 Boltzmann constant

 For the constant pertaining to energy of black body radiation see Stefan–Boltzmann constant
Values of k^{[1]} Units 1.3806488(13)×10^{−23} J K^{−1} 8.6173324(78)×10^{−5} eV K^{−1} 1.3806488(13)×10^{−16} erg K^{−1} For details, see Value in different units below. The Boltzmann constant (k or k_{B}) is the physical constant relating energy at the individual particle level with temperature, which must necessarily be observed at the collective or bulk level. It is the gas constant R divided by the Avogadro constant N_{A}:
It has the same units as entropy. It is named after the Austrian physicist Ludwig Boltzmann.
Contents
Bridge from macroscopic to microscopic physics
Boltzmann's constant, k, is a bridge between macroscopic and microscopic physics, since temperature (T) makes sense only in the macroscopic world, while the quantity kT gives a quantity of energy which is on the order of, though rarely exactly the same as, the energy of a given atom in a substance with a temperature T.
Macroscopically, the ideal gas law states that, for an ideal gas, the product of pressure P and volume V is proportional to the product of amount of substance n (in moles) and absolute temperature T:
where R is the gas constant (8.314 4621(75) J K^{−1} mol^{−1}^{[1]}). Introducing the Boltzmann constant transforms the ideal gas law into an equation about the microscopic properties of molecules,^{[citation needed]}^{[dubious – discuss]}
where N is the number of molecules of gas. (For n = 1 i.e. for 1 mole, N is equal to N_{A}, the Avogadro constant.) Thus, the left hand side of the equation is a macroscopic amount of pressurevolume work represented by the state of the bulk gas. The right hand side divides this energy into N units, one for each gas molecule, each of which represents kT amount of energy.
Role in the equipartition of energy
Given a thermodynamic system at an absolute temperature T, the thermal energy carried by each microscopic "degree of freedom" in the system is on the order of magnitude of kT/2 (i. e., about 2.07×10^{−21} J, or 0.013 eV, at room temperature).
Application to simple gas thermodynamics
In classical statistical mechanics, this average is predicted to hold exactly for homogeneous ideal gases. Monatomic ideal gases possess three degrees of freedom per atom, corresponding to the three spatial directions, which means a thermal energy of 1.5kT per atom (in the general case, DkT/2, where D is the number of spatial dimensions). As indicated in the article on heat capacity, this corresponds very well with experimental data. The thermal energy can be used to calculate the root mean square speed of the atoms, which is inversely proportional to the square root of the atomic mass. The root mean square speeds found at room temperature accurately reflect this, ranging from 1370 m/s for helium, down to 240 m/s for xenon.
Kinetic theory gives the average pressure P for an ideal gas as
Substituting that the average translational kinetic energy is
gives
so the ideal gas equation is regained.
The ideal gas equation is also followed quite well for molecular gases; but the form for the heat capacity is more complicated, because the molecules possess new internal degrees of freedom, as well as the three degrees of freedom for movement of the molecule as a whole. Diatomic gases, for example, possess a total of seven degrees of simple freedom per molecule that are related to atomic motion (three translational, two rotational, and two vibrational). At lower temperatures, not all these degrees of freedom may fully participate in the gas heat capacity, due to quantum mechanical limits on the availability of excited states, at the thermal energy available.
Role in Boltzmann factors
More generally, systems in equilibrium at temperature T have probability p of occupying a state i with energy E weighted by the corresponding Boltzmann factor:
Where Z is the partition function. Again, it is the energylike quantity kT which takes central importance.
Consequences of this include (in addition to the results for ideal gases above) the Arrhenius equation in chemical kinetics.
Role in the statistical definition of entropy
Further information: Entropy (statistical thermodynamics)In statistical mechanics, the entropy S of an isolated system at thermodynamic equilibrium is defined as the natural logarithm of W, the number of distinct microscopic states available to the system given the macroscopic constraints (such as a fixed total energy E):
This equation, which relates the microscopic details, or microstates, of the system (via W) to its macroscopic state (via the entropy S), is the central idea of statistical mechanics. Such is its importance that it is inscribed on Boltzmann's tombstone.
