Gamow-Teller matrix elements of mirror nuclei in the relativistic scalar-vector shell model

doi:10.1016/0370-2693(90)91889-J

Physics Letters B

Volume 247, Issue 4, 20 September 1990, Pages 485-487

https://doi.org/10.1016/0370-2693(90)91889-J Get rights and content

Abstract

We calculated allowed β-decay Gamow-Teller matrix elements of A = 15, 17, 39, 41 mirror nuclei in the relativistic scalar-vector shell model. The relativistic corrections are shown to present the features of the mechanism needed to account for their incomplete non-relativistic description (missing quenching).

References (8)

I.S. Towner et al.
Nucl. Phys. A
(1983)
H.J. Strubbe et al.
Nucl. Phys. A
(1970)
B.B. Serot et al.
Adv. Nucl. Phys.
(1986)
L.S. Celenza et al.

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Cited by (2)

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Elastic, inelastic and quasielastic electron scattering probes the electromagnetic response of nuclei in a wide range of energy and momentum transfer. We review electromagnetic response functions evaluated in relativistic models of nuclear structure, based on baryon and meson degrees of freedom (quantum hadrodynamics). Results obtained within different models and approximations of quantum hadrodynamics are compared with data. We emphasize constraints of current conservation and selfconsistency. Random-phase correlations are important and have different impact in different kinematical regimes.

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Gamow-Teller matrix elements of mirror nuclei in the relativistic scalar-vector shell model

Abstract

Nucl. Phys. A

Nucl. Phys. A

Adv. Nucl. Phys.