| Texto completo | |
| Autor(es): |
Avancini, Sidney S.
;
Dexheimer, Veronica
;
Farias, Ricardo L. S.
;
Timoteo, Varese S.
Número total de Autores: 4
|
| Tipo de documento: | Artigo Científico |
| Fonte: | PHYSICAL REVIEW C; v. 97, n. 3, p. 8-pg., 2018-03-26. |
| Resumo | |
In this article, we calculate the magnetization and other thermodynamical quantities for strongly magnetized quark matter within the Nambu-Jona-Lasinio model at zero temperature. We assume two scenarios: chemically equilibrated charge neutral matter present in the interiors of compact stars and zero-strangeness isospin-symmetric matter created in nuclear experiments. We show that the magnetization oscillates with density but in a much more smooth form than what was previously shown in the literature. As a consequence, we do not see the unphysical behavior in the pressure in the direction perpendicular to the magnetic field that was previously found. Finally, we also analyze the effects of a vector interaction on our results. (AU) | |
| Processo FAPESP: | 16/07061-3 - Teorias efetivas em sistemas hadrônicos de poucos e muitos corpos |
| Beneficiário: | Varese Salvador Timoteo |
| Modalidade de apoio: | Auxílio à Pesquisa - Regular |