Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread mixent
In reply to  ny@aol.com's message of Tue, 5 Jun 2012 00:14:05 -0400 (EDT):
Hi,
[snip]
http://sire.com/fusion.htm 

This page talks about gaps, but you don't need gaps. In fact almost all
elements have isotopes that work. Odd numbered elements however tend to make
better starting material because there are almost always fewer stable isotopes
of the odd numbered elements than of the even numbered ones. That means that the
element following the odd one is likely to have quite a few stable isotopes,
which are likely to include the ones that would form by addition of a proton to
the odd numbered nucleus.
In short, if you start with an odd numbered element, you almost always get a
stable isotope as end product.

e.g. 


H + Na23 (100%) = Mg24 (stable) + 11.69 MeV

H + Al27 (100%) = Si28 (stable) + 11.58 MeV

H + P31 (100%) = S32 (stable) + 8.86 MeV

H + Cl35 (75%) = Ar36 (stable) + 8.5 MeV

H + Cl37 (25%) = Ar38 (stable) + 10.24 MeV

H + Cu63 (69%) = Zn64 (stable) + 7.7 MeV

H + Cu65 (31%) = Zn66 (stable) + 8.93 MeV

etc.

Each of these reactions also has a less energetic alternative where an alpha
particle is emitted, also producing stable isotopes.

Both Na and Al are particularly attractive as they are very common.

(The 1 lb packet of salt you have in the cupboard would supply your home with
energy for well over 100 years, not counting the Chlorine reactions! ;)

Regards,

Robin van Spaandonk

http://rvanspaa.freehostia.com/project.html



Re: [Vo]:OT: Wisconsin will chose their governor in less than 24 hours

2012-06-05 Thread Vorl Bek
 This is another OFF TOPIC Wisconsin Political commentary. If not
 interested, please skip this post! You have been warned!

Why don't you use vortex-b for this stuff?



[Vo]:What Happened in CE 774?

2012-06-05 Thread Terry Blanton
http://www.nature.com/news/mysterious-radiation-burst-recorded-in-tree-rings-1.10768

Just over 1,200 years ago, the planet was hit by an extremely intense
burst of high-energy radiation of unknown cause, scientists studying
tree-ring data have found.

http://www.nature.com/nature/journal/vaop/ncurrent/full/nature11123.html

Is it possible that our sun generated an unprecedented energy burst?

T



Re: [Vo]:What Happened in CE 774?

2012-06-05 Thread David Roberson

I agree with you Terry that it could likely be some form of solar event.  Maybe 
you should check the historical sun spot record if available for that time 
frame to get some form of correlation.

It also makes one wonder if similar, ever more powerful, events in history have 
resulted in a driving mechanism for evolution.  The poor creatures around 
during such an occasion would not even know what hit them!  If this type of 
event happens frequently in the history of life on earth one would expect DNA 
to have a built in mechanism to correct for a moderate radiation burst.   I do 
recall reading about repeated sequences within our DNA and these bursts might 
indicate a good reason for that to be true.

Dave 








-Original Message-
From: Terry Blanton hohlr...@gmail.com
To: vortex-l vortex-l@eskimo.com
Sent: Tue, Jun 5, 2012 8:37 am
Subject: [Vo]:What Happened in CE 774?


http://www.nature.com/news/mysterious-radiation-burst-recorded-in-tree-rings-1.10768
Just over 1,200 years ago, the planet was hit by an extremely intense
urst of high-energy radiation of unknown cause, scientists studying
ree-ring data have found.
http://www.nature.com/nature/journal/vaop/ncurrent/full/nature11123.html
Is it possible that our sun generated an unprecedented energy burst?
T



RE: [Vo]:What Happened in CE 774?

2012-06-05 Thread Jones Beene
Interesting but was it from our sun, and/or was our sun triggered. This
was based on tree-ring data in Japan and North America, but I wonder about
South America. If there was a substantial variation between North and South
it could tell us something - although there are weather mechanisms for
mixing radiocarbon between hemispheres. 

Mauro Lacy may know this, since he follows the subject area.

If the 14Carbon increase were higher in the Southern Hemisphere, for
instance, then my bet for the culprit is an x-ray burst from eta Carinae. It
is the death star that produces massive directed cosmic rays at times -
and we do not know how far back its instability began.

http://www.mail-archive.com/vortex-l@eskimo.com/msg63181.html

If the rate of 14C in tree rings were found to be less in the Southern
Hemisphere, it would probably rule out this particular source, which at
various times has been the brightest star in the night-time sky (Sirius is
normally brighter but it is only 8+ light years away while eta Carinae, even
at its enormous distance of 8,000 ly - has been as bright as Sirius at
times. 


-Original Message-
From: Terry Blanton 

http://www.nature.com/news/mysterious-radiation-burst-recorded-in-tree-rings
-1.10768


Just over 1,200 years ago, the planet was hit by an extremely intense
burst of high-energy radiation of unknown cause, scientists studying
tree-ring data have found.

http://www.nature.com/nature/journal/vaop/ncurrent/full/nature11123.html


Is it possible that our sun generated an unprecedented energy burst?

T

attachment: winmail.dat

Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread David Roberson

I took a table of nuclides and performed a Energy difference between the 
different nickel isotopes, plus associated proton and electron, and the 
daughter copper isotopes and compared the net released energy to the energy 
required to overcome the coulomb barrier.  The most significant energy release 
which exceeds the barrier occurs when the Ni62 or Ni64 isotopes are converted.  
The delayed beta plus decay which is present for all of the other 
transformations looses a large amount of energy to a neutrino which promptly 
escapes the device.  I will demonstrate the numbers below.

These components are required to build Cu63 from Ni62
1 u = 931.494 MeV  Disregard the slight rounding errors, excel chart source of 
data

Ni62  Mass=61.92835 (u)  Energy=57685.88 MeV
Proton Mass=1.007276 (u)  Energy=938.2716 MeV
Electron Mass=.000549 (u) Energy=.510999 MeV

Coulomb Barrier Energy ~5.6 MeV according to Rossi in his paper

Cu63 Mass=62.9296 (u) Energy=58618.54 MeV

Mass of components of Cu63;Ni62 + Proton + Electron=62.936175 (u)  
Energy=58624.66 MeV

Mass decrease that must be released as energy=62.936175 - 62.9296 = .006575 (u) 
Energy=  6.12457 MeV - 5.6 MeV Barrier = .52457 MeV;Same Calculation for Cu65 
yields 1.8532 MeV
In these reactions there are no Beta Plus Decay radiation losses due to 
neutrino release and no 511 keV gammas.

Please note that I also calculated the expected energy release due to WL 
process on the isotopes such as Ni60 and had perfect energy correlation when 
the energy required to make a neutron from a proton and electron is included.

Exactly the same energy is seen in both paths (Rossi and WL)  when the 
starting point is a nickel isotope with a proton and an electron, and the final 
point is the next higher isotope of nickel.

I am working very hard to get a clear understanding of the coulomb barrier 
energy behavior.  I can show that the alpha process within stars stops once 
iron has been synthesized, but this is only true if the barrier energy is 
trapped within the nucleus in the form of mass.  I am approaching the problem 
from different directions to prove whether or not this hypothesis is accurate.  
 

Dave
 

-Original Message-
From: pagnucco pagnu...@htdconnect.com
To: vortex-l vortex-l@eskimo.com
Sent: Mon, Jun 4, 2012 11:49 pm
Subject: Re: [Vo]:about Triumph Management (and LENR)


David,
Can you explain your conclusion.
 can't see how any energy is released in these Ni -- Cu transmutations.
Lou Pagnucco
David Roberson wrote:
 I may have been a bit to fast in pointing out the possible endothermic
 nature of the Ni62 and Ni64 reactions.  They actually are the best two
 isotopes to use if you were not to rely upon the beta plus decay for a
 substantial portion of the energy release.  They further are not
 susceptible to having the 511 keV gammas that would no doubt be released
 by the reactions involving the other nickel isotopes since copper 63 and
 65 are stable and do not decay into nickel by that process.

 So, if Rossi is actually able to overcome the coulomb barrier by some
 mechanism and his device only uses the Ni62 and Ni64 isotopes then it
 could be functional.  The energy released per atom for these two isotopes
 is only 1 or 2  MeV after satisfying the coulomb barrier, but that is a
 lot more than any chemical reaction can deliver.  I wonder if the
 relatively modest amount of energy release also can be more safely
 directed toward useful forms such as vibrational coupling into the
 surrounding structure.

 All of my estimates and calculations assume the reaction path that has
 been suggested by Rossi instead of the WL process which would be much
 more energetic.  Each of these proposed mechanisms has it's own particular
 problems to overcome.

 Dave



 -Original Message-
 From: David Roberson dlrober...@aol.com
 To: vortex-l vortex-l@eskimo.com
 Sent: Mon, Jun 4, 2012 10:30 am
 Subject: Re: [Vo]:about Triumph Management (and LENR)


 I just wanted to point out that if Ni62 and Ni64 are the only isotopes
 that work then the addition of a proton to either results in the
 production of a stable isotope of copper which does not undergo beta plus
 decay.  Much less energy is released per atom if the beta plus decay is
 avoided.  My calculations suggest that these two reactions might actually
 be endothermic due to the large coulomb barrier.

 Perhaps this is a bit of misdirection?

 Dave



 -Original Message-
 From: integral.property.service integral.property.serv...@gmail.com
 To: vortex-l vortex-l@eskimo.com
 Sent: Mon, Jun 4, 2012 9:30 am
 Subject: Re: [Vo]:about Triumph Management (and LENR)


 A.R. from Florida with love,
 Andrea Rossi




Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread integral.property.serv...@gmail.com

Robin,

http://www.journal-of-nuclear-physics.com/?p=338
http://www.ecatplanet.net/rossiblog.php?msg_search=Guglinski
e+p+e = Hydride Anion = *
1. Trap * in lattice (Ni nano, C nano Cone, etc.)
2. Activate * {Cavitation, heat, RFG, Arc, coordinated oscillations, 
Lattice wave creation, etc.}
3. p+e portion of * enters Ni nucleus creating unstable isotope leaving 
e behind for charge balance.

