Coulomb excitation of Sn104 and the strength of the Sn100 shell closure

Coulomb excitation of Sn104 and the strength of the Sn100 shell closure. Guastalla, G., Dijulio, D. D., Górska, M., Cederkäll, J., Boutachkov, P., Golubev, P., Pietri, S., Grawe, H., Nowacki, F., Sieja, K., Algora, A., Ameil, F., Arici, T., Atac, A., Bentley, M. A., Blazhev, A., Bloor, D., Brambilla, S., Braun, N., Camera, F., Dombrádi, Z. S., Domingo Pardo, C., Estrade, A., Farinon, F., Gerl, J., Goel, N., Grèbosz, J., Habermann, T., Hoischen, R., Jansson, K., Jolie, J., Jungclaus, A., Kojouharov, I., Knoebel, R., Kumar, R., Kurcewicz, J., Kurz, N., Lalović, N., Merchan, E., Moschner, K., Naqvi, F., Nara Singh, B. S., Nyberg, J., Nociforo, C., Obertelli, A., Pfützner, M., Pietralla, N., Podolyák, Z., Prochazka, A., Ralet, D., Reiter, P., Rudolph, D., Schaffner, H., Schirru, F., Scruton, L., Sohler, D., Swaleh, T., Taprogge, J., Vajta, Z., Wadsworth, R., Warr, N., Weick, H., Wendt, A., Wieland, O., Winfield, J. S., & Wollersheim, H. J. Physical Review Letters, 110(17):172501, apr, 2013.

Paper doi abstract bibtex

A measurement of the reduced transition probability for the excitation of the ground state to the first 2+ state in Sn104 has been performed using relativistic Coulomb excitation at GSI. Sn104 is the lightest isotope in the Sn chain for which this quantity has been measured. The result is a key point in the discussion of the evolution of nuclear structure in the proximity of the doubly magic nucleus Sn100. The value B(E2;0+→2 +)=0.10(4) e2b2 is significantly lower than earlier results for Sn106 and heavier isotopes. The result is well reproduced by shell model predictions and therefore indicates a robust N=Z=50 shell closure. \textcopyright 2013 American Physical Society.

@article{guastalla_coulomb_2013,
abstract = {A measurement of the reduced transition probability for the excitation of the ground state to the first 2+ state in Sn104 has been performed using relativistic Coulomb excitation at GSI. Sn104 is the lightest isotope in the Sn chain for which this quantity has been measured. The result is a key point in the discussion of the evolution of nuclear structure in the proximity of the doubly magic nucleus Sn100. The value B(E2;0+→2 +)=0.10(4) e2b2 is significantly lower than earlier results for Sn106 and heavier isotopes. The result is well reproduced by shell model predictions and therefore indicates a robust N=Z=50 shell closure. {\textcopyright} 2013 American Physical Society.},
annote = {From Duplicate 2 (Coulomb excitation of Sn104 and the strength of the Sn100 shell closure - Guastalla, G.; Dijulio, D. D.; G{\'{o}}rska, M.; Cederk{\"{a}}ll, J.; Boutachkov, P.; Golubev, P.; Pietri, S.; Grawe, H.; Nowacki, F.; Sieja, K.; Algora, A.; Ameil, F.; Arici, T.; Atac, A.; Bentley, M. A.; Blazhev, A.; Bloor, D.; Brambilla, S.; Braun, N.; Camera, F.; Dombr{\'{a}}di, Z. S.; Domingo Pardo, C.; Estrade, A.; Farinon, F.; Gerl, J.; Goel, N.; Gr{\`{e}}bosz, J.; Habermann, T.; Hoischen, R.; Jansson, K.; Jolie, J.; Jungclaus, A.; Kojouharov, I.; Knoebel, R.; Kumar, R.; Kurcewicz, J.; Kurz, N.; Lalovi{\'{c}}, N.; Merchan, E.; Moschner, K.; Naqvi, F.; Nara Singh, B. S.; Nyberg, J.; Nociforo, C.; Obertelli, A.; Pf{\"{u}}tzner, M.; Pietralla, N.; Podoly{\'{a}}k, Z.; Prochazka, A.; Ralet, D.; Reiter, P.; Rudolph, D.; Schaffner, H.; Schirru, F.; Scruton, L.; Sohler, D.; Swaleh, T.; Taprogge, J.; Vajta, Zs; Wadsworth, R.; Warr, N.; Weick, H.; Wendt, A.; Wieland, O.; Winfield, J. S.; Wollersheim, H. J.)

Publisher: American Physical Society},
author = {Guastalla, G. and Dijulio, D. D. and G{\'{o}}rska, M. and Cederk{\"{a}}ll, J. and Boutachkov, P. and Golubev, P. and Pietri, S. and Grawe, H. and Nowacki, F. and Sieja, K. and Algora, A. and Ameil, F. and Arici, T. and Atac, A. and Bentley, M. A. and Blazhev, A. and Bloor, D. and Brambilla, S. and Braun, N. and Camera, F. and Dombr{\'{a}}di, Z. S. and {Domingo Pardo}, C. and Estrade, A. and Farinon, F. and Gerl, J. and Goel, N. and Gr{\`{e}}bosz, J. and Habermann, T. and Hoischen, R. and Jansson, K. and Jolie, J. and Jungclaus, A. and Kojouharov, I. and Knoebel, R. and Kumar, R. and Kurcewicz, J. and Kurz, N. and Lalovi{\'{c}}, N. and Merchan, E. and Moschner, K. and Naqvi, F. and {Nara Singh}, B. S. and Nyberg, J. and Nociforo, C. and Obertelli, A. and Pf{\"{u}}tzner, M. and Pietralla, N. and Podoly{\'{a}}k, Z. and Prochazka, A. and Ralet, D. and Reiter, P. and Rudolph, D. and Schaffner, H. and Schirru, F. and Scruton, L. and Sohler, D. and Swaleh, T. and Taprogge, J. and Vajta, Zs and Wadsworth, R. and Warr, N. and Weick, H. and Wendt, A. and Wieland, O. and Winfield, J. S. and Wollersheim, H. J.},
doi = {10.1103/PhysRevLett.110.172501},
issn = {00319007},
journal = {Physical Review Letters},
month = {apr},
number = {17},
pages = {172501},
title = {{Coulomb excitation of Sn104 and the strength of the Sn100 shell closure}},
url = {http://link.aps.org/doi/10.1103/PhysRevLett.110.172501},
volume = {110},
year = {2013}
}

Downloads: 0