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Gibbs Free Energy




In which measures the "useful" or process-initiating work obtainable from an Isothermal , Isobaric Thermodynamic System . Technically, the Gibbs free energy is the ''maximum'' amount of non-expansion work which can be extracted from a Closed System , and this maximum can be attained only in a completely Reversible Process . When a system changes from a well-defined initial state to a well-defined final state, the Gibbs free energy ''ΔG'' equals the work exchanged by the system with its surroundings, less the work of the pressure forces, during a reversible transformation of the system from the same initial state to the same final state.1.

Gibbs energy is also the chemical potential that is minimised when a system reaches equilibrium at constant pressure and temperature. As such, it is a convenient criterion of spontaineity for processes with constant pressure and temperature.

The Gibbs free energy, originally called ''available energy'', was developed in the 1870s by the American mathematical physicist Willard Gibbs . In 1873, in a foot-note, Gibbs defined what he called the “available energy” of a body as such:

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 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.


DEFINITIONS

’ 1873 available energy ( Free Energy ) graph, which shows a plane perpendicular to the axis of ''v'' ( Volume ) and passing through point A, which represents the initial state of the body. MN is the section of the surface of Dissipated Energy . Qε and Qη 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 = U+pV-TS \,

which is the same as:

:G = H-TS \,

where:
  • U is the s)

  • p is s)

  • V is Volume (SI Units: m3)

  • T is the s)

  • S is the Entropy (SI Units: joules per kelvin)

  • H is the Enthalpy (SI Units: joules)

  • The expression for the infinitesimal reversible change in the Gibbs free energy, for an Open System , subjected to the operation of external forces ''Xi'', which cause the external parameters of the system ''ai'' to change by an amount ''dai'', is given by:


  • \mu_i is the Chemical Potential of the ''i''-th chemical component. (SI Units: joules per particle Chemical Potential - IUPAC Gold Book or joules per mol)

  • N_i is the number of particles (or number of moles) composing the ''i''-th chemical component.


In the infinitesimal expression, the term involving the chemical potential accounts for changes in Gibbs free energy resulting from an influx of particles. In other words, it holds for an Open System only. 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 which shortens by an amount -''dl'' under a force ''f'' would result in a term ''fdl'' being added. If a quantity of energy -''de'' is acquired by a system at an electrical potential Ψ, the electrical work associated with this is -Ψ''de'', which would be included in the infinitesimal expression. Other work terms are added on per system requirements.2

Each quantity in the equations above can be divided by the amount of substance, measured in 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:

: rac{G}{N} = rac{G}{N}^\circ + kT\ln rac{p}

if the volume is known rather than pressure then it becomes:

: rac{G}{N} = rac{G}{N}^\circ + kT\ln rac{V^\circ}

or more conveniently as its Chemical Potential :

: rac{G}{N} = \mu = \mu^\circ + RT\ln rac{p}

In non-ideal systems, Fugacity comes into play.


OVERVIEW

In a simple manner, with respect to STP reacting systems, a general Rule Of Thumb is:

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 ΔG is negative. Essentially, this means that such a reaction will be favored and will release energy. The energy released equals the maximum amount of work that can be performed as a result of the chemical reaction. Conversely, if conditions indicated a positive ΔG, then energy--in the form of work--would have to be added to the reacting system to make the reaction go.


HISTORY

The quantity called "free energy" is essentially 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. The term affinity, as used in chemical relation, dates back to at least the time of Albertus Magnus in 1250.

From the 1998 textbook ''Modern Thermodynamics'' by Nobel Laureate and chemical engineering professor Ilya Prigogine we find: "As motion was explained by the Newtonian concept of force, chemists wanted a similar concept of ‘driving force’ for chemical change? Why do chemical reactions occur, and why do they stop at certain points? Chemists called the ‘force’ that caused chemical reactions affinity, but it lacked a clear definition."

During the entire 18th century, the dominant view in regards to heat and light was that put forward by Isaac Newton , called the “Newtonian hypothesis”, which stated that light and heat are forms of matter attracted or repelled by other forms of matter, with forces analogous to gravitation or to chemical affinity.

In the 19th century, the French chemist Marcellin Berthelot and the Danish chemist Julius Thomsen had attempted to quantify affinity using Heats Of Reaction . In 1875, after quantifying the heats of reaction for a large number of compounds, Berthelot proposed the “ Principle Of Maximum Work ” in which all chemical changes occurring without intervention of outside energy tend toward the production of bodies or of a system of bodies which liberate Heat .

In addition to this, in 1780 Antoine Lavoisier and Pierre-Simon Laplace laid the foundations of Thermochemistry by showing that the heat given out in a reaction is equal to the heat absorbed in the reverse reaction. They also investigated the Specific Heat and Latent Heat of a number of substances, and amounts of heat given out in combustion. Similarly, in 1840 Swiss chemist Germain Hess formulated the principle that the evolution of heat in a reaction is the same whether the process is accomplished in one-step or in a number of stages. This is known as Hess' Law . With the advent of the Mechanical Theory Of Heat in the early 19th century, Hess’s law came to be viewed as a consequence of the law of Conservation Of Energy .

Based on these and other ideas, Berthelot and Danish chemist Julius Thomsen , as well as others, considered the heat given out in the formation of a compound as a measure of the affinity, or the work done by the chemical forces. This view, however, was not entirely correct. In 1847, the English physicist James Joule showed that he could raise the temperature of water by turning a paddle wheel in it, thus showing that heat and mechanical work were equivalent or proportional to each other, i.e. approximately, dW \propto dQ. This statement came to be known as the Mechanical Equivalent Of Heat and was a precursory form of the First Law Of Thermodynamics .

