How unequal fluxes of high energy astrophysical neutrinos and antineutrinos can fake new physics (2016)
- Authors:
- Autor USP: FUNCHAL, RENATA ZUKANOVICH - IF
- Unidade: IF
- Subjects: BÓSON DE HIGGS; NEUTRINOS
- Language: Inglês
- Imprenta:
-
ABNT
NUNOKAWA, Hiroshi e PANES, Boris e FUNCHAL, Renata Zukanovich. How unequal fluxes of high energy astrophysical neutrinos and antineutrinos can fake new physics. . São Paulo: Instituto de Física, Universidade de São Paulo. Disponível em: https://arxiv.org/pdf/1604.08595.pdf. Acesso em: 01 jun. 2024. , 2016 -
APA
Nunokawa, H., Panes, B., & Funchal, R. Z. (2016). How unequal fluxes of high energy astrophysical neutrinos and antineutrinos can fake new physics. São Paulo: Instituto de Física, Universidade de São Paulo. Recuperado de https://arxiv.org/pdf/1604.08595.pdf -
NLM
Nunokawa H, Panes B, Funchal RZ. How unequal fluxes of high energy astrophysical neutrinos and antineutrinos can fake new physics [Internet]. 2016 ;[citado 2024 jun. 01 ] Available from: https://arxiv.org/pdf/1604.08595.pdf -
Vancouver
Nunokawa H, Panes B, Funchal RZ. How unequal fluxes of high energy astrophysical neutrinos and antineutrinos can fake new physics [Internet]. 2016 ;[citado 2024 jun. 01 ] Available from: https://arxiv.org/pdf/1604.08595.pdf - Majorana neutrinos: a phenomenological analysis
- Estudo do processo 'e POT.+'' POT.-''seta' 'W POT.+'' W POT-' num modelo com 4 neutrinos de Majorana
- Testing flavor changing neutrino interactions in long baseline experiments
- CP violation in vacuum neutrino oscillation experiments
- On the quest for the dynamics of ''nu' IND.'mü'' -> ''nu' IND.'tau'' conversion
- Flavor changing solution for atmospheric neutrino anomaly
- Gravitationally induced long-wavelenght oscillation solution to the solar neutrino problem
- Probing the LSND mass scale and four neutrino scenarios with a neutrino telescope
- Constraining the absolute neutrino mass scale and Majorana CP violating phases by future O'nu''beta''beta' decay experiments
- Measuring the spectras of high energy neutrinos with a kilometer-scale neutrino telescope
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