Jean Baptiste Perrin

Jean Baptiste Perrin
Perrin in 1926
Born	(1870-09-30)30 September 1870 Lille, France
Died	17 April 1942(1942-04-17) (aged 71) New York City, U.S.
Nationality	French
Alma mater	École Normale Supérieure University of Paris
Known for	Nature of cathode rays Brownian motion Avogadro constant Sedimentation equilibrium Perrin friction factors
Children	Francis Perrin
Awards	Matteucci Medal (1911) Fellow of the Royal Society (1918) Nobel Prize in Physics (1926)
Scientific career
Fields	Physics
Institutions	École Normale Supérieure University of Paris
Signature

Jean Baptiste Perrin ForMemRS^[1] (30 September 1870 – 17 April 1942) was a French physicist who, in his studies of the Brownian motion of minute particles suspended in liquids (sedimentation equilibrium), verified Albert Einstein's explanation of this phenomenon and thereby confirmed the atomic nature of matter. For this achievement he was honoured with the Nobel Prize in Physics in 1926.^[2]

Born in Lille, France, Perrin attended the École Normale Supérieure, the elite grande école in Paris. He became an assistant at the school during the period of 1894–97 when he began the study of cathode rays and X-rays. He was awarded the degree of docteur ès sciences (beyond PhD) in 1897. In the same year he was appointed as a lecturer in physical chemistry at the Sorbonne, Paris. He became a professor at the University in 1910, holding this post until the German occupation of France during World War II.

In 1895, Perrin showed that cathode rays were of negative electric charge in nature. He determined the Avogadro constant by several methods. He explained solar energy as due to the thermonuclear reactions of hydrogen.

In 1901 he proposed a hypothesis that each atom might have a positively charged nucleus, similarly to Hantaro Nagaoka later, but never developed it further.^[3] It came to be known the Rutherford model.

By mid 1900s, Perrin was interested in statistical mechanics questions, which are close to the study of Brownian motion.^[4] Following Albert Einstein's publication (1905) of a theoretical explanation of Brownian motion in terms of atoms, Perrin (along with Joseph Ulysses Chaudesaigues who was working in Perrin's lab) did the experimental work to test and verify Einstein's predictions, thereby providing data that would settle the century-long dispute about John Dalton's atomic theory, before the end of the decade.^[5][6][4] Carl Benedicks argued Perrin should receive the Nobel Prize in Physics; Perrin received the award in 1926 for this and other work on the discontinuous structure of matter, which put a definite end to the long struggle regarding the question of the physical reality of molecules.^[7]

Perrin was the author of a number of books and dissertations. Most notable of his publications were: "Rayons cathodiques et rayons X"; "Les Principes"; "Electrisation de contact"; "Réalité moléculaire"; "Matière et Lumière"; "Lumière et Reaction chimique".

Perrin was also the recipient of numerous prestigious awards including the Joule Prize of the Royal Society in 1896 and the La Caze Prize of the French Academy of Sciences. He was twice appointed a member of the Solvay Committee at Brussels in 1911 and in 1921. He also held memberships with the Royal Society of London and with the Academies of Sciences of Belgium, Sweden, Turin, Prague, Romania and China. He became a Commander of the Legion of Honour in 1926 and was made Commander of the Order of Léopold (Belgium).

In 1919, Perrin proposed that nuclear reactions can provide the source of energy in stars. He realized that the mass of a helium atom is less than that of four atoms of hydrogen, and that the mass-energy equivalence of Einstein implies that the nuclear fusion (4 H → He) could liberate sufficient energy to make stars shine for billions of years.^[8] A similar theory was first proposed by American chemist William Draper Harkins in 1915.^[9][10] It remained for Hans Bethe and Carl Friedrich von Weizsäcker to determine the detailed mechanism of stellar nucleosynthesis during the 1930s.^[11]

In 1927, he founded the Institut de Biologie Physico-Chimique together with chemist André Job and physiologist André Mayer. Funding was provided by Edmond James de Rothschild.^[12] In 1937, Perrin established the Palais de la Découverte, a science museum in Paris.

Perrin is considered the founding father of the National Centre for Scientific Research (Centre National de la Recherche Scientifique (CNRS)). Following a petition by Perrin signed by over 80 scientists, among them eight Nobel Prize laureates, the French education minister set up the Conseil Supérieur de la Recherche Scientifique (French National Research Council) in April 1933. In 1936, Perrin, now an undersecretary for research, founded the Service Central de la Recherche Scientifique (French Central Agency for Scientific Research).^[12] Both institutions were merged under the CNRS umbrella on October 19, 1939.^[13]

His notable students include Pierre Victor Auger. Jean Perrin was the father of Francis Perrin, also a physicist.^[14]

Perrin was an atheist and a socialist.^[15][16] He was an officer in the engineer corps during World War I.

After the death of Perrin's wife Henriette in 1938, Nine Choucroun (1896–1978), founder of the Nine Choucroun Prize, became Perrin's partner. In June 1940, when the Germans invaded France, Choucroun and Perrin escaped to Casablanca on the ocean liner Massilia, with part of the French government. In December 1941, they boarded the SS Excambion to New York City, arriving on December 23.^[17]

Perrin died at Mount Sinai Hospital in New York on 17 April 1942 at the age of 71.

After the War, in 1948, his remains were transported back to France by the cruiser Jeanne d'Arc and buried in the Panthéon.

Wikimedia Commons has media related to Jean Perrin.

• Jean Baptiste Perrin on Nobelprize.org
• Works by or about Jean Baptiste Perrin at the Internet Archive
• Mouvement brownien et molécules, by Jean Perrin, 1923 on Vidéothèque du CNRS (French)
• Jean Perrin et la réalité moléculaire on Vidéothèque du CNRS (French)