Crater has shown that, for two particles (with masses m1 and m2) in a Coulombic bound state, the charge distribution is equal to the sum of the two charge distributions obtained by taking m1→∞ and m2→∞, respectively, while keeping the same Coulombic potential. We provide a simple scaling criterion to determine whether an arbitrary Hamiltonian possesses this property. In particular, we show that, for a Coulombic system, fine structure corrections preserve this Crater property while two-particle relativistic corrections and/or hyperfine corrections may destroy it.

1.
Horace W.
Crater
, “
An Unusual Feature of Charge Densities for Two-Particle Bound States
,”
Am. J. Phys.
67
,
739
741
(
1999
).
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