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Determining the energy spectrum slope of diffuse superhigh-energy gamma radiation

T. S. YuldashbaevInstitute for Physics and Technology, Physics-Solar Research and Production Association, Uzbek Academy of Sciences, Tashkent, UzbekistanI I AbsalyamovaInstitute for Physics and Technology, Physics-Solar Research and Production Association, Uzbek Academy of Sciences, Tashkent, UzbekistanN.N. KulakhmedovInstitute for Physics and Technology, Physics-Solar Research and Production Association, Uzbek Academy of Sciences, Tashkent, UzbekistanKh. NuritdinovInstitute for Physics and Technology, Physics-Solar Research and Production Association, Uzbek Academy of Sciences, Tashkent, Uzbekistan
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We evaluate the primary gamma quanta (PGQ) energy spectrum slope at E γ > 1014 eV. To accomplish this, a new method based on analyzing the data obtained in high-mountain experiments with large-scale X-ray emulsion chambers (XECs) is used.

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