The energy output from a nuclear reaction is calculated by multiplying the mass defect (the difference between the total mass of the reactants and the total mass of the products) by 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 specific reaction:
\[
m_{\text{reactants}} = m\left(^{2}_1 \text{H}\right) + m\left(^{3}_1 \text{H}\right) = 2.014102 \, \text{u} + 3.016049 \, \text{u} = 5.030151 \, \text{u}
\]
\[
m_{\text{products}} = m\left(^{4}_2 \text{He}\right) + m\left(^{1}_0 \text{n}\right) = 4.002603 \, \text{u} + 1.008665 \, \text{u} = 5.011268 \, \text{u}
\]
The resulting mass defect is:
\[
\Delta m = m_{\text{reactants}} - m_{\text{products}} = 5.030151 \, \text{u} - 5.011268 \, \text{u} = 0.018883 \, \text{u}
\]
Converting the mass defect to energy:
\[
Q = \Delta m \cdot c^2 = 0.018883 \, \text{u} \times 931 \, \text{MeV}/c^2
\]
\[
Q = 17.6 \, \text{MeV}
\]
The energy released in this reaction is:
\[
\boxed{Q = 17.6 \, \text{MeV}}
\]