4. Ni Isotope = Cu + Cold Fusion Energy
6. Don't bother with trying to determine reaction with Quantitative 
Analysis, Mass changes incredibly small and energy incredibly large. E=MC2


Warm Regards,

Reliable

mix...@bigpond.com wrote:

In reply to  ny@aol.com's message of Tue, 5 Jun 2012 00:14:05 -0400 (EDT):
Hi,
[snip]
  
http://sire.com/fusion.htm 



This page talks about gaps, but you don't need gaps. In fact almost all
elements have isotopes that work. Odd numbered elements however tend to make
better starting material because there are almost always fewer stable isotopes
of the odd numbered elements than of the even numbered ones. That means that the
element following the odd one is likely to have quite a few stable isotopes,
which are likely to include the ones that would form by addition of a proton to
the odd numbered nucleus.
In short, if you start with an odd numbered element, you almost always get a
stable isotope as end product.

e.g. 



H + Na23 (100%) = Mg24 (stable) + 11.69 MeV

H + Al27 (100%) = Si28 (stable) + 11.58 MeV

H + P31 (100%) = S32 (stable) + 8.86 MeV

H + Cl35 (75%) = Ar36 (stable) + 8.5 MeV

H + Cl37 (25%) = Ar38 (stable) + 10.24 MeV

H + Cu63 (69%) = Zn64 (stable) + 7.7 MeV

H + Cu65 (31%) = Zn66 (stable) + 8.93 MeV

etc.

Each of these reactions also has a less energetic alternative where an alpha
particle is emitted, also producing stable isotopes.

Both Na and Al are particularly attractive as they are very common.

(The 1 lb packet of salt you have in the cupboard would supply your home with
energy for well over 100 years, not counting the Chlorine reactions! ;)

Regards,

Robin van Spaandonk

http://rvanspaa.freehostia.com/project.html


  




Re: [Vo]:OT: Wisconsin will chose their governor in less than 24 hours

2012-06-05 Thread ecat builder
Despite the high anti-incumbent sentiment in the U.S., Scott Walker
should easily win this election. (http://www.intrade.com/ has Walker
winning at +90%)

The reason Walker has support is simple: The unions tried to bully
their way into the governor's office using a recall vote that is
usually used only for malfeasance or misconduct. Most gubernatorial
recall attempts fail. And people generally prefer tea party ideals
over unions. (Unless you happen to be in a union, eh Steven?)

Perhaps back on topic: What if we could get a real money wager on
LENR+... Say, the demonstration of 1kW electricity continuous using
unconventional LENR fuel by 2015.  traded on an anonymous system like
intrade. That might be the surest and most accurate way to get a read
on the current state of commercial LENR. And interesting the effect it
would have on energy stocks.

- Brad

 Why don't you use vortex-b for this stuff?




Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread integral.property.serv...@gmail.com

David,
*
NASA's Bushnell UNLEASHED for LENR!*
http://www.usmessageboard.com/science-and-technology/226454-nasas-bushnell-unleashed-for-lenr.html#post5395486

Warm Regards,

Reliable

David Roberson wrote:
I took a table of nuclides and performed a Energy difference between 
the different nickel isotopes, plus associated proton and electron, 
and the daughter copper isotopes and compared the net released energy 
to the energy required to overcome the coulomb barrier.  The most 
significant energy release which exceeds the barrier occurs when the 
Ni62 or Ni64 isotopes are converted.  The delayed beta plus decay 
which is present for all of the other transformations looses a large 
amount of energy to a neutrino which promptly escapes the device.  I 
will demonstrate the numbers below.
 
These components are required to build Cu63 from Ni62
1 u = 931.494 MeV  Disregard the slight rounding errors, excel chart 
source of data
 
Ni62  Mass=61.92835 (u)  Energy=57685.88 MeV

Proton Mass=1.007276 (u)  Energy=938.2716 MeV
Electron Mass=.000549 (u) Energy=.510999 MeV
 
Coulomb Barrier Energy ~5.6 MeV according to Rossi in his paper
 
Cu63 Mass=62.9296 (u) Energy=58618.54 MeV
 
Mass of components of Cu63;Ni62 + Proton + Electron=62.936175 (u)  
Energy=58624.66 MeV
 
Mass decrease that must be released as energy=62.936175 - 62.9296 = 
.006575 (u) Energy=  6.12457 MeV - 5.6 MeV Barrier = .52457 MeV;Same 
Calculation for Cu65 yields 1.8532 MeV
In these reactions there are no Beta Plus Decay radiation losses due 
to neutrino release and no 511 keV gammas.
 
Please note that I also calculated the expected energy release due to 
WL process on the isotopes such as Ni60 and had perfect energy 
correlation when the energy required to make a neutron from a proton 
and electron is included.
 
Exactly the same energy is seen in both paths (Rossi and WL)  when 
the starting point is a nickel isotope with a proton and an electron, 
and the final point is the next higher isotope of nickel.
 
I am working very hard to get a clear understanding of the coulomb 
barrier energy behavior.  I can show that the alpha process within 
stars stops once iron has been synthesized, but this is only true if 
the barrier energy is trapped within the nucleus in the form of mass.  
I am approaching the problem from different directions to 
prove whether or not this hypothesis is accurate.   
 
Dave
 
-Original Message-

From: pagnucco pagnu...@htdconnect.com
To: vortex-l vortex-l@eskimo.com
Sent: Mon, Jun 4, 2012 11:49 pm
Subject: Re: [Vo]:about Triumph Management (and LENR)

David,

Can you explain your conclusion.
I can't see how any energy is released in these Ni -- Cu transmutations.

Lou Pagnucco

David Roberson wrote:
 I may have been a bit to fast in pointing out the possible endothermic
 nature of the Ni62 and Ni64 reactions.  They actually are the best two
 isotopes to use if you were not to rely upon the beta plus decay for a
 substantial portion of the energy release.  They further are not
 susceptible to having the 511 keV gammas that would no doubt be released
 by the reactions involving the other nickel isotopes since copper 63 and
 65 are stable and do not decay into nickel by that process.

 So, if Rossi is actually able to overcome the coulomb barrier by some
 mechanism and his device only uses the Ni62 and Ni64 isotopes then it
 could be functional.  The energy released per atom for these two isotopes
 is only 1 or 2  MeV after satisfying the coulomb barrier, but that is a
 lot more than any chemical reaction can deliver.  I wonder if the
 relatively modest amount of energy release also can be more safely
 directed toward useful forms such as vibrational coupling into the
 surrounding structure.

 All of my estimates and calculations assume the reaction path that has
 been suggested by Rossi instead of the WL process which would be much
 more energetic.  Each of these proposed mechanisms has it's own particular
 problems to overcome.

 Dave



 -Original Message-
 From: David Roberson dlrober...@aol.com mailto:dlrober...@aol.com
 To: vortex-l vortex-l@eskimo.com mailto:vortex-l@eskimo.com
 Sent: Mon, Jun 4, 2012 10:30 am
 Subject: Re: [Vo]:about Triumph Management (and LENR)


 I just wanted to point out that if Ni62 and Ni64 are the only isotopes
 that work then the addition of a proton to either results in the
 production of a stable isotope of copper which does not undergo beta plus
 decay.  Much less energy is released per atom if the beta plus decay is
 avoided.  My calculations suggest that these two reactions might actually
 be endothermic due to the large coulomb barrier.

 Perhaps this is a bit of misdirection?

 Dave



 -Original Message-
 From: integral.property.service integral.property.serv...@gmail.com 
mailto:integral.property.serv...@gmail.com
 To: vortex-l vortex-l@eskimo.com mailto:vortex-l@eskimo.com
 Sent: Mon, Jun 4, 2012 9:30 am
 Subject: Re: [Vo]:about Triumph Management (and 

[Vo]:discussion about RELIABILITY in LENR

2012-06-05 Thread Peter Gluck
Dear Colleagues,

I hope to discuss a lot of LENR subjects
with our colleague Abd.
Today, now, here:
http://egooutpeters.blogspot.ro/2012/06/discussing-with-my-colleague-abd-about.html
starting to exchange ideas re Reliability in CF/LENR.
Far from agreement but this makes a dispute interesting.

Peter
-- 
Dr. Peter Gluck
Cluj, Romania
http://egooutpeters.blogspot.com


Re: [Vo]:discussion about RELIABILITY in LENR

2012-06-05 Thread Peter Gluck
Dear Reliable,

I think you have an special personal interest in this discussion about
Reliability.
I know well the paper of Bushnell, everything OK
however windows do not melt, they break- have seen  many major accident and
have read about
Seveso, Flixborough, Oppau, Chernobyl
Why Bushnell does not tell wher and when the
windows melted. Is this a reliable statement?
Peter

On Tue, Jun 5, 2012 at 11:36 PM, integral.property.serv...@gmail.com 
integral.property.serv...@gmail.com wrote:

 G'Day,

 Bushnell says it all.

 http://futureinnovation.larc.**nasa.gov/view/articles/**
 futurism/bushnell/low-energy-**nuclear-reactions.htmlhttp://futureinnovation.larc.nasa.gov/view/articles/futurism/bushnell/low-energy-nuclear-reactions.html
 _Dennis Bushnell http://futureinnovation.larc.**nasa.gov/view/articles/**
 futurism/bushnell/bushnell-**bio.htmlhttp://futureinnovation.larc.nasa.gov/view/articles/futurism/bushnell/bushnell-bio.html
 _
 The current experiments are in the 10's to hundreds range. However,
 several labs have blown up studying LENR and windows have melted,
 indicating when the conditions are right prodigious amounts of energy can
 be produced and released.

