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(1.1) |
), T denotes a tritium nucleus (
), n denotes a neutron, and
denotes an alpha particle (
). At achievable mean plasma temperatures (i.e., less than about 10 keV), a D-T fusion reaction has a cross-section that
is approximately 100 times greater than that of a D-D fusion reaction (or a T-T fusion reaction) [2]. (There is, unfortunately, no H-H fusion reaction.) For this reason, D-T fusion is considered to be
more practical than D-D fusion, despite the fact that there is no natural source of tritium on the Earth. In fact, it is envisaged that D-T
fusion reactors will breed the requisite tritium within a blanket that surrounds the plasma via nuclear reactions such as
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(1.2) |
makes up 7.6% of terrestrial lithium, which makes up about 0.002% of the Earth's crust.
A D-T fusion reaction liberates
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(1.3) |
and
, respectively. Hence, the
kinetic energies of the neutron and the alpha particle generated by a D-T fusion reaction are
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(1.4) |
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(1.5) |
|
Consider a thermonuclear plasma consisting, principally, of electrons, deuterium ions (that are fully stripped of electrons), and (fully-stripped) tritium ions. All three species are assumed to have have Maxwellian
velocity distribution functions characterized by a common temperature,
. The rate of D-T fusion reactions occurring per unit volume within the plasma is [50]
is the deuteron number density,
the triton number density,
the cross-section for D-T fusion reactions,
the relative
velocity of the reacting species, and
denotes an average over the Maxwellian distributions of the reacting species. In the range of temperatures
–
keV, the D-T fusion reactivity,
, is accurately fitted by the following formula [2,4]
where
Here,
is measured in units of keV. The parameters
–
are specified in Table 1.1.
Figure 1.1 plots
for a realistic range of plasma temperatures. It can be seen that
is a rapidly increasing function of increasing temperature, and that
when
keV.