Timeline of thermodynamics, statistical mechanics, and random processes



A timeline of events related to statistical mechanics, and random processes.

Ancient times

Void argument

  • In c.485 BC, Parmenides makes the ontological argument against nothingness, essentially denying the possible existence of a void.
  • In c.460 BC, Leucippus, in opposition to Parmenides' denial of the void, proposes the atomic theory, which supposes that everything in the universe is either atoms or voids; a theory which, according to Aristotle, was stimulated into conception so to purposely contradict Parmenides' argument.
  • In c.350 BC, Aristotle proclaims, in opposition to Leucippus, the dictum horror vacui or “nature abhors a vacuum”. Aristotle reasoned that in a complete vacuum, infinite speed would be possible because motion would encounter no resistance. Since he did not accept the possibility of infinite speed, he decided that a vacuum was equally impossible.
  • In 1643, Galileo Galilei, while generally accepting the horror vacui of Aristotle, believes that nature’s vacuum-abhorrence is limited. Pumps operating in mines had already proven that nature would only fill a vacuum with water up to a height of 30 feet. Knowing this curious fact, Galileo encourages his former pupil Evangelista Torricelli to investigate these supposed limitations and in doing so invented the first vacuum and mercury thermometer.

Atomic postulates

  • 5th century BC - the classical elements are used to support various theories of combustion; Empedocles writes about his four-element theory of earth, water, air, and fire
  • 5th century BC - Leucippus and Democritus formulate the first philosophy of atomism
  • 1st century BC - Lucretius writes his epic atomistic poem De Rerum Natura

Before 1800

  • 1620 - Francis Bacon reviews a wide range of observations about heat and related phenomena, and suggests that heat is related to motion (Novum Organum, Book II, XI)
  • 1660 - Boyle's Law, relating the pressure and volume of a gas
  • 1669 - J.J. Becher puts forward a theory of combustion involving combustible earth (Latin terra pinguis).
  • 1676-1689 - Gottfried Leibniz develops the concept of conservation of energy
  • 1694-1734 - phlogiston and develops the theory
  • 1702 - Guillaume Amontons introduces the concept of gases
  • 1738 - Daniel Bernoulli publishes Hydrodynamics, initiating the kinetic theory
  • 1761 - temperature when melting
  • 1772 - Black's student phlogiston theory
  • 1776 - John Smeaton publishes a paper on experiments related to power, work, momentum, and kinetic energy, supporting the conservation of energy
  • 1777 - conduction
  • 1783 - caloric theory
  • 1784 - Jan Ingenhousz describes Brownian motion of charcoal particles on water
  • 1791 - Pierre Prévost shows that all bodies radiate heat, no matter how hot or cold they are
  • 1798 - Count Rumford (Benjamin Thompson) performs measurements of the frictional heat generated in boring cannons and develops the idea that heat is a form of kinetic energy; his measurements refute caloric theory, but are imprecise enough to leave room for doubt

1800-1847

  • 1804 - Sir John Leslie observes that a matte black surface radiates heat more effectively than a polished surface, suggesting the importance of black body radiation
  • 1805 - William Hyde Wollaston defends the conservation of energy in On the Force of Percussion
  • 1808 - atomic weight
  • 1810 - Sir John Leslie freezes water to ice artificially
  • 1813 - Peter Ewart supports the idea of the conservation of energy in his paper On the measure of moving force; the paper strongly influences Dalton and his pupil, James Joule
  • 1819 - Pierre Louis Dulong and crystal
  • 1820 - John Herapath develops some ideas in the kinetic theory of gases but mistakenly associates temperature with momentum rather than kinetic energy; his work receives little attention other than from Joule
  • 1822 - Joseph Fourier formally introduces the use of dimensions for physical quantities in his Theorie Analytique de la Chaleur
  • 1822 - Marc Séguin writes to John Herschel supporting the conservation of energy and kinetic theory
  • 1824 - second law of thermodynamics
  • 1827 - Robert Brown discovers the Brownian motion of pollen and dye particles in water
  • 1831 - Macedonio Melloni demonstrates that black body radiation can be reflected, refracted, and polarised in the same way as light
  • 1834 - Émile Clapeyron popularises Carnot's work through a graphical and analytic formulation
  • 1841 - Julius Robert von Mayer, an amateur scientist, writes a paper on the conservation of energy, but his lack of academic training leads to its rejection
  • 1842 - Mayer makes a connection between work, heat, and the human mechanical equivalent of heat
  • 1842 - reversed
  • 1843 - John James Waterston fully expounds the kinetic theory of gases, but is ridiculed and ignored
  • 1843 - James Joule experimentally finds the mechanical equivalent of heat
  • 1846 - Karl-Hermann Knoblauch publishes De calore radiante disquisitiones experimentis quibusdam novis illustratae
  • 1846 - Grove publishes an account of the general theory of the conservation of energy in On The Correlation of Physical Forces
  • 1847 - first law of thermodynamics

