*Ignoring the stuff about Coulomb barriers, the question seems to be asking whether it is possible that time is discrete.
12.
The higher the Coulomb barrier the more kinetic energy a proton requires to get close to a nucleus and be captured by it.
13.
In practice, temperatures needed to overcome the Coulomb barrier turn out to be smaller than expected due to quantum-mechanical Gamow.
14.
Even using these isotopes, the Coulomb barrier is large enough that the nuclei must be given great amounts of energy before they will fuse.
15.
If the energy of the incident particle is increased sufficiently, the Coulomb barrier is exceeded and the Schr�dinger's equation for each interaction.
16.
A proton requires more energy to be incorporated ( " captured " ) into an atomic nucleus when the Coulomb barrier is higher.
17.
The repulsive electrostatic force acts over longer distances, so kinetic energy is needed to overcome this " Coulomb barrier " before the reaction can take place.
18.
Their experiments indicated a nuclear interaction at lower energies than would be expected from a simple calculation of the Coulomb barrier between a deuteron and a target nucleus.
19.
Overcoming this repulsion costs a considerable amount of energy, which is known as the " Coulomb barrier " or " fusion barrier energy ".
20.
Under conditions encountered in astrophysical environments it is difficult to obtain p-nuclei through proton captures because the Coulomb barrier of a nucleus increases with increasing Proton number.
