2009 review of Ni-H effects since 1989 on rods at 200-400 C, S
Focardi, F Piantelli, 13 p pdf: Rich Murray 2010.01.31

http://www.enea.it/com/ingl/New_ingl/publications/pdf/Cold_Fusion_Italy.pdf

March 2009  217 pages
pages 171-182 13 page

[ a few minor typos corrected -- many pages of references to their work ]

5.3. Anomalous effect between 200 and 400 °C on Ni-H Systems.
Neither chemical nor electrochemical phenomenon
SERGIO FOCARDI, FRANCESCO PIANTELLI
I.M.O. Bologna and Siena,

Introduction

This report concerns the experimental results obtained by two groups of
researchers and collaborators, belonging to inter-university center I.M.O.
from Bologna (Focardi, Campari) and Siena (Piantelli, Gabbani,
Montalbano, Veronesi); all of them  have always participated to the
researches in the field of LENR.

All the references cited  in this report are listed in a chronological order;
they are divided into four different sets: articles published on journals
with referee (R), presentations in academies and national or international
conferences (A), presentation at national congresses of the Italian Physics
Society SIF (S), degree theses (T).

The research in the field of nickel – hydrogen systems started from an
experimental observation by F. Piantelli at the end of 1989 concerning a
strange thermal effect at low temperature in a sample of nickel with
hydrogen. Piantelli spoke of this effect to his friends S. Focardi and R.
Habel during the SIF congress in Trento (October 1990). They decided to
experimentally verify the observed phenomenon, which had been
obtained in a context completely different from the electrochemical one of
Fleischmann, Hawkins and Pons (J. Electroanal. Chem. 261, 301 (1989))
and with completely different working hypothesis which cannot be taken
back to be CF or electroweak interactions (EWI); at present this
hypothesis is going to be supported by  some experimental results while
concerning the CF there are not sufficient specific experimental proofs as
well as concerning EWI there are not the required energy amounts besides
some violations conservation laws.

The experiments were preceded by  many experimental observations
performed in Siena by Piantelli alone; they started in Bologna, Cagliari
and Siena and they were obviously  performed with a high degree of
discretion because of the importance of the phenomenon and its possible
use for energy production.

172

Later some experiments were performed also in Colleferro and in Pavia.
In any case the largest part of the experimental activity took always place
in Siena.

The initial phase was very slow because of the chronic lack of funding. It
was possible to perform the experiments thanks to the kind help of
colleagues and friends from the University of Siena and Bologna, from
INFN, ENEA, CNR of Pisa, CISE, Navy Academy and the Municipality
of Bologna. In this way, by means of  loans and direct participations, the
instrumentation necessary for the first experimental investigations became
available.

The first phase of the common work  ended at the end of 1993 with the
publication of the first obtained results (R1). It was shown that nickel
samples in a hydrogen atmosphere were able to produce additional power
up to 50 W, after absorbing a given amount of gas, at temperatures in the
range 150-400 °C, heated with power among 40 and 120 W. The energy
production started after perturbing the system with power or pressure
changes. In one case, before stopping the process, the system was kept for
24 days in stationary conditions with a power of 44 W corresponding to a
total energy of 90 MJ produced. This first important result had been
preceded by many experimental observations (A1). As a consequence of
these first results it was possible to involve new important partners, such
as FIAT AVIO S.p.A., the consortia T.E.S.C.A. (Bulla, Bergomi e Foglia,
Italkero, Ecosystem) and PROVITA s.r.l..

To the first experimental observations (A1) performed before the end of
1994 many other systematic measurements were added; some of them
were performed in Siena (8), others in Bologna (2), Colleferro (1) and
Pavia (1). The total number of performed measurements from which all
the experimental observations of  the phenomenon have been deduced is
equal to 21.

Power measurements are described in a detailed way in R2; they have
been obtained, starting from 1994, by means of the Newton law, to find
the thermal power emitted by the surface by means of the measured
temperature difference (Tc-Ta), where Tc is the temperature in a given
zone of the cell surface and Ta is the environment temperature inside the
lab. This power can be compared to  the electrical power supplied to the
system, thanks to an initial calibration performed before the system starts
the energy production.