 Warm Regards,

 Reliable


 Peter Gluck wrote:

 Dear Colleagues,

 I hope to discuss a lot of LENR subjects
 with our colleague Abd.
 Today, now, here: http://egooutpeters.blogspot.**
 ro/2012/06/discussing-with-my-**colleague-abd-about.htmlhttp://egooutpeters.blogspot.ro/2012/06/discussing-with-my-colleague-abd-about.html
 starting to exchange ideas re Reliability in CF/LENR.
 Far from agreement but this makes a dispute interesting.

 Peter
 --
 Dr. Peter Gluck
 Cluj, Romania
 http://egooutpeters.blogspot.**com http://egooutpeters.blogspot.com





-- 
Dr. Peter Gluck
Cluj, Romania
http://egooutpeters.blogspot.com


Re: [Vo]:What Happened in CE 774?

2012-06-05 Thread Harry Veeder
Maybe it was due to a terrestial LENR event belched up by volcano.

Harry

On Tue, Jun 5, 2012 at 9:59 AM, David Roberson dlrober...@aol.com wrote:
 I agree with you Terry that it could likely be some form of solar event.
 Maybe you should check the historical sun spot record if available for that
 time frame to get some form of correlation.

 It also makes one wonder if similar, ever more powerful, events in history
 have resulted in a driving mechanism for evolution.  The poor creatures
 around during such an occasion would not even know what hit them!  If this
 type of event happens frequently in the history of life on earth one would
 expect DNA to have a built in mechanism to correct for a moderate radiation
 burst.   I do recall reading about repeated sequences within our DNA and
 these bursts might indicate a good reason for that to be true.

 Dave




 -Original Message-
 From: Terry Blanton hohlr...@gmail.com
 To: vortex-l vortex-l@eskimo.com
 Sent: Tue, Jun 5, 2012 8:37 am
 Subject: [Vo]:What Happened in CE 774?

 http://www.nature.com/news/mysterious-radiation-burst-recorded-in-tree-rings-1.10768

 Just over 1,200 years ago, the planet was hit by an extremely intense
 burst of high-energy radiation of unknown cause, scientists studying
 tree-ring data have found.

 http://www.nature.com/nature/journal/vaop/ncurrent/full/nature11123.html

 Is it possible that our sun generated an unprecedented energy burst?

 T




Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread mixent
In reply to  David Roberson's message of Tue, 5 Jun 2012 11:24:41 -0400 (EDT):
Hi,
[snip]
I took a table of nuclides and performed a Energy difference between the 
different nickel isotopes, plus associated proton and electron, and the 
daughter copper isotopes and compared the net released energy to the energy 
required to overcome the coulomb barrier.  The most significant energy release 
which exceeds the barrier occurs when the Ni62 or 

You don't need any energy to overcome the Coulomb barrier, if the proton is
accompanied by an electron.
Regards,

Robin van Spaandonk

http://rvanspaa.freehostia.com/project.html



Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread mixent
In reply to  David Roberson's message of Tue, 5 Jun 2012 11:24:41 -0400 (EDT):
Hi,
[snip]
Coulomb Barrier Energy ~5.6 MeV according to Rossi in his paper

I seriously doubt that Rossi has any idea how this actually works.

Regards,

Robin van Spaandonk

http://rvanspaa.freehostia.com/project.html



Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread David Roberson

You would not need to overcome the Coulomb barrier if the electron-proton 
combination is bound together tightly.  In that case the attraction that the 
electron sees is balanced by the repulsion afforded the proton.  Perhaps a 
torque would be generated or some form of extreme tension would be applied to 
whatever type of bond exists between the two, especially if they formed some 
form of dipole spatial arrangement.

A neutron of course would behave in this manner, but so would a hydrino that is 
of low energy.  One problem that needs to be understood is that Rossi insists 
that copper is his only transformed element and that would suggest that a 
proton is driven into the nickel nucleus and not an electron-proton pair.  We 
will need to determine what happened to the energy associated with the electron 
in the pair and also why this reaction is not extremely common in the world.

I tend to believe that a barrier does prevent the reaction from occurring at 
low temperatures, but that it might be subject to reduction by electron 
screening of some sort.  Many questions remain to be answered.

It perplexes me when I try to understand why there is no problem with gamma 
radiation.  At this point in my understanding, I am not ready to accept the WL 
explanation as they require too many miracles.  I am inclined to believe that 
the only way to prevent the gammas from killing us all is for them to be 
suppressed from the beginning.  Perhaps the dense nature of the nickel crystal 
substrate does allow phonon processes to absorb the released energy.  One day 
it will seem obvious. 

Dave 


-Original Message-
From: mixent mix...@bigpond.com
To: vortex-l vortex-l@eskimo.com
Sent: Tue, Jun 5, 2012 5:49 pm
Subject: Re: [Vo]:about Triumph Management (and LENR)


In reply to  David Roberson's message of Tue, 5 Jun 2012 11:24:41 -0400 (EDT):
i,
snip]
I took a table of nuclides and performed a Energy difference between the 
ifferent nickel isotopes, plus associated proton and electron, and the daughter 
opper isotopes and compared the net released energy to the energy required to 
vercome the coulomb barrier.  The most significant energy release which exceeds 
he barrier occurs when the Ni62 or 
You don't need any energy to overcome the Coulomb barrier, if the proton is
ccompanied by an electron.
egards,
Robin van Spaandonk
http://rvanspaa.freehostia.com/project.html



Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread David Roberson

You may be correct in your assumption regarding knowledge, but there must be 
some level of barrier or LENR would be occurring all over the place, all the 
time.  I read somewhere that about 100 keV is in the ballpark for the barrier 
of hydrogen to hydrogen hot fusion.  Since the repulsion is proportional to the 
product of the number of protons, one obtains a guesstimate of 2.8 MeV if you 
use the number of protons in nickel(28) versus the 1 of the target hydrogen 
nucleus.  I am sure the actual barrier value is different than my rough 
calculation due to electron shielding and the actual distance required before 
the strong force takes over among other effects.

If anyone has an accurate barrier value for us to plug into our assumption 
please submit it.

Dave  



-Original Message-
From: mixent mix...@bigpond.com
To: vortex-l vortex-l@eskimo.com
Sent: Tue, Jun 5, 2012 5:51 pm
Subject: Re: [Vo]:about Triumph Management (and LENR)


In reply to  David Roberson's message of Tue, 5 Jun 2012 11:24:41 -0400 (EDT):
i,
snip]
Coulomb Barrier Energy ~5.6 MeV according to Rossi in his paper
I seriously doubt that Rossi has any idea how this actually works.
Regards,
Robin van Spaandonk
http://rvanspaa.freehostia.com/project.html



Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread mixent
In reply to  integral.property.serv...@gmail.com's message of Tue, 05 Jun 2012
11:38:12 -0500:
Hi,
[snip]
Robin,

http://www.journal-of-nuclear-physics.com/?p=338

Contrary to Feynman's hand waving use of the Heisenberg uncertainty principle,
there is no restriction imposed by this principle on the size of Hydrogen atoms.
(See at the end of http://rvanspaa.freehostia.com/theory-paper.html )

Hence the implication in the above paper that such orbitals can only exist
momentarily on that basis is incorrect.

For a mathematical description of such orbitals see:

http://rvanspaa.freehostia.com/Non-relativisitic.pdf


http://www.ecatplanet.net/rossiblog.php?msg_search=Guglinski
e+p+e = Hydride Anion = *
1. Trap * in lattice (Ni nano, C nano Cone, etc.)
2. Activate * {Cavitation, heat, RFG, Arc, coordinated oscillations, 
Lattice wave creation, etc.}
3. p+e portion of * enters Ni nucleus creating unstable isotope leaving 
e behind for charge balance.

This sounds a lot like Horace Heffner's theory. See
http://www.mtaonline.net/~hheffner/DeflationFusion.pdf

4. Ni Isotope = Cu + Cold Fusion Energy
6. Don't bother with trying to determine reaction with Quantitative 
Analysis, Mass changes incredibly small and energy incredibly large. E=MC2
[snip]
Regards,

Robin van Spaandonk

http://rvanspaa.freehostia.com/project.html



[Vo]:Transit of Venus - Live Stream

2012-06-05 Thread Patrick Ellul
Best stream i found so far. http://www.ustream.tv/nasaedge
Enjoy.

-- 
Patrick

www.tRacePerfect.com
The daily puzzle everyone can finish but not everyone can perfect!
The quickest puzzle ever!


Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread mixent
In reply to  David Roberson's message of Tue, 5 Jun 2012 18:38:46 -0400 (EDT):
Hi,
[snip]
A neutron of course would behave in this manner, but so would a hydrino that 
is of low energy.  One problem that needs to be understood is that Rossi 
insists that copper is his only transformed element and that would suggest 
that a proton is driven into the nickel nucleus and not an electron-proton 
pair.

Mills Hydrino may not get small enough to decrease the tunneling time for Ni, to
a sufficiently noticeable degree, however in my version, the Hydrino can shrink
to just a few fm, allowing it to come within range of the nuclear force, hence
effectively bypassing the Coulomb barrier altogether.

In Horace's theory, the electron actually enters the nucleus along with the
proton.

In my version, the electron may also momentarily get sucked in along with the
proton, then immediately ejected via an Internal Conversion reaction, carrying
the energy of the fusion reaction with it. This would produce fast electrons,
about 1% of which would produce x-rays, some of which would be hard (hence the
need for Pb shielding in Rossi's reactor).

As for Copper being the only product, even Rossi himself admits that a thorough
metals analysis is required to settle this issue (see his post about 40 hours @
600 ºC).

BTW the Hydrino concept in general implies that some portion of the energy comes
from Hydrino shrinkage. What that percentage might be is yet to be determined,
although based on the lack of external radiation, one might guess that it is
large, and that consequently the nuclear reactions are in fact only supplying a
small portion. 

Regards,

Robin van Spaandonk

http://rvanspaa.freehostia.com/project.html



Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread David Roberson

On occasion I find myself liking the hydrino concept.  The gamma radiation 
associated with element mutation is hard to accept without assuming a large 
amount of leakage.

