scholarly journals Magnetic Fields And High-Temperature Superconductivity In Excited Liquids. Unknown Particles

2021 ◽  
Vol 13 (3) ◽  
pp. 303-318
Author(s):  
Gennady V. Mishinsky ◽  
Keyword(s):  
Magnetic Fields ◽  
Electric Current ◽  
Nuclear Reactions ◽  
High Temperature Superconductivity ◽  
Chemical Elements ◽  
Liquid Media ◽  
Strong Magnetic Fields ◽  
Atomic Nuclei ◽  
Self Consistent Field ◽  
Unidirectional Motion

The article presents a number of experiments in liquid media on the transformation (transmutation) of atomic nuclei of some chemical elements into atomic nuclei of other chemical elements. In the theory of low-energy nuclear reactions, the transmutation of atomic nuclei occurs in strong magnetic fields, more than 30 T. Magnetic fields appear in ionized liquid media as a result of the unidirectional motion of an ensemble of electrons. The exchange interaction between electrons with parallel spins forms a self-consistent field in the medium, in which electrons pair into orthobosons with S = 1ћ. Orthobosons are attracted to each other and form orthoboson “solenoids” - “capsules” with strong magnetic fields inside. “Capsules” can fly out of liquid media, and then they are registered as unknown particles with strange properties. In some cases, when an electric current passes through the liquid, the electric current can be realized in the form of orthobosonic “solenoids” connected in continuous “filaments” from one electrode to another. Such “filaments” exhibit characteristics of superconductivity.

Nuclear Processes Related to the Ap Stars and the Heaviest Chemical Elements

1976 ◽  
Vol 32 ◽  
pp. 169-182
Author(s):  
B. Kuchowicz
Keyword(s):  
Nuclear Physics ◽  
Nuclear Reactions ◽  
Chemical Elements ◽  
Fission Products ◽  
Abundance Pattern ◽  
Isotopic Shifts ◽  
Processed Material ◽  
R Process ◽  
Ap Stars ◽  
Nuclear Processes

SummaryIsotopic shifts in the lines of the heavy elements in Ap stars, and the characteristic abundance pattern of these elements point to the fact that we are observing mainly the products of rapid neutron capture. The peculiar A stars may be treated as the show windows for the products of a recent r-process in their neighbourhood. This process can be located either in Supernovae exploding in a binary system in which the present Ap stars were secondaries, or in Supernovae exploding in young clusters. Secondary processes, e.g. spontaneous fission or nuclear reactions with highly abundant fission products, may occur further with the r-processed material in the surface of the Ap stars. The role of these stars to the theory of nucleosynthesis and to nuclear physics is emphasized.

Strong magnetic fields

1960 ◽  
Vol 70 (4) ◽  
pp. 693-714 ◽  
Author(s):  
G.M. Strakhovskii ◽  
N.V. Kravtsov
Keyword(s):  
Magnetic Fields ◽  
Strong Magnetic Fields

Magnetic molecular nanoclusters in strong magnetic fields

2002 ◽  
Vol 172 (11) ◽  
pp. 1303 ◽  
Author(s):  
Anatolii K. Zvezdin ◽  
Viktor V. Kostyuchenko ◽  
V.V. Platonov ◽  
V.I. Plis ◽  
A.I. Popov ◽  
...  
Keyword(s):  
Magnetic Fields ◽  
Strong Magnetic Fields

scholarly journals The measurement of the energy of cosmic rays - II—The curvature measurements and the energy spectrum

1936 ◽  
Vol 154 (883) ◽  
pp. 573-587 ◽  
Keyword(s):  
Magnetic Field ◽  
Energy Spectrum ◽  
Cosmic Rays ◽  
Magnetic Fields ◽  
Strong Magnetic Fields ◽  
The Earth ◽  
Primary Particles ◽  
Curvature Measurements

Both the penetrating power of the cosmic rays through material ab­sorbers and their ability to reach the earth in spite of its magnetic field, make it certain that the energy of many of the primary particles must reach at least 10 11 e-volts. However, the energy measurements by Kunze, and by Anderson, using cloud chambers in strong magnetic fields, have extended only to about 5 x 10 9 e-volts. Particles of greater energy were reported, but the curvature of their tracks was too small to be measured with certainty. We have extended these energy measurements to somewhat higher energies, using a large electro-magnet specially built for the purpose and described in Part I. As used in these experiments, the magnet allowed the photography of tracks 17 cm long in a field of about 14,000 gauss. The magnet weighed about 11,000 kilos and used a power of 25 kilowatts.

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