Halo Nuclei
Halo Nuclei
Halo Nuclei
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Binding energies of nuclei<br />
Stable Light nuclei: need a lot of energy to break it<br />
(example 4 He=2p+2n E=20 MeV)<br />
neutron dripline: 11 Li E=0.3 MeV<br />
proton dripline: 8 B E=0.1 MeV<br />
Binding energies ~ 100 times smaller<br />
PAN, July 2005<br />
(1 MeV=1.000.000 eV=1.6x10 -13 J)
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