1848-1899

  • 1848 - William Thomson extends the concept of absolute zero from gases to all substances
  • 1849 - temperature using his hypothesis of molecular vortices
  • 1850 - Rankine uses his vortex theory to establish accurate relationships between the temperature, steam will be negative.
  • 1850 - second law of thermodynamics, abandoning the caloric theory, but preserving Carnot's principle.
  • 1851 - Thomson gives an alternative statement of the second law.
  • 1852 - Joule and Thomson demonstrate that a rapidly expanding gas cools, later named the Joule-Thomson effect
  • 1854 - Helmholtz puts forward the idea of the heat death of the universe
  • 1854 - Clausius establishes the importance of dQ/T (Clausius's theorem), but does not yet name the quantity.
  • 1854 - Rankine introduces his thermodynamic function, later identified as entropy
  • 1856 - August Krönig publishes an account of the kinetic theory of gases, probably after reading Waterston's work
  • 1857 - Clausius gives a modern and compelling account of the kinetic theory of gases in his On the nature of motion called heat
  • 1859 - James Clerk Maxwell discovers the distribution law of molecular velocities
  • 1859 - black body is a function of only temperature and frequency
  • 1865 - Clausius introduces the modern macroscopic concept of entropy
  • 1865 - Josef Loschmidt applies Maxwell's theory to estimate the number-density of molecules in gases, given observed gas viscosities.
  • 1867 - Maxwell asks whether Maxwell's demon could reverse irreversible processes
  • 1870 - Clausius proves the scalar virial theorem
  • 1872 - H-theorem
  • 1874 - Thomson formally states the second law of thermodynamics.
  • 1876 - chemical thermodynamics in general.
  • 1876 - Loschmidt criticises Boltzmann's H theorem as being incompatible with microscopic reversibility (Loschmidt's paradox).
  • 1877 - Boltzmann states the relationship between entropy and probability.
  • 1879 - Jožef Stefan observes that the total radiant flux from a blackbody is proportional to the fourth power of its temperature and states the Stefan-Boltzmann law.
  • 1884 - Boltzmann derives the Stefan-Boltzmann blackbody radiant flux law from thermodynamic considerations.
  • 1888 - principle that the response of a chemical system perturbed from equilibrium will be to counteract the perturbation.
  • 1889 - Nernst equation.
  • 1889 - Arrhenius equation.
  • 1893 - Wilhelm Wien discovers the displacement law for a blackbody's maximum specific intensity.

1900-1944

  • 1900 - law of black-body radiation
  • 1905 - Albert Einstein argues that the reality of quanta would explain the photoelectric effect
  • 1905 - Einstein mathematically analyzes Brownian motion as a result of random molecular motion
  • 1906 - Nernst presents a formulation of the third law of thermodynamics
  • 1907 - Einstein uses quantum theory to estimate the heat capacity of an Einstein solid
  • 1909 - Constantin Carathéodory develops an axiomatic system of thermodynamics
  • 1910 - Einstein and Marian Smoluchowski find the Einstein-Smoluchowski formula for the attenuation coefficient due to density fluctuations in a gas
  • 1911 - Paul Ehrenfest and Tatjana Ehrenfest-Afanassjewa publish their classical review on the statistical mechanics of Boltzmann, Begriffliche Grundlagen der statistischen Auffassung in der Mechanik
  • 1912 - improved heat capacity estimate by allowing low-frequency phonons
  • 1916 - Sydney Chapman and David Enskog systematically develop the kinetic theory of gases.
  • 1916 - Einstein considers the thermodynamics of stimulated emission
  • 1919 - James Jeans discovers that the dynamical constants of motion determine the distribution function for a system of particles
  • 1920 - Megh Nad Saha states his ionization equation
  • 1923 - Debye and electrolytes
  • 1924 - Bose-Einstein statistics, in a paper translated by Einstein
  • 1926 - fermions
  • 1927 - John von Neumann introduces the density matrix representation and establishes quantum statistical mechanics
  • 1928 - John B. Johnson discovers Johnson noise in a resistor
  • 1928 - Harry Nyquist derives the fluctuation-dissipation relationship for a resistor to explain Johnson noise
  • 1929 - Onsager reciprocal relations
  • 1942 - Joseph Leo Doob states his theorem on Gauss-Markov processes
  • 1944 - Onsager gives an analytic solution to the 2D phase transition

1945-present

  • 1948 - Claude Elwood Shannon establishes information theory.
  • 1957 - Aleksandr Solomonovich Kompaneets derives his Compton scattering Fokker-Planck equation.
  • 1957 - Ryogo Kubo derives the first of the Green-Kubo relations for linear transport coefficients.
  • 1957 - Edwin T. Jaynes gives MaxEnt interpretation of thermodynamics from information theory.
  • 1972 - Jacob Bekenstein suggests that black holes have an entropy proportional to their surface area.
  • 1974 - Stephen Hawking predicts that black holes will radiate particles with a black-body spectrum which can cause black hole evaporation

See also

 
This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "Timeline_of_thermodynamics,_statistical_mechanics,_and_random_processes". A list of authors is available in Wikipedia.