Multimessenger signals of long-term core-collapse supernova simulations: synergetic observation strategies

被引:99
作者
Nakamura, Ko [1 ,2 ]
Horiuchi, Shunsaku [3 ]
Tanaka, Masaomi [4 ]
Hayama, Kazuhiro [4 ,5 ]
Takiwaki, Tomoya [4 ]
Kotake, Kei [4 ,6 ]
机构
[1] Waseda Univ, Fac Sci & Engn, Shinjuku Ku, Ohkubo 3-4-1, Tokyo 1698555, Japan
[2] Kyoto Univ, Yukawa Inst Theoret Phys, Kyoto 6068502, Japan
[3] Virginia Tech, Dept Phys, Ctr Neutrino Phys, Blacksburg, VA 24061 USA
[4] Natl Astron Observ Japan, Osawa 2-21-1, Mitaka, Tokyo 1818588, Japan
[5] Univ Tokyo, Inst Cosm Ray Res, KAGRA Observ, 238 Higashi Mozumi, Gifu 5061205, Japan
[6] Fukuoka Univ, Dept Appl Phys, Nanakuma Jonan 8-19-1, Fukuoka 8140180, Japan
基金
日本学术振兴会;
关键词
gravitational waves; neutrinos; supernovae: general; Galaxy: general; GENERAL-RELATIVISTIC SIMULATIONS; GRAVITATIONAL-WAVE SIGNATURES; STAR-FORMATION RATES; NEUTRINO BURST; SHOCK BREAKOUT; M-SUPERGIANTS; LIGHT CURVES; II PLATEAU; RADIATION HYDRODYNAMICS; MILKY-WAY;
D O I
10.1093/mnras/stw1453
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The next Galactic supernova is expected to bring great opportunities for the direct detection of gravitational waves (GW), full flavour neutrinos, and multiwavelength photons. To maximize the science return from such a rare event, it is essential to have established classes of possible situations and preparations for appropriate observations. To this end, we use a long-term numerical simulation of the core-collapse supernova (CCSN) of a 17 M-circle dot red supergiant progenitor to self-consistently model the multimessenger signals expected in GW, neutrino, and electromagnetic messengers. This supernova model takes into account the formation and evolution of a protoneutron star, neutrino-matter interaction, and neutrino transport, all within a two-dimensional shock hydrodynamics simulation. With this, we separately discuss three situations: (i) a CCSN at the Galactic Center, (ii) an extremely nearby CCSN within hundreds of parsecs, and (iii) a CCSN in nearby galaxies within several Mpc. These distance regimes necessitate different strategies for synergistic observations. In a Galactic CCSN, neutrinos provide strategic timing and pointing information. We explore how these in turn deliver an improvement in the sensitivity of GW analyses and help to guarantee observations of early electromagnetic signals. To facilitate the detection of multimessenger signals of CCSNe in extremely nearby and extragalactic distances, we compile a list of nearby red supergiant candidates and a list of nearby galaxies with their expected CCSN rates. By exploring the sequential multimessenger signals of a nearby CCSN, we discuss preparations for maximizing successful studies of such an unprecedented stirring event.
引用
收藏
页码:3296 / 3313
页数:18
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