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Observational constraints on Dark Matter models

by Eric Armengaud

Submission summary

Authors (as registered SciPost users): Eric Armengaud
Submission information
Preprint Link: scipost_202510_00019v1  (pdf)
Date submitted: Oct. 10, 2025, 9:23 p.m.
Submitted by: Eric Armengaud
Submitted to: SciPost Physics Lecture Notes
 for consideration in Collection:
Ontological classification
Academic field: Physics
Specialties:
  • Gravitation, Cosmology and Astroparticle Physics
Approaches: Experimental, Observational

Abstract

In this short course, which complements the lecture on Dark Matter alternatives, I provide concrete examples of how Dark Matter (DM) models can be tested, whether for generic DM properties, or specific scenarios. First, I review searches for WIMPs, one of the most well-studied DM candidates. I also showcase some constraints on DM models that predict a modification of the cosmological matter power spectrum at high k. To this end, I focus primarily on bounds derived from the Lyman-αforest observations, which I will present in a brief overview beforehand.

Current status:
In refereeing

Reports on this Submission

Report #2 by Anonymous (Referee 2) on 2026-1-11 (Contributed Report)

Disclosure of Generative AI use

The referee discloses that the following generative AI tools have been used in the preparation of this report:

Used to refine grammar of report

Report

In this lecture note, the author gives a short summary of how observations constrain Dark Matter models, including the detection of Weakly Interacting Massive Particles (WIMPs) and the associated challenges, in addition to the Lyman-$\alpha$ forest as a cosmological probe of the power spectrum and its constraints on Dark Matter models.

The goal of this lecture note is to give readers a brief overview of the current major efforts on the search for Dark Matter evidence and the reasons that some of these efforts, i.e. search for WIMPs, have so far been to no avail. The lecture note also includes a self-contained summary on the Lyman-$\alpha$ forest cosmological probe, where the features are produced by absorption of Lyman-$\alpha$ by neutral hydrogen at 1215A, which further defines the power spectrum through statistical fluctuations. The observed power spectrum is used to exclude Dark Matter candidates or constrain Dark Matter properties.

In short, the manuscript is well-structured and has the necessary details to present itself as a concise lecture note. I recommend this manuscript for publication in SciPost Physics Lecture Notes.

Recommendation

Publish (meets expectations and criteria for this Journal)

  • validity: -
  • significance: -
  • originality: -
  • clarity: -
  • formatting: -
  • grammar: -

Report #1 by Anonymous (Referee 1) on 2026-1-6 (Invited Report)

Strengths

The paper does a wonderful job in explaining few of the novel methods used to detect dark matter, with the key focus being the Lyman-alpha probe for detecting dark matter. The author first highlights the current experiments, both direct and indirect means of detection, which are in use for dark matter detection. These experiments rule out models for dark matter by putting constraints. The paper then steadily develops towards using the matter power spectrum and the Lyman-alpha forest to further constrain the dark matter space, proving its usefulness for a range of masses of dark matter.

Weaknesses

None

Report

The acceptance criteria of the journal are well met. The report is compact, yet highlights key details about the probes used to detect dark matter.

There are a few typos that could be fixed before publishing, such as a spelling error for 'modelling' in line 213, and removing an additional bracket in the expression for 'zeta' in line 219.

Requested changes

A spelling error for 'modelling' in line 213, and removing an additional bracket in the expression for 'zeta' in line 219.

Recommendation

Publish (surpasses expectations and criteria for this Journal; among top 10%)

  • validity: top
  • significance: high
  • originality: top
  • clarity: top
  • formatting: perfect
  • grammar: excellent

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