The -decay of N 12 ECT Trento 3rd October 2001 Hans O. U. Fynbo Outline • Why study -decay of light nuclei • Detection System 12 • N - Preliminary • Outlook Why study -decay of Light Nuclei ? – “Exact” A-body calculations possible for A12. • Shell-model states • Molecular-cluster states – Break-up mechanism not fixed by kinematics • Test case for 2He emission models – Crucial for bridging the A=5 and A=8 gaps in Big Bang and Stellar nuclear synthesis. Some recent theoretical interest Experiments • States near 3-threshold surprisingly unknown • 10.3MeV mainly known from 12 12 •-decays of N and B •The spin-parity of the 10.3MeV state is unknown •Important to determine cluster structure Latest evaluation Nucl. Phys. A506 (1990) Experiments Schwalm and Povh Nucl. Phys. 89 (1966) 401 Eyrich et al. Phys. Rev. C36 (1987) 416 Lewis et al. Nucl. Phys. A474 (1987) 499 The -decay of 12N •Unpublished data from Heidelberg from 1978 (Schwalm) •Main experimental problems are • Energy loss in target •Summing •Not possible to determine spin of the 10.3MeV state. •Indications for new state at 13MeV 12 N Motivation II :Breakup of the 12.71MeV state Balamuth, Zurmuhle and Tabor Phys. Rev. C10 (1974) 975 R-matrix based sequential break-up with order-of-emission interference A.A. Korshenninikov Sov. J. Nucl. Phys. 52 (1990) 827 Hyperspherical Harmonics expansion. Simultaneous emission. SAME DATA !! 12 N Motivation II :Breakup of the 12.71MeV state Experiment – ISOL type beam • Mass-separated • Low energy • Reduce energy loss – IGISOL • Fast • Chemically blind Detection System – Essentials • LargeSolid Angle – detect all particles • High Segmentation – no summing – New Complications • Detection is kinematics dependent • Deadlayer in detector Monte-Carlo simulations 12 N Results – Required corrections • Energy Loss in C-foil • Energy Loss in detector deadlayer. • Include in calibrations – Corrections different for each strip • Takes time - but can be done ! • Allows for much better resolution. – Many Cuts possible • Total momentum • Veto -particles with E-E • Efront = Eback ... 12 N Results Title: n122d_ls.eps Creator: HIGZ Version 1.27/03 Prev iew : This EPS picture w as not s av ed w ith a preview inc luded in it. Comment: This EPS picture w ill print to a Pos tSc ript printer, but not to other ty pes of printers. 12 N Results : The 10.3MeV state – Break-up mechanism known • Can we determine the spin-parity? – Method • Select 8Be 0+ branches by gating on diagonal • Use Monte-Carlo to correct for detection efficiency • Fit – 0+ favoured – Preliminary • Need more X-checks. Title: spin_of_103.eps Creator: HIGZ Version 1.27/03 Preview : This EPS picture w as not saved w ith a preview included in it. Comment: This EPS picture w ill print to a PostScript printer, but not to other ty pes of printers . 12 N Results : The 10.3MeV state Title: 103.eps Creator: HIGZ Version 1.27/03 Prev iew : This EPS picture w as not s av ed w ith a preview inc luded in it. Comment: This EPS picture w ill print to a Pos tSc ript printer, but not to other ty pes of printers. 12 N Results : The 12.71MeV state – Break-up mechanism unknown • Sequential R-matrix? • Democratic? – Compared to Data • Democratic best, but both models fail for the highest two peaks • Surprising similarity between models – Still work to do ! – Any ideas ? Title: 127.eps Creator: HIGZ Version 1.27/03 Prev iew : This EPS picture w as not s av ed w ith a preview inc luded in it. Comment: This EPS picture w ill print to a Pos tSc ript printer, but not to other ty pes of printers. 12 Title: esumei.eps Creator: HIGZ Version 1.27/03 Prev iew : This EPS picture w as not s av ed w ith a preview inc luded in it. Comment: This EPS picture w ill print to a Pos tSc ript printer, but not to other ty pes of printers. N Results : Total Data Pending – Fully understand the detailed response and acceptance of the detector system • Detection thresholds • Energy cut-off due to C-foil – Is there a state near 13MeV ? • Rotational band structure built on 0+ • Likely to be 2+ – Understand the break-up of the 12.71MeV state • Theoretical input most welcome! • Interesting to compare to the 15.11MeV state Outlook : Detection thresholds – Record spectrum in air from standard triple source • Test Monte-Carlo • Determine threshold • Easy “calibration” 5 y = 0.0327x - 0.1455 R2 = 0.9961 4.5 Low Energy Cut-off (MeV) 4 3.5 3 300 64 2.5 Linear (300) Linear (64) 2 y = 0.0191x + 0.091 R2 = 0.9976 1.5 1 0.5 0 0 20 40 60 80 100 120 140 160 CFD Voltage (mV) Work of Damian King CERNISOLDE Summer Student 2001 Outlook II – 9 Li available from most ISOLDE targets • Determine neutron energy from E, P conservation – 9C should be re-measured with lower thresholds • Breakup mechanism of low lying states – 12 B can be produced indirectly via 12Be • Very high yield – Try to improve yield of 12N Outlook III – Several Detector Projects • G.Nyman + B.Jonson (Guthenburg) ball of hybrid E-E telescopes • O.Tengblad (Madrid) cube of DSSSDs • J.Aysto (ISOLDE) ball of single detectors using TOF and pulseshaping 5 cm •Beam-coolers and Paul-traps •Reduce effect of C-foil •Plans underway at GANIL-SPIRAL and ISOLDE-CERN 10 cm
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