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2.2. Deuterium - The Ideal Baryometer

As may be seen in Fig. 1, the deuterium abundance (the ratio, by number, of deuterium to hydrogen: hereinafter, (D/H)P ident y2P) is a monotonic, rapidly decreasing function of the baryon abundance eta. The reason for this behavior is easily understood. Once BBN begins in earnest, when the temperature drops below ~ 80 keV, D is rapidly burned to 3H, 3He and 4He. The higher the baryon abundance, the faster the burning and the less D survives. For eta10 in the ``interesting'' range 1 - 10, y2P decreases with the ~ 1.6 power of eta. As a result, a 10% error in y2P corresponds to only a 6% error in eta. This strong dependence of y2P on eta10, combined with the simplicity of the evolution of D/H in the epochs following BBN, is responsible for the unique role of deuterium as a baryometer [2]. Because almost all the relevant reaction cross sections are measured in the laboratory at energies comparable to those of BBN, the theoretical uncertainties in the BBN-predicted abundance of deuterium is quite small, 8 - 10% for most of the interesting eta range shown in Fig. 3.

Figure 3

Figure 3. The predicted D/H abundance (solid curve) and the 2sigma theoretical uncertainty [3]. The horizontal lines show the range indicated by the observational data for both the high D/H (upper two lines ) and low D/H (lower two lines).

Deuterium and helium-4 are complementary, forming the crucial link in testing the consistency of BBN in the standard model. While the primordial-D abundance is very sensitive to the baryon density, the primordial-he abundance is relatively insensitive to eta. Deuterium provides a bound on the universal baryon density while helium-4 constrains the early expansion rate of the Universe, offerring bounds on particle physics beyond the standard model.

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