  The reaction 243 Am (n, 2n) populates the T of 16 hours ground state 242 g Am
with J of 1 or the 242 m Am isomer state J of 5 with T of 141 years. The former
state 242 g Am mostly beta decays to 242 Cm, or transmutes to 242 Pu via
electron capture. The absolute yield of 242 g Am is compatible with the
measured data, estimated by the alpha activity of 242 Cm by Norris in 1983. The
branching ratio defined by the ratio of the populations of the lowest intrinsic
states of 242 Am. Calculated yields of ground 242 g Am and isomer 242 m Am
states of the residual nucleus 242 Am are used to predict the relative yield of
isomer. These populations defined by the gamma decay of the excited states,
described by the standard kinetic equation. The ordering of the low and high
spin states is different in case of 236 Np and 242 Am nuclei, that explains
different shapes of relative yields near the (n, 2n) reaction threshold, though
the excitation energy dependences are similar. Data of 243 Am (n, F) at 5 MeV
and 15 MeV by Drapchinsky in 2004, support calculated 243Am (n,xnf) prefission
neutron contribution to prompt fission neutron spectra and calculated exclusive
neutron spectra of 243 Am (n, 2n) feeding the 242 g Am and isomer 242 m Am
states.