The constant of proportionality k serves to make the statistical mechanical entropy equal to the classical thermodynamic entropy of Clausius:
One could choose instead a rescaled dimensionless entropy in microscopic terms such that
This is a rather more natural form; and this rescaled entropy exactly corresponds to Shannon's subsequent information entropy.
The characteristic energy kT is thus the heat required to increase the rescaled entropy by one nat.
Role in semiconductor physics: the thermal voltage
In semiconductors, the relationship between the flow of electrical current and the electrostatic potential across a pn junction depends on a characteristic voltage called the thermal voltage, denoted V_{T}. The thermal voltage depends on absolute temperature T as
where q is the magnitude of the electrical charge on the electron with a value 1.602 176 565(35)×10^{−19} C^{[1]} and k is the Boltzmann constant in Joules/K. In electronvolts, the Boltzmann constant is 8.617 3324(78)×10^{−5} eV/K^{[1]}, making it easy to calculate that at room temperature (≈ 300 K), the value of the thermal voltage is approximately 25.85 millivolts ≈ 26 mV [1]. The thermal voltage is also important in plasmas and electrolyte solutions; in both cases it provides a measure of how much the spatial distribution of electrons or ions is affected by a boundary held at a fixed voltage.^{[2]}^{[3]}
History
Although Boltzmann first linked entropy and probability in 1877, it seems the relation was never expressed with a specific constant until Max Planck first introduced k , and gave an accurate value for it (1.346×10^{−23} J/K, about 2.5% lower than today's figure), in his derivation of the law of black body radiation in 1900–1901.^{[4]} Before 1900, equations involving Boltzmann factors were not written using the energies per molecule and Boltzmann's constant, but rather using a form of the gas constant R, and macroscopic energies for macroscopic quantities of the substance. The iconic terse form of the equation S = k log W on Boltzmann's tombstone is in fact due to Planck, not Boltzmann. Planck actually introduced it in the same work as his h.^{[5]}
As Planck wrote in his Nobel Prize lecture in 1920,^{[6]}
This constant is often referred to as Boltzmann's constant, although, to my knowledge, Boltzmann himself never introduced it — a peculiar state of affairs, which can be explained by the fact that Boltzmann, as appears from his occasional utterances, never gave thought to the possibility of carrying out an exact measurement of the constant.
This "peculiar state of affairs" can be understood by reference to one of the great scientific debates of the time. There was considerable disagreement in the second half of the nineteenth century as to whether atoms and molecules were "real" or whether they were simply a heuristic, a useful tool for solving problems. Nor was there agreement as to whether "chemical molecules" (as measured by atomic weights) were the same as "physical molecules" (as measured by kinetic theory). To continue the quotation from Planck's 1920 lecture:^{[6]}
Nothing can better illustrate the positive and hectic pace of progress which the art of experimenters has made over the past twenty years, than the fact that since that time, not only one, but a great number of methods have been discovered for measuring the mass of a molecule with practically the same accuracy as that attained for a planet.
