Rotational susceptibility of a hot and dense hadronic matter: A possible probe of QCD phase transition
We study the effect of rotation and the consequent angular momentum fluctuations in a hadron resonance gas produced in ultra-relativistic heavy ion collisions. The rotational susceptibilities ($χ_{\rm ω}$, $χ^{2}_{\rm ω}$, etc.), which quantify how much the system responds to a small angular velocity, are estimated for the first time, considering that these can be valuable indicators of the QCD phase transition. The higher-order rotational susceptibilities and their ratios are estimated in the presence and absence of baryon chemical potential ($μ_{\rm B}$) in the system. The effect of particle spin ($s$) and rotational chemical potential ($ω$) on the fluctuation of the angular momentum is studied. To consider a more realistic scenario, the effect of interactions between hadrons is taken into account by considering van der Waals-like interactions, which include both attractive and repulsive interactions. A phase transition, absent in an ideal hadron gas model, can be observed in an interacting hadron gas model.
Authors
- Dushmanta Sahu (ORCID: https://orcid.org/0000-0001-8980-1362)
- R. Sahoo (ORCID: https://orcid.org/0000-0003-3334-0661)
- Kshitish Kumar Pradhan (ORCID: https://orcid.org/0000-0002-3224-7089)
- Bhagyarathi Sahoo (ORCID: https://orcid.org/0000-0003-3699-0598)
Publication Details
- Journal
- ArXiv.org
- Published
- 2025-07-04
- Primary Topic
- Pulsars and Gravitational Waves Research
- Type
- article
- Field-Weighted Citation Impact
- 0.00