We study the effects of strong magnetic fields in dense stellar matter within an effective relativistic equation of state with the inclusion of hyperons and Δ(1232)-isobar degrees of freedom. The effects of high magnetic field interactions significantly affect the nuclear equation of state and the macroscopic properties of the star. In this framework we investigate the role of the presence of the Δ-isobars degrees of freedom in structure and in the bulk properties of the compact star.

Effects of strong magnetic fields in dense stellar matter / Lavagno A.; Lingua F.. - STAMPA. - 9, Issue S302:(2013), pp. 439-440. [10.1017/S1743921314002695]

Effects of strong magnetic fields in dense stellar matter

LAVAGNO, Andrea;LINGUA, FABIO
2013

Abstract

We study the effects of strong magnetic fields in dense stellar matter within an effective relativistic equation of state with the inclusion of hyperons and Δ(1232)-isobar degrees of freedom. The effects of high magnetic field interactions significantly affect the nuclear equation of state and the macroscopic properties of the star. In this framework we investigate the role of the presence of the Δ-isobars degrees of freedom in structure and in the bulk properties of the compact star.
Proceedings of the International Astronomical Union
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Utilizza questo identificativo per citare o creare un link a questo documento: http://hdl.handle.net/11583/2591166
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