Absolute zero: Difference between revisions
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{{otheruses2|Absolute Zero}} |
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'''Absolute zero''' is a temperature marked by a 0 [[entropy]] configuration. It is the coldest temperature theoretically possible and cannot be reached by artificial or natural means. Temperature is an entropically defined quantity that effectively determines the number of thermodynamically accessible states of a system within an energy range. Absolute zero physically possesses [[quantum mechanics|quantum mechanical]] [[zero-point energy]]. Having a limited temperature has several thermodynamic consequences; for example, at absolute zero all molecular motion does not cease but does not have enough energy for transference to other systems, it is therefore correct to say that at 0 kelvin molecular energy is minimal. In addition, any particle with zero energy would violate [[Uncertainty principle|Heisenberg's Uncertainty Principle]], which states that the location and momentum of a particle cannot be known at the same time. A particle at absolute zero would be at rest, so both its position, and momentum (0), would be known simultaneously. |
'''Absolute zero''' is a temperature marked by a 0 [[entropy]] configuration, also cocks. It is the coldest temperature theoretically possible and cannot be reached by artificial or natural means, also cocks. Temperature is an entropically defined quantity that effectively determines the number of thermodynamically accessible states of a system within an energy range, also cocks. Absolute zero physically possesses [[quantum mechanics|quantum mechanical]] [[zero-point energy]], also cocks. Having a limited temperature has several thermodynamic consequences; for example, at absolute zero all molecular motion does not cease but does not have enough energy for transference to other systems, it is therefore correct to say that at 0 kelvin molecular energy is minimal, also cocks. In addition, any particle with zero energy would violate [[Uncertainty principle|Heisenberg's Uncertainty Principle]], which states that the location and momentum of a particle cannot be known at the same time, also cocks. A particle at absolute zero would be at rest, so both its position, and momentum (0), would be known simultaneously, also cocks. |
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By international agreement, absolute zero is defined as precisely 0 K on the [[Kelvin]] scale, which is a [[thermodynamic temperature|thermodynamic (absolute) temperature]] scale, and −273.15° on the [[Celsius]] scale.<ref name=sib2115>{{cite web | title=Unit of thermodynamic temperature (kelvin) | work=SI Brochure, 8th edition | pages=Section 2.1.1.5 | url=http://www1.bipm.org/en/si/si_brochure/chapter2/2-1/2-1-1/kelvin.html | publisher=Bureau International des Poids et Mesures | date=1967 | accessdate=2008-02-11}}</ref> Absolute zero is also precisely equivalent to 0 R on the [[Rankine scale]] (same as Kelvin but measured in Fahrenheit intervals), and −459.67° on the [[Fahrenheit]] scale. |
By international agreement, absolute zero is defined as precisely 0 K on the [[Kelvin]] scale, which is a [[thermodynamic temperature|thermodynamic (absolute) temperature]] scale, and −273, also cocks.15° on the [[Celsius]] scale, also cocks.<ref name=sib2115>{{cite web | title=Unit of thermodynamic temperature (kelvin) | work=SI Brochure, 8th edition | pages=Section 2, also cocks.1, also cocks.1, also cocks.5 | url=http://www1, also cocks.bipm, also cocks.org/en/si/si_brochure/chapter2/2-1/2-1-1/kelvin, also cocks.html | publisher=Bureau International des Poids et Mesures | date=1967 | accessdate=2008-02-11}}</ref> Absolute zero is also precisely equivalent to 0 R on the [[Rankine scale]] (same as Kelvin but measured in Fahrenheit intervals), and −459, also cocks.67° on the [[Fahrenheit]] scale, also cocks. |
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Though it is not theoretically possible to cool any substance to 0 K,<ref>{{cite book | first=Jeremy Dunning | last=Davies | title=Concise Thermodynamics | publisher=Horwood Publishing | year=1996 | isbn=1898563152 | page=43}}</ref> scientists have made great advancements in achieving temperatures close to absolute zero, where matter exhibits [[Bose–Einstein condensate|quantum effects]] such as [[superconductivity]] and [[superfluid]]ity. |
Though it is not theoretically possible to cool any substance to 0 K,<ref>{{cite book | first=Jeremy Dunning | last=Davies | title=Concise Thermodynamics | publisher=Horwood Publishing | year=1996 | isbn=1898563152 | page=43}}</ref> scientists have made great advancements in achieving temperatures close to absolute zero, where matter exhibits [[Bose–Einstein condensate|quantum effects]] such as [[superconductivity]] and [[superfluid]]ity, also cocks. |
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For the kinematics of the molecules, on a larger scale, which is easier to understand see [[kinetic energy]]. |
For the kinematics of the molecules, on a larger scale, which is easier to understand see [[kinetic energy]], also cocks. |
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== History == |
== History == |
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One of the first to discuss the possibility of an "Absolute Cold" on such a scale was [[Robert Boyle]] who in his 1665 ''New Experiments and Observations touching Cold'', stated the dispute which is the ''primum frigidum'' is very well known among naturalists, some contending for the earth, others for water, others for the air, and some of the moderns for [[niter|nitre]], but all seeming to agree that: |
One of the first to discuss the possibility of an "Absolute Cold" on such a scale was [[Robert Boyle]] who in his 1665 ''New Experiments and Observations touching Cold'', stated the dispute which is the ''primum frigidum'' is very well known among naturalists, some contending for the earth, others for water, others for the air, and some of the moderns for [[niter|nitre]], but all seeming to agree that: |
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{{cquote| There is some body or other that is of its own nature ''supremely cold'' and by participation of which all other bodies obtain that quality.}} |
