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*GlowStick* 5.2

Scritto da Robert Greenyer on .

Alan Goldwater has started the second major experiment in the *GlowStick* 5 series.

This experiment will focus on Nickel pre-processing to begin with.

Live screen grabs

Live data is on HUGNetLab under GS5 - http://data.hugnetlab.com/

 

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0 #277 Robert Greenyer 2016-04-08 21:14
New test underway... calibrations started.
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0 #276 Robert Greenyer 2016-04-03 22:00
@Jones Beene,

It is not a bad idea and still valid according to Piantelli theory also as it is a transition metal.

We do need to focus on our exact replication attempts first. We can look into doing something like this afterwards - should we get lucky!
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0 #275 Jones Beene 2016-03-29 16:33
Zinc would be less compelling as a reactant if it were not a Mills catalyst (for hydrogen densification) and it has the lowest Rydberg “hole” (27.2 eV) in addition to its volatility (boiling point is ~900C). Thus it can probably do no harm to add zinc to a fuel mix – and it could have properties of interest. There is almost no downside risk.

One suggestion then is to add 100 mg zinc into a fuel mix in order to get data which will either validate what Parkhomov thinks is there, or if the result is null – to write-off the possibility of zinc as a reactant. A sliver of zinc metal can be used since it will vaporize anyway, it does not need to be a powder.
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0 #274 Jones Beene 2016-03-29 02:07
@Bob, "I have the answer back from Parkhomov on the "64Ni" question "About high content of 64Ni. We assume that in fact an impurity 64Zn was registered. Mass spectrometer cannot distinguish between these two isotopes."

Wow. This could be a major breakthrough... or not. The isotope in question was depleted by almost half, so it provided most of the excess heat. If the 4.4% of mass 64 was due to zinc, then about 8% of the starting nickel was zinc contamination which is high but not impossible. Since Parkhomov sounds fairly sure, then he may have seen the other zinc isotopes which were not mentioned.

Obviously, the next questions are something like this: was the depletion of the zinc-64 (compared to the starting level) due to its slight inherent radioactivity, and was the decay vastly accelerated? If so, then we must accept that accelerated beta decay can provide excess heat and possibly avoid detection. Other mechanisms are possible but 64Zn has an extremely long half-life, yet it is known to beta decay.

The bottom line is that it would be wise to add zinc to a glowstick experiment to see if it could really be this simple.
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0 #273 Robert Greenyer 2016-03-29 00:04
@Jones Beene

I have the answer back from Parkhomov on the "64Ni" question

"About high content of 64Ni. We assume that in fact an impurity 64Zn was registered. Mass spectrometer cannot distinguish between these two isotopes."
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0 #272 Robert Greenyer 2016-03-26 22:38
@Stoyan,

Thankyou for the reference.
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0 #271 Dr. Stoyan Sarg 2016-03-25 23:15
X-rays of the order of 100 keV are reported in the extensive document of the ENEA (Italian National Agency for New Technologies Energy and Environment) on cold fusion research, published in 2008 (see the link). It is shown in page 176. In the same page “a remarkable quantity of Cu and Zn” is also mentioned. Rossi claims a detection of Zn in his patent application WO 2009/125444 A1 (Fig. 3). A mass number 69 is also apparent in the ashes of E-cat test according to Lugano report, corresponding to 69Zn ( Appendix 3, Fig 11).
enea.it/.../...
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0 #270 Robert Greenyer 2016-03-22 23:27
@Jones

Well - 62Ni will be tested in time - we have it...

Will investigate the other.
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+1 #269 Jones Beene 2016-03-21 20:35
Here is a paper on Ni isotope fractionation in meteorites.

originslab.uchicago.edu/.../.. .

Russia is the world's largest nickel producer and much of it comes from meteorite impact sites. This nickel can be naturally enriched, substantially in 64Ni, which is the process called fractionation. This is exactly what could have happened with the Parkhomov nickel and he may not have realized this before now, based on the lack of further information in the paper.

Needless to say, the situation boils down to this. If you believe Rossi, then 62Ni would be active, but if you believe Parkhomov, then 64Ni is the isotope that works. I do not think it could be both based on Parkhomov's results.

Based on everything I have read, Parkhomov would be the one I would choose, especially since the theory behind 64Ni is stronger, and since 64Ni is a singularity of sorts, in terms of neutron heaviness. Plus the naturally enriched version should be much cheaper than buying pure isotope...
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