Physics opportunities with heavy-ion detectors in the CR

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Physics opportunities with heavy-ion detectors in the CR Subproject leader: Iris Dillmann (JLU Giessen/ GSI Darmstadt)

Decay detectors for CR  Go for pocket detectors, not vacuum detectors Position sensitive and particle identification detectors Multi-purpose detector, based on TUM Si stack German BMBF proposal pending (for 3 years): - JLU Giessen: 1 PhD + 48 k€ (Si-PIN diodes) + 50 k€ pocket - TU München: 1 PhD + 50 k€ (DSSDs) (Polycrystalline) Diamond detectors? Fast timing (≈ps); radiation hardness/ high count rate Collaboration with AP, SuperFRS (det), and TU München (Proposal to Helmholtz association in prep., ~100 k€ invest)

TUM Si stack detector Si-PIN diodes, build by Ludwig Maier, PhD TU München (2007) Active area: 20x20 mm2 Setup: x- and y-strip detectors, 14 Si-PIN diodes Used in bound-state b-decay measurements of 207Tl (PRL 95, 052501 (2005)) 20 mm

ESR detector vs. CR prototype detector Pockets: window 120x44 mm2 ESR: U up to 500 MeV/u (pocket depth 37 mm) CR: up to 740 MeV/u: pocket depth needs to be adapted (stopping range 132Sn: 57 mm; 72Ni: 101 mm) or prior use of degrader (disadvantage: ion losses, DE identification needs to be measured before) Active area: ESR: Si PIN diodes: 20x20 mm2 CR: Si PIN diodes 120x40 mm2 factor 12 larger

Position in ESR Inner position (C) needed for b- -decay Outer position (B) for EC/ b+ decay Too high EC/recombination rates at (D), (E); no inner position Stepping motor Photos: O. Klepper and A. Zschau

Positions in CR68 magnet stoch. cooling pick-up/kicker Schottky Circumference = 221.45 m, Brmax=13 Tm pocket magnet stoch. cooling pick-up/kicker inj./extr. kicker RF cavity detectors / beam diagnostics pocket valves A. Dolinskii

(Possible) Physics cases Parallel operation of Schottky pickups and decay detectors: Open ESR proposals: E073: Electron screening and a-decay (…withdrawn) E100: Bound-state b-decay of 205Tl (…waiting since >18 years) New and old ideas: (Partial) Half-lives of mixed EC/b-decay isotopes (fully stripped, H/He-like) b-delayed neutron (proton?) emitters Measurement of a-decay products

Physics cases  "Stellar lifetimes of SN isotopes" (Wed, 17:45) Sorry for the house advertising… Mixed decay isotopes Pure EC decay isotopes CR clocks Secondary CR spallation products SN isotopes Primary SN isotopes

Mixed EC/b-decay isotopes Stellar conditions: EC hindered, weak b+/b- decay channel determines t1/2 107 pps injected, 30min measured  ~1 event/d if partial t1/2= 25000 y b- ~10-5% b+~10-7% EC 835 keV 2+ 0+ 3+ b+~10-5% EC 1720 keV 970 keV 158 keV 1+ 2+ 3+ 4+ 1451 keV 0+ 

54Mn  CR chronometer if partial t1/2 of b- branch known EC 835 keV 2+ 0+ 3+ CR chronometer if partial t1/2 of b- branch known b+ branch measured Assuming same log ft for b- branch (factor 2-3 uncertainty) Direct: b-< 3.9*10-5  t1/2(b-)> 22000 y  Shell model prediction: t1/2(b-)~ 500 000 y Martinez-Pinedo et al., PRL 81, 281 (1998) Form factor for b- larger than for b+ decay  Quenching of GT necessary, not necessary for forbidden transitions

56Ni decay Most abundant isotope from SN explosions: early SN lightcurve Measure for acceleration time scale if t1/2> 10 My b+ EC 1720 keV 970 keV 158 keV 1+ 2+ 3+ 4+ 1451 keV 0+  Measurement (0.1 MBq source, 8*1010 at.): b+(158 keV) <6.3*10-5 %  t1/2(b+)> 27000 y Zaerpoor et al., PRC 59, 3393 (1999) Partial t1/2(b+) 2+: (0.6-3.3)*108 y 3+: (3.7-4.2)*104 y 4+: (2.6-5.0)*1012 y Quenching of GT, not for forbidden transition If quenched: t1/2(b+)= 73000 y  No CR chronometer Shell model predictions Lund Fisker et al., EPJA 5, 229 (1999)

Mixed EC/b-decay isotopes: s process s-process "branchings" Determines how much material is transferred to next isotope Interior of stars: high recombination rates but also high temperatures T≈30-1000 MK 43.9% EC/17.6% b+ 6.1% EC/ 2.2% b+ 6.9% EC 28 (4)% EC 72.1% EC 60 (5)% EC 86 (3)% EC 7.47% EC 2.92% EC

b-delayed neutron emission probability Sn Sn< Qb Important nuclear structure information Pn : b-strength above Sn t1/2(AZ+1): sensitive to low-lying b-strength Important for nuclear structure, astrophysics (r-process), and reactor physics 8He- 150La: ~200 datasets available, ~75 in non-fission region (A<70)

b-delayed neutron emitters Measuring Pn values without neutron detectors Complementary to standard methods Available methods (up to now): “n/b”: Neutron-beta coincidences “n-b”: Neutrons and betas counted separately (no coincidences) but simultaneously “g AZ+n”: Abundance of precursor determined via gamma-counting of any b-decay daughter “Pn AZ”: Normalization of the ratio eb/en with known Pn value from precursor AZ “g-g”: Number of neutron decays determined only via g-counting “ion”: Ion counting “fiss”: Fission yields

Advantages & Drawbacks + Independent on worldwide 3He shortage + Decay detector: cheaper than neutron detector array + Only few atoms/ injection needed + Independent on neutron energy (detection efficiency problem) - No cooling possible (isotopes too short-lived) - Low efficiency (could be increased by 2nd detector) - Produced ions have to be transferred from FRS into ESR (losses)

Possible cases: bn standards Possible standards selected by IAEA consultants' meeting (2011) 9Li: Pn= 50.8 (2) % 17N: Pn= 95.1 (7) % 87Br: Pn= 2.43 (14) % 88Br: Pn= 6.67 (17) % 94Rb: Pn= 10.19 (30) % 95Rb: Pn= 8.89 (33) % 137I: Pn= 7.33 (38) % Should be measured with independent methods and agree Standard for every mass region Missing: A>150 and A~60

Summary Multi-purpose decay detector for any decay product outside ESR (CR) acceptance (parallel oper. with Schottky's) Present collaboration: GSI (AP group, storage ring group), TU München, Edinburgh (consultative) Any more physics cases? ILIMA More partners needed !