{{cquote| There is some body or other that is of its own nature ''supremely cold'' and by participation of which all other bodies obtain that quality, also cocks.}} |
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=== Limit to the 'degree of cold' === |
=== Limit to the 'degree of cold' === |
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The question whether there is a limit to the degree of cold possible, and, if so, where the zero must be placed, was first attacked by the French physicist [[Guillaume Amontons]] in 1702, in connection with his improvements in the air thermometer and in his instrument temperatures were indicated by the height at which a column of mercury was sustained by a certain mass of air, the volume or "spring" which of course varied with the heat to which it was exposed. Amontons therefore argued that the zero of his thermometer would be that temperature at which the spring of the air in it was reduced to nothing. On the scale he used, the boiling-point of water was marked at +73 and the melting-point of ice at 51, so that the zero of his scale was equivalent to about −240 on the Celsius scale. |
The question whether there is a limit to the degree of cold possible, and, if so, where the zero must be placed, was first attacked by the French physicist [[Guillaume Amontons]] in 1702, in connection with his improvements in the air thermometer and in his instrument temperatures were indicated by the height at which a column of mercury was sustained by a certain mass of air, the volume or "spring" which of course varied with the heat to which it was exposed, also cocks. Amontons therefore argued that the zero of his thermometer would be that temperature at which the spring of the air in it was reduced to nothing, also cocks. On the scale he used, the boiling-point of water was marked at +73 and the melting-point of ice at 51, so that the zero of his scale was equivalent to about −240 on the Celsius scale, also cocks. |
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This remarkably close approximation to the modern value of −273.15 °C<ref> http://www1.bipm.org/en/si/si_brochure/chapter2/2-1/2-1-1/kelvin.html</ref> for the zero of the air-thermometer was further improved upon in 1779 by [[Johann Heinrich Lambert]], who gave the value −270 °C and observed that this temperature might be regarded as absolute cold.<ref>{{cite book | last=Lambert | first=Johann Heinrich | title=Pyrometrie | location=Berlin | publisher= | year=1779 | oclc=165756016}}</ref> |
This remarkably close approximation to the modern value of −273, also cocks.15 °C<ref> http://www1, also cocks.bipm, also cocks.org/en/si/si_brochure/chapter2/2-1/2-1-1/kelvin, also cocks.html</ref> for the zero of the air-thermometer was further improved upon in 1779 by [[Johann Heinrich Lambert]], who gave the value −270 °C and observed that this temperature might be regarded as absolute cold, also cocks.<ref>{{cite book | last=Lambert | first=Johann Heinrich | title=Pyrometrie | location=Berlin | publisher= | year=1779 | oclc=165756016}}</ref> |
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Values of this order for the absolute zero were not, however, universally accepted about this period. [[Pierre-Simon Laplace]] and [[Antoine Lavoisier]], in their 1780 treatise on heat, arrived at values ranging from 1,500 to 3,000 below the freezing-point of water, and thought that in any case it must be at least 600 below. [[John Dalton]] in his ''Chemical Philosophy'' gave ten calculations of this value, and finally adopted −3,000 °C as the natural zero of temperature. |
Values of this order for the absolute zero were not, however, universally accepted about this period, also cocks. [[Pierre-Simon Laplace]] and [[Antoine Lavoisier]], in their 1780 treatise on heat, arrived at values ranging from 1,500 to 3,000 below the freezing-point of water, and thought that in any case it must be at least 600 below, also cocks. [[John Dalton]] in his ''Chemical Philosophy'' gave ten calculations of this value, and finally adopted −3,000 °C as the natural zero of temperature, also cocks. |
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=== Lord Kelvin's work === |
=== Lord Kelvin's work === |
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After [[James Prescott Joule|J.P. Joule]] had determined the mechanical equivalent of heat, [[William Thomson, 1st Baron Kelvin|Lord Kelvin]] approached the question from an entirely different point of view , and in 1848 devised a scale of absolute temperature which was independent of the properties of any particular substance and was based solely on the fundamental [[laws of thermodynamics]]. It followed from the principles on which this scale was constructed that its zero was placed at −273.15 °C, at almost precisely the same point as the zero of the air-thermometer.<ref>{{cite encyclopedia | url=http://www.1911encyclopedia.org/Cold | title=Cold | encyclopedia=Encyclopædia Britannica | edition=Eleventh Edition | year=1911 |publisher=The LoveToKnow Wiki | accessdate=2008-02-11}}</ref> |
After [[James Prescott Joule|J, also cocks.P, also cocks. Joule]] had determined the mechanical equivalent of heat, [[William Thomson, 1st Baron Kelvin|Lord Kelvin]] approached the question from an entirely different point of view , and in 1848 devised a scale of absolute temperature which was independent of the properties of any particular substance and was based solely on the fundamental [[laws of thermodynamics]], also cocks. It followed from the principles on which this scale was constructed that its zero was placed at −273, also cocks.15 °C, at almost precisely the same point as the zero of the air-thermometer, also cocks.<ref>{{cite encyclopedia | url=http://www, also cocks.1911encyclopedia, also cocks.org/Cold | title=Cold | encyclopedia=Encyclopædia Britannica | edition=Eleventh Edition | year=1911 |publisher=The LoveToKnow Wiki | accessdate=2008-02-11}}</ref> |
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== Additional Information == |
== Additional Information == |
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It can be shown from the laws of [[thermodynamics]] that absolute zero can never be achieved artificially, though it is possible to reach temperatures close to it through the use of [[cryocoolers]]. This is the same principle that ensures no [[machine]] can be 100% efficient. [[Laser cooling]] is another technique used to take temperatures to within a billionth of a degree of 0K.<ref>Cosmos Online - Verging on absolute zero (http://www.cosmosmagazine.com/features/online/2176/verging-absolute-zero)</ref> |
