Quantum Astronomy. Part I

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dc.creatorIlyanok, Alexander M.
dc.date1999-12-28
dc.date.accessioned2026-07-07T02:35:13Z
dc.date.available2026-07-07T02:35:13Z
dc.descriptionThe article describes new model of the Sun having a hollow core as introduced in [1]. The model helps to explain a number of experimental facts of kinetics, energetics, and Sun spectroscopy based on classic physics. The origin of the Sun's energy is not the thermonuclear process taking place in its core, but the coherent, anisotropic, gravitational compression of the atomic hydrogen in the solar shell at the temperature of 6289 K.
dc.descriptionIn Russian
dc.identifierhttps://arxiv.org/abs/astro-ph/9912537
dc.identifierhttp://arxiv.org/abs/astro-ph/9912537
dc.identifierVesti of the Institute of Modern Knowledge, 1999, vol.2-3, p.61-71
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15535
dc.subjectAstrophysics
dc.titleQuantum Astronomy. Part I
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