2020 Fiscal Year Annual Research Report

マグネター駆動型超新星爆発の研究

Research Project

Project/Area Number	18J21778
Research Institution	The University of Tokyo
Principal Investigator	OMAND CONOR 東京大学, 理学系研究科, 特別研究員(DC1)
Project Period (FY)	2018-04-25 – 2021-03-31
Keywords	Magnetar / Pulsar / Pulsar Wind Nebula / Radio Emission / Supernova / Superluminous Supernova / Fast Radio Burst / Spectroscopy
Outline of Annual Research Achievements	I joined a new collaboration which was doing a large radio survey of superluminous supernova (SLSN) remanants. I wrote a comparison between my method and their method of determining pulsar parameters from optical light curves, and altered my code to generate radio light curves in a consistent way. We published the survey results and pulsar constraints, and found that the model, with the assumptions we are currently using, is inconsistent with several supernovae. I continued working on code for determining optical spectra, but decided to collaborate with a group that has already developed similar code. We are modeling these spectra now. I wrote my PhD thesis and graduated.
Research Progress Status	令和2年度が最終年度であるため、記入しない。
Strategy for Future Research Activity	令和2年度が最終年度であるため、記入しない。