Equilibrium models of relativistic stars with a toroidal magnetic field
Joachim Frieben,Luciano Rezzolla +1 more
TLDR
In this article, a model of rotating relativistic stars with a toroidal magnetic field and rotation has been proposed to compute the surface deformation and the quadrupole distortion up to significant levels of rotation and magnetisation.Abstract:
We have computed models of rotating relativistic stars with a toroidal magnetic field and investigated the combined e ects of magnetic field and rotation on the apparent shape (i.e. the surface deformation), which could be relevant for the electromagnetic emission, and on the internal matter distribution (i.e. the quadrupole distortion), which could be relevant for the emission of gravitational waves. Using a sample of eight di erent cold nuclear-physics equations of state, we have computed models of maximum field strength, as well as the distortion coe cients for the surface and the quadrupolar deformations. Surprisingly, we find that nonrotating models admit arbitrary levels of magnetisation, accompanied by a growth of size and quadrupole distortion to which we could not find a limit. Rotating models, on the other hand, are subject to a mass-shedding limit at frequencies well below the corresponding ones for unmagnetised stars. Overall, the space of solutions can be split into three distinct classes for which the surface deformation and the quadrupole distortion are either: prolate and prolate, oblate and prolate, or oblate and oblate, respectively. We also derive a simple formula expressing the relativistic distortion coe cients and that allows one to compute the surface deformation and the quadrupole distortion up to significant levels of rotation and magnetisation, essentially covering all known magnetars. Such formula replaces Newtonian equivalent expressions that overestimate the quadrupole distortion by about a factor of five and are inadequate for strongly-relativistic objects like neutron stars.read more
Citations
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Binary Neutron Star Mergers: A Review of Einstein's Richest Laboratory
Luca Baiotti,Luciano Rezzolla +1 more
TL;DR: The recent progress in understanding what could be considered Einstein's richest laboratory is reviewed, highlighting in particular the numerous significant advances of the last decade in models, techniques and results for fully general-relativistic dynamical simulations.
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Rotating Stars in Relativity
TL;DR: The latest theoretical understanding of rotating stars in relativity is reviewed and several new sections have been added on equilibria in modified theories of gravity, approximate universal relationships, the one-arm spiral instability, and on analytic solutions for the exterior spacetime.
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Neutron Stars—Cooling and Transport
TL;DR: In this paper, the basics of thermal evolution for isolated neutron stars with strong magnetic fields are reviewed, including most relevant thermodynamic and kinetic properties in the stellar core, crust, and blanketing envelopes.
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Approximate Universal Relations for Neutron Stars and Quark Stars
TL;DR: Universal I-love-Q relations as discussed by the authors break degeneracies among astrophysical observables, leading to a variety of applications: (i) X-ray measurements of the nuclear matter equation of state, (ii) gravitational wave measurements of intrinsic spin of inspiraling compact objects, and (iii) gravitational and astrophysical tests of General Relativity that are independent of the equations of state.
Journal ArticleDOI
Approximate Universal Relations for Neutron Stars and Quark Stars
TL;DR: Universal relations between the star's moment of inertia (I ), its tidal Love number (Love) and its quadrupole moment (Q) have been studied in the context of astrophysics as discussed by the authors.
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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