the new fuels with magnecular structure - Institute for Basic Research

THE NEW FUELS WITH MAGNECULAR STRUCTURE 43
The infrared signatures of conventional molecules constituting magnecules are
expected to be mutated, in the sense that the shape of their peaks is not the
conventional one. As indicated in the preceding section, the mutations most important
for industrial applications are those due to the presence of new IR peaks
representing new internal bonds. Nevertheless, various other forms of IR mutations
are possible.
Feature 5: Mutation of magnecular weights.
While molecules preserve their structure and related atomic weight at conventional
temperatures and pressures, this is not the case for gas magnecules,
which can mutate in time, that is, change their atomic weight with consequential
change of the shape and location of their MS peaks. Since we are referring
to gases whose constituents notoriously collide with each other, magnecules can
break-down during collisions into fragments which can then recombine with other
fragments or other magnecules to form new clusters.
Feature 6: Accretion or emission of individual atoms, dimers or
molecules.
Magnecules are expected to experience accretion or emission of individual
atoms, dimer or molecules without necessarily breaking down into parts. It follows
that the peaks of Feature 1 are not expected to remain the same over a
sufficient period of time for the same gas under the same conditions.
Feature 7: Anomalous adhesion.
Magnetically polarized gases have anomalous adhesion to walls of disparate
nature, not necessarily of paramagnetic character, as compared to the same unpolarized
gas. This is due to the well-known property that magnetism can be
propagated by induction, according to which a magnetically polarized molecule
with a sufficiently intense magnetic moment can induce a corresponding polarization
of valence and/or other electrons in the atoms constituting the wall surface.
Once such a polarization is created by induction, magnecules can have strong
magnetic bonds to the indicated walls. In turn, this implies that the background
of GC-MS following scans and conventional flushing are often similar to the scan
themselves. As a matter of fact, backgrounds following routine flushing are often
used to identify the most dominant magnecules. Notice that the magnetic polarization
here considered does not require that the walls of the instrument are of