<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>α</mml:mi></mml:math>-cluster structure of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow/><mml:mrow><mml:mn>44</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">Ti</mml:mi></mml:math>in core-excited<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>α</mml:mi><mml:mrow><mml:msup><mml:mrow><mml:mo>+</mml:mo></mml:mrow><mml:mrow><mml:mn>40</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mi mathvariant="normal">Ca</mml:mi></mml:math>model
書誌事項
- 公開日
- 1998-05-01
- 権利情報
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- http://link.aps.org/licenses/aps-default-license
- DOI
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- 10.1103/physrevc.57.2760
- 公開者
- American Physical Society (APS)
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説明
It is shown that all the rotational bands in ${}^{44}\mathrm{Ti}$ at low and high excitation energies can be well explained in an $\ensuremath{\alpha}$-cluster model in which the $\ensuremath{\alpha}$-like excitation of the core, ${}^{40}\mathrm{Ca}$, is incorporated by employing density-dependent M3Y (DDM3Y) double folding potentials.
収録刊行物
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- Physical Review C
-
Physical Review C 57 (5), 2760-2762, 1998-05-01
American Physical Society (APS)
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詳細情報 詳細情報について
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- CRID
- 1363388845176989696
-
- ISSN
- 1089490X
- 05562813
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- データソース種別
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- Crossref
- OpenAIRE
