An energy distribution whose peak becomes higher at lower temperatures might help to explain why the Lugano reactor's surface temperature appeared to be too high for how it looked visually.
Harry On Wed, Feb 24, 2016 at 2:20 PM, H LV <hveeder...@gmail.com> wrote: > How about the Maxwell-boltzmann distribution? > http://ibchem.com/IB/ibnotes/full/sta_htm/Maxwell_Boltzmann.htm > > Lower temperatures have higher peaks which is the opposite of a > blackbody distribution. > > Harry > > On Wed, Feb 24, 2016 at 12:45 PM, Bob Higgins <rj.bob.higg...@gmail.com> > wrote: >> One of the researchers that I discussed this with suggested that the >> spectrum looked like a blackbody radiation. I did some analysis and can >> tell you that it does NOT look like blackbody radiation. Blackbody >> radiation cuts off very sharply on the high energy side. At 100 million >> degrees, there would be some energy at 100keV, but by the time it got to >> 1MeV, the blackbody radiation would have declined by 40 orders of magnitude. >> That is not what is seen here. >> >> It is really hard to explain a continuous spectrum that looks like it >> probably spans at least 2 orders of magnitude in photon energy with maximum >> energies over 1MeV. The best explanations so far (and there has not been a >> chance for widespread vetting) are that it is due to: 1) Bremsstrahlung >> from really high energy light charged particles [electrons, positrons] with >> a distribution of energy, or 2) interference in the NaI detector by a flux >> of neutral particles causing the apparent spectrum by activation of the Na, >> I, and Th in the detector crystal. >> >> Thank you for the links. I will have a look these papers. >> >> On Wed, Feb 24, 2016 at 10:29 AM, Daniel Rocha <danieldi...@gmail.com> >> wrote: >>> >>> The peak is at least 10x more than that of you provided... >>> >>> Bob Higgins, in my work with Akito, I proposed that in cold fusion you >>> have, unlike the conventional fusion, the fusion of more than 2 nuclei. >>> There are not experiments with more than 2 nuclei fusioning (C12 is formed >>> by B8, which is stable for 10^-15s, I am talking here of something less than >>> 10^-23s in coincidence). This will form an excited ball that will shine at a >>> few kev. There will surely be brehmstralung, from this weak gama rays. >>> >>> http://vixra.org/abs/1209.0057 >>> >>> http://vixra.org/abs/1401.0202 >> >>
