DC Field | Value | Language |
dc.contributor.author | Ivanov, M. A. | - |
dc.date.accessioned | 2016-04-05T11:00:10Z | - |
dc.date.accessioned | 2017-07-27T11:59:42Z | - |
dc.date.available | 2016-04-05T11:00:10Z | - |
dc.date.available | 2017-07-27T11:59:42Z | - |
dc.date.issued | 2004 | - |
dc.identifier.citation | Ivanov, M. A. Galaxy number counts in a presence of the graviton background / М. А. Ivanov // http://arxiv.org/a/ivanov_m_1.html | ru_RU |
dc.identifier.uri | https://libeldoc.bsuir.by/handle/123456789/6341 | - |
dc.description.abstract | In the model of low-energy quantum gravity by the author, cosmological redshifts are caused by interactions of photons with gravitons. Non-forehead collisions with gravitons will lead to an additional relaxation of any photonic flux. Using only the luminosity distance and a geometrical one as functions of a redshift in this model, theoretical predictions for galaxy number counts are considered here. The Schechter luminosity function with \alpha =-2.43 is used. The considered model provides a good fit to galaxy observations by Yasuda et al. (AJ, 122 (2001) 1104) if the same K-corrections are added. It is shown that observations of N(z) for different magnitudes m are a lot more informative than the ones of N(m). | ru_RU |
dc.language.iso | en | ru_RU |
dc.subject | публикации ученых | ru_RU |
dc.title | Galaxy number counts in a presence of the graviton background | ru_RU |
dc.type | Article | ru_RU |
Appears in Collections: | Публикации в зарубежных изданиях
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