Study of the giant dipole resonance around the magic number 28
The present study unfolds the relative importance of N / Z , shell effects, and thermal fluctuations in shaping the temperature dependence of the isovector giant dipole resonance (IVGDR) width. To this end, we measured the γ -ray spectra from excited Zn 62 , 68 populated through 4 He + 58 , 64 Ni reactions at beam energies of 28 MeV and 40 MeV, and compared the corresponding IVGDR widths with those for nuclei close to the doubly magic 56 Ni and moderately away from it. The large-area modular BaF 2 detector array was used to detect high-energy γ rays ( E γ > 4 MeV). The Bayesian inference approach was combined with the statistical model analysis to extract the IVGDR parameters from the measured spectra. Calculation of IVGDR widths was performed using various theoretical approaches, specifically the thermal shape fluctuation model (TSFM) with microscopic energy density functional inputs. TSFM calculation was also performed using the free energy surfaces from the deformed liquid drop model. For 68 Zn, the width is observed to increase closely following the TSFM prediction. In contrast, suppression of the width is noticed for 62 Zn at low temperatures, similar to other nearby nuclei with N and/or Z closer to 28. Moreover, 68 Zn indicates an early onset of the saturation in the IVGDR width mimicking structural changes appropriately comprehended by the microscopic calculations. These findings suggest that the relative influence of microscopic effects and thermal broadening in the IVGDR width is strongly governed by the proximity of the decaying nucleus to magicity. • The isovector giant dipole resonance width in 62 Zn and 68 Zn have been measured and analyzed to understand the relative importance of N / Z , microscopic effects and thermal excitations in determining the width at temperatures around 1 MeV. • Contrasting temperature dependence of the IVGDR width is observed for 68 Zn compared to other nearby nuclei, indicating that the closeness to magicity plays a crucial role in deciding the relative importance of thermal and non-thermal characteristics of IVGDR width.
Authors
- Deepak Pandit (ORCID: https://orcid.org/0000-0002-2640-6151)
- D. Mondal (ORCID: https://orcid.org/0009-0003-8804-7398)
- Sujan Kumar Roy (ORCID: https://orcid.org/0000-0002-1688-3827)
- Rajkumar Santra (ORCID: https://orcid.org/0009-0002-0373-570X)
- Chandrani Sen (ORCID: https://orcid.org/0000-0002-5304-917X)
- Pratap Roy (ORCID: https://orcid.org/0000-0002-4838-4467)
- S. Mukhopadhyay (ORCID: https://orcid.org/0000-0003-2666-3200)
- A. De (ORCID: https://orcid.org/0000-0001-8607-4905)
- Jhilam Sadhukhan (ORCID: https://orcid.org/0000-0003-1963-1390)
- T. K. Rana (ORCID: https://orcid.org/0000-0001-7585-0753)
- Srijit Bhattacharya (ORCID: https://orcid.org/0000-0002-1513-1703)
- Gourab Banerjee (ORCID: https://orcid.org/0009-0002-7395-3198)
- Balaram Dey (ORCID: https://orcid.org/0000-0002-9168-3219)
- Surajit Pal
- Saumanti Sadhukhan
Institutions
- Variable Energy Cyclotron Centre (IN)
- Saha Institute of Nuclear Physics (IN)
- Homi Bhabha National Institute (IN)
- Raiganj University (IN)
- Bankura University (IN)
- West Bengal State University (IN)
Publication Details
- Journal
- Physics Letters B
- Published
- 2025-06-16
- DOI
- https://doi.org/10.1016/j.physletb.2025.139652
- Citations
- 1
- Primary Topic
- Quantum Chromodynamics and Particle Interactions
- Type
- article
- Field-Weighted Citation Impact
- 1.87