coulomb barrier वाक्य
उदाहरण वाक्य
मोबाइल
- In the context of nuclear reactions this is called a Coulomb barrier.
- Is this the Coulomb barrier ? and 2 . why does it release energy?
- It is called the Coulomb barrier.
- The nuclei do not actually have to have enough energy to overcome the Coulomb barrier completely.
- The absence of the Coulomb barrier enabled the neutron's discovery by James Chadwick in 1932.
- The Coulomb barrier is smallest for isotopes of hydrogen, as their nuclei contain only a single positive charge.
- From this distribution, the fraction of particles with a velocity high enough to overcome the Coulomb barrier can be determined.
- Which is the probability of an s-wave nuclide to penetrate the Coulomb barrier, according to the WKB approximation.
- The Coulomb barrier causes the cross section to have a strong exponential dependence on the center-of-mass energy.
- The neutrino is not repelled in anyway, so there's not really a'coulomb barrier'style activation energy.
- *Ignoring the stuff about Coulomb barriers, the question seems to be asking whether it is possible that time is discrete.
- The higher the Coulomb barrier the more kinetic energy a proton requires to get close to a nucleus and be captured by it.
- In practice, temperatures needed to overcome the Coulomb barrier turn out to be smaller than expected due to quantum-mechanical Gamow.
- Even using these isotopes, the Coulomb barrier is large enough that the nuclei must be given great amounts of energy before they will fuse.
- If the energy of the incident particle is increased sufficiently, the Coulomb barrier is exceeded and the Schr�dinger's equation for each interaction.
- A proton requires more energy to be incorporated ( " captured " ) into an atomic nucleus when the Coulomb barrier is higher.
- The repulsive electrostatic force acts over longer distances, so kinetic energy is needed to overcome this " Coulomb barrier " before the reaction can take place.
- 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.
- Overcoming this repulsion costs a considerable amount of energy, which is known as the " Coulomb barrier " or " fusion barrier energy ".
- 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.
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