Proton distribution radii of $^{16-24}$O: signatures of new shell closures and neutron skin

التفاصيل البيبلوغرافية
العنوان: Proton distribution radii of $^{16-24}$O: signatures of new shell closures and neutron skin
المؤلفون: 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., Janik, R., Knöbel, R., Kurcewicz, J., Litvinov, Yu. A., Marta, M., Mostazo, M., Mukha, I., Nociforo, C., Ong, H. J., 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, J. S.
المصدر: Phys. Rev. Lett. 129, 142502 (2022)
سنة النشر: 2022
المجموعة: Nuclear Experiment
Nuclear Theory
مصطلحات موضوعية: Nuclear Experiment, Nuclear Theory
الوصف: The root mean square radii of the proton density distribution in $^{16-24}$O derived from measurements of charge changing cross sections with a carbon target at $\sim$900$A$ MeV together with the matter radii portray thick neutron skin for $^{22 - 24}$O despite $^{22,24}$O 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 it ab initio calculations employing the chiral NNLO$_{\mathrm{sat}}$ interaction, though skin thickness predictions are challenged. Shell model predictions agree well with the data.
Comment: 6 pages, 3 figures, accepted for publication in Physical Review Letters
نوع الوثيقة: Working Paper
DOI: 10.1103/PhysRevLett.129.142502
URL الوصول: http://arxiv.org/abs/2209.00722
رقم الأكسشن: edsarx.2209.00722
قاعدة البيانات: arXiv
الوصف
DOI:10.1103/PhysRevLett.129.142502