A lot of energy is required to setup the condensate of SPPs, but once the SPP condensate is in place, it is highly efficient because it recycles energy produced by the meson decay chain back into the SPP condensate. The energy loss comes from EMF production and the generation of electrons. Any energy from muon catalyzed fusion or pion or magnetic based nuclear disruption would find it way into the condensate.
Inputs The SPP provides three mechanisms that produce energy: entanglement, particle production and magnetism. outputs The SPP produces heat, XUV and X-ray radiation, magnetism, and electrons as output. On Thu, Oct 29, 2015 at 9:49 AM, Stephen Cooke <[email protected]> wrote: > 1 GeV could be enough to generate Phi Mesons and Kaons through nucleon > resonance, although I suppose other factors such as resonance Windows and > conservation of states would need to be taken into account. I wonder if > they can provide an initial trigger to initiate LENR in the correctly > resonating medium. If nucleon disintegration is triggered perhaps enough > energy is generated and particles to sustain the process. > > I suppose I cosmic radiation is a trigger the South Atlantic Anomally > will suddenly become prime real estate! 😉 > > Sent from my iPhone > > On 29 Oct 2015, at 13:55, Jones Beene <[email protected]> wrote: > > Interesting conjecture and it shouldn’t be too hard to falsify. This > precise suggestion with Rydberg matter has not come up before AFAIK, but > going back to the early days of cold fusion, it had been suggested that one > reason why P&F seemed to have a higher success rate was the elevation of > Salt Lake City… which permitted a much larger flux of cosmic rays. Muons > are known to catalyze deuterium fusion, no Rydberg matter required. > > > > However (and I do not have a citation) this premise was apparently tested > many years ago, and found not to be accurate. Apparently Pd-D cold fusion > does not benefit from higher muon flux. That could mean many things – > including the lack of deuteron fusion as the relevant explanation for > excess heat. > > > > *From:* Stephen Cooke > > > > I meant "encounter a 1 GeV muon" but neutrino encounters (with possibly > even higher Energy) might also be potentially interesting if they can occur. > > > > Would Rydberg Matter or UDD be more sensitive to muons from cosmic rays > or may be even neutrinos? Than ordinary matter? > > > > Cosmic ray muons have can have high energy for example there are 10000 1 > GeV muons per sq meter per second. Their interaction with ordinary matter > is very low. I think this has been discussed before but I wonder if there > is a higher cross section with Rydberg matter. > > > > What is the surface area of the Rydberg matter > > > > 10000 per sq m /s is I think about 864 per sq mm per day, which implies > if that if Rydberg matter or UDD is a few 10s micrometers in size it should > encounter a neutrino about daily on average. > > > > The rest would depend on the probability of an encounter actually > reacting with the matter,I suppose relativistic effects on the wave > functions would also be important at these energies. > > > > I guess this has come up before so if you have a link let me know. > >
