Constraints on neutron stars equation of state using the tidal deformability derived from BNS mergers
نویسندگان
چکیده
منابع مشابه
Spin and Isospin Asymmetry, Equation of State and Neutron Stars
In the present work, we have obtained the equation of state for neutron star matter considering the in uence of the ferromagnetic and antiferromagnetic spin state. We have also investigated the structure of neutron stars. According to our results, the spin asymmetry stiens the equation of state and leads to high mass for the neutron star.
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متن کاملspin and isospin asymmetry, equation of state and neutron stars
in the present work, we have obtained the equation of state for neutron star matter considering the in uence of the ferromagnetic and antiferromagnetic spin state. we have also investigated the structure of neutron stars. according to our results, the spin asymmetry sti ens the equation of state and leads to high mass for the neutron star.
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Tanja Hinderer, Benjamin D. Lackey, Ryan N. Lang, and Jocelyn S. Read Theoretical Astrophysics, California Institute of Technology, Pasadena, California 91125, USA Department of Physics, University of Wisconsin–Milwaukee, P.O. Box 413, Milwaukee, Wisconsin 53201, USA Department of Physics and MIT Kavli Institute, MIT, 77 Massachusetts Avenue, Cambridge, Massachusetts 02139, USA Gravitational As...
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The kilohertz frequencies of QPOs from accreting neutron star systems imply that they are generated in regions of strong gravity, close to the star. This suggests that observations of the QPOs can be used to constrain the properties of neutron stars themselves, and in particular to inform us about the properties of cold matter beyond nuclear densities. Here we discuss some relatively model-inse...
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ژورنال
عنوان ژورنال: HNPS Proceedings
سال: 2020
ISSN: 2654-0088,2654-007X
DOI: 10.12681/hnps.2989