25 February 2019 to 1 March 2019
Budker INP
Asia/Novosibirsk timezone

Electro-weak production of pseudovector C-even heavy quarkonia in electron-positron collisions on Belle II and BES III

26 Feb 2019, 15:30
20m
Conference room

Conference room

Invited Oral Spectroscopy of light and heavy quarks Mesons of heavy quarks

Speaker

Prof. Nikolay Achasov (Sobolev Institute for Mathematics)

Description

It is shown that the $e^+e^-\to Z\to\chi_{c1}/\chi_{b1}$ and $e^+e^-\to\gamma^{\ast}\gamma^{\ast}\to\chi_{c1}/\chi_{b1}$ contributions do not interfere in the total cross sections. That is, the creation of longitudinally polarized electron-positron beams allows to study separately the $e^+e^-\to Z\to\chi_{c1}/\chi_{b1}$ and $e^+e^-\to\gamma^{\ast}\gamma^{\ast}\to\chi_{c1}/\chi_{b1}$. In the discussed energy region the weak interaction grows with energy increase $\propto G_FE^2$, where $G_F=10^{-5}m_p^{-2}$ is the Fermi constant. $G_FE^2=1.4\times 10^{-4}$ for $\chi_{c1}(1P)$ and $G_FE^2=1.7\times 10^{-4}$ for $\chi_{c1}(3872)$. That is, $G_FE^2\sim \alpha^2$ in the BES III energy region. $G_FE^2=1.1\times 10^{-3}$ for $\chi_{b1}(1P)$ and $G_FE^2=1.2\times 10^{-3}$ for $\chi_{b1}(2P)$. That is, $G_FE^2\gg\alpha^2$ in the Belle II energy region. The BESS III luminosity $10^{33} cm^{-2}s^{-1}$ gives possibilities to register near hundred of events $e^+e^-\to Z\to\chi_{c1}(1P)$ per day and near thirty of them in the well-known channel $\chi_{c1}(1P)\to\gamma\psi(1S)$. If $\chi_{c1}(3872)=\chi_{c1}(2P)$, then also near hundred of events $e^+e^-\to Z\to\chi_{c1}(3872)$ per day may be registered and several of them in the channel $\chi_{c1}(3872)\to\gamma\psi(2S)$, several tens of them in the channel $\chi_{c1}(3872)\to D^0\bar D^{0\ast}+c.c$. The huge Belle II luminosity $8\times 10^{35} cm^{-2}s^{-1}$ gives possibilities to register near hundred thousand of events each $e^+e^-\to Z\to\chi_{b1}(1P)$ and $e^+e^-\to Z\to\chi_{b1}(1P)$ per day and several tens of thousands of them in the well-known channels $\chi_{b1}(1P)\to\gamma\Upsilon(1S)$ and $\chi_{b1}(2P)\to\gamma\Upsilon(2S)$.

Summary

The new elegant experimental probes appear. In particular, they could find out whether is $\chi_{c1}(3872)=\chi_{c1}(2P)$ and search out the
$\chi_{b1}(2P)\to\rho\Upsilon(1S)$.

The work was supported by the program of fundamental scientific researches of the SB RAS No. II.15.1., project No. 0314-2016-0021.

The work also is partially supported by the Russian Foundation for Basic Research Grant No. 16-02-00065.

REFERENCES

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Primary author

Prof. Nikolay Achasov (Sobolev Institute for Mathematics)

Presentation Materials

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