Comment on 'From Coulomb excitation cross sections to nonresonant astrophysical rates in three-body systems: The Ne-17 case'

Casal J.; Rodriguez-Gallardo M.; Arias J. M.; Garrido E.; de Diego R.

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Comment on 'From Coulomb excitation cross sections to nonresonant astrophysical rates in three-body systems: The Ne-17 case'

机译：评论“从三体系中的非伦族天体物理率从库仑激励横断面评论：NE-17案例”

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Parfenova et al. state in [Phys. Rev. C 98, 034608 (2018)] that the results presented by Casal et al. [Phys. Rev. C 94, 054622 (2016)] concerning the radiative capture for Ne-17 formation are incorrect and their conclusions erroneous mainly because of two reasons: (1) it is "expressed" that the resonant rate is not important for O-15(2p, gamma)Ne-17 since it is negligibly small compared with the nonresonant contribution to the rate, and (2) the electromagnetic dipole cross section predicted is dramatically different from the available experimental data for Ne-17 + Pb-208 at 500 MeV/u [Phys. Lett. B 759, 200 (2016)]. We demonstrate here that these conclusions are incorrectly extracted from our work.

机译：Parfenova等人在[Phys.Rev.C 98，034608（2018）]中指出，Casal等人[Phys.Rev.C 94，054622（2016）]提出的关于Ne-17形成的辐射俘获的结果是不正确的，他们的结论是错误的，主要是因为两个原因：（1）“表示”共振率对O-15（2p，γ）Ne-17不重要，因为它与对速率的非共振贡献，以及（2）预测的电磁偶极子截面与在500 MeV/u下的Ne-17+Pb-208的可用实验数据显著不同[Phys.Lett.B 759200（2016）]。我们在此证明，这些结论是从我们的工作中错误地提取出来的。

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《Physical review, C》 |2020年第6期|共2页
作者
Casal J.; Rodriguez-Gallardo M.; Arias J. M.; Garrido E.; de Diego R.;
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Dipartimento Fis &

Astron G Galilei Via Marzolo 8 I-35131 Padua Italy;

Univ Seville Fac Fis Dept Fis Aom Mol &

Nucl Apartado 1065 E-41080 Seville Spain;

Univ Seville Fac Fis Dept Fis Aom Mol &

Nucl Apartado 1065 E-41080 Seville Spain;

CSIC Inst Estruct Mat Serrano 123 E-28006 Madrid Spain;

Univ Complutense Madrid Dept Estruct Mat Fis Term &

Elect E-28040 Madrid Spain;

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中图分类原子核物理学、高能物理学;
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Comment on 'From Coulomb excitation cross sections to nonresonant astrophysical rates in three-body systems: The Ne-17 case'

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