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{{Thermodynamics|expanded=Potentials}}
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In [[thermodynamics]], the '''Gibbs free energy''' ([[IUPAC]] recommended name: '''Gibbs energy''' or '''Gibbs function'''; also known as '''free enthalpy'''<ref>{{cite book | last1=Greiner | first1=Walter | last2=Neise | first2=Ludwig | last3=Stöcker | first3=Horst | title=Thermodynamics and statistical mechanics
| publisher=Springer-Verlag | year=1995 | page=101 }}</ref> to distinguish it from [[Helmholtz free energy]]) is a [[thermodynamic potential]] that measures the "usefulness" or process-initiating [[Work (thermodynamics)|work]] obtainable from a [[thermodynamic system]] at a constant temperature and pressure ([[isothermal]], [[Isobaric process|isobaric]]).  Just as in [[mechanics]], where [[potential energy]] is defined as capacity to do work, similarly different potentials have different meanings.  The Gibbs free energy (SI units J/mol) is the ''maximum'' amount of non-expansion work that can be extracted from a [[closed system]]; this maximum can be attained only in a completely [[reversible process (thermodynamics)|reversible process]]. When a system changes from a well-defined initial state to a well-defined final state, the Gibbs free energy Δ''G'' equals the work exchanged by the system with its surroundings, minus the work of the [[pressure]] forces, during a reversible transformation of the system from the same initial state to the same final state.<ref name="Perrot" >{{cite book | last = Perrot | first = Pierre | title = A to Z of Thermodynamics | publisher = Oxford University Press | year = 1998 | isbn = 0-19-856552-6}}</ref>
 
Gibbs energy (also referred to as ∆G) is also the chemical potential that is minimized when a system reaches equilibrium at constant pressure and temperature. Its derivative with respect to the reaction coordinate of the system vanishes at the equilibrium point. As such, it is a convenient criterion of spontaneity for processes with constant pressure and temperature.
 
The Gibbs free energy, originally called ''available energy'', was developed in the 1870s by the American mathematician [[Josiah Willard Gibbs]]. In 1873, Gibbs described this “available energy” as
{{quote|the greatest amount of mechanical work which can be obtained from a given quantity of a certain substance in a given initial state, without increasing its total [[Volume (thermodynamics)|volume]] or allowing [[heat]] to pass to or from external bodies, except such as at the close of the processes are left in their initial condition.<ref>J.W. Gibbs, “A Method of Geometrical Representation of the Thermodynamic Properties of Substances by Means of Surfaces,” ''Transactions of the Connecticut Academy of Arts and Sciences'' 2, Dec. 1873, pp. 382-404 (quotation on p. 400).</ref>}}
 
The initial state of the body, according to Gibbs, is supposed to be such that "the body can be made to pass from it to states of [[dissipated energy]] by [[Reversible process (thermodynamics)|reversible processes]]."  In his 1876 [[magnum opus]] ''[[On the Equilibrium of Heterogeneous Substances]]'', a graphical analysis of multi-phase chemical systems, he engaged his thoughts on chemical free energy in full.
 
== Overview ==
[[File:Diamond.jpg|thumb|right|The reaction C<sub>(s)</sub><sup>diamond</sup>⇒C<sub>(s)</sub><sup>graphite</sup> has a negative change in Gibbs free energy and is therefore thermodynamically favorable at 25°C and 1 atm. However, even though favorable, it is so slow that it is not observed.  Whether a reaction is thermodynamically favorable does not determine its rate.]]
In a simple manner, with respect to [[standard temperature and pressure|STP]] reacting systems, a general [[rule of thumb]] is that every system seeks to achieve a minimum of free energy.
 
Hence, out of this general natural tendency, a quantitative measure as to how near or far a potential reaction is from this minimum is when the calculated energetics of the process indicate that the change in Gibbs free energy Δ''G'' is negative.  In essence, this means that such a reaction will be favoured and will release energy.  The energy released equals the maximum amount of work that can be performed as a result of the chemical reaction.  In contrast, if conditions indicated a positive Δ''G'', then energy—in the form of work—would have to be added to the reacting system for the reaction to occur.
 
