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Core-collapse supernovae are dramatic explosions marking the catastrophic endof massive stars. The only means to get direct information about the supernovaengine is from observations of neutrinos emitted by the forming neutron star,and through gravitational waves which are produced when the hydrodynamic flowor the neutrino flux is not perfectly spherically symmetric. Themultidimensionality of the supernova engine, which breaks the sphericity of thecentral core such as convection, rotation, magnetic fields, and hydrodynamicinstabilities of the supernova shock, is attracting great attention as the mostimportant ingredient to understand the long-veiled explosion mechanism. Basedon our recent work, we summarize properties of gravitational waves, neutrinos,and explosive nucleosynthesis obtained in a series of our multidimensionalhydrodynamic simulations and discuss how the mystery of the central engines canbe unraveled by deciphering these multimessengers produced under the thickveils of massive stars.

Multimessengers from core-collapse supernovae: multidimensionality as a key to bridge theory and observation