Mu-Tau Neutrinos: Influencing Fast Flavor Conversions in Supernovae

被引:57
作者
Capozzi, Francesco [1 ]
Chakraborty, Madhurima [2 ]
Chakraborty, Sovan [2 ]
Sen, Manibrata [3 ,4 ]
机构
[1] Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst, Fohringer Ring 6, D-80805 Munich, Germany
[2] Indian Inst Technol, Gauhati 781039, Assam, India
[3] Northwestern Univ, Dept Phys & Astron, 2145 Sheridan Rd, Evanston, IL 60208 USA
[4] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
基金
美国国家科学基金会;
关键词
Supernovae - Chemical elements - Charged particles;
D O I
10.1103/PhysRevLett.125.251801
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Neutrinos in a core-collapse supernova can undergo fast flavor conversions with a possible impact on the explosion mechanism and nucleosynthesis. We perform the first nonlinear simulations of fast conversions in the presence of three neutrino flavors. The recent supernova simulations with muon production call for such an analysis, as they relax the standard nu(mu,tau) = (nu) over bar (mu,tau) (two-flavor) assumption. Our results show the significance of muon and tau lepton number angular distributions, together with the traditional electron lepton number ones. Indeed, our three-flavor results are potentially very different from two-flavor ones. These results strengthen the need to further investigate the occurrence of fast conversions in supernova simulation data, including the degeneracy breaking of mu and tau neutrinos.
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页数:6
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