Detectability of collective neutrino oscillation signatures in the supernova explosion of a 8.8 M⊙ star
Abstract
In order to investigate the impact of collective neutrino oscillations (CNOs) on the neutrino signal from a nearby supernova, we perform three-flavor neutrino oscillation simulations employing the multiangle effect. The background hydrodynamic model is based on the neutrino hydrodynamic simulation of a 8.8 M⊙ progenitor star. In this work, we find that CNO commences after some 100 ms post bounce. Before this, CNO is suppressed by matter-induced decoherence. In the inverted mass hierarchy, the spectrum of $$\bar{ν}_e$$ becomes softer after the onset of CNO. To evaluate the detectability of this modification, we define a hardness ratio between the number of high energy neutrino events and low energy neutrino events adopting a fixed critical energy. We show that Hyper-Kamiokande (HK) can distinguish the effect of CNO for supernova distances out to ~ 10 kpc. On the other hand, for the normal mass hierarchy, the spectrum of ν e becomes softer after the onset of CNO, and we show that DUNE can distinguish this feature for supernova distances out to ~ 10 kpc . More work is necessary to optimize the best value of critical energy for maximum sensitivity. We also show that if the spectrum of $$\bar{ν}_e$$ in HK becomes softer due to CNO, the spectrum of $$ν_e$$ in DUNE becomes harder, and vice versa. These synergistic observations in $$\bar{ν}_e$$ and $$ν_e$$, by HK and DUNE, respectively, will be an intriguing opportunity to test the occurrence of CNO.
- Authors:
-
[2];
[3];
[4];
[5]
- Univ. of Tokyo (Japan); National Astronomical Observatory of Japan, Tokyo (Japan)
- National Astronomical Observatory of Japan, Tokyo (Japan)
- Univ. of Tokyo (Japan)
- Virginia Polytechnic Inst. and State Univ. (Virginia Tech), Blacksburg, VA (United States)
- Tohoku Univ., Sendai (Japan)
- Publication Date:
- Research Org.:
- Virginia Polytechnic Inst. and State Univ. (Virginia Tech), Blacksburg, VA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC); Japan Society for the Promotion of Science (JSPS); Ministry of Education, Culture, Sports, Science and Technology (MEXT); National Science Foundation (NSF)
- OSTI Identifier:
- 1803939
- Grant/Contract Number:
- SC0020262; JP17H01130; JP17K14306; JP17K17655; JP19J13632; JP18H01212; JP15H01039; JP17H06357; JP17H06364; JP17H05206; JP26104001; JP26104007; JP19H05803; 01321802; 01311904; AST-1908960; PHY-1914409
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review. D.
- Additional Journal Information:
- Journal Volume: 101; Journal Issue: 6; Journal ID: ISSN 2470-0010
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Astronomy & Astrophysics; Physics
Citation Formats
Sasaki, Hirokazu, Takiwaki, Tomoya, Kawagoe, Shio, Horiuchi, Shunsaku, and Ishidoshiro, Koji. Detectability of collective neutrino oscillation signatures in the supernova explosion of a 8.8 M⊙ star. United States: N. p., 2020.
Web. doi:10.1103/physrevd.101.063027.
Sasaki, Hirokazu, Takiwaki, Tomoya, Kawagoe, Shio, Horiuchi, Shunsaku, & Ishidoshiro, Koji. Detectability of collective neutrino oscillation signatures in the supernova explosion of a 8.8 M⊙ star. United States. https://doi.org/10.1103/physrevd.101.063027
Sasaki, Hirokazu, Takiwaki, Tomoya, Kawagoe, Shio, Horiuchi, Shunsaku, and Ishidoshiro, Koji. Thu .
"Detectability of collective neutrino oscillation signatures in the supernova explosion of a 8.8 M⊙ star". United States. https://doi.org/10.1103/physrevd.101.063027. https://www.osti.gov/servlets/purl/1803939.
@article{osti_1803939,
title = {Detectability of collective neutrino oscillation signatures in the supernova explosion of a 8.8 M⊙ star},
author = {Sasaki, Hirokazu and Takiwaki, Tomoya and Kawagoe, Shio and Horiuchi, Shunsaku and Ishidoshiro, Koji},
abstractNote = {In order to investigate the impact of collective neutrino oscillations (CNOs) on the neutrino signal from a nearby supernova, we perform three-flavor neutrino oscillation simulations employing the multiangle effect. The background hydrodynamic model is based on the neutrino hydrodynamic simulation of a 8.8 M⊙ progenitor star. In this work, we find that CNO commences after some 100 ms post bounce. Before this, CNO is suppressed by matter-induced decoherence. In the inverted mass hierarchy, the spectrum of $\bar{ν}_e$ becomes softer after the onset of CNO. To evaluate the detectability of this modification, we define a hardness ratio between the number of high energy neutrino events and low energy neutrino events adopting a fixed critical energy. We show that Hyper-Kamiokande (HK) can distinguish the effect of CNO for supernova distances out to ~ 10 kpc. On the other hand, for the normal mass hierarchy, the spectrum of ν e becomes softer after the onset of CNO, and we show that DUNE can distinguish this feature for supernova distances out to ~ 10 kpc . More work is necessary to optimize the best value of critical energy for maximum sensitivity. We also show that if the spectrum of $\bar{ν}_e$ in HK becomes softer due to CNO, the spectrum of $ν_e$ in DUNE becomes harder, and vice versa. These synergistic observations in $\bar{ν}_e$ and $ν_e$, by HK and DUNE, respectively, will be an intriguing opportunity to test the occurrence of CNO.},
doi = {10.1103/physrevd.101.063027},
journal = {Physical Review. D.},
number = 6,
volume = 101,
place = {United States},
year = {Thu Mar 26 00:00:00 EDT 2020},
month = {Thu Mar 26 00:00:00 EDT 2020}
}
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