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
y2P)
is a monotonic, rapidly decreasing function of the baryon abundance
. 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
10 in the
``interesting'' range 1 - 10, y2P decreases with the ~ 1.6
power of
. As a
result, a 10% error in y2P corresponds
to only a 6% error in
.
This strong dependence of y2P
on
10,
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
range shown in Fig. 3.
![]() |
Figure 3. The predicted D/H abundance
(solid curve) and the 2 |
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
.
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.