Thermodynamics
From Wikipedia, the free encyclopedia.
Thermodynamics (Greek: thermos = heat and dynamic = change) is the physics of energy, heat, work, entropy and the spontaneity of processes. Thermodynamics is closely related to statistical mechanics from which many thermodynamic relationships can be derived.
While dealing with processes in which systems exchange matter or energy, classical thermodynamics is not concerned with the rate at which such processes take place, termed kinetics. For this reason, the use of the term "thermodynamics" usually refers to equilibrium thermodynamics. In this connection, a central concept in thermodynamics is that of quasistatic processes, which are idealized, "infinitely slow" processes. Timedependent thermodynamic processes are studied by nonequilibrium thermodynamics.
Thermodynamic laws are of very general validity, and they do not depend on the details of the interactions or the systems being studied. This means they can be applied to systems about which one knows nothing other than the balance of energy and matter transfer with the environment. Examples of this include Einstein's prediction of spontaneous emission around the turn of the 20th century and the current research into the thermodynamics of black holes.
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Thermodynamic parameters
The parameters used to describe the state of a system generally depend on the exact system under consideration, and the conditions under which that system is maintained. The most commonly considered parameters are:
 Statistical parameters:
 Temperature: T
 Entropy: S
 Two more parameters can be considered for open system:

 Number of particles N, of each component of the system
 Chemical potential, μ of each component of the system
The mechanical parameters listed above can be described in terms of fundamental classical or quantum physics, while the statistical parameters can only be understood in terms of statistical mechanics.
In most applications of thermodynamics, one or more of these parameters will be held constant, while one or more of the remaining parameters are allowed to vary. Mathematically, this means the system can be described as a point in ndimensional space, where n is the number of parameters not held fixed. Using statistical mechanics, combined with the laws of classical or quantum physics, equations of state can be derived which express each of these parameters in terms of the others. The simplest and most important of these equations of state is the ideal gas law
 pV = nRT
where R is the universal gas constant.
and its derived equation:
 pV = NkT
where k is the Boltzmann constant.
Thermodynamic potentials
Four quantities, called thermodynamic potentials, can be defined in terms of the thermodynamic parameters of a physical system:

 Internal energy E: dE=TdS  pdV
 Helmholtz free energy A: dA = −SdT  pdV
 Gibbs free energy G: dG = −SdT + Vdp
 Enthalpy H: dH = TdS + Vdp
Using the above differential forms of the four thermodynamic potentials, combined with the chain rule of product differentiation, the four potentials can be expressed in terms of each other and the thermodynamic parameters, as below:

 E = H − PV = A + TS
 A = E − TS = G − PV
 G = A + PV = H − TS
 H = G + TS = E + PV
The above relationships between the thermodynamic potentials and the thermodynamic parameters do not depend upon the particular system being studied; they are universal relationships that can be derived using statistical mechanics, with no regard for the forces or interaction potentials between the components of the system. However, the dependence of any one of these four thermodynamic potentials cannot be expressed in terms of the thermodynamic parameters of the system without knowledge of the interaction potentials between system components, the quantum energy levels and their corresponding degeneracies, or the partition function of the system under study. However, once the dependence of one of the thermodynamic functions upon the thermodynamic variables is determined, the three other thermodynamic potentials can be easily derived using the above equations.
Thermodynamic systems
A thermodynamic system is that part of the universe that is under consideration. A real or imaginary boundary separates the system from the rest of the universe, which is referred to as the environment, or sometimes as a reservoir. A useful classification of thermodynamic systems is based on the nature of the boundary and the flows of matter, energy and entropy through it.
There are three kinds of systems depending on the kinds of exchanges taking place between a system and its environment:

 isolated systems: not exchanging heat, matter or work with their environment. Mathematically, this implies that TdS, dN, and pdV are all zero, and therefore dE is zero. An example of an isolated system would be an insulated container, such as an insulated gas cylinder.
 closed systems: exchanging energy (heat and work) but not
matter with their environment. In this case, only dN is generally
zero. A greenhouse is an example of a closed system exchanging heat
but not work with its environment. Whether a system exchanges heat,
work or both is usually thought of as a property of its boundary,
which can be
 adiabatic boundary: not allowing heat exchange, TdS = 0
 rigid boundary: not allowing exchange of work, pdV = 0
 open systems: exchanging energy (heat and work) and matter with their environment. A boundary allowing matter exchange is called permeable. The ocean would be an example of an open system.
In reality, a system can never be absolutely isolated from its environment, because there is always at least some slight coupling, even if only via minimal gravitational attraction. In analyzing a system in steadystate, the energy into the system is equal to the energy leaving the system. _{ [1] (http://www.tpub.com/content/doe/h1012v1/css/h1012v1_94.htm)}
When a system is at equilibrium under a given set of conditions, it is said to be in a definite state. The state of the system can be described by a number of intensive variables and extensive variables. The properties of the system can be described by an equation of state which specifies the relationship between these variables.
The laws of thermodynamics
Alternative statements that are mathematically equivalent can be given for each law.
 Zeroth law: Thermodynamic equilibrium. When two systems are put in contact with each other, there will be a net exchange of energy and/or matter between them unless they are in thermodynamic equilibrium. Two systems are in thermodynamic equilibrium with each other if they stay the same after being put in contact. The zeroth law is stated as

 If systems A and B are in thermodynamic equilibrium, and systems B and C are in thermodynamic equilibrium, then systems A and C are also in thermodynamic equilibrium.
 While this is a fundamental concept of thermodynamics, the need to state it explicitly as a law was not perceived until the first third of the 20th century, long after the first three laws were already widely in use, hence the zero numbering. There is still some discussion about its status.
 Thermodynamic equilibrium includes thermal equilibrium (associated to heat exchange and parameterized by temperature), mechanical equilibrium (associated to work exchange and parameterized generalized forces such as pressure), and chemical equilibrium (associated to matter exchange and parameterized by chemical potential).
 1st Law: Conservation of energy. This is a fundamental principle of mechanics, and more generally of physics. In thermodynamics, it is used to give a precise definition of heat. It is stated as follows:

