Unphysical properties in a class of interacting dark energy models
Unphysical properties in a class of interacting dark energy models
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Models with non-gravitational interactions between the dark matter and dark energy components are an alternative to the standard cosmological scenario. These models are characterized by an interaction term, and a frequently used parameterization is \(Q = 3\xi H \rho_{x}\), where \(H\) is the Hubble parameter and \(\rho_{x}\) is the dark energy dens...
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Unphysical properties in a class of interacting dark energy models
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TN_cdi_proquest_journals_2296985659
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2296985659
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E-ISSN
2331-8422
DOI
10.48550/arxiv.1909.10336
