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PROPERTIES OF MATTER IN ULTRAHIGH MAGNETIC-FIELDS AND STRUCTURE OF THE SURFACE OF NEUTRON-STARS
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Physics.
1995 (English)In: USPEKHI FIZICHESKIKH NAUK, Vol. 165, no 2, 121-142 p.Article, book review (Other scientific) Published
Abstract [en]

The physical properties of atoms, molecules, and solids in ultrahigh magnrtic fields B much greater than 10(9) G, which are believed to exist on the surface of neutron stars, are discussed. In such magnetic fields atoms are strongly deformed and elongated

Place, publisher, year, edition, pages
MEZHDUNARODNAYA KNIGA , 1995. Vol. 165, no 2, 121-142 p.
Keyword [en]
PULSAR POLAR CAPS; THOMAS-FERMI THEORY; DENSITY-FUNCTIONAL CALCULATIONS; HARTREE-FOCK CALCULATIONS; HYDROGEN-ATOM; CONDENSED MATTER; GROUND-STATE; POTENTIAL DROPS; BINDING-ENERGY; BETA-DECAY
Identifiers
URN: urn:nbn:se:uu:diva-76899OAI: oai:DiVA.org:uu-76899DiVA: diva2:104811
Note
Addresses: LIBERMAN MA, RUSSIAN ACAD SCI, PL KAPITSA PHYS PROBLEMS INST, UL KOSYGINA 2, MOSCOW 117334, RUSSIA. UNIV UPPSALA, DEPT PHYS, S-75121 UPPSALA, SWEDEN.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-15

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