Dear Rich.

Have you seen the brand new patent -published *just in time* (January 13)
WO 20110005506  "Method and apparstus for carrying out nickel and hydrogen
exotermal reaction" inventor Andrea Rossi?

Peter

On Sat, Jan 15, 2011 at 7:15 AM, Rich Murray <[email protected]> wrote:

> A new energy source from nuclear fusion, S Focardi, A Rossi, 9p text
> 2010.03.22: Rich Murray 2011.01.14
>
> http://www.journal-of-nuclear-physics.com/files/Rossi-Focardi_paper.pdf
> 9 pages
>
> A new energy source from nuclear fusion
> S. Focardi (1)
> and A. Rossi (2)
> (1) Physics Department Bologna University and INFN Bologna Section
> (2) Leonardo Corp. (USA) - Inventor of the Patent
> March 22, 2010
>
> Abstract
>
> A process (international patent publication N. WO 2009/125444 A1)
> capable of producing large amounts of energy by a nuclear fusion process
> between nickel and hydrogen, occurring below 1000 K, is described.
> Experimental values of the ratios between output and input energies
> obtained in a certain number of experiments are reported.
> The occurrence of the effect is justified on the basis of existing
> experimental and theoretical results.
> Measurements performed during the experiments allow to exclude
> neutron and gamma rays emissions.
>
> The patented apparatus is able of producing a constant and reliable
> amount of energy for a period of months.
>
> Two different samples of material used in the experiments labelled in table
> 1 as method A (288 kWh produced) and method B (4774 kWh produced)
> were analysed at Padua University SIMS.
> In the long period sample, the mass analysis showed the presence of
> three peaks in the mass region 63-65 a.m.u.
> which correspond respectively to Cu 63, elements (Ni 64 and Zn 64)
> deriving from Cu 64 decay and Cu 65.
> These allowed us the determination of the ratio Cu 63/Cu 65=1,6
> different from the value (2,24) relative to the copper isotopic natural
> composition.
> The peak in the mass spectrum at a.m.u.=64, due to Ni 64
> and Zn 64 (both caming from Cu 64 decay)
> requires the existence of Ni 63 which,
> absent in natural Ni composition, must have been in precedence
> produced starting by more light nickel isotopes.
> More details on this analysis will be given in a successive paper [8].
>
> 6. email address
> [email protected]
> [email protected]
>
>

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