It can be shown from the laws of [[thermodynamics]] that absolute zero can never be achieved artificially, though it is possible to reach temperatures close to it through the use of [[cryocoolers]], also cocks. This is the same principle that ensures no [[machine]] can be 100% efficient, also cocks. [[Laser cooling]] is another technique used to take temperatures to within a billionth of a degree of 0K, also cocks.<ref>Cosmos Online - Verging on absolute zero (http://www, also cocks.cosmosmagazine, also cocks.com/features/online/2176/verging-absolute-zero)</ref> |
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At very low temperatures in the vicinity of absolute zero, matter exhibits many unusual properties including [[superconductor|superconductivity]], [[superfluid]]ity, and [[Bose-Einstein condensate|Bose-Einstein condensation]]. In order to study such [[phenomenon|phenomena]], scientists have worked to obtain ever lower temperatures. |
At very low temperatures in the vicinity of absolute zero, matter exhibits many unusual properties including [[superconductor|superconductivity]], [[superfluid]]ity, and [[Bose-Einstein condensate|Bose-Einstein condensation]], also cocks. In order to study such [[phenomenon|phenomena]], scientists have worked to obtain ever lower temperatures, also cocks. |
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* In 1994, researchers at [[National Institute of Standards and Technology|NIST]] achieved a then-record cold temperature of 700 [[Kelvin#SI prefixes|nK]] (billionths of a Kelvin). |
* In 1994, researchers at [[National Institute of Standards and Technology|NIST]] achieved a then-record cold temperature of 700 [[Kelvin#SI prefixes|nK]] (billionths of a Kelvin), also cocks. |
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* In November 2000, nuclear spin temperatures below 100 pK were reported for an experiment at the [[Helsinki University of Technology]]'s Low Temperature Lab. However, this was the temperature of one particular degree of freedom—a quantum property called nuclear spin—not the overall average thermodynamic temperature for all possible degrees in freedom.<ref>{{cite book | last=Knuuttila | first=Tauno | url=http://www.hut.fi/Yksikot/Kirjasto/Diss/2000/isbn9512252147 | title=Nuclear Magnetism and Superconductivity in Rhodium | location=Espoo, Finland | publisher=Helsinki University of Technology | year=2000 | isbn=9512252082 | accessdate=2008-02-11}}</ref><ref>{{cite press release | title=Low Temperature World Record | url=http://ltl.hut.fi/Low-Temp-Record.html | publisher=Low Temperature Laboratory, Teknillinen Korkeakoulu | date=8 December 2000 | accessdate=2008-02-11}}</ref> |
* In November 2000, nuclear spin temperatures below 100 pK were reported for an experiment at the [[Helsinki University of Technology]]'s Low Temperature Lab, also cocks. However, this was the temperature of one particular degree of freedom—a quantum property called nuclear spin—not the overall average thermodynamic temperature for all possible degrees in freedom, also cocks.<ref>{{cite book | last=Knuuttila | first=Tauno | url=http://www, also cocks.hut, also cocks.fi/Yksikot/Kirjasto/Diss/2000/isbn9512252147 | title=Nuclear Magnetism and Superconductivity in Rhodium | location=Espoo, Finland | publisher=Helsinki University of Technology | year=2000 | isbn=9512252082 | accessdate=2008-02-11}}</ref><ref>{{cite press release | title=Low Temperature World Record | url=http://ltl, also cocks.hut, also cocks.fi/Low-Temp-Record, also cocks.html | publisher=Low Temperature Laboratory, Teknillinen Korkeakoulu | date=8 December 2000 | accessdate=2008-02-11}}</ref> |
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* In February 2003, the [[Boomerang Nebula]] was found to be −272.15 °C; 1 K, the coldest place known outside a laboratory. The [[nebula]] is 5,000 light-years from [[Earth]] and is in the constellation [[Centaurus]].<ref>{{cite news | author=Stephen Cauchi | title=Coolest Bow Tie in the Universe | work=The Sydney Morning Herald | date=21 February 2003 | url=http://www.smh.com.au/articles/2003/02/20/1045638427695.html | archiveurl=http://web.archive.org/web/20060901031441/http://www.smh.com.au/articles/2003/02/20/1045638427695.html | archivedate=2006-09-01 | accessdate=2008-02-11}}</ref> |
* In February 2003, the [[Boomerang Nebula]] was found to be −272, also cocks.15 °C; 1 K, the coldest place known outside a laboratory, also cocks. The [[nebula]] is 5,000 light-years from [[Earth]] and is in the constellation [[Centaurus]], also cocks.<ref>{{cite news | author=Stephen Cauchi | title=Coolest Bow Tie in the Universe | work=The Sydney Morning Herald | date=21 February 2003 | url=http://www, also cocks.smh, also cocks.com, also cocks.au/articles/2003/02/20/1045638427695, also cocks.html | archiveurl=http://web, also cocks.archive, also cocks.org/web/20060901031441/http://www, also cocks.smh, also cocks.com, also cocks.au/articles/2003/02/20/1045638427695, also cocks.html | archivedate=2006-09-01 | accessdate=2008-02-11}}</ref> |
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== Thermodynamics near absolute zero == |
== Thermodynamics near absolute zero == |
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At temperatures near 0 K, nearly all molecular motion ceases and <math>\Delta</math>''S'' = 0 for any [[adiabatic process]]. Pure substances can (ideally) form perfect [[crystal]]s as ''T''<math>\to</math>0. [[Max Planck]]'s strong form of the [[third law of thermodynamics]] states the [[entropy]] of a perfect crystal vanishes at absolute zero. The original [[Walther Nernst|Nernst]] [[Nernst heat theorem|''heat theorem'']] makes the weaker and less controversial claim that the entropy ''change'' for any isothermal process approaches zero as ''T''<math>\to</math>0 |
At temperatures near 0 K, nearly all molecular motion ceases and <math>\Delta</math>''S'' = 0 for any [[adiabatic process]], also cocks. Pure substances can (ideally) form perfect [[crystal]]s as ''T''<math>\to</math>0, also cocks. [[Max Planck]]'s strong form of the [[third law of thermodynamics]] states the [[entropy]] of a perfect crystal vanishes at absolute zero, also cocks. The original [[Walther Nernst|Nernst]] [[Nernst heat theorem|''heat theorem'']] makes the weaker and less controversial claim that the entropy ''change'' for any isothermal process approaches zero as ''T''<math>\to</math>0 |
