$Distribution function of nuclei from $\mathcal{e}^±$ scattering in the presence of a strong primordial magnetic field$

Distribution function of nuclei from $\mathcal{e}^±$ scattering in the presence of a strong primordial magnetic field

The amplitude of the primordial magnetic field (PMF) is constrained from observational limits on primordial nuclear abundances. Within this constraint, it is possible that nuclear motion is regulated by Coulomb scattering with electrons and positrons (e±s), while e±s are affected by a PMF rather tha...

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Veröffentlicht in:	Physical review. D 2021-12, Vol.104 (12)
Hauptverfasser:	Kusakabe, Motohiko, Kedia, Atul, Mathews, Grant J., Sasankan, Nishanth
Format:	Artikel
Sprache:	eng
Schlagworte:	ASTRONOMY AND ASTROPHYSICS big bang nucleosynthesis CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS evolution of the universe particle astrophysics primordial magnetic fields quantum statistical mechanics space and astrophysical plasma
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