The equation can also be seen from the perspective of both the system and its surroundings (the universe). For the purposes of calculation, we assume the reaction is the only reaction going on in the universe. Thus the entropy released or absorbed by the system is actually the entropy that the environment must absorb or release respectively. Thus the reaction will only be allowed if the total entropy change of the universe is equal to zero (a [[thermal equilibrium]] state) or positive. The input of heat into an "endergonic" chemical reaction (e.g. the elimination of [[cyclohexanol]] to [[cyclohexene]]) can be seen as coupling an inherently unfavourable reaction (elimination) to a favourable one (burning of coal or the energy source of a heat source) such that the total entropy change of the universe is more than or equal to zero, making the Gibbs free energy of the coupled reaction negative.
 
In traditional use, the term “free” was attached to Gibbs free energy for systems at constant pressure and temperature to mean "available in the form of useful work."<ref name="Perrot" />  For Gibbs free energy, we add the qualification that it is the energy free for non-volume work.<ref>{{cite book | last = Reiss | first = Howard | title = Methods of Thermodynamics | publisher = Dover Publications | year = 1965 | isbn = 0-486-69445-3}}</ref> (A similar meaning applies used in conjunction with Helmholtz free energy, for systems at constant volume and temperature).  However, an increasing number of books and journal articles do not include the attachment “free”, referring to G as simply "Gibbs energy". This is the result of a 1988 [[IUPAC]] meeting to set unified terminologies for the international scientific community, in which the adjective ‘free’ was supposedly banished.<ref>{{cite journal|title=Glossary of Atmospheric Chemistry Terms (Recommendations 1990) |url=http://www.iupac.org/publications/pac/1990/pdf/6211x2167.pdf|journal=[[Pure and Applied Chemistry|Pure Appl. Chem.]]|volume=62|pages=2167&ndash;2219|year=1990|last=[[International Union of Pure and Applied Chemistry]] Commission on Atmospheric Chemistry|accessdate=2006-12-28|doi=10.1351/pac199062112167|first1=J. G.|issue=11}}</ref>
<ref>{{cite book|last=[[International Union of Pure and Applied Chemistry]] Commission on Physicochemical Symbols Terminology and Units|title=Quantities, Units and Symbols in Physical Chemistry (2nd Edition)|publisher=Blackwell Scientific Publications|location=Oxford|year=1993
|url=http://www.iupac.org/home/publications/e-resources/nomenclature-and-terminology/quantities-units-and-symbols-in-physical-chemistry-green-book.html|isbn=0-632-03583-8|accessdate=2013-12-20|pages=251}}</ref>
<ref>{{cite journal|title=Glossary of Terms in Quantities and Units in Clinical Chemistry (IUPAC-IFCC Recommendations 1996) |url=http://www.iupac.org/publications/pac/1996/pdf/6804x0957.pdf|journal=[[Pure and Applied Chemistry|Pure Appl. Chem.]]|volume=68|pages=957&ndash;1000|year=1996|last=[[International Union of Pure and Applied Chemistry]] Commission on Quantities and Units in Clinical Chemistry|coauthors=[[International Federation of Clinical Chemistry and Laboratory Medicine]] Committee on Quantities and Units|accessdate=2006-12-28|doi=10.1351/pac199668040957|first1=H. P.|issue=4}}</ref>  This standard, however, has not yet been universally adopted.
 
==History==
{{see also|Thermodynamic free energy#History|l1=Thermodynamic free energy}}
The quantity called "free energy" is a more advanced and accurate replacement for the outdated term ''affinity'', which was used by chemists in previous years to describe the ''force'' that caused [[chemical reaction]]s.
 
