the new fuels with magnecular structure - Institute for Basic Research

52 RUGGERO MARIA SANTILLI
It should be stressed that the lack of verification of any one of the above conditions
generally implies the impossibility to detect magnecules. For instance, the
use of a feeding line with 0.5 mm ID is un-necessarily large for a conventional
light gas, while it is necessary for a gas with magnecular structure such as magnegas.
This is due to the unique adhesion of the magnecules against the walls
of the feeding line, resulting in occluded lines which prevent the passage of the
most important magnecules to be detected, those with large atomic weight.
Similarly, it is customary for tests of conventional gases to use GC-MS with
columns at high temperature to obtain readings in the shortest possible time,
since conventional molecules are perfectly stable under the temperatures here
considered. The use of such method would equally prevent the test of the very
species to be detected, because, as indicated earlier, they have a characteristic
Curie Temperature at which all magnetic features are lost. Magnecules are stable
at ordinary temperatures and, consequently, they should be measured at ordinary
temperatures.
Along similar lines, recall that GC-MS with a short ramp time are generally
used for rapidity of results. Again, the use of such a practice, which has been
proven by extensive evidence to be effective for molecules, prevents clear detection
of magnecules. If the ramp time is not of the order of 25 minutes, e.g., it is of
the order of one minute, all the peaks of magnecules generally combine into one
single large peak, as described below. In this case the analyst is generally lead
to inspect an individual section of said large peak. However, in so doing, the
analyst identifies conventional molecules constituting the magnecule, and not the
magnecule itself.
When these detectors with short ramp times are equipped with IRD, the latter
identify the infrared signatures of individual conventional molecules constituting
said large unique peak, and do not identify the possible IR signature of the single
large peak itself. Therefore, a GC-MS with short ramp time is basically unsuited
for the detection of magnecules because it cannot separate all existing species
into individual peaks.
In conclusion, the experimental evidence of the above occurrences establishes
the need in the detection of gas magnecules of avoiding, rather than using, techniques
and equipment with a proved efficiency for molecules, thus avoiding the
use of GC-MS without IRD, with short ramp time, high column temperatures,
microscopic feeding lines, and other techniques. On the contrary, new techniques
specifically conceived for the detection of magnecules should be worked out.