-----Original Message----- From: [email protected] In reply to Harry Veeder's message:
>"Neutron and gamma continuous recording in ST >lab. No difference for spectra during experiments >showing extra heat and background" >Does this mean they did not detect any anomalous gamma or neutrons emissions? >If so then it is more evidence that the Celani doesn't produce excess heat. RvS: > It's still possible that any putative excess heat is either non nuclear, or a form of nuclear that doesn't produce gammas and doesn't rely on neutrons. Or ... both, depending on semantics. In fact, the vast majority of nuclear reactions in stars do not produce gammas or neutrons. 99.9999+ % of all stellar nuclear reactions consist of only a single reversible reaction. It can be called reversible proton fusion (RPF), and has been generally ignored by science. Due to the short lifetime of the new nucleus, it is confusing to use the word "fusion" at all. Two protons temporarily bind to helium-2 (aka the diproton) and then, after a tiny delay, the reaction reverses. Only rarely does anything else happen. The Pauli exclusion principle tells us that two identical fermions - particles with half-integer spin like protons - have a combined wave function that is anti-symmetric with respect to exchange of the particles and cannot really fuse (with one extremely rare exception - which is why the sun can eventually produce heat in a very slow burn). http://en.wikipedia.org/wiki/Proton%E2%80%93proton_chain_reaction "In the Sun, deuterium-producing events are rare (diprotons, the much more common result of nuclear reactions within the star, immediately decay back into two protons)...." In short, almost all stellar fusion in reversible and it is likely that this proton reaction happens in condensed matter as well. RPF always produces quantum color change in quarks, due to same wave function incompatibility - which can be exothermic or endothermic. It is possible that some solar heat derives from this mechanism. RPF apparently occurs in Casimir cavities or within a metal matrix in an earthly environment, and it seems from all of these Ni-H experiments going back to 1991, that the process can be engineered to be exothermic with no gammas. This is a strong working hypothesis for Ni-H energy gain. It involves excess heat, no gammas and no neutrons. Average proton mass is depleted. Color change is coupled to the matrix via magnons. Jones
