Internal energy
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In thermodynamics, the internal energy of a system is the energy contained within the system. It is the energy necessary to create or prepare the system in any given state, but does not include the kinetic energy of motion of the system as a whole, nor the potential energy of the system as a whole due to external force fields which includes the energy of displacement of the system's surroundings. It keeps account of the gains and losses of energy of the system that are due to changes in its internal state.^{[1]}^{[2]}
Internal energy  

Common symbols  U 
SI unit  J 
In SI base units  m^{2}*kg/s^{2} 
Derivations from other quantities 
The internal energy of a system can be increased by introduction of matter or by heat, or reduced when thermodynamic work is done by the system.^{[3]} When matter transfer is prevented by impermeable containing walls, the system is said to be closed and the first law of thermodynamics defines the change in internal energy as the difference between the energy added to the system as heat and the thermodynamic work done by the system on its surroundings. If the containing walls pass neither matter nor energy, the system is said to be isolated and its internal energy cannot change.
The internal energy of a given state of a system cannot be directly measured and knowledge of all components is rarely interesting. Thermodynamics is chiefly concerned only with changes in the internal energy, not with its absolute value. Changes, relative to a reference state, are determined from convenient chains of thermodynamic operations and thermodynamic processes by which a given state can be prepared. Such a process can be described by certain extensive state variables of the system, for example, entropy, mole numbers, or electric dipole moment. For practical considerations in thermodynamics and engineering it is rarely necessary or convenient to consider all energies belonging to the total intrinsic energy of a system, such as the energy given by the equivalence of mass. Customarily, thermodynamic descriptions include only items relevant to the processes under study.
The internal energy is one of the two cardinal state functions of the state variables, and its value depends only on the current state of the system and not on the processes undergone to prepare it. It is an extensive quantity. It is the one and only cardinal thermodynamic potential.^{[4]} All other thermodynamic potentials are formulated from the internal energy. In practical considerations in thermodynamics it is rarely necessary, nor convenient, to consider all intrinsic energies of a system, such as the energy given by the massenergy equivalence. Conveniently, it can be explained in microscopic terms by the random kinetic energy due to the microscopic motion of the system's particles from translations, rotations, and vibrations, and by the potential energy associated with microscopic forces, including chemical bonds. For study of thermonuclear reactions, the static rest mass energy of the constituents of matter are important.
The unit of energy in the International System of Units (SI) is the joule (J). Sometimes it is convenient to use a corresponding intensive energy density, called specific internal energy, which is either relative to the mass of the system, with the unit J/kg, or relative to the amount of substance with unit J/mol (molar internal energy).
Cardinal functionsEdit
The internal energy, U(S,V,{N_{j}}), expresses the thermodynamics of a system in the energylanguage, or in the energy representation. As a function of state, its arguments are exclusively extensive variables of state. Alongside the internal energy, the other cardinal function of state of a thermodynamic system is its entropy, as a function, S(U,V,{N_{j}}), of the same list of extensive variables of state, except that the entropy, S, is replaced in the list by the internal energy, U. It expresses the entropy representation.^{[4]}^{[5]}^{[6]}
Each cardinal function is a monotonic function of each of its natural or canonical variables. Each provides its characteristic or fundamental equation, for example U = U(S,V,{N_{j}}), that by itself contains all thermodynamic information about the system. The fundamental equations for the two cardinal functions can in principle be interconverted by solving, for example, U = U(S,V,{N_{j}}) for S, to get S = S(U,V,{N_{j}}).
In contrast, Legendre transforms are necessary to derive fundamental equations for other thermodynamic potentials and Massieu functions. The entropy as a function only of extensive state variables is the one and only cardinal function of state for the generation of Massieu functions. It is not itself customarily designated a 'Massieu function', though rationally it might be thought of as such, corresponding to the term 'thermodynamic potential', which includes the internal energy.^{[5]}^{[7]}^{[8]}
For real and practical systems, explicit expressions of the fundamental equations are almost always unavailable, but the functional relations exist in principle. Formal, in principle, manipulations of them are valuable for the understanding of thermodynamics.
