Searching for isovector signatures in the neutron-rich oxygen and calcium isotopes

We search for potential isovector signatures in the neutron-rich oxygen and calcium isotopes within the framework of a relativistic mean-field theory with an exact treatment of pairing correlations. To probe the isovector sector we calibrate a few relativistic density functionals using the same isos...

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Main Authors: Wei-Chia Chen, J. Piekarewicz
Format: Article
Language:English
Published: Elsevier 2015-09-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269315005304
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author Wei-Chia Chen
J. Piekarewicz
author_facet Wei-Chia Chen
J. Piekarewicz
author_sort Wei-Chia Chen
collection DOAJ
description We search for potential isovector signatures in the neutron-rich oxygen and calcium isotopes within the framework of a relativistic mean-field theory with an exact treatment of pairing correlations. To probe the isovector sector we calibrate a few relativistic density functionals using the same isoscalar constraints but with one differing isovector assumption. It is found that under certain conditions, the isotopic chain in oxygen can be made to terminate at the experimentally observed 24O isotope and in the case of the calcium isotopes at 60Ca. To produce such behavior, the resulting symmetry energy must be soft, with predicted values for the symmetry energy and its slope at saturation density being J=(30.92±0.47) MeV and L=(51.0±1.5) MeV, respectively. As a consequence, the neutron-skin thickness of 208Pb is rather small: Rskin208=(0.161±0.011) fm. This same model—labeled “FSUGarnet”—predicts R1.4=(13.0±0.1) km for the radius of a “canonical” 1.4M⊙ neutron star, yet is also able to support a two-solar-mass neutron star.
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spelling doaj.art-3aa307ffaba141eb9d1af4b6bb2b68d92022-12-22T03:14:40ZengElsevierPhysics Letters B0370-26931873-24452015-09-01748C28428810.1016/j.physletb.2015.07.020Searching for isovector signatures in the neutron-rich oxygen and calcium isotopesWei-Chia ChenJ. PiekarewiczWe search for potential isovector signatures in the neutron-rich oxygen and calcium isotopes within the framework of a relativistic mean-field theory with an exact treatment of pairing correlations. To probe the isovector sector we calibrate a few relativistic density functionals using the same isoscalar constraints but with one differing isovector assumption. It is found that under certain conditions, the isotopic chain in oxygen can be made to terminate at the experimentally observed 24O isotope and in the case of the calcium isotopes at 60Ca. To produce such behavior, the resulting symmetry energy must be soft, with predicted values for the symmetry energy and its slope at saturation density being J=(30.92±0.47) MeV and L=(51.0±1.5) MeV, respectively. As a consequence, the neutron-skin thickness of 208Pb is rather small: Rskin208=(0.161±0.011) fm. This same model—labeled “FSUGarnet”—predicts R1.4=(13.0±0.1) km for the radius of a “canonical” 1.4M⊙ neutron star, yet is also able to support a two-solar-mass neutron star.http://www.sciencedirect.com/science/article/pii/S0370269315005304
spellingShingle Wei-Chia Chen
J. Piekarewicz
Searching for isovector signatures in the neutron-rich oxygen and calcium isotopes
Physics Letters B
title Searching for isovector signatures in the neutron-rich oxygen and calcium isotopes
title_full Searching for isovector signatures in the neutron-rich oxygen and calcium isotopes
title_fullStr Searching for isovector signatures in the neutron-rich oxygen and calcium isotopes
title_full_unstemmed Searching for isovector signatures in the neutron-rich oxygen and calcium isotopes
title_short Searching for isovector signatures in the neutron-rich oxygen and calcium isotopes
title_sort searching for isovector signatures in the neutron rich oxygen and calcium isotopes
url http://www.sciencedirect.com/science/article/pii/S0370269315005304
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