We consider a model of dark matter fluid based on a sector of Horndeski gravity. The model is very successful, at the background level, in reproducing the evolution of the Universe from early times to today. However, at the perturbative level the model fails. To show this, we use the code hi_class and we compute the matter power spectrum and the cosmic microwave background spectrum. Our results confirm, in a new and independent way, that this sector of Horndeski gravity is not viable to describe dark matter, in agreement with the recent constraints coming from the measurement of the speed of gravitational waves obtained from the observation of the neutron star merger event GW170817.
Testing Horndeski gravity as dark matter with hi_class / Casalino, A.; Rinaldi, M.. - In: PHYSICS OF THE DARK UNIVERSE. - ISSN 2212-6864. - STAMPA. - 2019:23(2019).
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Titolo: | Testing Horndeski gravity as dark matter with hi_class |
Autori: | Casalino, A.; Rinaldi, M. |
Autori Unitn: | |
Titolo del periodico: | PHYSICS OF THE DARK UNIVERSE |
Anno di pubblicazione: | 2019 |
Numero e parte del fascicolo: | 23 |
Codice identificativo Scopus: | 2-s2.0-85059555432 |
Codice identificativo ISI: | WOS:000460330200001 |
Digital Object Identifier (DOI): | http://dx.doi.org/10.1016/j.dark.2018.11.004 |
Handle: | http://hdl.handle.net/11572/219162 |
Citazione: | Testing Horndeski gravity as dark matter with hi_class / Casalino, A.; Rinaldi, M.. - In: PHYSICS OF THE DARK UNIVERSE. - ISSN 2212-6864. - STAMPA. - 2019:23(2019). |
Appare nelle tipologie: | 03.1 Articolo su rivista (Journal article) |
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