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The Super-Kamiokande detector
Super-Kamiokande is the world's largest water Cherenkov detector, with net mass 50,000 tons. During the period April, 1996 to July, 2001, Super-Kamiokande I collected 1678 live-days of data,Expand
Determination of solar neutrino oscillation parameters using 1496 days of Super-Kamiokande-I data
Abstract A number of different fits to solar neutrino mixing and mass square difference were performed using 1496 days of Super-Kamiokande-I's solar neutrino data. These data select two allowed areasExpand
Numerical Analysis of Standing Accretion Shock Instability with Neutrino Heating in Supernova Cores
We have numerically studied the instability of the spherically symmetric standing accretion shock wave against nonspherical perturbations. We have in mind the application to collapse-drivenExpand
THREE-DIMENSIONAL SIMULATIONS OF STANDING ACCRETION SHOCK INSTABILITY IN CORE-COLLAPSE SUPERNOVAE
We have studied nonaxisymmetric standing accretion shock instabilities, or SASI, using three-dimensional (3D) hydrodynamical simulations. This is an extension of our previous study of axisymmetricExpand
Supernova Neutrino Light Curves and Spectra for Various Progenitor Stars: From Core Collapse to Proto-neutron Star Cooling
We present a new series of supernova neutrino light curves and spectra calculated by numerical simulations for a variety of progenitor stellar masses (13-50M⊙) and metallicities (Z = 0.02 and 0.004),Expand
r-Process Nucleosynthesis in Magnetohydrodynamic Jet Explosions of Core-Collapse Supernovae
We investigate the r-process nucleosynthesis during a purely magnetohydrodynamic (MHD) explosion in a massive star of 13 M☉. The two-dimensional MHD simulations have been carried out from the onsetExpand
EFFECTS OF ROTATION ON STANDING ACCRETION SHOCK INSTABILITY IN NONLINEAR PHASE FOR CORE-COLLAPSE SUPERNOVAE
We study the effects of rotation on standing accretion shock instability (SASI) by performing three-dimensional hydrodynamics simulations. Taking into account a realistic equation of state andExpand
Gravitational Radiation from Standing Accretion Shock Instability in Core-Collapse Supernovae
We present the results of numerical experiments in which we study how asphericities induced by the growth of the standing accretion shock instability (SASI) produce gravitational waveforms in theExpand
Excitation of g-Modes in a Proto-Neutron Star by the Standing Accretion Shock Instability
The acoustic-revival mechanism in core-collapse supernovae, proposed recently by the Arizona group led by A. Burrows, is an interesting new scenario. With an aim to understanding the elementaryExpand
STOCHASTIC NATURE OF GRAVITATIONAL WAVES FROM SUPERNOVA EXPLOSIONS WITH STANDING ACCRETION SHOCK INSTABILITY
We study the properties of gravitational waves (GWs) based on three-dimensional (3D) simulations, which demonstrate neutrino-driven explosions aided by standing accretion shock instability (SASI).Expand
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