A simple alternative to the Breit-Wigner distribution

Abstract

First, we discuss the conditions under which the non-relativistic and relativistic types of the Breit-Wigner energy distributions are obtained. Then, upon insisting on the correct normalization of the energy distribution, we introduce a Flatt\'e-like relativistic distribution -- denominated as Sill distribution -- that (i) contains left-threshold effects, (ii) is properly normalized for any decay width, (iii) can be obtained as an appropriate limit in which the decay width is a constant, (iv) is easily generalized to the multi-channel case (v) as well as to a convoluted form in case of a decay chain and -- last but not least -- (vi) is simple to deal with. We compare the Sill distribution to spectral functions derived within specific QFT models and show that it fairs well in concrete examples that involve a fit to experimental data for the , a1(1260), and K*(982) mesons as well as the (1232) baryon. We also present a study of the f2(1270) which has more than one possible decay channels. Finally, we discuss the limitations of the Sill distribution using the a0(980)-a0(1450) and the K0(700)-K0(1430) resonances as examples.

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