Study of dynamics of the process $e^+e^-\to \pi^+\pi^-\pi^0$ in the energy range 1.15--2.00 GeV
The dynamics of the process $ e^+e^- \to \pi^+\pi^-\pi^0 $ is studied in the energy region from 1.15 to 2.00 GeV using data accumulated with the SND detector at the VEPP-2000 $e^+e^-$ collider. The Dalitz plot distribution and $\pi^+\pi^-$ mass spectrum are analyzed in a model including the intermed...
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creator | SND Collaboration Achasov, M. N Barnyakov, A. Yu Baykov, A. A Beloborodov, K. I Berdyugin, A. V Berkaev, D. E Bogdanchikov, A. G Botov, A. A Dimova, T. V Druzhinin, V. P Golubev, V. B Kirpotin, A. N Kardapoltsev, L. V Kasaev, A. S Kharlamov, A. G Koop, I. A Korol, A. A Kovrizhin, D. P Kupich, A. S Martin, K. A Melnikova, N. A Muchnoi, N. Yu Obrazovsky, A. E Pakhtusova, E. V Pugachev, K. V Rabusov, D. V Rogovsky, Yu. A Savchenko, Y. S Senchenko, A. I Serednyakov, S. I Shatilov, D. N Shatunov, Yu. M Shtol, D. A Shwartz, D. B Silagadze, Z. K Surin, I. K Timoshenko, M. V Usov, Yu. V Zhabin, V. N Zhulanov, V. V |
description | The dynamics of the process $ e^+e^- \to \pi^+\pi^-\pi^0 $ is studied in the
energy region from 1.15 to 2.00 GeV using data accumulated with the SND
detector at the VEPP-2000 $e^+e^-$ collider. The Dalitz plot distribution and
$\pi^+\pi^-$ mass spectrum are analyzed in a model including the intermediate
states $\rho(770)\pi$, $\rho(1450)\pi$, and $\omega\pi^0$. As a result, the
energy dependences of the $\rho(770)\pi$ and $\rho(1450)\pi$ cross sections and
the relative phases between the $\rho(770)\pi$ amplitude and the $\rho(1450)\pi
$ and $\omega\pi^0$ amplitudes are obtained. The $\rho(1450)\pi$ cross section
has a peak in the energy region of the $\omega(1650)$ resonance (1.55-1.75
GeV). In this energy range the contributions of the $\rho(770)\pi$ and
$\rho(1450)\pi$ states are of the same order of magnitude. No resonance
structure near 1.65 GeV is observed in the $\rho(770)\pi$ cross section. We
conclude that the intermediate state $\rho(1450)\pi$ gives a significant
contribution to the decay of $\omega (1650)\to\pi^+\pi^-\pi^0$, whereas the
$\rho(770)\pi$ mechanism dominates in the decay
$\omega(1420)\to\pi^+\pi^-\pi^0$. |
doi_str_mv | 10.48550/arxiv.2007.14595 |
format | Article |
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energy region from 1.15 to 2.00 GeV using data accumulated with the SND
detector at the VEPP-2000 $e^+e^-$ collider. The Dalitz plot distribution and
$\pi^+\pi^-$ mass spectrum are analyzed in a model including the intermediate
states $\rho(770)\pi$, $\rho(1450)\pi$, and $\omega\pi^0$. As a result, the
energy dependences of the $\rho(770)\pi$ and $\rho(1450)\pi$ cross sections and
the relative phases between the $\rho(770)\pi$ amplitude and the $\rho(1450)\pi
$ and $\omega\pi^0$ amplitudes are obtained. The $\rho(1450)\pi$ cross section
has a peak in the energy region of the $\omega(1650)$ resonance (1.55-1.75
GeV). In this energy range the contributions of the $\rho(770)\pi$ and
$\rho(1450)\pi$ states are of the same order of magnitude. No resonance
structure near 1.65 GeV is observed in the $\rho(770)\pi$ cross section. We
conclude that the intermediate state $\rho(1450)\pi$ gives a significant
contribution to the decay of $\omega (1650)\to\pi^+\pi^-\pi^0$, whereas the
$\rho(770)\pi$ mechanism dominates in the decay