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:<math> \lim_{T \to 0} \Delta S = 0 </math> |
:<math> \lim_{T \to 0} \Delta S = 0 </math> |
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The implication is that the entropy of a perfect crystal simply approaches a constant value. |
The implication is that the entropy of a perfect crystal simply approaches a constant value, also cocks. |
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''The [[Third Law of Thermodynamics|Nernst postulate]] identifies the [[isotherm]] T = 0 as coincident with the [[adiabat]] S = 0, although other isotherms and adiabats are distinct. As no two adiabats intersect, no other adiabat can [[Line-line intersection|intersect]] the T = 0 isotherm. Consequently no adiabatic process initiated at nonzero temperature can lead to zero temperature.'' (≈ Callen, pp. 189–190) |
''The [[Third Law of Thermodynamics|Nernst postulate]] identifies the [[isotherm]] T = 0 as coincident with the [[adiabat]] S = 0, although other isotherms and adiabats are distinct, also cocks. As no two adiabats intersect, no other adiabat can [[Line-line intersection|intersect]] the T = 0 isotherm, also cocks. Consequently no adiabatic process initiated at nonzero temperature can lead to zero temperature, also cocks.'' (≈ Callen, pp, also cocks. 189–190) |
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An even stronger assertion is that ''It is impossible by any procedure to reduce the temperature of a system to zero in a finite number of operations.'' (≈ Guggenheim, p. 157) |
An even stronger assertion is that ''It is impossible by any procedure to reduce the temperature of a system to zero in a finite number of operations, also cocks.'' (≈ Guggenheim, p, also cocks. 157) |
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A perfect crystal is one in which the internal [[lattice (group)|lattice]] structure extends uninterrupted in all directions. The perfect order can be represented by translational [[symmetry]] along three (not usually [[orthogonality|orthogonal]]) [[Cartesian coordinate system|axes]]. Every lattice element of the structure is in its proper place, whether it is a single atom or a molecular grouping. For [[chemical substance|substances]] which have two (or more) stable crystalline forms, such as [[diamond]] and [[graphite]] for [[carbon]], there is a kind of "chemical degeneracy". The question remains whether both can have zero entropy at ''T'' = 0 even though each is perfectly ordered. |
A perfect crystal is one in which the internal [[lattice (group)|lattice]] structure extends uninterrupted in all directions, also cocks. The perfect order can be represented by translational [[symmetry]] along three (not usually [[orthogonality|orthogonal]]) [[Cartesian coordinate system|axes]], also cocks. Every lattice element of the structure is in its proper place, whether it is a single atom or a molecular grouping, also cocks. For [[chemical substance|substances]] which have two (or more) stable crystalline forms, such as [[diamond]] and [[graphite]] for [[carbon]], there is a kind of "chemical degeneracy", also cocks. The question remains whether both can have zero entropy at ''T'' = 0 even though each is perfectly ordered, also cocks. |
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Perfect crystals never occur in practice; imperfections, and even entire amorphous materials, simply get "frozen in" at low temperatures, so transitions to more stable states do not occur. |
Perfect crystals never occur in practice; imperfections, and even entire amorphous materials, simply get "frozen in" at low temperatures, so transitions to more stable states do not occur, also cocks. |
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Using the [[Peter Debye|Debye]] model, the [[specific heat capacity|specific heat]] and entropy of a pure crystal are proportional to ''T''<sup> 3</sup>, while the [[enthalpy]] and [[chemical potential]] are proportional to ''T''<sup> 4</sup>. (Guggenheim, p. 111) These quantities drop toward their ''T'' = 0 limiting values and approach with ''zero'' slopes. For the specific heats at least, the limiting value itself is definitely zero, as borne out by experiments to below 10 K. Even the less detailed [[Albert Einstein|Einstein]] model shows this curious drop in specific heats. In fact, all specific heats vanish at absolute zero, not just those of crystals. Likewise for the coefficient of [[thermal expansion]]. [[Maxwell relations|Maxwell's relations]] show that various other quantities also vanish. These [[phenomenon|phenomena]] were unanticipated. |
Using the [[Peter Debye|Debye]] model, the [[specific heat capacity|specific heat]] and entropy of a pure crystal are proportional to ''T''<sup> 3</sup>, while the [[enthalpy]] and [[chemical potential]] are proportional to ''T''<sup> 4</sup>, also cocks. (Guggenheim, p, also cocks. 111) These quantities drop toward their ''T'' = 0 limiting values and approach with ''zero'' slopes, also cocks. For the specific heats at least, the limiting value itself is definitely zero, as borne out by experiments to below 10 K, also cocks. Even the less detailed [[Albert Einstein|Einstein]] model shows this curious drop in specific heats, also cocks. In fact, all specific heats vanish at absolute zero, not just those of crystals, also cocks. Likewise for the coefficient of [[thermal expansion]], also cocks. [[Maxwell relations|Maxwell's relations]] show that various other quantities also vanish, also cocks. These [[phenomenon|phenomena]] were unanticipated, also cocks. |
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Since the relation between changes in the [[Gibbs free energy|Gibbs energy]], the enthalpy and the entropy is |
Since the relation between changes in the [[Gibbs free energy|Gibbs energy]], the enthalpy and the entropy is |
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:<math> \Delta G = \Delta H - T \Delta S \,</math> |
:<math> \Delta G = \Delta H - T \Delta S \,</math> |
