It would take four Deuterons (Deutero-Hydrinos?) or two 2-Helium-4
atoms to form 59-Prasodymium-141 from a Stable 55-Cesium-133 atom.
"Caesium (cesium in USA) is not a common element - about the 45th most abundant in the earth's crust. Caesium occurs in pollucite (a hydrated caesium silicate of aluminium - 2Cs2O.2Al2O3.9SiO2.H2O). Pollucite is found in Norh America, Italy, Kazakstan, and Sweden. Caesium is also found in rhodizite, a borate mineral containing aluminium, caesium, beryllium, and sodium. This is found in the Urals and in Madgascar. Caesium is also contained in some potassium ores."
There's that possible radio Potassium-40 and Argon Electronium (*e-) exposure again.
where the stable (*e-) is formed in the Cesium
Stable 59-Prasodymium-141 Isotope.
Fred
>>>>>>>>>>>>>>
Jed wrote:
----- Original Message -----From: TP SparberSent: 6/19/2006 11:03:37 AMSubject: RE: [Vo]: Long awaited Iwamura paperI'm waiting for Jones Beene to jump on the Argon that
is trapped in the lattice waiting for Deuterons to form
the Hydrino-Deuteride. :-)
http://lenr-canr.org/acrobat/IwamuraYobservatiod.pdf
Thanks Jed
Fred
Iwamura paper:
"The surface of the plate was covered
by layers of CaO and Pd, which were obtained by five times alternatingly sputtering 20-Å-thick CaO and 200-Å
-thick Pd layers. Then a 400-Å-thick Pd layer was sputtered on the surface of the CaO and Pd layers. These
processes are performed by Ar ion beam sputtering method or magnetron sputtering method. After forming a Pd
complex, Cs was deposited on the surface of the thin Pd layer. Cs was deposited by electrochemical method or
ion implantation method."
