Authors: Akito Takahashi
As a model mechanism to explain anomalous excess heat results observed by nano-Ni-H systems, the weak-strong (WS) fusion rate estimation during the unresolved effective life time of end state for the 4H/TSC condensation/collapse motion is of key issue. The effective life of collapsed end state on the order of 1 fs is expected. Computer simulation study was done in this work using the HME-Langevin program, using several key conditions as time-dependent TSC trapping potential, fix-up at 2.4 fm p-p distance of proton hard core collision, and the DDL (deep Dirac level) component effect by relativistic motion of electrons. Computer simulation generated chaotic oscillation of p-p distance of 4H/TSC in the range of 3-100 fm, behaving as near stable (strange attractor) lasting for rather long time ( a few fs or more may be expected).
Comments: 25 Pages. Preprint of draft paper to JCF16 Proceedings
Unique-IP document downloads: 175 times
Vixra.org is a pre-print repository rather than a journal. Articles hosted may not yet have been verified by peer-review and should be treated as preliminary. In particular, anything that appears to include financial or legal advice or proposed medical treatments should be treated with due caution. Vixra.org will not be responsible for any consequences of actions that result from any form of use of any documents on this website.
Add your own feedback and questions here:
You are equally welcome to be positive or negative about any paper but please be polite. If you are being critical you must mention at least one specific error, otherwise your comment will be deleted as unhelpful.