In 1873, [[Willard Gibbs]] published ''A Method of Geometrical Representation of the Thermodynamic Properties of Substances by Means of Surfaces'', in which he introduced the preliminary outline of the principles of his new equation able to predict or estimate the tendencies of various natural processes to ensue when bodies or systems are brought into contact. By studying the interactions of homogeneous substances in contact, i.e., bodies, being in composition part solid, part liquid, and part vapor, and by using a three-dimensional [[Volume (thermodynamics)|volume]]-[[entropy]]-[[internal energy]] graph, Gibbs was able to determine three states of equilibrium, i.e., "necessarily stable", "neutral", and "unstable", and whether or not changes would ensue.
 
Hence, in 1882, the German scientist [[Hermann von Helmholtz]] stated that affinity is the largest quantity of work which can be gained when the reaction is carried out in a reversible manner, e.g., electrical work in a reversible cell.  The maximum work is thus regarded as the diminution of the free, or available, energy of the system (''Gibbs free energy'' ''G'' at ''T'' = constant, ''P'' = constant or ''Helmholtz free energy'' ''F'' at ''T'' = constant, ''V'' = constant), whilst the heat given out is usually a measure of the diminution of the total energy of the system ([[Internal energy]]). Thus, ''G'' or ''F'' is the amount of energy “free” for work under the given conditions.
 
Until this point, the general view had been such that: “all chemical reactions drive the system to a state of equilibrium in which the affinities of the reactions vanish”.  Over the next 60 years, the term affinity came to be replaced with the term free energy.  According to chemistry historian Henry Leicester, the influential 1923 textbook ''Thermodynamics and the Free Energy of Chemical Substances'' by [[Gilbert N. Lewis]] and [[Merle Randall]] led to the replacement of the term “affinity” by the term “free energy” in much of the English-speaking world.
 
==Graphical interpretation==
Gibbs free energy was originally defined graphically.  In 1873, American engineer [[Willard Gibbs]] published his first thermodynamics paper, “Graphical Methods in the Thermodynamics of Fluids”, in which Gibbs used the two coordinates of the entropy and volume to represent the state of the body. In his second follow-up paper, “A Method of Geometrical Representation of the Thermodynamic Properties of Substances by Means of Surfaces”, published later that year, Gibbs added in the third coordinate of the energy of the body, defined on three figures. In 1874, Scottish physicist [[James Clerk Maxwell]] used Gibbs' figures to make a 3D energy-entropy-volume [[Maxwell's thermodynamic surface|thermodynamic surface]] of a fictitious water-like substance.<ref>James Clerk Maxwell, Elizabeth Garber, Stephen G. Brush, and C. W. Francis Everitt (1995), ''[http://books.google.com/books?id=hA-oIDR0eXkC&pg=PA248 Maxwell on heat and statistical mechanics: on "avoiding all personal enquiries" of molecules]'', Lehigh University Press, ISBN 093422334, p. 248.</ref> Thus, in order to understand the very difficult concept of Gibbs free energy one must be able to understand its interpretation as Gibbs defined originally by section AB on his figure 3 and as Maxwell sculpted that section on his [[Maxwell's thermodynamic surface|3D surface figure]].
 
[[File:Gibbs-Maxwell surfaces.png|1000px|center|thumb|American engineer [[Willard Gibbs]]' 1873 figures two and three (above left and middle) used by Scottish physicist [[James Clerk Maxwell]] in 1874 to create a three-dimensional [[entropy]] (x), [[Volume (thermodynamics)|volume]] (y), [[energy]] (z) '''[[Maxwell's thermodynamic surface|thermodynamic surface]]''' diagram for a fictitious water-like substance, transposed the two figures of Gibbs (above right) onto the volume-entropy coordinates (transposed to bottom of cube) and energy-entropy coordinates (flipped upside down and transposed to back of cube), respectively, of a three-dimensional [[Cartesian coordinates]]; the region AB being the first-ever three-dimensional representation of Gibbs free energy, or what Gibbs called "available energy"; the region AC being its capacity for [[entropy]], what Gibbs defined as "the amount by which the entropy of the body can be increased without changing the energy of the body or increasing its volume.]]
 
