====== TTP05-05 Energy-square equations for relativistic closed systems. ====== The most powerful relativistic two-body equations have only half as many components as their Dirac-Breit and Bethe-Salpeter counterparts and contain only the square of the total cms energy. In this letter, the "energy-square" theorem is extended to systems of $n>2$ Dirac particles. The case $n=3$ is discussed for baryons. |**Hartmut Pilkuhn** | |** Physics Letters B 614 62-65 2005 ** | | {{preprints:2005:ttp05-05.pdf|PDF}} {{preprints:2005:ttp05-05.ps|PostScript}} | | |