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@ARTICLE{Kaur:247108,
author = {Kaur, S. and Kanungo, R. and Horiuchi, W. and Hagen, G. and
Holt, J. D. and Hu, B. S. and Miyagi, T. and Suzuki, T. and
Ameil, F. and Atkinson, J. and Ayyad, Y. and Bagchi, S. and
Cortina-Gil, D. and Dillmann, I. and Estrade, Alfredo and
Evdokimov, Alexei and Farinon, Fabio and Geissel, Hans and
Guastalla, Giulia and Janik, R. and Knöbel, R. and
Kurcewicz, Jan and Litvinov, Yu. A. and Marta, Michele and
Mostazo, M. and Mukha, I. and Nociforo, C. and Ong, H. J.
and Otsuka, T. and Pietri, S. and Prochazka, Andrej and
Scheidenberger, C. and Sitar, B. and Strmen, P. and Takechi,
M. and Tanaka, J. and Tanihata, I. and Terashima, S. and
Vargas, J. and Weick, H. and Winfield, J. S.},
title = {{P}roton {D}istribution {R}adii of $^{16–24}{O}$ :
{S}ignatures of {N}ew {S}hell {C}losures and {N}eutron
{S}kin},
journal = {Physical review letters},
volume = {129},
number = {14},
issn = {0031-9007},
address = {College Park, Md.},
publisher = {APS},
reportid = {GSI-2022-00834, arXiv:2209.00722},
pages = {142502},
year = {2022},
note = {6 pages, 3 figures, accepted for publication in Physical
Review Letters},
abstract = {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.},
cin = {FRS / ATP / EXM / ACO / DTL / SuperFRS@FAIR /
SuperFRS-EC@FAIR},
ddc = {530},
cid = {I:(DE-Ds200)FRS-20110310OR124 /
I:(DE-Ds200)ATP-20051214OR020 /
I:(DE-Ds200)EXM-20080818OR100 /
I:(DE-Ds200)ACO-20051214OR053 /
I:(DE-Ds200)DTL-20051214OR031 /
I:(DE-Ds200)Coll-FAIR-SuperFRS /
I:(DE-Ds200)Coll-FAIR-SuperFRS-EC},
pnm = {612 - Cosmic Matter in the Laboratory (POF4-612) / 631 -
Matter – Dynamics, Mechanisms and Control (POF4-631) / PSP
1.2.10 Super-FRS Experiment Collaboration (Super-FRS EC)
(PSP-1-2-10)},
pid = {G:(DE-HGF)POF4-612 / G:(DE-HGF)POF4-631 /
G:(DE-Ds200)PSP-1-2-10},
experiment = {EXP:(DE-Ds200)S395-20200803},
typ = {PUB:(DE-HGF)16},
eprint = {2209.00722},
howpublished = {arXiv:2209.00722},
archivePrefix = {arXiv},
SLACcitation = {$\%\%CITATION$ = $arXiv:2209.00722;\%\%$},
pubmed = {pmid:36240396},
UT = {WOS:000878188000010},
doi = {10.1103/PhysRevLett.129.142502},
url = {https://repository.gsi.de/record/247108},
}