Yes, Figure 3 looks like it’s not properly normalized before background
subtraction and only shows >= 500 keV, but if properly
processed all the peaks should disappear ... Its also appears much stronger
above 500 keV than the current result, suggesting even
more radiation in the low energy
The surface plasmon polariton (SPP) is first born out of concentrated
infrared photons, but it gets to a stage where it can extract nuclear
binding energy out of the nucleus. That energy is stored and downshifted
through FANO resonance in a soliton until the SPP decays whereupon its EMF
energy
You make some good points about MFMP.
I’m not an immediate member of MFMP. I’m volunteering my time/resources
when/where I can. If MFMP had more resources, they could
certainly do a better job. Do they deserve the resources? I think so. I have
nothing but mutual respect for them and what
It’s difficult for me to answer all your Qs at this point in time (due to time
constraints), but let me try to add a few things (and
Alan can certainly chime in here if he has the time)...
These cells were never really designed as accurate calorimeters to the level
that I think you are
From: Axil Axil
http://newenergytimes.com/v2/library/2004/2004Focardi-EvidenceOfElectromagneticRadiation.pdf
Evidence of electromagnetic radiation from Ni-H Systems. This MFMP radiation
observation is nothing new.
Figure 3 in this report is rather reminiscent of what we see
On Wed, Feb 24, 2016 at 10:38 PM, Mark Jurich wrote:
The Geiger Counter was essentially brain dead during this part of the run
> and also with a post Ba calibration on the low end... The detected
> radiation wasn’t shown to be sourced from the active cell.
I am a big fan of
The generation of black light was seen by R Mills many years ago. Will MFMP
reinvent the hydrino to explain their new found results?
On Wed, Feb 24, 2016 at 11:19 PM, Axil Axil wrote:
>
>
The Geiger Counter was essentially brain dead during this part of the run and
also with a post Ba calibration on the low end...
There were very few Gammas above 200 keV for this particular event (see the
linear graph, for example... A more sensitive (to low
energy X-ray/Gammas) donut Geiger
One reason why Rossi might do fuel prep as a preliminary first step is that
the fuel prep stage produces radiation since it is done at low
temperatures.. After he gets the fuel prepared, he loads it in the
operational reactor. Maybe Rossi does not want to see any radiation coming
out of his
On Wed, Feb 24, 2016 at 10:08 PM, Mark Jurich wrote:
Not sure what you mean by “full-blown calorimetry”, but I can tell you this
> (having been assisting Alan rather closely for the last several months).
By "full-blown calorimetry," I have in mind mass flow calorimetry,
http://newenergytimes.com/v2/library/2004/2004Focardi-EvidenceOfElectromagneticRadiation.pdf
Evidence of electromagnetic radiation from Ni-H Systems
This MFMP radiation observation is nothing new.
On Wed, Feb 24, 2016 at 9:43 AM, Jones Beene wrote:
> Where is the big
Not sure what you mean by “full-blown calorimetry”, but I can tell you this
(having been assisting Alan rather closely for the last
several months).
Typically Alan would first characterize the GlowStick Cell by inserting a
thermocouple dead center, on the active side with a dummy
loaded fuel
I wrote:
Although I do not find Ed Storms's theory persuasive, I suspect I know how
> he would reply to this. He might say that what MFMP have observed in the
> NaI detector is a hot-fusion side channel, which he makes allowances for.
> Note that although MFMP believe that the signal is strong,
On Wed, Feb 24, 2016 at 11:12 AM, Bob Higgins
wrote:
There is presently no description in a hydroton theory for MeV+ electron
> emission.
>
Although I do not find Ed Storms's theory persuasive, I suspect I know how
he would reply to this. He might say that what MFMP
On Wed, Feb 24, 2016 at 12:45 PM, Mark Jurich wrote:
Right now, we are working on beefing up the Geiger Counting Sensitivity,
> Coincidence Detection and obtaining another detector to confirm. It’s only
> one instrument, we need another to confirm. Temporary High Voltage
>
I get the impression the Glowstick 5-2 test did not use full-blown
calorimetry, and instead just used two thermocouples, one for the live tube
and one for the blank.
Eric
In LENR we get either High energy radiation (x-rays) or Heat: not both.
This is based on the temperature of the Reactor. A cold reactor produces
X-Rays.
