Ludwig Boltzmann
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Ludwig Boltzmann
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Born |
Ludwig Eduard Boltzmann
February 20, 1844 |
Died | September 5, 1906 (aged 62) |
Residence | Austria, Germany |
Nationality | Austrian |
Alma mater | University of Vienna |
Known for | |
Awards | ForMemRS (1899) |
Scientific career | |
Fields | Physics |
Institutions | |
Doctoral advisor | Josef Stefan |
Other academic advisors | Robert Bunsen Leo Königsberger Gustav Kirchhoff Hermann von Helmholtz |
Doctoral students | |
Other notable students | |
Signature | |
Ludwig Eduard Boltzmann (German pronunciation: [ˈluːtvɪç ˈbɔlt͡sman]; February 20, 1844 – September 5, 1906) was an Austrian physicist and philosopher whose greatest achievement was in the development of statistical mechanics, which explains and predicts how the properties of atoms (such as mass, charge, and structure) determine the physical properties of matter (such as viscosity, thermal conductivity, and diffusion).
Boltzmann coined the word ergodic while he was working on a problem in statistical mechanics.
Biography
Childhood and education
Boltzmann was born in Vienna, the capital of the Austrian Empire.
His father, Ludwig Georg Boltzmann, was a revenue official. His
grandfather, who had moved to Vienna from Berlin, was a clock
manufacturer, and Boltzmann's mother, Katharina Pauernfeind, was
originally from Salzburg. He received his primary education from a private tutor at the home of his parents. Boltzmann attended high school in Linz, Upper Austria. When Boltzmann was 15, his father died.
Boltzmann studied physics at the University of Vienna, starting in 1863. Among his teachers were Josef Loschmidt, Joseph Stefan, Andreas von Ettingshausen and Jozef Petzval. Boltzmann received his PhD degree in 1866 working under the supervision of Stefan; his dissertation was on the kinetic theory of gases. In 1867 he became a Privatdozent
(lecturer). After obtaining his doctorate degree, Boltzmann worked two
more years as Stefan's assistant. It was Stefan who introduced
Boltzmann to Maxwell's work.
Academic career
In 1869 at age 25, thanks to a letter of recommendation written by Stefan, he was appointed full Professor of Mathematical Physics at the University of Graz in the province of Styria. In 1869 he spent several months in Heidelberg working with Robert Bunsen and Leo Königsberger and in 1871 with Gustav Kirchhoff and Hermann von Helmholtz in Berlin. In 1873 Boltzmann joined the University of Vienna as Professor of Mathematics and there he stayed until 1876.
In 1872, long before women were admitted to Austrian universities, he
met Henriette von Aigentler, an aspiring teacher of mathematics and
physics in Graz. She was refused permission to audit lectures
unofficially. Boltzmann advised her to appeal, which she did,
successfully. On July 17, 1876 Ludwig Boltzmann married Henriette; they
had three daughters and two sons. Boltzmann went back to Graz to take up the chair of Experimental Physics. Among his students in Graz were Svante Arrhenius and Walther Nernst. He spent 14 happy years in Graz and it was there that he developed his statistical concept of nature.
Boltzmann was appointed to the Chair of Theoretical Physics at the University of Munich in Bavaria, Germany in 1890.
In 1894, Boltzmann succeeded his teacher Joseph Stefan as Professor of Theoretical Physics at the University of Vienna.
Final years
Boltzmann spent a great deal of effort in his final years defending his theories. He did not get along with some of his colleagues in Vienna, particularly Ernst Mach, who became a professor of philosophy and history of sciences in 1895. That same year Georg Helm and Wilhelm Ostwald presented their position on energetics at a meeting in Lübeck.
They saw energy, and not matter, as the chief component of the
universe. Boltzmann's position carried the day among other physicists
who supported his atomic theories in the debate. In 1900, Boltzmann went to the University of Leipzig, on the invitation of Wilhelm Ostwald. Ostwald offered Boltzmann the professorial chair in physics, which became vacant when Gustav Heinrich Wiedemann died. After Mach retired due to bad health, Boltzmann returned to Vienna in 1902. In 1903, Boltzmann, together with Gustav von Escherich and Emil Müller, founded the Austrian Mathematical Society. His students included Karl Přibram, Paul Ehrenfest and Lise Meitner.
In Vienna, Boltzmann taught physics and also lectured on philosophy. Boltzmann's lectures on natural philosophy
were very popular and received considerable attention. His first
lecture was an enormous success. Even though the largest lecture hall
had been chosen for it, the people stood all the way down the staircase.
Because of the great successes of Boltzmann's philosophical lectures,
the Emperor invited him for a reception at the Palace.
