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Dawn of the dark : Unified dark sectors and the EDGES Cosmic Dawn 21-cm signal

Yang, W. (author)
Pan, S. (author)
Vagnozzi, Sunny (author)
Stockholms universitet,KTH,Nordic Institute for Theoretical Physics NORDITA,Kavli Institute for Cosmology (KICC), Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, United Kingdom; Oskar Klein Centre for Cosmoparticle Physics, Stockholm University, Roslagstullsbacken 21A, Stockholm, SE-106 91, Sweden,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC),Nordiska institutet för teoretisk fysik (Nordita)
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Valentino, E. D. (author)
Mota, D. F. (author)
Capozziello, S. (author)
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 (creator_code:org_t)
2019-11-28
2019
English.
In: Journal of Cosmology and Astroparticle Physics. - : Institute of Physics Publishing. - 1475-7516. ; 2019:11
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • While the origin and composition of dark matter and dark energy remains unknown, it is possible that they might represent two manifestations of a single entity, as occurring in unified dark sector models. On the other hand, advances in our understanding of the dark sector of the Universe might arise from Cosmic Dawn, the epoch when the first stars formed. In particular, the first detection of the global 21-cm absorption signal at Cosmic Dawn from the EDGES experiment opens up a new arena wherein to test models of dark matter and dark energy. Here, we consider generalized and modified Chaplygin gas models as candidate unified dark sector models. We first constrain these models against Cosmic Microwave Background data from the Planck satellite, before exploring how the inclusion of the global 21-cm signal measured by EDGES can improve limits on the model parameters, finding that the uncertainties on the parameters of the Chaplygin gas models can be reduced by a factor between 1.5 and 10. We also find that within the generalized Chaplygin gas model, the tension between the CMB and local determinations of the Hubble constant H0 is reduced from ≈ 4σ to ≈ 1.3σ. In conclusion, we find that the global 21-cm signal at Cosmic Dawn can provide an extraordinary window onto the physics of unified dark sectors. 

Subject headings

NATURVETENSKAP  -- Fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences (hsv//eng)

Keyword

Cosmological parameters from CMBR
cosmological simulations
dark energy theory
dark matter theory

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ref (subject category)
art (subject category)

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