Description and definitionEdit
The internal energy U of a given state of the system is determined relative to that of a standard state of the system, by adding up the macroscopic transfers of energy that accompany a change of state from the reference state to the given state:
where ΔU denotes the difference between the internal energy of the given state and that of the reference state, and the E_{i} are the various energies transferred to the system in the steps from the reference state to the given state. It is the energy needed to create the given state of the system from the reference state.
From a nonrelativistic microscopic point of view, it may be divided into microscopic potential energy, U_{micro pot}, and microscopic kinetic energy, U_{micro kin}, components:
The microscopic kinetic energy of a system arises as the sum of the motions of all the system's particles with respect to the centerofmass frame, whether it be the motion of atoms, molecules, atomic nuclei, electrons, or other particles. The microscopic potential energy algebraic summative components are those of the chemical and nuclear particle bonds, and the physical force fields within the system, such as due to internal induced electric or magnetic dipole moment, as well as the energy of deformation of solids (stressstrain). Usually, the split into microscopic kinetic and potential energies is outside the scope of macroscopic thermodynamics.
Internal energy does not include the energy due to motion or location of a system as a whole. That is to say, it excludes any kinetic or potential energy the body may have because of its motion or location in external gravitational, electrostatic, or electromagnetic fields. It does, however, include the contribution of such a field to the energy due to the coupling of the internal degrees of freedom of the object with the field. In such a case, the field is included in the thermodynamic description of the object in the form of an additional external parameter.
For practical considerations in thermodynamics or engineering, it is rarely necessary, convenient, nor even possible, to consider all energies belonging to the total intrinsic energy of a sample system, such as the energy given by the equivalence of mass. Typically, descriptions only include components relevant to the system under study. Indeed, in most systems under consideration, especially through thermodynamics, it is impossible to calculate the total internal energy.^{[9]} Therefore, a convenient null reference point may be chosen for the internal energy.
The internal energy is an extensive property: it depends on the size of the system, or on the amount of substance it contains.
At any temperature greater than absolute zero, microscopic potential energy and kinetic energy are constantly converted into one another, but the sum remains constant in an isolated system (cf. table). In the classical picture of thermodynamics, kinetic energy vanishes at zero temperature and the internal energy is purely potential energy. However, quantum mechanics has demonstrated that even at zero temperature particles maintain a residual energy of motion, the zero point energy. A system at absolute zero is merely in its quantummechanical ground state, the lowest energy state available. At absolute zero a system of given composition has attained its minimum attainable entropy.
The microscopic kinetic energy portion of the internal energy gives rise to the temperature of the system. Statistical mechanics relates the pseudorandom kinetic energy of individual particles to the mean kinetic energy of the entire ensemble of particles comprising a system. Furthermore, it relates the mean microscopic kinetic energy to the macroscopically observed empirical property that is expressed as temperature of the system. While temperature is an intensive measure, this energy expresses the concept as an extensive property of the system, often referred to as the thermal energy,^{[10]}^{[11]} The scaling property between temperature and thermal energy is the entropy change of the system.
Statistical mechanics considers any system to be statistically distributed across an ensemble of N microstates. In a system that is in thermodynamic contact equilibrium with a heat reservoir, each microstate has an energy E_{i} and is associated with a probability p_{i}. The internal energy is the mean value of the system's total energy, i.e., the sum of all microstate energies, each weighted by its probability of occurrence:
This is the statistical expression of the law of conservation of energy.
Internal energy changesEdit

Thermodynamics is chiefly concerned only with the changes, ΔU, in internal energy.
For a closed system, with matter transfer excluded, the changes in internal energy are due to heat transfer Q and due to work. The latter can be split into two kinds, pressurevolume work W_{pressurevolume}, and frictional and other kinds, such as electrical polarization, which do not alter the volume of the system, and are called isochoric, W_{isochoric}. Accordingly, the internal energy change ΔU for a process may be written^{[3]}
 ^{[note 1]}
When a closed system receives energy as heat, this energy increases the internal energy. It is distributed between microscopic kinetic and microscopic potential energies. In general, thermodynamics does not trace this distribution. In an ideal gas all of the extra energy results in a temperature increase, as it is stored solely as microscopic kinetic energy; such heating is said to be sensible.
