Wilhelm Wien was born on January 13, 1864 at Fischhausen, in East
Prussia. He was the son of the landowner Carl Wien, and seemed destined
for the life of a gentleman farmer, but an economic crisis and his own
secret sense of vocation led him to University studies. When in 1866 his
parents moved to Drachstein, in the Rastenburg district of East Prussia,
Wien went to school in 1879 first at Rastenburg and later, from 1880 till
1882, at the City School at Heidelberg. After leaving school he went,
in 1882, to the University of Göttingen to study mathematics and
the natural sciences and in the same year also to the University of Berlin.
From 1883 until 1885 he worked in the laboratory of Hermann von Helmholtz
and in 1886 he took his doctorate with a thesis on his experiments on
the diffraction of light on sections of metals and on the influence of
materials on the colour of refracted light.
His studies were then interrupted by the illness of his father and, until
1890, he helped in the management of his father's land. He was, however,
able to spend, during this period, one semester with Helmholtz and in
1887 he did experiments on the permeability of metals to light and heat
rays. When his father's land was sold he returned to the laboratory of
Helmholtz, who had been moved to, and had become President of, the Physikalisch-Technische
Reichsanstalt, established for the study of industrial problems. Here
he remained until 1896 when he was appointed Professor of Physics at Aix-la-Chapelle
in succession to Philipp Lenard. In 1899, he was appointed Professor of
Physics at the University of Giessen. In 1900 he became Professor of the
same subject at Würzburg, in succession to W.C. Röntgen, and
in this year he published his Lehrbuch der Hydrodynamik (Textbook
of hydrodynamics).
In 1902 he was invited to succeed Ludwig Boltzmann as Professor
of Physics at the University of Leipzig and in 1906 to succeed Drude
as Professor of Physics at the University of Berlin; but he
refused both these invitations.
In 1920 he was appointed Professor of Physics at Munich, where he
remained throughout the rest of his life.
In addition to the early work already mentioned, Wien worked, at
the Physikalisch-Technische Reichsanstalt, with Holborn on
methods of measuring high temperatures with the Le Chatelier
thermoelements and at the same time did theoretical work on
thermodynamics, especially on the laws governing the radiation of
heat.
In 1893 he announced the law which states that the wavelength
changes with the temperature, a law which later became the law of
displacement.
In 1894 he published a paper on temperature and the entropy of
radiation, in which the terms temperature and entropy were
extended to radiation in empty space. In this work he was led to
define an ideal body, which he called the black body, which
completely absorbs all radiations. In 1896 he published the
formula of Wien, which was the result of work undertaken to find
a formula for the composition of the radiation of such a black
body. Later it was proved that this formula is valid only for the
short waves, but Wien's work enabled Max Planck to resolve the
problem of radiation in thermal equilibrium by means of quantum
physics. For this work Wien was awarded the Nobel Prize for
Physics for 1911. An interesting point about it is that this
theoretical work came from an Institute devoted to technical
problems and it led to new techniques for illumination and the
measurement of high temperatures.
When Wien moved, in 1896, to Aix-la-Chapelle to succeed Lenard, he found
there a laboratory equipped for the study of electrical discharges in
vacuo and in 1897 he began to work on the nature of cathode rays.
Using a very high vacuum tube with a Lenard window, he confirmed the discovery
that dean Perrin had made two years earlier, that cathode rays are composed
of rapidly-moving, negatively-charged particles (electrons). And then,
almost at the same time as Sir J.J. Thomson in Cambridge, but by a different
method, he measured the relation of the electric charge on these particles
to their mass and found, as Thomson did, that they are about two thousand
times lighter than the atoms of hydrogen.
In 1898 Wien studied the canal rays discovered by Goldstein and
concluded that they were the positive equivalent of the
negatively-charged cathode rays. He measured their deviation by
magnetic and electric fields and concluded that they are composed
of positively-charged particles never heavier than
electrons.
The method used by Wien resulted some 20 years later in the
spectrography of masses, which has made possible the precise
measurement of the masses of various atoms and their isotopes,
necessary for the calculation of the energies released by nuclear
reactions. In 1900 Wien published a theoretical paper on the
possibility of an electromagnetic basis for mechanics.
Subsequently he did further work on the canal rays, showing, in
1912, that, if the pressure is not extremely weak, these rays
lose and regain, by collision with atoms of residual gas, their
electric charge along their course of travel. In 1918 he
published further work on these rays on the measurement of the
progressive decrease of their luminosity after they leave the
cathode and from these experiments he deduced what classical
physics calls the decay of the luminous vibrations in the atoms,
which corresponds in quantum physics to the limited duration of
excited states of atoms.
In this, and other, respects Wien's work contributed to the transition
from Newtonian to quantum physics. As Max von Laue wrote of him, his "immortal
glory" was that "he led us to the very gates of quantum physics".
Wien was a member of the Academies of Sciences of Berlin, Göttingen,
Vienna, Stockholm, Christiania and Washington, and an Honorary member
of the Physical Society of Frankfurt-on-Main.
In 1898 he married Luise Mehler of Aix-la-Chapelle. They had four
children. He died in Munich on August 30, 1928.
From Nobel Lectures, Physics 1901-1921, Elsevier Publishing Company, Amsterdam, 1967
This autobiography/biography was first published in the book series Les Prix Nobel. It was later edited and republished in Nobel Lectures. To cite this document, always state the source as shown above.
Copyright © The Nobel Foundation 1911