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Page 1
Magnetohydrodynamic Simulations of Self-Consistent Rotating Neutron Stars with Mixed Poloidal and Toroidal Magnetic Fields.
Phys Rev Lett. 2022 Feb 11;128(6):061101. doi: 10.1103/PhysRevLett.128.061101.
Phys Rev Lett. 2022.
PMID: 35213191
Gravitational wave content and stability of uniformly, rotating, triaxial neutron stars in general relativity.
Tsokaros A, Ruiz M, Paschalidis V, Shapiro SL, Baiotti L, Uryū K.
Tsokaros A, et al. Among authors: uryu k.
Phys Rev D. 2017 Jun 15;95(12):124057. doi: 10.1103/PhysRevD.95.124057. Epub 2017 Jun 30.
Phys Rev D. 2017.
PMID: 29888340
Free PMC article.
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Great Impostors: Extremely Compact, Merging Binary Neutron Stars in the Mass Gap Posing as Binary Black Holes.
Tsokaros A, Ruiz M, Shapiro SL, Sun L, Uryū K.
Tsokaros A, et al. Among authors: uryu k.
Phys Rev Lett. 2020 Feb 21;124(7):071101. doi: 10.1103/PhysRevLett.124.071101.
Phys Rev Lett. 2020.
PMID: 32142310
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Dynamically Stable Ergostars Exist: General Relativistic Models and Simulations.
Tsokaros A, Ruiz M, Sun L, Shapiro SL, Uryū K.
Tsokaros A, et al. Among authors: uryu k.
Phys Rev Lett. 2019 Dec 6;123(23):231103. doi: 10.1103/PhysRevLett.123.231103.
Phys Rev Lett. 2019.
PMID: 31868499
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Binary neutron stars: Equilibrium models beyond spatial conformal flatness.
Uryū K, Limousin F, Friedman JL, Gourgoulhon E, Shibata M.
Uryū K, et al.
Phys Rev Lett. 2006 Oct 27;97(17):171101. doi: 10.1103/PhysRevLett.97.171101. Epub 2006 Oct 27.
Phys Rev Lett. 2006.
PMID: 17155457
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