activity
20072026
most citedHyper-Kamiokande Design Report

417 citations · 3.4k across the 62 of their papers we have counts for

collaborators
Showing 2023Show all

6 papers · 1 filter

astro-ph.HE2023★ 4 cited

Gravitational Collapse of White Dwarfs to Neutron Stars. I. From Initial Conditions to Explosions with Neutrino-radiation Hydrodynamics Simulations

Masamitsu Mori, Ryo Sawada, Yudai Suwa +3

This paper provides collapses of massive, fully convective, and non-rotating white dwarfs (WDs) formed by accretion-induced collapse or merger-induced collapse and the subsequent e…

astro-ph.SR2023★ 4 cited

Impacts of the reaction rate on nucleosynthesis in pair-instability supernovae

Hiroki Kawashimo, Ryo Sawada, Yudai Suwa +3

Nuclear reactions are key to our understanding of stellar evolution, particularly the rate, which is known to significantly influence the…

astro-ph.HE2023★ 1 cited

Observing Supernova Neutrino Light Curves with Super-Kamiokande. IV. Development of SPECIAL BLEND: a New Public Analysis Code for Supernova Neutrinos

Akira Harada, Yudai Suwa, Masayuki Harada +6

Supernova neutrinos are invaluable signals that offer information about the interior of supernovae. Because a nearby supernova can occur at any time, preparing for future supernova…

astro-ph.HE2023★ 17 cited

Long-term gravitational wave asteroseismology of supernova: from core collapse to 20 seconds postbounce

Masamitsu Mori, Yudai Suwa, Tomoya Takiwaki

We use an asteroseismology method to calculate the frequencies of gravitational waves in a long-term core-collapse supernova simulation, with a mass of 9.6 . The simulatio…

astro-ph.HE2023★ 2 cited

Timing coincidence search for supernova neutrinos with optical transient surveys

Sean Heston, Emily Kehoe, Yudai Suwa +1

Neutrinos allow the probing of stellar interiors during core collapse, helping to understand the different stages and processes in the collapse. To date, supernova neutrinos have o…

astro-ph.HE2023★ 5 cited

Updating the Ni Problem in Core-collapse Supernova Explosion

Ryo Sawada, Yudai Suwa

Details of the core-collapse supernova (CCSN) explosion mechanism still need to be fully understood. There is an increasing number of successful examples of reproducing explosions…