Author/Authors :
B. Sun، نويسنده , , R. Kn?bel، نويسنده , , Yu.A. Litvinov، نويسنده , , H. Geissel، نويسنده , , J. Meng، نويسنده , , K. Beckert، نويسنده , , F. Bosch، نويسنده , , D. Boutin، نويسنده , , C. Brandau، نويسنده , , L. Chen، نويسنده , , I.J. Cullen، نويسنده , , C. Dimopoulou، نويسنده , , B. Fabian، نويسنده , , M. Hausmann، نويسنده , , C. Kozhuharov، نويسنده , , S.A. Litvinov، نويسنده , , Michèle M. M. Mazzocco، نويسنده , , F. Montes، نويسنده , , S. Hofmann and G. Münzenberg، نويسنده , , A. Musumarra، نويسنده , , et al.، نويسنده ,
Abstract :
The previously pioneered Isochronous Mass Spectrometry (IMS) has been extended by an additional precise magnetic-rigidity determination to enable accurate large-scale measurements of stored short-lived relativistic nuclei with the FRS-ESR facility at 382 MeV/u. With this novel experimental tool the mass resolving power and accuracy have been improved by a factor of about 3. The recorded broad-band revolution time spectrum corresponds to the mass-over-charge range of about 6%. A mass resolving power of 200 000 (FWHM) and a typical accuracy of 120 keV have been achieved almost over the entire spectrum. The masses of 35 neutron-rich nuclides have been directly measured in the element range from aluminum to barium. The Masses of 8 nuclides (85,86As, 89Se, 123Ag, 138Te, 140,141I, 143Xe) have been measured for the first time. The results are compared with previous experimental data and theoretical predictions. The evolution of the N=50 shell closure towards doubly-magic 78Ni is discussed.
Keywords :
Comparison with other data , various nuclear mass models , Atomic masses , 31–56 , A=33 , 79–146 , Z=13 , Measured , masses using isochronous mass spectrometry technique , deduced , two-neutron separation , neutron shell gap energies