Resumen
Using appropriate QCD finite energy sum rules, we discuss the influence of an external magnetic field and baryonic density on the axial-vector coupling constant gA. This scenario corresponds to a magnetar environment. We found that gA decreases both as function of the magnetic field strength and the baryonic density. It turns out that at the nuclear density ρ0 the axial-vector coupling takes the value gA⁎≈0.92. Although gA decreases in general with the magnetic field intensity, gA⁎ does not change in a relevant way with the magnetic field.
Idioma original | Inglés |
---|---|
Páginas (desde-hasta) | 43-47 |
Número de páginas | 5 |
Publicación | Nuclear and Particle Physics Proceedings |
Volumen | 343 |
DOI | |
Estado | Publicada - 2024 |
Nota bibliográfica
Publisher Copyright:© 2023 Elsevier B.V.
Áreas temáticas de ASJC Scopus
- Física nuclear y de alta energía