Halo Nuclei

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<strong>Halo</strong> nuclei and density distributions | Y(r) 2 | density (fm -3 ) density (fm -3 ) 0.1 0.075 0.05 0.025 0 18 C core 19 C (a) (b) 10 -1 10 -3 halo neutron 10 -5 10 -7 0 5 10 15 20 radius (fm) Calculated particle density distributions (H. Lenske). PAN, July 2005
<strong>Halo</strong> nuclei and Quantum Mechanics Heisenberg’s uncertainty principle: dx dv > ћ/2m large spatial extension Æ narrow velocity distribution! Probability of finding the nucleon at r is | Y(r) 2 | . Probability of finding the nucleon with velocity v is | Y(v) 2 | . x p v PAN, July 2005
Page 1 and 2: Halo Nuclei F. M. Nunes PAN, July 2
Page 3 and 4: Lifetimes of nuclei Stable Light nu
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: Deuteron: the first halo nucleus D=
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

Halo Nuclei

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