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Igor Tamm

Igor Tamm is a astronomy topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand Igor Tamm rather than just read about it. In short: Igor Yevgenyevich Tamm (Russian: И́горь Евге́ньевич Тамм; 8 July 1895 – 12 April 1971) was a Soviet physicist who received the 1958 Nobel Prize in Physics, jointly with Pavel Cherenkov and Ilya Frank, for their 1934 discovery and demonstration of Cherenkov radiation. He also predicted the quasi-particle of sound: the phonon; and in 1951, together with Andrei Sakharov, proposed the Tokamak system.

Igor Tamm — main illustration
Igor Tamm — illustration

Key takeaways

  • Igor Tamm belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect Igor Tamm to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Igor Tamm from memory before moving on to harder problems.

Reference excerpt

Igor Yevgenyevich Tamm (Russian: И́горь Евге́ньевич Тамм; 8 July 1895 – 12 April 1971) was a Soviet physicist who received the 1958 Nobel Prize in Physics, jointly with Pavel Cherenkov and Ilya Frank, for their 1934 discovery and demonstration of Cherenkov radiation. He also predicted the quasi-particle of sound: the phonon; and in 1951, together with Andrei Sakharov, proposed the Tokamak system.

Biography

Igor Tamm was born in 1895 in Vladivostok into the family of Eugene Tamm, a civil engineer, and his wife Olga Davydova. According to Russian sources, Tamm had German noble descent on his father's side through his grandfather Theodor Tamm, who emigrated from Thuringia. Although his surname "Tamm" is rather common in Estonia, other sources state he was Jewish or had Jewish ancestry. He studied at a gymnasium in Elisavetgrad (now Kropyvnytskyi, Ukraine). In 1913–1914 he studied at the University of Edinburgh together with his school-friend Boris Hessen. At the outbreak of World War I in 1914 he joined the army as a volunteer field medic. In 1917 he joined the Revolutionary movement and became an active anti-war campaigner, serving on revolutionary committees after the March Revolution. He returned to the Moscow State University from which he graduated in 1918. Tamm married Nataliya Shuyskaya (1894–1980) in September 1917. Shе belonged to a noble Rurikid Shuysky family. They eventually had two children, Irina (1921–2009, chemist) and Evgeny (1926–2008, experimental physicist and famous mountain climber, leader of the Soviet Everest expedition in 1982). On 1 May 1923, Tamm began teaching physics at the Second Moscow State University. The same year, he finished his first scientific paper, Electrodynamics of the Anisotropic Medium in the Special Theory of Relativity. In 1928, he spent a few months with Paul Ehrenfest at the University of Leiden and made a life-long friendship with Paul Dirac. From 1934 until his death in 1971 Tamm was the head of the theoretical department at Lebedev Physical Institute in Moscow. In 1932, Tamm published a paper with his proposal of the concept of surface states. This concept is important for metal–oxide–semiconductor field-effect transistor (MOSFET) physics. In 1934, Tamm and Semen Altshuller suggested that the neutron has a non-zero magnetic moment, the idea was met with scepticism at that time, as the neutron was supposed to be an elementary particle with zero charge, and thus could not have a magnetic moment. The same year, Tamm coined an idea that proton-neutron interactions can be described as an exchange force transmitted by a yet unknown massive particle, this idea was later developed by Hideki Yukawa into a theory of meson forces. In 1945 he developed an approximation method for many-body physics. As Sidney Dancoff developed it independently in 1950, it is now called the Tamm-Dancoff approximation. He was the Nobel Laureate in Physics for the year 1958 together with Pavel Cherenkov and Ilya Frank for the discovery and the interpretation of the Cherenkov-Vavilov effect. In late 1940s to early 1950s Tamm was involved in the Soviet thermonuclear bomb project; in 1949–1953 he spent most of his time in the "secret city" of Sarov, working as a head of the theoretical group developing the hydrogen bomb, however he retired from the project and returned to the Moscow Lebedev Physical Institute after the first successful test of a hydrogen bomb in 1953. In 1951, together with Andrei Sakharov, Tamm proposed a tokamak system for the realization of controlled thermonuclear fusion on the basis of toroidal magnetic thermonuclear reactor and soon after the first such devices were built by the INF. Results from the T-3 Soviet magnetic confinement device in 1968, when the plasma parameters unique for that time were obtained, showed temperatures in their machine to be over an order of magnitude higher than what was expected by the rest of the community. The western scientists visited the experiment and verified the high temperatures and confinement, sparking a wave of optimism for the prospects of the tokamak as well as construction of new experiments, which is still the dominant magnetic confinement device today. In 1964 he was elected a Member of the German Academy of Sciences Leopoldina. Tamm was a student of Leonid Isaakovich Mandelshtam in science and life. Tamm was an atheist. Tamm died in Moscow, Soviet Union on 12 April 1971, the Lunar crater Tamm is named after him. He is buried at Novodevichy Cemetery.

References

Further reading

L. I. Mandelshtam, I. E. Tamm "The uncertainty relation between energy and time in nonrelativistic quantum mechanics", Izv. Akad. Nauk SSSR (ser. fiz.) 9, 122–128 (1945). English translation: J. Phys. (USSR) 9, 249–254 (1945).

External links Igor Tamm on Nobelprize.org including his Nobel Lecture, 11 December 1958 General Characteristics of Radiation Emitted by Systems Moving with Super-Light Velocities with Some Applications to Plasma Physics Igor Tamm on INSPIRE-HEP

Illustrations

Igor Tamm illustration
Igor Tamm: Tamm on the 2000 Russian stamp "Idea of phonons, 1929"
Tamm on the 2000 Russian stamp "Idea of phonons, 1929"

Worked examples

Example 1 — a first encounter with Igor Tamm

Start with the simplest possible case. Write down what Igor Tamm claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In astronomy, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to Igor Tamm before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about Igor Tamm ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of Igor Tamm

In research
Igor Tamm appears in astronomy research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses Igor Tamm in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
Igor Tamm is common in secondary-school and first-year university syllabi. It links to neighbouring topics 1895 births, 1971 deaths, Academic staff of Moscow State Pedagogical University, so understanding it makes those chapters shorter.
In everyday life
Look for Igor Tamm outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.
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How to study Igor Tamm in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Igor Tamm means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain Igor Tamm out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Igor Tamm in simple terms?

Igor Yevgenyevich Tamm (Russian: И́горь Евге́ньевич Тамм; 8 July 1895 – 12 April 1971) was a Soviet physicist who received the 1958 Nobel Prize in Physics, jointly with Pavel Cherenkov and Ilya Frank, for their 1934 discovery and demonstration of Cherenkov radiation. He also predicted the quasi-par…

Why does Igor Tamm matter?

Because it connects several astronomy ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study Igor Tamm?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on Igor Tamm.

Tags

  • 1895 births
  • 1971 deaths
  • Academic staff of Moscow State Pedagogical University
  • Academic staff of Moscow State University
  • Academic staff of the Moscow Institute of Physics and Technology
  • Alumni of the University of Edinburgh
  • Experimental physicists
  • Full Members of the USSR Academy of Sciences
  • Heroes of Socialist Labour
  • Members of the German National Academy of Sciences Leopoldina
  • Moscow State University alumni
  • Nobel laureates in Physics

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