Coulomb Displacement Energies Between Analog Levels for 3 ≤a≤ 239

Antony, M. S.; Pape, A.; Britz, J.

doi:10.1006/adnd.1997.0740

Cited by 70 publications

(35 citation statements)

References 3 publications

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“…(The entries selected from Ref. [9] have A 50, involve analog states of ground states, have measurement errors quoted and do not include mirror nucleus pairs.) The clean linear behaviour persists to A = 238, the best fit slope being 0.702(1) MeV, close to the mirror nucleus value, with an intercept of −0.453(15) MeV, again far from zero.…”

Section: Exchange Coulomb Termmentioning

confidence: 99%

Mutual influence of terms in a semi-empirical mass formula

Kirson

2008

Nuclear Physics A

115

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Section: Exchange Coulomb Termmentioning

confidence: 99%

Mutual influence of terms in a semi-empirical mass formula

Kirson

2008

Nuclear Physics A

115

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“…Many such states have been identified [69]. By fitting the available data on the IAS, Danielewicz and Lee obtained the constraint [42,61] shown as a parallelogram in Fig.…”

Section: Symmetry Energy Constraints From Isobaric Analog Statesmentioning

confidence: 99%

Constraints on the symmetry energy and neutron skins from experiments and theory

et al. 2012

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The symmetry energy contribution to the nuclear equation of state impacts various phenomena in nuclear astrophysics, nuclear structure, and nuclear reactions. Its determination is a key objective of contemporary nuclear physics, with consequences for the understanding of dense matter within neutron stars. We examine the results of laboratory experiments that have provided initial constraints on the nuclear symmetry energy and on its density dependence at and somewhat below normal nuclear matter density. Even though some of these constraints have been derived from properties of nuclei while others have been derived from the nuclear response to electroweak and hadronic probes, within experimental uncertainties-they are consistent with each other. We also examine the most frequently used theoretical models that predict the symmetry energy and its slope parameter. By comparing existing constraints on the symmetry pressure to theories, we demonstrate how contributions of three-body forces, which are essential ingredients in neutron matter models, can be determined.

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“…Numerous excitation energies of isobaric analog are known experimentally [9]. These energies are related to the ground state energies of neighboring isobaric nuclei.…”

Section: Energy Differences T T (A)mentioning

confidence: 99%

“…Here, the experimentally established excitation energies E 1 (T = 0) for the first excited T = 0 states compiled in Refs. [9,17] were added to the T = 1 ground-state mass values. Without this correction, the symmetry energy coefficients a(A) display anomalies.…”

Section: Symmetry and Pairing Energiesmentioning

confidence: 99%