Unfortunately, there are some serious questions as to whether or not hydinos 
exist.

It would be convenient if the proton and electron were sucked into the nucleus 
since that would eliminate the barrier entirely.   If this is true, why is it 
difficult to achieve rapid LENR activity and the corresponding high powers?  
Has anyone been able to answer the question as to why the reaction rate is 
relatively low under this condition?

Is it possible that the reaction rate for LENR devices is throttled by the lack 
of hydrinos or your version of them?   Maybe they are not too easily 
constructed in the real world and that is why a special condition must be 
achieved where they can be generated.  That would be a neat reason for the 
difficulties encountered in our experiments.  If this is the case, it would be 
a good idea to concentrate on a method of controlled generation for these 
components.

I wonder about the electron being ejected from the nucleus with all of the 
reaction energy.  Has anyone calculated how much ionization would be generated 
by an electron with 6 MeV of energy?  Would that not be easy to see in the 
experiments?

We are limited in our thought processes by the lack of data and I can hardly 
wait until we finally obtain output material from Rossi's and DGT's devices 
that can be independently measured.

Dave



-Original Message-
From: mixent mix...@bigpond.com
To: vortex-l vortex-l@eskimo.com
Sent: Tue, Jun 5, 2012 7:14 pm
Subject: Re: [Vo]:about Triumph Management (and LENR)


In reply to  David Roberson's message of Tue, 5 Jun 2012 18:38:46 -0400 (EDT):
i,
snip]
A neutron of course would behave in this manner, but so would a hydrino that is 
f low energy.  One problem that needs to be understood is that Rossi insists 
hat copper is his only transformed element and that would suggest that a proton 
s driven into the nickel nucleus and not an electron-proton pair.
Mills Hydrino may not get small enough to decrease the tunneling time for Ni, to
 sufficiently noticeable degree, however in my version, the Hydrino can shrink
o just a few fm, allowing it to come within range of the nuclear force, hence
ffectively bypassing the Coulomb barrier altogether.
In Horace's theory, the electron actually enters the nucleus along with the
roton.
In my version, the electron may also momentarily get sucked in along with the
roton, then immediately ejected via an Internal Conversion reaction, carrying
he energy of the fusion reaction with it. This would produce fast electrons,
bout 1% of which would produce x-rays, some of which would be hard (hence the
eed for Pb shielding in Rossi's reactor).
As for Copper being the only product, even Rossi himself admits that a thorough
etals analysis is required to settle this issue (see his post about 40 hours @
00 ºC).
BTW the Hydrino concept in general implies that some portion of the energy comes
rom Hydrino shrinkage. What that percentage might be is yet to be determined,
lthough based on the lack of external radiation, one might guess that it is
arge, and that consequently the nuclear reactions are in fact only supplying a
mall portion. 
Regards,
Robin van Spaandonk
http://rvanspaa.freehostia.com/project.html



Re: [Vo]:Transit of Venus - Live Stream

2012-06-05 Thread Harry Veeder
thanks.
Harry

On Tue, Jun 5, 2012 at 7:02 PM, Patrick Ellul ellulpatr...@gmail.com wrote:
 Best stream i found so far. http://www.ustream.tv/nasaedge
 Enjoy.

 --
 Patrick

 www.tRacePerfect.com
 The daily puzzle everyone can finish but not everyone can perfect!
 The quickest puzzle ever!




Re: [Vo]:Transit of Venus - Live Stream

2012-06-05 Thread Patrick Ellul
welcome. Please do share if you find a better stream.

On Wed, Jun 6, 2012 at 10:51 AM, Harry Veeder hveeder...@gmail.com wrote:

 thanks.
 Harry

 On Tue, Jun 5, 2012 at 7:02 PM, Patrick Ellul ellulpatr...@gmail.com
 wrote:
  Best stream i found so far. http://www.ustream.tv/nasaedge
  Enjoy.
 
  --
  Patrick
 
  www.tRacePerfect.com
  The daily puzzle everyone can finish but not everyone can perfect!
  The quickest puzzle ever!
 




-- 
Patrick

www.tRacePerfect.com
The daily puzzle everyone can finish but not everyone can perfect!
The quickest puzzle ever!


Re: [Vo]:Transit of Venus - Live Stream

2012-06-05 Thread Harry Veeder
I'd be interested to know if anyone was able to see the transit with a
crude pinhole camera. I tried but the clouds would not co-operate.


harry

On Tue, Jun 5, 2012 at 8:57 PM, Patrick Ellul ellulpatr...@gmail.com wrote:
 welcome. Please do share if you find a better stream.

 On Wed, Jun 6, 2012 at 10:51 AM, Harry Veeder hveeder...@gmail.com wrote:

 thanks.
 Harry

 On Tue, Jun 5, 2012 at 7:02 PM, Patrick Ellul ellulpatr...@gmail.com
 wrote:
  Best stream i found so far. http://www.ustream.tv/nasaedge
  Enjoy.
 
  --
  Patrick
 
  www.tRacePerfect.com
  The daily puzzle everyone can finish but not everyone can perfect!
  The quickest puzzle ever!
 




 --
 Patrick

 www.tRacePerfect.com
 The daily puzzle everyone can finish but not everyone can perfect!
 The quickest puzzle ever!




Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread Terry Blanton
On Tue, Jun 5, 2012 at 9:12 PM, Jones Beene jone...@pacbell.net wrote:

 This is why many of us keep saying that Mills is his own worst enemy for not
 following up on promises to release samples for independent testing. He may
 be forced to do this if Rossi is really making the progress he is claiming
 (highly doubtful).

It's amazing how so many people do not listen even though they read
this list.  Lately, I am amused by those who try to explain the
dissociation of the H2 molecule otherwise than the metal surface
explanations we have discussed.

So, Beene, who do you think will win the race?  It seems to be getting
close.  Ahern?

T



Re: [Vo]:Transit of Venus - Live Stream

2012-06-05 Thread Robert
I used a pair of binoculars to project the image of the transit on to a dark 
surface. With a bit of eyepiece-focusing, the transit was quite clear.
I think that the Venus blemish may be too small to be coherent with a simple 
pinhole.

Harry Veeder hveeder...@gmail.com wrote:

I'd be interested to know if anyone was able to see the transit with a
crude pinhole camera. I tried but the clouds would not co-operate.


harry

On Tue, Jun 5, 2012 at 8:57 PM, Patrick Ellul ellulpatr...@gmail.com wrote:
 welcome. Please do share if you find a better stream.

 On Wed, Jun 6, 2012 at 10:51 AM, Harry Veeder hveeder...@gmail.com wrote:

 thanks.
 Harry

 On Tue, Jun 5, 2012 at 7:02 PM, Patrick Ellul ellulpatr...@gmail.com
 wrote:
  Best stream i found so far. http://www.ustream.tv/nasaedge
  Enjoy.
 
  --
  Patrick
 
  www.tRacePerfect.com
  The daily puzzle everyone can finish but not everyone can perfect!
  The quickest puzzle ever!
 




 --
 Patrick

 www.tRacePerfect.com
 The daily puzzle everyone can finish but not everyone can perfect!
 The quickest puzzle ever!





Re: [Vo]:discussion about RELIABILITY in LENR

2012-06-05 Thread Abd ul-Rahman Lomax

At 02:29 PM 6/5/2012, Peter Gluck wrote:

I hope to discuss a lot of LENR subjects
with our colleague Abd.
Today, now, here:
http://egooutpeters.blogspot.ro/2012/06/discussing-with-my-colleague-abd-about.htmlhttp://egooutpeters.blogspot.ro/2012/06/discussing-with-my-colleague-abd-about.html
starting to exchange ideas re Reliability in CF/LENR.
Far from agreement but this makes a dispute interesting.


I don't see that we are far from agreement, but 
maybe Peter sees something I don't.


Here is the discussion, with my responses interspersed:


DISCUSSING WITH MY COLLEAGUE ABD ABOUT RELIABILITY
I have to apologize again, my old age weaknesses allow me
 to answer to Abd only step by step, in fragments to his so well
 ordered arguments. I have to recognize that in 
our LENR circles, what he says is more happily/readily accepted than my ideas.


Perhaps. What that means, I don't know. Maybe 
nothing. Peter, you have extensive experience, 
which is to be respected. I'm a writer, so it's 
my business to be effectively communicative. I'm still learning, though.



 So, now about reliability.


[I wrote:]

Well, they *may be* inherent weaknesses of PdD 
LENR set up by known methods. A premature 
vision of an ultimate application can kill new 
discoveries, allowing them to be dismissed as 
worthless even if they are real, and if their 
reality is in question, it's a double whammy. 
What we need is Science, and it comes before 
Energy, if we need reliability for Energy. *We 
do not need reliability for Science.* It is desirable, that's all.


I think there definitely are inherent 
weaknesses, uncontrollable hidden parameters in 
the Pd-D cells and these are almost ubiquitous 
in this system. and difficultly curable. I have 
met similar things in my lab-pilot-plant 
practice, something that went fine 1000 times 
suddenly became impossible, a colorless product 
(as it has to be) coming out red or dirty grey 
with no obvious explanation first. Many times I 
was thinking to write a report about occult 
phenomena in technology, but then we found a 
simple straightforward causal explanation and we 
solved the problem by removing, killing that cause.


Yes. Until you identified the cause, it was 
totally mysterious. Gremlins. Bad juju. Whatever.



The weaknesses of the Pd D cells are unusually stubborn,


Electrochemical PdD experiments are *extremely* 
complex. With gas-loading, the complexity may be 
reduced, but a great deal depends on the exact 
structure of the particles or Pd material. And it 
will change with loading and deloading.


I am firmly convinced that poisoning of the 
active centers (NAE) by adsorption of gases that 
are NOT deuterium (it seems everything goes not 
only the very polar gases as I thought) explains 
this long series of troubles. I will write a new 
paper about poisoning these days. Nobody will believe it- just the Pd-D cells.


