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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},
}