Stjepan Mohorovičić
Stjepan Mohorovičić | |
|---|---|
 Portrait of Stjepan Mohorovičić | |
| Born | 20 August 1890 |
| Died | 13 February 1980 (aged 89) |
| Citizenship | Hungarian-Croatian (1890–1918) Croatian (1918–1945) Yugoslavian (1945–1980) |
| Alma mater | University of Zagreb |
| Known for | Discovering Positronium |
| Scientific career | |
| Fields | Physics, Geophysics, Meteorology |
Stjepan Mohorovičić (August 20, 1890 – February 13, 1980) was a Croatian physicist, geophysicist and meteorologist.
Biography[edit]
Mohorovičić was born in the town of Bakar.[1] His father was the world-famous geophysicist Andrija Mohorovičić. He studied mathematics and physics at the University of Zagreb where among others his professors were Vinko Dvořák and Andrija Mohorovičić, and later he studied at Göttingen where some of his professors were Arnold Sommerfeld, Woldemar Voigt and David Hilbert.[1] Later on he received a doctorate degree from the University of Zagreb. Mohorovičić was an opponent of Einstein's theory of relativity.[2] Because of his longtime opposition and criticisms of theory of relativity he remained a high school professor his whole life. His work went largely ignored, especially in Croatia. He died in Zagreb.[1]
Scientific work[edit]
His scientific interests included seismology, meteorology, astrophysics and theoretical physics. He began his career in seismology with his father. In 1913 he developed a new method for locating the hypocenter of an earthquake and gave an independent verification of discontinuity theory put forward by his father.[3] In 1916 he published an idea of the existence of smaller discontinuities in Earth's crust and mantle.[4] He put forward his own theory about the composition and the formation of the Moon,[5] explosive formation of lunar craters[6] and predicted the existence of Moho layer on the Moon.[7] The existence of Moho layer on the Moon was confirmed in 1969 by seismic measurements done by Apollo 11 crew.
Mohorovičić is often called "the father of positronium" because his most significant work is the prediction of the existence of positronium.[8] Positronium is the bound state of an electron and a positron and therefore the lightest atom. It was experimentally discovered in 1951 by Martin Deutsch and became known as positronium. Mohorovičić in his paper also calculated spectra of positronium and predicted the existence of positronium in stars because of which he suggested the identification of possible spectral lines of positronium in spectra of stars. He was searching for spectra of positronium in the sky, but unsuccessfully. Positronium lines were first identified in lab in 1975 by Canter et al. and in outer space in spectra of Crab Nebula in 1984 by J. E. McClintock.[9][10]
See also[edit]
References[edit]
- ^ a b c "Mohorovičić, Stjepan". arhinet.arhiv.hr (in Croatian). Croatian State Archives. Retrieved 2015-01-16.
- ^ Milena Wazeck (2009). Einstein's Opponents: The Public Controversy About the Theory of Relativity in the 1920s. Cambridge University Press. ISBN 978-1107017443.
- ^ S. Mohorovičić (1914). "Die reduzierte Laufzeitkurve und die Abhängigkeit der Herdtiefe eines Bebens von der Entfernung des Inflexionspunktes der primären Laufzeitkurve: I. Mitteilung: Die Ausbreitung der Erdbebenstrahlen in den obersten Schniten der Erde". Gerlands Beitr. Z. Geophysik. Vol. 13. pp. 217–240.
- ^ S. Mohorovičić (1916). "Die reduzierte Laufzeitkurve und die Abhängigkeit der Herdtiefe eines Bebens von der Entfernung des Inflexionspunktes der primären Laufzeitkurve: II. Mitteilung: Die Ausbreitung der Erdbebenstrahlen in den tiefen Schichten der Erde". Gerlands Beitr. Z. Geophysik. Vol. 14, no. 3. pp. 187–189.
- ^ S. Mohorovičić (1923). "Über die Konstitution des Erd- und Mondinnern". Astronomische Nachrichten. Vol. 220, no. 15. pp. 245–250.
- ^ S. Mohorovičić (1928). "Experimentalle Untersuchungen über die entstehung der Mondkrater: eineuer Beitrag zur. Explosionshypothes". Archiv za Hemiju i Farmaciju, Zagreb. Vol. 2. pp. 66–76.
- ^ S. Mohorovičić (1927). "Über Nahbeben und über Konstitution des Erd-und Mondinnern". Gerlands Beitr. Z. Geophysik. Vol. 17. pp. 180–231.
- ^ S. Mohorovičić (1934). "Möglichkeit neuer Elemente und ihre Bedeutung für die Astrophysik". Astronomische Nachrichten. 253 (4): 93–108. Bibcode:1934AN....253...93M. doi:10.1002/asna.19342530402.
- ^ K. F. Canter; A. P. Mills; S. Berko (1975). "Observations of Positronium Lyman-α Radiation". Phys. Rev. Lett. 34 (4): 177–180. Bibcode:1975PhRvL..34..177C. doi:10.1103/PhysRevLett.34.177.(Erratum: Phys. Rev. Lett. 34, 848 (1975))
- ^ J.E. McClintock (1984). "On The Detection Of Positrons Via The Optical Lines Of Positronium". Astrophys. J. 282: 291–295. Bibcode:1984ApJ...282..291M. doi:10.1086/162202.
External links[edit]
- Milan Randić (2009). "Positronium – Hydrogen Like and Unlike" (PDF). Croat. Chem. Acta. 82 (4): 791–800. Retrieved September 11, 2023.
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