==Definitions==
[[File:Wykres Gibbsa.svg|275px|thumb|right|[[Willard Gibbs]]’ 1873 '''available energy''' (free energy) graph, which shows a plane perpendicular to the axis of ''v'' ([[Volume (thermodynamics)|volume]]) and passing through point A, which represents the initial state of the body.  MN is the section of the surface of [[dissipated energy]]. Q''ε'' and Q''η'' are sections of the planes ''η'' = 0 and ''ε'' = 0, and therefore parallel to the axes of ''ε'' ([[internal energy]]) and ''η'' ([[entropy]]), respectively. AD and AE are the energy and entropy of the body in its initial state, AB and AC its ''available energy'' (Gibbs free energy) and its ''capacity for entropy'' (the amount by which the entropy of the body can be increased without changing the energy of the body or increasing its volume) respectively.]]
The Gibbs free energy is defined as:
 
:''G(p,T)'' = ''U'' + ''pV'' − ''TS''
 
which is the same as:
:''G(p,T)'' = ''H'' − ''TS''
 
where:
* ''U'' is the [[internal energy]] ([[SI]] unit: [[joule]])
* ''p'' is [[pressure]] (SI unit: [[Pascal (unit)|pascal]])
* ''V'' is [[Volume (thermodynamics)|volume]] (SI unit: m<sup>3</sup>)
* ''T'' is the [[temperature]] (SI unit: [[kelvin]])
* ''S'' is the [[entropy]] (SI unit: joule per kelvin)
* ''H'' is the [[enthalpy]] (SI unit: joule)
 
The expression for the infinitesimal reversible change in the Gibbs free energy as a function of its 'natural variables' p and T, for an [[Thermodynamic_system#Open_system|open system]], subjected to the operation of external forces (for instance electrical or magnetical) ''X<sub>i</sub>'', which cause the external parameters of the system ''a<sub>i</sub>'' to change by an amount d''a<sub>i</sub>'', can be derived as follows from the First Law for reversible processes:
 
<math>T\mathrm{d}S= \mathrm{d}U + p\mathrm{d}V-\sum_{i=1}^k \mu_i \,\mathrm{d}N_i + \sum_{i=1}^n X_i \,\mathrm{d}a_i + \cdots</math>
<br>
<math>\mathrm{d}(TS) - S\mathrm{d}T= \mathrm{d}U + \mathrm{d}(pV) - V\mathrm{d}p-\sum_{i=1}^k \mu_i \,\mathrm{d}N_i + \sum_{i=1}^n X_i \,\mathrm{d}a_i + \cdots</math>
<br>
<math>\mathrm{d}(U-TS+pV)=V\mathrm{d}p-S\mathrm{d}T+\sum_{i=1}^k \mu_i \,\mathrm{d}N_i - \sum_{i=1}^n X_i \,\mathrm{d}a_i + \cdots</math>
<br>
<math>\mathrm{d}G =V\mathrm{d}p-S\mathrm{d}T+\sum_{i=1}^k \mu_i \,\mathrm{d}N_i - \sum_{i=1}^n X_i \,\mathrm{d}a_i + \cdots</math>
 
where:
* ''μ''<sub>''i''</sub> is the [[chemical potential]] of the ''i''th [[chemical species|chemical component]]. (SI unit: joules per particle<ref>[http://goldbook.iupac.org/C01032.html Chemical Potential] - IUPAC Gold Book</ref> or joules per mole<ref name="Perrot" />)
* ''N''<sub>''i''</sub> is the [[particle number|number of particles]] (or number of moles) composing the ''i''th chemical component.
 
This is one form of '''Gibbs fundamental equation'''.<ref>{{cite book | last = Müller | first = Ingo | title = A History of Thermodynamics - the Doctrine of Energy and Entropy | publisher = Springer | year = 2007 | isbn = 978-3-540-46226-2}}</ref>  In the infinitesimal expression, the term involving the chemical potential accounts for changes in Gibbs free energy resulting from an influx or outflux of particles. In other words, it holds for an [[Open system (systems theory)|open system]]. For a [[closed system]], this term may be dropped.
 
