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the new fuels with magnecular structure - Institute for Basic Research

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114 RUGGERO MARIA SANTILLI<br />

Figure 38. A view of one of <strong>the</strong> numerous GC-MS scans conducted at <strong>the</strong> Toxic Analytic<br />

Laboratory in Cali<strong>for</strong>nia establishing in a final <strong>for</strong>m <strong>the</strong> <strong>magnecular</strong> character of <strong>the</strong> species<br />

here studied. In fact, <strong>the</strong> molecular seeving process used by Adsorption <strong>Research</strong> Laboratory<br />

could only allow <strong>the</strong> separation of hydrogen and definitely not <strong>the</strong> numerous heavy clusters<br />

identified in this scan. Since hydrogen has only one electron and, consequently can only <strong>for</strong>m<br />

under valence bond H 2, <strong>the</strong> heavy species of hydrogen here considered establishes <strong>the</strong> existence<br />

of a non-valence bond beyond any possible or o<strong>the</strong>rwise credible doubt.<br />

3) The same type of MH used in <strong>the</strong> preceding tests was submitted to CG-<br />

MS scans via <strong>the</strong> use of a HP GC 5890 and a HP MS 5972 <strong>with</strong> operating<br />

conditions specifically set <strong>for</strong> <strong>the</strong> detection of magnecules (Section 5 and Ref. [5]).<br />

The results of <strong>the</strong>se third tests are reproduced in Fig. 37. As one can see, by<br />

keeping in mind <strong>the</strong> results of GC-FTIS of Fig. 36, <strong>the</strong> GC-MS measurements<br />

should have shown only two peaks, that <strong>for</strong> hydrogen H 2 at about 2 a.m.u., and<br />

that <strong>for</strong> methane CH 4 at about 16 a.m.u. On <strong>the</strong> contrary, <strong>the</strong>se GC-MS tests<br />

confirm <strong>the</strong> existence of a large peak at about 2 a.m.u. evidently representing<br />

hydrogen, but do not show any peak at 16 a.m.u. proportional to <strong>the</strong> 0.78% of<br />

methane, and exhibit instead <strong>the</strong> presence of a considerable number of additional<br />

peaks in macroscopic percentages all <strong>the</strong> way to 18 a.m.u. This GC-MS scan<br />

establishes <strong>the</strong> existence beyond credible doubt of a <strong>magnecular</strong> <strong>structure</strong> in <strong>the</strong><br />

type of MH here studied. Note, in particular, <strong>the</strong> existence of well identified<br />

peaks in macroscopic percentage <strong>with</strong> atomic weight of 3, 4, 5, 6, 7, 8 and higher<br />

values which peaks, <strong>for</strong> <strong>the</strong> gas under consideration here, can only be explained as<br />

magnecules composed of individual H atoms as well as H molecules in increasing<br />

numbers.

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