173

Fig. 1.a)

Temperatures are referred to the lab temperature
(Tc - Ta)

Fig 1b)

Tipical result of the experiments performed at Physics Department of Siena

Fig. 1 - Monitoring of the energy production

a) calibration curve as a function of the supplied power (blue);
temperature curve after energy production starting (red)

b) energy production process:
temperature (red) and supplied power (blue) as a function of time.
When the temperature increases, because of the energy production
phenomenon, there is a decrease of the provided power
due to the growth of Pt heater resistance
supplied by constant continuous voltage.

174

Moreover, since the system is continuously monitored, it is possible to
evaluate the fluctuations and all the variations in the system behavior. In
order to evaluate the produced energy we used the resistance variation
technique both of a Pt-100 thermometer and of the Pt heater as a function
of the temperature with a supply system in direct current with rigorously
constant voltage; the actual produced power is evaluated by means of the
decrease of the current due to the increase of the temperature caused by
the beginning of the energy production process.

Hydrogen absorption in nickel

The observed phenomena of thermal energy production by the Ni-H
system starts after the absorption of a certain amount of hydrogen by the
nickel. The amount of absorbed hydrogen is not constant and it possibly
depends on the metallic sample treatment. In some situations we did not
observed any absorption (nor energy production); in others only small
quantities of hydrogen were absorbed. Finally, in other situations, a very
large amount of H was absorbed and in very short times (A2, A7).
In order to be sure that the hydrogen pressure decrease inside the cell was
not due to leaks, we always worked at H pressure smaller than the
atmospheric one (R1); when the pressure decreased because of the
absorption process we reintroduced other hydrogen in order to recover the
starting value. In the fastest observed case (A3, T4) the whole loading
process lasted for 80 hours only.

Generally the absorption process lasted for several days. Moreover we
have observed the existence of some temperature values corresponding to
extremely high gas absorption rates from the nickel (A3); this
phenomenon had never been reported in the previous literature.

>From the study of the H loading phenomenon we conclude that this first
process is essential in order to observe the energy production. In other
words, if the metal does not absorb the hydrogen, there is not any
anomalous effect.

The gas absorption was put into  evidence not only by means of the
pressure decrease but also by the experimental diagram pressure-power:
in some regions it is in complete disagreement with the Gay-Lussac law
connecting pressure and temperature;  there is also a clear indication of
hysteresis (A3).

175
                                 a)
                       b)
Fig.2

a) Hydrogen absorption as a function of the temperature in a heating
and cooling cycle

b) Hydrogen absorption as a function of the time (red) in a test with
step supply

Energy production from the Ni-H system

The first observations of the energy production by the system were
obtained from the temperature changes of the Pt heater located inside the
experimental cells (the description of the experimental setup can be found
in R1).

Later on, because of   some criticisms  which attributed the observed
effect to the modifications of the  Pt electrical resistance due to the
hydrogen absorption by the Pt itself, we decided to measure the effects
from outside the cells (R2).

In summary, as already pointed out, the adopted technique uses the
Newton law: we measured the  difference (Tc-Ta) between the
temperature Tc in a region of the container external wall and the
temperature Ta of a thermometer, located far from the container, which
measures the lab environment temperature, as a function of the supply
electric power. In this way, at the beginning of the experiment (when no
anomalous phenomenon is present), we obtained the experimental
calibration curve; the produced energy is evaluated from the comparison
among the curves obtained when the system is producing energy and the
calibration curve.

The best results were  obtained by means of two cells which produced
about 900 MJ and 600 MJ working for 278 days and 319 days
respectively before being stopped. At the end of the experiment the first
one gave an energy production with a power equal to about 70 W to be
compared with the supply power equal to 29 W (total 99W).

176

Observation of events of nuclear origin

During the experiments, which altogether lasted for about 15 years, many
phenomena witnessing nuclear reactions inside Ni samples in H
atmosphere were observed. While it was producing energy, the cell which
produced 900 MJ emitted neutrons for some days; this emission was
observed with two different techniques, i.e. by means of
3He neutron counters and the Au activation.
The last method (R3) allowed to evaluate
the flux of emitted neutrons: it was 10 neutrons/cmE2-s,
which is equal to 1000 times the neutron flux due to cosmic radiation.

