How primordial magnetic fields shrink galaxies
Sergio Martin-Alvarez, Adrianne Slyz, Julien Devriendt, Carlos, G\'omez-Guijarro

TL;DR
This study uses high-resolution cosmological simulations to investigate how primordial magnetic fields influence galaxy formation, revealing they can delay star formation, reduce disk size, and increase central gas concentration, especially with stellar feedback.
Contribution
The paper demonstrates, through simulations, that primordial magnetic fields significantly impact galaxy morphology and dynamics, highlighting magnetic braking and feedback interactions as key mechanisms.
Findings
Primordial magnetic fields delay star formation onset.
Magnetic fields reduce galactic disk size and angular momentum.
Effects are amplified with stellar feedback.
Abstract
As one of the prime contributors to the interstellar medium energy budget, magnetic fields naturally play a part in shaping the evolution of galaxies. Galactic magnetic fields can originate from strong primordial magnetic fields provided these latter remain below current observational upper limits. To understand how such magnetic fields would affect the global morphological and dynamical properties of galaxies, we use a suite of high-resolution constrained transport magneto-hydrodynamic cosmological zoom simulations where we vary the initial magnetic field strength and configuration along with the prescription for stellar feedback. We find that strong primordial magnetic fields delay the onset of star formation and drain the rotational support of the galaxy, diminishing the radial size of the galactic disk and driving a higher amount of gas towards the centre. This is also reflected in…
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