Why can we not produce a "giant" nucleus?

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Discussion Overview

The discussion centers around the question of why "giant" nuclei cannot be produced in nuclear physics, contrasting this with the existence of "giant" molecules in condensed matter physics. Participants explore the conditions necessary for large nuclei, the forces at play, and the differences between atomic and nuclear structures.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants note that while "giant" molecules exist in condensed matter physics, such as crystals, the concept does not translate to nuclear physics.
  • One participant suggests that neutron stars represent a form of "giant" nucleus, as they contain a large number of neutrons.
  • Questions are raised about the finite number of neutrons in small nuclei and the conditions necessary for the existence of "giant" atoms.
  • Several participants discuss the role of binding forces, specifically the strong nuclear force and gravitational forces in neutron stars, in countering Coulomb repulsion between protons.
  • There is mention of degeneracy pressure as a balancing force in neutron stars, alongside gravitational forces.
  • Participants express uncertainty about why adding many neutrons to a stable nucleus leads to instability, with references to beta decay as a relevant process.
  • Some participants argue that the comparison between crystals and nuclei is flawed due to the different nature of forces involved in each context.
  • There are discussions about the implications of Coulomb repulsion and the nature of forces acting on neutral matter versus charged particles.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the nature of forces in nuclei and the conditions for stability, indicating that the discussion remains unresolved on several key points.

Contextual Notes

There are limitations in the discussion regarding the assumptions made about the forces involved, the definitions of "giant" nuclei versus "giant" molecules, and the specific conditions under which beta decay occurs.

  • #31
TeethWhitener said:
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.
The repulsive force between neutral atoms is the exchange force due to the Pauli principle. It grows for ##r\to 0## only like ##r^{-1}##. An exponential is a traditional but incorrect approximation.

But I just realized that all this onöy applies to atoms and not to nuclei. It is still relevant for the formation of neutron stars since gravitation must overcome the repulsive force between atoms...
 
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  • #32
fxdung said:
But why in the Earth we only see a finite number of neutrons in atoms?What is the condition to exist a "giant" atom?
Actually, when gravity is holding them together instead of strong nuclear force (I’m talking about neutron stars) that’s the condition of having a giant atom... because gravity decays much slower than nuclear forces over distances. However, try not to make it too big because it will collapse and becomes a black hole.
 
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  • #33
What is an exchange force as Prf Neumaier said?
 
  • #35
Reminds me of an article on the Russian 'heavy isotope' factory, and their extraordinary work to push further and further beyond known nuclei, into 'super-heavy country'. Part of the problem is the lower periodic table's 'magic numbers' no longer hold. To put it politely, the nucleus becomes too big for neat 'shells' to hold sway. The hoped-for 'Island of Stability' may prove nothing more than a 'shoal'...

IMHO, chemical analogy may be gold, mercury and lead, whose nuclei are so massive they significantly alter the behaviour of their inner electron 'shells', the relativistic effects causing remarkable changes in properties. Metals, yes, but anomalous colour, melting point etc. IIRC, copper almost qualifies...

And, I learned about the 'drip line', beyond which lesser nuclei shed surplus neutrons they cannot stabilise...
 
  • #36
Apart from the giant nucleus. Why is it not possible to have a 2 neutron bound state. (I'm not sure if that should be asked in a separate thread, but it is so closely related). For the 2 neutron bound state there is no electric repulsion and if they have opposite spin they could both sit in the ground state. Shouldn't that be extremely stable?
 
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  • #38
Already the nucleon-nucleon potential is a quite complicated beast. Particularly it's spin-dependent. Model calculations, e.g., based on effective low-energy effective descriptions of the nuclear two-body force (the most modern version is based on a systematic expansion using chiral effective theory; historically there are effective one-boson exchange models like the Walecka model too), show that the two-nucleon system has only one bound state, namely the deuteron with ##S=1## and total angular momentum ##J=1##. That implies that the orbital angular momentum must be ##L=0## or ##L=2##, and indeed the bound state is a mixture of both, dominated by ##L=0## but with a small admixture of the ##L=2## state to account for the non-vanishing electrical quadrupole moment.

Now consider two protons or two neutrons. Since they are identical fermions the only bound state possible for the pn system (the deuteron) is not allowed for these systems, because for them the two-body wave function must be antisymmetric. The spatial part and spin of the bound state is symmetric, and this cannot be for pp or nn. Thus neither the pp nor the nn system have any bound state.
 

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