Enthalpy
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Categories: Articles needing additional references from February 2008 | Thermodynamics | Enthalpy | Fundamental physics concepts
In thermodynamics and molecular chemistry, the enthalpy or heat content (denoted as H, 'h', or rarely as χ) is a quotient or description of thermodynamic potential of a system, which can be used to calculate the "useful" work obtainable from a closed thermodynamic system under constant pressure. The term enthalpy is composed of the prefix en-, meaning to "put into" and the Greek word -thalpein, meaning "to heat", although the original definition is thought to have stemmed from the word, "enthalpos" (ἐνθάλπος).[1] It is often calculated as a differential sum, describing the changes within exo- and endothermic reactions, which minimize at equilibrium.
HistoryOver the history of thermodynamics, several terms have been used to denote what is now known as the enthalpy of a system. Originally, it was thought that the word "enthalpy" was created by Benoit Paul Émile Clapeyron and Rudolf Clausius through the publishing of the Clausius-Clapeyron relation in "The Mollier Steam Tables and Diagrams" in 1827, but it was later published that the earliest recording of the word was in 1875, by Josiah Willard Gibbs in the publication "Physical Chemistry: an Advanced Treatise"[2], although it is not referenced in Gibbs' works directly[3]. In 1909, Keith Landler discussed Gibbs' work on the 'heat function for constant pressure' and noted that Heike Kamerlingh Onnes had coined its modern name from the Greek word "enthalpos" (ενθαλπος) meaning "to put heat into." [1] Original definitionThis is the heat change which occurs when 1 mol of a substance reacts completely with oxygen to form products at 298 K and 1 atm. The function H was introduced by the Dutch physicist Heike Kamerlingh Onnes in early 20th century in the following form:
where (all units given in SI)
Application and extended formulaOverviewIn terms of thermodynamics, enthalpy can be calculated by determining the requirements for creating a system from "nothingness"; the mechanical work required, Failed to parse (Missing texvc executable; please see math/README to configure.): pV differs, based upon the constancy of conditions present at the creation of the thermodynamic system. Internal energy, Failed to parse (Missing texvc executable; please see math/README to configure.): U , must be supplied to remove particles from a surrounding in order to allow space for the creation of a system, providing that environmental variables, such as pressure (Failed to parse (Missing texvc executable; please see math/README to configure.): p ) remain constant. This internal energy also includes the energy required for activation and the breaking of bonded compounds into gaseous species. This process is calculated within enthalpy calculations as Failed to parse (Missing texvc executable; please see math/README to configure.): U + pV , to label the amount of energy or work required to "set aside space for" and "create" the system; describing the work done by both the reaction or formation of systems, and the surroundings. For systems at constant pressure, the change in enthalpy is the heat received by the system plus the non-mechanical work that has been done. Therefore, the change in enthalpy can be devised or represented without the need for compressive or expansive mechanics; for a simple system, with a constant number of particles, the difference in enthalpy is the maximum amount of thermal energy derivable from a thermodynamic process in which the pressure is held constant. The term Failed to parse (Missing texvc executable; please see math/README to configure.): p Failed to parse (Missing texvc executable; please see math/README to configure.): V is the work required to displace the surrounding atmosphere in order to vacate the space to be occupied by the system. RelationshipsAs an expansion of the first law of thermodynamics, enthalpy can be related to several other thermodynamic formulae. As with the original definition of the first law;
represents the infinitesimal increase of the systematic or internal energy.
represents the infinitesimal amount of energy attributed or added to the system.
