A survey of the parameter space of the compressible liquid drop model as applied to the neutron star inner crust
TLDR
In this article, the authors present a systematic survey of the range of predictions of the neutron star inner crust composition, crust-core transition densities and pressures, and density range of the nuclear "pasta" phases at the bottom of the crust provided by the compressible liquid drop model in the light of current experimental and theoretical constraints on model parameters.Abstract:
We present a systematic survey the range of predictions of the neutron star inner crust composition, crust-core transition densities and pressures, and density range of the nuclear ‘pasta’ phases at the bottom of the crust provided by the compressible liquid drop model in the light of current experimental and theoretical constraints on model parameters. Using a Skyrme-like model for nuclear matter, we construct baseline sequences of crust models by consistently varying the density dependence of the bulk symmetry energy at nuclear saturation density, L, under two conditions: (i) that the magnitude of the symmetry energy at saturation density J is held constant, and (ii) J correlates with L under the constraint that the pure neutron matter (PNM) EoS satises the results of ab-initio calculations at low densities. Such baseline crust models facilitate consistent exploration of the L dependence of crustal properties. The remaining surface energy and symmetric nuclear matter parameters are systematically varied around the baseline, and dierent functional forms of the PNM EoS at sub-saturation densities implemented, to estimate theoretical ‘error bars’ for the baseline predictions. Inner crust composition and transition densities are shown to be most sensitive to the surface energy at very low proton fractions and to the behavior of the sub-saturation PNM EoS. Recent calculations of the energies of neutron drops suggest that the low-proton-fraction surface energy might be higher than predicted in Skyrme-like models, which our study suggests may result in a greatly reduced volume of pasta in the crust than conventionally predicted.read more
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Maximum elastic deformations of relativistic stars
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Unified equation of state for neutron stars on a microscopic basis
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Combined Constraints on the Equation of State of Dense Neutron-rich Matter from Terrestrial Nuclear Experiments and Observations of Neutron Stars
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Combined Constraints on the Equation of State of Dense Neutron-Rich Matter from Terrestrial Experiments and Observations of Neutron Stars
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TL;DR: Within the parameter space of dense neutron-rich matter limited by existing constraints mainly from terrestrial nuclear experiments, this paper investigated how the neutron star maximum mass $M{max}}>2.01\pm0.04$ M$_\odot, radius $10.83$ km and tidal deformability $\Lambda_{1.4}=800$ from the recent observation of GW170817 is found to provide upper limits on some EOS parameters consistent with but far less restrictive than the existing constraints of other observables studied.
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Towards understanding astrophysical effects of nuclear symmetry energy
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References
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Vo,H. Vocca,C. Vorvick,Sergey P. Vyatchanin,A. R. Wade,L. E. Wade,Madeline Wade,R. C. Walet,Michelle E. Walker,L. Wallace,S. Walsh,G. Wang,Haiyan Wang,J. Z. Wang,W. H. Wang,Y. F. Wang,R. L. Ward,J. Warner,M. Was,Jennifer Watchi,B. A. Weaver,L.-W. Wei,M. Weinert,A. J. Weinstein,Rainer Weiss,Linqing Wen,E. K. Wessel,P. Weßels,J. Westerweck,Tobias Westphal,K. Wette,James Whelan,S. E. Whitcomb,B. F. Whiting,C. Whittle,D. M. Wilken,David A. Williams,Roy Williams,A. R. Williamson,J. L. Willis,Benno Willke,M. H. Wimmer,Walter Winkler,C. C. Wipf,H. Wittel,Graham Woan,J. Woehler,J. K. Wofford,K. W. K. Wong,John Worden,J. L. Wright,D. S. Wu,Daniel Wysocki,S. Xiao,H. Yamamoto,C. C. Yancey,Lili Yang,M. J. Yap,Maher Yazback,Hang Yu,Haocun Yu,M. Yvert,A. K. Zadrożny,Michele Zanolin,T. Zelenova,J. P. Zendri,M. Zevin,L. Zhang,Mi Zhang,T. Zhang,Yanxi Zhang,Chunnong Zhao,Minchuan Zhou,Zifan Zhou,Sylvia J. Zhu,Xing-Jiang Zhu,Aaron Zimmerman,Michael E Zucker,J. Zweizig +1134 more