Impact of spin-orbit currents on the electroweak skin of neutron-rich nuclei

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Date
2012
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American Physical Society
Abstract
Background: Measurements of neutron radii provide important constraints on the isovector sector of nuclear density functionals and offer vital guidance in areas as diverse as atomic parity violation, heavy-ion collisions, and neutron-star structure. Purpose: We assess the impact of spin-orbit currents on the electromagnetic- and weak-charge radii of a variety of nuclei. Special emphasis is placed on the experimentally accessible electroweak skin, defined as the difference between weak-charge and electromagnetic-charge radii. Methods: Two accurately calibrated relativistic mean-field models are used to compute proton, neutron, charge, and weak-charge radii of a variety of nuclei. Results: We find that spin-orbit contributions to the electroweak skin of light neutron-richnuclei, such as 22O and 48Ca, are significant and result in a substantial increase in the size of the electroweak skin relative to theneutron skin. Conclusions: Given that spin-orbit contributions to both the charge and weak-charge radii of nuclei are often as large as present or anticipated experimental error bars, future calculations must incorporate spin-orbit currents in the calculation ofelectroweak form factors.
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Horowitz, C. J., & Piekarewicz, J. (2012). Impact of spin-orbit currents on the electroweak skin of neutron-rich nuclei. Physical Review C - Nuclear Physics, 86(4), 045503. http://dx.doi.org/10.1103/PhysRevC.86.045503
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© 2012 American Physical Society.
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Article