Vadim Kuzmin (physicist)

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Vadim Alekseyevich Kuzmin
Vadim Alexeevich Kuzmin.jpg
Native nameВадим Алексеевич Кузьмин
Born(1937-04-16)16 April 1937
Moscow
Died 17 September 2015(2015-09-17) (aged 78)
Moscow
Education Moscow State University
Known for GZK limit
Scientific career
Institutions Institute for Nuclear Research

Vadim Alekseyevich Kuzmin (Russian : Вади́м Алексе́евич Кузьми́н; 16 April 1937 – 17 September 2015) was a Russian theoretical physicist.

Russian language East Slavic language

Russian is an East Slavic language, which is official in the Russian Federation, Belarus, Kazakhstan and Kyrgyzstan, as well as being widely used throughout Eastern Europe, the Baltic states, the Caucasus and Central Asia. It was the de facto language of the Soviet Union until its dissolution on 25 December 1991. Although, nowadays, nearly three decades after the breakup of the Soviet Union, Russian is used in official capacity or in public life in all the post-Soviet nation-states, as well as in Israel and Mongolia, the rise of state-specific varieties of this language tends to be strongly denied in Russia, in line with the Russian World ideology.

Contents

Biography

Kuzmin completed his undergraduate studies in 1961 at Moscow State University and his PhD in 1971 at Lebedev Institute. He has been a member of the Institute for Nuclear Research in Moscow since its founding in 1970. There, he became a professor and chair of the department of particle astrophysics and cosmology. In 1987, he obtained the Russian doctoral title.

Moscow State University university in Moscow, Russia

Moscow State University is a coeducational and public research university located in Moscow, Russia. It was founded on 23 January [O.S. 12 January] 1755 by Mikhail Lomonosov. MSU was renamed after Lomonosov in 1940 and was then known as Lomonosov University. It also houses the tallest educational building in the world. Its current rector is Viktor Sadovnichiy. According to the 2018 QS World University Rankings, it is the highest-ranking Russian educational institution and is widely considered the most prestigious university in the former Soviet Union.

Institute for Nuclear Research of the Russian Academy of Sciences is a Russian scientific research centre "for further development of the experimental base and fundamental research activities in the field of atomic nucleus, elementary particle and cosmic ray physics and neutrino astrophysics".

Cosmology academic study of the Universe

Cosmology is a branch of astronomy concerned with the studies of the origin and evolution of the universe, from the Big Bang to today and on into the future. It is the scientific study of the origin, evolution, and eventual fate of the universe. Physical cosmology is the scientific study of the universe's origin, its large-scale structures and dynamics, and its ultimate fate, as well as the laws of science that govern these areas.

In the 1980s, he was a pioneer in the theory of elektroweak baryogenesis. In 1985, his influential work with Valery Rubakov and Mikhail E. Shaposhnikov estimated the rate of anomalous electroweak process that violated baryon-number conservation in the cosmic plasma of the early universe. [1]

Baryogenesis hypothesized processes that could produce baryonic asymmetry, favoring matter (baryons) over antimatter (antibaryons)

In physical cosmology, baryogenesis is the hypothetical physical process that took place during the early universe that produced baryonic asymmetry, i.e. the imbalance of matter (baryons) and antimatter (antibaryons) in the observed universe.

In neutrino physics, he proposed an experiment using gallium/germanium detectors to detect solar neutrinos. In 1970, he proposed neutron/antineutron oscillations as a possibility for observing violation of baryon number.

Gallium Chemical element with atomic number 31

Gallium is a chemical element with symbol Ga and atomic number 31. It is in group 13 of the periodic table, and thus has similarities to the other metals of the group, aluminium, indium, and thallium. Gallium does not occur as a free element in nature, but as gallium(III) compounds in trace amounts in zinc ores and in bauxite. Elemental gallium is a soft, silvery blue metal at standard temperature and pressure, a brittle solid at low temperatures, and a liquid at temperatures greater than 29.76 °C (85.57 °F).

