2014/09/22 by Débora P. Menezes, Marcus Benghi Pinto, Marcus B. Pinto +4
Mathematics · Physics and Astronomy · #Cold Atom Physics and Bose-Einstein Condensates #High-Energy Particle Collisions Research #Loop (graph theory) #Magnetic field #Mathematics #Particle physics #Phase (matter) #Phase diagram #Physics #Position (finance) #Pulsars and Gravitational Waves Research #Quantum electrodynamics #Quantum mechanics #Quark #Strange matter #Subject matter #Theoretical physics #hep-ph #nucl-th
paper · pdf · doi:10.1088/1742-6596/630/1/012026
published in Journal of Physics Conference Series 630, 012026 (IOP Publishing) · Talk given at the "XXXVII Brazilian Meeting on Nuclear Physics (XXXVII RTFNB)", Maresias, SP, Brazil, 8-12 September 2014
arxiv created 2014/09/22 · openalex publication_date 2015/07/15 · arxiv updated 2015/08/10 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
In the present work we are interested in understanding various properties of quark matter subject to strong magnetic fields described by the Nambu-Jona-Lasinio model with Polyakov loop. We start by analysing the differences arising from two different vector interactions in the Lagrangian densities, at zero temperature, and apply the results to stellar matter. We then investigate the position of the critical end point for different chemical potential and density scenarios.