Related Experiment Video
Updated: Aug 9, 2026

10:42
Preparing an Isotopically Pure 229Th Ion Beam for Studies of 229mTh
Published on: May 3, 2019
Stabilization of nuclear isovector valence-shell excitations
G Rainovski1, N Pietralla, T Ahn
1Department of Physics and Astronomy, SUNY at Stony Brook, Stony Brook, New York 11794-3800, USA.
Physical Review Letters
|April 12, 2006
Summary
Researchers studied excited states in Cerium-138 (138Ce) using Coulomb excitation. They identified a mixed-symmetry state, finding its stability is linked to nuclear subshell structure.
Area of Science:
- Nuclear Physics
- Atomic Physics
Background:
- Understanding nuclear structure and the behavior of excited states is crucial in nuclear physics.
- Mixed-symmetry states offer insights into nuclear dynamics and collective excitations.
Purpose of the Study:
- To investigate the properties of excited states in Cerium-138 (138Ce) using Coulomb excitation.
- To identify and characterize mixed-symmetry states in 138Ce and their dependence on nuclear structure.
Main Methods:
- Utilized the 12C(138Ce, 138Ce*) Coulomb excitation reaction at 480 MeV.
- Measured relative cross sections via gamma-ray yields using the Gammasphere detector array.
- Analyzed E2 and M1 strength distributions for the lowest six 2+ states up to 2.7 MeV.
Main Results:
- Identified the 2(4)+ state in 138Ce as the primary component of the one-phonon mixed-symmetry state.
- Observed significant mixing between this mixed-symmetry state and a nearby isoscalar state.
- This mixing was found to be over four times larger than in the neighboring isotone, Barium-136 (136Ba).
Conclusions:
- The findings provide direct evidence that the stability of mixed-symmetry states is strongly influenced by the underlying nuclear subshell structure.
- The enhanced mixing in 138Ce compared to 136Ba highlights the role of specific nuclear configurations in stabilizing these states.
Related Concept Videos
Nuclear Stability
Protons and neutrons, collectively called nucleons, are packed together tightly in a nucleus. With a radius of about 10−15 meters, a nucleus is quite small compared to the radius of the entire atom, which is about 10−10 meters. Nuclei are extremely dense compared to bulk matter, averaging 1.8 × 1014 grams per cubic centimeter. If the earth’s density were equal to the average nuclear density, the earth’s radius would be only about 200 meters.
To hold positively charged protons together in the...
To hold positively charged protons together in the...
Atomic Nuclei: Nuclear Relaxation Processes
In the absence of an external magnetic field, nuclear spin states are degenerate and randomly oriented. When a magnetic field is applied, the spins begin to precess and orient themselves along (lower energy) or against (higher energy) the direction of the field. At equilibrium, a slight excess population of spins exists in the lower energy state. Because the direction of the magnetic field is fixed as the z-axis, the precessing magnetic moments are randomly oriented around the z-axis. This...
Stability of Equilibrium Configuration
Understanding the stability of equilibrium configurations is a fundamental part of mechanical engineering. In any system, there are three distinct types of equilibrium: stable, neutral, and unstable.
A stable equilibrium occurs when a system tends to return to its original position when given a small displacement, and the potential energy is at its minimum. An example of a stable equilibrium is when a cantilever beam is fixed at one end and a weight is attached to the other end. If the weight...
A stable equilibrium occurs when a system tends to return to its original position when given a small displacement, and the potential energy is at its minimum. An example of a stable equilibrium is when a cantilever beam is fixed at one end and a weight is attached to the other end. If the weight...
Nuclear Binding Energy
The difference between the calculated and experimentally measured masses is known as the mass defect of the atom. In the case of helium-4, the mass defect indicates a “loss” in mass of 4.0331 amu – 4.0026 amu = 0.0305 amu. The loss in mass accompanying the formation of an atom from protons, neutrons, and electrons is due to the conversion of that mass into energy that is evolved as the atom forms. The nuclear binding energy is the energy produced when the atoms’ nucleons are bound together;...
Atomic Nuclei: Nuclear Spin State Overview
NMR-active nuclei have energy levels called 'spin states' that are associated with the orientations of their nuclear magnetic moments. In the absence of a magnetic field, the nuclear magnetic moments are randomly oriented, and the spin states are degenerate. When an external magnetic field is applied, the spin states have only 2 + 1 orientations available to them. A proton with = ½ has two available orientations. Similarly, for a quadrupolar nucleus with a nuclear spin value of one, the...
Atomic Nuclei: Types of Nuclear Relaxation
Nuclear relaxation restores the equilibrium population imbalance and can occur via spin–lattice or spin–spin mechanisms, which are first-order exponential decay processes.
In spin–lattice or longitudinal relaxation, the excited spins exchange energy with the surrounding lattice as they return to the lower energy level. Among several mechanisms that contribute to spin–lattice relaxation, magnetic dipolar interactions are significant. Here, the excited nucleus transfers energy to a nearby...
In spin–lattice or longitudinal relaxation, the excited spins exchange energy with the surrounding lattice as they return to the lower energy level. Among several mechanisms that contribute to spin–lattice relaxation, magnetic dipolar interactions are significant. Here, the excited nucleus transfers energy to a nearby...

