Return to the clickable list of items
157) Comments and questions
Ludwik Kowalski (7/8/04)
Department of Mathematical Sciences
Montclair State University, Upper Montclair, NJ, 07043
In unit #150
I posted comments and questions related to a paper on calorimetry. I was
prompted by a message from Richard Eskimos. In this unit I decided to do the
same about a paper on unexpected charged particles. In planning to start a
research project in that area, using CR-39 detectors, I selected a paper
published by Andrei Lipson, and his coworkers. They are experts in using track
detectors of charged particles in the area of cold fusion. The title of that
paper is ÒPhenomenon of an Energetic Charged Particle Emission From
Hydrogen/Deuterium Loaded Metals;Ó it can be downloadable from the www.lenr-canr.org website.
That paper,
like the one chosen to ask questions about excess heat, was presented to
experts attending the 10th International Cold Fusion Conference. It is not
surprising that somebody who has not read earlier papers has difficulties with
understanding numerous detail. As in unit #150 I want to ask questions
illustrating difficulties encountered by non-experts in reading conference
papers.
What follows
is the text part of the article with questions and comments (in red). The four
authors of this paper are A.G.
Lipson, A.S. Roussetski, G.H. Miley and E.I. Aaunin. They represent
prestigeous research centers: (a) University of Illinois at Urbana-Champaign,
Department of Nuclear, Plasma and Radiological Engineering, Urbana, IL, (b) Lebedev Physics Institute, of the
Russian Academy of Sciences and, c) Institute of Physical Chemistry, of the
Russian Academy of Sciences. The text of the paper (without figures) is in
black while my comments and questions are in red. Will the answers to my
questions be provided by some readers? I hope so. It will not be difficult to
incorporate such input into this text by using a different color.
Abstract
The new
phenomenon of energetic alpha (up to 16.0 MeV) and proton (~1.7 MeV) emissions
has been discovered from a metal surface possessing a large affinity for
hydrogen and loaded/excited by electrolysis, glow discharge or powerful laser.
These various experiments on charged particle detection show a remarkable
feature, namely all exhibit a similar specific energy yield of long-range
alphas (1 alpha particle per 10-15 eV input energy/Pd(Ti) target atom)
independent of the excitation power of delivering method (electrolysis, glow
discharge or laser irradiation). This result suggests the mechanism of energy
transfer causing the energetic particle emissions in hydrogen loaded metal
targets is similar despite the seemingly dissimilar excitation techniques.
I.
Introduction
Charged
particle emissions from the surface of Pd and Ti deuterides have been studied
since the beginning of experiments on Low Energy Nuclear Reactions (LENR)
product detection in metal deuterides. First experiments on this charged
particle detection were mainly, referenced to confirm generation of DD-reaction
products (3.0 MeV protons and 1.0 MeV tritons) in metal deuterium system.
However, alongside with charged DD-reaction products, there were appeared
reports concerning detection of more energetic particles than would be expected
from DD-reaction [1-4], especially during hundred-keV accelerator deuteron
bombardment of Ti and Pd targets.
Earlier we
just reported that during exothermic deuterium or hydrogen desorption we found
high energy alpha-particle emission in the energy range 8-14 MeV, that could
not be ascribed to known natural alpha -- emitters. Indeed, the typical charged
particle spectrum taken in vacuum using SSB -- detector during about 8 days
shows no counts beyond a 8.0 MeV energy (Fig. 1 [5]).
(1***) The
SSB probably stands for the ÒSolid State Barrier,Ó a common Si detector.
Figure 1.
That is not
surprise because maximal alpha energy of radon series is about 7.8 MeV, while
energy of cosmic induced protons rarely exceeds 2.0 MeV. In contrast to
Background, the dE-E spectra detected from Au/Pd/PdO:D(H)x samples during
exothermic deuterium desorption clear showed presence of high energy
alpha-component (Fig.2 [6]).
(2***)
What are the horizontal segments in the second bin (0.5 to 1 MeV)? I am
referring to Figure 1.
