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1 | Hypothesis to explain Lugano, MFMP 'Bang!' and Parkhomov observations, assuming Piantelli empirically tested theory / standard model | ||||||||||||||||||||||||||
2 | Bob W. Greenyer B.Eng.(Hons.) | NOTE: This spreadsheet is for comment only, It is subject to revision and may contain material errors | How to do a Parkhomov | ||||||||||||||||||||||||
3 | |||||||||||||||||||||||||||
4 | Piantelli patent | << Most of the basis for these calculations is here, however the 6.7MeV energy of ejected 1H and detailing of 7Li as key receiver was in his pre-Lugano | Patent extension | ||||||||||||||||||||||||
5 | Gammas reported here from previously published Piantelli experiments | ||||||||||||||||||||||||||
6 | Focardi/Rossi | << Focardi stopped working with Piantelli before Piantelli had developed his understanding of Proton capture / ejection and this shows in the Focardi/Rossi paper here | |||||||||||||||||||||||||
7 | The author has discovered this paper for the first time after completing the exercise below and it is largely in line with the work herein | ||||||||||||||||||||||||||
8 | Key from this paper is reference to other work right at the end | ||||||||||||||||||||||||||
9 | "The effect of electron screening on low-energy fusion processes has been investigated by Assembaum et al [20]: they report the increasing of the Coulomb | ||||||||||||||||||||||||||
10 | barrier penetrability and calculate, for some reactions induced by protons (p + Li7 and p + B11) quantitative effects, that look very relevant, though probably | ||||||||||||||||||||||||||
11 | not sufficient to interpret our experimental results. More recently, in a series of interesting papers [21-23], Raiola et al con- | ||||||||||||||||||||||||||
12 | firmed experimentally the significant increase of nuclear reactions cross sections in metals due to electron screening." | ||||||||||||||||||||||||||
13 | [20] H. J. Assenbaum, K. Langanke and C. Rolfs, Z. Phys. A 327, 468 (1987). | ||||||||||||||||||||||||||
14 | [21] F. Raiola et al, Eur. Phys. Journal A 13, 377 (2002). [22] F. Raiola et al, Eur. Phys. Journal A 19, 283 (2004). [23] F. Raiola et al, Eur. Phys. Journal A 27, 79 (2006). | ||||||||||||||||||||||||||
15 | |||||||||||||||||||||||||||
16 | This is not a hypothesis focussing on the mode of transmutation of Ni isotopes, such as that based on 7Li neutron transfer, it is one focussing on the Rossi/Parkhomov/MFMP results | ||||||||||||||||||||||||||
17 | Predictions assume that published Piantelli based reactions are valid and potential for ejected high energy 1H from Ni | WHAT IS AN ION? | Useful presentation on Nuclear interactions | ||||||||||||||||||||||||
18 | It is a kind of virtual electron capture | ||||||||||||||||||||||||||
19 | 1H+xNi reactions and decays are listed lower down (reactions from 15+) as are reactions between alpha and 6Li and 7Li (reactions from 31+) | Proposed | |||||||||||||||||||||||||
20 | Fuel | Product | Daughter | Further | |||||||||||||||||||||||
21 | Natural element | at | How likely? | Product | at | decay | daughter | Daughter | Phase at | Reaction | |||||||||||||||||
22 | proportion | Reaction (required energy) | 1130ºC | Products | Q-values (keV) | Threshold (keV) | stability | 1130ºC | half-life | mode(s) | isotope(s) | stability | 1130ºC | Participant | |||||||||||||
23 | use NNDC calculator here | Type "isotope of ..." and get decay tables from wikipedia | |||||||||||||||||||||||||
24 | 1 | 100.00% | 27Al + 1H(Elab=0.0 MeV) | liquid | 28Si+γ | 11585.02 | 0.100 | 0.0 0.0 | Stable | Solid | ? | ||||||||||||||||
25 | 2 | 24Mg+α | 1600.88 | 0.100 | 0.0 0.0 | Stable | liquid?* | Y | α captures electrons and becomes 4HE or may interact with 58Ni to produce 62Ni (see reaction below) | ||||||||||||||||||
26 | 3 | Trace | 26Al + 1H(Elab=0.0 MeV) | liquid | 27Si+γ | 7463.25 | 0.160 | 0.0 0.0 | unstable | 4.16(2) s | β+ | 27Al | Stable | Liquid | Y | proceed via reaction 1 | |||||||||||
27 | |||||||||||||||||||||||||||
28 | 4 | 24Mg + 1H(Elab=0.0 MeV) | liquid?* | 25Al+γ | 2271.57 | 0.470 | 0.0 0.0 | unstable | liquid | 7.183(12) s | β+ | 25Mg | Stable | Liquid?* | Y | ||||||||||||
29 | 5 | 25Mg + 1H(Elab=0.0 MeV) | liquid?* | 26Al+γ | 6306.31 | 0.050 | 0.0 0.0 | 7.17(24)×10^5 years | β+ | 26Mg | Stable | Liquid?* | Y | For the purpose of this reaction, it remains as 26Al and proceeds by reaction 3 | |||||||||||||
