Measurements of neutrons in the Xe+CsI reaction by the Highly Granular Neutron Detector prototype in the BM@N experiment

19 Sept 2025, 09:20
20m
LHEP-215/NICA Hall - NICA Hall (VBLHEP)

LHEP-215/NICA Hall - NICA Hall

VBLHEP

35
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20 min. Projects NICA/MPD/SPD/BM@N at JINR Projects NICA/MPD/SPD/BM@N at JINR

Speaker

Zubankov, Aleksandr (Institute for Nuclear Research of the Russian Academy of Sciences)

Description

A Highly Granular time-of-flight Neutron Detector (HGND) is currently under development for use in the BM@N experiment to measure the yields and flow of neutrons with energies of 0.3–4 GeV [1]. The ratio of neutron to proton yields and the neutron-proton differential directed flow are sensitive to the contribution of symmetry energy to the equation of state of dense nuclear matter in Au-Au heavy ion collisions [2]. Such measurements in the BM@N experiment allow the equation of state (EoS) to be studied at a beam energy of 2.5-4A GeV, which is important for investigating the properties of astrophysical objects, such as neutron stars. Additionally, measuring the neutron energy spectra in projectile fragmentation enables estimation of the emitting source temperature [3].
To validate the concept of the full-scale HGND, a compact HGND prototype was constructed and tested in collisions of 3.8A GeV Xe with a CsI target at the BM@N experiment [4]. Neutron energy is reconstructed using the time-of-flight method individually in each cell. This configuration provides high neutron detection efficiency, good spatial resolution and time resolution of about 270 ps.
The HGND prototype was placed at 0 degrees to measure spectator neutrons and neutrons from electromagnetic dissociation (EMD). The reconstructed neutron kinetic energy spectra by time-of-flight are compared with the Geant4 modelling in the full geometry of the BM@N setup using the DCM-QGSM-SMM model and UrQMD-AMC model in Cascade mode and with Skyrme forces as heavy-ion collision generators and using the RELDIS model as EMD event generator. Neutron yields in the HGND prototype acceptance and cross-sections were obtained by correcting for model-estimated efficiencies for central and semi-central nuclear collisions and for EMD.

  1. F. Guber et al., Experiment. Instrum. Exp. Tech., 67, 447–456
    (2024).
  2. X.-X. Long, G.-F. Wei, Phys. Rev. C, 109, 054619 (2024).
  3. P. Pawłowski et al., Phys. Rev. C, 108, 044610 (2023).
  4. A. Zubankov et al., arXiv:2503.12624 [physics.ins-det] (2025).

Authors

Afanasiev, Sergei (JINR) Golubeva, Marina (INR RAS) Guber, Fedor (INR RAS, Moscow) Ivashkin, Alexander (INR RAS, Moscow) Karpushkin, Nikolay (INR RAS) Kutinova, O. Lyapin, Daniil Makhnev, Aleksandr (INR of RAS) Morozov, Sergey (Institute for Nuclear Research RAS) Parfenov, Peter (JINR, NRNU MEPhI) Plotnikov, Vassili Pshenichnov, Igor (Institute for Nuclear Research, Russian Academy of Sciences) Sakulin, Dmitriy (JINR) Mr Savenkov, Savva (MIPT, INR RAS) Shabanov, Arseniy (INR RAS) Sukhov, Evgeni (JINR) Svetlichnyi, Aleksandr (MIPT, INR RAS) Taer, Georgy Ustinov, Valentin (JINR VBLHEP) Zubankov, Aleksandr (Institute for Nuclear Research of the Russian Academy of Sciences)

Presentation materials