$\omega(1420)\to\pi^+\pi^-\pi^0$.</description><identifier>DOI: 10.48550/arxiv.2007.14595</identifier><language>eng</language><subject>Physics - High Energy Physics - Experiment</subject><creationdate>2020-07</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2007.14595$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.1140/epjc/s10052-020-08524-4$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.48550/arXiv.2007.14595$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>SND Collaboration</creatorcontrib><creatorcontrib>Achasov, M. N</creatorcontrib><creatorcontrib>Barnyakov, A. Yu</creatorcontrib><creatorcontrib>Baykov, A. A</creatorcontrib><creatorcontrib>Beloborodov, K. I</creatorcontrib><creatorcontrib>Berdyugin, A. V</creatorcontrib><creatorcontrib>Berkaev, D. E</creatorcontrib><creatorcontrib>Bogdanchikov, A. G</creatorcontrib><creatorcontrib>Botov, A. A</creatorcontrib><creatorcontrib>Dimova, T. V</creatorcontrib><creatorcontrib>Druzhinin, V. P</creatorcontrib><creatorcontrib>Golubev, V. B</creatorcontrib><creatorcontrib>Kirpotin, A. N</creatorcontrib><creatorcontrib>Kardapoltsev, L. V</creatorcontrib><creatorcontrib>Kasaev, A. S</creatorcontrib><creatorcontrib>Kharlamov, A. G</creatorcontrib><creatorcontrib>Koop, I. A</creatorcontrib><creatorcontrib>Korol, A. A</creatorcontrib><creatorcontrib>Kovrizhin, D. P</creatorcontrib><creatorcontrib>Kupich, A. S</creatorcontrib><creatorcontrib>Martin, K. A</creatorcontrib><creatorcontrib>Melnikova, N. A</creatorcontrib><creatorcontrib>Muchnoi, N. Yu</creatorcontrib><creatorcontrib>Obrazovsky, A. E</creatorcontrib><creatorcontrib>Pakhtusova, E. V</creatorcontrib><creatorcontrib>Pugachev, K. V</creatorcontrib><creatorcontrib>Rabusov, D. V</creatorcontrib><creatorcontrib>Rogovsky, Yu. A</creatorcontrib><creatorcontrib>Savchenko, Y. S</creatorcontrib><creatorcontrib>Senchenko, A. I</creatorcontrib><creatorcontrib>Serednyakov, S. I</creatorcontrib><creatorcontrib>Shatilov, D. N</creatorcontrib><creatorcontrib>Shatunov, Yu. M</creatorcontrib><creatorcontrib>Shtol, D. A</creatorcontrib><creatorcontrib>Shwartz, D. B</creatorcontrib><creatorcontrib>Silagadze, Z. K</creatorcontrib><creatorcontrib>Surin, I. K</creatorcontrib><creatorcontrib>Timoshenko, M. V</creatorcontrib><creatorcontrib>Usov, Yu. V</creatorcontrib><creatorcontrib>Zhabin, V. N</creatorcontrib><creatorcontrib>Zhulanov, V. V</creatorcontrib><title>Study of dynamics of the process $e^+e^-\to \pi^+\pi^-\pi^0$ in the energy range 1.15--2.00 GeV</title><description>The dynamics of the process $ e^+e^- \to \pi^+\pi^-\pi^0 $ is studied in the
energy region from 1.15 to 2.00 GeV using data accumulated with the SND
detector at the VEPP-2000 $e^+e^-$ collider. The Dalitz plot distribution and
$\pi^+\pi^-$ mass spectrum are analyzed in a model including the intermediate
states $\rho(770)\pi$, $\rho(1450)\pi$, and $\omega\pi^0$. As a result, the
energy dependences of the $\rho(770)\pi$ and $\rho(1450)\pi$ cross sections and
the relative phases between the $\rho(770)\pi$ amplitude and the $\rho(1450)\pi
$ and $\omega\pi^0$ amplitudes are obtained. The $\rho(1450)\pi$ cross section
has a peak in the energy region of the $\omega(1650)$ resonance (1.55-1.75
GeV). In this energy range the contributions of the $\rho(770)\pi$ and
$\rho(1450)\pi$ states are of the same order of magnitude. No resonance
structure near 1.65 GeV is observed in the $\rho(770)\pi$ cross section. We
conclude that the intermediate state $\rho(1450)\pi$ gives a significant
contribution to the decay of $\omega (1650)\to\pi^+\pi^-\pi^0$, whereas the
$\rho(770)\pi$ mechanism dominates in the decay
