Di-pion emission in heavy quarkonia decays

dc.creatorSimonov, Yu. A.
dc.date2007-12-13
dc.date2008-02-04
dc.date.accessioned2026-07-07T11:13:44Z
dc.date.available2026-07-07T11:13:44Z
dc.descriptionThe di-pion spectrum for the $Υ(nS) \to Υ(n'S))$ transition with $n\leq 4$ has the form $\frac{dw}{dq}\sim $ (phase space) $ |η-x|^2$, with $x=\frac{q^2-4m^2_π}{(ΔM)^2 -4 m^2_π}< q^2 \equiv M^2_{ππ}, $ and $ΔM=M(nS) -M(n'S)$. The parameter $η$ is calculated and the spectrum is shown to reproduce the experimental data for all 3 types of decays: $3\to 1, 2\to 1$ and $3\to 2$ with $η\approx 0.5; 0$, and -3, respectively.
dc.description3 pages, 2 figures; Journal version
dc.identifierhttps://arxiv.org/abs/0712.2197
dc.identifierhttp://arxiv.org/abs/0712.2197
dc.identifierJETPLett.87:121-123,2008
dc.identifierdoi:10.1007/s11448-008-3001-5
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191820
dc.subjectHigh Energy Physics - Phenomenology
dc.titleDi-pion emission in heavy quarkonia decays
dc.typetext

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