When atomic nuclei are bound together, creating a
network of bonds is created which forms a molecule. There are two general types
When an atomic nucleus is replaced with another atom core number
of a molecular
bond, there will be a chemical reaction and there is liberated
or absorbed energy, Vol joints are strong.
When there is no change, we get a general binding molecule, eg. DNA molecules, and there will
only be a minor adjustment of the binding
energy, the connectors are weak.
It is the atomic nucleus which controls the bond joints between the individual nuclei.
There are two parts, one part will try to pull
together the atomic nuclei and the second part will try
to bump the the cores away.
It is the atomic nucleus mass attraction that tries to
pull the cores together and it is atomic nuclei radiation that attempts to push away the cores, the common name is the black body
radiation pressure and is used in astronomy, Example the sun.
Radiation pressure in atomic nuclei is more specific because it is directional specific against each of
the atomic nuclei.
I am currently working on developing the classic principal physics and nuclear
Molecular bonds is about computer simulated models, with some programming work. I therefore have to set priorities.
I do not have resources for this development work so far
I Would like to give an explanation of how it can be done.
There is a huge potential in molecular bonds. You will have knowledge of the exact coordinates set for each atomic nucleus
and the strong and weak individual link between the individual cores, and how the whole molecule affects its environments and total control
of all chemical molecule compounds.
You should be aware that when you work in and around the atomic nucleus
it is very large forces acting between the cores, but it
can be very small margins that decides the outcome, so
be careful with accuracy.
I would not recommend it
work in joule, but use of mass formula set instead
can be downloaded here.
Mass is a much simpler way to manage energy levels and makes
the programming work much easier.
Mass is energy;
The type obtained in the context of molecular bonds is of the kinetic energytype,
and the energy of atomic nuclei is rest energy.
I show the standard formula for mass attraction
The standard formula mx = (V x
x c 2 ) / V
Where V is the spacer variable
and (Vx x c2) is the atom nucleus
mass (convected Albert Einsteins formula).
is the mass attraction from the core of the atom at a given distance.
is the atomic nucleus volume, the formulas can be found here
The total mass attraction between the two atomic nuclei
is the sum of Mass1 + Mass2
mTotal = mM1 + mM2
The unknown factor in this calculation is the distance
between the two nuclei and this you need to download in a calculation based
on the mole mass.
Mass attraction is not thermally dependent and is,
therefore,a constant of the distance between two cores
You now have the force that pulls together the atomic nuclei, which is the same as trying to bump them off.
The radiation pressure is directionally between the two
It will take a very long time before it is
possible to calculate the radiation pressure from the
nuclei precisely, it will also be a clumsy way to do it.
Unlike mass attraction, the radiation
pressure is temperature dependent, and a calibration is
needed to set the parametersize, use the molar mass for it.
In addition the molemass volum and mass, the temperature you use be in Kelvin, you must also
Correct for the pressure, an ATM. = (9.8) 2 m or form
zero point at an atm.
Once you have completed this, you have a complete
set of formulas and you are ready to make your first molecule simulator.
The electrons in the molecule have a slight influence on how the bond will proceed and should in the first instance be omitted.
program so that in the initial phase there is a great distance between
the atomic nuclei and let the program slowly pull them together.
program shall simulate all the links as shown in fig.23a. When all links have
the same force each other your molecule is finished.