Figure 2
New insight
was recently obtained from the use of CR-39 track detectors to the study
energetic particle emissions from the surface of Pd/Ti loaded with
hydrogen/deuterium [7]. Experimental runs with CR-39 to detect long-range
alpha-particles in-situ during electrolysis of Pd/dielectric substrate cathodes showed
energetic alphas (9 < Ea
< 16 MeV) yield Na ~ (2-5)*10-4 s-1 -cm-2 Pd in 4p-str accompanied by even more intensive emission of ~ 1.7 MeV
protons.
The
objective of present research was focused to study energetic charged particle
emission (ECPE) at various power loading and/or excitation conditions applied
to the metals with large affinity to hydrogen/deuterium and determine a
specific yield of ECPE, depending on excitation power applied to the sample.
II.
Experimental Technique
For charged
particle detection the purified ÒRadtrackÓ CR-39 plastic track detectors (with
the size 2.0*1.0 cm2) by Landauer Inc.
AND Fukuvi Chemical have been used. Especial purification procedure utilized
for detector manufacturing as well as hermetic saving condition allow to
minimize initial alpha track density of these CR-39 to less than 20 cm-2.
(3***) In
other words less than 40 tracks per detector. A useful number to know.
Figure 3a
and Figure 3b
(4***) Good to know that Radtrack and Fukuvi detectors are not different. Is it true that Fukuvi detectors are no longer commercially available?
These
detectors were calibrated with alpha-sources (in the range of 1.6 Ð 7.7 MeV)
and by monoenergetic cyclotron alpha-beams (in the energy range of 10.0 Ð 30.0
MeV) as well as by proton beams with energy ranging of 2.0-3.0 MeV. (Fig.3a,b). For energetic proton detection the
detectors were also calibrated with Van DeGraaf accelerator by monoenergetic
proton beams (energy ranging from 0.75 ² Ep ² 3.0 MeV), (Fig.2). After the beam
exposure detectors were etched in 6N-NaOH at t=70¡C during 7 hrs. and
investigated with optic microscope. Typical view of alpha-track picture is
presented in Fig 4. As seen, at normal interaction of
monoenergetic cyclotron beam with detector, the tracks observed after the
etching have almost ideal circle-like shape. These nuclear tracks can be easy
distinguished from the defects of CR-39 subsurface structure.
Figure 4
The
efficiency of CR-39 detection with respect to different energy alphas and
protons were estimated in accordance with their critical angles qc being determined by formula [4]: qc= sin-1{[1-(dE/2h)2]/[1+(dE/2h)2]}, where dE-is the
track diameter produced by charged particle with energy E (Fig 1,2), and h =
9.1µm is the depth of etched layer in CR-39 at our etching condition. Knowledge
of the critical angles calculated from above formula allow to determine the
efficiency e of the charged particle detection
as:
e = 0.5 * (1-sin qc)
(5***)
This is wrong; replace sin by cos. Efficiency is defined as the ratio of the
solid angle over 4*p. I suppose they reprint the same
mistake from the 2002 paper (ICCF9 in China). Am I the first one who noticed
it? I do not think that the reference 1 has anything to do with the efficiency
of CR-39 detectors.
In
electrolysis experiments the freshly opened CR-39 detector chips were attached
either to the Pd thin film cathode(Foreground)
(6***) It
is not clear to me how to apply CR-39 to a cathode during the electrolysis.
They used a very thin cathode. Somehow (according to their 2002 paper at ICCF9
in China) they placed the Cr-39 detectors (open and shielded) inside the
electrolyte, next to the thin cathode. This if not at all obvious from reading
this paper. Why there is no illustration? Why there is no reference to their earlier
paper at this place?
or to the
substrate side or/and immersed in electrolyte in the cell (Background).
(7***)
This formulation (with two ÒorÓ) is confusing. I would measure the background
by placing the CR-39 detectors next to an identical cathode that has not been
loaded with hydrogen, for example, at zero current. I will assume they did
this.
Background
experiments showed proportional growth of track density vs. time for CR-39
immersed in electrolyte (Fig.4). At large Background duration [long exposure]
it is possible to observe two separate alpha-peaks with track diameters located
at 8.0 and 9.0 µm, respectively (Fig.5). The energy positions of these peaks
are in good agreement with conventional alpha-Background and are normally
corresponded to about 7.0 MeV radon (8.0 µm) and 5.0 MeV (9.0 µm) thoron series
of natural alpha-nuclides.