represents the infinitesimal amount of energy acted out by the system on the surroundings. As a differentiating expression, the value of H can be defined as
Where
For a process that is not reversible, the second law of thermodynamics states that the increase in heat Failed to parse (Missing texvc executable; please see math/README to configure.): \delta Q
is less than or equal to the product Failed to parse (Missing texvc executable; please see math/README to configure.): T\mathrm{d}S
of temperature Failed to parse (Missing texvc executable; please see math/README to configure.): T
and the increase in entropy Failed to parse (Missing texvc executable; please see math/README to configure.): \mathrm{d}S
is zero and thus
over any isobar in state space is the maximum thermal energy attainable from the system. If, in addition, the entropy is held constant as well, i.e., Failed to parse (Missing texvc executable; please see math/README to configure.): \mathrm{d}S = 0 , the above equation becomes:
In a more general form, the first law describes the internal energy with additional terms involving the chemical potential and the number of particles of various types. The differential statement for Failed to parse (Missing texvc executable; please see math/README to configure.): \mathrm{d}H is then:
is the chemical potential for an i-type particle, and Failed to parse (Missing texvc executable; please see math/README to configure.): N_i
is the number of such particles. It is seen that, not only must the Failed to parse (Missing texvc executable; please see math/README to configure.): V\mathrm{d}p
term be set to zero by requiring the pressures of the initial and final states to be the same, but the Failed to parse (Missing texvc executable; please see math/README to configure.): \mu_i \mathrm{d}N_i terms must be zero as well, by requiring that the particle numbers remain unchanged. Any further generalization will add even more terms whose extensive differential term must be set to zero in order for the interpretation of the enthalpy to hold. Heats of reactionThe total enthalpy of a system cannot be measured directly; the enthalpy change of a system is measured instead. Enthalpy change is defined by the following equation:
For an exothermic reaction at constant pressure, the system's change in enthalpy is equal to the energy released in the reaction, including the energy retained in the system and lost through expansion against its surroundings. In a similar manner, for an endothermic reaction, the system's change in enthalpy is equal to the energy absorbed in the reaction, including the energy lost by the system and gained from compression from its surroundings. A relatively easy way to determine whether or not a reaction is exothermic or endothermic is to determine the sign of ΔH. If ΔH is positive, the reaction is endothermic, that is heat is absorbed by the system due to the products of the reaction having a greater enthalpy than the reactants. On the other hand if ΔH is negative, the reaction is exothermic, that is the overall decrease in enthalpy is achieved by the generation of heat. Although enthalpy is commonly used in engineering and science, it is impossible to measure directly, as enthalpy has no datum (reference point). Therefore enthalpy can only accurately be used in a closed system. However, few real world applications exist in closed isolation, and it is for this reason that two or more closed systems cannot be compared using enthalpy as a basis, although sometimes this is done erroneously. Open systemsIn thermodynamic open systems, matter may flow in and out of the system boundaries. The first law of thermodynamics for open systems states: the increase in the internal energy of a system is equal to the amount of energy added to the system by matter flowing in and by heating, minus the amount lost by matter flowing out and in the form of work done by the system. The first law for open systems is given by:
Image:First law open system.png
During steady, continuous operation, an energy balance applied to an open system equates shaft work performed by the system to heat added plus net enthalpy added.
The region of space enclosed by open system boundaries is usually called a control volume, and it may or may not correspond to physical walls. If we choose the shape of the control volume such that all flow in or out occurs perpendicular to its surface, then the flow of matter into the system performs work as if it were a piston of fluid pushing mass into the system, and the system performs work on the flow of matter out as if it were driving a piston of fluid. There are then two types of work performed: flow work described above which is performed on the fluid (this is also often called Failed to parse (Missing texvc executable; please see math/README to configure.): pV work) and shaft work which may be performed on some mechanical device. These two types of work are expressed in the equation:
work in fluids for open systems:
Standard enthalpy changesDefinitionsStandard enthalpy change of combustion
Standard enthalpy change of hydrogenation
Standard enthalpy change of formation
Standard enthalpy change of reaction
A common standard enthalpy change is the standard enthalpy change of formation, which has been determined for a vast number of substances. The enthalpy change of any reaction under any conditions can be computed, given the standard enthalpy change of formation of all of the reactants and products. Other types of standard enthalpy change include combustion (standard enthalpy change of combustion), neutralisation (standard enthalpy change of neutralisation), melting/freezing (standard enthalpy change of fusion), vaporisation/condensation (standard enthalpy change of vaporisation), atomisation (standard enthalpy change of atomisation), mixing (standard enthalpy change of mixing), dissolution (standard enthalpy change of solution), and denaturation (standard enthalpy change of denaturation). Examples: Inorganic compounds (at 25 °C)
Specific enthalpyThe specific enthalpy of a working mass is a property of that mass used in thermodynamics, defined as Failed to parse (Missing texvc executable; please see math/README to configure.): h=u+p \cdot v where u is the specific internal energy, p is the pressure, and v is specific volume. In other words, Failed to parse (Missing texvc executable; please see math/README to configure.): h = H/m where Failed to parse (Missing texvc executable; please see math/README to configure.): m is the mass of the system. The SI unit for specific enthalpy is joules per kilogram. Notes
References
See also
External links
ast:Entalpía bs:Entalpija bg:Енталпия ca:Entalpia cs:Entalpie da:Entalpi de:Enthalpie el:Ενθαλπία es:Entalpía eo:Entalpio fr:Enthalpie gl:Entalpía ko:엔탈피 hr:Entalpija id:Entalpi it:Entalpia he:אנתלפיה hu:Entalpia mk:Енталпија ms:Entalpi nl:Enthalpie ja:エンタルピー no:Entalpi nn:Entalpi pl:Entalpia pt:Entalpia ro:Entalpie ru:Энтальпия sk:Entalpia sl:Entalpija fi:Entalpia sv:Entalpi vi:Enthalpy tr:Entalpi uk:Ентальпія vec:Entalpìa |


