Proton Distribution Radii of O 16-24: Signatures of New Shell Closures and Neutron Skin

S. Kaur; R. Kanungo; W. Horiuchi; G. Hagen; J. D. Holt; B. S. Hu; T. Miyagi; T. Suzuki; F. Ameil; J. Atkinson; Y. Ayyad; S. Bagchi; D. Cortina-Gil; I. Dillmann; A. Estradé; A. Evdokimov; F. Farinon; H. Geissel; G. Guastalla; R. Janik; R. Knöbel; J. Kurcewicz; Yu A. Litvinov; M. Marta; M. Mostazo; I. Mukha; C. Nociforo; H. J. Ong; T. Otsuka; S. Pietri; A. Prochazka; C. Scheidenberger; B. Sitar; P. Strmen; M. Takechi; J. Tanaka; I. Tanihata; S. Terashima; J. Vargas; H. Weick; J. S. Winfield

doi:10.1103/PhysRevLett.129.142502

Proton Distribution Radii of O 16-24: Signatures of New Shell Closures and Neutron Skin

S. Kaur
, R. Kanungo
, W. Horiuchi
, G. Hagen
, J. D. Holt
, B. S. Hu
, T. Miyagi
, T. Suzuki
, F. Ameil
, J. Atkinson
, Y. Ayyad
, S. Bagchi
, D. Cortina-Gil
, I. Dillmann
, A. Estradé
, A. Evdokimov
, F. Farinon
, H. Geissel
, G. Guastalla
, R. Janik

R. Knöbel, J. Kurcewicz, Yu A. Litvinov, M. Marta, M. Mostazo, I. Mukha, C. Nociforo, H. J. Ong, T. Otsuka, S. Pietri, A. Prochazka, C. Scheidenberger, B. Sitar, P. Strmen, M. Takechi, J. Tanaka, I. Tanihata, S. Terashima, J. Vargas, H. Weick, J. S. Winfield

物理学院

科研成果: 期刊稿件 › 文章 › 同行评审

37 引用（Scopus）

摘要

The root mean square radii of the proton density distribution in O16-24 derived from measurements of charge changing cross sections with a carbon target at ∼900A MeV together with the matter radii portray thick neutron skin for O22-24 despite O22,24 being doubly magic. Imprints of the shell closures at N=14 and 16 are reflected in local minima of their proton radii that provide evidence for the tensor interaction causing them. The radii agree with ab initio calculations employing the chiral NNLOsat interaction, though skin thickness predictions are challenged. Shell model predictions agree well with the data.

源语言	英语
文章编号	142502
期刊	Physical Review Letters
卷	129
期	14
DOI	https://doi.org/10.1103/PhysRevLett.129.142502
出版状态	已出版 - 30 9月 2022

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Kaur, S., Kanungo, R., Horiuchi, W., Hagen, G., Holt, J. D., Hu, B. S., Miyagi, T., Suzuki, T., Ameil, F., Atkinson, J., Ayyad, Y., Bagchi, S., Cortina-Gil, D., Dillmann, I., Estradé, A., Evdokimov, A., Farinon, F., Geissel, H., Guastalla, G., ... Winfield, J. S. (2022). Proton Distribution Radii of O 16-24: Signatures of New Shell Closures and Neutron Skin. Physical Review Letters, 129(14), 文章 142502. https://doi.org/10.1103/PhysRevLett.129.142502

@article{37902c2fe002450c92cf6819c488439d,

title = "Proton Distribution Radii of O 16-24: Signatures of New Shell Closures and Neutron Skin",

abstract = "The root mean square radii of the proton density distribution in O16-24 derived from measurements of charge changing cross sections with a carbon target at ∼900A MeV together with the matter radii portray thick neutron skin for O22-24 despite O22,24 being doubly magic. Imprints of the shell closures at N=14 and 16 are reflected in local minima of their proton radii that provide evidence for the tensor interaction causing them. The radii agree with ab initio calculations employing the chiral NNLOsat interaction, though skin thickness predictions are challenged. Shell model predictions agree well with the data.",

author = "S. Kaur and R. Kanungo and W. Horiuchi and G. Hagen and Holt, \{J. D.\} and Hu, \{B. S.\} and T. Miyagi and T. Suzuki and F. Ameil and J. Atkinson and Y. Ayyad and S. Bagchi and D. Cortina-Gil and I. Dillmann and A. Estrad{\'e} and A. Evdokimov and F. Farinon and H. Geissel and G. Guastalla and R. Janik and R. Kn{\"o}bel and J. Kurcewicz and Litvinov, \{Yu A.\} and M. Marta and M. Mostazo and I. Mukha and C. Nociforo and Ong, \{H. J.\} and T. Otsuka and S. Pietri and A. Prochazka and C. Scheidenberger and B. Sitar and P. Strmen and M. Takechi and J. Tanaka and I. Tanihata and S. Terashima and J. Vargas and H. Weick and Winfield, \{J. S.\}",

note = "Publisher Copyright: {\textcopyright} 2022 American Physical Society.",

year = "2022",

month = sep,

day = "30",

doi = "10.1103/PhysRevLett.129.142502",

language = "英语",

volume = "129",

journal = "Physical Review Letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "14",

