fxdung
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In Condensed Matter Physics there are "giant" molecules that are macro bodies(e.g crystals).But why in Nuclear Physics we can not produce a "giant" nucleus?
The discussion centers on the impossibility of producing a "giant" nucleus in Nuclear Physics, contrasting it with "giant" molecules in Condensed Matter Physics. Neutron stars exemplify large nuclear structures, where the absence of protons eliminates Coulomb repulsion, allowing gravity and degeneracy pressure to maintain stability. The strong nuclear force's short range limits the size of terrestrial nuclei, while beta decay explains the instability of large neutron-rich nuclei. The conversation highlights the complexities of nuclear forces and the conditions necessary for stable nuclear configurations.
PREREQUISITESPhysicists, astrophysicists, and students of nuclear physics seeking to understand the limitations of nuclear structure and the forces governing stability in atomic nuclei.
They exist and are called neutron stars.fxdung said:In Condensed Matter Physics there are "giant" molecules that are macro bodies(e.g crystals).But why in Nuclear Physics we can not produce a "giant" nucleus?
hilbert2 said:There needs to be a binding force that cancels the Coulomb repulsion between protons. In small nuclei it is the strong nuclear force and in neutron stars it's gravitation.
fxdung said:Why there are not too many neutrons in small nuclei?
PeterDonis said:Neutron stars have no protons so there is no Coulomb repulsion to cancel. However, Coulomb repulsion is not the only effect involved. There is also degeneracy pressure, which is what balances gravity in a neutron star.
The Coulomb force only acts between two charged particles.hilbert2 said:But isn't the coulomb force the first thing that has to be overcome when squeezing ordinary matter to neutron matter?
That was already answered: The range of the strong nuclear force is short and Coulomb repulsion (Which has infinite range) is strong.fxdung said:The vinicity neutrons have strong force,why is there a limit to how large nucleus can be(despite of short range force)?
This is not sufficient to answer the query. It only explains why nuclei with many protons cannot exist. But why adding many neutrons to a stable nucleus makes it unstable needs an additional explanation - beta decay. Wikipedia has a good synopsis.Dale said:That was already answered: The range of the strong nuclear force is short and Coulomb repulsion (Which has infinite range) is strong.
That is true, both the strong force and the weak force are important.A. Neumaier said:But why adding many neutrons to a stable nucleus makes it unstable needs an additional explanation - beta decay.
A nucleus with p protons and n neutrons will beta decay if and only if the binding energy of a nucleus with p+1 protons and n-1 neutrons is smaller by more than the mass of an electron.fxdung said:What is the condition for beta decay easily happens?
...because gravitation changes the binding energy balance. (For terrestrial nuclei gravitation is negligible.)fxdung said:And with neutron star this condition does not happen,does it?
There is alpha decay where two neutrons and two protons detach. There can also be neutrons emitted. All that matters is that the sum of the masses of the products be less than the original nucleusfxdung said:why is there not the process that neutrons detach the nuclei, but it must there be beta decay?
fxdung said:In Condensed Matter Physics there are "giant" molecules that are macro bodies(e.g crystals).But why in Nuclear Physics we can not produce a "giant" nucleus?
That is a defensible claim! Although I usually think they look more like pasta or butter, but something food-like.ZapperZ said:You might as well claim that a cow looks like a Frank Gehry building.
hilbert2 said:Even a hypothetical piece of matter composed of only protons would probably keep at constant volume if compressed below its Schwarzschild radius.
fxdung said:What is the degeneracy pressure?
PeterDonis said:No, it would collapse. A static object made of ordinary matter can't remain static at a radius below 9/8 of the Schwarzschild radius for its mass.
Neutron stars have protons - just not as many as neutrons. The interior has many neutrons and a few protons and electrons. The outer parts have nuclei and even regular atoms.PeterDonis said:Neutron stars have no protons so there is no Coulomb repulsion to cancel. However, Coulomb repulsion is not the only effect involved. There is also degeneracy pressure, which is what balances gravity in a neutron star.
mfb said:Neutron stars have protons
mfb said:The outer parts have nuclei and even regular atoms.
The ##O(r^{-6})## part of the van der Waals potential is the attractive portion of it (induced dipole-induced dipole). The repulsive portion is far more complicated, but an exponential works pretty well as an approximation.A. Neumaier said:It is the van der Waals force between neutral matter. This is still more long range (namely ##O(r^{-6})##) than the exponentially decaying strong force.