I'll believe it in that I consider it possible. 
Why not? However, I don't see this as explaining 
the difference between the first, second, and 
third current excursions in SRI P13/P14, which 
was a sealed cell. It's not impossible, though, 
because the first and second excursions, showing 
no heat, may have cleaned off the cathode.


It was crucial to identify the reasons for such 
variability. The skeptics did not get the import 
of variability, they thought that it meant that 
the effect was down in the noise. However, that's 
what SRI P13/P14 showed so clearly: the effect, 
when it appears, is striking, not marginal. Of 
course, sometimes there is an effect close to the 
noise. But a strong, quite visible effect is one 
of the characteristics of a successful 
replication of the FPHE, not something 
questionable, where we look at a plot and say, 
Well, see, it's a little bit above the noise 
there, for a few hours. Maybe. Or maybe that is 
just noise a little higher than usual.



Reality is really good if it is repeatable and it is bad when it plays
 perfidiously hide and seek with us.


Ultimately, it appears, reality does play hide 
and seek, at the quantum level. But I don't think 
that's happening here. Regardless, reality is not 
bad. Period. It's just reality. We make up good 
and bad. This is not you, but scientists who 
reject experimental data because they don't see 
repeatability in it are just fooling themselves. 
What they don't see means nothing. Saying I 
don't understand this is fine. Saying you must 
have made a mistake, is the problem, unless the 
error can be identified. Not just guessed.


I agree with Abd re the premature vision- it is 
not good to focus only and immediately on 
applications and not explore the full richness 
of the phenomena, process, and product, whatever.


It's not as powerful, and it runs the risk of an 
enormous waste of time. Look, it was obvious from 
the beginning that there *might be* enormous 
promise from cold fusion. But it was also 
obvious, within a few months, that this was not 
going to be easy, at least 

Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread pagnucco
Thanks ny.min,

I assumed that a neutron was captured by 62Ni which then beta-decays to
63Cu.  (Unless my quick calculations are wrong,) when you substract the
minimum energy required to form a neutron from an electron + proton
(approx. 780 Kev) from the energy released from that beta-day, you do wind
up with about an excess of over 0.006[u] energy - close to your
calculation.

I am not sure whether you are proposing direct proton capture via
screening.  If not, it looks like either W-L theory, or hydrinos could
explain the transmutations Rossi is claiming.

Lou Pagnucco

ny.min wrote:
 http://sire.com/fusion.htm

 -Original Message-
 From: pagnucco lt;pagnu...@htdconnect.comgt;
 To: vortex-l lt;vortex-l@eskimo.comgt;
 Sent: Mon, Jun 4, 2012 10:49 pm
 Subject: Re: [Vo]:about Triumph Management (and LENR)




 David,

 Can you explain your conclusion.
 I can't see how any energy is released in these Ni --gt; Cu
 transmutations.

 Lou Pagnucco

 David Roberson wrote:
 gt; I may have been a bit to fast in pointing out the possible
 endothermic
 gt; nature of the Ni62 and Ni64 reactions.  They actually are the best
 two
 gt; isotopes to use if you were not to rely upon the beta plus decay for
 a
 gt; substantial portion of the energy release.  They further are not
 gt; susceptible to having the 511 keV gammas that would no doubt be
 released
 gt; by the reactions involving the other nickel isotopes since copper 63
 and
 gt; 65 are stable and do not decay into nickel by that process.
 gt;
 gt; So, if Rossi is actually able to overcome the coulomb barrier by some
 gt; mechanism and his device only uses the Ni62 and Ni64 isotopes then it
 gt; could be functional.  The energy released per atom for these two
 isotopes
 gt; is only 1 or 2  MeV after satisfying the coulomb barrier, but that is
 a
 gt; lot more than any chemical reaction can deliver.  I wonder if the
 gt; relatively modest amount of energy release also can be more safely
 gt; directed toward useful forms such as vibrational coupling into the
 gt; surrounding structure.
 gt;
 gt; All of my estimates and calculations assume the reaction path that
 has
 gt; been suggested by Rossi instead of the WL process which would be
 much
 gt; more energetic.  Each of these proposed mechanisms has it's own
 particular
 gt; problems to overcome.
 gt;
 gt; Dave
 gt;
 gt;
 gt;
 gt; -Original Message-
 gt; From: David Roberson lt;dlrober...@aol.comgt;
 gt; To: vortex-l lt;vortex-l@eskimo.comgt;
 gt; Sent: Mon, Jun 4, 2012 10:30 am
 gt; Subject: Re: [Vo]:about Triumph Management (and LENR)
 gt;
 gt;
 gt; I just wanted to point out that if Ni62 and Ni64 are the only
 isotopes
 gt; that work then the addition of a proton to either results in the
 gt; production of a stable isotope of copper which does not undergo beta
 plus
 gt; decay.  Much less energy is released per atom if the beta plus decay
 is
 gt; avoided.  My calculations suggest that these two reactions might
 actually
 gt; be endothermic due to the large coulomb barrier.
 gt;
 gt; Perhaps this is a bit of misdirection?
 gt;
 gt; Dave
 gt;
 gt;
 gt;
 gt; -Original Message-
 gt; From: integral.property.service
 lt;integral.property.serv...@gmail.comgt;
 gt; To: vortex-l lt;vortex-l@eskimo.comgt;
 gt; Sent: Mon, Jun 4, 2012 9:30 am
 gt; Subject: Re: [Vo]:about Triumph Management (and LENR)
 gt;
 gt;
 gt; A.R. from Florida with love,
 gt; Andrea Rossi











Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread pagnucco
David,

According to my rough calculations the Ni-to-Cu transmutations do release
significant energy, as you claimed - see my reply to ny.min.  I am not
sure how much energy is siphoned off by the neutrino, though.

I assumed a neutron capture by the Ni nucleus, so no there would be no
need to consider the coulomb barrier.  Excess energy is released, if we
assume the conversion of electron+proton--to--neutron takes approximately
780 Kev.  So W-L theory, or hydrinos, or some kind of screening, could
explain the transmutations, if they are real.

Lou Pagnucco

David Roberson wrote:
 I took a table of nuclides and performed a Energy difference between the
 different nickel isotopes, plus associated proton and electron, and the
 daughter copper isotopes and compared the net released energy to the
 energy required to overcome the coulomb barrier.  The most significant
 energy release which exceeds the barrier occurs when the Ni62 or Ni64
 isotopes are converted.  The delayed beta plus decay which is present for
 all of the other transformations looses a large amount of energy to a
 neutrino which promptly escapes the device.  I will demonstrate the
 numbers below.

 These components are required to build Cu63 from Ni62
 1 u = 931.494 MeV  Disregard the slight rounding errors, excel chart
 source of data

 Ni62  Mass=61.92835 (u)  Energy=57685.88 MeV
 Proton Mass=1.007276 (u)  Energy=938.2716 MeV
 Electron Mass=.000549 (u) Energy=.510999 MeV

 Coulomb Barrier Energy ~5.6 MeV according to Rossi in his paper

 Cu63 Mass=62.9296 (u) Energy=58618.54 MeV

 Mass of components of Cu63;Ni62 + Proton + Electron=62.936175 (u)
 Energy=58624.66 MeV

 Mass decrease that must be released as energy=62.936175 - 62.9296 =
 .006575 (u) Energy=  6.12457 MeV - 5.6 MeV Barrier = .52457 MeV;Same
 Calculation for Cu65 yields 1.8532 MeV
 In these reactions there are no Beta Plus Decay radiation losses due to
 neutrino release and no 511 keV gammas.

 Please note that I also calculated the expected energy release due to WL
 process on the isotopes such as Ni60 and had perfect energy correlation
 when the energy required to make a neutron from a proton and electron is
 included.

 Exactly the same energy is seen in both paths (Rossi and WL)  when the
 starting point is a nickel isotope with a proton and an electron, and the
 final point is the next higher isotope of nickel.

 I am working very hard to get a clear understanding of the coulomb barrier
 energy behavior.  I can show that the alpha process within stars stops
 once iron has been synthesized, but this is only true if the barrier
 energy is trapped within the nucleus in the form of mass.  I am
 approaching the problem from different directions to prove whether or not
 this hypothesis is accurate.

 Dave


 -Original Message-
 From: pagnucco pagnu...@htdconnect.com
 To: vortex-l vortex-l@eskimo.com
 Sent: Mon, Jun 4, 2012 11:49 pm
 Subject: Re: [Vo]:about Triumph Management (and LENR)


 David,
 Can you explain your conclusion.
  can't see how any energy is released in these Ni -- Cu transmutations.
 Lou Pagnucco
 David Roberson wrote:
  I may have been a bit to fast in pointing out the possible endothermic
  nature of the Ni62 and Ni64 reactions.  They actually are the best two
  isotopes to use if you were not to rely upon the beta plus decay for a
  substantial portion of the energy release.  They further are not
  susceptible to having the 511 keV gammas that would no doubt be released
  by the reactions involving the other nickel isotopes since copper 63 and
  65 are stable and do not decay into nickel by that process.

  So, if Rossi is actually able to overcome the coulomb barrier by some
  mechanism and his device only uses the Ni62 and Ni64 isotopes then it
  could be functional.  The energy released per atom for these two isotopes
  is only 1 or 2  MeV after satisfying the coulomb barrier, but that is a
  lot more than any chemical reaction can deliver.  I wonder if the
  relatively modest amount of energy release also can be more safely
  directed toward useful forms such as vibrational coupling into the
  surrounding structure.

  All of my estimates and calculations assume the reaction path that has
  been suggested by Rossi instead of the WL process which would be much
  more energetic.  Each of these proposed mechanisms has it's own
 particular
  problems to overcome.

