Author/Authors :
Morone، نويسنده , , M.C. and Oliviero، نويسنده , , G. and Campajola، نويسنده , , L. and D’Onofrio، نويسنده , , A. and Gialanella، نويسنده , , L. and Commara، نويسنده , , M.La and Roca، نويسنده , , Marيa V. and Romano، نويسنده , , M. and Romoli، نويسنده , , M. and Terrasi، نويسنده , , F. and Barna، نويسنده , , R. and Pasquale، نويسنده , , D.De and Aliotta، نويسنده , , M. and Cherubini، نويسنده , , S. and Lattuada، نويسنده , , M. and Romano، نويسنده , , S. and Spitaleri، نويسنده , , C.، نويسنده ,
Abstract :
In the framework of Coulomb dissociation experiments, performed to reconstruct the cross section of the inverse radiative capture process, the detection of breakup fragments is usually performed using separate detectors, which unavoidably are not sensitive to small relative angles. It is shown, by means of Monte Carlo simulations, that the phase-space constraints imposed by the detection geometry can bias, specially at very low relative energies, the extracted cross section, which turns out to be strongly dependent upon the assumed angular distribution of fragments in the intrinsic reference frame. A solution to the problem of the model-dependence of the response function is proposed, making use of a single three-stage detector for the identification and the relative energy measurement of the breakup fragments. A test measurement on the reaction 208Pb(16O, 12C-α)208Pb at 126 MeV incident energy has been performed, using a gas–Si–CsI tritelescope. The results indicate the feasibility of measuring very low relative energies in the Coulomb dissociation approach to the solution of important problems in nuclear astrophysics via the accurate determination of reaction rates at energies far below the Coulomb barrier.