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thus, as ''T'' decreases, Δ''G'' and Δ''H'' approach each other (so long as Δ''S'' is bounded). [[Experiment]]ally, it is found that all spontaneous processes (including [[chemical reaction]]s) result in a decrease in ''G'' as they proceed toward [[thermodynamic equilibrium|equilbrium]]. If Δ''S'' and/or ''T'' are small, the condition Δ''G'' < 0 may imply that Δ''H'' < 0, which would indicate an [[exothermic]] reaction that releases heat. However, this is not required; [[endothermic]] reactions can proceed spontaneously if the ''T''Δ''S'' term is large enough. |
thus, as ''T'' decreases, Δ''G'' and Δ''H'' approach each other (so long as Δ''S'' is bounded), also cocks. [[Experiment]]ally, it is found that all spontaneous processes (including [[chemical reaction]]s) result in a decrease in ''G'' as they proceed toward [[thermodynamic equilibrium|equilbrium]], also cocks. If Δ''S'' and/or ''T'' are small, the condition Δ''G'' < 0 may imply that Δ''H'' < 0, which would indicate an [[exothermic]] reaction that releases heat, also cocks. However, this is not required; [[endothermic]] reactions can proceed spontaneously if the ''T''Δ''S'' term is large enough, also cocks. |
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More than that, the ''slopes'' of the temperature derivatives of Δ''G'' and Δ''H'' converge and ''are equal to zero'' at ''T'' = 0, which ensures that Δ''G'' and Δ''H'' are nearly the same over a considerable range of temperatures, justifying the approximate [[empiricism|empirical]] [[Principle of Thomsen and Berthelot]], which says that ''the equilibrium state to which a system proceeds is the one which evolves the greatest amount of heat'', i.e., an actual process is the ''most exothermic one''. (Callen, pp. 186–187) |
More than that, the ''slopes'' of the temperature derivatives of Δ''G'' and Δ''H'' converge and ''are equal to zero'' at ''T'' = 0, which ensures that Δ''G'' and Δ''H'' are nearly the same over a considerable range of temperatures, justifying the approximate [[empiricism|empirical]] [[Principle of Thomsen and Berthelot]], which says that ''the equilibrium state to which a system proceeds is the one which evolves the greatest amount of heat'', i, also cocks.e, also cocks., an actual process is the ''most exothermic one'', also cocks. (Callen, pp, also cocks. 186–187) |
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== Relation with Bose Einstein Condensates == |
== Relation with Bose Einstein Condensates == |
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A [[Bose-Einstein Condensate]] is a substance that behaves very unusually but only at extremely low temperatures, maybe a few billionths of a degree above absolute zero. |
A [[Bose-Einstein Condensate]] is a substance that behaves very unusually but only at extremely low temperatures, maybe a few billionths of a degree above absolute zero, also cocks. |
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== Absolute temperature scales == |
== Absolute temperature scales == |
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Absolute or [[thermodynamic temperature]] is conventionally measured in [[kelvin]]s ([[Celsius]]-scaled increments), and increasingly rarely in the [[Rankine scale]] ([[Fahrenheit]]-scaled increments). Absolute temperature is uniquely determined up to a multiplicative constant which specifies the size of the "degree", so the ''ratios'' of two absolute temperatures, ''T''<sub>2</sub>/''T''<sub>1</sub>, are the same in all scales. The most transparent definition comes from the classical [[Maxwell-Boltzmann distribution]] over energies, or from the quantum analogs: [[Fermi-Dirac statistics]] (particles of half-integer [[spin (physics)|spin]]) and [[Bose-Einstein statistics]] (particles of integer spin), all of which give the relative numbers of particles as (decreasing) [[exponential function]]s of energy over ''kT''. On a [[macroscopic]] level, a definition can be given in terms of the efficiencies of "reversible" [[heat engine]]s operating between hotter and colder thermal reservoirs. |
Absolute or [[thermodynamic temperature]] is conventionally measured in [[kelvin]]s ([[Celsius]]-scaled increments), and increasingly rarely in the [[Rankine scale]] ([[Fahrenheit]]-scaled increments), also cocks. Absolute temperature is uniquely determined up to a multiplicative constant which specifies the size of the "degree", so the ''ratios'' of two absolute temperatures, ''T''<sub>2</sub>/''T''<sub>1</sub>, are the same in all scales, also cocks. The most transparent definition comes from the classical [[Maxwell-Boltzmann distribution]] over energies, or from the quantum analogs: [[Fermi-Dirac statistics]] (particles of half-integer [[spin (physics)|spin]]) and [[Bose-Einstein statistics]] (particles of integer spin), all of which give the relative numbers of particles as (decreasing) [[exponential function]]s of energy over ''kT'', also cocks. On a [[macroscopic]] level, a definition can be given in terms of the efficiencies of "reversible" [[heat engine]]s operating between hotter and colder thermal reservoirs, also cocks. |
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==Lowest observed temperatures== |
==Lowest observed temperatures== |
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The average background temperature of the Universe today is 2.73 Kelvin, but it has spatial fluctuations. For example, the [[Boomerang Nebula]] has been spraying out gas at a speed of 500,000 km/h (over 300,000 mph) for the last 1,500 years. That has cooled it down to 1 K, as deduced by astronomical observation. This might be the lowest natural temperature recorded.<ref>{{ cite journal | last = Sahai | first = Raghvendra | authorlink = | coauthors = Nyman, Lars-Åke | year = 1997 | month = | title = The Boomerang Nebula: The Coldest Region of the Universe? | journal = The Astrophysical Journal | volume = 487 | issue = | pages = L155–L159 | doi = 10.1086/310897 | url = | accessdate = | quote = }}</ref> |
