| Автор | J Szabelski |
| Автор | J Wdowczyk |
| Автор | A W Wolfendale |
| Дата выпуска | 1989-12-01 |
| dc.description | One way of explaining the observed excess of cosmic-ray muons in the gamma -ray induced showers from the direction of Cygnus X-3 is to postulate a dramatic increase in the photonuclear cross section at energies above 10<sup>4</sup> GeV. Such a model is examined here. It is demonstrated that there are apparently no objections to such behaviour, and indeed further anomalies in cosmic-ray physics might be explainable in this way. |
| Формат | application.pdf |
| Издатель | Institute of Physics Publishing |
| Название | High-energy cosmic rays and the characteristics of photon-nucleus collisions |
| Тип | paper |
| DOI | 10.1088/0954-3899/15/12/013 |
| Electronic ISSN | 1361-6471 |
| Print ISSN | 0954-3899 |
| Журнал | Journal of Physics G: Nuclear and Particle Physics |
| Том | 15 |
| Первая страница | 1893 |
| Последняя страница | 1898 |
| Аффилиация | J Szabelski; Inst. of Nucl. Studies, Lodz, Poland |
| Аффилиация | J Wdowczyk; Inst. of Nucl. Studies, Lodz, Poland |
| Аффилиация | A W Wolfendale; Inst. of Nucl. Studies, Lodz, Poland |
| Выпуск | 12 |
