TY - JOUR
T1 - Potential Impact of Fast Flavor Oscillations on Neutrino-driven Winds and Their Nucleosynthesis
AU - Xiong, Zewei
AU - Sieverding, Andre
AU - Sen, Manibrata
AU - Qian, Yong Zhong
N1 - Publisher Copyright:
© 2020. The American Astronomical Society. All rights reserved..
PY - 2020/9/10
Y1 - 2020/9/10
N2 - 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.
AB - 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.
UR - http://www.scopus.com/inward/record.url?scp=85091024856&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85091024856&partnerID=8YFLogxK
U2 - 10.3847/1538-4357/abac5e
DO - 10.3847/1538-4357/abac5e
M3 - Article
AN - SCOPUS:85091024856
SN - 0004-637X
VL - 900
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 144
ER -