2024/09/10 by Nikolas Cruz-Camacho, Cruz-Camacho, Nikolas, Rajesh Kumar +13 · 1 citation
Earth and Planetary Sciences · Engineering · Physics and Astronomy · #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #High Energy Physics - Phenomenology (hep-ph) #High-pressure geophysics and materials #Hydrocarbon exploration and reservoir analysis #Nuclear Theory (nucl-th) #Quantum, superfluid, helium dynamics
paper · pdf · doi:10.48550/arxiv.2409.06837
openalex publication_date 2024/09/10 · openalex created_date 2024/10/22 · openalex updated_date 2026/07/28
In this paper we explore independently for the first time three chemical potentials (baryon μB, charged μQ, and strange μS) in the Chiral mean-field (CMF) model. We designed and implemented CMF++, a new version of the CMF model rewritten in C++ that is optimized, modular, and well-documented. CMF++ has been integrated into the MUSES Calculation Engine as a free and open source software module. The runtime improved in more than 4 orders of magnitude across all 3 chemical potentials, when compared to the legacy code. Here we focus on the zero temperature case and study stable, as well as metastable and unstable, vacuum, hadronic, and quark phases, showing how phase boundaries vary with the different chemical potentials. Due to the significant numerical improvements in CMF++, we can calculate for the first time high-order susceptibilities within the CMF framework to study the properties of the quark deconfinement phase transition. We found phases of matter that include a light hadronic phase, strangeness-dominated hadronic phase, and quark deconfinement within our μB, μS, μQ phase space. The phase transitions are of first, second (quantum critical point), and third order between these phases and we even identified a tricritical point.