In 1906, Boltzmann's deteriorating mental condition forced him to resign his position. He committed suicide on September 5, 1906, by hanging himself while on vacation with his wife and daughter in Duino, near Trieste (then Austria). He is buried in the Viennese Zentralfriedhof. His tombstone bears the inscription of Boltzmann's entropy formula:
Philosophy
Boltzmann's kinetic theory of gases seemed to presuppose the reality of atoms and molecules, but almost all German philosophers and many scientists like Ernst Mach and the physical chemist Wilhelm Ostwald disbelieved their existence.
During the 1890s Boltzmann attempted to formulate a compromise position
which would allow both atomists and anti-atomists to do physics without
arguing over atoms. His solution was to use Hertz's theory that atoms were Bilder,
that is, models or pictures. Atomists could think the pictures were the
real atoms while the anti-atomists could think of the pictures as
representing a useful but unreal model, but this did not fully satisfy
either group. Furthermore, Ostwald and many defenders of "pure
thermodynamics" were trying hard to refute the kinetic theory of gases
and statistical mechanics because of Boltzmann's assumptions about atoms
and molecules and especially statistical interpretation of the second law of thermodynamics.
Around the turn of the century, Boltzmann's science was being
threatened by another philosophical objection. Some physicists,
including Mach's student, Gustav Jaumann,
interpreted Hertz to mean that all electromagnetic behavior is
continuous, as if there were no atoms and molecules, and likewise as if
all physical behavior were ultimately electromagnetic. This movement
around 1900 deeply depressed Boltzmann since it could mean the end of
his kinetic theory and statistical interpretation of the second law of
thermodynamics.
After Mach's resignation in Vienna in 1901, Boltzmann returned
there and decided to become a philosopher himself to refute
philosophical objections to his physics, but he soon became discouraged
again. In 1904 at a physics conference in St. Louis most physicists
seemed to reject atoms and he was not even invited to the physics
section. Rather, he was stuck in a section called "applied mathematics",
he violently attacked philosophy, especially on allegedly Darwinian
grounds but actually in terms of Lamarck's
theory of the inheritance of acquired characteristics that people
inherited bad philosophy from the past and that it was hard for
scientists to overcome such inheritance.
In 1905 Boltzmann corresponded extensively with the Austro-German philosopher Franz Brentano
with the hope of gaining a better mastery of philosophy, apparently, so
that he could better refute its relevancy in science, but he became
discouraged about this approach as well.
Physics
Boltzmann's most important scientific contributions were in kinetic theory, including the Maxwell–Boltzmann distribution for molecular speeds in a gas. In addition, Maxwell–Boltzmann statistics and the Boltzmann distribution over energies remain the foundations of classical statistical mechanics. They are applicable to the many phenomena that do not require quantum statistics and provide a remarkable insight into the meaning of temperature.
Much of the physics establishment did not share his belief in the reality of atoms and molecules — a belief shared, however, by Maxwell in Scotland and Gibbs in the United States; and by most chemists since the discoveries of John Dalton
in 1808. He had a long-running dispute with the editor of the
preeminent German physics journal of his day, who refused to let
Boltzmann refer to atoms and molecules as anything other than convenient
theoretical constructs. Only a couple of years after Boltzmann's death, Perrin's studies of colloidal suspensions (1908–1909), based on Einstein's theoretical studies of 1905, confirmed the values of Avogadro's number and Boltzmann's constant, and convinced the world that the tiny particles really exist.
To quote Planck, "The logarithmic connection between entropy and probability was first stated by L. Boltzmann in his kinetic theory of gases". This famous formula for entropy S is
where kB is Boltzmann's constant, and ln is the natural logarithm. W is Wahrscheinlichkeit, a German word meaning the probability of occurrence of a macrostate or, more precisely, the number of possible microstates corresponding to the macroscopic state of a system — number of (unobservable) "ways" in the (observable) thermodynamic state of a system can be realized by assigning different positions and momenta to the various molecules. Boltzmann's paradigm was an ideal gas of N identical particles, of which Ni are in the ith microscopic condition (range) of position and momentum. W can be counted using the formula for permutations
where i ranges over all possible molecular conditions. ( denotes factorial.) The "correction" in the denominator is because identical particles in the same condition are indistinguishable.
Boltzmann was also one of the founders of quantum mechanics due
to his suggestion in 1877 that the energy levels of a physical system
could be discrete.
The equation for S is engraved on Boltzmann's tombstone at the Vienna Zentralfriedhof — his second grave.
