Influence of Nuclear Structure on Sub-Barrier Hindrance in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="normal">N</mml:mi><mml:mi mathvariant="normal">i</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">N</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:math>Fusion
C. L. JiangPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAK. E. RehmPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAR. V. F. JanssensPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAH. EsbensenPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAI. AhmadPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAB. B. BackPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAP. CollonUniversity of Notre Dame, Notre Dame, Indiana 46556, USAC. N. DavidsPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAJ. P. GreenePhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USADeborah J. HendersonPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAG. MukherjeePhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAR. C. PardoPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAM. PaulHebrew University, Jerusalem 90914, IsraelT. PenningtonPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAD. SeweryniakPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAS. SinhaPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USAZ. ZhouPhysics Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
2004lv
ABI
Аннотация
Fusion-evaporation cross sections for $^{64}\mathrm{N}\mathrm{i}+^{64}\mathrm{N}\mathrm{i}$ have been measured down to the 10 nb level. For fusion between two open-shell nuclei, this is the first observation of a maximum in the $S$-factor, which signals a strong sub-barrier hindrance. A comparison with the $^{58}\mathrm{N}\mathrm{i}+^{58}\mathrm{N}\mathrm{i}$, $^{58}\mathrm{N}\mathrm{i}+^{60}\mathrm{N}\mathrm{i}$, and $^{58}\mathrm{N}\mathrm{i}+^{64}\mathrm{N}\mathrm{i}$ systems indicates a strong dependence of the energy where the hindrance occurs on the stiffness of the interacting nuclei.
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