Nuclear Astrophysics - Nuclear Physics

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Experimental quests & tools • Ground-state properties & spectroscopy masses, β-decay rates, spectra • Resonance properties elastic, inelastic scattering transfer reactions • Capture reactions resonant & direct capture Coulomb dissociation indirect methods (ANC, THM, etc.) www.cyc.ucl.ac.be/CARINA a mengoni for CARINA
Main goals of the CARINA (*) network ‣ To carry out mapping studies of the European situation in terms of projects, facilities and teams in order to identify the available instrumentation and human potential. ‣ To develop the research capabilities of existing Large Scale Facilities (LSF) and of smaller laboratories and enhance involvement in the future RIB facilities. ‣ To record the needs for new instrumentation and techniques; look for existing “solutions” in other fields. ‣ To coordinate research efforts by defining and proposing common research goals and by encouraging new collaborations and new R&D projects. (*) CARINA: Challenges and Advanced Research in <strong>Nuclear</strong> <strong>Astrophysics</strong> Date of beginning: 1 January 2005 Date of end: 31 December 2008 Budget: 35 k€ Co-ordinator: Carmen Angulo (CRC, Louvain-la-Neuve)
Page 1 and 2: Nuclear Astrophysics • energy gen
Page 3 and 4: Explosive burning - astrophysical s
Page 5 and 6: Novae nucleosynthesis 18 F(p,α) 15
Page 7 and 8: Nucleosynthesis Mixing (abundance d
Page 9 and 10: The r-process r path www.cyc.ucl.ac
Page 11 and 12: Endpoint of the r-processr r-proces
Page 13 and 14: Effects: during r-processr process:
Page 15: Summary: nuclear physics for the r-
Page 19 and 20: N-02 CARINA activities in 2006 •
Page 21 and 22: N-02 CARINA activities in 2006 •
Page 23 and 24: Instrumentation for nuclear astroph
Page 25 and 26: Some additional key reactions 14 O(
Page 27: The end
Page 30: Example: 3 He + 3 He → 4 He + 2p

Nuclear Astrophysics - Nuclear Physics

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