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The Collective Model and the Fermi Gas Model
Lesson 6 The Collective Model and the Fermi Gas Model
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Evidence for Nuclear Collective Behavior
Existence of permanently deformed nuclei, giving rise to “collective excitations”, such as rotation and vibration Systematics of low lying 2+ states in many nuclei Large transition probabilities for 2+0+ transitions in deformed nuclei Existence of giant multipole excitations in nuclei
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Deformed Nuclei Which nuclei? A= , A>220 What shapes?
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How do we describe these shapes?
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Rotational Excitations
Basic picture is that of a rigid rotor
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Are nuclei rigid rotors?
No, irrotational rigid
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Backbending
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Rotations in Odd A nuclei
The formula on the previous slide dealt with rotational excitations in e-e nuclei. What about odd A nuclei? Here one has the complication of coupling the angular momentum of the rotational motion and the angular momentum of the odd nucleon.
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Rotations in Odd A nuclei (cont.)
For K 1/2 I=K, K+1, K+2, ... For K=1/2 I=1/2, 3/2, 5/2, ...
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Nuclear Vibrations In analogy to molecules, if we have rotations, then we should also consider vibrational states How do we describe them? Most nuclei are spherical, so we base our description on vibrations of a sphere.
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Shapes of nuclei shaded areas are deformed nuclei
Types of vibrations of spherical nuclei
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Formal description of vibrations
Suppose =0 Suppose =1 Suppose =2
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Nuclear Vibrations
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Levels resulting from these motions
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You can build rotational levels on these vibrational levels
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Net Result
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Nilsson model Build a shell model on a deformed h.o. potential instead of a spherical potential Superdeformed nuclei Hyperdeformed nuclei
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Successes of Nilsson model
Nuclide Z N Exp. Shell Nilsson 19F 9 10 1/2+ 5/2+ 21Ne 11 3/2+ 21Na 23Na 12 23Mg
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Real World Nilsson Model
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Fermi Gas Model Treat the nucleus as a gas of non-interacting fermions
Suitable for predicting the properties of highly excited nuclei
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Details Consider a box with dimensions Lx,Ly,Lz in which particle states are characterized by their quantum numbers, nx,ny,nz. Change our descriptive coordinates to px,py,pz, or their wavenumbers kx,ky,kz where ki=ni/Li=pi/ The highest occupied level Fermi level.
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Making the box a nucleus
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Thermodynamics of a Fermi gas
Start with the Boltzmann equation S=kBln Applying it to nuclei
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Relation between Temperature and Level Density
Lang and LeCouteur Ericson
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What is the utility of all this?
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