In many cases and with different cells, electromagnetic radiation emission
(with energy of the order of 100 keV) was observed; by comparing of the
spectrum measured by means of NaI(Tl) and Ge counters, located close to
the cell, with that due to the environment background in the lab (A3). The
Ni sample, once extracted from the cell which produced 900 MJ, kept for
many hours in contact with a photographic emulsion, left a radiographic
impression (T4). The same sample, put inside a Wilson cloud chamber,
allowed photography of the tracks due to heavy particles (A5).

Other events, whose existence can only be due to nuclear reactions, were
observed at the end of the experiments by means of the SEM-EDAX
technique for the analysis of the  used sample surfaces. Taking into
account the fact that the used system  is the gas-metal couple, constituted
by hydrogen and nickel, if we find on the surfaces other elements, not
present in any component of the cell, they must come from nuclear
reactions. As reported in A5, on the whole we observed in remarkable
quantity Cu and Zn (with atomic number greater than Ni), F, Na, Mg, Al,
Si, P, S, Cl, K, Ca, Mn, Cr, Fe (Fig. 3).

The fact that nuclear reactions took place in experiments in which there
was thermal energy production is witnessed also by an accurate inspection
of the Ni sample surface; in fact locally, in some regions, there are surface
deformations and considerable ruptures which cannot be justified on the
basis of the temperature (around 400 °C at maximum) produced by the
heater and measured and on the basis of the embrittlement because very
low amount of the absorbed H ( X< 0.08).

177

Fig. 3 - SEM-EDAX analysis of the surfaces

a) spectrum detected on the rod surface in a region where there was not energy
production

b) spectrum detected on the rod surface  in a region where there was energy
production as measured by means of the temperature on the external cell
surface

178

Fig. 4 a)
Fig. 4 b)
Fig. 4 c)

179

Fig. 4 d)

Fig. 4

a) 411 keV peak of the Au activated by neutrons

b) photograph of heavy particles emitted by the Ni rod after the extraction
from the cell

c) a photon emission spectrum measured by means of NaI(Tl) counter

d) a photon emission spectrum measured by means of Ge counter

Bibliography

Reviews

(R1) S. FOCARDI, R. HABEL AND F. PIANTELLI - Anomalous Heat Production
in Ni-H Systems. Il Nuovo Cimento 1994, Vol 107A, pp 163-167

(R2) S. FOCARDI, V. GABBANI, V. MONTALBANO, F. PIANTELLI AND  S.
VERONESI  -  Large excess heat production in Ni-H Systems. Il Nuovo
Cimento 1998, Vol 111A, pp 1233-1242.

(R3) BATTAGLIA, L. DADDI, S. FOCARDI, V. GABBANI, V. MONTALBANO, F.
PIANTELLI, P.G. SONA AND S. VERONESI - Neutron emission in Ni-H Systems.
Il Nuovo Cimento 1999, Vol 112A, pp  921-931.

Proceedings

(A1) F. PIANTELLI, Atti Accad. Fisiocritici, Serie XV, Tomo XXII, pag 89
(1993).

(A2) S. FOCARDI, V. GABBANI, V. MONTALBANO, F. PIANTELLI AND  S.
VERONESI, Atti Accad. Fisiocritici, Serie XV, Tomo XV, (1996) pp 109-115.

180

(A3) S. FOCARDI, V. GABBANI, V. MONTALBANO, F. PIANTELLI AND  S.
VERONESI  -  On the Ni-H System. Conference Proceedings vol 64, “Asti
Workshop on Anomalies in Hydrogen/Deuterium loaded metals”, W.J.M.F.
Collis (Ed.), SIF Bologna 1999 pp 35-47.

(A4) S. FOCARDI, V. GABBANI, V. MONTALBANO,F. PIANTELLI AND  S.
VERONESI - Gamma emission from Ni-H Systems at 420-750 °K
Atti Accad. Fisiocritici, Serie XV, Tomo XVIII, (1999) pags 109-118

(A5)  E.  G.  CAMPARI, S. FOCARDI, V. GABBANI, V. MONTALBANO, F.
PIANTELLI, E. PORCU, E. TOSTI AND  S. VERONESI –  Ni-H Systems.
Proceedings of the 8th International Conference on Cold Fusion, Lerici
(La Spezia), Italy 21-26 May 2000, pp 69-74.