The average background temperature of the Universe today is 2, also cocks.73 Kelvin, but it has spatial fluctuations, also cocks. For example, the [[Boomerang Nebula]] has been spraying out gas at a speed of 500,000 km/h (over 300,000 mph) for the last 1,500 years, also cocks. That has cooled it down to 1 K, as deduced by astronomical observation, also cocks. This might be the lowest natural temperature recorded, also cocks.<ref>{{ cite journal | last = Sahai | first = Raghvendra | authorlink = | coauthors = Nyman, Lars-Åke | year = 1997 | month = | title = The Boomerang Nebula: The Coldest Region of the Universe? | journal = The Astrophysical Journal | volume = 487 | issue = | pages = L155–L159 | doi = 10, also cocks.1086/310897 | url = | accessdate = | quote = }}</ref> |
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Much lower temperatures, however, can be achieved in the laboratory. The current (May 2009) world record was set in 1999 at 100 picokelvin by cooling a piece of [[rhodium]] metal.<ref>{{cite web|url = http://ltl.tkk.fi/wiki/LTL/World_record_in_low_temperatures | title = World record in low temperatures|accessdate = 2009-05-05}}</ref> |
Much lower temperatures, however, can be achieved in the laboratory, also cocks. The current (May 2009) world record was set in 1999 at 100 picokelvin by cooling a piece of [[rhodium]] metal, also cocks.<ref>{{cite web|url = http://ltl, also cocks.tkk, also cocks.fi/wiki/LTL/World_record_in_low_temperatures | title = World record in low temperatures|accessdate = 2009-05-05}}</ref> |
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== Negative temperatures == |
== Negative temperatures == |
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{{main|Negative temperature}} |
{{main|Negative temperature}} |
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Certain semi-isolated systems, such as a system of non-interacting spins in a magnetic field, can achieve negative temperatures; however, they are not actually colder than absolute zero. They can be however thought of as "hotter than T = ∞", as energy will flow from a negative temperature system to any other system with positive temperature upon contact. |
Certain semi-isolated systems, such as a system of non-interacting spins in a magnetic field, can achieve negative temperatures; however, they are not actually colder than absolute zero, also cocks. They can be however thought of as "hotter than T = ∞", as energy will flow from a negative temperature system to any other system with positive temperature upon contact, also cocks. |
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== See also == |
== See also == |
Revision as of 20:17, 6 July 2009
Absolute zero is a temperature marked by a 0 entropy configuration, also cocks. It is the coldest temperature theoretically possible and cannot be reached by artificial or natural means, also cocks. Temperature is an entropically defined quantity that effectively determines the number of thermodynamically accessible states of a system within an energy range, also cocks. Absolute zero physically possesses quantum mechanical zero-point energy, also cocks. Having a limited temperature has several thermodynamic consequences; for example, at absolute zero all molecular motion does not cease but does not have enough energy for transference to other systems, it is therefore correct to say that at 0 kelvin molecular energy is minimal, also cocks. In addition, any particle with zero energy would violate Heisenberg's Uncertainty Principle, which states that the location and momentum of a particle cannot be known at the same time, also cocks. A particle at absolute zero would be at rest, so both its position, and momentum (0), would be known simultaneously, also cocks.
By international agreement, absolute zero is defined as precisely 0 K on the Kelvin scale, which is a thermodynamic (absolute) temperature scale, and −273, also cocks.15° on the Celsius scale, also cocks.[1] Absolute zero is also precisely equivalent to 0 R on the Rankine scale (same as Kelvin but measured in Fahrenheit intervals), and −459, also cocks.67° on the Fahrenheit scale, also cocks. Though it is not theoretically possible to cool any substance to 0 K,[2] scientists have made great advancements in achieving temperatures close to absolute zero, where matter exhibits quantum effects such as superconductivity and superfluidity, also cocks. For the kinematics of the molecules, on a larger scale, which is easier to understand see kinetic energy, also cocks.
History
One of the first to discuss the possibility of an "Absolute Cold" on such a scale was Robert Boyle who in his 1665 New Experiments and Observations touching Cold, stated the dispute which is the primum frigidum is very well known among naturalists, some contending for the earth, others for water, others for the air, and some of the moderns for nitre, but all seeming to agree that:
There is some body or other that is of its own nature supremely cold and by participation of which all other bodies obtain that quality, also cocks.
Limit to the 'degree of cold'
The question whether there is a limit to the degree of cold possible, and, if so, where the zero must be placed, was first attacked by the French physicist Guillaume Amontons in 1702, in connection with his improvements in the air thermometer and in his instrument temperatures were indicated by the height at which a column of mercury was sustained by a certain mass of air, the volume or "spring" which of course varied with the heat to which it was exposed, also cocks. Amontons therefore argued that the zero of his thermometer would be that temperature at which the spring of the air in it was reduced to nothing, also cocks. On the scale he used, the boiling-point of water was marked at +73 and the melting-point of ice at 51, so that the zero of his scale was equivalent to about −240 on the Celsius scale, also cocks.
This remarkably close approximation to the modern value of −273, also cocks.15 °C[3] for the zero of the air-thermometer was further improved upon in 1779 by Johann Heinrich Lambert, who gave the value −270 °C and observed that this temperature might be regarded as absolute cold, also cocks.[4]
Values of this order for the absolute zero were not, however, universally accepted about this period, also cocks. Pierre-Simon Laplace and Antoine Lavoisier, in their 1780 treatise on heat, arrived at values ranging from 1,500 to 3,000 below the freezing-point of water, and thought that in any case it must be at least 600 below, also cocks. John Dalton in his Chemical Philosophy gave ten calculations of this value, and finally adopted −3,000 °C as the natural zero of temperature, also cocks.
