The Cosmological Baryon Density from Deuterium in QSO Spectra
Abstract
Description
The primordial D/H ratio now provides the best measure of the cosmological density of baryons. We describe in detail how we deduce the D/H ratio from absorption lines in the spectra of quasars, and we present our first two measurements of D/H in different QSOs, which agree to within the random errors. We describe how we correct D/H for blending with Lyman alpha forest H lines. For our two QSOs these corrections are small, because the D lines are narrow, deep and constrained by H and metal lines. The similarity of the two measurements rules out ad hoc astrophysical effects, such as the destruction of D without production of metals, or unusual data problems. We are confident that we have measured the primordial abundance of D (log D/H $= -4.62 \pm 0.05$), which is the first such measurement because other values in the literature are much larger, and apparently strongly contaminated.
27 pages, 6 figures, uses sprocl.sty. Conference Proceeding of the International Symposium on "Origin of Matter and Evolution of Galaxies in the Universe", Atami, Japan, January 18-20, 1996. Manuscript is also available at http://nately.ucsd.edu/papers/papers.html ; Tables have been slightly revised
27 pages, 6 figures, uses sprocl.sty. Conference Proceeding of the International Symposium on "Origin of Matter and Evolution of Galaxies in the Universe", Atami, Japan, January 18-20, 1996. Manuscript is also available at http://nately.ucsd.edu/papers/papers.html ; Tables have been slightly revised