activity
20242026
most citedThermal fluctuations of matter composition and quark nucleation in compact stars

4 citations · 8 across the 5 of their papers we have counts for

collaborators

6 papers

nucl-th2026

Coexistence of strange quark stars and neutron stars: metastability and nucleation in proto-neutron stars

Mirco Guerrini, Giuseppe Pagliara, Luca Passarella +1

If strange quark matter (SQM) is absolutely stable, hadronic neutron stars (NSs) and strange quark stars (QSs) may coexist in the so-called two-families scenario. A key issue is ex…

nucl-th2026

Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis

Luca Passarella, Mirco Guerrini, Giuseppe Pagliara +2

Hadronic stars and strange quark stars could coexist within the so-called two-families scenario. In this respect, hadronic matter and strange quark matter correspond to two distinc…

astro-ph.HE2025

On the formation of strange quark stars from supernova in compact binaries

L. M. Becerra, F. Cipolletta, A. Drago +4

Strange quark stars (SQSs), namely compact stars entirely composed of deconfined quark matter, are characterized by similar masses and compactness to neutron stars (NSs) and have b…

nucl-th2025★ 3 cited

Framework for phase transitions between the Maxwell and Gibbs constructions at finite temperature

Constantinos Constantinou, Mirco Guerrini, Tianqi Zhao +2

The characteristics of the hadron-to-quark first-order phase transition differ depending on whether charge neutrality is locally or globally fulfilled. In -equilibrated matter,…

nucl-th2025★ 1 cited

Role of thermal fluctuations in nucleation of three-flavor quark matter

Mirco Guerrini, Giuseppe Pagliara, Andrea Lavagno +1

We present a framework that aims to investigate the role of thermal fluctuations of the matter composition and color-superconductivity in the nucleation of three-flavor deconfined…

nucl-th2024★ 4 cited

Thermal fluctuations of matter composition and quark nucleation in compact stars

Mirco Guerrini, Giuseppe Pagliara, Alessandro Drago +1

At the extreme densities reached in the core of neutron stars, it is possible that quark deconfined matter is produced. The formation of this new phase of strongly interacting matt…