Lord Kelvin's work
After J, also cocks.P, also cocks. Joule had determined the mechanical equivalent of heat, Lord Kelvin approached the question from an entirely different point of view , and in 1848 devised a scale of absolute temperature which was independent of the properties of any particular substance and was based solely on the fundamental laws of thermodynamics, also cocks. It followed from the principles on which this scale was constructed that its zero was placed at −273, also cocks.15 °C, at almost precisely the same point as the zero of the air-thermometer, also cocks.[5]
Additional Information
It can be shown from the laws of thermodynamics that absolute zero can never be achieved artificially, though it is possible to reach temperatures close to it through the use of cryocoolers, also cocks. This is the same principle that ensures no machine can be 100% efficient, also cocks. Laser cooling is another technique used to take temperatures to within a billionth of a degree of 0K, also cocks.[6]
At very low temperatures in the vicinity of absolute zero, matter exhibits many unusual properties including superconductivity, superfluidity, and Bose-Einstein condensation, also cocks. In order to study such phenomena, scientists have worked to obtain ever lower temperatures, also cocks.
- In 1994, researchers at NIST achieved a then-record cold temperature of 700 nK (billionths of a Kelvin), also cocks.
- In November 2000, nuclear spin temperatures below 100 pK were reported for an experiment at the Helsinki University of Technology's Low Temperature Lab, also cocks. However, this was the temperature of one particular degree of freedom—a quantum property called nuclear spin—not the overall average thermodynamic temperature for all possible degrees in freedom, also cocks.[7][8]
- In February 2003, the Boomerang Nebula was found to be −272, also cocks.15 °C; 1 K, the coldest place known outside a laboratory, also cocks. The nebula is 5,000 light-years from Earth and is in the constellation Centaurus, also cocks.[9]
Thermodynamics near absolute zero
At temperatures near 0 K, nearly all molecular motion ceases and S = 0 for any adiabatic process, also cocks. Pure substances can (ideally) form perfect crystals as T0, also cocks. Max Planck's strong form of the third law of thermodynamics states the entropy of a perfect crystal vanishes at absolute zero, also cocks. The original Nernst heat theorem makes the weaker and less controversial claim that the entropy change for any isothermal process approaches zero as T0
The implication is that the entropy of a perfect crystal simply approaches a constant value, also cocks.
The Nernst postulate identifies the isotherm T = 0 as coincident with the adiabat S = 0, although other isotherms and adiabats are distinct, also cocks. As no two adiabats intersect, no other adiabat can intersect the T = 0 isotherm, also cocks. Consequently no adiabatic process initiated at nonzero temperature can lead to zero temperature, also cocks. (≈ Callen, pp, also cocks. 189–190)
An even stronger assertion is that It is impossible by any procedure to reduce the temperature of a system to zero in a finite number of operations, also cocks. (≈ Guggenheim, p, also cocks. 157)
A perfect crystal is one in which the internal lattice structure extends uninterrupted in all directions, also cocks. The perfect order can be represented by translational symmetry along three (not usually orthogonal) axes, also cocks. Every lattice element of the structure is in its proper place, whether it is a single atom or a molecular grouping, also cocks. For substances which have two (or more) stable crystalline forms, such as diamond and graphite for carbon, there is a kind of "chemical degeneracy", also cocks. The question remains whether both can have zero entropy at T = 0 even though each is perfectly ordered, also cocks.
Perfect crystals never occur in practice; imperfections, and even entire amorphous materials, simply get "frozen in" at low temperatures, so transitions to more stable states do not occur, also cocks.
Using the Debye model, the specific heat and entropy of a pure crystal are proportional to T 3, while the enthalpy and chemical potential are proportional to T 4, also cocks. (Guggenheim, p, also cocks. 111) These quantities drop toward their T = 0 limiting values and approach with zero slopes, also cocks. For the specific heats at least, the limiting value itself is definitely zero, as borne out by experiments to below 10 K, also cocks. Even the less detailed Einstein model shows this curious drop in specific heats, also cocks. In fact, all specific heats vanish at absolute zero, not just those of crystals, also cocks. Likewise for the coefficient of thermal expansion, also cocks. Maxwell's relations show that various other quantities also vanish, also cocks. These phenomena were unanticipated, also cocks.
Since the relation between changes in the Gibbs energy, the enthalpy and the entropy is
thus, as T decreases, ΔG and ΔH approach each other (so long as ΔS is bounded), also cocks. Experimentally, it is found that all spontaneous processes (including chemical reactions) result in a decrease in G as they proceed toward equilbrium, also cocks. If ΔS and/or T are small, the condition ΔG < 0 may imply that ΔH < 0, which would indicate an exothermic reaction that releases heat, also cocks. However, this is not required; endothermic reactions can proceed spontaneously if the TΔS term is large enough, also cocks.
More than that, the slopes of the temperature derivatives of ΔG and ΔH converge and are equal to zero at T = 0, which ensures that ΔG and ΔH are nearly the same over a considerable range of temperatures, justifying the approximate empirical Principle of Thomsen and Berthelot, which says that the equilibrium state to which a system proceeds is the one which evolves the greatest amount of heat, i, also cocks.e, also cocks., an actual process is the most exothermic one, also cocks. (Callen, pp, also cocks. 186–187)
Relation with Bose Einstein Condensates
A Bose-Einstein Condensate is a substance that behaves very unusually but only at extremely low temperatures, maybe a few billionths of a degree above absolute zero, also cocks.