Any number of extra terms may be added, depending on the particular system being considered. Aside from [[mechanical work]], a system may, in addition, perform numerous other types of work.  For example, in the infinitesimal expression, the contractile work energy associated with a thermodynamic system that is a contractile fiber that shortens by an amount −d''l'' under a force ''f'' would result in a term ''f''d''l'' being added.  If a quantity of charge −d''e'' is acquired by a system at an electrical potential Ψ, the electrical work associated with this is −Ψd''e'', which would be included in the infinitesimal expression.  Other work terms are added on per system requirements.<ref>{{cite book | last = Katchalsky | first = A. | coauthors = Curran, Peter, F.| title = Nonequilibrium Thermodynamics in Biophysics | publisher = [[Harvard University Press]] | year = 1965 | id = CCN 65-22045}}</ref>
 
Each quantity in the equations above can be divided by the amount of substance, measured in [[Mole (unit)|moles]], to form ''molar Gibbs free energy''. The Gibbs free energy is one of the most important thermodynamic functions for the characterization of a system. It is a factor in determining outcomes such as the [[voltage]] of an [[electrochemical cell]], and the [[equilibrium constant]] for a [[reversible reaction]]. In isothermal, isobaric systems, Gibbs free energy can be thought of as a "dynamic" quantity, in that it is a representative measure of the competing effects of the enthalpic and entropic driving forces involved in a thermodynamic process.
 
The temperature dependence of the Gibbs energy for an [[ideal gas]] is given by the [[Gibbs-Helmholtz equation]] and its pressure dependence is given by:
 
:<math>\frac{G}{N}  = \frac{G}{N}^\circ  + kT\ln \frac{p}{{p^\circ }}</math>
 
if the volume is known rather than pressure then it becomes:
 
:<math>\frac{G}{N}  = \frac{G}{N}^\circ  + kT\ln \frac{V^\circ}{{V }}</math>
 
or more conveniently as its [[chemical potential]]:
 
:<math>\frac{G}{N}  = \mu  = \mu^\circ  + kT\ln \frac{p}{{p^\circ }}.</math>
 
In non-ideal systems, [[fugacity]] comes into play.
 
==Derivation==
The Gibbs free energy [[total differential]] [[Thermodynamic potential#Natural_variables|natural variables]] may be derived via [[Legendre transform]]s of the [[internal energy]].
:<math>\mathrm{d}U = T\mathrm{d}S - p \,\mathrm{d}V + \sum_i \mu_i \,\mathrm{d} N_i\,</math>.
 
Because ''S'', ''V'', and ''N''<sub>''i''</sub> are [[Intensive and extensive properties|extensive variables]], [[Homogeneous function|Euler's homogeneous function theorem]] allows easy integration of d''U'':<ref name="Salzman2001">{{cite web |url=http://www.chem.arizona.edu/~salzmanr/480a/480ants/opensys/opensys.html |title=Open Systems |accessdate=2007-10-11 |last=Salzman |first=William R. |date=2001-08-21 |work=Chemical Thermodynamics |publisher=[[University of Arizona]] |archiveurl=http://web.archive.org/web/20070707224025/http://www.chem.arizona.edu/~salzmanr/480a/480ants/opensys/opensys.html |archivedate=2007-07-07}}</ref>
 
:<math>U = T S - p V + \sum_i \mu_i N_i\,</math>.
 
The definition of ''G'' from above is
 
:<math>G = U + p V - T S\,</math>.
 
Taking the total differential, we have
 
:<math>\mathrm{d} G = \mathrm{d}U + p\,\mathrm{d}V + V\mathrm{d}p - T\mathrm{d}S - S\mathrm{d}T\,</math>.
 
Replacing d''U'' with the result from the first law gives<ref name="Salzman2001"/>
 
:<math>\mathrm{d} G = T\mathrm{d}S - p\,\mathrm{d}V + \sum_i \mu_i \,\mathrm{d} N_i + p \,\mathrm{d}V + V\mathrm{d}p - T\mathrm{d}S - S\mathrm{d}T\,</math>
:<math>\mathrm{d} G = V\mathrm{d}p - S\mathrm{d}T + \sum_i \mu_i \,\mathrm{d} N_i \,</math>.
 