 The work exchanged in an adiabatic process depends only on the initial and the final state and not on the details of the process.
 or

 The net sum of exchange of heat and work of a system with the environment is a change of property. The amount of property change is determined only by the initial and final states and is independent on the path through which the process takes place.
 or

 The heat flowing into a system equals the increase in internal energy of the system plus the work done by the system.
 or

 Energy cannot be created or destroyed, only modified in form.
Mathematically, it can be represented as
where Q = energy input into system, ΔU = change in internal energy of the system, and ±W = work done on or by the system.
 2nd Law: A far reaching and powerful law, it is typically stated in one of two ways:
 or

 It is impossible to obtain a process that, operating in cycle, produces no other effect than a positive heat flow from a colder body to a hotter one. (Clausius Statement)
 The entropy of a thermally isolated macroscopic system never decreases (see Maxwell's demon), however a microscopic system may exhibit fluctuations of entropy opposite to that dictated by the second law (see Fluctuation Theorem). In fact the mathematical proof of the Fluctuation Theorem from timereversible dynamics and the Axiom of Causality, constitutes a proof of the Second Law. In a logical sense the Second Law thus ceases to be a "Law" of Physics and instead becomes a theorem which is valid for large systems or long times.
 3rd Law: This law explains why it is so hard to cool something to absolute zero:

 All processes cease as temperature approaches zero.
 As temperature goes to 0, the entropy of a system approaches a constant.
These laws have been humorously summarised as Ginsberg's theorem: (1) you can't win, (2) you can't break even, and (3) you can't get out of the game.
Or, alternatively: (1) you can't get anything without working for it, (2) the most you can accomplish by working is to break even, and (3) you can only break even at absolute zero.
Or, (1) you cannot win or quit the game, (2) you cannot tie the game unless it is very cold, (3) the weather doesn't get that cold.
More about the 2nd Law
The Second Law is exhibited (coarsely) by a box of electrical cables. Cables added from time to time tangle, inside the 'closed system' (cables in a box) by adding and then removing cables. The best way to untangle is to start by taking the cables out of the box and placing them stretched out. The cables in a closed system (the box) will never untangle, but giving them some extra space starts the process of untangling (by going outside the closed system).
C.P. Snow said the following in a Rede Lecture in 1959 entitled "The Two Cultures and the Scientific Revolution."
 "A good many times I have been present at gatherings of people who, by the standards of the traditional culture, are thought highly educated and who have with considerable gusto been expressing their incredulity at the illiteracy of scientists. Once or twice I have been provoked and have asked the company how many of them could describe the Second Law of Thermodynamics. The response was cold: it was also negative."
The laws of thermodynamics and mechanics
The First Law of thermodynamics is an exact consequence of the laws of mechanics—classical or quantum. The Fluctuation Theorem shows that the Second Law of Thermodynamics is also an exact consequence of the laws of mechanics except that it is only valid in the large system or long time limit.
Examples
Substances describable by temperature alone
Blackbody radiation is an example, since photon number is not conserved. Such a state is completely described by its temperature, although if phase transitions or spontaneous symmetry breaking occur other variables may be needed to discriminate among the phases. (This problem does not arise for blackbody radiation.) Given the internal energy as a function of temperature, we can define F = U  TS.
Substances describable by temperature and pressure alone
Most "pure" nonmagnetic substances fall into this category. This state is completely described by its temperature and pressure, except at phase transitions and perhaps spontaneous symmetry breaking in the ordered phase. Given U and V (or the density ρ) as a function of T and P, we can define the Helmholtz energy as before and the Gibbs energy as G = U  TS + PV and the enthalpy as H = U + PV.
Substances describable by temperature, pressure and chemical potential
If there are more than one kind of atom/molecule, a substance would fall into this category. This state is completely described by its temperature, pressure and chemical potentials, except at phase transitions and perhaps spontaneous symmetry breaking in the ordered phase.
Substances describable by temperature and magnetic field
If a substance is a ferromagnet or a superconductor, for example, it would fall into this category. It is completely described by its temperature and magnetic field, except at phase transitions and perhaps spontaneous symmetry breaking in the ordered phase.
See also
 Thermodynamic properties
 Thermodynamic equations
 important publications in thermodynamics
 Onsager reciprocal relations  sometimes called the Furth Law of Thermodynamics
 Statistical Mechanics
 Legendre transformation
 Thermodynamics also touches upon the fields of:
 Phase equilibrium
 Fluid dynamics
 Calorimetry
 Thermal analysis
 Thermochemistry also known as chemical thermodynamics
Quotes
"Thermodynamics is the only physical theory of universal content which, within the framework of the applicability of its basic concepts, I am convinced will never be overthrown." — Albert Einstein
"In this house, we obey the laws of thermodynamics!" (after Lisa constructs a perpetual motion machine whose energy increases with time) — Homer Simpson
"Any given thing gets less energy than it puts in, perpetual motion, therefore, is impossible."
Units
Wikibooks (http://wikibooks.org/wiki/Wikibooks_portal)
 Engineering Thermodynamics (http://wikibooks.org/wiki/Engineering_Thermodynamics)
General subfields within physics  
Classical mechanics  Condensed matter physics  Continuum mechanics  Electromagnetism  General relativity  Particle physics  Quantum field theory  Quantum mechanics  Solid state physics  Special relativity  Statistical mechanics  Thermodynamics 