Spatial distribution of Cherenkov light from cascade showers in water


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Abstract

The spatial distribution of the Cherenkov light generated by cascade showers is analyzed using the NEVOD Cherenkov water detector. The dependence of the Cherenkov light intensity on the depth of shower development at various distances from the shower axis is investigated for the first time. The experimental data are compared with the Cherenkov light distributions predicted by various models for the scattering of cascade particles.

About the authors

V. A. Khomyakov

National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Author for correspondence.
Email: VAKhomyakov@mephi.ru
Russian Federation, Kashirskoe sh. 31, Moscow, 115409

A. G. Bogdanov

National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: VAKhomyakov@mephi.ru
Russian Federation, Kashirskoe sh. 31, Moscow, 115409

V. V. Kindin

National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: VAKhomyakov@mephi.ru
Russian Federation, Kashirskoe sh. 31, Moscow, 115409

R. P. Kokoulin

National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: VAKhomyakov@mephi.ru
Russian Federation, Kashirskoe sh. 31, Moscow, 115409

A. A. Petrukhin

National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: VAKhomyakov@mephi.ru
Russian Federation, Kashirskoe sh. 31, Moscow, 115409

S. S. Khokhlov

National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: VAKhomyakov@mephi.ru
Russian Federation, Kashirskoe sh. 31, Moscow, 115409

V. V. Shutenko

National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: VAKhomyakov@mephi.ru
Russian Federation, Kashirskoe sh. 31, Moscow, 115409

I. I. Yashin

National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)

Email: VAKhomyakov@mephi.ru
Russian Federation, Kashirskoe sh. 31, Moscow, 115409

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