标题： 重子暗物质与大爆炸核合成 显示英文标题

标题： Baryonic Dark Matter and Big-Bang Nucleosynthesis

摘要： 附上的论文于1992年2月提交给Ap.J Lett进行发表。 由于它预测了原始氘的丰度，这与观测结果相矛盾，并且与之前作者发表的分析和结论不一致，因此被拒绝了。 然而，在最近的一篇发表于NATURE（1994年4月14日）第368卷第599-603页的文章中，Songalia、Cowie、Hogan和Rugers描述了一项最近的测量（1993年11月），使用凯克10米望远镜测量了我们与一个遥远类星体之间的高红移云中的氘丰度。 他们发现D/H\approx 1.9-2.5 x10^{-4}，这与我们的预测D/H=(2.1+\- 0.35)x10^{-4}非常一致，这比以前认为的要大一个数量级。 Songalia等人发现，从大爆炸核合成推导出的重子密度“与目前观测到的所有重子构成的发光物质量一致”，而我们也得出了相同的结论。 我们在此发布1991年未发表的论文，该论文曾在国际会议上报告过，仅作为预印本分发，主要是因为它所涉及的物理内容及其令人悲伤的道德教训：如果你提交一篇正确的论文，其重要结果与“官方路线”相矛盾，那么它被接受发表的机会非常渺茫。 显示英文摘要

摘要： The enclosed paper was submitted for publication in Ap.J Lett. in February 1992. It has been rejected on the grounds that it predicts primordial Deuterium abundance which is contradicted by observations and because it disagreed with published analysis and conclusions of previous authors. However, in a recent article in NATURE (14 April 1994) Vol. 368 pp. 599-603, Songalia, Cowie, Hogan and Rugers describe a recent measurement (November 1993) with the Keck 10-m Telescope, of the Deuterium abundance in a high redshift cloud between us and a distant quasar. They find D/H\approx 1.9-2.5 x10^{-4} in good agreement with our prediction D/H=(2.1+\- 0.35)x10^{-4}, which is larger by an order of magnitude than believed before. Songalia et al. found that the baryon density inferred from Big Bang Nucleosynthesis is "consistent with the amount of presently observed luminous matter comprising all the baryons in the Universe" while we found the same. We post here our unpublished 1991 paper, which was reported in international conferences and was distributed only as a preprint, mainly because of its physics and its sad moral: If you submit for publication a correct paper with important results that contradict the "party line" it has only slim chances to be accepted for publication.