(8***) In other words, the
electrolyte or cathode (or both) contained traces of emitters of natural alpha
particles.
Figure 5
(9***)
According to this figure they can distinguish diameters differing by only 0.1 m.
In order to
separate high-energy alphas and low-energy protons that could be possibly
emitted during electrolysis runs, the thin Cu-foils (25 µm thick) were inserted
between the cathode metallic coating and the CR-39 surface. 25 µm Cu coating is
completely absorbs all alpha-particles and protons with energies below 9.0 and
2.3 MeV, respectively.
(10***) I
suppose that a separate experiment was conducted to show that the foil itself
is not alpha radioactive (at a very low level). Why is nothing said about this?
Alpha particles from the surface of the foil, interpreted as if they were
traversing the foil, could be assigned more energy than they really have.
Background
measurements in experiments with Cu-covered CR-39 were performed similarly to
that with open detectors. As expected, these background experiments showed
significant reduction( ~2 times) in the total track density compared to that
obtained with open CR-39 detectors.
(11***)
Why Òas expected?Ó On what basis could one expect that one half of all tracks
recorded with the open detector (without the Cu foil) would be due to low
energy alpha particles and protons? I suppose this was based on their earlier
data. How else would one predict the percentage of low energy particles (such
as 50%)?
(12***)
How large were these densities? What about errors of judgment in deciding which
tracks to count and which to attribute to surface defects on CR-39? Based on my limited experience, I
suspect that the adjective ÒtypicalÓ, used above to describe Figure #4, might
be an exaggeration.
In
experiments with glow discharge and laser irradiation for particles
identification and their energy estimation, we used CR-39 Fukuvi detectors
covered with Al or Cu foils with the thickness in the range of 11-66 or 25-50
µm, respectively. The experimental set ups used for deuterium glow discharge
Ti-cathode bombardment and for powerful picosecond laser irradiation of Ti and
TiDx targets are described elsewhere []. Power densities applied to the
loaded/excited Pd or Ti samples (with respect to the total sample volume)
during the electrolysis experiment, in glow discharge (GD) bombardment and in
Laser irradiation are estimated as (2-5)x102, 105-106
and ~1021 W/cm3, respectively.
(13***)
Why per cubic cm and not per square cm?
In series of
experiments with GD the detectors covered with 11-33 µm Al foils were placed
behind the holes drilled in the Mo anode at the distance of 3.0 cm from the
surface of Ti cathode.
In the laser
experiment detectors, shielded with 11-66 µm of Al or 25-50 µm of Cu were
placed at different angles toward the target (20 cm from the front of the
target perpendicular to the beam direction and 4 cm distance behind the target)
Utilization
of shielding foils of various thickness alongside with CR-39 calibration data
allow identify and roughly reconstruct energy spectra of emitted alpha
particles and protons.
III.
Experimental Results
a.
Electrolysis
The
Foreground runs with electrolysis of Pd-thin film cathodes the exposed CR-39
detectors (t~2.0-30 days) showed the appearance of unusual diameter tracks that
were not observed in Background detectors exposed in the same electrolytic
cell. Indeed, in the track diameters distribution N(d), two significant peaks
located at 7.0m and 6.0m observed in the Foreground runs
(with electrolysis) with opened CR-39 detectors (Fig 6).
Figure 6
At the same
time, almost no counts for tracks with d < 7.5m was found in the corresponding Background runs for detectors
exposed in the same electrolytic cells.
(14***) I
replaced mm by microns (mm instead of mm was an obvious typing error).
The low
diameter tracks appeared to accompany an electrolysis of the thin Pd-film and
Pd-black cathodes. The intensity of charged particle emissions and ratio
between 6.0 and 7.0 µm peaks during electrolysis are strongly depended upon the
cathode history and structure (Table 1). It should be noted that generation of
charged particle emissions during the electrolysis of thin Pd cathodes has a good
reproducibility (in contrast to the irreproducible emission of DD-products in
Pd-D systems).
