Rohta Takahashi

Accretion process onto super-spinning objects (2009)

Bambi, Cosimo, Freese, Katherine, Harada, Tomohiro, Takahashi, Rohta, Yoshida, Naoki

The accretion process onto spinning objects in Kerr spacetimes is studied with numerical simulations. Our results show that accretion onto compact objects with Kerr parameter (characterizing the...

Testing the Accretion Flow with Plasma Wave Heating Mechanism for Sagittarius a* by the 1.3MM Vlbi Measurements (2009)

Huang, Lei, Takahashi, Rohta, Shen, Zhi-Qiang

The vicinity of the supermassive black hole associated with the compact radio source Sagittarius (Sgr) A* is believed to dominate the observed emission at wavelengths near and shorter than $\sim$ 1...

Is the Carter-Israel conjecture correct? (2009)

Bambi, Cosimo, Freese, Katherine, Takahashi, Rohta

According to the Carter-Israel conjecture, the end-state of the gravitational collapse of matter is a Kerr-Newman black hole. Nevertheless, neither the theory nor observations can confirm that. In...

An Approach Detecting the Event Horizon of Sgr A* (2008)

Miyoshi, Makoto, Kameno, Seiji, Ishituka, Jose K., Shen, Zhi-Qiang, Takahashi, Rohta, Horiuchi, Shinji

Imaging the vicinity of a black hole is one of the ultimate goals of VLBI astronomy. The closest massive black hole, Sgr A*, located at the Galactic center, is the leading candidate for such...

Radiation Hydrodynamics in Kerr Spacetime: Equations without Coordinate Singularity at the Event Horizon (2007)

Takahashi, Rohta

Equations of fully general relativistic radiation hydrodynamics around a rotating black hole are derived by using the Kerr-Schild coordinate where there is no coordinate singularity at the event...

Equations of general relativistic radiation hydrodynamics in Kerr space-time (2007)

Takahashi, Rohta

Equations of fully general relativistic radiation hydrodynamics in Kerr space-time are derived. While the interactions between matter and radiation are introduced in the comoving frame, the...

Horizon-Penetrating Transonic Accretion Disks around Rotating Black Holes (2007)

Takahashi, Rohta

The stationary hydrodynamic equations for the transonic accretion disks and flows around rotating black holes are presented by using the Kerr-Schild coordinate where there is no coordinate...

Advection-dominated accretion flows with causal viscosity (2007)

Takahashi, Rohta

We present the basic equations and sample solutions for the steady-state global transonic solutions of the advection-dominated accretion flows (ADAFs) with a causal viscosity prescription. The...

Eclipsing light curves for accretion flows around a rotating black hole and atmospheric effects of the companion star (2007)

Takahashi, Rohta, Watarai, Ken-Ya

We calculate eclipsing light curves for accretion flows around a rotating black hole taking into account the atmospheric effects of the companion star. In the cases of no atmospheric effects, the...

Eclipsing Light-Curve Asymmetry for Black-Hole Accretion Flows (2005)

Watarai, Ken-ya, Takahashi, Rohta, Fukue, Jun

We propose an eclipsing light-curve diagnosis for black-hole accretion flows. When emission from an inner accretion disk around a black hole is occulted by a companion star, the observed light curve...

Black Hole Shadows of Charged Spinning Black Holes (2005)

Takahashi, Rohta

We propose a method for measuring the black hole charge by imaging a black hole shadow in a galactic center by future interferometers. Even when the black hole is uncharged, it is possible to confirm...

Shapes and Positions of Black Hole Shadows in Accretion Disks and Spin Parameters of Black Holes (2004)

Takahashi, Rohta

Can we determine a spin parameter of a black hole by observation of a black hole shadow in an accretion disk? In order to answer this question, we make a qualitative analysis and a quantitative...

X-Ray Microlensing of Bright Quasars (2001)

Takahashi, Rohta, Yonehara, Atsunori, Mineshige, Shin

We calculated the expected microlens light curves for several accretion-flow models and compared the results to find what aspects of distinct flow structures can be extracted from the microlens light...