the new fuels with magnecular structure - Institute for Basic Research

THE NEW FUELS WITH MAGNECULAR STRUCTURE 51
the IRD and detect no signature at the 481 a.m.u. value, the only IR signature
being that at 44 a.m.u. of the CO 2 as well as those of smaller molecules. The
production of the gas under intense magnetic fields then confirm that the peak
here considered at 481 a.m.u. is indeed a magnecule composed of a large number
of ordinary light molecules, dimers and individual atoms, in accordance with
Definition.
Note that the IRD scan in the above test has solely identified conventional
molecules without any additional unknown. Yet, the conclusion that the gas
considered is solely composed of molecule would be nonscientific for numerous
reasons, such as: 1) magnetic bonds are transparent to IR scans with available
frequencies; 2) there is no IR detection, specifically, at 481 a.m.u.; and 3) IRD
do not detect molecules, but only dimers.
Therefore, even though the IRD has detected CO 2 in the above test, the actual
detection was for the C–O dimer, in which case the claim of the presence of the
full CO 2 molecule is a personal opinion, and not an experimental fact.
The anomalous energy content, weigh and other features of magnegas confirm
the above conclusions, because the latter can only be explained by assuming that
a certain percentage of IR counts is indeed due to complete molecules, while the
remaining percentage is due to unpaired dimers trapped in the magnecules. The
freeing of these dimers and atoms at the time of the combustion, and their recombination
into molecules as in Eqs. (2.5) then explains the anomalous energy
content.
In addition to the above basic requirements, numerous other precautions in
the use of the GC-MS equipped with IRD are necessary for the detection of
magnecules, such as:
i) the MS equipment should permit measurements of peaks at ordinary temperature,
and avoid the high temperatures of the GC-MS column successfully
used for molecules;
ii) the feeding lines should be cryogenically cooled;
iii) the GC-MS/IRD should be equipped with feeding lines of at least 0.5 mm
ID;
iv) the GC-MS should be set to detect peaks at large atomic weights usually
not expected; and
v) the ramp time should be the longest allowed by the instrument, e.g., of at
least 25 minutes.