The SPP absorb nuclear binding energy and store it in a whispering gallery
wave(WGW) in a dark mode. The energy is stored inside the WGW until
Note that the E correlation found by Bob Higgs, 1/E^2, may be obtained by
the inverse Stirling approximation n(lnn)-n=n(ln(1 +(n- 1))-1)~ n(n - 2)
~n^2, since n~E, we have the fit 1/E^2
--
Daniel Rocha - RJ
danieldi...@gmail.com
There is the occasional report of gammas and even neutrons in LENR, going back
a long way - but the numbers are always far removed from having a direct
correlation to heat. Here is a reality check on the issue of how far removed
gamma radiation will be - as being any kind of validation for
He is in the PST zone … Predictive Standard Time
From: Jed Rothwell
Jones Beene wrote: Here is the blog…
http://www.quantumheat.org/index.php/en/home/mfmp-blog/515-glowstick-5-2
Thanks.
I see he made that comment tomorrow at 2 a.m. That's prescient. And hard
working!
-
Jones Beene wrote:
> Here is the blog…
>
>
>
> http://www.quantumheat.org/index.php/en/home/mfmp-blog/515-glowstick-5-2
>
Thanks.
I see he made that comment tomorrow at 2 a.m. That's prescient. And hard
working!
- Jed
From: Jed Rothwell
Alan Goldwater – the experimenter - just posted he is NOT claiming excess heat.
. . .
Where is that discussion? Where did he post it?
Here is the blog…
http://www.quantumheat.org/index.php/en/home/mfmp-blog/515-glowstick-5-2
I think you're onto something here, because Focardi once said that Rossi's
contribution was to introduce a "catalyst" (probably Tungsten) that split
H2 gas into H1 gas before being loaded into the reactor. This started a
pre-LENR reaction of the H1 gas recombining into H2 gas inside the Nickel
Jones Beene wrote:
> Alan Goldwater – the experimenter - just posted he is NOT claiming excess
> heat. . . .
>
Where is that discussion? Where did he post it?
- Jed
It is worth noting that we cannot label this experiment as evidence of thermal
gain.
Alan Goldwater – the experimenter - just posted he is NOT claiming excess heat.
This is despite the fact that others seem to be trying to put words in his
mouth.
AG: “During the testing, just after the
Bob Higgins,
do not forget that all these energies come from nuclear potentials which
are in sort of equilibrium, a chaotic one, with coulomb potential. this
strong inhibition is expected given that, in my view, lenr seem to be set
around the threshold of fusion and scattering. and a larger
This is very helpful… seeing that most of the ordinary efforts have been well
attended to and the obvious bugs eliminated makes the signal more mysterious…
that’s a good thing.
From: Bob Higgins [mailto:rj.bob.higg...@gmail.com]
Sent: Wednesday, February 24, 2016 3:51 PM
To:
Alan has a full set of gamma check sources. Initial calibration was done
with 137Cs. The energy scale drifted over time with heating from the
reactor. The background always showed the 78keV x-ray and 1461 40K
background peaks. I re-calibrated the energy scale on every file,
resampled each to
Yes, exactly. 1.2 would be very close to the limits of the GlowStick, and Alan
can fill you in on the exact values if you join the
chat at:
http://magicsound.us/MFMP/video/
The description is here:
http://www.quantumheat.org/index.php/en/home/mfmp-blog/515-glowstick-5-2
- Mark Jurich
Mark Jurich wrote:
We (Team MFMP) did not see much heat (if/any) above the noise level of this
> crude calorimeter . . .
>
I am sorry to hear this is a crude calorimeter. Where is it described?
If it is quite crude, perhaps the heat of 1.2 times input is a mistake.
- Jed
Was there some sort of calibration with some known radiation sources performed
with the same NaI instrument in the lab setting. Say placing a Coleman lantern
mantle, thorium laced, for a reading, or a banana or cupful of Salt Substitute
KCl…. Plenty of known ‘reference radiation sources’ are
Yeah ... I don't thinks so. Think about it. At 100,000,000K, you get some
small output at 100keV. But, by the time you get to 1MeV, the blackbody
radiation intensity is down by 40 orders of magnitude - I.E. by a factor of
1E-40 . So what are you saying, that some parts of the reaction are at 1
>
> Bob Higgins,
>
It could really be a black body radiation. Consider many cooling bodies.