Boltzmann equation
The Boltzmann equation was developed to describe the dynamics of an ideal gas.
where ƒ represents the distribution function of single-particle position and momentum at a given time (see the Maxwell–Boltzmann distribution), F is a force, m is the mass of a particle, t is the time and v is an average velocity of particles.
This equation describes the temporal and spatial
variation of the probability distribution for the position and momentum
of a density distribution of a cloud of points in single-particle phase space. (See Hamiltonian mechanics.)
The first term on the left-hand side represents the explicit time
variation of the distribution function, while the second term gives the
spatial variation, and the third term describes the effect of any force
acting on the particles. The right-hand side of the equation represents
the effect of collisions.
In principle, the above equation completely describes the dynamics of an ensemble of gas particles, given appropriate boundary conditions. This first-order differential equation has a deceptively simple appearance, since ƒ can represent an arbitrary single-particle distribution function. Also, the force acting on the particles depends directly on the velocity distribution function ƒ. The Boltzmann equation is notoriously difficult to integrate. David Hilbert spent years trying to solve it without any real success.
The form of the collision term assumed by Boltzmann was approximate. However, for an ideal gas the standard Chapman–Enskog solution of the Boltzmann equation is highly accurate. It is expected to lead to incorrect results for an ideal gas only under shock wave conditions.
Boltzmann tried for many years to "prove" the second law of thermodynamics using his gas-dynamical equation — his famous H-theorem. However the key assumption he made in formulating the collision term was "molecular chaos", an assumption which breaks time-reversal symmetry as is necessary for anything
which could imply the second law. It was from the probabilistic
assumption alone that Boltzmann's apparent success emanated, so his long
dispute with Loschmidt and others over Loschmidt's paradox ultimately ended in his failure.
Finally, in the 1970s E.G.D. Cohen
and J. R. Dorfman proved that a systematic (power series) extension of
the Boltzmann equation to high densities is mathematically impossible.
Consequently, nonequilibrium statistical mechanics for dense gases and liquids focuses on the Green–Kubo relations, the fluctuation theorem, and other approaches instead.
Second thermodynamics law as a law of disorder
The idea that the second law of thermodynamics
or "entropy law" is a law of disorder (or that dynamically ordered
states are "infinitely improbable") is due to Boltzmann's view of the
second law of thermodynamics.
In particular, it was Boltzmann's attempt to reduce it to a stochastic collision function, or law of probability following from the random collisions of mechanical particles. Following Maxwell,
Boltzmann modeled gas molecules as colliding billiard balls in a box,
noting that with each collision nonequilibrium velocity distributions
(groups of molecules moving at the same speed and in the same direction)
would become increasingly disordered leading to a final state of
macroscopic uniformity and maximum microscopic disorder or the state of
maximum entropy (where the macroscopic uniformity corresponds to the
obliteration of all field potentials or gradients).
The second law, he argued, was thus simply the result of the fact that
in a world of mechanically colliding particles disordered states are the
most probable. Because there are so many more possible disordered
states than ordered ones, a system will almost always be found either in
the state of maximum disorder – the macrostate with the greatest number
of accessible microstates such as a gas in a box at equilibrium – or
moving towards it. A dynamically ordered state, one with molecules
moving "at the same speed and in the same direction", Boltzmann
concluded, is thus "the most improbable case conceivable...an infinitely
improbable configuration of energy."
Boltzmann accomplished the feat of showing that the second law of
thermodynamics is only a statistical fact. The gradual disordering of
energy is analogous to the disordering of an initially ordered pack of cards
under repeated shuffling, and just as the cards will finally return to
their original order if shuffled a gigantic number of times, so the
entire universe must some-day regain, by pure chance, the state from
which it first set out. (This optimistic coda to the idea of the dying
universe becomes somewhat muted when one attempts to estimate the
timeline which will probably elapse before it spontaneously occurs.)
The tendency for entropy increase seems to cause difficulty to
beginners in thermodynamics, but is easy to understand from the
standpoint of the theory of probability. Consider two ordinary dice,
with both sixes face up. After the dice are shaken, the chance of
finding these two sixes face up is small (1 in 36); thus one can say
that the random motion (the agitation) of the dice, like the chaotic
collisions of molecules because of thermal energy, causes the less
probable state to change to one that is more probable. With millions of
dice, like the millions of atoms involved in thermodynamic calculations,
the probability of their all being sixes becomes so vanishingly small
that the system must move to one of the more probable states.
However, mathematically the odds of all the dice results not being a
pair sixes is also as hard as the ones of all of them being sixes, and since statistically the data
tend to balance, one in every 36 pairs of dice will tend to be a pair
of sixes, and the cards -when shuffled- will sometimes present a certain
temporary sequence order even if in its whole the deck was disordered.