30 | |||||||||||||||||||||||||||
31 | 6 | 28Si + 1H(Elab=0.0 MeV) | Solid | 29P+γ | 2748.63 | 0.560 | 0.0 0.0 | unstable | gas | 4.142(15) s | β+ | 29Si | Stable | Solid | ? | Likely to boil out and condense as stable 29Si out of reaction zone | |||||||||||
32 | 7 | 29Si + 1H(Elab=0.0 MeV) | Solid | 30P+γ | 5594.50 | 0.310 | 0.0 0.0 | unstable | gas | 2.498(4) min | β+ | 30Si | Stable | Solid | ? | Likely to boil out and condense as stable 30Si out of reaction zone | |||||||||||
33 | 8 | 100.00% | 30Si + 1H(Elab=0.0 MeV) | Solid | 31P+γ | 7296.55 | 0.020 | 0.0 0.0 | Stable | gas | N*** | Likely to boil out and remain as stable 31P out of reaction zone | |||||||||||||||
34 | |||||||||||||||||||||||||||
35 | 9 | 7.59% | 6Li + 1H(Elab=0.0 MeV) | liquid | 7Be+γ | 5606.85 | 0.070 | 0.0 0.0 | 53.22(6) d | EC | 7Li | Stable | Liquid | Y | Gamma thermalised, 7Li proceeds to further stage, electron density speeds 7Be EC decay rate (H- and potential for ejected electron?) | ||||||||||||
36 | 10 | 3He+α | 4019.72 | 0.000 | 0.0 0.0 | Stable | gas | N | α captures electrons and becomes 4He, gasses leave reaction zone | ||||||||||||||||||
37 | 11 | 4He+3He | 4019.72 | 0.003 | 0.0 0.0 | Stable | gas | N | 4He and 3He leave reaction zone | ||||||||||||||||||
38 | 12 | 92.41% | 7Li + 1H(Elab=0.0 MeV) | liquid | 4He+α | 17346.20 | 0.000 | 0.0 0.0 | Stable | gas | N | α captures electrons and becomes 4He | |||||||||||||||
39 | 13 | 8Be+γ | 17254.40 | 0.040 | 0.0 0.0 | unstable | 6.7(17)×10−17 s | α | 4He | Stable | Gas | N | α captures electrons and becomes 4He | ||||||||||||||
40 | *** | NOTE: there are likely many other reactions, 31P could proceed to 32S which is stable and would go to gas phase | |||||||||||||||||||||||||
41 | |||||||||||||||||||||||||||
42 | Aluminium completely disappeared from Lugano fuel (see page 53 of Lugano report) | ||||||||||||||||||||||||||
43 | Silicon found in Lugano ash (p.53) and MFMP 'Bang!' reactor sintered core | ||||||||||||||||||||||||||
44 | Magnesium not found in ash in Lugano but present in fuel | ||||||||||||||||||||||||||
45 | Nickel oxides are very green or grey, the sintered fuel rod was never green and not grey to begin with in “Bang!” | ||||||||||||||||||||||||||
46 | Initial presence of 3 isotopes of phosphorous may account for immediate red/brown colour that fades over time to grey (with slight brown) | ||||||||||||||||||||||||||
47 | Given that the sample is claimed in Lugano to have been taken from the centre, the P would likely have condensed out at the cooler ends (280ºC) which is in line with our lower assessment of the Lugano reactors actual temperatures. | ||||||||||||||||||||||||||
48 | 28, 29 and 30Si might account for the silicon found in our Bang sintered ash rod sample and in Lugano ash | ||||||||||||||||||||||||||
49 | Higher silicon after time would account for greying of ash as would oxidation of Nickel, Parkhomovs old successful ash grey | ||||||||||||||||||||||||||
50 | Remaining potential for stable 31P could leave residual red/brown tinge, perhaps even a phosphide | Wikipedia photo of powdered Phosphorus | |||||||||||||||||||||||||
51 | Helium dissipates in chamber / maintains pressure / less likely to leak than Hydrogen | ||||||||||||||||||||||||||
52 | |||||||||||||||||||||||||||
53 | SPECULATION: Could the captured H-, through Ni nucleus reorganisation, result in 1 “virtual neutron” and an ejected electron (and nutrinos in the mix) may accelerate decay of 7Be and promote α to 4He conversion | ||||||||||||||||||||||||||
54 | β+ & β- decay | ||||||||||||||||||||||||||
55 | α decay | ||||||||||||||||||||||||||
56 | |||||||||||||||||||||||||||
57 | * Mg boiling point at 1 atm is 1091ºC, it may still be a liquid at 1130ºC at pressures calculated in 'Bang!' and 27th/2/2015 Parkhomov reactions, might want to keep below this until 27Al & Mg burned | ||||||||||||||||||||||||||
58 | |||||||||||||||||||||||||||
59 | Nickel oxides are first removed by the high pressure H2 evolved from the LiAlH4 and then fixed into Alumina. N2 is fixed into Aluminum Nitride, evidence of Nitrogen fixing | ||||||||||||||||||||||||||
60 | was found on the MFMP 'Bang!' EDX of our shards however, since we loaded under Argon, this may have happened after the breach of the core, when it was hot and exposed to the air. All the same N is present. | ||||||||||||||||||||||||||
