The energy released in a nuclear reaction is given by the mass defect (the difference between the total mass of the reactants and the total mass of the products) times the square of the speed of light:
\[
Q = (\Delta m) c^2
\]
where:
\[
\Delta m = \left( m_{\text{reactants}} - m_{\text{products}} \right)
\]
For this reaction:
\[
m_{\text{reactants}} = m\left(^{2}_1 \text{H}\right) + m\left(^{3}_1 \text{H}\right) = 2.014102 \, \text{u} + 3.016049 \, \text{u} = 5.030151 \, \text{u}
\]
\[
m_{\text{products}} = m\left(^{4}_2 \text{He}\right) + m\left(^{1}_0 \text{n}\right) = 4.002603 \, \text{u} + 1.008665 \, \text{u} = 5.011268 \, \text{u}
\]
Thus, the mass defect is:
\[
\Delta m = m_{\text{reactants}} - m_{\text{products}} = 5.030151 \, \text{u} - 5.011268 \, \text{u} = 0.018883 \, \text{u}
\]
Now, converting the mass defect into energy:
\[
Q = \Delta m \cdot c^2 = 0.018883 \, \text{u} \times 931 \, \text{MeV}/c^2
\]
\[
Q = 17.6 \, \text{MeV}
\]
Thus, the energy released in the reaction is:
\[
\boxed{Q = 17.6 \, \text{MeV}}
\]