Примери коришћења Binding energy на Енглеском и њихови преводи на Српски
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Ni has the highest nuclear binding energy of any nuclide.
The binding energy per nucleon increases with mass number up to nickel-62.
Nickel-62 has the highest binding energy per nucleon of any isotope.
A correction must also be made for the mass equivalent of the binding energy Eb.
Notice that iron-56 has the most binding energy per nucleon, making it the most stable nucleus.
The binding energy E of such a neutron star, when expressed in mass units via E=mc², is the equivalence of 1 solar mass.
More accurate calculations taking into account the effects of the finite size of the nucleus indicate that the binding energy first exceeds 2mc2 for Z> Zcr≈ 173.
Nickel-62 has the highest binding energy per nucleon of any isotope for any element(8.7946 Mev/nucleon).
A uranium-235 atom absorbs a neutron, and splits into two new atoms(fission fragments),releasing three new neutrons and a large amount of binding energy.
I understand that the binding energy of the nucleus is released when the atom is assembled from its constituent nucleons.
The amount of energy needed to remove oradd an electron- the electron binding energy- is far less than the binding energy of nucleons.
This helium-4 binding energy also accounts for why it is a product of nuclear fusion and radioactive decay.
More accurate calculations taking into account the effects of the finite size of the nucleus indicate that the binding energy first exceeds the limit for elements with more than 173 protons.
The difference in binding energy(comparing the before and after states) determines which decays are energetically possible and which are not.
In inelastic collisions, kinetic energy is dissipated in various forms of energy, such as heat,sound, binding energy(breaking bound structures).
This is due to the very high nuclear binding energy of helium-4 with respect to the next three elements after helium.
Skimming the textbook does not prepare a student for questions such as«Outline in detail the mechanism of hydrolysis of a peptide bond by trypsin,paying special attention to the role of transition state binding energy.».
This helium-4 binding energy also accounts for its commonality as a product in both nuclear fusion and radioactive decay.
I said,"We didn't pass through each other because elementary particles have mass andbecause the space between elementary particles is filled with the binding energy that also has the properties of mass, and we've known that for 800 years.".
The binding energy E of such a neutron star, when expressed in mass units via the mass-energy equivalence formula E= mc2, is 1 solar mass.
However, since the mass of protons and deuterons can be measured by mass spectrometry, the mass of a neutron can be deduced by subtracting proton mass from deuteron mass,with the difference being the mass of the neutron plus the binding energy of deuterium(expressed as a positive emitted energy). .
Any mass defect due to nuclear binding energy is experimentally a small fraction(less than 1%) of the mass of equal number of free nucleons.
Although for Z> 137, the wave function of the Dirac ground state is oscillatory, rather than bound, and there is no gap between the positive and negative energy spectra, as in the Klein paradox,[13]more accurate calculations taking into account the effects of the finite size of the nucleus indicate that the binding energy first exceeds 2mc2 for Z> Zcr≈ 173.
This deficit is part of the binding energy of the new nucleus, and it is the non-recoverable loss of the energy that causes the fused particles to remain together in a state that requires this energy to separate.
Unequal fissions are energetically more favorable because this allows one product to be closer to the energetic minimum near mass 60 u(only a quarter of the average fissionable mass),while the other nucleus with mass 135 u is still not far out of the range of the most tightly bound nuclei(another statement of this, is that the atomic binding energy curve is slightly steeper to the left of mass 120 u than to the right of it).
The weak interaction does not produce bound states nor does it involve binding energy- something that gravity does on an astronomical scale, that the electromagnetic force does at the atomic level, and that the strong nuclear force does inside nuclei.
In the first few superactinides, the binding energies of the added electrons are predicted to be small enough that they can lose all their valence electrons;
In the first few superactinides, the binding energies of the added electrons are predicted to be small enough that they can lose all their valence electrons; for example, unbihexium(element 126) could easily form a +8 oxidation state, and even higher oxidation states for the next few elements may be possible.
He treated the structure of the various nuclear components discussing their binding energies and their stability.
In works such as The Solitary One(1911), details of the figure are eliminated andthe massive forms seem ready to explode with bound energy.