Halo Nuclei

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Nucleus~1/1000 Atom Nucleon~1/10 Nucleus Nucleon=proton,neutron PAN, July 2005
Lifetimes of nuclei Stable Light nuclei: Z approx. equal to N (live virtually for ever) Adding many neutrons brings instability fineutron dripline Adding many protons brings instability fiproton dripline (very short lifetimes) PAN, July 2005
Page 1: Halo Nuclei F. M. Nunes PAN, July 2
Page 5 and 6: Binding energies of nuclei Stable L
Page 7 and 8: Halo nuclei: sizes Very large spati
Page 9 and 10: Halo nuclei: simplified spectra 3p+
Page 11 and 12: Structure (example for 8 B) Microsc
Page 13 and 14: Deuteron: the first halo nucleus D=
Page 15 and 16: Halo nuclei and Quantum Mechanics H
Page 17 and 18: Borromean Halo nuclei Some halo nuc
Page 19 and 20: Halo nuclei: what are the present i
Page 21 and 22: Halo nuclei: elastic scattering PAN
Page 29 and 30: Halo nuclei: breakup PAN, July 2005
Page 35 and 36: Halo nuclei: transfer PAN, July 200
Page 41 and 42: Halo nuclei: fusion PAN, July 2005
Page 43 and 44: Halo nuclei: fusion PAN, July 2005
Page 45 and 46: Halo nuclei: what are our tools? Re
Page 47 and 48: The end Questions? PAN, July 2005
Page 49: Dripline nuclei and Astrophysics PA

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