Neutron Star Structure and the Equation of State
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In this article, Buchdahl and Tolman showed that the moment of inertia and the binding energy of a neutron star are nearly universal functions of the star's compactness, which can be understood by considering two analytic, yet realistic, solutions of Einstein's equations.Abstract:
The structure of neutron stars is considered from theoretical and observational perspectives We demonstrate an important aspect of neutron star structure: the neutron star radius is primarily determined by the behavior of the pressure of matter in the vicinity of nuclear matter equilibrium density In the event that extreme softening does not occur at these densities, the radius is virtually independent of the mass and is determined by the magnitude of the pressure For equations of state with extreme softening or those that are self-bound, the radius is more sensitive to the mass Our results show that in the absence of extreme softening, a measurement of the radius of a neutron star more accurate than about 1 km will usefully constrain the equation of state We also show that the pressure near nuclear matter density is primarily a function of the density dependence of the nuclear symmetry energy, while the nuclear incompressibility and skewness parameters play secondary roles In addition, we show that the moment of inertia and the binding energy of neutron stars, for a large class of equations of state, are nearly universal functions of the star's compactness These features can be understood by considering two analytic, yet realistic, solutions of Einstein's equations, by, respectively, Buchdahl and Tolman We deduce useful approximations for the fraction of the moment of inertia residing in the crust, which is a function of the stellar compactness and, in addition, the pressure at the core-crust interfaceread more
Citations
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Relation between gravitational mass and baryonic mass for non-rotating and rapidly rotating neutron stars
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Are there nuclear structure effects on the isoscalar giant monopole resonance and nuclear incompressibility near A∼90?
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On magnetic-field-induced corrections to the orbital and epicyclic frequencies: paper II. Slowly rotating magnetized neutron stars
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The Parkes pulsar timing array second data release: Timing analysis
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TL;DR: The Parkes Pulsar Timing Array (PPTA) project has been used to detect correlated signals such as nanohertz-frequency gravitational waves over time spans of up to 24 years as discussed by the authors.
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Temperature dependence of the nuclear symmetry energy and equation of state of charge neutral n + p + e + μ matter in beta equilibrium
TL;DR: In this paper, the temperature and density dependence of the nuclear symmetry energy was studied in the nonrelativistic mean field theory by using a density-dependent finite range effective interaction, and the temperature evolution of the interaction part of symmetry energy is decided by the nature of the finite range exchange interactions acting between a pair of like and unlike nucleons.
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Swinkels,Marek Szczepanczyk,M. Tacca,S. C. Tait,Colm Talbot,D. Talukder,David B. Tanner,Márton Tápai,Andrea Taracchini,Jay D. Tasson,J. A. Taylor,R. Taylor,Sumanta Tewari,T. Theeg,F. Thies,E. G. Thomas,M. Thomas,P. Thomas,K. A. Thorne,Kip S. Thorne,Eric Thrane,S. N. Tiwari,V. Tiwari,K. V. Tokmakov,K. Toland,M. Tonelli,Z. Tornasi,Alejandro Torres-Forné,C. I. Torrie,D. Töyrä,F. Travasso,G. Traylor,J. Trinastic,M. C. Tringali,L. Trozzo,K. W. Tsang,Maggie Tse,R. Tso,Leo Tsukada,Daichi Tsuna,D. Tuyenbayev,K. Ueno,D. Ugolini,C. S. Unnikrishnan,A. L. Urban,S. A. Usman,H. Vahlbruch,G. Vajente,G. Valdes,Michele Vallisneri,N. van Bakel,M. van Beuzekom,J. F. J. van den Brand,C. Van Den Broeck,D. C. Vander-Hyde,L. van der Schaaf,J. V. van Heijningen,A. A. van Veggel,M. Vardaro,Vijay Varma,S. Vass,M. Vasúth,Alberto Vecchio,G. Vedovato,John Veitch,P. J. Veitch,K. Venkateswara,G. Venugopalan,D. Verkindt,F. Vetrano,A. Viceré,Aaron Viets,Serena Vinciguerra,D. J. Vine,J-Y. Vinet,Salvatore Vitale,T. 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