A second mechanism of change of internal energy of a closed system is the doing of work on the system, either in mechanical form by changing pressure or volume, or by other perturbations, such as directing an electric current through the system.
If the system is not closed, the third mechanism that can increase the internal energy is transfer of matter into the system. This increase, ΔU_{matter} cannot be split into heat and work components. If the system is so set up physically that heat and work can be done on it by pathways separate from and independent of matter transfer, then the transfers of energy add to change the internal energy:
If a system undergoes certain phase transformations while being heated, such as melting and vaporization, it may be observed that the temperature of the system does not change until the entire sample has completed the transformation. The energy introduced into the system while the temperature did not change is called a latent energy, or latent heat, in contrast to sensible heat, which is associated with temperature change.
Internal energy of the ideal gasEdit
Thermodynamics often uses the concept of the ideal gas for teaching purposes, and as an approximation for working systems. The ideal gas is a gas of particles considered as point objects that interact only by elastic collisions and fill a volume such that their free mean path between collisions is much larger than their diameter. Such systems approximate the monatomic gases, helium and the other noble gases. Here the kinetic energy consists only of the translational energy of the individual atoms. Monatomic particles do not rotate or vibrate, and are not electronically excited to higher energies except at very high temperatures.
Therefore, internal energy changes in an ideal gas may be described solely by changes in its kinetic energy. Kinetic energy is simply the internal energy of the perfect gas and depends entirely on its pressure, volume and thermodynamic temperature.
The internal energy of an ideal gas is proportional to its mass (number of moles) n and to its temperature T
where c is the molar heat capacity (at constant volume) of the gas. The internal energy may be written as a function of the three extensive properties S, V, n (entropy, volume, mass) in the following way ^{[12]}^{[13]}
where const is an arbitrary positive constant and where R is the universal gas constant. It is easily seen that U is a linearly homogeneous function of the three variables (that is, it is extensive in these variables), and that it is weakly convex. Knowing temperature and pressure to be the derivatives the ideal gas law immediately follows.
Internal energy of a closed thermodynamic systemEdit
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The above summation of all components of change in internal energy assumes that a positive energy denotes heat added to the system or work done on the system, while a negative energy denotes work of the system on the environment.
Typically this relationship is expressed in infinitesimal terms using the differentials of each term. Only the internal energy is an exact differential. For a system undergoing only thermodynamics processes, i.e. a closed system that can exchange only heat and work, the change in the internal energy is
which constitutes the first law of thermodynamics.^{[note 1]} It may be expressed in terms of other thermodynamic parameters. Each term is composed of an intensive variable (a generalized force) and its conjugate infinitesimal extensive variable (a generalized displacement).
For example, for a nonviscous fluid, the mechanical work done on the system may be related to the pressure p and volume V. The pressure is the intensive generalized force, while the volume is the extensive generalized displacement:
 .
This defines the direction of work, W, to be energy flow from the working system to the surroundings, indicated by a negative term.^{[note 1]} Taking the direction of heat transfer Q to be into the working fluid and assuming a reversible process, the heat is
 .
 is temperature
 is entropy
and the change in internal energy becomes
Changes due to temperature and volumeEdit
The expression relating changes in internal energy to changes in temperature and volume is
This is useful if the equation of state is known.
In case of an ideal gas, we can derive that , i.e. the internal energy of an ideal gas can be written as a function that depends only on the temperature.
The expression relating changes in internal energy to changes in temperature and volume is
The equation of state is the ideal gas law
Solve for pressure:
Substitute in to internal energy expression:
Take the derivative of pressure with respect to temperature:
Replace:
And simplify:
To express dU in terms of dT and dV, the term
is substituted in the fundamental thermodynamic relation
This gives:
The term is the heat capacity at constant volume
The partial derivative of S with respect to V can be evaluated if the equation of state is known. From the fundamental thermodynamic relation, it follows that the differential of the Helmholtz free energy A is given by:
The symmetry of second derivatives of A with respect to T and V yields the Maxwell relation:
This gives the expression above.
