The TDHF code Sky3D version 1.2
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arXiv
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| Hauptverfasser: | , , , , |
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| Format: | Preprint |
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2024
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| _version_ | 1866910446557069312 |
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| author | Abhishek Stevenson, Paul Shi, Yue Yüksel, Esra Umar, Sait |
| author_facet | Abhishek Stevenson, Paul Shi, Yue Yüksel, Esra Umar, Sait |
| contents | The Sky3D code has been widely used to describe nuclear ground states, collective vibrational excitations, and heavy-ion collisions. The approach is based on Skyrme forces or related energy density functionals. The static and dynamic equations are solved on a three-dimensional grid, and pairing is been implemented in the BCS approximation. This updated version of the code aims to facilitate the calculation of nuclear strength functions in the regime of linear response theory, while retaining all existing functionality and use cases. The strength functions are benchmarked against available RPA codes, and the user has the freedom of choice when selecting the nature of external excitation (from monopole to hexadecapole and more). Some utility programs are also provided that calculate the strength function from the time-dependent output of the dynamic calculations of the Sky3D code. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2405_08531 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | The TDHF code Sky3D version 1.2 Abhishek Stevenson, Paul Shi, Yue Yüksel, Esra Umar, Sait Computational Physics Nuclear Theory The Sky3D code has been widely used to describe nuclear ground states, collective vibrational excitations, and heavy-ion collisions. The approach is based on Skyrme forces or related energy density functionals. The static and dynamic equations are solved on a three-dimensional grid, and pairing is been implemented in the BCS approximation. This updated version of the code aims to facilitate the calculation of nuclear strength functions in the regime of linear response theory, while retaining all existing functionality and use cases. The strength functions are benchmarked against available RPA codes, and the user has the freedom of choice when selecting the nature of external excitation (from monopole to hexadecapole and more). Some utility programs are also provided that calculate the strength function from the time-dependent output of the dynamic calculations of the Sky3D code. |
| title | The TDHF code Sky3D version 1.2 |
| topic | Computational Physics Nuclear Theory |
| url | https://arxiv.org/abs/2405.08531 |