  Dave



  -Original Message-
  From: David Roberson dlrober...@aol.com
  To: vortex-l vortex-l@eskimo.com
  Sent: Mon, Jun 4, 2012 10:30 am
  Subject: Re: [Vo]:about Triumph Management (and LENR)


  I just wanted to point out that if Ni62 and Ni64 are the only isotopes
  that work then the addition of a proton to either results in the
  production of a stable isotope of copper which does not undergo beta plus
  decay.  Much less energy is released per atom if the beta plus decay is
  avoided.  My calculations suggest that these two reactions might actually
  be endothermic due to 

[Vo]:Mars One - Humans on Mars in 2023

2012-06-05 Thread Patrick Ellul
Funded by marketing it as one big reality show... Possible?? And would you
buy a one way ticket to Mars?

http://mars-one.com/en/

Regards,
Patrick

-- 
Patrick

www.tRacePerfect.com
The daily puzzle everyone can finish but not everyone can perfect!
The quickest puzzle ever!


Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread mixent
In reply to  David Roberson's message of Tue, 5 Jun 2012 20:42:05 -0400 (EDT):
Hi,
[snip]

On occasion I find myself liking the hydrino concept.  The gamma radiation 
associated with element mutation is hard to accept without assuming a large 
amount of leakage.

If the electron is ejected, which is a fast reaction, then there is no gamma
radiation produced (slow reaction).
Another possibility is that the reacting particle is actually a Hydrino
molecule, and that one of the two protons gets ejected carrying the energy.
Since protons are far more massive than electrons, they produce almost no
bremsstrahlung.
Where proton addition would create an unstable nucleus, it's also possible that
the electron is captured in an enhanced electron capture reaction. I say
enhanced because in normal EC reactions the nucleus has to try to grab a
fast moving K electron on it's way through, whereas the Hydrino electron is
already present, and not really intent on going anywhere. ;-)


Unfortunately, there are some serious questions as to whether or not hydinos 
exist.

Indeed!


It would be convenient if the proton and electron were sucked into the nucleus 
since that would eliminate the barrier entirely.   If this is true, why is it 
difficult to achieve rapid LENR activity and the corresponding high powers?  
Has anyone been able to answer the question as to why the reaction rate is 
relatively low under this condition?

Lack of sufficiently shrunken Hydrinos. As they get smaller is gets ever more
difficult to catalyze shrinkage to a lower level.
(I suspect the primary reason why Mills is using H[n=1/4]).


Is it possible that the reaction rate for LENR devices is throttled by the 
lack of hydrinos or your version of them?

Highly probable; see above.

   Maybe they are not too easily constructed in the real world and that is why 
 a special condition must be achieved where they can be generated.  That would 
 be a neat reason for the difficulties encountered in our experiments.  If 
 this is the case, it would be a good idea to concentrate on a method of 
 controlled generation for these components.

I've already found it (in theory), I just need a bit of technical (engineering)
help, and the finances to do it. Depending on what has to be paid for and how
much it costs, the cost could vary anywhere from nothing to say 100 grand.
Any university with an engineering department and a few willing grad students
could probably do it for nothing. The device is quite simple.
Testing it however could be a bit dicey, as it *might* produce copious gamma
rays.
It should produce power at the (multi)kilowatt level.
(Consistently and controllably over a wide range).


I wonder about the electron being ejected from the nucleus with all of the 
reaction energy.  Has anyone calculated how much ionization would be generated 
by an electron with 6 MeV of energy?  Would that not be easy to see in the 
experiments?

Beta emitters are generally relatively easily shielded AFAIK. However there are
not many multi kilowatt beta emitters around!


We are limited in our thought processes by the lack of data and I can hardly 
wait until we finally obtain output material from Rossi's and DGT's devices 
that can be independently measured.

:-)

Regards,

Robin van Spaandonk

http://rvanspaa.freehostia.com/project.html



Re: [Vo]:Mars One - Humans on Mars in 2023

2012-06-05 Thread mixent
In reply to  Patrick Ellul's message of Wed, 6 Jun 2012 14:10:21 +1000:
Hi,
[snip]

I wrote to Elon Musk offering to help him build a fusion powered shuttle to get
us there in 2 days at 1 g with only 20% fuel mass. 

No response.


Funded by marketing it as one big reality show... Possible?? And would you
buy a one way ticket to Mars?

http://mars-one.com/en/

Regards,
Patrick
Regards,

Robin van Spaandonk

http://rvanspaa.freehostia.com/project.html



Re: [Vo]:Mars One - Humans on Mars in 2023

2012-06-05 Thread Daniel Rocha
Realities shows are successful because the success of one relies on the
humiliation and exclusion of other participants, like in the
old Coliseum. That is not possible in this mission, though, unless you kill
passengers, like in the old Coliseum.

2012/6/6 Patrick Ellul ellulpatr...@gmail.com

 Funded by marketing it as one big reality show... Possible?? And would you
 buy a one way ticket to Mars?

 http://mars-one.com/en/

 Regards,
 Patrick

 --
 Patrick

 www.tRacePerfect.com
 The daily puzzle everyone can finish but not everyone can perfect!
 The quickest puzzle ever!




-- 
Daniel Rocha - RJ
danieldi...@gmail.com


Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread David Roberson

The half life of Ni63 is 98.7 years.  That path would not be useful in Rossi's 
device.

Dave



-Original Message-
From: pagnucco pagnu...@htdconnect.com
To: vortex-l vortex-l@eskimo.com
Sent: Tue, Jun 5, 2012 11:14 pm
Subject: Re: [Vo]:about Triumph Management (and LENR)


Thanks ny.min,
I assumed that a neutron was captured by 62Ni which then beta-decays to
3Cu.  (Unless my quick calculations are wrong,) when you substract the
inimum energy required to form a neutron from an electron + proton
approx. 780 Kev) from the energy released from that beta-day, you do wind
p with about an excess of over 0.006[u] energy - close to your
alculation.
I am not sure whether you are proposing direct proton capture via
creening.  If not, it looks like either W-L theory, or hydrinos could
xplain the transmutations Rossi is claiming.
Lou Pagnucco
ny.min wrote:
 http://sire.com/fusion.htm

 -Original Message-
 From: pagnucco lt;pagnu...@htdconnect.comgt;
 To: vortex-l lt;vortex-l@eskimo.comgt;
 Sent: Mon, Jun 4, 2012 10:49 pm
 Subject: Re: [Vo]:about Triumph Management (and LENR)




 David,

 Can you explain your conclusion.
 I can't see how any energy is released in these Ni --gt; Cu
 transmutations.

 Lou Pagnucco

 David Roberson wrote:
 gt; I may have been a bit to fast in pointing out the possible
 endothermic
 gt; nature of the Ni62 and Ni64 reactions.  They actually are the best
 two
 gt; isotopes to use if you were not to rely upon the beta plus decay for
 a
 gt; substantial portion of the energy release.  They further are not
 gt; susceptible to having the 511 keV gammas that would no doubt be
 released
 gt; by the reactions involving the other nickel isotopes since copper 63
 and
 gt; 65 are stable and do not decay into nickel by that process.
 gt;
 gt; So, if Rossi is actually able to overcome the coulomb barrier by some
 gt; mechanism and his device only uses the Ni62 and Ni64 isotopes then it
 gt; could be functional.  The energy released per atom for these two
 isotopes
 gt; is only 1 or 2  MeV after satisfying the coulomb barrier, but that is
 a
 gt; lot more than any chemical reaction can deliver.  I wonder if the
 gt; relatively modest amount of energy release also can be more safely
 gt; directed toward useful forms such as vibrational coupling into the
 gt; surrounding structure.
 gt;
 gt; All of my estimates and calculations assume the reaction path that
 has
 gt; been suggested by Rossi instead of the WL process which would be
 much
 gt; more energetic.  Each of these proposed mechanisms has it's own
 particular
 gt; problems to overcome.
 gt;
 gt; Dave
 gt;
 gt;
 gt;
 gt; -Original Message-
 gt; From: David Roberson lt;dlrober...@aol.comgt;
 gt; To: vortex-l lt;vortex-l@eskimo.comgt;
 gt; Sent: Mon, Jun 4, 2012 10:30 am
 gt; Subject: Re: [Vo]:about Triumph Management (and LENR)
 gt;
 gt;
 gt; I just wanted to point out that if Ni62 and Ni64 are the only
 isotopes
 gt; that work then the addition of a proton to either results in the
 gt; production of a stable isotope of copper which does not undergo beta
 plus
 gt; decay.  Much less energy is released per atom if the beta plus decay
 is
 gt; avoided.  My calculations suggest that these two reactions might
 actually
 gt; be endothermic due to the large coulomb barrier.
 gt;
 gt; Perhaps this is a bit of misdirection?
 gt;
 gt; Dave
 gt;
 gt;
 gt;
 gt; -Original Message-
 gt; From: integral.property.service
 lt;integral.property.serv...@gmail.comgt;
 gt; To: vortex-l lt;vortex-l@eskimo.comgt;
 gt; Sent: Mon, Jun 4, 2012 9:30 am
 gt; Subject: Re: [Vo]:about Triumph Management (and LENR)
 gt;
 gt;
 gt; A.R. from Florida with love,
 gt; Andrea Rossi











Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread mixent
In reply to  pagnu...@htdconnect.com's message of Tue, 5 Jun 2012 23:54:39 -0400
(EDT):
Hi,
[snip]
According to my rough calculations the Ni-to-Cu transmutations do release
significant energy, as you claimed - see my reply to ny.min.  I am not
sure how much energy is siphoned off by the neutrino, though.

From looking at many beta decay reactions I get the impression that roughly 2/3
of the energy goes to neutrinos, and 1/3 to the electron/positron, but it varies
from one reaction the next.

Regards,

Robin van Spaandonk

http://rvanspaa.freehostia.com/project.html



[Vo]:Mills Hyrdrino project (was :about Triumph Management (and LENR))

2012-06-05 Thread Jojo Jaro

Robin,

I read your webpage regarding this potential Fusion Project, although I 
found it rather lacking in detail and I am still unsure what you are trying 
to achieve or how to achieve it.  Are you in a position to reveal more of 
your theory in terms an Engineer amd a businessman can understand, not a 
physicist trained in Quantum Mechanics.  I'm sure I'm not alone in this 
forum that is eager to hear a comprehensive and clear presentation of your 
ideas just as Axil has superbly done.  Please gather your ideas into one 
comprehensive narrative and post them here or at your site.


