The study of hadronic rescattering on K<sup>∗0</sup> resonance yield in baryon-rich QCD matter
Abstract The effect of hadronic rescattering on K ∗0 resonance yield can be studied by measuring K ∗0 / K ratio as a function of centrality or multiplicity. This study investigates how the size of the system and the chemical composition (meson–meson versus meson–baryon interaction) of the matter formed in heavy-ion collisions impact the process of hadronic rescattering. It is shown that existing calculation of K ∗0 / K ratio, which considers the interaction of K ∗0 and K mesons with only light mesons in the hadronic medium (neglecting interactions with baryons), fails to explain the measured K ∗0 / K ratio at RHIC beam energy scan (BES) energies. To understand the multiplicity dependence of the K ∗0 / K ratio at RHIC BES and SPS energies ( <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:msqrt> <mml:mrow> <mml:msub> <mml:mrow> <mml:mi>s</mml:mi> </mml:mrow> <mml:mrow> <mml:mi mathvariant="italic">NN</mml:mi> </mml:mrow> </mml:msub> </mml:mrow> </mml:msqrt> </mml:math> < 20 GeV), the ultra relativistic quantum molecular dynamics (UrQMD) model is employed. UrQMD calculations suggest that for a given multiplicity, K ∗0 / K is more suppressed in Au+Au collision at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:msqrt> <mml:mrow> <mml:msub> <mml:mrow> <mml:mi>s</mml:mi> </mml:mrow> <mml:mrow> <mml:mi mathvariant="italic">NN</mml:mi> </mml:mrow> </mml:msub> </mml:mrow> </mml:msqrt> </mml:math> = 7.7 GeV, compared to that in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:msqrt> <mml:mrow> <mml:msub> <mml:mrow> <mml:mi>s</mml:mi> </mml:mrow> <mml:mrow> <mml:mi mathvariant="italic">NN</mml:mi> </mml:mrow> </mml:msub> </mml:mrow> </mml:msqrt> </mml:math> = 200 GeV. This is possibly because of formation different type of quantum chromodynamics medium at 200 and 7.7 GeV, and change in interaction cross-section between hadrons with change in particle type and energy.
Authors
- A. K. Sahoo (ORCID: https://orcid.org/0000-0003-4652-9850)
- Subhash Singha (ORCID: https://orcid.org/0000-0002-3952-3648)
- Md. Nasim (ORCID: https://orcid.org/0000-0003-1071-7630)
Institutions
- Chinese Academy of Sciences (CN)
- Indian Institute of Science Education and Research Berhampur (IN)
- Institute of Modern Physics (CN)
Publication Details
- Journal
- Journal of Physics G Nuclear and Particle Physics
- Published
- 2024-10-16
- DOI
- https://doi.org/10.1088/1361-6471/ad8768
- Citations
- 3
- Primary Topic
- High-Energy Particle Collisions Research
- Type
- article
- Field-Weighted Citation Impact
- 1.98