Extremely efficient fully three-dimensional hydrodynamic simulations of supernova remnants for the new age of microcalorimetric X-ray astronomy

• Project/Area Number: 24K07092
• Research Category: Grant-in-Aid for Scientific Research (C)
• Allocation Type: Multi-year Fund
• Section: 一般
• Review Section: Basic Section 16010:Astronomy-related
• Research Institution: Kyoto University
• Principal Investigator: 李 兆衡 京都大学, 理学研究科, 講師 (50611844)
• Project Period (FY): 2024-04-01 – 2029-03-31
• Project Status: Granted (Fiscal Year 2024)
• Budget Amount: ¥4,810,000 (Direct Cost: ¥3,700,000、Indirect Cost: ¥1,110,000); Fiscal Year 2028: ¥910,000 (Direct Cost: ¥700,000、Indirect Cost: ¥210,000); Fiscal Year 2027: ¥910,000 (Direct Cost: ¥700,000、Indirect Cost: ¥210,000); Fiscal Year 2026: ¥910,000 (Direct Cost: ¥700,000、Indirect Cost: ¥210,000); Fiscal Year 2025: ¥910,000 (Direct Cost: ¥700,000、Indirect Cost: ¥210,000); Fiscal Year 2024: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
• Keywords: Supernova remnants / X-ray astronomy / Plasma / Hydrodynamics

Outline of Research at the Start

With the application of our extremely efficient fully three-dimensional hydrodynamic simulation tool, this project will provide the SN/SNR community an extensive library of theoretical results such as broadband spectral templates and evolution models for various explosions in a diverse environment.