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Updated: Jul 10, 2025

Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
Cosmic-void observations reconciled with primordial magnetogenesis
David N Hosking1,2,3,4, Alexander A Schekochihin5,6
1Oxford Astrophysics, Denys Wilkinson Building, Keble Road, Oxford, OX1 3RH, UK. dhosking@princeton.edu.
Early Universe magnetic fields from the electroweak phase transition (EWPT) are too weak. A new theory involving magnetic reconnection strengthens these relic fields, aligning them with observations and potentially resolving the Hubble tension.
Area of Science:
- Cosmology
- Astrophysics
- Particle Physics
Background:
- The intergalactic medium's weak magnetic field may originate from the early Universe.
- Standard models predict relic magnetic fields from the electroweak phase transition (EWPT) are too weak to explain observed phenomena like gamma-ray scattering from blazars.
Purpose of the Study:
- To propose a new mechanism for the decay of early Universe magnetic fields.
- To reconcile the EWPT-relic hypothesis with observational constraints.
- To investigate the potential of these relic fields to address cosmological puzzles like the Hubble tension.
Main Methods:
- Investigating turbulent magnetohydrodynamic decay.
- Proposing magnetic reconnection as the mediating process for field decay.
- Conserving the mean square fluctuation level of magnetic helicity during decay.
Main Results:
- The proposed theory predicts relic magnetic fields several orders of magnitude stronger than previously thought.
- This significant strengthening restores consistency between the EWPT-relic hypothesis and observational data.
- Efficient EWPT magnetogenesis can generate fields strong enough to impact recombination and seed galaxy-cluster fields.
Conclusions:
- Magnetic reconnection offers a viable pathway for preserving early Universe magnetic fields.
- The EWPT-relic hypothesis is strengthened by this new understanding of magnetic field decay.
- These stronger relic fields have implications for resolving the Hubble tension and understanding cosmic magnetic field origins.
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