Slow moving neutrons (thermal neutrons, those with energies of order 0.05eV) are easily captured by nuclei, which may then become neutron rich and decay by (electron) emission. The thermal neutron capture cross sectional area (expressed in barns, [10^{24}cm^{2}]) is a measure of how easily neutrons are absorbed by nuclei, the larger the csa, the greater probability of absorption. The cross section for thermal neutrons is measured for those with speeds of 2200 metres per second. In nuclear reactors, Zirconium, with a low neutron absorption, is used to contain the fuel rods, whereas Uranium238 absorbs neutrons and is either induced into nuclear fission, or goes on absorbing more neutrons and eventually becoming Plutonium239. Those isotopes with a magic number of neutrons, N magic, have very low neutron absorptions. Xenon135 has the highest thermal neutron csa of any known isotope; it is produced by the fission of uranium as a fission product in nuclear reactors, where it presents a problem being the most serious reactor poison, and may delay the restart of a reactor after a period of shutdown.
The above chart shows the thermal neutron capture cross sectional areas for some stable and unstable isotopes of xenon. The thermal neutron csa for Xe135, the nuclear reactor poison, is extremely high; being four magnitudes higher than any other isotope of xenon. Note also the very distinctive odd/even 'combshaped' bars  the isotopes with an odd number of neutrons (oddN) have a higher csa for thermal neutrons, they would like to capture a neutron to become an isotope with an even number of neutrons, and if they do so, their apetite for capturing another neutron is much diminished (much lower thermal neutron csa for evenN nuclei). Note that xenon, Z=54, has an even number of protons (Zeven), so xenon nuclei with Neven also have an even number of alpha particles (Helium nuclei) within them. Nuclei like to possess an even number of helium nuclei (Neven Zeven), for then they are more stable. See Nuclear Spin for the reason.