Changes due to temperature and pressureEdit
When considering fluids or solids, an expression in terms of the temperature and pressure is usually more useful:
where it is assumed that the heat capacity at constant pressure is related to the heat capacity at constant volume according to:
The partial derivative of the pressure with respect to temperature at constant volume can be expressed in terms of the coefficient of thermal expansion
and the isothermal compressibility
by writing:
and equating dV to zero and solving for the ratio dp/dT. This gives:
Substituting (2) and (3) in (1) gives the above expression.
Changes due to volume at constant temperatureEdit
The internal pressure is defined as a partial derivative of the internal energy with respect to the volume at constant temperature:
Consistency with statistical definitionEdit
Differentiating^{[clarification needed]} yields:
The two terms are identified as and , respectively,^{[14]} providing the first law of thermodynamics.
Internal energy of multicomponent systemsEdit
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In addition to including the entropy S and volume V terms in the internal energy, a system is often described also in terms of the number of particles or chemical species it contains:
where N_{j} are the molar amounts of constituents of type j in the system. The internal energy is an extensive function of the extensive variables S, V, and the amounts N_{j}, the internal energy may be written as a linearly homogeneous function of first degree:
where α is a factor describing the growth of the system. The differential internal energy may be written as
which shows (or defines) temperature T to be the partial derivative of U with respect to entropy S and pressure p to be the negative of the similar derivative with respect to volume V
and where the coefficients are the chemical potentials for the components of type i in the system. The chemical potentials are defined as the partial derivatives of the energy with respect to the variations in composition:
As conjugate variables to the composition , the chemical potentials are intensive properties, intrinsically characteristic of the qualitative nature of the system, and not proportional to its extent. Under conditions of constant T and p, because of the extensive nature of U and its independent variables, using Euler's homogeneous function theorem, the differential dU may be integrated and yields an expression for the internal energy:
 .
The sum over the composition of the system is the Gibbs free energy:
that arises from changing the composition of the system at constant temperature and pressure. For a single component system, the chemical potential equals the Gibbs energy per amount of substance, i.e. particles or moles according to the original definition of the unit for .
Internal energy in an elastic mediumEdit
For an elastic medium the mechanical energy term of the internal energy is expressed in terms of the stress and strain involved in elastic processes. In Einstein notation for tensors, with summation over repeated indices, the infinitesimal statement is
Euler's theorem yields for the internal energy:^{[15]}
For a linearly elastic material, the stress is related to the strain by:
where the C_{ijkl} are the components of the 4thrank elastic constant tensor of the medium.
Elastic deformations, such as sound, passing through a body, or other forms of macroscopic internal agitation or turbulent motion create states when the system is not in thermodynamic equilibrium. While such energies of motion continue, they contribute to the total energy of the system; thermodynamic internal energy pertains only when such motions have ceased.
HistoryEdit
James Joule studied the relationship between heat, work, and temperature. He observed that friction in a liquid, such as caused by its agitation with work by a paddle wheel, caused an increase in its temperature, which he described as producing a quantity of heat. Expressed in modern units, he found that c. 4186 joules of energy were needed to raise the temperature of one kilogram of water by one degree Celsius.^{[16]}
NotesEdit
 ^ ^{a} ^{b} ^{c} This article uses the sign convention of the mechanical work as typically defined in chemistry, which is different from the convention used in physics. In chemistry, work performed by the system against the environment, e.g., a system expansion, is negative, while in physics this is taken to be positive.
See alsoEdit
ReferencesEdit
 ^ Crawford, F. H. (1963), pp. 106–107.
 ^ Haase, R. (1971), pp. 24–28.
 ^ ^{a} ^{b} Born, M. (1949), Appendix 8, pp. 146–149.
