Pregled bibliografske jedinice broj: 449007
Pygmy Dipole Strength in Exotic Nuclei and the Equation of State
Pygmy Dipole Strength in Exotic Nuclei and the Equation of State // American Institute of Physics Conference Proceedings 1165 / Matko Milin, Tamara Niksic, Suzana Szilner, Dario Vretenar (ur.).
Dubrovnik, Hrvatska: American Institute of Physics (AIP), 2009. str. 181-184 (predavanje, međunarodna recenzija, cjeloviti rad (in extenso), znanstveni)
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Naslov
Pygmy Dipole Strength in Exotic Nuclei and the Equation of State
Autori
Klimkiewicz, A ; Paar, Nils ; Adrich, P ; Fallot, M ; Bleis, T ; Rossi, D ; Boretzky, K ; Aumann, T ; Alvarez-Pol, H ; Aksouh, F ; Benlliure, J ; Berg, T ; Boehmer, M ; Casarejos, E ; Chartier, M ; Chatillon, A ; Cortina-Gil, D ; Datta Pramanik, U ; Elze, Th. W ; Emling, H ; Ershova, O ; Fernando-Dominguez, B ; Geissel, H ; Gorska, M ; Heil, C ; Hellström, M ; Johansson, H ; Jones, K. L. ; Junghans, A ; Kiselev, O ; Kratz, J. V. ; Kulessa, R ; Kurz, N ; Labiche, M ; Lemmon, R. ; Litvinov, Y ; Mahata, K ; Maierbeck, P ; Nilsson, T ; Nociforo, C ; Palit, R ; Paschalis, S ; Plag, R ; Reifarth, R ; Simon, H ; Sümmerer, K ; Surówka, G ; Vretenar, Dario ; Wagner, A ; Waluś, I. W. ; Weick, H. ; Winkler M
Vrsta, podvrsta i kategorija rada
Radovi u zbornicima skupova, cjeloviti rad (in extenso), znanstveni
Izvornik
American Institute of Physics Conference Proceedings 1165
/ Matko Milin, Tamara Niksic, Suzana Szilner, Dario Vretenar - : American Institute of Physics (AIP), 2009, 181-184
ISBN
978-0-7354-0702-2
Skup
NUCLEAR STRUCTURE AND DYNAMICS '09
Mjesto i datum
Dubrovnik, Hrvatska, 04.05.2009. - 08.05.2009
Vrsta sudjelovanja
Predavanje
Vrsta recenzije
Međunarodna recenzija
Ključne riječi
symmetry energy; ion beams; coulomb excitation; neutron skin
Sažetak
A concentration of dipole strength at energies below the giant dipole resonance was observed in neutron-rich nuclei around 132Sn in an experiment using the FRS-LAND setup. This so- called “pygmy” dipole strength can be related to the parameters of the symmetry energy and to the neutron skin thickness on the grounds of a relativistic quasiparticle random-phase approximation. Using this ansatz and the experimental findings for 130Sn and 132Sn, we derive a value of the symmetry energy pressure of 0 = 2.2±0.5 MeV/fm3. Neutron skin thicknesses of Rn−Rp = 0.23±0.03 fm and 0.24±0.03 fm for 130Sn and 132Sn, respectively, have been determined. Preliminary results on 68Ni from a similar experiment using an improved setup indicate an enhanced cross section at low energies, while the results for 58Ni are in accordance with results from photoabsorption measurements.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Projekti:
UKF 17/08
119-1191005-1010 - Nuklearna struktura i nuklearna astrofizika (Vretenar, Dario, MZOS ) ( CroRIS)
Ustanove:
Prirodoslovno-matematički fakultet, Zagreb