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V</creator><scope>GOX</scope></search><sort><creationdate>20200729</creationdate><title>Study of dynamics of the process $e^+e^-\to \pi^+\pi^-\pi^0$ in the energy range 1.15--2.00 GeV</title><author>SND Collaboration ; Achasov, M. N ; Barnyakov, A. Yu ; Baykov, A. A ; Beloborodov, K. I ; Berdyugin, A. V ; Berkaev, D. E ; Bogdanchikov, A. G ; Botov, A. A ; Dimova, T. V ; Druzhinin, V. P ; Golubev, V. B ; Kirpotin, A. N ; Kardapoltsev, L. V ; Kasaev, A. S ; Kharlamov, A. G ; Koop, I. A ; Korol, A. A ; Kovrizhin, D. P ; Kupich, A. S ; Martin, K. A ; Melnikova, N. A ; Muchnoi, N. Yu ; Obrazovsky, A. E ; Pakhtusova, E. V ; Pugachev, K. V ; Rabusov, D. V ; Rogovsky, Yu. A ; Savchenko, Y. S ; Senchenko, A. I ; Serednyakov, S. I ; Shatilov, D. N ; Shatunov, Yu. M ; Shtol, D. A ; Shwartz, D. B ; Silagadze, Z. K ; Surin, I. K ; Timoshenko, M. V ; Usov, Yu. V ; Zhabin, V. N ; Zhulanov, V. 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B</creatorcontrib><creatorcontrib>Silagadze, Z. K</creatorcontrib><creatorcontrib>Surin, I. K</creatorcontrib><creatorcontrib>Timoshenko, M. V</creatorcontrib><creatorcontrib>Usov, Yu. V</creatorcontrib><creatorcontrib>Zhabin, V. N</creatorcontrib><creatorcontrib>Zhulanov, V. V</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>SND Collaboration</au><au>Achasov, M. N</au><au>Barnyakov, A. Yu</au><au>Baykov, A. A</au><au>Beloborodov, K. I</au><au>Berdyugin, A. V</au><au>Berkaev, D. E</au><au>Bogdanchikov, A. G</au><au>Botov, A. A</au><au>Dimova, T. V</au><au>Druzhinin, V. P</au><au>Golubev, V. B</au><au>Kirpotin, A. N</au><au>Kardapoltsev, L. V</au><au>Kasaev, A. S</au><au>Kharlamov, A. G</au><au>Koop, I. A</au><au>Korol, A. A</au><au>Kovrizhin, D. P</au><au>Kupich, A. S</au><au>Martin, K. A</au><au>Melnikova, N. A</au><au>Muchnoi, N. Yu</au><au>Obrazovsky, A. E</au><au>Pakhtusova, E. V</au><au>Pugachev, K. V</au><au>Rabusov, D. V</au><au>Rogovsky, Yu. A</au><au>Savchenko, Y. S</au><au>Senchenko, A. I</au><au>Serednyakov, S. I</au><au>Shatilov, D. N</au><au>Shatunov, Yu. M</au><au>Shtol, D. A</au><au>Shwartz, D. B</au><au>Silagadze, Z. K</au><au>Surin, I. K</au><au>Timoshenko, M. V</au><au>Usov, Yu. V</au><au>Zhabin, V. N</au><au>Zhulanov, V. V</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Study of dynamics of the process $e^+e^-\to \pi^+\pi^-\pi^0$ in the energy range 1.15--2.00 GeV</atitle><date>2020-07-29</date><risdate>2020</risdate><abstract>The dynamics of the process $ e^+e^- \to \pi^+\pi^-\pi^0 $ is studied in the
energy region from 1.15 to 2.00 GeV using data accumulated with the SND
detector at the VEPP-2000 $e^+e^-$ collider. The Dalitz plot distribution and
$\pi^+\pi^-$ mass spectrum are analyzed in a model including the intermediate
states $\rho(770)\pi$, $\rho(1450)\pi$, and $\omega\pi^0$. As a result, the
energy dependences of the $\rho(770)\pi$ and $\rho(1450)\pi$ cross sections and
the relative phases between the $\rho(770)\pi$ amplitude and the $\rho(1450)\pi
$ and $\omega\pi^0$ amplitudes are obtained. The $\rho(1450)\pi$ cross section
has a peak in the energy region of the $\omega(1650)$ resonance (1.55-1.75
GeV). In this energy range the contributions of the $\rho(770)\pi$ and
$\rho(1450)\pi$ states are of the same order of magnitude. No resonance
structure near 1.65 GeV is observed in the $\rho(770)\pi$ cross section. We
conclude that the intermediate state $\rho(1450)\pi$ gives a significant
contribution to the decay of $\omega (1650)\to\pi^+\pi^-\pi^0$, whereas the
$\rho(770)\pi$ mechanism dominates in the decay
$\omega(1420)\to\pi^+\pi^-\pi^0$.</abstract><doi>10.48550/arxiv.2007.14595</doi><oa>free_for_read</oa></addata></record> |
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subjects | Physics - High Energy Physics - Experiment |
title | Study of dynamics of the process $e^+e^-\to \pi^+\pi^-\pi^0$ in the energy range 1.15--2.00 GeV |
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