 ^ ^{a} ^{b} Tschoegl, N.W. (2000), p. 17.
 ^ ^{a} ^{b} Callen, H.B. (1960/1985), Chapter 5.
 ^ Münster, A. (1970), p. 6.
 ^ Münster, A. (1970), Chapter 3.
 ^ Bailyn, M. (1994), pp. 206–209.
 ^ I. Klotz, R. Rosenberg, Chemical Thermodynamics  Basic Concepts and Methods, 7th ed., Wiley (2008), p.39
 ^ Leland, T.W. Jr., Mansoori, G.A., pp. 15, 16.
 ^ Thermal energy – Hyperphysics
 ^ van Gool, W.; Bruggink, J.J.C. (Eds) (1985). Energy and time in the economic and physical sciences. NorthHolland. pp. 41–56. ISBN 9780444877482.CS1 maint: extra text: authors list (link)
 ^ Grubbström, Robert W. (2007). "An Attempt to Introduce Dynamics Into Generalised Exergy Considerations". Applied Energy. 84 (7–8): 701–718. doi:10.1016/j.apenergy.2007.01.003.
 ^ Roger, Bowley (2011) [1999]. Introductory statistical mechanics. Clarendon Press. ISBN 9780198505754. OCLC 969703928.
 ^ Landau & Lifshitz 1986
 ^ Joule, J.P. (1850). "On the Mechanical Equivalent of Heat". Philosophical Transactions of the Royal Society. 140: 61–82. doi:10.1098/rstl.1850.0004.
Bibliography of cited referencesEdit
 Adkins, C.J. (1968/1975). Equilibrium Thermodynamics, second edition, McGrawHill, London, ISBN 0070840571.
 Bailyn, M. (1994). A Survey of Thermodynamics, American Institute of Physics Press, New York, ISBN 0883187973.
 Born, M. (1949). Natural Philosophy of Cause and Chance, Oxford University Press, London.
 Callen, H.B. (1960/1985), Thermodynamics and an Introduction to Thermostatistics, (first edition 1960), second edition 1985, John Wiley & Sons, New York, ISBN 0471862568.
 Crawford, F. H. (1963). Heat, Thermodynamics, and Statistical Physics, Rupert HartDavis, London, Harcourt, Brace & World, Inc.
 Haase, R. (1971). Survey of Fundamental Laws, chapter 1 of Thermodynamics, pages 1–97 of volume 1, ed. W. Jost, of Physical Chemistry. An Advanced Treatise, ed. H. Eyring, D. Henderson, W. Jost, Academic Press, New York, lcn 73–117081.
 Thomas W. Leland, Jr., G. A. Mansoori (ed.), Basic Principles of Classical and Statistical Thermodynamics (PDF)
 Landau, L. D.; Lifshitz, E. M. (1986). Theory of Elasticity (Course of Theoretical Physics Volume 7). (Translated from Russian by J.B. Sykes and W.H. Reid) (Third ed.). Boston, MA: Butterworth Heinemann. ISBN 9780750626330.CS1 maint: ref=harv (link)
 Münster, A. (1970), Classical Thermodynamics, translated by E.S. Halberstadt, Wiley–Interscience, London, ISBN 0471624306.
 Planck, M., (1923/1927). Treatise on Thermodynamics, translated by A. Ogg, third English edition, Longmans, Green and Co., London.
 Tschoegl, N.W. (2000). Fundamentals of Equilibrium and SteadyState Thermodynamics, Elsevier, Amsterdam, ISBN 0444504265.
BibliographyEdit
 Alberty, R. A. (2001). "Use of Legendre transforms in chemical thermodynamics" (PDF). Pure Appl. Chem. 73 (8): 1349–1380. doi:10.1351/pac200173081349.
 Lewis, Gilbert Newton; Randall, Merle: Revised by Pitzer, Kenneth S. & Brewer, Leo (1961). Thermodynamics (2nd ed.). New York, NY USA: McGrawHill Book Co. ISBN 9780071138093.CS1 maint: multiple names: authors list (link)