The natural variables of ''G'' are then ''p'', ''T'', and {''N''<sub>''i''</sub>}.
 
=== Homogeneous systems ===
 
Because some of the natural variables are intensive, d''G'' may not be integrated using Euler integrals as is the case with internal energy. However, simply substituting the [[Gibbs-Duhem relation]] result for ''U'' into the definition of ''G'' gives a standard expression for ''G'':<ref name="Salzman2001"/>
 
:<math>G = T S - p V + \sum_i \mu_i N_i + p V - T S\,</math>
:<math>G = \sum_i \mu_i N_i\,</math>.
 
This result applies to homogeneous, macroscopic systems, but not to all thermodynamic systems.<ref>{{cite doi|10.1063/1.1740312}}</ref>
 
==Free energy of reactions==
To derive the Gibbs free energy equation for an [[isolated system]], let ''S''<sub>tot</sub> be the total entropy of the [[isolated system]], that is, a system that cannot exchange heat or mass with its surroundings. According to the [[second law of thermodynamics]]:
:<math> \Delta S_{tot} \ge 0 \,</math>
and if Δ''S''<sub>tot</sub> = 0 then the process is reversible. The heat transfer ''Q'' vanishes for an adiabatic system. Any [[adiabatic process]] that is also reversible is called an [[isentropic]] <math> \left( {Q\over T} = \Delta S = 0 \right) \,</math> process.
 
Now consider a system having internal entropy ''S''<sub>int</sub>. Such a system is thermally connected to its surroundings, which have entropy ''S''<sub>ext</sub>. The entropy form of the second law applies only to the closed system formed by both the system and its surroundings.  Therefore a process is possible only if
:<math> \Delta S_{int} + \Delta S_{ext} \ge 0 \,</math>.
 
If ''Q'' is the heat transferred to the system from the surroundings, then −''Q'' is the heat lost by the surroundings, so that
 
<math>\Delta S_{ext} = - {Q \over T},</math>  corresponds to the entropy change of the surroundings.
 
:We now have:
:<math> \Delta S_{int} - {Q \over T} \ge 0  \,</math>
:Multiplying both sides by ''T'':
:<math> T \Delta S_{int} - Q \ge 0 \,</math>
 
''Q'' is the heat transferred ''to'' the system; if the process is now assumed to be [[isobaric process|isobaric]], then ''Q''<sub>p</sub> = Δ''H'':
:<math> T \Delta S_{int} - \Delta H \ge 0\, </math>
Δ''H'' is the enthalpy change of reaction (for a chemical reaction at constant pressure). Then:
:<math> \Delta H - T \Delta S_{int} \le 0 \,</math>
for a possible process. Let the change Δ''G'' in Gibbs free energy be defined as
:<math> \Delta G = \Delta H - T \Delta S_{int} \,</math> ''(eq.1)''
Notice that it is not defined in terms of any external state functions, such as Δ''S''<sub>ext</sub> or Δ''S''<sub>tot</sub>. Then the second law, which also tells us about the spontaneity of the reaction,  
 
becomes:
:<math> \Delta G < 0 \,</math> '''favoured reaction''' (Spontaneous)
:<math> \Delta G = 0 \,</math> Neither the forward nor the reverse reaction prevails ([[Chemical equilibrium|Equilibrium]])
:<math> \Delta G > 0 \,</math> '''disfavoured reaction''' (Nonspontaneous)
 
Gibbs free energy ''G'' itself is defined as
:<math> G = H - T S_{int} \,</math>  ''(eq.2)''
but notice that to obtain equation (1) from equation (2) we must assume that ''T'' is constant. Thus, Gibbs free energy is most useful for thermochemical processes at constant temperature and pressure: both isothermal and isobaric.  Such processes don't move on a ''P''-''V'' diagram, such as phase change of a pure substance, which takes place at the saturation pressure and temperature. Chemical reactions, however, do undergo changes in [[chemical potential]], which is a state function.  Thus, thermodynamic processes are not confined to the two dimensional ''P''-''V'' diagram.  There is a third dimension for ''n'', the quantity of gas.  For the study of explosive chemicals, the processes are not necessarily isothermal and isobaric. For these studies, Helmholtz free energy is used.
 
