Consider the following fusion reaction, which allows stars to produce
progressively heavier elements: \({ }_{2}^{3} \mathrm{He}+{ }_{2}^{4}
\mathrm{He} \rightarrow{ }_{4}^{7} \mathrm{Be}+\gamma\). The mass of \({
}_{2}^{3} \mathrm{He}\) is \(3.016029 \mathrm{u}\), the mass of \({ }_{2}^{4}\) He
is \(4.002603 \mathrm{u}\), and the mass of \({ }_{4}^{7} \mathrm{Be}\) is
\(7.0169298 \mathrm{u}\). The atomic mass unit is \(u=1.66 \cdot 10^{-27}
\mathrm{~kg} .\) Assuming the Be atom is at rest after the reaction and
neglecting any potential energy between the atoms and kinetic energy of the He
nuclei, calculate the minimum possible energy and maximum possible wavelength
of the photon \(\gamma\) that is released in this reaction.