71 citations · 175 across the 7 of their papers we have counts for
8 papers
Yukawa textures due to selection rules in magnetized orbifold models
Tatsuo Kobayashi, Tomoyasu Kori, Shuhei Miyamoto +2
We study systematically Yukawa textures, which can be derived from magnetized and orbifold models with various magnetic fluxes and Scherk-Schw…
More about modular symmetries and non-invertible properties in magnetized compactifications
Tatsuo Kobayashi, Shuhei Miyamoto, Riku Nakano +2
We study the modular symmetry in magnetized compactifications. The zero-modes with different Scherk-Schwarz phases transform each other. A generic model does not include modes with…
Lepton mass textures from non-invertible multiplication rules
Tatsuo Kobayashi, Hajime Otsuka, Morimitsu Tanimoto +1
We study the lepton mass textures, which are derived by gauging of symmetries. We can obtain various textures for the Yukawa couplings in the charged…
Gravitational waves from very massive stars collapsing to a black hole
Haruki Uchida, Masaru Shibata, Koh Takahashi +1
We compute gravitational waves emitted by the collapse of a rotating very massive star (VMS) core leading directly to a black hole in axisymmetric numerical-relativity simulations.…
Black Hole Formation and Explosion from Rapidly Rotating Very Massive Stars
Haruki Uchida, Masaru Shibata, Koh Takahashi +1
We explore the formation process of a black hole (BH) through the pair-instability collapse of a rotating Population III very massive star in axisymmetric numerical relativity. As…
Gravitational Collapse of Rotating Supermassive Stars including Nuclear Burning Effects
Haruki Uchida, Masaru Shibata, Takashi Yoshida +2
Supermassive stars (SMSs) of mass are candidates for seeds of supermassive black holes found in the center of many massive galaxies. We simulate the gravitat…
Gravitational waves from supermassive stars collapsing to a supermassive black hole
Masaru Shibata, Yuichiro Sekiguchi, Haruki Uchida +1
We derive the gravitational waveform from the collapse of a rapidly rotating supermassive star (SMS) core leading directly to a seed of a supermassive black hole (SMBH) in axisymme…
Stability of rigidly rotating supermassive stars against gravitational collapse
Masaru Shibata, Haruki Uchida, Yuichiro Sekiguchi
We revisit secular stability against quasi-radial collapse for rigidly rotating supermassive stars (SMSs) in general relativity. We suppose that the SMSs are in a nuclear-burning p…