2020
DOI: 10.1103/physrevd.102.103518
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Structure formation in a Dirac-Milne universe: Comparison with the standard cosmological model

Abstract: HAL is a multi-disciplinary open access archive for the deposit and dissemination of scientific research documents, whether they are published or not. The documents may come from teaching and research institutions in France or abroad, or from public or private research centers. L'archive ouverte pluridisciplinaire HAL, est destinée au dépôt et à la diffusion de documents scientifiques de niveau recherche, publiés ou non, émanant des établissements d'enseignement et de recherche français ou étrangers, des labor… Show more

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Cited by 8 publications
(24 citation statements)
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“…Despite these tremendous differences in the initial timescales, the D-M universe, with only one adjustable parameter H 0 , presents several elements of concordance: its age, equal to 1/H 0 , is almost equal to the age of the ΛCDM universe for H 0 ≈ 70 km s −1 Mpc −1 , while the H(z) dependence of cosmic chronometers is nicely reproduced in coasting universes (Melia & Maier 2013), along with primordial nucleosynthesis 1 and the SNIa luminosity distance (Sethi et al 1999;Chodorowski 2005;Benoit-Lévy & Chardin 2012). Also, its non linear structure formation mechanism appears to reproduce the main features of the matter power spectrum starting from a single scale of matter-antimatter domains at decoupling (Manfredi et al 2018(Manfredi et al , 2020. In addition, the D-M cosmology does not suffer from the horizon problem (Benoit-Lévy & Chardin 2012) and therefore does not require inflation.…”
Section: The Dirac-milne Universementioning
confidence: 72%
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“…Despite these tremendous differences in the initial timescales, the D-M universe, with only one adjustable parameter H 0 , presents several elements of concordance: its age, equal to 1/H 0 , is almost equal to the age of the ΛCDM universe for H 0 ≈ 70 km s −1 Mpc −1 , while the H(z) dependence of cosmic chronometers is nicely reproduced in coasting universes (Melia & Maier 2013), along with primordial nucleosynthesis 1 and the SNIa luminosity distance (Sethi et al 1999;Chodorowski 2005;Benoit-Lévy & Chardin 2012). Also, its non linear structure formation mechanism appears to reproduce the main features of the matter power spectrum starting from a single scale of matter-antimatter domains at decoupling (Manfredi et al 2018(Manfredi et al , 2020. In addition, the D-M cosmology does not suffer from the horizon problem (Benoit-Lévy & Chardin 2012) and therefore does not require inflation.…”
Section: The Dirac-milne Universementioning
confidence: 72%
“…It is fundamental to note that although existing in nature, the Dirac particle-hole system has no Newtonian expression, even when the three Newtonian mass parameters (inertial, gravitational active, and gravitational passive) are used (Manfredi et al 2018). On the other hand, as studied in Manfredi et al (2018Manfredi et al ( , 2020, the gravitational sector of matter and antimatter in the D-M universe can be expressed with two separate gravitational potentials, using the following coupled Poisson equations:…”
Section: Gravitational Setup In the D-m Universementioning
confidence: 99%
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“…Namely, a stage preceding the acceleration should be a Milne's-like, i.e., linear in a cosmic time. The Milne's-like universes have been much discussed again recently [33][34][35][36][37][38].…”
Section: Vacuum Energy Problem As a Criterion For Finding The Preferred Reference Framementioning
confidence: 99%