...
首页> 外文期刊>Astroparticle physics >An upper limit to the photon fraction in cosmic rays above 10(19) eV from the Pierre Auger Observatory
【24h】

An upper limit to the photon fraction in cosmic rays above 10(19) eV from the Pierre Auger Observatory

机译:皮埃尔·奥格天文台的宇宙射线中高于10(19)eV的光子分数的上限

获取原文
获取原文并翻译 | 示例
           

摘要

An upper limit of 16% (at 95% c.l.) is derived for the photon fraction in cosmic rays with energies greater than 10(19) eV, based on observations of the depth of shower maximum performed with the hybrid detector of the Pierre Auger Observatory. This is the first such limit on photons obtained by observing the fluorescence light profile of air showers. This upper limit confirms and improves on previous results from the Haverah Park and AGASA surface arrays. Additional data recorded with the Auger surface detectors for a subset of the event sample support the conclusion that a photon origin of the observed events is not favored. (c) 2006 Elsevier B.V. All rights reserved.
机译:根据皮埃尔·俄格天文台的混合探测器对最大淋浴深度的观察,得出能量大于10(19)eV的宇宙射线中光子分数的上限为16%(在95%cl处) 。这是通过观察空气喷淋的荧光轮廓获得的光子的第一个这样的限制。该上限证实并改善了Haverah Park和AGASA表面阵列的先前结果。用俄歇表面探测器记录的事件样本子集的其他数据支持这样的结论,即不赞成观察到的事件的光子起源。 (c)2006 Elsevier B.V.保留所有权利。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号