By 1865 the German physicist Rudolf Clausius had shown that this equivalence principle needed amendment. That is, one can use the heat derived from a Combustion Reaction in a coal furnace to boil water, and use this heat to vaporize steam, and then use the enhanced high pressure energy of the vaporized steam to push a piston. Thus, we might naively reason that one can entirely convert the initial combustion heat of the chemical reaction into the work of pushing the piston. Clausius showed, however, that we need to take into account the work that the molecules of the working body, i.e. the water molecules in the cylinder, do on each other as they pass or transform from one step of or State of the Engine Cycle to the next, e.g. from (P1,V1) to (P2,V2). Clausius originally called this the “transformation content” of the body, and then later changed the name to Entropy . Thus, the heat used to transform the working body of molecules from one state to the next cannot be used to do external work, e.g. to push the piston. Clausius defined this ''transformation heat'' as ''dQ = TdS''.

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 - 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 will ensue. In 1876, Gibbs built on this framework by introducing the concept of Chemical Potential so to take into account chemical reactions and states of bodies which are chemically different from each other. In his own words, to summarize his results in 1873, Gibbs states:

In this description, as used by Gibbs, ''ε'' refers to the Internal Energy of the body, ''η'' refers to the Entropy of the body, and ''ν'' is the Volume of the body.

Hence, in 1882, after the introduction of these arguments by Clausius and Gibbs, the German scientist Hermann Von Helmholtz stated, in opposition to Berthelot and Thomas’ hypothesis that chemical affinity is a measure of the heat of reaction of chemical reaction as based on the principle of maximal work, that affinity is not the heat given out in the formation of a compound but rather it 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.

Up 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 Reactions'' 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.


WHAT DOES THE TERM ‘FREE’ MEAN?

In the 18th and 19th centuries, the Theory Of Heat , i.e. that heat is a form of energy having relation to vibratory motion, was beginning to supplant both the Caloric Theory , i.e. that heat is a fluid, and the Four Element Theory in which heat was the lightest of the four elements. Many textbooks and teaching articles during these centuries presented these theories side by side. Similarly, during these years, Heat was beginning to be distinguished into different classification categories, such as “free heat”, “combined heat”, “radiant heat”, Specific Heat , Heat Capacity , “absolute heat”, “latent caloric”, “free” or “perceptible” caloric (''calorique sensible''), among others.

In 1780, for example, , loss of vis viva, and increase of vis viva.’” In this manner, the total mass of caloric in a body, called ''absolute heat'', was regarded as a mixture of two components; the free or perceptible caloric could affect a thermometer while the other component, the latent caloric, could not. 3 The use of the words “latent heat” implied a similarity to latent heat in the more usual sense; it was regarded as chemically bound to the molecules of the body. In the Adiabatic Compression of a gas the absolute heat remained constant by the observed rise of temperature, indicating that some latent caloric had become “free” or perceptible.

During the early 19th century, the concept of perceptible or free caloric began to be referred to as “free heat” or heat set free. In 1824, for example, the French physicist Sadi Carnot , in his famous “Reflections on the Motive Power of Fire”, speaks of quantities of heat ‘absorbed or set free’ in different transformations. In 1882, the German physicist and physiologist Hermann Von Helmholtz coined the phrase ‘free energy’ for the expression ''E – TS'', in which the change in F (or G) determines the amount of Energy ‘free’ for Work under the given conditions. 4

Thus, in traditional use, the term “free” was attached to Gibbs free energy, i.e. for systems at constant pressure and temperature, or to Helmholtz free energy, i.e. for systems at constant volume and temperature, to mean ‘available in the form of useful work.’ With reference to the Gibbs free energy, we add the qualification that it is the energy free for non-volume work.5

:\Delta G^\circ = -RT(\ln K_{eq}) = -2.303RT(\log K_{eq})

which relates the equilibrium constant with Gibbs free energy.


STANDARD CHANGE OF FORMATION

The standard Gibbs free energy of formation of a compound is the change of Gibbs free energy that accompanies the formation of 1 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 100 Kilopascal s). Its symbol is Δ''G''fO.

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''G'' = Δ''G''˚ + ''RT'' ln ''Q''
At equilibrium, Δ''G''=0 and ''Q'' = ''K'' so the equation becomes Δ''G''˚= −''RT'' ln ''K''


WHAT IS LIFE?

See Also: Entropy and life


To a good approximation, one of the most oft-quoted references in , which Schrödinger equates with death, by feeding on Negative Entropy . Specifically, according to Schrödinger, an organism avoids decay by eating, drinking, breathing, and in the case of plants assimilating, a process called Metabolism .

In the past, Schrödinger states, this process would have been considered an exchange of matter or energy, such that organisms stay alive by exchanging energy. He uses the example of how caloric values are printed in certain menus in the United States or Germany, but states that these caloric energy exchange values are useless in trying to quantify life. He then asks “what then is that precious something contained in our food which keeps us from death?” The answer, according to Schrödinger, is that because according the Second Law Of Thermodynamics an organism continually produces “positive entropy” it must continually draw in “negative entropy” from its environment to stay alive. Or, specifically “the essential thing in metabolism is that the organism succeeds in freeing itself from all the entropy it cannot help producing while alive.”

These suppositions, because they were intended for a lay audience, however, met with great opposition in the physics community. In later editions of his book, Schrödinger attached a note to chapter six explaining his use of the term “negative entropy”. He states “the remarks on ''negative entropy'' have met with doubt and opposition from physicist colleagues. Let me say first, that if I had been catering for them alone I should have let the discussion turn on free energy instead. It is the more familiar notion in this context. But this highly technical term seemed too linguistically near to ''energy'' for making the average reader alive to the contrast between the two things.”


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