61 | |||||||||||||||||||||||||||
62 | The Li, Al and H are the fuel and the surface area of the Nickel is the reaction surface, since the secondary reaction only takes place in the immediate vacinity of a non-changing Ni surface area, the rate is | ||||||||||||||||||||||||||
63 | relatively constant until all fuel burned. It may increase slightly as the reaction progresses due to fragments breaking away from the sintered body | ||||||||||||||||||||||||||
64 | into the liquid Li Al H. Nickel provides the key primary reaction resulting in Ni isotopic transmutation perhaps through a combination of virtual neutrons/ejected electron, | ||||||||||||||||||||||||||
65 | or Piantelli nuclear re-organisations and ejected 1H and e- which would only travel extremely small distances ordinarily, but in this case, the recipients (Li,Al,Mg and Si atoms) are directly next to the Nickel | ||||||||||||||||||||||||||
66 | Above 600bar (pressures calculated to be in MFMP and Parkhomov cells, Ni should absorb H/H- into the bulk allowing bulk transmutation over time) | ||||||||||||||||||||||||||
67 | |||||||||||||||||||||||||||
68 | 'Bang!' potential emissions at time of testing with Geiger tube | ||||||||||||||||||||||||||
69 | Half lives | ||||||||||||||||||||||||||
70 | Bang!' Minnesota | Interval | 29P | 30P (longest | Ratio of peak emission rate at this time | ||||||||||||||||||||||
71 | time past midnight | from 'Bang!' | NM** | meaningful) | |||||||||||||||||||||||
72 | 17:29:00 | Time of bang | |||||||||||||||||||||||||
73 | 34:34:00 | Time of photo | Photo | 17:05:00 | 247 | 6.84 | 0.0087360 | is 9/1000ths potentially not material | |||||||||||||||||||
74 | 45:03:00 | Testing with GM | 27:34:00 | 399 | 11.04 | 0.0004764 | is 5/10,000ths likely not material | ||||||||||||||||||||
75 | |||||||||||||||||||||||||||
76 | ** Not Meaningful as mostly decayed | ||||||||||||||||||||||||||
77 | |||||||||||||||||||||||||||
78 | Testing this hypothesis | 2 | |||||||||||||||||||||||||
79 | |||||||||||||||||||||||||||
80 | Evidence for proposed reaction zone Silicon has already been found in both Lugano and 'Bang!' experiments, does Dr. Parkhomov's 'successful' cores have Si? | ||||||||||||||||||||||||||
81 | Need to capture gas and look for helium, helium would NOT be from fusion, but from standard decay reactions. | ||||||||||||||||||||||||||
82 | Deliberately blow up reactor and immediately dump in cloud chamber, as we know there are no unstable elements in fuel, a few spirals would be interesting! | ||||||||||||||||||||||||||
83 | Look for traces of 31P | ||||||||||||||||||||||||||
84 | |||||||||||||||||||||||||||
85 | Caveats | ||||||||||||||||||||||||||
86 | |||||||||||||||||||||||||||
87 | Dr. Parkhomov's reactor tubes had high percentage of Si, the MFMP used 99.8% pure Al2O3, BUT we did have a SiC element in the mix! | ||||||||||||||||||||||||||
88 | If Phosphorous isotopes were above 300ºC and in air why did it not spontaneously ignite? | ||||||||||||||||||||||||||
89 | If minute amounts of Phosphorous did exist, it may have condensed onto the rod in H2 atmosphere because of the enclosed nature of the apparatus | ||||||||||||||||||||||||||
90 | or perhaps it was in solution with the LiAl and then came to the surface as Li solidified at 180.5ºC, below Phosphorous auto-ignition temperature in air | ||||||||||||||||||||||||||
91 | |||||||||||||||||||||||||||
92 | Nucelear Magnetic Resonance | ||||||||||||||||||||||||||
93 | |||||||||||||||||||||||||||
94 | Carbon is reported to be in the Lugano fuel but not the ash, 13C and 1H are both examples of NMR nuclei | ||||||||||||||||||||||||||
95 | Hydrogen is resonant at 50Mhz in a 1.4T field, 900mhz in a 21Tesla field | ||||||||||||||||||||||||||
96 | Could radio frequency drive the 1H or could an extremely high momentary current in a low turn coil cause very high momentary magnetic field to resonate the 1H or 13C | ||||||||||||||||||||||||||
97 | Perhaps one of these? | or a little ground Samarium-Cobalt in low temp reactor, | |||||||||||||||||||||||||
98 | |||||||||||||||||||||||||||
99 | 13C +1H would go to stable 14N that would be fixed out of the fuel by the Aluminum on the reactor walls as seen in the 'Bang!' reactor | ||||||||||||||||||||||||||
100 | 14C +1H would go to stable 15N that would be fixed out of the fuel by the Aluminum on the reactor walls as seen in the 'Bang!' reactor |