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SUMMARY:Investigation of spectator-driven effects on anisotropic flow form
 ation at the NICA energy range
DTSTART;VALUE=DATE-TIME:20261028T070000Z
DTEND;VALUE=DATE-TIME:20261028T071500Z
DTSTAMP;VALUE=DATE-TIME:20261102T005257Z
UID:indico-contribution-6289@cern.ch
DESCRIPTION:Speakers: Nikita Bikmetov (JINR)\nAnisotropic flow is a fundam
 ental observable in relativistic heavy-ion collisions that describes the a
 nisotropy in the azimuthal distribution of emitted particles. It develops 
 mainly due to pressure gradients generated during the early stages of the 
 collision\, which transform the spatial anisotropy of the initial overlap 
 region into momentum anisotropy of the final-state particles. In the energ
 y range of NICA complex\, due to longer passge time\, spectators can stron
 gly influence the observed flow through interactions with emitted particle
 s.\nIn this work\, we study the influence of spectator matter on anisotrop
 ic flows in Ag+Ag\, Au+Au\, Xe+Xe\, and U+U collisions at (\\sqrt{s_{NN}}=
 2.4)–4.5 GeV using a modern transport model. Calculations with and witho
 ut spectator propagation are compared for different particle species\, col
 lision energies\, and centralities to estimate the spectator contribution 
 to the directed (v1)\, elliptic (v2)\, triangular (v3)\, and quadrangular 
 (v4) flow coefficients.\n\nhttps://indico.particle.mephi.ru/event/626/cont
 ributions/6289/
LOCATION: Conference Hall 2
URL:https://indico.particle.mephi.ru/event/626/contributions/6289/
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