{
"id": "astro-ph/0405454",
"version": "v1",
"published": "2004-05-24T09:16:07.000Z",
"updated": "2004-05-24T09:16:07.000Z",
"title": "The law of evolution of energy density in the universe imposed by quantum cosmology and its consequences",
"authors": [
"V. E. Kuzmichev",
"V. V. Kuzmichev"
],
"comment": "17 pages, 3 EPS figure; full version is to appear in the volume \"Progress in General Relativity and Quantum Cosmology Research\" (Nova Science)",
"categories": [
"astro-ph",
"gr-qc"
],
"abstract": "The quantum model of homogeneous and isotropic universe filled with the uniform scalar field is considered. This model predicts effective inverse square-law dependence of the mean total energy density <\\rho> on the expectation value of cosmological scale factor where the averaging is performed over the state with large quantum numbers. Such a law of decreasing of <\\rho> during the expansion of the universe allows to describe the observed coordinate distances to type Ia supernovae and radio galaxies in the redshift interval z = 0.01 - 1.8. A comparison with phenomenological models with the cosmological constant (\\Lambda CDM) and with zero dark energy component (\\Omega_{M} = 1) is made. It is shown that observed small deviations of the coordinate distances to some sources from the predictions of above mentioned simple quantum model can be explained by the fluctuations \\delta a of the scale factor about the average value . These fluctuations can arise due to finite widths of quasistationary states in the early universe. During expansion the fluctuations \\delta a grow with time and manifest themselves in the form of observed relative increase or decrease of coordinate distances. The amplitudes of fluctuations \\delta a/ calculated from observed positions of individual supernovae are in good agreement with their estimations in quantum theory. Possible consequences from the conclusions of quantum theory are discussed.",
"revisions": [
{
"version": "v1",
"updated": "2004-05-24T09:16:07.000Z"
}
],
"analyses": {
"keywords": [
"energy density",
"quantum cosmology",
"coordinate distances",
"consequences"
],
"note": {
"typesetting": "TeX",
"pages": 17,
"language": "en",
"license": "arXiv",
"status": "editable",
"inspire": 650852,
"adsabs": "2004astro.ph..5454K"
}
}
}