RHIC $\sqrt{s_{NN}}=200$ GeV hadron yields and the isospin dependent equation of state

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Autori principali: Nana, Feyisola, Martín, Jordi Salinas San, Noronha-Hostler, Jacquelyn
Natura: Preprint
Pubblicazione: 2024
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author Nana, Feyisola
Martín, Jordi Salinas San
Noronha-Hostler, Jacquelyn
author_facet Nana, Feyisola
Martín, Jordi Salinas San
Noronha-Hostler, Jacquelyn
contents The statistical hadronization model has been successful in extracting information at chemical freeze-out in heavy-ion collisions. At RHIC, with a collision energy of $\sqrt{s_{NN}}=200$ GeV, many different ion species have been used for $A$+$A$ collisions. This allows for a scan across the charge fraction $Y_Q=Z/A$, where $Z$ is the proton number and $A$ is the baryon number. We first make predictions for $A$+$A$ collisions that do not yet have published experimental data on hadron yield ratios (O+O, Ru+Ru, Zr+Zr). We then use both the experimental and predicted yield ratios to perform thermal fits across $Y_Q$, enabling us to extract $s/n_B$ and other thermodynamic information at chemical freeze-out. Using the relation between $s/n_B$ and $Y_Q$, we can calculate a new constraint on the finite temperature equation of state at finite densities. We discuss implications of this constraint and propose future runs that can help connect to the equation of state relevant for neutron star mergers.
format Preprint
id arxiv_https___arxiv_org_abs_2411_03705
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle RHIC $\sqrt{s_{NN}}=200$ GeV hadron yields and the isospin dependent equation of state
Nana, Feyisola
Martín, Jordi Salinas San
Noronha-Hostler, Jacquelyn
Nuclear Theory
High Energy Physics - Phenomenology
The statistical hadronization model has been successful in extracting information at chemical freeze-out in heavy-ion collisions. At RHIC, with a collision energy of $\sqrt{s_{NN}}=200$ GeV, many different ion species have been used for $A$+$A$ collisions. This allows for a scan across the charge fraction $Y_Q=Z/A$, where $Z$ is the proton number and $A$ is the baryon number. We first make predictions for $A$+$A$ collisions that do not yet have published experimental data on hadron yield ratios (O+O, Ru+Ru, Zr+Zr). We then use both the experimental and predicted yield ratios to perform thermal fits across $Y_Q$, enabling us to extract $s/n_B$ and other thermodynamic information at chemical freeze-out. Using the relation between $s/n_B$ and $Y_Q$, we can calculate a new constraint on the finite temperature equation of state at finite densities. We discuss implications of this constraint and propose future runs that can help connect to the equation of state relevant for neutron star mergers.
title RHIC $\sqrt{s_{NN}}=200$ GeV hadron yields and the isospin dependent equation of state
topic Nuclear Theory
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2411.03705