At the limit of stability, atomic nuclei can exhibit unique structure due to the proximity to the particle- decay threshold. In particular, if orbitals near the Fermi surface have low angular momenta, they can induce spatially extended wave functions for valence neutrons, forming nuclear halo. In light p and psd shells, halo nuclei have so far served as a benchmark for understanding of...
Astro-ν interactions are studied by inverse β decays and ν-properties beynod the standard model are studied by neutrinoless double beta decays (0νββ). The β and ββ nuclear matrix elements (NMES) consist mainly of the axial-vector spin (σ) isospin(τ) components, The delta-isobar (Δ) resonance excited by the quark τσ...