(15***)
According to Karabut, emission of charged particles is highly reproducible when
Pd is bombarded with D (glow discharge). Is it a contradiction?
In the
Foreground runs with the same cathode being carried out with 25 µm Cu-film
shielded CR-39 chips, the 7.0 and 6.0 mm peaks disappeared. But the other maximums ranging from 7.5 to
11.4 mm have appeared that were not found
in Cu-shielded Background detectors (Fig 7).
(16***)
This discussion of differences between Figures 6 and 7 is not clear to me.
Figure 7
The
experiments with Cu-shielded detectors and a knowledge of CR-39 calibration
curves (Fig 1,2) allowed to identify the energy and type of particles emitted
in the Foreground runs with open CR-39 detectors. Taking into account stopping
powers and ranges of 25 µm Cu-film with respect to the alphas and protons with
different energies, the initial energies of emitted particles were also
calculated. Comparison of pictures obtained with opened and shielded detectors
shows that 6 µm peak is completely disappeared while a broad near 7.0 µm peak
in Fig. 6 shifted to the larger track diameters and split at least by 3 narrow
peaks (Fig 7). Disappearance of 6.0 µm peak in a shielded detector indicates to
the low MeV proton nature of this peak. In accordance with our calibration data
the estimated proton energy would be within 1.5-1.7 MeV (Fig 8a, b [7]).
Fig 8 a
Fig. 8 b
(17***)
Figure 8a has a line saying Ò39 detectors;Ó it is confusing. The Òopen Cr-39
detectorsÓ should be in one line. And what is Ò25 mcmCu/CRÓ below that line?
(18***)
Why are figures 8a and 8b not labeled consistently? Their legends are in
different places.
(19***)
These two figures show that 20 alpha particle tracks and 120 proton tracks were
recorded on 3 cm^2 of Cr-39? Can this 1:6 ratio be interpreted in terms the
higher Coulomb barrier penetrability of protons with respect to alpha
particles?
(20***)
How long did it take to accumulate so many tracks? A person attempting to
reproduce the experiment would need to know this. In other words, what was the
average emission rate? Information about the electrolytic cell should also be
provided.
In contrast
to 6.0 µm peak, the 7.0 µm maximum, accordingly to its shift and splitting
after crossing the Cu-shield should be ascribed to a broad 11-16 MeV
alpha-peak. Indeed, the stopping range of alphas ranging from 11-16 MeV (for
open Cr-39) would be consistent with observed narrow bands with energies 11.6,
12.5 and 14-16 MeV, respectively for Cu-covered detectors (Fig 8a). Due to
higher resolution of CR-39 alpha-tracks for the lower energy particles (Fig 1)
the broad 11-16 MeV alpha band could be observed as the single individual
maximums after these particles crossed the Cu-foil. Therefore, we showed that
electrochemical loading of Pd thin film cathodes on dielectric substrates
unambiguously produce high-energy charged particles: 1.5-1.7 MeV protons and
11-16 MeV alphas.
b. Glow
Discharge
Let us consider
in details new results on ECPE obtained for more powerful loading process
during low energy deuteron bombardment of Ti-cathode. Typical spectra of
charged particles emitted in such GD obtained with 11 and 33 µm shielded CR-39
detectors are shown in Fig 9.
Figure 9
(21***)
This figure shows ~80 tracks/cm2 in 7 hrs (50+20+10=80). It also
shows that diameter become wider (lowering of energy) when a thicker shield is
inserted. But why didn't they show diameters (and numbers of tracks) detected
with the unshielded detectors? Does it mean that using unshielded detectors is
not possible in the case of their glow discharge experiments?
As seen, the
spectrum of charged particles of 11 µm shielded CR-39 contains 3 characteristic
peaks with track diameters 5.2, 6.2 and 7.2 µm, respectively. In accordance
with Fukuvi Cr-39 calibration those peaks have to be corresponded to 3.0 MeV
protons (5.2 µm), 1.4 MeV/2.8 MeV protons /deuterons (6.2 µm) and 13.0 ± 2.0
MeV alphas (7.2 µm). Indeed, increase in Al shielding thickness from 11 to 33
µm leads to corresponding increase in track diameters for all three peaks
observed at for 11 µm Al-covered Cr-39 detectors.
