The Problem of the Coplanarity of Energy Flows in EAS Cores
- Authors: Mukhamedshin R.A.1
-
Affiliations:
- Institute for Nuclear Research of the Russian Academy of Sciences
- Issue: Vol 88, No 5 (2025)
- Pages: 418-426
- Section: ЭЛЕМЕНТАРНЫЕ ЧАСТИЦЫ И ПОЛЯ. Эксперимент
- URL: https://journals.rcsi.science/0044-0027/article/view/364762
- DOI: https://doi.org/10.7868/S3034628225050048
- ID: 364762
Cite item
Abstract
The effect of the tendency towards the coplanar arrival of the most energetic particles and/or groups of particles in gamma–hadron families, observed in high-altitude and stratospheric experiments withX-ray emulsion chambers, is discussed. The experimental data are compared with calculations carried out within the framework of various versions of the FANSY 2.0 model, one of the versions of which reproduces the coplanar generation of the most energetic particles in hadron interactions at superhigh energies. The entire set of experimental data on the azimuthal characteristics ofg-ray−hadron families observed at levels of 25, 75, and 600 g/cm2 in the atmosphere cannot be explained even within the framework of the FANSY 2.0/2D model, which uses the hypothesis of a connection between coplanarity and the local 3D ↔ 2D evolution of the metric signature at ultrahigh energies.
Keywords
About the authors
R. A. Mukhamedshin
Institute for Nuclear Research of the Russian Academy of Sciences
Email: rauf_m@mail.ru
Moscow, Russia
References
- A. S. Borisov, K. V. Cherdyntseva, Z. M. Guseva, V. G. Denisova, A. M. Dunaevsky, E. A. Kanevskaya, V. M. Maximenko, R. A. Nam, V. S. Puchkov, S. A. Slavatinsky, M. D. Smirnova, Yu. A. Smorodin, A. V. Uryson, N. G. Zelevinskaya, M. V. Zimin, G. B. Zhdanov, et al. (Pamir Collab.), in Proceedings of the 4th ISVHECRI (Beijing, 1986), p. 429.
- A. S. Borisov, Z. M. Guseva, V. G. Denisova, S. A. Karpova, V. M. Maksimenko, V. S. Puchkov, S. A. Slavatinsky, Yu. A. Smorodin, and R. A. Mukhamedshin, in Proceedings of the 8th ISVHECRI (Tokyo, 1994), p. 49.
- V. V. Kopenkin, A. K. Managadze, I. V. Rakobolskaya, and T. M. Roganova, Phys. Rev. D 52, 2766 (1995); doi: https://doi.org/10.1103/PhysRevD.52.2766
- Pamir Collab., Preprint INP MSU no 89-67/144 (1989).
- A. S. Borisov, R. A. Mukhamedshin, V. S. Puchkov, S. A. Slavatinsky, and G. B. Zhdanov, Nucl. Phys. B Proc. Suppl. 97, 118 (2001); doi: 10.1016/S0920-5632(01)01209-9
- A. V. Apanasenko, N. A. Dobrotin, L. A. Goncharova, K. A. Kotelnikov, and N. G. Polukhina, in Proceedings of the 15th ICRC (Plovdiv, 1977), Vol. 7, p. 220.
- V. I. Osedlo, I. V. Rakobolskaya, V. I. Galkin, A. K. Managadze, L. G. Sveshnikova, L. A. Goncharova, K. A. Kotelnikov, A. G. Martynov, and N. G. Polukhina, in Proceedings of the 27th ICRC (Hamburg, 2001), Vol. 1, p. 1426.
- J. N. Capdevielle, J. Phys. G 14, 503 (1988); doi: 10.1088/0305-4616/14/4/012
- R. Attallah, J. N. Capdevielle, and M. C. Talai, J. Phys. G 31, 909 (2005); doi: 10.1088/0954-3899/31/5/008
- R. A. Mukhamedshin, JHEP 0505, 049 (2005); doi: 10.1134/S1547477106040030
- R. A. Mukhamedshin, Nucl. Phys. B Proc. Suppl. 196C, 98 (2009); doi: 10.1016/j.nuclphysbps.2009.09.016
- А. К. Манагадзе, Р. А. Мухамедшин, Изв. РАН. Cер. физ. 77, 1573 (2013) [A. K. Managadze and R. A. Mukhamedshin, Bull. Russ. Acad. Sci.: Phys. 77, 1315 (2013); doi: 10.3103/S106287381311021X].
- T. Wibig, hep-ph/0003230.
- I. I. Royzen, Mod. Phys. Lett. A 9, 3517 (1994); doi: 10.1142/S021773239400335X
- J. N. Capdevielle, Nucl. Phys. B Proc. Suppl. 175, 137 (2008); doi: 10.1016/j.nuclphysbps.2007.10.022
- T. S. Yuldashbaev, Kh. Nuritdinov, and V. M. Chudakov, Nuovo Cimento C 24, 569 (2001).
- R. A. Mukhamedshin, Nucl. Phys. B Proc. Suppl. 75A, 131 (1999).
- L. Anchordoqui, D. C. Dai, M. Fairbairn, G. Landsberg, and D. Stojkovic, Mod. Phys. Lett. A 27, 1250021 (2012); doi: 10.1142/S0217732312500216
- D. Stojkovic, arXiv: 1406.2696v1 [gr-qc].
- E. Lyndon and P. Bryant, J. Instrum. 3, S08001 (2008); doi: 10.1088/1748-0221/3/08/S08001
- R. A. Mukhamedshin, Eur. Phys. J. C 79, 441 (2019); doi: 10.1140/epjc/s10052-019-6931-0
- R. A. Mukhamedshin, Eur. Phys. J. Plus. 134, 584 (2019); doi: 10.1140/epjp/i2019-12933-2
- R.A. Mukhamedshin, Eur. Phys. J. C 82, 155 (2022); doi: 10.1140/epjc/s10052-022-10082-w
- Р. А. Мухамедшин, Изв. РАН. Сер. физ. 85, 534 (2021) [R. A. Mukhamedshin, Bull. Russ. Acad. Sci.: Phys. 85, 402 (2021); doi: 10.3103/S1062873821040237].
- R. A. Mukhamedshin, Eur. Phys. J. С 60, 345 (2009); doi: 10.1140/epjc/s10052-009-0945-y
- J. Kempa, R. Mukhamedshin, and M. Tamada, J. Phys.: Conf. Ser. 409, 012109 (2013); doi: 10.1088/1742-6596/409/1/012109
- A. M. Dunaevsky, S. V. Pashkov, and S. A. Slavatinsky, in Proceedings of the 18th ICRC (Bangalore, India, 1983); Vol. 5, p. 449.
Supplementary files


