Alexander Friedmann

From Wikipedia, the free encyclopedia
This article is about the Russian cosmologist. For the Russian astrophysicist, see Alexei Fridman. For the Polish Orthodox Jewish rabbi, see Alexander Zusia Friedman.
In this Eastern Slavic naming convention, the patronymic is Alexandrovich and the family name is Friedmann.
Alexander Friedmann
Aleksandr Fridman.png
Alexander Friedmann
Born
Alexander Alexandrovich Friedmann

(1888-06-16)June 16, 1888
Saint Petersburg, Russian Empire
DiedSeptember 16, 1925(1925-09-16) (aged 37)
Leningrad, USSR
NationalityRussian
Alma materSt. Petersburg State University
Known for
Spouse(s)Natalia Malinina
Scientific career
FieldsMathematics and physics
InstitutionsPetrograd Polytechnical Institute
Main Geophysical Observatory
Doctoral advisorVladimir Steklov
Doctoral students
Signature
Aleksandr Fridman signature.png
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Alexander Alexandrovich Friedmann (also spelled Friedman or Fridman /ˈfriːdmən/; Russian: Алекса́ндр Алекса́ндрович Фри́дман) (June 16 [O.S. 4], 1888 – September 16, 1925) was a Russian and Soviet physicist and mathematician. He is best known for his pioneering theory that the universe was expanding, governed by a set of equations he developed now known as the Friedmann equations.

Early life[]

Alexander Friedmann was born to the composer and ballet dancer Alexander Friedmann (who was a son of a baptized Jewish cantonist) and the pianist Ludmila Ignatievna Voyachek (who was a daughter of the Czech composer Hynek Vojáček).[1] Friedmann was baptized into the Russian Orthodox Church as an infant, and lived much of his life in Saint Petersburg.

Friedmann obtained his degree from St. Petersburg State University in 1910, and became a lecturer at Saint Petersburg Mining Institute.

From his school days, Friedmann found a lifelong companion in Jacob Tamarkin, who was also a distinguished mathematician.[2]

World War I[]

Friedmann fought in World War I on behalf of Imperial Russia, as an army aviator, an instructor and eventually, under the revolutionary regime, as the head of an airplane factory.[3]

Professorship[]

Friedmann in 1922 introduced the idea of an expanding universe that contained moving matter. Correspondence with Einstein suggests that Einstein was unwilling to accept the idea of an evolving Universe and worked instead to modify his equations to ensure a static eternal Universe as believed from Newton's time. Some years later, in 1926 Hubble published the redshift vs distance relationship, namely, all the galaxies in the neighborhood seemed to be receding at a rate proportional to their distance, formalising an observation made earlier by Carl Wilhelm Wirtz. It may be noted that in 1927 Belgian astronomer Georges Lemaître also independently reached the conclusion of an evolving Universe.[4]

In June 1925 Friedmann was given the job of the director of Main Geophysical Observatory in Leningrad. In July 1925 he participated in a record-setting balloon flight, reaching the elevation of 7,400 m (24,300 ft).[5]

Work[]

Relativity[]

Friedmann's 1924 papers, including "Über die Möglichkeit einer Welt mit konstanter negativer Krümmung des Raumes" ("On the possibility of a world with constant negative curvature of space") published by the German physics journal Zeitschrift für Physik (Vol. 21, pp. 326–332), demonstrated that he had command of all three Friedmann models describing positive, zero and negative curvature respectively, a decade before Robertson and Walker published their analysis.

This dynamic cosmological model of general relativity would come to form the standard for both the Big Bang and Steady State theories. Friedmann's work supports both theories equally, so it was not until the detection of the cosmic microwave background radiation that the Steady State theory was abandoned in favor of the current favorite Big Bang paradigm.

The classic solution of the Einstein field equations that describes a homogeneous and isotropic universe is called the Friedmann–Lemaître–Robertson–Walker metric, or FLRW, after Friedmann, Georges Lemaître, Howard P. Robertson and Arthur Geoffrey Walker, who worked on the problem in 1920s and 30s independently of Friedmann.

Hydrodynamics and meteorology[]

In addition to general relativity, Friedmann's interests included hydrodynamics and meteorology.