(22***)
The above text is too condensed, for my taste. They interpreting say the peaks
with track diameters 5.2, 6.2 and 7.2 µm. The first is due to protons of 3 MeV,
the second is due either to to 1.4 MeV protons or 2.8 MeV deuterons, and the
third is due to 13 MeV alphas. The last sentence is confusing, unless the
phrase Òobserved at for 11 mm
Al-covered Cr-39 detectorsÓ is removed. They probably say that all red peaks
(even single counts) shift to the right (diameters become larger).
The shifts
of these peaks (5.2 →5.6
µm; 6.2 → 6.6+6.8 µm (spitting) and 7.2 →7.6 µm) is really corresponded to the
energy losses of 3.0 MeV protons (from DD-reaction), 2.8 MeV deuterons and 13.0
MeV alphas, in accordance with the stopping ranges of these energetic particles
in Al. In Fig. 10 the more detailed picture of alpha emission is presented and
compared to the background in GD chamber.
Figure 10
As seen from
the Fig. 10 the energetic alpha emission in GD at given discharge parameters
exceeds the background counts in the range of 7.2 µm track diameters about 25
times.
(23***) I
can not see this from Figure 10. By the way, why some blue background bars
indicate negative negative densities? But I do see that this time they refer to
Al shielding (while Figure 9 referred to Cu shielding). I suppose it was the
same experiment in which some detectors were covered with Cu and others with
Al. It looks that they had about 45 tracks/cm2 in 7 hrs.
At the same
time the usual alpha-background (d ³ 8.0 µm ) in presence of GD is not
significantly distinguished from that in absence of glow discharge voltage. The
yield of energetic alphas after background subtracting was found to be Nα = 0.12 ± 0.02 a/s in 4¹ ster.
(24***)
But according to Karabut, who used the Pd target (not Ti target) the rate of
emission of energetic alphas (at 1000 volts) was about 1 per second. This is
nearly ten times more than the above number. Why is this not discussed? I would
use Pd to increase the yield?
This yield
of energetic alphas is about 2-3 orders of magnitude high than that detected in
electrolysis experiment.
(25`***)
Aha, here is the answer to my previous question; for the electrolysis the rate
was about 0.001 to 0.0001 per second.
The yield of
2.8 MeV deuterons in GD experiment is about 2-3 times larger than for alphas.
(26***)
Can this ratio also be interpreted in terms the higher Coulomb barrier
penetrability of deuterons with respect to alpha particles? What I have in mind
is a barrier lowered by screening.
In Fig. 11
the spectra of charged particles obtained for two different GD voltages are
presented.
Figure 11
As it is
expected the 3.0 MeV peak from DD-reaction in Ti under deuteron bombardment is
strongly depended on GD voltage. Meanwhile, the intensities of 2.8 MeV deuteron
and 13 MeV alpha peaks are depended on the GD voltage much weaker.
(27***) On
what basis is this expected? Why should the effect of discharge voltage on the
probability of emission of DD protons be much more pronounced than on the
probabilities of emission of more more energetic particles?
In Fig 12a and 12b the
more detail pictures of dependencies shows This fact indicate to absence of
direct connection between energetic charged particle emission and DD-reaction.
The detailed yield dependencies for 3.0 MeV protons, 2.8 MeV deuterons and 13.0
MeV alphas on discharge voltages in the range of 0.8-2.45 kV are presented in
Fig 12 a, b.
Figure 12
a and Figure 12 b.
As seen, the
yields of energetic deuterons and alpha particles normalized to the effective
discharge power almost independent on deuteron energy Ed, while DD-reaction
yield of 3.0 MeV protons tends to grow exponentially with increase in Ed. The
experiments showed that the yields of energetic deuterons and alpha particles
in Glow discharge are roughly proportional to GD power applied to the Ti
cathode (Fig. 13)
Figure 13
(28***)
Zeros below the x axis should be replaced by numbers of watts.
