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

T.K. Kuo and J.T. Pantaleone, Rev. Mod. Phys. 61

1989

Earlier work this paper cites.

S. Pastor and G. Raffelt, Phys. Rev. Lett. 89

2002

Earlier work this paper cites.

H. Duan, G.M. Fuller and Y.Z. Qian, Phys. Rev. D 74

2006

Earlier work this paper cites.

S. Hannestad, G.G. Raffelt, G. Sigl and Y.Y.Y. Wong, Phys. Rev. D 74

2007

Earlier work this paper cites.

H. Duan, G.M. Fuller, J. Carlson and Y.-Z. Quian, Phys. Rev. Lett. 99

2007

Cited alongside, same era.

A. Esteban-Pretel, S. Pastor, R. Tomas, G.G. Raffelt and G. Sigl, Phys. Rev. D 76

2007

Cited alongside, same era.

G.L. Fogli, E. Lisi, A. Marrone, and A. Mirizzi, JCAP 12

2007

Cited alongside, same era.

G.G. Raffelt and A.Y. Smirnov, Phys. Rev. D 76

2007

Cited alongside, same era.

G.G. Raffelt, astro-ph/0701677

Cited in the paper.

H. Duan, G.M. Fuller and J. Carlson, arXiv:0803.3650 [astro-ph]

Original

Cited in the paper.

J. Gava and C. Volpe, arXiv:0807.3418 [astro-ph]

Original

Cited in the paper.

With respect to Foglilast , 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 Foglilast are, however, negligible

Cited in the paper.

Note that, for no ν ¯ \overline{\nu} spectral split ( J ¯ l = 0 \overline{J}_{l}=0 ), one recovers from Eq. ( 11

Cited in the paper.

Multi-angle simulations appear to suppress nonadiabatic features emerging at single-angle, such as the bipolar oscillations (see Foglilast ) and the ν ¯ \overline{\nu} split (see Foglilast and this work)

Original

Cited in the paper.

H. Duan, G.M. Fuller and Y.-Z. Qian, Phys. Rev. D 76

2007

Later among the works it cites.

G.G. Raffelt and A.Y. Smirnov, Phys. Rev. D 76

2008

Closest in time.

B. Dasgupta and A. Dighe, Phys. Rev. D 77

2008

Closest in time.