If an isolated system (''Q'' = 0) is at constant pressure (''Q'' = Δ''H''), then
:<math> \Delta H = 0  \,</math>
 
Therefore the Gibbs free energy of an isolated system is <!-- 3/3/2010 10:48 EST: Isolated, not closed; closed systems can exchange energy and therefore have non-zero enthalpy changes -->
 
:<math> \Delta G = -T \Delta S \,</math>
 
and if Δ''G'' ≤ 0 then this implies that Δ''S'' ≥ 0, back to where we started the derivation of Δ''G.''
 
==Useful identities==
 
:<math>\Delta G = \Delta H - T \Delta S \,</math> (for constant temperature)
:<math>\Delta_r G^\circ = -R T \ln K \,</math>
:<math>\Delta_r G = \Delta_r G^\circ + R T \ln Q_r \,</math> (see [[Chemical equilibrium]])
:<math>\Delta G = -nFE \,</math>
:<math>\Delta G^\circ = -nFE^\circ \,</math>
 
and rearranging gives
 
:<math>nFE^\circ = RT \ln K \,</math>
:<math>nFE = nFE^\circ - R T \ln Q_r \, \,</math>
:<math>E = E^\circ - \frac{R T}{n F} \ln Q_r \, \,</math>
 
which relates the electrical potential of a reaction to the equilibrium coefficient for that reaction ([[Nernst equation]]).
 
where
 
Δ''G'' = change in Gibbs free energy, Δ''H'' = change in [[enthalpy]], ''T'' = absolute [[temperature]], Δ''S'' = change in [[entropy]], ''R'' = [[gas constant]], ln = [[natural logarithm]], Δ<sub>r</sub>''G'' = change of reaction in Gibbs free energy, Δ<sub>r</sub>''G°'' = standard change of reaction in Gibbs free energy, ''K'' = [[equilibrium constant]], ''Q<sub>r</sub>'' = [[reaction quotient]], ''n'' = number of [[electrons]] per [[Mole (unit)|mole]] product, ''F'' = [[Faraday constant]] ([[coulomb]]s per [[Mole (unit)|mole]]), and ''E'' = [[electrode potential]] of the reaction. Moreover, we also have:
 
:<math>K_{eq}=e^{- \frac{\Delta_r G^\circ}{RT}}</math>
:<math>\Delta_r G^\circ = -RT(\ln K_{eq}) = -2.303RT(\log_{10} K_{eq})</math>
 
which relates the equilibrium constant with Gibbs free energy.
 
==Gibbs free energy, the second law of thermodynamics, and metabolism==
A particular chemical reaction is said to proceed spontaneously if the hypothetical total change in entropy of the universe due to that reaction is greater than or equal to zero Joules per mole. As discussed in the Overview, under certain assumptions Gibbs free energy can be thought of as a negative proxy for the change in total entropy of the universe (it's negative because change in Gibbs free energy is negative when change in total entropy of the universe is positive, and visa versa). Thus, a reaction with a positive Gibbs free energy will not proceed spontaneously. However, in biological systems, energy inputs from other energy sources (including the sun and exothermic chemical reactions) are "coupled" with reactions that are not entropically favored (have a Gibbs free energy less than zero). Between two (or more) coupled reactions, total entropy in the universe always increases. This coupling allows an endergonic reactions, such as photosynthesis and DNA synthesis, to proceed without decreasing the total entropy of the universe. Thus biological systems do not violate the second law of thermodynamics
 
==Standard energy change of formation==
The [[Standard Gibbs function of formation|standard Gibbs free energy of formation]] of a compound is the change of Gibbs free energy that accompanies the formation of 1 [[mole (unit)|mole]] of that substance from its component elements, at their [[standard state]]s (the most stable form of the element at 25 degrees Celsius and 101.3 [[kilopascal]]s). Its symbol is Δ<sub>f</sub>''G''˚.
 
