Browsing School of Mathematical Sciences by Author "Uryu, K"
Now showing items 1-10 of 10
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Conservation laws and evolution schemes in geodesic, hydrodynamic, and magnetohydrodynamic flows
Markakis, C; Uryu, K; Gourgoulhon, E; Nicolas, J-P; Andersson, N; Pouri, A; Witzany, V (2017-09-13) -
Equilibrium solutions of relativistic rotating stars with mixed poloidal and toroidal magnetic fields
Uryu, K; Gourgoulhon, E; Markakis, CM; Fujisawa, K; Tsokaros, A; Eriguchi, Y (2014-11-07) -
Inferring the neutron star equation of state from binary inspiral waveforms
Markakis, C; Read, JS; Shibata, M; Uryu, K; Creighton, JDE; Friedman, JLThe properties of neutron star matter above nuclear density are not precisely known. Gravitational waves emitted from binary neutron stars during their late stages of inspiral and merger contain imprints of the neutron-star ... -
Magnetohydrodynamics in stationary and axisymmetric spacetimes: A fully covariant approach
Gourgoulhon, E; Markakis, C; Uryu, K; Eriguchi, Y (2011-05-03) -
Measuring the neutron star equation of state with gravitational wave observations
Read, JS; Markakis, C; Shibata, M; Uryu, K; Creighton, JDE; Friedman, JL (2009-06) -
Neutron star equation of state via gravitational wave observations
Markakis, C; Read, JS; Shibata, M; Uryu, K; Creighton, JDE; Friedman, JL; Lackey, BDGravitational wave observations can potentially measure properties of neutron star equations of state by measuring departures from the point-particle limit of the gravitational waveform produced in the late inspiral of a ... -
New code for equilibriums and quasiequilibrium initial data of compact objects. IV. Rotating relativistic stars with mixed poloidal and toroidal magnetic fields
Uryu, K; Yoshida, S; Gourgoulhon, E; Markakis, C; Fujisawa, K; Tsokaros, A; Taniguchi, K; Eriguchi, Y (American Physical Society, 2019-12-19)A new code for computing fully general relativistic solutions of strongly magnetized rapidly rotating compact stars is developed as a part of the Compact Object CALculator (cocal) code. The full set of Einstein’s equations, ... -
Quasi-equilibrium models of magnetized compact objects
Markakis, C; Uryu, K; Gourgoulhon, E (2011) -
Quasiequilibrium models for triaxially deformed rotating compact stars
Huang, X; Markakis, C; Sugiyama, N; Uryu, K (2008-12) -
Thermodynamics of magnetized binary compact objects
Uryu, K; Gourgoulhon, E; Markakis, C (2010-11-30)