Students[]

Physicists George Gamow, Vladimir Fock and Lev Vasilievich Keller[5] were among his students.

Personal life[]

In 1911, he married Ekaterina Dorofeeva, though he later divorced her. He married Natalia Malinina in 1923. They had a religious wedding ceremony, though both were far from religious.[6]

Death[]

Friedmann died on September 16, 1925 from misdiagnosed typhoid fever. He had allegedly contracted the bacteria on his way back from his honeymoon in Crimea when he ate an unwashed pear he bought from a railway station.[7]

Named after Friedmann[]

The moon crater Fridman is named after him [8]

Alexander Friedmann International Seminar[]

Alexander Friedmann International Seminar is a periodical scientific event. The objective of the meeting is to promote contacts between scientists working in the field of Relativity, Gravitation and Cosmology and related fields. The First Alexander Friedmann International Seminar on Gravitation and Cosmology devoted to the centenary of his birth took place in 1988.

Selected publications[]

  • Friedman, A. (1922). "Über die Krümmung des Raumes". Zeitschrift für Physik. 10 (1): 377–386. Bibcode:1922ZPhy...10..377F. doi:10.1007/BF01332580. S2CID 125190902.. English translation in: Friedman, A. (1999). "On the curvature of space". General Relativity and Gravitation. 31 (12): 1991–2000. Bibcode:1999GReGr..31.1991F. doi:10.1023/A:1026751225741. S2CID 122950995. The original Russian manuscript of this paper is preserved in the Ehrenfest archive, together with some letters and unpublished work.
  • Friedman, A. (1924). "Über die Möglichkeit einer Welt mit konstanter negativer Krümmung des Raumes". Zeitschrift für Physik. 21 (1): 326–332. Bibcode:1924ZPhy...21..326F. doi:10.1007/BF01328280. S2CID 120551579.. English translation in: Friedmann, A. (1999). "On the Possibility of a World with Constant Negative Curvature of Space". General Relativity and Gravitation. 31 (12): 2001–2008. Bibcode:1999GReGr..31.2001F. doi:10.1023/A:1026755309811. S2CID 123512351.

References[]

  1. ^ Hassani, Sadri (2013). Mathematical Physics: A Modern Introduction to Its Foundations. Springer Science+Business Media. ISBN 9783319011950. Retrieved May 22, 2021.
  2. ^ Pyenson L. Book review. Physics Today [serial online]. September 1994; 47(9):93. Available from: MasterFILE Premier, Ipswich, MA. Accessed October 18, 2012.
  3. ^ Pyenson L. Book review. Physics Today [serial online]. September 1994;47(9):93. Available from: MasterFILE Premier, Ipswich, MA. Accessed October 18, 2012.
  4. ^ Daintith J. Dictionary Of Scientists [e-book]. Oxford University Press; 1999. Available from: eBook Collection (EBSCOhost), Ipswich, MA. Accessed October 18, 2012.
  5. ^ Jump up to: a b Davidson et al., A Voyage Through Turbulence, Cambridge University Press, ISBN 9780521149310, September 2011 (for a partial and legal excerpt of the book, see: [1])
  6. ^ Eduard A. Tropp; Viktor Ya. Frenkel; Artur D. Chernin (2006). "The final year". Alexander A Friedmann: The Man who Made the Universe Expand. Cambridge University Press. p. 209. ISBN 9780521025881. [Alexander Friedmann and Natalia Malinina] even had a religious wedding ceremony in the Crimea, though both were far from religious. “Just to make it stronger,” Friedmann said to his wife (she told this to her sister Sofia).
  7. ^ Френкель, Виктор Яковлевич (1988-07-01). "Александр Александрович Фридман (Биографический очерк)". Успехи физических наук (in Russian). 155 (7): 481–516. ISSN 0042-1294.
  8. ^ Menzel, D. H. (1971). "Report on Lunar Nomenclature by The Working Group of Commission 17 of the IAU". Space Science Reviews. 12 (2): 136–186. Bibcode:1971SSRv...12..136M. doi:10.1007/BF00171763. S2CID 122125855.

Bibliography[]

External links[]

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