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Welcome to my homepage, developing the classic head physics
Binding molecule.

When atomic nuclei are bound together, creating a network of bonds is created which forms a molecule.

There are two particles that are stable at rest (an electron and a proton) they have many properties to trap, but there are also some properties that are different, you can see more about it in the middle section (Mass formation).

The proton also called hydrogen H1, has its mass stabilization c2 and is part of the structure of the nuclear nucleus and in molar bonds.

The electron has its mass stabilization c.
The mass stabilization means it is locked and it does not form part of any bonds.
I use the term for it; that it is the ghost particle of the universe.

There is only one way a molecule can be formed;
It is the mass attraction of the atomic nucleus that tries to contract the molecule and it is the atomic nucleus radiation system that tries to push the molecule apart.
The common term is the black body radiation pressure and used in astronomy, such as the Sun. Radiation pressure in molecules looks a little more complicated but that's just a challenge.

The strongest links come first and the weak ones eventually.
We get the following order:
Chemical bonding
Molebinding Step 1 (Plastic and equivalent products)
Molecular binding step 2 (bio molecule parts and the like)
Molecular binding step 3 (weakest link; molecular composition, such as viruses, bacteria and bodies that can mutate, these linkages are thermally weak).

Like the nucleus of the atom, we also have sub-molecules here, because the stabilization points oscillate above the balance point and sometimes form in a form that enzymes use as molecular structures to separate other molecules.
After this, there are no more possible bonding options.

I am currently working on developing the classic principal physics and nuclear structure.
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 Appeal

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,
is the mass attraction from the core of the atom at a given distance.
Vx 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 nuclei
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.

Make the program so that in the initial phase there is a great distance between the atomic nuclei and let the program slowly pull them together.

The program shall simulate all the links as shown in fig.23a. When all links have the same force each other your molecule is finished.


The Universe.

Classic big bang.

Mass formation.

Atom structure.

Atom binding.

Molecular binding.

Particle radiation

Magnetic fields.

Mass attraction.


Micro physics



Ultima update : 01 July 2020
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