Potential Impact of Fast Flavor Oscillations on Neutrino-driven Winds and Their Nucleosynthesis
Abstract
The wind driven by the intense neutrino emission from a protoneutron star (PNS) is an important site for producing nuclei heavier than the Fe group. Because of certain features in the neutrino angular distributions, the so-called fast flavor oscillations may occur very close to the PNS surface, effectively resetting the neutrino luminosities and energy spectra that drive the wind. Using the unoscillated neutrino emission characteristics from two core-collapse supernova simulations representative of relevant progenitors at the lower and higher mass end, we study the potential effects of fast flavor oscillations on neutrino-driven winds and their nucleosynthesis. We find that such oscillations can increase the total mass loss by factors up to ~1.5–1.7 and lead to significantly more proton-rich conditions. The latter effect can greatly enhance the production of 64Zn and the so-called light p-nuclei 74Se, 78Kr, and 84Sr. Implications for abundances in metal-poor stars, Galactic chemical evolution in general, and isotopic anomalies in meteorites are discussed.
- Authors:
-
- Univ. of Minnesota, Minneapolis, MN (United States). School of Physics and Astronomy
- Northwestern Univ., Evanston, IL (United States). Dept. of Physics and Astronomy; Univ. of California, Berkeley, CA (United States). Dept. of Physics
- Publication Date:
- Research Org.:
- Univ. of Minnesota, Minneapolis, MN (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Nuclear Physics (NP)
- OSTI Identifier:
- 1800667
- Grant/Contract Number:
- FG02-87ER40328
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal (Online)
- Additional Journal Information:
- Journal Name: The Astrophysical Journal (Online); Journal Volume: 900; Journal Issue: 2; Journal ID: ISSN 1538-4357
- Publisher:
- IOP Publishing
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; nucleosynthesis; neutrino oscillations; supernovae; explosive nucleosynthesis
Citation Formats
Xiong, Zewei, Sieverding, Andre, Sen, Manibrata, and Qian, Yong-Zhong. Potential Impact of Fast Flavor Oscillations on Neutrino-driven Winds and Their Nucleosynthesis. United States: N. p., 2020.
Web. doi:10.3847/1538-4357/abac5e.
Xiong, Zewei, Sieverding, Andre, Sen, Manibrata, & Qian, Yong-Zhong. Potential Impact of Fast Flavor Oscillations on Neutrino-driven Winds and Their Nucleosynthesis. United States. https://doi.org/10.3847/1538-4357/abac5e
Xiong, Zewei, Sieverding, Andre, Sen, Manibrata, and Qian, Yong-Zhong. Thu .
"Potential Impact of Fast Flavor Oscillations on Neutrino-driven Winds and Their Nucleosynthesis". United States. https://doi.org/10.3847/1538-4357/abac5e. https://www.osti.gov/servlets/purl/1800667.
@article{osti_1800667,
title = {Potential Impact of Fast Flavor Oscillations on Neutrino-driven Winds and Their Nucleosynthesis},
author = {Xiong, Zewei and Sieverding, Andre and Sen, Manibrata and Qian, Yong-Zhong},
abstractNote = {The wind driven by the intense neutrino emission from a protoneutron star (PNS) is an important site for producing nuclei heavier than the Fe group. Because of certain features in the neutrino angular distributions, the so-called fast flavor oscillations may occur very close to the PNS surface, effectively resetting the neutrino luminosities and energy spectra that drive the wind. Using the unoscillated neutrino emission characteristics from two core-collapse supernova simulations representative of relevant progenitors at the lower and higher mass end, we study the potential effects of fast flavor oscillations on neutrino-driven winds and their nucleosynthesis. We find that such oscillations can increase the total mass loss by factors up to ~1.5–1.7 and lead to significantly more proton-rich conditions. The latter effect can greatly enhance the production of 64Zn and the so-called light p-nuclei 74Se, 78Kr, and 84Sr. Implications for abundances in metal-poor stars, Galactic chemical evolution in general, and isotopic anomalies in meteorites are discussed.},
doi = {10.3847/1538-4357/abac5e},
journal = {The Astrophysical Journal (Online)},
number = 2,
volume = 900,
place = {United States},
year = {Thu Sep 10 00:00:00 EDT 2020},
month = {Thu Sep 10 00:00:00 EDT 2020}
}
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