Abstract
Using the Geant4 code, we have performed a full-scale simulation of the LSD response to the neutrino burst from SN 1987A. The neutrino flux parameters were chosen according to one of the models: the standard collapse model or the rotational supernova explosion model. We showed that, depending on the chosen parameters, one can either obtain the required number of pulses in the detector or reproduce their energy spectrum, but not both together. The interaction of neutrino radiation both with LSD itself and with the material of the surrounding rock was taken into account in our simulation. We also explored the hypothesis that the entire unique LSD signal at 2:52 UT was produced by neutrino fluxes from the surrounding granite. However, this hypothesis was not confirmed by our simulation. The results obtained provide a rich material for possible interpretations.
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ACKNOWLEDGMENTS
This study was performed in 2019 and was essentially finished in early 2020, before the death of our coauthors A.S. Malgin and O.G. Ryazhskaya. We think their contribution to this study to be decisive and devote the paper to their memory with gratitude. We thank V.S. Imshennik and D.K. Nadyozhin, who has also passed away, for the useful discussions and sincere interest in this study. We are grateful to the referee whose remarks contributed significantly to an improvement of the text of our paper.
Funding
The work of A.V. Yudin was supported by the Russian Science Foundation (project no. 21-12-00061).
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Translated by V. Astakhov
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Manukovskiy, K.V., Yudin, A.V., Agafonova, N.Y. et al. Simulation of the LSD Response to the Neutrino Burst from SN 1987A. J. Exp. Theor. Phys. 134, 277–289 (2022). https://doi.org/10.1134/S1063776122030165
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DOI: https://doi.org/10.1134/S1063776122030165