The fact of
near linear dependence of energetic charged particle emission yields on
effective power applied to the Ti cathode leads to a simple assumption that the
yield of ECPE from the surface of metals with large affinity to hydrogen could
be further increase with increase in specific power applied to these metals.
c. Laser
Experiment
(29***)
Their laser induced fusion is probably not cold. This is the end of my questions and comments.
In order to
check the assumption of ECPE yield increase with applied specific power we have
performed a search of energetic alphas in ultra-high specific power applied
experiments on picosecond laser excitation of Ti/TiHx and TiDx targets. The
details of this experiments, including set up are described in another report
published in this Proceedings [8]. We note here that powerful laser irradiation
of solid targets (polymers and some metals including Al , Pb LiD and so on) was
studied during last 10 years to induce intense MeV protons and heavy ion
emissions as well as to the purposes of inertial DD-fusion and isotope
separation (see review article [9]). Here in experiments with powerful laser
we, probably, first use targets possessing large affinity to hydrogen/deuterium
(Ti and TiDx foils of 30 µm-thick). The parameters of laser were: power density
P=2x1018 W/cm2, pulse duration τ = 1.5x10-12 s and wave
length λ = 1.054 µm. To compare our results
with usually employed targets (to produce intense proton beams) we also used
polyethylene (PE) film targets of 35 µm-thick.
The main
charged particle component emitted on laser shots with both Ti(TiDx) and PE
targets was found to be protons (deuterons) with energies Ep ² 1.0 MeV (Np ~ 1011/pulse).
The heavy ion component with mass A > 4 was also detected. However, besides
these species during the shots on Ti and TiDx targets we found we found also
energetic alpha particles that were not detected in experiments with PE (Fig.)
As seen the laser shots on Ti-target produce the same tracks at the CR-39
detectors covered with 11 µm of Al (d=7.2µm) that were detected for of
electrolysis and GD loading experiments. The similar shots on PE target showed
possible alpha emission level comparable with background in vacuum chamber of
target installation.
Figure 14
In Fig. 15
the spectra of alpha particles detected in the same laser shot by CR-39 detectors
covered with various shielding and placed between 0-30 ¡ with respect to TiDx-
target are presented.
Figure 15
The main
peak in Fig 15 corresponding to 13.0 ± 2.0 MeV alphas is shifted to larger
track diameters for 33 and 66 µm Al shielded detectors, well in accordance with
13 MeV alphas stopping range in Al. For 50 µm Cu covered detector this peak is
completely disappeared because the 50 µm thick Cu shielding will stop all alpha
particles with energy E ² 15.0 MeV.
The same
energy alpha-particle emission, but about 30 times less in intensity was
detected from the opposite side of Ti/TiDx target (the angle between the
detector and target ¥ = 180¡) (Fig 16.) Here as in Fig 15. a track diameter
corresponding to alpha peak (d=9.9 µm) is also in good agreement with stopping
range of 13.0 MeV alphas in the sandwich consisting of Cu-shielding and Ti-foil
[25µm Cu(shielding) +30 µm Ti(sample thickness)]. This fact allow assume that
alphas were originated mainly at the front side of the Ti target. The estimated
average intensities of alpha emission from the front and opposite sides of
Ti/TiDx targets (taking into account geometrical efficiency of measurement) was
found to be If ~ 2x104/pulse-sr-1 sr. and Io ~7x102/pulse-
sr-1, respectively.
Figure 16
In Fig 17
the results of alpha-spectra reconstruction from CR-39 data obtained for
various shielding type and thickness (taking into account cyclotron
calibration) are presented. The results of such reconstruction for Ti and TiDx
targets within experimental error are close one to another. In the Fig. 18 a
comparison of alpha spectra obtained from laser experiment with Ti-target and
Pd-glass electrolysis are shown. As seen from this figure, the spectra of laser
experiment and electrolysis detection look quite similar within the measurement
error (determined by standard deviations of alpha-calibrations and errors of
track diameter measurements) and both spread in the energy range of 10-17 MeV.
