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SUPER HEAVY ELEMENTS IN USABLE QUANTITIES
This project is part of our superluminal warp drive research. We believe that spending time and money in this direction is very important as we see the future of the humanity among the stars.
We are developing a technology to synthesize stable super heavy elements in usable quantities. We anticipate this elements to show some unique properties which can be utilized for space travel such as special relativity effects and change the curvature of space-time in exotic ways.
In nature all of the heavy elements are produced by nuclear fusion reactions, mostly in supernova explosions and neutron star collisions, so, this is to date the only known and proven mechanism to produce heavy elements in usable quantities.
In our research we have shown that the fusion of heavy elements, as the heaviest observationally stable element – 238U, is feasible, at least in principle with the help of existing technologies. And the fusion of lighter – than z = 184 – nuclei is conceptually viable examining the tunnel effect assisted by an auxiliary field that will produce a Sauter like effect, and this is the pathway to explore the synthesis of elements higher than z = 118. The production of theoretical untested elements like Unoctquadium-184 or close Z species could open a new chapter in the physics of super-heavy elements, and leads to a deeper understanding of nuclear decay channels and stability conditions. Nuclear fusion of heavy elements will open the breach to produce neutron rich elements, so we may obtain a deep insight into the physics of the island of stability.
In the article we published we also reviewed basic aspects of fusion physics related to the assisted fusion mechanism. An enhanced fusion perspective is found generalizing the work for space dependent fields and the cases of 2H, 106Pd and 238U are presented for several test fields. A final section reviewing laser confinement fusion actual experiments capable of achieving the required energies is also reported.
You can read more about that in the “Press and Research papers” section of the web site.
SUPER HEAVY ELEMENTS IN USABLE QUANTITIES
This project is part of our superluminal warp drive research. We believe that spending time and money in this direction is very important as we see the future of the humanity among the stars.
We are developing a technology to synthesize stable super heavy elements in usable quantities. We anticipate this elements to show some unique properties which can be utilized for space travel such as special relativity effects and change the curvature of space-time in exotic ways.
In nature all of the heavy elements are produced by nuclear fusion reactions, mostly in supernova explosions and neutron star collisions, so, this is to date the only known and proven mechanism to produce heavy elements in usable quantities.
In our research we have shown that the fusion of heavy elements, as the heaviest observationally stable element – 238U, is feasible, at least in principle with the help of existing technologies. And the fusion of lighter – than z = 184 – nuclei is conceptually viable examining the tunnel effect assisted by an auxiliary field that will produce a Sauter like effect, and this is the pathway to explore the synthesis of elements higher than z = 118. The production of theoretical untested elements like Unoctquadium-184 or close Z species could open a new chapter in the physics of super-heavy elements, and leads to a deeper understanding of nuclear decay channels and stability conditions. Nuclear fusion of heavy elements will open the breach to produce neutron rich elements, so we may obtain a deep insight into the physics of the island of stability.
In the article we published we also reviewed basic aspects of fusion physics related to the assisted fusion mechanism. An enhanced fusion perspective is found generalizing the work for space dependent fields and the cases of 2H, 106Pd and 238U are presented for several test fields. A final section reviewing laser confinement fusion actual experiments capable of achieving the required energies is also reported.
You can read more about that in the “Press and Research papers” section of the web site.