All elements in their standard states ([[oxygen]] gas, [[graphite]], etc.) have 0 standard Gibbs free energy change of formation, as there is no change involved.
 
:Δ<sub>r</sub>''G'' = Δ<sub>r</sub>''G''˚ + ''RT'' ln ''Q<sub>r</sub>''; ''Q<sub>r</sub>'' is the [[reaction quotient]].
At equilibrium, Δ<sub>r</sub>''G'' = 0 and ''Q<sub>r</sub>'' = ''K'' so the equation becomes Δ<sub>r</sub>''G''˚ = −''RT'' ln ''K''; ''K'' is the [[equilibrium constant]].
 
===Table of selected substances<ref>CRC Handbook of Chemistry and Physics, 2009, pp. 5-4 - 5-42, 90th ed., Lide</ref>===
{| class="wikitable sortable"
|-
! Substance
! State
! Δ<sub>f</sub>''G°''([[Joule (unit)|kJ]]/[[Mole (unit)|mol]])
! Δ<sub>f</sub>''G°''([[cal|kcal]]/[[Mole (unit)|mol]])
|-
| NO
| g
| 87.6
| 20.9
|-
| NO<sub>2</sub>
| g
| 51.3
| 12.3
|-
| N<sub>2</sub>O
| g
| 103.7
| 24.78
|-
| H<sub>2</sub>O
| g
| -228.6
| −54.64
|-
| H<sub>2</sub>O
| l
| -237.1
| −56.67
|-
| CO<sub>2</sub>
| g
| -394.4
| −94.26
|-
| CO
| g
| -137.2
| −32.79
|-
| CH<sub>4</sub>
| g
| -50.5
| −12.1
|-
| C<sub>2</sub>H<sub>6</sub>
| g
| -32.9
| −7.65
|-
| C<sub>3</sub>H<sub>8</sub>
| g
| -23.4
| −5.59
|-
| C<sub>6</sub>H<sub>6</sub>
| g
| 129.7
| 29.76
|-
| C<sub>6</sub>H<sub>6</sub>
| l
| 124.5
| 31.00
|}
 
==See also==
* [[Calphad]]
* [[Electron equivalent]]
* [[Enthalpy-entropy compensation]]
* [[Free entropy]]
* [[Grand potential]]
* [[Thermodynamic free energy]]
 
== References ==
{{reflist}}
 
==External links==
* [http://www.iupac.org/goldbook/G02629.pdf IUPAC definition (Gibbs energy)]
* [http://wine1.sb.fsu.edu/chm1046/notes/Thermody/Gibbs/Gibbs.htm Gibbs energy] - Florida State University
* [http://scienceworld.wolfram.com/physics/GibbsFreeEnergy.html Gibbs Free Energy] - Eric Weissteins World of Physics
* [http://2ndlaw.oxy.edu/gibbs.html Entropy and Gibbs Free Energy] - www.2ndlaw.oxy.edu
* [http://hyperphysics.phy-astr.gsu.edu/hbase/thermo/helmholtz.html#c2 Gibbs Free Energy] - Georgia State University
* [http://mc2.cchem.berkeley.edu/Java/Gibbs/Gibbs.html Gibbs Free Energy Java Applet] - University of California, Berkeley
* [http://xenon.che.ilstu.edu/genchemhelphomepage/topicreview/bp/ch21/gibbs.html#driving Gibbs Free Energy] - Illinois State University
* [http://www.composite-agency.com/product.htm Using Gibbs Free Energy for prediction of chemical driven material ageing]
 
{{DEFAULTSORT:Gibbs Free Energy}}
<!--Categories-->
[[Category:Concepts in physics]]
[[Category:State functions]]
[[Category:Thermodynamic free energy]]

Latest revision as of 20:55, 25 August 2014

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