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OHe can form in Neutral stars or white dwarfs?

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OHe, composed of lepton-like doubly charged particles bound with primordial helium nuclei, can form in neutral stars or white dwarfs. The OHe hypothesis suggests that OHe dark atoms, with charged particles O$^{--}$ bound to helium nuclei, could constitute a significant portion of dark matter. These OHe atoms interact with nuclei through Coulomb and nuclear forces, potentially forming bound states with various nuclei, leading to keV binding energies. The stabilization of these bound states is crucial and likely involves the presence of a barrier in the OHe-nucleus potential . Additionally, the interaction of OHe with nuclei can result in the formation of O-beryllium ions, posing challenges due to the potential overabundance of anomalous isotopes in terrestrial matter .

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Open access Some potential problems of OHe composite dark matter Jean-René Cudell, Maxim Yu. Khlopov, Quentin Wallemacq - Show less +2 more 18 Dec 2014 13 Citations	Not addressed in the paper.
Open access The nuclear physics of OHe Jean-René Cudell, Maxim Yu. Khlopov, Quentin Wallemacq - Show less +2 more 24 Nov 2012 15 Citations	Not addressed in the paper.
Open access•Posted Content Towards Nuclear Physics of OHe Dark Matter Maxim Yu. Khlopov, A. G. Mayorov, Evgeny Soldatov - Show less +2 more 15 Nov 2011-arXiv: High Energy Physics - Phenomenology 2 Citations	Not addressed in the paper.
Open access•Posted Content The nuclear physics of OHe Jean-René Cudell, Maxim Yu. Khlopov, Quentin Wallemacq - Show less +2 more 24 Nov 2012-arXiv: Cosmology and Nongalactic Astrophysics 19 Citations	Not addressed in the paper.
Open access Towards Nuclear Physics of OHe Dark Matter Maxim Yu. Khlopov, A. G. Mayorov, Evgeny Soldatov - Show less +2 more 16 Nov 2011 4 Citations	Not addressed in the paper.

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