Ginzburg’s “Physical
Minimum” at the beginning of the XXI century
By Dr. Muhter Ahat
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Alexei A. Abrikosov Argonne National Laboratory Argonne, IL, USA Born 1928 |
Vitaly L. Ginzburg P.N. Lebedev Physical Institute Moscow, Russia Born 1916 |
Anthony J. Leggett University of Illinois Urbana, IL, USA Born 1938 |
The 2003 Noble prize in physics was shared by A. A. Abrikosov, Vitaly
L. Ginzburg, and Anthony J. Leggett. The prize was awarded to their
contributions in understanding of superconductivity and superfluidity. According
to the tradition of Noble Prize, each winner will give a talk and it is called
“Noble Lecture”.
Vintly L. Ginzburg, 87 years old, is from the Lebedev Physical Institute of the
Academy of Science, Russia. In his lecture, he outlined what he has been done,
how he collaborated with Landau and others, how important were their
contributions in the theory of superconductivity. More interestingly, he raised
questions for younger generations. He comes up with the excellent ideas and
categorizes the major issues in physics. He called it: “Physical Minimum” at the
beginning of the XXI century. Here is his list of “Physical Minimum”:
1. Controlled nuclear fusion.
2. High-temperature and room-temperature superconductivity.
3. Metallic hydrogen. Other exotic substances.
4. Two-dimensional electron liquids, the anomalous Hall effect and other
effects.
5. Some questions of solid-state physics heterostructures in
semiconductors, quantum wells and dots, metal-dielectric transitions, charge-
and spin density waves, mesoscopics.
6. Second-order and related phase transitions. Some examples of such
transitions. Cooling sin particular, laser cooling to superlow temperatures.
Bose-Einstein condensation in gases.
7. Surface physics, Clusters.
8. Liquid crystals, Ferroelectrics, Ferrotoroics.
9. Fullerenes, Nanotubes.
10. The behavior of matter in superstrong magnetic fields.
11. Nonlinear physics. Turbulence, Solitons, Chaos, Strange attractors.
12. X-ray lasers, gamma-ray lasers, superhigh-power lasers.
13. Superheavy elements, Exotic nuclei.
14. Mass spectrum, Quarks and gluons, Quantum chromodynamics, Quark-gluon
plasma.
15. Unified theory of weak and electromagnetic interactions, W± and Z0
bosons, Leptons.
16. Standard Model, Grand unification, Superunification. Proton decay,
Neutrino mass. Magnetic monopoles.
17. Fundamental length, Particle interaction at high and superhigh
energies, Colliders.
18. Nonconservation of CP invariance.
19. Nonlinear phenomena in vacuum and in superstrong magnetic fields,
Phase transitions in a vacuum.
20. Strings, M theory.
21. Experimental verification of the general theory of relativity.
22. Gravitational waves and their detection.
23. The cosmological problem, Inflation, The L term and “quintessence.”
Relationship between cosmology and high-energy physics.
24. Neutron stars and pulsars, Supernova stars.
25. Black holes, Cosmic strings.
26. Quasars and galactic nuclei, Formation of galaxies.
27. The problem of dark matter hidden mass and its detection.
28. The origin of superhigh-energy cosmic rays.
29. Gamma-ray bursts, Hypernovae.
30. Neutrino physics and astronomy, Neutrino oscillations.
As you noted this is very interesting and very helpful, especially, if you want
to pursue a higher degree in physics, it will be a good starting, it may help
you find right field for study. The original article is published in:
“Reviews of Modern Physics", Volume 76, July 2004, page: 981-998.