Study of the effect of neutrino oscillation on the supernova neutrino signal with the LVD detector

被引:3
作者
Aglietta, M [1 ]
Antonioli, P
Bari, G
Castagnoli, C
Fulgione, W
Galeotti, P
Garbini, M
Ghis, PL
Giusti, P
Kemp, E
Malguin, AS
Menghetti, H
Pesci, A
Pless, IA
Porta, A
Ryasny, VG
Ryazhskaya, OG
Saavedra, O
Sartorelli, G
Selvi, M
Vigorito, C
Vissani, F
Votano, L
Yakushev, VF
Zatsepin, GT
Zichichi, A
机构
[1] Univ Turin, Inst Phys Interplanetary Space, IFSI, CNR, Turin, Italy
[2] Ist Nazl Fis Nucl, I-10125 Turin, Italy
[3] Univ Bologna, Bologna, Italy
[4] Ist Nazl Fis Nucl, I-40126 Bologna, Italy
[5] Univ Campinas, Campinas, Brazil
[6] Russian Acad Sci, Inst Nucl Res, Moscow, Russia
[7] MIT, Cambridge, MA 02139 USA
[8] Ist Nazl Fis Nucl, LNGS, Assergi, Italy
[9] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy
关键词
D O I
10.1016/j.nuclphysbps.2004.11.029
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We present an update of our previous study [1] on how nu oscillations affect the signal from a supernova core collapse observed in the LVD detector at LNGS. In this paper we use a recent, more precise determination of the cross section [2] to calculate the expected number of inverse beta decay events; we introduce in the simulation also the nu-Fe interactions; we include the Earth matter effects; and finally we study also the inverted mass hierarchy case.
引用
收藏
页码:115 / 118
页数:4
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