Search Results - "ERIGUCHI, Yoshiharu"
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Prolate stars due to meridional flows
Published in Monthly notices of the Royal Astronomical Society. Letters (01-02-2014)“…We have shown analytically that shapes of incompressible stars could be prolate if appropriate meridional flows exist. Although this result is strictly valid…”
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Appearance of the prolate and the toroidal magnetic field dominated stars: Analytic approach
Published in Publications of the Astronomical Society of Japan (01-06-2015)“…We have analyzed magnetized equilibrium states and shown a condition for the appearance of the prolate and the toroidal magnetic field-dominated stars using…”
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Magnetohydrodynamics in stationary and axisymmetric spacetimes: A fully covariant approach
Published in Physical review. D, Particles, fields, gravitation, and cosmology (03-05-2011)Get full text
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Counter effects of meridional flows and magnetic fields in stationary axisymmetric self-gravitating barotropes under the ideal MHD approximation: clear examples - toroidal configurations
Published in Monthly notices of the Royal Astronomical Society (11-05-2013)“…We obtain the general forms for the current density and the vorticity from the integrability conditions of the basic equations which govern the stationary…”
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Twisted-Torus Equilibrium Structures of Magnetic Fields in Magnetized Stars
Published in The Astrophysical journal (01-11-2006)“…We have investigated the "universality" of the twisted-torus equilibrium structures of the magnetic fields in deformed stars. The Tomimura-Eriguchi scheme for…”
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Coexistence of oppositely flowing multi-φ currents: key to large toroidal magnetic fields within stars
Published in Monthly notices of the Royal Astronomical Society (21-06-2013)Get full text
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Coexistence of oppositely flowing multi- currents: key to large toroidal magnetic fields within stars
Published in Monthly notices of the Royal Astronomical Society (21-06-2013)“…We will show the importance of coexistence of oppositely flowing currents for magnetized stars to sustain strong toroidal magnetic fields within the stars by…”
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Axisymmetric and stationary structures of magnetized barotropic stars with extremely strong magnetic fields deep inside
Published in Monthly notices of the Royal Astronomical Society (01-05-2012)“…We have succeeded in obtaining magnetized star models that have extremely strong magnetic fields in the interior of the star. In our formulation, arbitrary…”
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Equilibrium solutions of relativistic rotating stars with mixed poloidal and toroidal magnetic fields
Published in Physical review. D, Particles, fields, gravitation, and cosmology (07-11-2014)“…Stationary and axisymmetric solutions of relativistic rotating stars with strong mixed poloidal and toroidal magnetic fields are obtained numerically. Because…”
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Possible evolutionary transition from rapidly rotating neutron stars to strange stars due to spin-down
Published in Progress of theoretical physics (01-05-2005)Get full text
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Equilibrium states of magnetized toroid–central compact object systems
Published in Monthly notices of the Royal Astronomical Society (11-07-2009)“…Equilibrium configurations of self-gravitating magnetized toroid–central compact object systems have been constructed in the framework of the Newtonian…”
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New exact solutions of magnetic ellipsoidal figures of equilibrium
Published in Monthly notices of the Royal Astronomical Society. Letters (01-09-2011)“…Abstract In this Letter we report brand new analytic stationary solutions of constant density stars with magnetic field and self-gravity. These solutions…”
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Equilibrium states of magnetized toroid-central compact object systems
Published in Monthly notices of the Royal Astronomical Society (11-07-2009)Get full text
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Dynamical instability of differentially rotating stars
Published in Monthly notices of the Royal Astronomical Society (01-08-2002)“…We study the dynamical instability against bar-mode deformation of differentially rotating stars. We performed numerical simulation and linear perturbation…”
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Dynamical bar-mode instability of differentially rotating stars: effects of equations of state and velocity profiles
Published in Monthly notices of the Royal Astronomical Society (01-08-2003)“…As an extension of our previous work, we investigate the dynamical instability against non-axisymmetric bar-mode deformations of differentially rotating stars…”
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New numerical method for constructing quasiequilibrium sequences of irrotational binary neutron stars in general relativity
Published in Physical review. D, Particles and fields (15-06-2000)Get full text
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Darwin-Riemann Problems in Newtonian Gravity
Published in Progress of theoretical physics. Supplement (01-01-1999)“…In this paper, we have reviewed the present status of the theory of equilibrium configurations of compact binary star systems in Newtonian gravity…”
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