Anyways, I am prepared to spend a small fortune in getting a commercial cold 
fusion reactor to the market, if (a big IF) I am convinced of the 
theoritical viability of the project.  I have been looking for such an 
opportunity as well as pursuing this goal myself.  Despite my obvious lack 
of success thus far, many times, I feel that I am closer to 
commericialization than Mill's endless hydrino pronounciations.


Quite honestly, Mills has had decades and considerably more than $100,000 
that you estimate, to bring his Hydrino Theory reactor to fruition without 
apparent success.  No insult or ridicule intended,  but what makes you think 
that you can build a reactor based on his theory that will outperform what 
he has produced so far, when the maestro himself has been unsuccessful?


Please do not take this post as a snide remark to ridicule or to insult.  I 
guenuinely want to know.



Jojo



- Original Message - 
From: mix...@bigpond.com

To: vortex-l@eskimo.com
Sent: Wednesday, June 06, 2012 12:13 PM
Subject: Re: [Vo]:about Triumph Management (and LENR)


I've already found it (in theory), I just need a bit of technical 
(engineering)
help, and the finances to do it. Depending on what has to be paid for and 
how

much it costs, the cost could vary anywhere from nothing to say 100 grand.
Any university with an engineering department and a few willing grad 
students

could probably do it for nothing. The device is quite simple.
Testing it however could be a bit dicey, as it *might* produce copious gamma
rays.
It should produce power at the (multi)kilowatt level.
(Consistently and controllably over a wide range).

Regards,

Robin van Spaandonk

http://rvanspaa.freehostia.com/project.html




Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread mixent
In reply to  David Roberson's message of Wed, 6 Jun 2012 00:27:52 -0400 (EDT):
Hi,
[snip]

The half life of Ni63 is 98.7 years.  That path would not be useful in Rossi's 
device.

The capture alone yields over 6 MeV. The beta decay energy is tiny by
comparison. Unless you are implying that the reaction is not useful because the
Ni63 would remain radioactive for so long. However Ni63 could be a useful
portable/remote/no-moving-parts energy source. Initially about 32 W/kg, dropping
off to half that after 100 years. Think of the sort of applications that
currently use solar panels.
Regards,

Robin van Spaandonk

http://rvanspaa.freehostia.com/project.html



Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread David Roberson


Lou,
 
If WL works and you capture a neutron to form Ni63 from Ni62 you would have a 
half life of 98.7 years before the beta decay.   There would be a very small 
quantity of Cu63 as a result.

I have made numerous calculations which demonstrate that you get the same 
amount of energy release regardless of the path between two of these points as 
long as you start and end at the same isotopes.  As example, Ni62 + neutron = 
Ni63 plus energy.  Next Ni63 beta decays to Cu63 and releases energy.  The sum 
of these energy releases is exactly the same as if you take Ni62 and add a 
proton and electron to arrive at Cu63.  You must subtract the energy of 
formation for the neutron from the first path to make the balance.

In this beta decay:Ni63 to Cu63 the neutrino has 49.52 keV while the beta 
particle has 17.425 keV.  Most of the energy shows up in the neutrino which 
seems typical of the beta plus decays as well.  The decay energy in this case 
is much less than in the other more typical examples.  The beta plus decay of 
Cu59 into Ni59 releases 3.7773 MeV typically.  Only 1.7226 MeV is given to the 
positron.

Dave




-Original Message-
From: pagnucco pagnu...@htdconnect.com
To: vortex-l vortex-l@eskimo.com
Sent: Tue, Jun 5, 2012 11:54 pm
Subject: Re: [Vo]:about Triumph Management (and LENR)


David,
According to my rough calculations the Ni-to-Cu transmutations do release
ignificant energy, as you claimed - see my reply to ny.min.  I am not
ure how much energy is siphoned off by the neutrino, though.
I assumed a neutron capture by the Ni nucleus, so no there would be no
eed to consider the coulomb barrier.  Excess energy is released, if we
ssume the conversion of electron+proton--to--neutron takes approximately
80 Kev.  So W-L theory, or hydrinos, or some kind of screening, could
xplain the transmutations, if they are real.
Lou Pagnucco
David Roberson wrote:
 I took a table of nuclides and performed a Energy difference between the
 different nickel isotopes, plus associated proton and electron, and the
 daughter copper isotopes and compared the net released energy to the
 energy required to overcome the coulomb barrier.  The most significant
 energy release which exceeds the barrier occurs when the Ni62 or Ni64
 isotopes are converted.  The delayed beta plus decay which is present for
 all of the other transformations looses a large amount of energy to a
 neutrino which promptly escapes the device.  I will demonstrate the
 numbers below.

 These components are required to build Cu63 from Ni62
 1 u = 931.494 MeV  Disregard the slight rounding errors, excel chart
 source of data

 Ni62  Mass=61.92835 (u)  Energy=57685.88 MeV
 Proton Mass=1.007276 (u)  Energy=938.2716 MeV
 Electron Mass=.000549 (u) Energy=.510999 MeV

 Coulomb Barrier Energy ~5.6 MeV according to Rossi in his paper

 Cu63 Mass=62.9296 (u) Energy=58618.54 MeV

 Mass of components of Cu63;Ni62 + Proton + Electron=62.936175 (u)
 Energy=58624.66 MeV

 Mass decrease that must be released as energy=62.936175 - 62.9296 =
 .006575 (u) Energy=  6.12457 MeV - 5.6 MeV Barrier = .52457 MeV;Same
 Calculation for Cu65 yields 1.8532 MeV
 In these reactions there are no Beta Plus Decay radiation losses due to
 neutrino release and no 511 keV gammas.

 Please note that I also calculated the expected energy release due to WL
 process on the isotopes such as Ni60 and had perfect energy correlation
 when the energy required to make a neutron from a proton and electron is
 included.

 Exactly the same energy is seen in both paths (Rossi and WL)  when the
 starting point is a nickel isotope with a proton and an electron, and the
 final point is the next higher isotope of nickel.

 I am working very hard to get a clear understanding of the coulomb barrier
 energy behavior.  I can show that the alpha process within stars stops
 once iron has been synthesized, but this is only true if the barrier
 energy is trapped within the nucleus in the form of mass.  I am
 approaching the problem from different directions to prove whether or not
 this hypothesis is accurate.

 Dave


 -Original Message-
 From: pagnucco pagnu...@htdconnect.com
 To: vortex-l vortex-l@eskimo.com
 Sent: Mon, Jun 4, 2012 11:49 pm
 Subject: Re: [Vo]:about Triumph Management (and LENR)


 David,
 Can you explain your conclusion.
  can't see how any energy is released in these Ni -- Cu transmutations.
 Lou Pagnucco
 David Roberson wrote:
  I may have been a bit to fast in pointing out the possible endothermic
  nature of the Ni62 and Ni64 reactions.  They actually are the best two
  isotopes to use if you were not to rely upon the beta plus decay for a
  substantial portion of the energy release.  They further are not
  susceptible to having the 511 keV gammas that would no doubt be released
  by the reactions involving the other nickel isotopes since copper 63 and
  65 are stable and do not decay into nickel by that process.

  So, if Rossi is actually able to overcome the coulomb 

Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread David Roberson

I have long wondered whether or not protons generate bremsstrahlung radiation 
in the same manner as electrons.  It seems that the charge is responsible for 
the radiation and not the mass unless you are suggesting that the slower rate 
of deceleration of a proton versus and electron as it travels through matter is 
the reason.  Would the same deceleration rate for either particle generate the 
same radiation effect?

The flip side of this coin is that the proton would travel proportionally 
further as a result of the lower deceleration rate.

Dave



-Original Message-
From: mixent mix...@bigpond.com
To: vortex-l vortex-l@eskimo.com
Sent: Wed, Jun 6, 2012 12:14 am
Subject: Re: [Vo]:about Triumph Management (and LENR)

snip

Another possibility is that the reacting particle is actually a Hydrino
olecule, and that one of the two protons gets ejected carrying the energy.
ince protons are far more massive than electrons, they produce almost no
remsstrahlung.
here proton addition would create an unstable nucleus, it's also possible that
he electron is captured in an enhanced electron capture reaction. I say
enhanced because in normal EC reactions the nucleus has to try to grab a
ast moving K electron on it's way through, whereas the Hydrino electron is
lready present, and not really intent on going anywhere. ;-)

obin van Spaandonk
http://rvanspaa.freehostia.com/project.html
snip


Re: [Vo]:Mills Hyrdrino project (was :about Triumph Management (and LENR))

2012-06-05 Thread mixent
In reply to  Jojo Jaro's message of Wed, 6 Jun 2012 12:46:44 +0800:
Hi Jojo,
[snip]
Quite honestly, Mills has had decades and considerably more than $100,000 
that you estimate, to bring his Hydrino Theory reactor to fruition without 
apparent success.  No insult or ridicule intended,  but what makes you think 
that you can build a reactor based on his theory that will outperform what 
he has produced so far, when the maestro himself has been unsuccessful?

Please do not take this post as a snide remark to ridicule or to insult.  I 
guenuinely want to know.
[snip]

1) Mills is not interested in fusion reactions.

2) By concentrating solely on Hydrino reactions Mills is constantly having
trouble achieving an acceptable COP.

3) Fusion reactions deliver on average about 1 thousand to 10 thousand times
more energy/Hydrino than hydrino reactions themselves, consequently an
acceptable COP should not be a problem.

4) I have potentially come up with a way of bypassing the catalysis steps he
requires. It is these catalysis steps that prevent him from achieving very large
energy output/Hydrino.

5) I would produce mostly severely shrunken Hydrinos, and very rapidly, leading
to almost instantaneous fusion (micro to milliseconds).

