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Chern-Simmons electrodynamics and torsion dark matter axions

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arxiv 2404.13517 v1 pith:JPIRYYQ5 submitted 2024-04-21 hep-ph astro-ph.HEhep-th

classification hep-phastro-ph.HEhep-th
keywords darktorsionmagneticaxialaxionaxionsapproximateddamping
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abstract

In this paper, we delve into the influence of torsion axial pseudo vector on dark photons in an axion torsionic background, as investigated previously by Duncan et al[ Nucl Phys B 387:215 (1992)]. Notably, axial torsion, owing to its significantly greater mass compared to axions, gives rise to magnetic helicity in torsionful Chern-Simons (CS) electrodynamics, leading to the damping of magnetic fields. In QCD scale the damping from dark massive photons leads us to obtain a magnetic field of $10^{-8}$ Gauss, which is approximated the order of magnitude of magnetic fields at present universe. This result is obtained by considering that torsion has the value of the 1 MeV at the early universe, and can be improved to the higher value of $10^{-3}$ Gauss when the axial torsion 0-component is given by $10^{8}$ MeV and the mass of dark photon is approximated equal to the axion. The axion plays a crucial role in achieving CS dynamo action arising from axions. This study is useful in deepening our understanding of fundamental physics, from nuclear interactions to the nature of dark matter.

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  1. Reheating chiral dynamos with spin-0 and massive spin-1 torsions via chiral asymmetry

    astro-ph.CO 2025-02 reject novelty 4.0 of 10

    Adding a constant torsion trace to the chiral dynamo equation produces exponential magnetic growth with a sign set by torsion chirality, but the supporting equations and headline field strengths are not reliable.

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