Kotaro Kyutoku (Assistant Prof. in KEK and iTHEMS visiting researcher. Former iTHEMS SPDR) has published a book "Origins of the Gravitational Wave" in Japanese with Masaru Shibata (Max Planck Institute and Kyoto Univ.).
It contains excellent explanations on general relativity and black holes, structure of neutron stars, supernova explosion, gamma-ray burst, gravitational wave, mergers of black holes and neutron stars, and current/future gravitational wave detectors on earth and space.
Everybody who is interested in GW should have one in his/her bookshelf. English translation will be called for.

A joint research group consisting of Masaomi Ono, a Research Scientist at RIKEN, and others has theoretically predicted that an unstable isotope Technetium-98 (98Tc) could be synthesized by neutrinos emitted from supernova explosions.
Supernovae are important events in the evolution of stars and galaxies, but the details of how the explosions occur are still unknown. This research found a method to investigate the role of electron anti-neutrinos in supernovae. By measuring the amount of 98Ru (an isotope of Ruthenium) in meteorites, it should be possible to estimate how much of its progenitor 98Tc was present in the material at the time when the Solar System formed. The amount of 98Tc in turn is sensitive to the characteristics, such as temperature, of electron anti-neutrinos in the supernova process; as well as to how much time passed between the supernova and the formation of the Solar System.
(This work appeared in Physical Review Letters on Sept. 4, 2018.)

Caption: We can estimate the age of heavy elements in the primordial Solar System by measuring the traces left in meteorites by specific radioactive nuclei synthesized in certain types of supernovae.
Credit: NAOJ (National Astronomical Observatory of Japan)

My name is Gen Kurosawa. I study “Biological Timing”. We know timing of meal influences timing of sleep. Similarly, we know timing of taking medicine influences its efficacy. We know these facts, but we do not really know why. To answer these questions, my approach is to use two types of models. Mainly, I try to develop simpler models to understand the essence in Biological Timing. Simultaneously, I use realistic models (ex. 180 variable ODE model with genes and proteins) to make detailed predictions which can be tested experimentally in a very near future. At iTHEMS, I am happy that I can interact with colleagues from various disciplines.