[Vo]:Large Excess heat production in Ni-H systems (Focardi et al, 1998)
This is Focardi's and Piantelli's improved experiment from the fall of 1996 (published in 1998) which seems to have largely been over looked by the Pd-D community. What usually gets mentioned is their earlier experiment from 1994 and CERN's subsequent replication which did not find excess heat. It is odd that the 1998 paper makes no mention of CERN experiment. Harry Large excess heat production in Ni-H systems S. FOCARDI, V. GABBANI, V. MONTALBANO, F. PIANTELLI and S. VERONESI http://newenergytimes.com/v2/library/1998/1998FocardiS-LargeExcessHeatProductionNiH.pdf
Re: [Vo]:Large Excess heat production in Ni-H systems (Focardi et al, 1998)
H Veeder hveeder...@gmail.com wrote: This is Focardi's and Piantelli's improved experiment from the fall of 1996 (published in 1998) which seems to have largely been over looked by the Pd-D community. It is not overlooked. Everyone knows about it. But it could not be replicated, and some people question the calorimetry. Ni-H heat has not been widely replicated, but that is not for lack of trying. - Jed
Re: [Vo]:Large Excess heat production in Ni-H systems (Focardi et al, 1998)
Thanks Harry for the refresher in history. When I read this report it screams out that Rossi has something real and also why powdered nickel is such a good idea. I wonder why the earlier pioneers did not try powder to increase the surface area of the device? Rossi seems to have read the cards correctly. Dave -Original Message- From: H Veeder hveeder...@gmail.com To: vortex-l vortex-l@eskimo.com Sent: Mon, Jun 24, 2013 3:00 pm Subject: [Vo]:Large Excess heat production in Ni-H systems (Focardi et al, 1998) This is Focardi's and Piantelli's improved experiment from the fall of 1996 (published in 1998) which seems to have largely been over looked by the Pd-D community. What usually gets mentioned is their earlier experiment from 1994 and CERN's subsequent replication which did not find excess heat. It is odd that the 1998 paper makes no mention of CERN experiment. Harry Large excess heat production in Ni-H systems S. FOCARDI, V. GABBANI, V. MONTALBANO, F. PIANTELLI and S. VERONESI http://newenergytimes.com/v2/library/1998/1998FocardiS-LargeExcessHeatProductionNiH.pdf
Re: [Vo]:Large Excess heat production in Ni-H systems (Focardi et al, 1998)
The surface area of the powder is important, but it may be the magnetic nature of the nickel that is a critical factor in LENR. When the temperature of nickel exceeds its curie temperature, the global magnetic property of the metal breaks down by heat induced formation of nano-scopic areas of magnetic domains that become correlated. These structures provide the electron vortex rotations required for the formation of anapole magnetic moments. Direct observation and dynamics of spontaneous skyrmion-like magnetic domains in a ferromagnet * http://www.nature.com/nnano/journal/vaop/ncurrent/abs/nnano.2013.69.html?WT.mc_id=TWT_NatureNano * The structure and dynamics of submicrometre magnetic domains are the main factors determining the physical properties of magnetic materials1http://www.nature.com/nnano/journal/vaop/ncurrent/full/nnano.2013.69.html#ref1, 2http://www.nature.com/nnano/journal/vaop/ncurrent/full/nnano.2013.69.html#ref2. Here, we report the first observation of skyrmion-like magnetic nanodomains in a ferromagnetic manganite, La0.5Ba0.5MnO3, using Lorentz transmission electron microscopy (LTEM). The skyrmion-like magnetic domains appear as clusters above the Curie temperature. We found that the repeated reversal of magnetic chirality is caused by thermal fluctuation. The closely spaced clusters exhibit dynamic coupling, and the repeated magnetization reversal becomes fully synchronized with the same chirality. Quantitative analysis of such dynamics was performed by LTEM to directly determine the barrier energy for the magnetization reversal of skyrmion-like nanometre domains. This study is expected to pave the way for further investigation of the unresolved nature and dynamics of magnetic vortex-like nanodomains.** * * * * On Mon, Jun 24, 2013 at 5:51 PM, David Roberson dlrober...@aol.com wrote: Thanks Harry for the refresher in history. When I read this report it screams out that Rossi has something real and also why powdered nickel is such a good idea. I wonder why the earlier pioneers did not try powder to increase the surface area of the device? Rossi seems to have read the cards correctly. Dave -Original Message- From: H Veeder hveeder...@gmail.com To: vortex-l vortex-l@eskimo.com Sent: Mon, Jun 24, 2013 3:00 pm Subject: [Vo]:Large Excess heat production in Ni-H systems (Focardi et al, 1998) This is Focardi's and Piantelli's improved experiment from the fall of 1996 (published in 1998) which seems to have largely been over looked by the Pd-D community. What usually gets mentioned is their earlier experiment from 1994 and CERN's subsequent replication which did not find excess heat. It is odd that the 1998 paper makes no mention of CERN experiment. Harry Large excess heat production in Ni-H systems S. FOCARDI, V. GABBANI, V. MONTALBANO, F. PIANTELLI and S. VERONESI http://newenergytimes.com/v2/library/1998/1998FocardiS-LargeExcessHeatProductionNiH.pdf
Re: [Vo]:Large Excess heat production in Ni-H systems (Focardi et al, 1998)
On Mon, Jun 24, 2013 at 3:44 PM, Jed Rothwell jedrothw...@gmail.com wrote: H Veeder hveeder...@gmail.com wrote: This is Focardi's and Piantelli's improved experiment from the fall of 1996 (published in 1998) which seems to have largely been over looked by the Pd-D community. It is not overlooked. Everyone knows about it. But it could not be replicated, and some people question the calorimetry. Ni-H heat has not been widely replicated, but that is not for lack of trying. - Jed Every knows about it, is not the same as every one has read it. Harry
Re: [Vo]:Large Excess heat production in Ni-H systems (Focardi et al, 1998)
H Veeder hveeder...@gmail.com wrote: Every knows about it, is not the same as every one has read it. Everyone talked about it! Piantelli rubs some people the wrong way. - Jed
