dorsal/arxiv
View SchemaReply to Comment on Extension of the Bethe-Weizsacker mass formula to light nuclei and some new shell closures
| Authors | C. Samanta, S. Adhikari |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/0405009 |
| URL | https://arxiv.org/abs/nucl-th/0405009 |
| DOI | 10.1103/PhysRevC.69.049804 |
| Journal | Phys.Rev. C69 (2004) 049804 |
Abstract
Some properties of the modified Bethe-Weizsacker mass formula (BWM) are discussed. As BWM has no shell effect included, the extra-stability or, magicity in nuclei clearly stands out when experimental mass data are compared with BWM predictions. If the shell effect quenches, the BWM predictions come closer to the experimental data.
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"abstract": "Some properties of the modified Bethe-Weizsacker mass formula (BWM) are\ndiscussed. As BWM has no shell effect included, the extra-stability or,\nmagicity in nuclei clearly stands out when experimental mass data are compared\nwith BWM predictions. If the shell effect quenches, the BWM predictions come\ncloser to the experimental data.",
"arxiv_id": "nucl-th/0405009",
"authors": [
"C. Samanta",
"S. Adhikari"
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"doi": "10.1103/PhysRevC.69.049804",
"journal_ref": "Phys.Rev. C69 (2004) 049804",
"title": "Reply to Comment on Extension of the Bethe-Weizsacker mass formula to light nuclei and some new shell closures",
"url": "https://arxiv.org/abs/nucl-th/0405009"
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