Significance for the EPR Argument of the Neutron Synthesis from Hydrogen and of a New Controlled Nuclear Fusion without Coulomb Barrier

2021 ◽  
Author(s):  
Simone Beghella Bartoli
Keyword(s):  
Coulomb Barrier ◽  
Nuclear Fusion ◽  
Epr Argument

Nuclear Fusion in Stars

2018 ◽  
Author(s):  
Prasenjit Saha ◽  
Paul A. Taylor
Keyword(s):  
General Principle ◽  
Coulomb Barrier ◽  
Nuclear Reactions ◽  
Nuclear Fusion ◽  
Relative Speed ◽  
Quantum Tunnelling ◽  
Analytic Approximations ◽  
The Many ◽  
Potential Interactions

This chapter enumerates some of the many nuclear reactions in stars. It focuses on a general principle: nuclear fusion requires overcoming the Coulomb barrier between nuclei, which is possible through the relatively infrequent process of quantum tunnelling. The tunnelling probability depends on the atomic num-bers and mass numbers of the nuclei involved, and also on their relative speed. These translate into steep and interesting temperature dependencies for nuclear reactions. Analytic approximations yield a rate that is almost vanishingly rare, yet within the incredibly large number of potential interactions within stars quantum tunnelling can still provide the underlying ignition of nuclear reactions.

Neutrinos reveal final secret of Sun’s nuclear fusion

Nature ◽  
2020 ◽  
Vol 583 (7814) ◽  
pp. 20-21
Author(s):  
Davide Castelvecchi
Keyword(s):  
Nuclear Fusion

Status of muon catalysis of nuclear fusion reactions

1990 ◽  
Vol 160 (8) ◽  
pp. 47-103 ◽  
Author(s):  
Leonid I. Men'shikov ◽  
L.N. Somov
Keyword(s):  
Nuclear Fusion ◽  
Fusion Reactions ◽  
Nuclear Fusion Reactions ◽  
Muon Catalysis

BUBBLE NUCLEAR FUSION TECHNOLOGY-STATUS AND CHALLENGES

2005 ◽  
Vol 17 (3) ◽  
pp. 191-224 ◽  
Author(s):  
R. P. Taleyarkhan ◽  
Richard T. Lahey, Jr. ◽  
Academician R. I. Nigmatulin
Keyword(s):  
Nuclear Fusion ◽  
Fusion Technology
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