Germanium Chemical element with atomic number 32

Germanium is a chemical element with symbol Ge and atomic number 32. It is a lustrous, hard, grayish-white metalloid in the carbon group, chemically similar to its group neighbours silicon and tin. Pure germanium is a semiconductor with an appearance similar to elemental silicon. Like silicon, germanium naturally reacts and forms complexes with oxygen in nature.

Solar neutrino neutrinos produced in the core of the sun through various nuclear fusion reactions

Electron neutrinos are produced in the Sun as a product of nuclear fusion. Solar neutrinos constitute by far the largest flux of neutrinos from natural sources observed on Earth, as compared with e.g. atmospheric neutrinos or the diffuse supernova neutrino background.

In 1970, he independently discovered the Sakharov conditions.

In 1966, he and Georgiy Zatsepin predicted (what is now called) the GZK limit for cosmic rays. [2]

Georgiy Timofeyevich Zatsepin was a Soviet/Russian astrophysicist known for his works in cosmic rays physics and neutrino astrophysics. He was born in Moscow.

In 2000, he became a corresponding member of the Russian Academy of Sciences. In 2006, he received the Pomeranchuk Prize with Howard Georgi. In 2003, he received the Moisey Markov Prize.

Related Research Articles

Neutrino Elementary particle with very low mass that interacts only via the weak force and gravity

A neutrino is a fermion that interacts only via the weak subatomic force and gravity. The neutrino is so named because it is electrically neutral and because its rest mass is so small (-ino) that it was long thought to be zero. The mass of the neutrino is much smaller than that of the other known elementary particles. The weak force has a very short range, the gravitational interaction is extremely weak, and neutrinos, as leptons, do not participate in the strong interaction. Thus, neutrinos typically pass through normal matter unimpeded and undetected.

The Greisen–Zatsepin–Kuzmin limit (GZK limit) is a theoretical upper limit on the energy of cosmic ray protons traveling from other galaxies through the intergalactic medium to our galaxy. The limit is 5×1019 eV, or about 8 joules. The limit is set by slowing interactions of the protons with the microwave background radiation over long distances (~160 million light-years). The limit is at the same order of magnitude as the upper limit for energy at which cosmic rays have experimentally been detected. For example, one extreme-energy cosmic ray has been detected which appeared to possess a record 3.12×1020 eV (50 joules) of energy (about the same as the kinetic energy of a 95 km/h baseball).

In physics, a chiral anomaly is the anomalous nonconservation of a chiral current. In everyday terms, it is equivalent to a sealed box that contained equal number of positive and negative charged particles, that when opened was found to have more positive than negative particles, or vice versa.

Sphaleron

A sphaleron is a static (time-independent) solution to the electroweak field equations of the Standard Model of particle physics, and is involved in certain hypothetical processes that violate baryon and lepton numbers. Such processes cannot be represented by perturbative methods such as Feynman diagrams, and are therefore called non-perturbative. Geometrically, a sphaleron is a saddle point of the electroweak potential.

In physical cosmology, leptogenesis is the generic term for hypothetical physical processes that produced an asymmetry between leptons and antileptons in the very early universe, resulting in the present-day dominance of leptons over antileptons. In the currently accepted Standard Model, lepton number is conserved; it is not possible to create leptons directly without corresponding antileptons. Leptogenesis can therefore only take place in theories of physics beyond the Standard Model.

In physics, the baryon asymmetry problem, also known as the matter asymmetry problem or the matter-antimatter asymmetry problem, is the observed imbalance in baryonic matter and antibaryonic matter in the observable universe. Neither the standard model of particle physics, nor the theory of general relativity provides a known explanation for why this should be so, and it is a natural assumption that the universe be neutral with all conserved charges. The Big Bang should have produced equal amounts of matter and antimatter. Since this does not seem to have been the case, it is likely some physical laws must have acted differently or did not exist for matter and antimatter. Several competing hypotheses exist to explain the imbalance of matter and antimatter that resulted in baryogenesis. However, there is as of yet no consensus theory to explain the phenomenon. As remarked in a 2012 research paper, "The origin of matter remains one of the great mysteries in physics."

