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Novel Shape Evolution in Sn Isotopes from Magic Numbers 50 to 82
Tomoaki Togashi1, Yusuke Tsunoda1, Takaharu Otsuka1,2,3,4,5
1Center for Nuclear Study, University of Tokyo, Hongo, Bunkyo-ku, Tokyo 113-0033, Japan.
Physical Review Letters
|August 25, 2018
Summary
Shape evolution in tin (Sn) isotopes is explained by proton excitations from the 1g_{9/2} orbital. Monte Carlo shell model calculations reveal a quantum phase transition around neutron number 66.
Area of Science:
- Nuclear Physics
- Atomic Physics
- Quantum Mechanics
Background:
- The behavior of tin (Sn) isotopes has been a long-standing puzzle in nuclear physics.
- Understanding shape evolution and phase transitions in atomic nuclei is crucial for nuclear structure theory.
Purpose of the Study:
- To present a unified explanation for the novel shape evolution observed in Sn isotopes (100-138Sn).
- To elucidate the underlying mechanisms driving the significant increase in B(E2;0_{1}^{+}→2_{1}^{+}) values around 110Sn.
- To identify and characterize quantum phase transitions in this isotopic chain.
Main Methods:
- State-of-the-art Monte Carlo shell model calculations.
- Utilizing a large model space with eight single-particle orbits for protons and neutrons.
- Activating protons in the 1g_{9/2} orbital with a fixed Hamiltonian and effective charges.
Main Results:
- A novel shape evolution across the Sn isotopes (100-138Sn) is successfully explained.
- The increase in B(E2;0_{1}^{+}→2_{1}^{+}) values is attributed to shape evolution driven by proton excitations from the 1g_{9/2} orbital.
- A second-order quantum phase transition is identified around neutron number N=66, linking deformed and spherical pairing phases.
Conclusions:
- The study provides a comprehensive description of shape and shell evolution in Sn isotopes.
- Findings cover phenomena from the Gamow-Teller decay of 100Sn to the enhanced double magicity of 132Sn.
- Proton excitations play a key role in the observed nuclear structure changes.
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