They will have different black body distributions at different times. So
what you see is the sum of many black bodies at different times of a
cooling process. It will be steep at large temperatures, since
AFAIK, the Lugano team never publicly commented on the errors found in
their analyses. Tom Clarke makes a good case for some portions of the
surface envelope to be at 780C. If this were the whole story, the reactor
would have been seen as a barely detectable red glow. MFMP found in its
replica
If I remember correctly, the Lugano team did not provide any internal
temperatures. They only reported the surface temperatures which were
high enough that the reactor should have glowed white hot if it
behaved like an incandescent body. However, as Jed pointed out, the
pictures they provided were
Why can't the peak be at 100eV or 10eV and many order of magnitude more
intense. There is not much in the shown signal
that indicates a peak in teh extreme spectra near the seen peak in the
background. I think it looks like a 1/X^n curve that continues
way below the cutof of the instrument. The
I don't think that is the reason for the Lugano appearance. The Lugano
reactor was like an incandescent light bulb and it was not analyzed that
way. If you analyzed an incandescent light bulb, the appearance and its
radiated power would not be represented by the temperature of the glass
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 wrote:
> How about the
This is akin to ascribing a temperature to an electron ensemble having a
certain distribution of kinetic energy. It is valid to consider it that
way, but it is still the electron energy distribution that is determining
the "characteristic temperature". May turn out to have some meaning if
looked
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 wrote:
> One of
The one and only thing that has kept this from looking like a complete fiasco
and amateur-hour is Greenyer’s cryptic message about the 5 hour self-sustaining
event.
Now you are saying that there is no 5 hour event?
The so-called gamma signal is a joke. There is little there but noise.
This
http://egooutpeters.blogspot.ro/2016/02/feb-24-2016-lenr-cities-european-leader.html
please try to discover Vanderberghe's Law for LENR energy density, similar
to Moore's Law in IT.. and man y other things...industry is preparing for
the LENR Era.
Peter
--
Dr. Peter Gluck
Cluj, Romania
The plot looks like the Landau distribution for ionizing particles
On Wed, Feb 24, 2016 at 1:28 PM, Bob Higgins
wrote:
> I am not sure where the idea of "5-hour self-sustaining event" came from.
> I never said it. I only discussed the radiation outburst. Did you read
Folks, it is true that Bob G might have overhyped this, but you have to realize
the number of years he has devoted to this and the
knowledge he has acquired over those years. I do not blame him for doing it.
Yes, the Spectrum Result has to be verified/replicated. We (Team MFMP) did not
see
I just raised the price to $15.
-Original Message-
From: Frank Znidarsic
To: rvargo1062
Sent: Wed, Feb 24, 2016 1:17 pm
Subject: Fwd: Interesting marketing game
-Original Message-
From: Frank Znidarsic
To:
I would have to investigate this further, but this distribution as an E^2
in the denominator and the measured spectrum is approx. 1/E^2 .
On Wed, Feb 24, 2016 at 11:05 AM, Daniel Rocha
wrote:
> Bob Higgins, what about a
>
I am not sure where the idea of "5-hour self-sustaining event" came from.
I never said it. I only discussed the radiation outburst. Did you read
what I wrote? That was just a web article. There is still more analysis
to come.
You have no case for the radiation event being small or due to
Apart from the interesting physics that will give the theoreticians
something to chew on, It seems important that the significance of what
Rossi said earlier, that the heat comes from the lead absorbing the
gamma rays, is now appreciated.
I noticed this when I was trying to provide a link to my books and apps.
If you search amazon for "Znidarsic Science Books" only the higher priced
versions of the my book come up. Where is my $10 version. Apparently the
secondary vendors do a lot a business and pay for premium advertising.
At the paper, we didn't have any experimental data to analyze and these
nuclei are very hard to analyze, even a single proton is hard. With
multiple bodies, the difficult is outstanding. So, the idea was to have
something spread and with a peak, such that it could explain why detecting
any
Bob Higgins, what about a
https://en.wikipedia.org/wiki/Relativistic_Breit%E2%80%93Wigner_distribution
?
The high energies seen might require the production of D-mesons. A timeline
based decay chain map as holmlid has done would tell what subatomic
particles are being produced and how they decay to lower energies.
The nuclear process involved might be the decay of the proton and neutron
in the
From: Bob Higgins
Ø
Ø Where is your analysis that this spectrum could have come from a puff of
radon gas?
Bob, Santa Cruz CA is a radon hot spot. We are not talking about a “puff” we
are talking about natural emission of Radon from earth, which is variable
throughout the day.
I vote for option #2 being the source of this signal, the ‘neutral’ particles
being crazy neutrons, ‘mischugenons’ as described Edward Teller in earlier
closely related cold fusion work. Some few of us have been able to produce
these critters. It’s good news if this particular recipe works and
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
On Wed, 2016-02-24 at 06:43 -0800, Jones Beene wrote:
> What am I missing?
>
Gamma Rays!
Craig
If the burst was from Rn-222 then I would expect various Radon daughters
to show up on the gamma spectrum. Rn-222 is an alpha emitter.
Bob
WA7ZQR
On 2/24/2016 9:03 AM, Jones Beene wrote:
*From:* Daniel Rocha
In figure 7 (compare with figure 6), it seems that the signal is
above the
Besides electrons, the production of kaons whose substantial energy content
would be available to produce gamma radiation in the MeV range is a
candidate for the radiation profile observed..