Astroparticle physics, also called particle astrophysics, is a branch of particle physics that studies elementary particles of astronomical origin and their relation to astrophysics and cosmology. It is a relatively new field of research emerging at the intersection of particle physics, astronomy, astrophysics, detector physics, relativity, solid state physics, and cosmology. Partly motivated by the discovery of neutrino oscillation, the field has undergone rapid development, both theoretically and experimentally, since the early 2000s.

Artem Isahaki (Isaakovich) Alikhanian was a Soviet Armenian physicist, one of the founders and first director of the Yerevan Physics Institute, a correspondent member of the Academy of Sciences of the USSR (1946), academic of the Armenian Academy of Sciences. With Pyotr Kapitsa, Lev Landau, Igor Kurchatov, Abraham Alikhanov and others, he laid the foundations of nuclear physics in the Soviet Union. He is known as the "father of Armenian physics".

The Pomeranchuk Prize is an international award for theoretical physics, awarded annually since 1998 by the Institute for Theoretical and Experimental Physics (ITEP) from Moscow. It is named after Russian physicist Isaak Yakovlevich Pomeranchuk, who together with Landau established the Theoretical Physics Department of the Institute.

Aleksandr Evgenievich Chudakov was a Soviet Russian physicist in the field of cosmic-ray physics, known for Chudakov Effect, the effect of decreasing ionization losses for narrow electron-positron pairs and for experimentally confirming existence of the transition radiation. He was also the chairman of the IUPAP Cosmic Ray Commission.

Moisey Alexandrovich Markov was a Soviet physicist-theorist who mostly worked in the area of quantum mechanics, nuclear physics and particle physics He is particularly known for having proposed the idea of underwater neutrino telescopes in 1960 that was originally developed in the master thesis of his student Igor Mikhailovich Zheleznykh.

The Affleck–Dine mechanism is a postulated mechanism for explaining baryogenesis during the primordial Universe immediately following the Big Bang. Thus, the AD mechanism may explain the asymmetry between matter and anti-matter in the current Universe. It was proposed in 1985 by Ian Affleck and Michael Dine of Princeton University.

The neutrino minimal standard model is an extension of the Standard Model of particle physics, by the addition of three right-handed neutrinos with masses smaller than the electroweak scale. Introduced by Takehiko Asaka and Mikhail Shaposhnikov in 2005., it has provided a highly constrained model for many topics in physics and cosmology, such as baryogenesis and neutrino oscillations.

Vladimir Lobashev Russian particle physicist

Vladimir Mikhailovich Lobashev was a Russian physicist and expert in nuclear physics and particle physics. He authored over 200 papers, of which 25 were considered groundbreaking.

Valery Rubakov Russian physicist

Valery Anatolyevich Rubakov is a Russian theoretical physicist. His scientific interests include quantum field theory, elementary particle physics, and cosmology. He is affiliated with the Institute for Nuclear Research (INR) of the Russian Academy of Sciences in Moscow.

References

  1. V. A. Kuzmin; V. A. Rubakov; M. E. Shaposhnikov (1985-05-16). "On anomalous electroweak baryon-number non-conservation in the early universe". Physics Letters B. 155 (1–2): 36–42. Bibcode:1985PhLB..155...36K. doi:10.1016/0370-2693(85)91028-7.
  2. Zatsepin, G. T.; Kuz'min, V. A. (1966). "Upper Limit of the Spectrum of Cosmic Rays" (PDF). Journal of Experimental and Theoretical Physics Letters. 4: 7880. Bibcode:1966JETPL...4...78Z.