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title: "An Alternative Method to Solve the Hadronic Cosmic-Ray Diffusion Equations. The Muon and Neutrino Fluxes • CBPF Index"
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**Nota de Física****Publicado**

# **An Alternative Method to Solve the Hadronic Cosmic-Ray Diffusion Equations. The Muon and Neutrino Fluxes**

**H. M. Portella; F.M.O. Castro; N. Amato; R. H. C. Maldonado**

1992

[**Descargar PDF **0,3 MB](https://index.cbpf.br/files/publicacao/6ad2a767639f62b11adbb66b/pdf) [**Contactar al responsable**](mailto:apub@cbpf.br?subject=An%20Alternative%20Method%20to%20Solve%20the%20Hadronic%20Cosmic-Ray%20Diffusion%20Equations.%20The%20Muon%20and%20Neutrino%20Fluxes)

## **Datos de la publicación**

<dl>

<dt>Autores</dt>
<dd>H. M. Portella; F.M.O. Castro; N. Amato; R. H. C. Maldonado</dd>

<dt>Tipo</dt>
<dd>Nota de Física</dd>

<dt>Estado</dt>
<dd>Publicado</dd>

<dt>Fecha de publicación</dt>
<dd>1992</dd>

<dt>Descripción</dt>
<dd>The integro-differential equations which describe the diffusion of the hadronic component in the atmosphere are solved exactly using the successive approximation method and we derived the numbers of the produced muons and neutrinos from the hadron fluxes obtained as the solution of the above equations. The primary cosmic ray spectrum used in our calculation is presented in a general form G(E).</dd>

<dt>Año</dt>
<dd>1992</dd>

<dt>Número</dt>
<dd>CBPF-NF-043/92</dd>

<dt>Vínculo con tesis</dt>
<dd>No</dd>

<dt>Vínculo con beca</dt>
<dd>No</dd>

</dl>

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