Gunnar Nordström

Gunnar Nordström

Nordström at the age of 35
Born 12 March 1881
Helsinki, Finland
Died 24 December 1923(1923-12-24) (aged 42)
Helsinki, Finland
Residence Finland, Germany, Switzerland, the Netherlands
Citizenship Russian, Finnish
Nationality Finnish
Fields Physics, Mechanics
Institutions Helsinki University of Technology
University of Helsinki
University of Göttingen
University of Leiden
Alma mater Helsinki University of Technology (Engineer),
University of Helsinki (Master of Science, and PhD)
Academic advisors Paul Ehrenfest, Walther Nernst (briefly)
Known for Nordström's theory of gravitation
Kaluza–Klein theory
Reissner–Nordström metric
Influences Albert Einstein
Influenced Albert Einstein, Rolf Nevanlinna

Gunnar Nordström (12 March 1881 – 24 December 1923) was a Finnish theoretical physicist best remembered for his theory of gravitation, which was an early competitor of general relativity. Nordström is often designated by modern writers as The Einstein of Finland due to his novel work in similar fields with similar methods to Einstein.[1][2]

Education and career

A picture taken in Helsinki in 1900 of three high school graduates wearing student caps, Gunnar Nordström on the left.

Nordström graduated high-school from Brobergska Skolan in central Helsinki 1899. At first he went on to study mechanical engineering at the Polytechnic institute in Helsinki, later renamed Helsinki University of Technology and today a part of the Aalto University. During his studies he developed an interest for more theoretical subjects, proceeding after graduation to further study for a master's degree in natural science, mathematics and economy at the University of Helsinki (1903–1907).[3]

Nordström then moved to Göttingen, Germany, where he had been recommended to go to study physical chemistry. However, he soon lost interest in the intended field and moved to study electrodynamics, a field the University of Göttingen was renowned for at the time.[1] He returned to Finland to complete his doctoral dissertation at the University of Helsinki in 1910, and become a docent at the university. Subsequently he became fascinated with the very novel and soon burgeoning field of gravitation and wanted to move to the Netherlands where scientists with contributions to that fields such as Hendrik Lorentz, Paul Ehrenfest and Willem de Sitter were active. Nordström was able to move to Leiden in 1916 to work under Ehrenfest, in the midst of the First World War, due to his Russian passport. Nordström spent considerable time in Leiden where he met a Dutch physics student, Cornelia van Leeuwen, with whom he went on to have several children.[3] After the war he declined a professorship at the University of Berlin, a post awarded instead to Max Born, in order to return to Finland in 1918 and hold at first the professorship of physics and later the professorship of mechanics at the Helsinki University of Technology.

One of the keys to Nordström's success as a scientist was his ability to learn to apply differential geometry to physics, a new approach that also would eventually lead Albert Einstein to the theory of general relativity. Few other scientists of the time in the World were able to make effective use of this new analytical tool, with the notable exception of Ernst Lindelöf.[4]

Contributions to theory

During the time in Leiden Nordström solved the field equations for the spherically symmetric charged body, thus extending Hans Reissner's results for a point charge. The metric for a non-rotating charge distribution is nowadays known as the Reissner–Nordström metric. Nordström maintained frequent contact with many of the other great physicists of the era, including Niels Bohr and Albert Einstein. For example, it was Bohr's contributions that helped Nordström to circumvent the Russian censorship of German post to Finland,[2] Finland was at the time a grand duchy of the Russian empire.

The theory for which Nordström was arguably most famous in his own lifetime, his theory of gravitation, was for a long time considered as a competitor to Einstein's theory of general relativity which was published in 1915, after Nordström's theory. In 1914 Nordström introduced an additional space dimension to his theory, which provided coupling to electromagnetism. This was the first of the extra dimensional theories, which later came to be known as Kaluza–Klein theory. Kaluza and Klein, whose names are commonly used today for the theory, did not publish their work until the 1920s. Some speculations as to why Nordström's contribution fell into oblivion are that his theory was partly published in Swedish and that Einstein in a later publication referenced to Kaluza alone.[1] Today extra dimensions and theories thereof are widely researched, debated and even looked for experimentally.

Nordström's theory of gravitation was subsequently experimentally found to be inferior to Einstein's as it did not predict the bending of light which was observed during the solar eclipse in 1919.[2] However, Nordström and Einstein were in friendly competition or by some measure even cooperating scientists, not rivals. This can be seen from Nordström's public admiration of Einstein's work, as demonstrated by the two occasions on which Nordström nominated Einstein for the Nobel prize in physics for his theory of relativity.[1] Einstein never received the Nobel prize for the theory, as the first experimental evidence presented in 1919 could at the time still be disputed and there was not yet a consensus or even general understanding in the scientific community of the complex mathematical models that Einstein, Nordström and others had developed. Nordström's scalar theory is today mainly used as a pedagogical tool when learning general relativity.[5]

Today there is a limited public knowledge of Nordström's contributions to science even in Finland.[2] However, after his death a number of Finnish physicists and mathematicians devoted their time to the theory of relativity and differential geometry presumably due to the legacy he left. On the other hand, the most notable opponent of general relativity in the Finnish scientific world was Hjalmar Mellin, the previous rector of the Helsinki University of Technology where Nordström held professorship.[4]

Death

Nordström died in December 1923, at the age of 42, from pernicious anemia. The illness was perhaps caused by exposure to radioactive substances. Nordström was known to be interested in radioactivity, and a firm adherent to the then-widespread misconception that radioactivity was beneficial for one's health. Among his publications there is one from 1913 regarding the measurement of the radioactive emancipation power of different springs and ground waters in Finland.[1][2] Nordström was known for experimenting with radioactive substances[1] and for enjoying the Finnish sauna tradition using water from a spring rich in radium.[4]

Selected publications

During Nordström's career he published 34 articles and research papers in languages including German, Dutch, Finnish, and his mother-tongue Swedish. Nordström is probably the first person to write about the theory of relativity in the languages of Finland.

See also

External links

References

  1. 1 2 3 4 5 6 eva isaksson – suomalainen Einstein: painovoiman teoriaa 1910-luvulla http://www.helsinki.fi/~eisaksso/nordstrom/gunnar.html
  2. 1 2 3 4 5 Raimo Keskinen (1981): Gunnar Nordström 1881B1923. Arkhimedes 2/1981, s. 71B84. In Finnish, excerpt http://www.tieteessatapahtuu.fi/797/KESKINEN.pdf
  3. 1 2 http://www.helsinki.fi/keskusarkisto/virkamiehet_2/H-O.pdf – List of faculty at the university of Helsinki, Helsinki University Central archive. (I have chosen to use this source when conflicting information was available in less official sources, mainly regarding graduation years)
  4. 1 2 3 Totuuden nimessä: Kaksitoista merkittävää Suomen Tiedeseuran jäsentä (In the name of truth: twelve important members of the Finnish society of science), pages 173–176
  5. ↑ John D. Norton – some lesser known thought experiments in gravitation. http://www.pitt.edu/~jdnorton/papers/einstein-nordstroem-HGR3.pdf
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