NUSTAR, Super-FRS, Fixed Target Physics and In-ring Experiments

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Lifetime measurements with radioisotopesa147Sm 143 Nd, T 1/2 :1.06 x 10 11 y144Nd a decay, T 1/2 :2.29 x 10 15 y Moon surface is ~ 5 x 10 9 y oldAppollo 15: “genesis rock”… so the sun should beas old (at least) !H. Simon ● Crossing bounds: From exotic nucl. sys. toFAIRH. Simon ● Crossing bounds: From exotic nucl. sys. to 10/90
abundanceConsequences:Stars use nuclear energy (fusion) seed production up ~ A=56 „slow‟ processsolar abundancesAnd how are heavierelements (A ≥ 56 )produced ?H,He96-99%iron peakstructuresbroad & narrowLi,Be,Bsuppressed2.24g Aumass number AH. Simon ● Crossing bounds: From exotic nucl. sys. to FAIR 11/90
Page 1 and 2: Crossing bounds: From exoticnuclear
Page 3 and 4: Menu1. NUSTAR: Nuclear Structure As
Page 6: Magnitude/Distance analysis (Invers
Page 9: Spectral analysis (blackbody radiat
Page 13 and 14: Tomography of the sun via neutrinos
Page 15 and 16: Possible way out …Coulomb dissoci
Page 17 and 18: To be explained …Radioactive Beam
Page 19 and 20: Physics with radioactive beamsNucle
Page 21 and 22: Exotica: HaloesH. Simon ● Crossin
Page 23 and 24: Cross section reflects size (Taniha
Page 25 and 26: PRL 104 (2010) 06270119,20,22C @ 40
Page 27 and 28: Bridging the A=5,8 gaps for heavy e
Page 29 and 30: Elastic proton scattering- inverse
Page 31 and 32: Experimental Setup (less schematic)
Page 33 and 34: Exploring Unbound Lithium isotopes1
Page 35 and 36: Intensities for detailed studiespri
Page 37 and 38: Results and current limits …14Be
Page 39 and 40: Quasi-free scattering in inverse ki
Page 41 and 42: Experimental Setup (less schematic)
Page 43 and 44: The origin of elementsDsRgSunBig ba
Page 45 and 46: Nucleosynthesis in the r-process (r
Page 47 and 48: Studies of neutron-rich nuclei in t
Page 49 and 50: Dipole-strength distributions in ne
Page 51 and 52: Additional Information from g spect
Page 53 and 54: Preparing for FAIR ~2017/18Intensit
Page 55 and 56: RIBs produced by fragmentation or f
Page 57 and 58: Comparison of FRS with Super-FRS, i
Page 59 and 60: Production of radioactive beamsby f
Page 61 and 62:
Br-DE-TOF method: RequirementsNO CH
Page 63 and 64:
FRS & RISING Super-FRS HISPEC/DESPE
Page 65 and 66:
New Shell Structure: Cr isotopes•
Page 67 and 68:
NUSTAR Experiments(NUclear STructur
Page 69 and 70:
Mass: Fundamental Property of Nucle
Page 71 and 72:
ILIMA: Set-UpIsochronous Mass Spect
Page 73 and 74:
Schottky Pick-Up in the ESRH. Simon
Page 75 and 76:
Time-of-Flight detector for the IMS
Page 77 and 78:
Page 79 and 80:
Reactions with Relativistic Radioac
Page 81 and 82:
CALIFA CsI/phoswitch calorimeterGen
Page 83 and 84:
Neutron detector NeuLANDs t < 100 p
Page 85 and 86:
Page 87 and 88:
Realization of an RIB electron coll
Page 89 and 90:
Summary: there is no smoking gun
Page 91 and 92:
Final Remarks• FAIR offers unique
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NUSTAR, Super-FRS, Fixed Target Physics and In-ring Experiments

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