(A6) E. G. CAMPARI, S. FOCARDI, V. GABBANI, V. MONTALBANO, F.
PIANTELLI, S. VERONESI  – Thermal Surface effects in Hydrogen and metals
Proceedings Workshop TESMI, A. Lorusso e V. Nassisi eds, Lecce 2002, 35
(2002).

(A7)  E.  G.  CAMPARI, S. FOCARDI, V. GABBANI, V. MONTALBANO, F.
PIANTELLI, S. VERONESI – Overview of H-Ni Systems: old experiments and
new setup.  5th Asti Workshop on Anomalies in Hydrogen\Deuterium
Loaded Metals, Asti 19-21 March 2004, to appear on Condensed Matter
Nuclear Physics

(A8) S. FOCARDI, V. GABBANI, V. MONTALBANO, F. PIANTELLI, S. VERONESI
- Evidence of electromagnetic radiation from Ni-H Systems, The 11th
International Conference on Condensed Matter Nuclear Science,
Marsiglia 31 October-5 November 2004.

(A9)  E.  G.  CAMPARI, S. FOCARDI, V. GABBANI, V. MONTALBANO, F.
PIANTELLI, S. VERONESI  - Surface Analysis of hydrogen loaded nickel
ALLOYS, The 11th
International Conference on Condensed Matter Nuclear Science,
Marsiglia 31 October-5 November 2004.

(A10) E. G. CAMPARI, G. FASANO, S. FOCARDI, S. LORUSSO, V. GABBANI, V.
MONTALBANO, F. PIANTELLI, C. STANGHINI, S. VERONESI -  Photon and
particle emission, heat production and surface transformation in Ni-H
system, The 11th
International Conference on Condensed Matter Nuclear
Science,  October-5 November 2004.

(A11) E. G. CAMPARI, S. FOCARDI, V. GABBANI, V. MONTALBANO, F.
PIANTELLI, S. VERONESI  – Overview of H-Ni Systems: evidence di H
adsorption, Heat production, Photon  and particle emission and surface
transmutations. - The 6 International  Workshop on Anomalies in
Hydrogen/Deuterium loaded Metals, Siena 13-16  May 2005

181

(A12) E. G. CAMPARI, S. FOCARDI, V. GABBANI, V. MONTALBANO, F.
PIANTELLI, S. VERONESI –  New experiments on Ni-H Systems – Atti
Accademia dei Fisiocritici  (2005) (in stampa).

(A13) E. G. CAMPARI, S. FOCARDI, V. GABBANI, V. MONTALBANO, F.
PIANTELLI, S. VERONESI  - Energy production and nuclear reaction in Ni-H
Systems - The 7 International  Workshop on Anomalies in Hydrogen/
Deuterium loaded Metals, Asti 23-27 September 2006

Presentations at national and international conferences

(S1) S. FOCARDI, R. HABEL AND F. PIANTELLI - Evidenza di reazioni nucleari
in sistemi nichel-idrogeno a 400 gradi Celsius, 81 o
Congresso Nazionale della Società Italiana di fisica, Perugia
2-7 ottobre 1995.

(S2) S. FOCARDI, V. GABBANI,R. HABEL, V. MONTALBANO, F. PIANTELLI, G.
SOLVETTI, A. TOMBARI, S. VERONESI  -  Evidence of Heat Production and
Nuclear reactions in Hydrogen Loaded Nickel Rods in Siena Experiments. –
Convegno “Stato della fusione fredda in Italia” – Siena (1995)

(S3) S. FOCARDI, V. GABBANI, V. MONTALBANO, F. PIANTELLI, C.
STANGHINI, S. VERONESI -  New Esperimental Evidance of Nuclear Reactions
in Ni-H Systems – LXXXI  Congresso nazionale S.I.F.   – Verona (1996)

(S4) E. CAMPARI, S. FOCARDI, V. GABBANI, R. HABEL, V. MONTALBANO, F.
PIANTELLI, S. VERONESI, E I. USAI - Studio di sistemi Ni-H nella regione 600-
800 K, 83 o Congresso Nazionale della Società Italiana di fisica, Como
27-31 ottobre 1997.

