FRIB WorkshopNov 2008 FRIB WorkshopNov 2008 FRIB WorkshopNov
FRIB Workshop/Nov. 2008
FRIB Workshop/Nov. 2008
FRIB Workshop/Nov. 2008
FRIB Workshop/Nov. 2008
FRIB Workshop/Nov. 2008
112 Sn FRIB Workshop/Nov. 2008
FRIB Workshop/Nov. 2008
From EGMR and EISGDR to K∞ However, the available GMR data can lead to a wide range of values for K∞ (100 --500 Me. V!) So, "microscopic approach": l. Select "suitable" effective interactions. l. Calculate the GMR strength distributions in an RPA approach l. Compare with the experimental EGMR and EISGDR K∞ FRIB Workshop/Nov. 2008
This number is consistent with both GMR and ISGDR Data and with non-relativistic and relativistic calculations FRIB Workshop/Nov. 2008
FRIB Workshop/Nov. 2008
Excitation energy spectra at 0 deg FRIB Workshop/Nov. 2008
FRIB Workshop/Nov. 2008
FRIB Workshop/Nov. 2008
FRIB Workshop/Nov. 2008
Why are tins so “Fluffy”? FRIB Workshop/Nov. 2008
FRIB Workshop/Nov. 2008
FRIB Workshop/Nov. 2008
FRIB Workshop/Nov. 2008
Kt = -500 (50) FRIB Workshop/Nov. 2008
Data from H. Sagawa et al. , Phys. Rev. C 76, 034327 (2007) FRIB Workshop/Nov. 2008
G. Colo’s talk on Saturday FRIB Workshop/Nov. 2008
G. Colo’s talk on Saturday FRIB Workshop/Nov. 2008
Towards very neutron-rich nuclei v Kt v Kcore and Kskin “soft GMR” akin to pigmy GDR’s. v Need inverse reactions 2 H, 4 He, or 6 Li targets beams of 35 -100 Me. V/A v. First experiment performed at GANIL 56 Ni + 2 H, with active target MAYA FRIB Workshop/Nov. 2008
Ionization chamber Drift Au foil chamber Si wall Moving flap Cs. I wall Diamond MAYA @ GANIL MAYA FRIB Workshop/Nov. 2008
# counts/Me. V 58 Ni (d, d’) d break-up MAYA @ GANIL C. Monrozeau et al. , Phys. Rev. Lett. 100, 042501 (2008) FRIB Workshop/Nov. 2008
Analysis with Gaussian fits FRIB Workshop/Nov. 2008
Multipole Decomposition Analysis FRIB Workshop/Nov. 2008
FRIB Workshop/Nov. 2008
FRIB Workshop/Nov. 2008
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