}

Kaur, S, Kanungo, R, Horiuchi, W, Hagen, G, Holt, JD, Hu, BS, Miyagi, T, Suzuki, T, Ameil, F, Atkinson, J, Ayyad, Y, Bagchi, S, Cortina-Gil, D, Dillmann, I, Estradé, A, Evdokimov, A, Farinon, F, Geissel, H, Guastalla, G, Janik, R, Knöbel, R, Kurcewicz, J, Litvinov, YA, Marta, M, Mostazo, M, Mukha, I, Nociforo, C, Ong, HJ, Otsuka, T, Pietri, S, Prochazka, A, Scheidenberger, C, Sitar, B, Strmen, P, Takechi, M, Tanaka, J, Tanihata, I, Terashima, S, Vargas, J, Weick, H & Winfield, JS 2022, 'Proton Distribution Radii of O 16-24: Signatures of New Shell Closures and Neutron Skin', Physical Review Letters, 卷 129, 号码 14, 142502. https://doi.org/10.1103/PhysRevLett.129.142502

TY - JOUR

T1 - Proton Distribution Radii of O 16-24

T2 - Signatures of New Shell Closures and Neutron Skin

AU - Kaur, S.

AU - Kanungo, R.

AU - Horiuchi, W.

AU - Hagen, G.

AU - Holt, J. D.

AU - Hu, B. S.

AU - Miyagi, T.

AU - Suzuki, T.

AU - Ameil, F.

AU - Atkinson, J.

AU - Ayyad, Y.

AU - Bagchi, S.

AU - Cortina-Gil, D.

AU - Dillmann, I.

AU - Estradé, A.

AU - Evdokimov, A.

AU - Farinon, F.

AU - Geissel, H.

AU - Guastalla, G.

AU - Janik, R.

AU - Knöbel, R.

AU - Kurcewicz, J.

AU - Litvinov, Yu A.

AU - Marta, M.

AU - Mostazo, M.

AU - Mukha, I.

AU - Nociforo, C.

AU - Ong, H. J.

AU - Otsuka, T.

AU - Pietri, S.

AU - Prochazka, A.

AU - Scheidenberger, C.

AU - Sitar, B.

AU - Strmen, P.

AU - Takechi, M.

AU - Tanaka, J.

AU - Tanihata, I.

AU - Terashima, S.

AU - Vargas, J.

AU - Weick, H.

AU - Winfield, J. S.

PY - 2022/9/30

Y1 - 2022/9/30

N2 - The root mean square radii of the proton density distribution in O16-24 derived from measurements of charge changing cross sections with a carbon target at ∼900A MeV together with the matter radii portray thick neutron skin for O22-24 despite O22,24 being doubly magic. Imprints of the shell closures at N=14 and 16 are reflected in local minima of their proton radii that provide evidence for the tensor interaction causing them. The radii agree with ab initio calculations employing the chiral NNLOsat interaction, though skin thickness predictions are challenged. Shell model predictions agree well with the data.

AB - The root mean square radii of the proton density distribution in O16-24 derived from measurements of charge changing cross sections with a carbon target at ∼900A MeV together with the matter radii portray thick neutron skin for O22-24 despite O22,24 being doubly magic. Imprints of the shell closures at N=14 and 16 are reflected in local minima of their proton radii that provide evidence for the tensor interaction causing them. The radii agree with ab initio calculations employing the chiral NNLOsat interaction, though skin thickness predictions are challenged. Shell model predictions agree well with the data.

UR - https://www.scopus.com/pages/publications/85139855475

U2 - 10.1103/PhysRevLett.129.142502

DO - 10.1103/PhysRevLett.129.142502

M3 - 文章

C2 - 36240396

AN - SCOPUS:85139855475

SN - 0031-9007

VL - 129

JO - Physical Review Letters

JF - Physical Review Letters

IS - 14

M1 - 142502

ER -

Proton Distribution Radii of O 16-24: Signatures of New Shell Closures and Neutron Skin

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