Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
1995-08-31
Phys.Rev.D53:3998,1996; Erratum-ibid.D55:1699,1997
Physics
High Energy Physics
High Energy Physics - Phenomenology
16 pages in REVTeX, no figures
Scientific paper
10.1103/PhysRevD.53.3998 10.1103
This is the continuation of a previous article, in which the Bjorken and Voloshin sum rules were interpreted as statements of conservation of probability and energy. Here the formalism is extended to higher moments of the Hamiltonian operator. From the conservation of the second moment of the Hamiltonian operator one can derive a sum rule which, in the small velocity limit, reduces to the Bigi--Grozin--Shifman--Uraltsev--Vainshtein (BGSUV) sum rule. On the other hand, the conservation of the third moment of the Hamiltonian operator gives a new sum rule, which is related to the matrix element of the heavy quark counterpart of the Darwin term in atomic physics. The general case of the higher order moments is also discussed.
Chow Chi-Keung
Pirjol Dan
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