Low-energy spectral features of supernova (anti)neutrinos in inverted hierarchy

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 78, Issue 9, 2008, Pages

  Fogli, G L ^a,b   Lisi, E ^b   Marrone, A ^a,b   Mirizzi, A ^b,c   Tamborra, I ^a,b  

^a UNIVERSITY OF BARI   (Italy)

^b INFN SEZIONE DI BARI   (Italy)

^c MAX PLANCK INSTITUT FÜR PHYSIK   (Germany)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 56249129708     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.78.097301     Document Type: Article

References (19)

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14. With respect to, in Fig. 2 we have used 100 energy modes (instead of 60) and a 250 km radial range (instead of 200 km); the resulting differences with the analogous Fig. 5 of are, however, negligible.
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17. Note that, for no ν̄ spectral split (J̄l=0), one recovers from Eq. 11 the "sum rule" Jh=J̄.
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19. Multiangle simulations appear to suppress nonadiabatic features emerging at single-angle, such as the bipolar oscillations (see) and the ν̄ split (see and this work).