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> &lt; 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.

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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
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article

The study of hadronic rescattering on K∗0 resonance yield in baryon-rich QCD matter

A. K. Sahoo, Subhash Singha, Md. Nasim
3 citations
Journal of Physics G Nuclear and Particle Physics
High-Energy Particle Collisions Research
1.98
article

The study of hadronic rescattering on K∗0 resonance yield in baryon-rich QCD matter

A. K. Sahoo, Subhash Singha, Md. Nasim
article en
3 citations

Abstract

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> &lt; 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.

Journal of Physics G Nuclear and Particle PhysicsVol. 52(1)
Chinese Academy of Sciences (CN), Indian Institute of Science Education and Research Berhampur (IN), Institute of Modern Physics (CN)
Openalex Percentile: Top 9%
High-Energy Particle Collisions Research
1.98
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