Phase Transition and Hybrid Star in a Nonlinear σ- ω model
S. Acharya, L. Maharana, R. Mohanty, P. K. Panda
Abstract
The phase transition between the nuclear matter and the quark matter is examined. The relativistic mean field theory(RMF) is consider with interacting nucleons and mesons using TM1 parameter set for the nuclear matter equations of state. It is found that the trasition point depends on coupling constant αs and bag pressure. From the study of the structure of a hybrid neutron star, it is observed that the star contains quark matter in the interior and neutron matter on the outer perifery.
Create a lesson
Related papers
Deconfinement and the Charge Susceptibility Matrix of QCD
Christopher Grace, Brady Mowbray, Christopher Plumberg
Separating entanglement at emission from femtoscopic correlations
Isaac Vidaña
Competitive constraints on exotic tensor currents from EC/β+ ratios
Victor Dumenil, Leendert Hayen
Comment on arXiv:2604.27678
V. A. Kizka
Impact of ab initio E1 strength on neutron capture rates along the nickel isotopic chain
Francesca Bonaiti, Joanna E. Sobczyk
Final-state centrality in relativistic heavy-ion simulations from neural networks
Anibal Bezerra, Fernando G. Gardim