On Wed, Feb 24, 2016 at 12:12 PM, Bob Higgins
wrote:
> For many years, I have
Adding to my post. So, it is like a sort of blackbody for something like a
"nano neutron star".
Jones,
Where is your analysis that this spectrum could have come from a puff of
radon gas? There were longer background measurements that were entirely
constant in photometric reduction. The indications of radon come primarily
from the characteristic x-ray peak at 78keV (due to lead and bismuth
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
The secondary vendor does not even have to touch the product. Just take the
order for you @ $50, order the product at $10, and have it shipped to your
address. What it you did this for 10,000 products?
I learn something new each day.
-Original Message-
From: Frank Znidarsic
From: Stefan Israelsson Tampe
* But the main frequency is invisible we only see the tail here what the
peak is in the invisible range of this instrument. We simply don't know the
magnitude of the radiation energy. But I agree that it is way to early to call
this a success. It is an
My Cold Fusion book sells for $10 at Amazon. Why then is if for sale at $50.
It appears that someone picks products up and resells then at a much higher
cost. Let the buyer beware. I wonder how prevalent this is.
From: Daniel Rocha
In figure 7 (compare with figure 6), it seems that the signal is above the
background, in the region of 10-50kev by up to 100. So, that like >10 sigma.
There is definitely something there.
There is of course “something” there. But not necessarily LENR.
The
For many years, I have been saying that excess heat is a poor test for LENR
- a poor and insensitive indicator of LENR. What has been seen in this
experiment (GS5.2), is a clear indication of LENR via a radiation
signature. This was a high signal-to-noise spectrum and getting such a
spectrum
It is a good start- good news will breed GREAT news
http://egooutpeters.blogspot.ro/2016/02/feb-24-2016-lenr-mfmps-demonstrable.html
--
Dr. Peter Gluck
Cluj, Romania
http://egooutpeters.blogspot.com
I may be wrong, but I'm under the impression that they have repeated
this several times and there is more information to be released today.
Bob
WA7ZQR
On 2/24/2016 6:43 AM, Jones Beene wrote:
Where is the big surprise?
I woke this morning with anticipation - expecting to see proof from
But the main frequency is invisible we only see the tail here what the peak
is in the invisible range of this instrument.
We simply don't know the magnitude of the radiation energy. But I agree
that it is way to early to call this a success.
It is an interesting lead and it should be repeated.
On
Jones Beene wrote:
> Instead, we get graphs of modest gain at the noise level and radiation
> counts peaking in the few hundred per second – when we need to seeing a
> million times more . . .
>
Cold fusion never does that. If it were a million times more, it would be
plasma
In figure 7 (compare with figure 6), it seems that the signal is above the
background, in the region of 10-50kev by up to 100. So, that like >10
sigma. There is definitely something there.
Well, if weren't slightly above background, it wouldn't be cold fusion,
right?
2016-02-24 12:47 GMT-03:00 Jones Beene :
> Well - OK... there is a tiny signal - but let's look at the counts per
> minute or per second.
>
> We are talking about 20 per second or so instead of a
>From a nuclear science perspective the spectrum is something to get
excited about.
If a famous laboratory produced this spectrum I think it would be in the news.
Harry
On Wed, Feb 24, 2016 at 10:47 AM, Jones Beene wrote:
> Well - OK... there is a tiny signal - but let's
Well - OK... there is a tiny signal - but let's look at the counts per minute
or per second.
We are talking about 20 per second or so instead of a background of 4 or so.
This is really "banana level" (bananas are slightly radioactive).
You would need to see trillions of times this level if
from
https://docs.google.com/document/d/1OAcb975m_AXMFz25zcl07kllERqVjSbZsWv_P1A3xQc/edit?pref=2=1
Bob Higgins writes:
"There was a significant gamma outburst measured in GS5.2 whose
broadband high energy spectrum is not only unexplainable by known
chemistry and physics, but may also not be
I hope so. Cold Fusion have proven to be inaccessible to the experimenter.
That's why I stopped writing books, doing experiments, and started programming
apps.
I have a nice video on my latest app.
Yes a little underwhelming but if they truly have a hands down recipe to
repeatable anomalous heat it will probably get a number of industry labs and
their funding off the fence wrt LENR. Now researchers can prove to their
management this is real.
Fran
From: Jones Beene
Where is the big surprise?
I woke this morning with anticipation - expecting to see proof from MFMP of
a 5 hour self-sustained reaction. Instead, we get graphs of modest gain at
the noise level and radiation counts peaking in the few hundred per second -
when we need to seeing a million times
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