6) As a consequence, the power output is a simple function of Hydrino production
rate and that in turn is simply a matter or regulating an electrical current.
(In fact the device shares some aspects of an old electronic vacuum tube, which
is why it can be so readily controlled over a wide range of power outputs).

7) I would prefer to use the p-B11 reaction if that proves possible, because it
is very clean in a nuclear sense.

8) There is sufficient Boron in the oceans to last us for many millions of
years.


Regards,

Robin van Spaandonk

http://rvanspaa.freehostia.com/project.html



Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread David Roberson

Actually I am far from convinced that the WL theory is sound.  Everything that 
I have seen thus far suggests that neutrons decay into protons, electrons and 
neutrinos but that the chance of a reversal is not very good unless you are 
within a nucleus.

All of the neutron generators that I am familiar with use fusion or fission 
reactions to generate them.  Does anyone know of a proven design which operates 
according to the WL theory?

That is the main reason that I do not believe that the process you outline is 
valid.  The WL theory looks like a free lunch to me.

I would love to be found wrong in my belief toward that theory as it would make 
life so much less complicated, but I just can not accept the many miracles.  
NASA please prove me wrong!

Dave



-Original Message-
From: mixent mix...@bigpond.com
To: vortex-l vortex-l@eskimo.com
Sent: Wed, Jun 6, 2012 12:52 am
Subject: Re: [Vo]:about Triumph Management (and LENR)


In reply to  David Roberson's message of Wed, 6 Jun 2012 00:27:52 -0400 (EDT):
i,
snip]

The half life of Ni63 is 98.7 years.  That path would not be useful in Rossi's 
evice.

he capture alone yields over 6 MeV. The beta decay energy is tiny by
omparison. Unless you are implying that the reaction is not useful because the
i63 would remain radioactive for so long. However Ni63 could be a useful
ortable/remote/no-moving-parts energy source. Initially about 32 W/kg, dropping
ff to half that after 100 years. Think of the sort of applications that
urrently use solar panels.
egards,
Robin van Spaandonk
http://rvanspaa.freehostia.com/project.html



Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread mixent
In reply to  David Roberson's message of Wed, 6 Jun 2012 01:12:10 -0400 (EDT):
Hi,
[snip]

I have long wondered whether or not protons generate bremsstrahlung radiation 
in the same manner as electrons.  It seems that the charge is responsible for 
the radiation and not the mass unless you are suggesting that the slower rate 
of deceleration of a proton versus and electron as it travels through matter 
is the reason.  

Precisely. Furthermore the actual velocity of a proton is about 2000 times lower
than that of an electron of the same energy (relativistic considerations aside).


Would the same deceleration rate for either particle generate the same 
radiation effect?

I suspect so.


The flip side of this coin is that the proton would travel proportionally 
further as a result of the lower deceleration rate.

Actually, I don't think they travel as far. I suspect this is because they are
much slower, and consequently have more time to interact with the electrons of
the atoms they pass through than an electron of equivalent energy. Alpha
particles have even shorter trajectories.
Besides, the positively charged particles tend to attract the electrons of other
atoms, dragging them away from their parent atoms, whereas a fast electron
pushes other electrons away, making them more inclined to simply move over a
little rather then get stripped from their parent atom.
This means that fast electrons don't get as many opportunities to dispose of
their energy and hence travel farther.
[snip]
Regards,

Robin van Spaandonk

http://rvanspaa.freehostia.com/project.html



Re: [Vo]:about Triumph Management (and LENR)

2012-06-05 Thread mixent
In reply to  David Roberson's message of Wed, 6 Jun 2012 01:31:12 -0400 (EDT):
Hi Dave,
[snip]

Actually I agree. I was just playing Devil's advocate a little.


Actually I am far from convinced that the WL theory is sound.  Everything 
that I have seen thus far suggests that neutrons decay into protons, electrons 
and neutrinos but that the chance of a reversal is not very good unless you 
are within a nucleus.

All of the neutron generators that I am familiar with use fusion or fission 
reactions to generate them.  Does anyone know of a proven design which 
operates according to the WL theory?

That is the main reason that I do not believe that the process you outline is 
valid.  The WL theory looks like a free lunch to me.

I would love to be found wrong in my belief toward that theory as it would 
make life so much less complicated, but I just can not accept the many 
miracles.  NASA please prove me wrong!

Dave



-Original Message-
From: mixent mix...@bigpond.com
To: vortex-l vortex-l@eskimo.com
Sent: Wed, Jun 6, 2012 12:52 am
Subject: Re: [Vo]:about Triumph Management (and LENR)


In reply to  David Roberson's message of Wed, 6 Jun 2012 00:27:52 -0400 (EDT):
i,
snip]

The half life of Ni63 is 98.7 years.  That path would not be useful in Rossi's 
evice.

he capture alone yields over 6 MeV. The beta decay energy is tiny by
omparison. Unless you are implying that the reaction is not useful because the
i63 would remain radioactive for so long. However Ni63 could be a useful
ortable/remote/no-moving-parts energy source. Initially about 32 W/kg, dropping
ff to half that after 100 years. Think of the sort of applications that
urrently use solar panels.
egards,
Robin van Spaandonk
http://rvanspaa.freehostia.com/project.html
Regards,

Robin van Spaandonk

http://rvanspaa.freehostia.com/project.html



Re: [Vo]:Mills Hyrdrino project (was :about Triumph Management (and LENR))

2012-06-05 Thread Jojo Jaro
Have you come up with a way to produce these hydrinos cheaply (in terms of 
energy.)?


It seems to me that the first step is to prove your theory with a relatively 
cheap Hydrino Generator.  I guess once you are able to create copious 
amounts of hydrinos, it would be a simple thing to produce power, whether 
there is actual Fusion or not; did I understand you correctly?



Jojo


- Original Message - 
From: mix...@bigpond.com

To: vortex-l@eskimo.com
Sent: Wednesday, June 06, 2012 1:20 PM
Subject: Re: [Vo]:Mills Hyrdrino project (was :about Triumph Management (and 
LENR))



In reply to  Jojo Jaro's message of Wed, 6 Jun 2012 12:46:44 +0800:
Hi Jojo,
[snip]

Quite honestly, Mills has had decades and considerably more than $100,000
that you estimate, to bring his Hydrino Theory reactor to fruition without
apparent success.  No insult or ridicule intended,  but what makes you 
think

that you can build a reactor based on his theory that will outperform what
he has produced so far, when the maestro himself has been unsuccessful?

Please do not take this post as a snide remark to ridicule or to insult.  I
guenuinely want to know.

[snip]

1) Mills is not interested in fusion reactions.

2) By concentrating solely on Hydrino reactions Mills is constantly having
trouble achieving an acceptable COP.

3) Fusion reactions deliver on average about 1 thousand to 10 thousand times
more energy/Hydrino than hydrino reactions themselves, consequently an
acceptable COP should not be a problem.

4) I have potentially come up with a way of bypassing the catalysis steps he
requires. It is these catalysis steps that prevent him from achieving very 
large

energy output/Hydrino.

5) I would produce mostly severely shrunken Hydrinos, and very rapidly, 
leading

to almost instantaneous fusion (micro to milliseconds).

6) As a consequence, the power output is a simple function of Hydrino 
production
rate and that in turn is simply a matter or regulating an electrical 
current.
(In fact the device shares some aspects of an old electronic vacuum tube, 
which

is why it can be so readily controlled over a wide range of power outputs).

7) I would prefer to use the p-B11 reaction if that proves possible, because 
it

is very clean in a nuclear sense.

8) There is sufficient Boron in the oceans to last us for many millions of
years.


Regards,

Robin van Spaandonk

http://rvanspaa.freehostia.com/project.html




Re: [Vo]:discussion about RELIABILITY in LENR

2012-06-05 Thread Eric Walker
On Tue, Jun 5, 2012 at 8:21 PM, Abd ul-Rahman Lomax a...@lomaxdesign.comwrote:

Of the 33 cells, 12 were showing no anomalous heat, and no anomalous helium
 was detected. 18 showed heat, and, from them, helium was detected within an
 order of magnitude of the helium expected from d - He-4. The more heat,
 the more helium, within experimental error. (The measurements were rough,
 unfortunately, only order-of-magnitude detection.)


Forgive my introducing a tangential but related question to this thread.

An important possibility that has been raised by Ed Storms and possibly
others is that there is a nuclear active environment that is only gradually
formed, and that once this environment is sufficiently present, for
example, on the surface of a palladium cathode, LENR will proceed more
readily (for the present purpose, let's assume a single family of reactions
here, excepting cavitation and so on).  Implicitly this possibility is to
be contrasted with a nuclear active environment that does not undergo
modification over time and remains unchanged by the reaction.

In the limiting case, there is the general understanding that known
substrates are modified after a temperature spike above some threshold.
 Once a large excursion has occurred, substrates appear to become
ineffective.  Below this limit, however, the makeup of the nuclear active
environment (NAE) could be dynamic or it could be static.  One motivation
for introducing a changing, cumulative NAE, as I understand it, is to
explain the long initiation times that were needed in Pd-D electrolysis
experiments, especially in the early days.  Sometimes it took weeks or
months before anything was seen.

So we have two broad possibilities -- (1) a changing NAE and (2) a static
NAE.  One way to model (2) is to assume independent power excursion events
that occur at some average rate X.  I think this system can be studied with
a Poisson distribution.

  http://en.wikipedia.org/wiki/Poisson_distribution

If the average rate X is high, the first excursion is likely to happen
earlier than in a system for which the average rate is low, but there is
variability, so you can't be sure.  If the average rate is very low, you
might not see even a single excursion during the course of your
observations over a period of months, say.  For a moderate average rate,
you could see several events in close in time and then not see anything, at
which point the experiment is terminated.  Presumably if the NAE is
dynamic, all bets are off and something altogether different could be
happening.

Two questions:

   - Do we have solid evidence that there is a dynamic NAE rather than a
   static one?  Or is the evidence just barely above noise at this point?
   - If there is no clear evidence yet, is there a clever experiment that
   could settle this question for at least one system?

Eric