Value in different units
Values of k Units Comments 1.380 6488(13)×10^{−23} J/K SI units, 2010 CODATA value^{[1]} 8.617 3324(78)×10^{−5} eV/K 2010 CODATA value^{[1]}
1 electronvolt = 1.602 176 565(35)×10^{−19} J^{[1]}1/k_{B} = 11 604.519(11) K/eV
2.083 6618(19)×10^{10} Hz/K 2010 CODATA value^{[1]}
1 Hz·h = 6.626 069 57(29)×10^{−34} J^{[1]}3.166 8114(29)×10^{−6} E_{H}/K E_{H} = 2R_{∞}hc = 4.359 744 34(19)×10^{−18} J^{[1]}
= 6.579 683 920 729(33) Hz·h^{[1]}1.380 6488(13)×10^{−16} erg/K 1 erg = 1×10^{−7} J 3.297 6230(30)×10^{−24} cal/K 1 Steam Table calorie = 4.1868 J 1.832 0128(17)×10^{−24} cal/°R 1 degree Rankine = 5/9 K 5.657 3016(51)×10^{−24} ft lb/°R 1 footpound force = 1.355 817 948 331 4004 J 0.695 034 76(63) cm^{−1}/K 2010 CODATA value^{[1]}
1 cm^{−1 }·hc = 1.986 445 683(87)×10^{−23} J0.001 987 2041(18) kcal/mol/K per mole form often used in statistical mechanics—using thermochemical cal=4.184 Joules 0.008 314 4621(75) kJ/mol/K per mole form often used in statistical mechanics 4.10 pN·nm kT in piconewton nanometer at 24°C, used in biophysics −228.5991678(40) dBW/K/Hz in decibel watts, used in telecommunications Since k is a physical constant of proportionality between temperature and energy, its numerical value depends on the choice of units for energy and temperature. The Kelvin temperature scale is based on the Celsius scale which divides the temperature range of liquid water into one hundred increments. The small numerical value of the constant in the metric system reflects the small energy in joules required to increase a particle's energy by raising the temperature by 1 K. The characteristic energy kT is a term encountered in many physical relationships.
Planck units
The Boltzmann constant provides a mapping from this characteristic microscopic energy E to the macroscopic temperature scale T = E/k. In physics research another definition is often encountered in setting k to unity, resulting in the Planck units or natural units for temperature and energy. In this context temperature is measured effectively in units of energy and the Boltzmann constant is not explicitly needed.^{[7]}:
This simplifies many physical relationships and makes the definition of thermodynamic entropy coincide with that of information entropy:
The value chosen for the Planck unit of temperature is that corresponding to the energy of the Planck mass or 1.416 833(85)×10^{32} K^{[1]}.
References
 ^ ^{a} ^{b} ^{c} ^{d} ^{e} ^{f} ^{g} ^{h} ^{i} ^{j} ^{k} ^{l} ^{m} P.J. Mohr, B.N. Taylor, and D.B. Newell (2011), "The 2010 CODATA Recommended Values of the Fundamental Physical Constants" (Web Version 6.0). This database was developed by J. Baker, M. Douma, and S. Kotochigova. Available: http://physics.nist.gov/constants [Thursday, 02Jun2011 21:00:12 EDT]. National Institute of Standards and Technology, Gaithersburg, MD 20899.
 ^ Kirby BJ., Micro and Nanoscale Fluid Mechanics: Transport in Microfluidic Devices, http://www.kirbyresearch.com/textbook
 ^ Tabeling (2006), Introduction to Microfluidics
 ^ Planck, Max (1901), "Ueber das Gesetz der Energieverteilung im Normalspectrum", Ann. Phys. 309 (3): 553–63, Bibcode 1901AnP...309..553P, doi:10.1002/andp.19013090310, http://www.physik.uniaugsburg.de/annalen/history/historicpapers/1901_309_553563.pdf. English translation: "On the Law of Distribution of Energy in the Normal Spectrum".
 ^ http://www.bourbaphy.fr/duplantier2.pdf
 ^ ^{a} ^{b} Planck, Max (2 June 1920), The Genesis and Present State of Development of the Quantum Theory (Nobel Lecture), http://nobelprize.org/nobel_prizes/physics/laureates/1918/plancklecture.html
 ^ Kalinin, M; Kononogov, S (2005), "Boltzmann's Constant, the Energy Meaning of Temperature, and Thermodynamic Irreversibility", Measurement Techniques 48 (7): 632–36, doi:10.1007/s1101800501959
Categories: Statistical mechanics
 Thermodynamics
 Fundamental constants
 Physical constants
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