Figure 17
and Figure 18
IV
Discussions and Conclusions
Thus, in
three independent studies of ECPE during hydrogen(deuterium) loading of Pd and
Ti targets or excitation of their hydrides/deuterides, the similar energetic
alpha particles and protons/deuterons are found to be emitted, despite the
seemingly dissimilar loading/excitation techniques. We found that the absolute
intensity of ECPE is roughly proportional to the specific power applied to the
metal target during its loading or excitation (Fig 19). There are three
different power density areas corresponding to the studied ranges of specific
power applied in experiments on ECPE detection with hydrogen/deuterium
loading/excitation of Ti and Pd: electrolysis -((2-6)x102 W/cm3);
GD -(105-106 W/cm3) and laser irradiation - (~
1022 W/cm3) are presented in this graph. On the other
hand, the specific energy required to emit one alpha particle (E > 8.0 MeV)
in all these loading /excitation cases was found to be Es = 17 ± 8 eV/at.Ti(Pd)
and practically independent on excitation power applied to the target (Fig.
20).
The
discovered property of the metals with large affinity to hydrogen to emit
energetic charged particles is probably concerned to peculiarities of these
metals. On one side, during hydrogen loading the metals such as Pd and Ti are
subjected to strong plastic deformation accompanied by massive generation of
non-equilibrium phonons. On the other side, the metals with large affinity to
hydrogen may capture high amount of helium (from surrounding atmosphere or
during the loading alongside with hydrogen), which have tend to segregate in
the site of high internal strain. We assume that loading or excitation
procedure produce non-equilibrium phonons in the near-surface layer of Pd or
Ti. These phonons would be focused (concentrated ) in the some specific sites
with high internal strain near the surface. If mechanisms of energy transfer
from the concentrated optic phonon modes (with high amplitude and frequency) to
the atoms captured in the sites with high internal strain is really existed
[10], then such energy transfer can lead to effective acceleration of the light
atoms captured in the sites of high internal strain (hydrogen, deuterium
helium).
Figure 19
and Figure 20
Regardless
of mechanisms involved in ECPE phenomenon in Pd and Ti, we emphasize that some
peculiarities of LENR could be more clear, taking into account similarities
between processes observed in electrolytic loading of these metals (LENR effects)
and powerful laser irradiation effects. These similarities include:
-Neutron
spectra for deuterated targets in laser and LENR experiments : besides 2.45 MeV
peak high energy neutrons up to 10 MeV (compare: P.A. Norreys et al., Plasma
Phys. Control. Fusion, 40, 175(1998) and A.G. Lipson et al., Fusion Tech., 38, 238 (2000)). High energy component
of neutron spectra in laser case is explained by presence of MeV deuterons
(Probably similar effect in LENR case).
-Charged
particle emissions, including their energy ranges
-Isotope separations and exotic
transmutations
-Production of craters at the target
surface.
-Possible generation of isomeric
states of nuclei in solids (after-emissions of gamma and X-rays)
References
1. F.F.
Cecil, D. Ferg, H. Liu et al., Nuclear Phys. A539, 75 (1992).
2. R.
Taniguchi, Trans. Fusion Tech., 26 (4T), 186 (1994).
3. J.
Kasagi, T. Ohtsuki, K.Ishu and M. Hiraga, J. Phys. Soc. Japan 64, 777 (1995).
4. A.
Takahashi, K. Maruta, K. Ochiai, H. Miyamaru, Fusion Tech. 34, 256 (1998).
5. A.G.
Lipson, B.F. Lyakhov, A.S. Roussetski et al., Fusion Tech., 38, 238 (2000).
6. A.G.
Lipson, A.S. Roussetski, A. Takahashi and J. Kasagi, Bull. Lebedev Phys. Inst.,
No.10, 22 (2001).,
7. A.G.
Lipson , A.S. Roussetski and G.H. Miley., Trans. Am. Nucl. Soc., 88, 638 (2003).
8. A.S.
Roussetski et al., in this Proceedings.
9. K.W.
Ledingham, P. McKenna, R.P. Singhal, Science, 300, 1107 (2003).
10. P.L.
Hagelstein, ÒAnomalies in Metal DeuteridesÓ, Proc. ICCF-9, Beijing, May 2002.