A new calculation of atmospheric neutrino flux: The FLUKA approach

被引：9

作者：

Battistoni, G

Bloise, C

Cavalli, D

Ferrari, A

Montaruli, T

Rancati, T

Resconi, S

Ronga, F

Sala, PR

机构：

[1] Ist Nazl Fis Nucl, I-20133 Milan, Italy

[2] Univ Milan, Dipartimento Fis, I-20133 Milan, Italy

[3] Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Roma, Italy

[4] Univ Bari, I-70126 Bari, Italy

[5] Ist Nazl Fis Nucl, Dipartimento Fis Bari, I-70126 Bari, Italy

来源：

NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS | 1999年 / 70卷

关键词：

D O I：

10.1016/S0920-5632(98)00451-4

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：

Preliminary results from a full 3-D calculation of atmospheric neutrino fluxes using the FLUKA interaction model are presented and compared to previous existing calculations. This effort is motivated mainly by the 3-D capability and the satisfactory degree of accuracy of the hadron-nucleus models embedded in the FLUKA code. Here we show examples of benchmarking tests of the model with cosmic ray experiment results. A comparison of our calculation of the atmospheric neutrino flux with that of the Bartol group, for E-nu > 1 GeV, is presented.

引用

页码：358 / 360

页数：3

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