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Article overview
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Observing primordial magnetic fields through Dark Matter | Sabir Ramazanov
; Federico R. Urban
; Alexander Vikman
; | Date: |
7 Oct 2020 | Abstract: | Primordial magnetic fields are often thought to be the early Universe seeds
that have bloomed into what we observe today as galactic and extra-galactic
magnetic fields. Owing to their minuscule strength, primordial magnetic fields
are very hard to detect in cosmological and astrophysical observations. We show
how this changes if a part of neutral Dark Matter has a magnetic
susceptibility. In this way, by studying Dark Matter one can obtain information
about the properties of primordial magnetic fields, even if the latter have a
comoving amplitude $B_0 lesssim0.01~mbox{nG}$. In our model Dark Matter is a
stable singlet scalar $chi$, which interacts with electromagnetism through the
Rayleigh operator as $chi^2 F_{mu
u} F^{mu
u}/Lambda^2$. For primordial
magnetic fields present in the early Universe this operator forces the
$Z_2$-symmetry of the model to be spontaneously broken. Later, when the
primordial magnetic field redshifts below a critical value, the symmetry is
restored through an "inverse phase transition". At that point the field $chi$
begins to oscillate and acts as a "magnetomorphic" Dark Matter component,
inheriting the properties of the primordial magnetic field space distribution.
In particular, for a nearly flat spectrum of magnetic field fluctuations, the
scalar $chi$ carries a emph{statistically anisotropic isocurvature mode}. We
discuss the parameter space of the model and consider the possibility that the
bulk of the Dark Matter is composed of the same particles $chi$ produced via
the freeze-in mechanism. | Source: | arXiv, 2010.03383 | Services: | Forum | Review | PDF | Favorites |
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