Light element synthesis in baryon isocurvature models

D. Lohiya; P. Kumar

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arXiv · astro-ph/0602425

Light element synthesis in baryon isocurvature models

D. Lohiya·P. Kumar

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Abstract

The prejudice against baryon isocurvature models is primarily because of their inconsistency with early universe light element nucleosynthesis results. We propose that incipient low metallicity (Pop II) star forming regions can be expected to have environments conducive to Deuterium production by spallation, up to levels observed in the universe.

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D. Lohiya, P. Kumar. 2006-02-20. Light element synthesis in baryon isocurvature models. https://arxiv.org/abs/astro-ph/0602425

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