(S5) E. CAMPARI, S. FOCARDI, V. GABBANI,  V. MONTALBANO, F. PIANTELLI
E S. VERONESI  - Emissione di raggi gamma da sistemi Ni-H,
84 o Congresso Nazionale della Società Italiana di fisica, Salerno
28 settembre-2 ottobre 1998.

(S6) E. CAMPARI, S. FOCARDI, V. GABBANI,  V. MONTALBANO, F. PIANTELLI
E S. VERONESI  - Comportamento dei sistemi Ni-H,
85 o Congresso Nazionale della Società Italiana di fisica,
Pavia 20-24 settembre 1999.

(S7) E. CAMPARI, S. FOCARDI, V. GABBANI, V. MONTALBANO, F. PIANTELLI,
E. SALI, C. STANGHINI E S. VERONESI - Alcuni aspetti delle interazioni Ni-H,
86 o Congresso Nazionale della Società Italiana di fisica,
Palermo 6-11 ottobre 2000.

(S8) E. CAMPARI, G. FASANO, S. FOCARDI, V. GABBANI, V. MONTALBANO, F.
PIANTELLI, C. STANGHINI E S. VERONESI - Interazioni H-superfici metalliche:
effetto FASEC, analisi comparata dei risultati sperimentali,
90 o Congresso Nazionale della Società Italiana di fisica,
Brescia 20-25 settembre 2004.

182

(S9) S. FOCARDI E F. PIANTELLI – Produzione di energia e reazioni nucleari in
sistemi Ni-H a 400 o C,
Conferenza nazionale sulla politica energetica in Italia,
Università di Bologna, 18-19 aprile 2005.

Degree theses

(T1) ANTONELLA  DI  FABRIZIO -  Studio degli effetti termici in
sistemi nichelidrogeno, Università di Bologna,
Anno Accademico 1993-1994, sessione invernale.

(T2) LARA  STUPAZZONI  - Misure del flusso di neutroni emessi in processi di
fusione fredda, Università di Bologna,
Anno Accademico 1994-1995, sessione autunnale.

(T3) RAFFAELE  MOLTI  -  Misure di radioattività ambientale,
Università di Bologna, Anno Accademico 1994-1995, terza sessione.

(T4) ALESSANDRO  VENTURA  -  Un apparato sperimentale per lo studio di
sistemi Ni-H.
Università di Bologna,  Anno Accademico 1995-1996, sessione estiva.

(T5) ANNA ELISABETTA ZIRI - Spettro della radiazione gamma con rivelatori al
germanio e allo ioduro di sodio,
Università di Bologna, Anno Accademico 1995-1996, sessione autunnale.

(T6) BARBARA  MIRRI  -  Studio dei sistemi nichel-idrogeno,
Università di Bologna, Anno Accademico 1995-1996, sessione invernale.

(T7) ELENA FIUMANA  - Caratteristiche dei sistemi Ni-H nella regione 300-500
o C,
Università di Bologna, Anno Accademico 1995-1996, sessione invernale.

(T8) GIUSEPPE  PETTINATO -  Rivelazione di neutroni (E<10 MeV) con un
contatore a scintillazione NaI(Tl),
Università di Bologna, Anno Accademico 1995-1996, sessione invernale.

(T9) ANNALISA  BERNARDINI -  Studio di processi nucleari in sistemi Ni-H,
Università di Bologna, Anno Accademico 1996-1997, seconda sessione.

(T10) BORIS  VICINI  -  Studio dei fenomeni nei sistemi Ni-H,
Università di Bologna, Anno Accademico 1996-1997, terza sessione.

(T11) PAOLA  ZUCCHETTI -  Evidenze di reazioni nucleari in sistemi
nichelidrogeno,
Corso di perfezionamento in fisica,
Università di Bologna, Anno Accademico 1996-1997.

(T12) ALESSANDRA  FORNACIARI  -  Sistemi metallo-idrogeno,
Università di Bologna, Anno Accademico 2000-2001, seconda sessione.

(T13) FEDERICA  SALAMI -  Sistemi Pd-idrogeno,
Università di Bologna, Anno Accademico 2000-2001, terza sessione.

(T14) CLAUDIO  CERRETO  -  Processi nucleari nei sistemi TI/H a temperatura
ambiente,
Università di Bologna,  Anno Accademico 2004-2005, seconda sessione.

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