MG11 |
Participant |
Suwa, Yudai | |
|
Institution |
Dept. of Physics, The University of Tokyo - 7-3-1 Hongo, Bunkyo-ku - Tokyo - - JAPAN | |
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Session |
Talk |
Abstract |
|
APT1 |
Gravitational Collapse of Population III Stars |
Population III stars are thought to be very massive stars. However, their properties are not clarified yet. Population III stars are thought to be very massive stars. However, their properties are not clarified yet. In this research, we investigate the features of magneto-rotational dynamics of such stars with computer simulations. We inquire the dependences of the mass of black hole on rotaion and magnetic field. In addition, we also study the features of gravitational waves and neutrinos from such stars. |