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5–7 Dec 2018
CERN
Europe/Zurich timezone

STRUCTURE OF β-DECAY STRENGTH FUNCTION Sβ(E), WIGNER SPIN-ISOSPIN SU(4) SYMMETRY, AND SU(4) REGION

5 Dec 2018, 17:30
2h
61/1-201 - Pas perdus - Not a meeting room - (CERN)

61/1-201 - Pas perdus - Not a meeting room -

CERN

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Speaker

Igor Izosimov (Joint Institute for Nuclear Research)

Description

The strength function $ S_{\beta}(E) $ governs [1,2] the nuclear energy distribution of elementary charge-exchange excitations and their combinations like proton particle $({\pi}p)$-neutron hole $({\nu}h)$ coupled into a spin-parity $I^{\pi}$ : $[{\pi}p \otimes {\nu}h]I^{\pi}$ and neutron particle $({\nu}p)$-proton hole $({\pi}h)$ coupled into a spin-parity $I^{\pi} : [{\nu}p \otimes {\pi}h]I^{\pi}$. The strength function of Fermi-type $\beta$-transitions takes into account excitations $[{\pi}p \otimes {\nu}h]0^{+}$ or $[{\nu}p \otimes {\pi}h]0^{+}$. Since isospin is a quite good quantum number, the strength of the Fermi-type transitions is concentrated in the region of the isobar-analogue resonance ($IAR$). The strength function for $\beta$-transitions of the Gamow–Teller ($GT$) type describes excitations $[{\pi}p \otimes {\nu}h]1^{+}$ or $[{\nu}p \otimes {\pi}h]1^{+}$. Residual interaction can cause collectivization of these configurations and occurrence of resonances in $ S_{\beta}(E)$. In heavy and middle nuclei, because of repulsive character of the spin-isospin residual interaction [1,2], the energy of $GT$ resonance is larger than the energy of $IAR (E_{GT} > E_{IAR})$. One of the consequence of the Wigner spin-isospin $SU(4)$ symmetry is $E_{GT} = E_{IAR}$. $SU(4)$ symmetry-restoration effect induced by the residual interaction, which displaces the $GT$ towards the $IAR$ with increasing $(N-Z)/A$. In $^{6}Li$ nucleus (g.s. is the tango halo [3] state, IAR is the Borromean halo resonance) for low energy $GT$ phonon (reduced $GT$ strength $B(GT) \approx {5g_{A}}^{2}/4{\pi} (\Sigma($Ikeda sum rule$ ) = {6g_{A}}^{2}/4{\pi}$ we have $E_{GT} < E_{IAR}, E_{GT}-E_{IAR} = -3562.88 keV$, and $(N-Z)/A=0.33$ for $^{6}He$ ($^{6}He$ g.s. is the parent, Borromean halo state). Such situation may be connected with contribution of the attractive [4] component of residual interaction in this nucleus. It will be very interesting to find a region of atomic nuclei, where the $E_{} \approx E_{IAR}$ and spin-isospin $SU(4)$ symmetry determine the nuclear properties ($SU(4)$ region). Difference of the $E_{GT} - E_{IAR}$ energies as a function of the neutron [1,2] excess was analyzed. Datum for $^{6}He$ $\beta^{-}$ - decay was added to the data analyzed in [1,2].
Estimations shows that the value $Z/N \approx 0.6$ corresponds to the $SU(4)$ region. Different manifestations of the $SU(4)$ symmetry and possible experiments are discussed.

  1. Yu.V. Naumov, A.A. Bykov, I.N. Izosimov, Sov.J.Part.Nucl.14 (1983) 167.
  2. I.N. Izosimov, Physics of Particles and Nuclei 30 (1999) 131.
  3. I.N. Izosimov, JINR Preprint E6-2017-79, Dubna, 2017.
  4. Y. Fujita, et al., Phys. Rev. C 91 (2015) 064316, and references therein.

Primary author

Igor Izosimov (Joint Institute for Nuclear Research)

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