Bob,

 

While it is true that Rossi's first demo had lead shielding, none of the
recent versions have had any shielding. You can see in the new paper and
pictures - there is no shielding. At the first demo 2011 - the radioactive
signal seen by Celani et al was seen at startup only. 

 

BTW - there was an elaborate detector setup used to look for radiation in
the initial and many other demos - in which sensors were placed under the
lead - and none of them saw radiation. There has never been data showing of
tens of keV - so there is no reason to imagine that there ever was any -
other than at startup.

 

The reason for this situation of needing lead shielding at one time - IMO is
that Rossi used only natural nickel at first, and this required  a
radioactive trigger at startup, but now he no longer uses bulk nickel so he
does not need a trigger nor shielding.

 

That changeover of design could have been because Rossi discovered (some
time in the last year) the identity of the active isotope. 

 

Once he pinpointed the active isotope, then he was able to enrich and no
longer needs the trigger nor the shielding.

 

 

From: Bob Higgins 

 

As a Rossi watcher, I notice what he has done historically.  All of his low
temperature reactors have been lined with a thin layer of lead.  Rossi
states that the reaction emits low energy photons in the 10's of keV up to
about 100keV.  This is consistent with the amount of lead that has been seen
in photos of his reactors.  I don't believe this lead would be needed if the
photons from the reaction were only in the neighborhood of 300eV.  The 300eV
photons would be absorbed in the nickel-rich fuel, and the containing
stainless cell.

 

While the reaction you are describing could exist (I am unqualified to say),
I don't believe it is consistent with the "Rossi effect".

Jones Beene wrote:

As mentioned previously, the value of ~300 eV could be a key to
understanding the excess heat of the Rossi effect. This mass-energy level
would be witnessed as a photon at the upper limit of ultraviolet spectrum or
a soft x-ray. This value is most unusual for photon emission in condensed
matter - being far above chemical and far below nuclear origin; but it fits
the experimental results in a way that nothing else has been able to do.

 

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