chemical substance in order for a [[photochemical reaction]] to take place.
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== Reactions activated by light ==
  
The second law of photochemistry, the [[Stark-Einstein law]], states that for each photon of light absorbed by a chemical system, only one molecule is activated for a photochemical reaction. This is also known as the [[photoequivalence law]] and  was derived by [[Albert Einstein]] at the time when the [[quantum mechanics|quantum (photon) theory]] of light was being developed.
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A photochemical reaction may be thought of as a reaction that proceeds with the absorption of light.  Normally, a reaction (not just a photochemical reaction) occurs when the molecules involved gain the [[activation energy]] necessary to undergo change. For example, for the [[combustion]] of [[gasoline]] (a [[hydrocarbon]]) to produce carbon dioxide and water, activation energy is supplied in the form of heat or a spark. In the case of photochemical reactions, light provides the activation energy.
  
Photochemistry may also be introduced to laymen as a [[chemical reaction|reaction]] that proceeds with the absorption of light.  Normally a reaction (not just a photochemical reaction) occurs when a molecule gains the necessary [[activation energy]] to undergo change. A simple example can be the [[combustion]] of [[gasoline]] (a [[hydrocarbon]]) into carbon dioxide and water.  This is a chemical reaction where one or more molecules/[[chemical species]] are converted into others. For this reaction to take place [[activation energy]] should be supplied.  The [[activation energy]] is provided in the form of heat or a spark. In case of photochemical reactions light provides the [[activation energy]].
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The absorption of a photon of light by a reactant molecule may permit a reaction to occur not just by bringing the molecule to the necessary activation energy, but also by changing the symmetry of the molecule's electronic configuration, enabling an otherwise inaccessible reaction path.
  
The absorption of a photon of light by a reactant molecule may also permit a reaction to occur not just by bringing the molecule to the necessary activation energy, but also by changing the symmetry of the molecule's electronic configuration, enabling an otherwise inaccessible reaction path, as described by the [[Woodward-Hoffmann_rules | Woodward-Hoffmann selection rules]].  A 2+2 cycloaddition reaction is one example of a [[pericyclic reaction]] that can be analyzed using these rules or by the related frontier [[molecular orbital]] theory. 
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== Laws of photochemistry ==
  
==Main concepts==
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The first law of photochemistry, known as the [[Grotthuss-Draper law]] (for chemists [[Theodor Grotthuss]] and [[John W. Draper]]), states that light must be absorbed by a chemical substance in order for a [[photochemical reaction]] to take place.
The pillars of photochemistry are [[UV/VIS spectroscopy]], [[photochemical reaction]]s in organic chemistry and [[photosynthesis]] in biochemistry.
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The second law of photochemistry, the [[Stark-Einstein law]], states that for each photon of light absorbed by a chemical system, only one molecule is activated for a photochemical reaction. This is also known as the [[photoequivalence law]] and was derived by [[Albert Einstein]] at the time when the [[quantum mechanics|quantum (photon) theory]] of light was being developed.
  
 
==Regions of the electromagnetic spectrum==
 
==Regions of the electromagnetic spectrum==
The [[electromagnetic spectrum]] is broad, however, a photochemist will find themselves working with several key regions. Some of the most widely used sections of the electromagnetic spectrum include:
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* Visible Light: 400–700 nm wavelengths
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The [[electromagnetic spectrum]] is broad, but photochemists find themselves working with several key regions, noted here:
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* Visible Light: 400–700 nanometer (nm) wavelengths
 
* Ultraviolet: 100–400 nm wavelengths
 
* Ultraviolet: 100–400 nm wavelengths
 
* Near Infrared: 700–1000 nm wavelengths
 
* Near Infrared: 700–1000 nm wavelengths
 
* Far infrared: 15–1000 µm wavelengths
 
* Far infrared: 15–1000 µm wavelengths
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== Units and constants ==
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Like most scientific disciplines, photochemistry utilizes the SI or metric measurement system. Important units and constants that show up regularly include the [[meter]] (and variants such as centimeter, millimeter, micrometer, and nanometer), seconds, hertz, joules, moles, the [[gas constant]] ''R'', and the [[Boltzmann constant]]. These units and constants are also integral to the field of [[physical chemistry]].
  
 
==See also==
 
==See also==
*[[Photoelectrochemical cell]]
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*[[Photochemical and Photobiological Sciences]]
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* [[Chemical reaction]]
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* [[Electromagnetic spectrum]]
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* [[Light]]
  
 
==References ==
 
==References ==
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[[Category:Chemistry]]
 
[[Category:Chemistry]]
  
{{credit|146973909}}
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{{credits|Photochemistry|146973909}}

Revision as of 23:51, 20 August 2007

Significant regions of the electromagnetic spectrum, with their approximate wavelengths. The bottom part of the illustration shows an expanded version of the visible spectrum.

Photochemistry, a sub-discipline of chemistry, is the study of the interactions between atoms, small molecules, and light (or electromagnetic radiation).[1] The chemical reactions that take place through these interactions are known as photochemical reactions. The main pillars of photochemistry are photochemical reactions in organic chemistry, UV/VIS (ultraviolet/visible) spectroscopy, and photosynthesis in biochemistry.

Reactions activated by light

A photochemical reaction may be thought of as a reaction that proceeds with the absorption of light. Normally, a reaction (not just a photochemical reaction) occurs when the molecules involved gain the activation energy necessary to undergo change. For example, for the combustion of gasoline (a hydrocarbon) to produce carbon dioxide and water, activation energy is supplied in the form of heat or a spark. In the case of photochemical reactions, light provides the activation energy.

The absorption of a photon of light by a reactant molecule may permit a reaction to occur not just by bringing the molecule to the necessary activation energy, but also by changing the symmetry of the molecule's electronic configuration, enabling an otherwise inaccessible reaction path.

Laws of photochemistry

The first law of photochemistry, known as the Grotthuss-Draper law (for chemists Theodor Grotthuss and John W. Draper), states that light must be absorbed by a chemical substance in order for a photochemical reaction to take place.

The second law of photochemistry, the Stark-Einstein law, states that for each photon of light absorbed by a chemical system, only one molecule is activated for a photochemical reaction. This is also known as the photoequivalence law and was derived by Albert Einstein at the time when the quantum (photon) theory of light was being developed.

Regions of the electromagnetic spectrum

The electromagnetic spectrum is broad, but photochemists find themselves working with several key regions, noted here:

  • Visible Light: 400–700 nanometer (nm) wavelengths
  • Ultraviolet: 100–400 nm wavelengths
  • Near Infrared: 700–1000 nm wavelengths
  • Far infrared: 15–1000 µm wavelengths

Units and constants

Like most scientific disciplines, photochemistry utilizes the SI or metric measurement system. Important units and constants that show up regularly include the meter (and variants such as centimeter, millimeter, micrometer, and nanometer), seconds, hertz, joules, moles, the gas constant R, and the Boltzmann constant. These units and constants are also integral to the field of physical chemistry.

See also

References
ISBN links support NWE through referral fees

  1. International Union of Pure and Applied Chemistry. "photochemistry". Compendium of Chemical Terminology Internet edition.

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