Intense magnetic field by twisted neutrinos beam in supernovae

被引：0

作者：

Pour, Reyhane Mohamadi ^{[1
]}

Sobhani, Hassan ^{[2
]}

Kermani, Hamid Arjomand ^{[1
]}

机构：

[1] Shahid Bahonar Univ Kerman, Fac Phys, Kerman, Iran

[2] Nucl Sci & Technol Res Inst NSTRI, Photon & Quantum Technol Res Sch, Tehran, Iran

来源：

EUROPEAN PHYSICAL JOURNAL A | 2022年 / 58卷 / 07期

关键词：

ORBITAL ANGULAR-MOMENTUM; ASTROPHYSICAL JETS; MAGNETODYNAMIC MECHANISM; GENERATION; ACCRETION; FLOWS; LIGHT; STAR;

D O I：

10.1140/epja/s10050-022-00776-w

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

The azimuthal and axial magnetic fields generated by the Laguerre-Gaussian neutrino beam in plasma are considered for the first time in this work. The generation of self-consistent azimuthal and axial magnetic fields by Ampere's law is a powerful mechanism that could be responsible for the supernovae magnetic fields. The neutrino beam with a doughnut shape profile is a better choice than a Gaussian profile to form and propagate jets. The azimuthal and axial magnetic fields generated by hollow neutrino beams can explain the formation and propagation of the jets. This result may be relevant to the understanding of the origin of magnetic fields and the acceleration of jets in astrophysics.

引用

页数：7

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