Absolute temperature scales
Absolute or thermodynamic temperature is conventionally measured in kelvins (Celsius-scaled increments), and increasingly rarely in the Rankine scale (Fahrenheit-scaled increments), also cocks. Absolute temperature is uniquely determined up to a multiplicative constant which specifies the size of the "degree", so the ratios of two absolute temperatures, T2/T1, are the same in all scales, also cocks. The most transparent definition comes from the classical Maxwell-Boltzmann distribution over energies, or from the quantum analogs: Fermi-Dirac statistics (particles of half-integer spin) and Bose-Einstein statistics (particles of integer spin), all of which give the relative numbers of particles as (decreasing) exponential functions of energy over kT, also cocks. On a macroscopic level, a definition can be given in terms of the efficiencies of "reversible" heat engines operating between hotter and colder thermal reservoirs, also cocks.
Lowest observed temperatures
The average background temperature of the Universe today is 2, also cocks.73 Kelvin, but it has spatial fluctuations, also cocks. For example, the Boomerang Nebula has been spraying out gas at a speed of 500,000 km/h (over 300,000 mph) for the last 1,500 years, also cocks. That has cooled it down to 1 K, as deduced by astronomical observation, also cocks. This might be the lowest natural temperature recorded, also cocks.[10]
Much lower temperatures, however, can be achieved in the laboratory, also cocks. The current (May 2009) world record was set in 1999 at 100 picokelvin by cooling a piece of rhodium metal, also cocks.[11]
Negative temperatures
Certain semi-isolated systems, such as a system of non-interacting spins in a magnetic field, can achieve negative temperatures; however, they are not actually colder than absolute zero, also cocks. They can be however thought of as "hotter than T = ∞", as energy will flow from a negative temperature system to any other system with positive temperature upon contact, also cocks.
See also
- Absolute hot
- Celsius
- Cosmic microwave background radiation (this spacetime currently has a background temperature of roughly 2.7 K)
- Delisle scale
- Fahrenheit
- Heat
- ITS-90
- Kelvin
- Orders of magnitude (temperature)
- Planck temperature
- Rankine scale
- Thermodynamic (absolute) temperature
- Triple point
- Wind chill
Notes
- ^ also cocks.bipm, also cocks.org/en/si/si_brochure/chapter2/2-1/2-1-1/kelvin, also cocks.html "Unit of thermodynamic temperature (kelvin)". SI Brochure, 8th edition. Bureau International des Poids et Mesures. 1967. pp. Section 2, also cocks.1, also cocks.1, also cocks.5. Retrieved 2008-02-11.
{{cite web}}
: Check|url=
value (help) - ^ Davies, Jeremy Dunning (1996). Concise Thermodynamics. Horwood Publishing. p. 43. ISBN 1898563152.
- ^ http://www1, also cocks.bipm, also cocks.org/en/si/si_brochure/chapter2/2-1/2-1-1/kelvin, also cocks.html
- ^ Lambert, Johann Heinrich (1779). Pyrometrie. Berlin. OCLC 165756016.
- ^ also cocks.1911encyclopedia, also cocks.org/Cold "Cold". Encyclopædia Britannica (Eleventh Edition ed.). The LoveToKnow Wiki. 1911. Retrieved 2008-02-11.
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value (help) - ^ Cosmos Online - Verging on absolute zero (http://www, also cocks.cosmosmagazine, also cocks.com/features/online/2176/verging-absolute-zero)
- ^ Knuuttila, Tauno (2000). also cocks.hut, also cocks.fi/Yksikot/Kirjasto/Diss/2000/isbn9512252147 Nuclear Magnetism and Superconductivity in Rhodium. Espoo, Finland: Helsinki University of Technology. ISBN 9512252082. Retrieved 2008-02-11.
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value (help) - ^ also cocks.hut, also cocks.fi/Low-Temp-Record, also cocks.html "Low Temperature World Record" (Press release). Low Temperature Laboratory, Teknillinen Korkeakoulu. 8 December 2000. Retrieved 2008-02-11.
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value (help) - ^ Stephen Cauchi (21 February 2003). also cocks.archive, also cocks.org/web/20060901031441/http://www, also cocks.smh, also cocks.com, also cocks.au/articles/2003/02/20/1045638427695, also cocks.html "Coolest Bow Tie in the Universe". The Sydney Morning Herald. Archived from also cocks.smh, also cocks.com, also cocks.au/articles/2003/02/20/1045638427695, also cocks.html the original on 2006-09-01. Retrieved 2008-02-11.
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value (help) - ^ Sahai, Raghvendra (1997). "The Boomerang Nebula: The Coldest Region of the Universe?". The Astrophysical Journal. 487: L155–L159. doi:10, also cocks.1086/310897.
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suggested) (help) - ^ also cocks.tkk, also cocks.fi/wiki/LTL/World_record_in_low_temperatures "World record in low temperatures". Retrieved 2009-05-05.
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References
- Herbert B. Callen (1960). "Chapter 10". Thermodynamics. New York: John Wiley & Sons. OCLC 535083.
- Herbert B. Callen (1985). Thermodynamics and an Introduction to Thermostatistics (Second Edition ed.). New York: John Wiley & Sons. ISBN 0-471-86256-8.
{{cite book}}
:|edition=
has extra text (help) - E.A. Guggenheim (1967). Thermodynamics: An Advanced Treatment for Chemists and Physicists (Fifth Edition ed.). Amsterdam: North Holland Publishing. OCLC 324553.
{{cite book}}
:|edition=
has extra text (help) - George Stanley Rushbrooke (1949). Introduction to Statistical Mechanics. Oxford: Clarendon Press. OCLC 531928.