Rates of $$D^{*}_{0}(2400)$$ D0∗(2400) , $$ D_J^*(3000) $$ DJ∗(3000) as the $$D^{*}_{0}(2P)$$ D0∗(2P) and $$D^{*}_{0}(3P)$$ D0∗(3P) in B decays
Abstract In this paper, we use the instantaneous Bethe–Salpeter method to calculate the semi-leptonic and non-leptonic production of the orbitally excited scalar $$ D_0^* $$ D0∗ in B meson decays. When the final state is 1P state $$ D_0^*(2400) $$ D0∗(2400) , our theoretical decay rate is consistent...
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doaj-0daa63a2116740e9a0005880cc8117e52020-11-25T03:54:38ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522019-09-0179911110.1140/epjc/s10052-019-7305-3Rates of $$D^{*}_{0}(2400)$$ D0∗(2400) , $$ D_J^*(3000) $$ DJ∗(3000) as the $$D^{*}_{0}(2P)$$ D0∗(2P) and $$D^{*}_{0}(3P)$$ D0∗(3P) in B decaysXiao-Ze Tan0Yue Jiang1Tianhong Wang2Tian Zhou3Geng Li4Zi-Kan Geng5Guo-Li Wang6Department of Physics, Harbin Institute of TechnologyDepartment of Physics, Harbin Institute of TechnologyDepartment of Physics, Harbin Institute of TechnologyDepartment of Physics, Harbin Institute of TechnologyDepartment of Physics, Harbin Institute of TechnologyDepartment of Physics, Harbin Institute of TechnologyDepartment of Physics, Harbin Institute of TechnologyAbstract In this paper, we use the instantaneous Bethe–Salpeter method to calculate the semi-leptonic and non-leptonic production of the orbitally excited scalar $$ D_0^* $$ D0∗ in B meson decays. When the final state is 1P state $$ D_0^*(2400) $$ D0∗(2400) , our theoretical decay rate is consistent with experimental data. For $$ D_J^*(3000) $$ DJ∗(3000) final state, which was observed by LHCb collaboration recently and here treated as the orbitally excited scalar $$D^{*}_{0}(2P)$$ D0∗(2P) , its rate is in the order of $$ 10^{-4} \sim 10^{-6}$$ 10-4∼10-6 . We find the special node structure of $$D^{*}_{0}(2P)$$ D0∗(2P) wave function possibly results in the suppression of its branching ratio and the abnormal uncertainty. The 3P states production rate is in the order of $$ 10^{-5}$$ 10-5 .http://link.springer.com/article/10.1140/epjc/s10052-019-7305-3 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Xiao-Ze Tan Yue Jiang Tianhong Wang Tian Zhou Geng Li Zi-Kan Geng Guo-Li Wang |
spellingShingle |
Xiao-Ze Tan Yue Jiang Tianhong Wang Tian Zhou Geng Li Zi-Kan Geng Guo-Li Wang Rates of $$D^{*}_{0}(2400)$$ D0∗(2400) , $$ D_J^*(3000) $$ DJ∗(3000) as the $$D^{*}_{0}(2P)$$ D0∗(2P) and $$D^{*}_{0}(3P)$$ D0∗(3P) in B decays European Physical Journal C: Particles and Fields |
author_facet |
Xiao-Ze Tan Yue Jiang Tianhong Wang Tian Zhou Geng Li Zi-Kan Geng Guo-Li Wang |
author_sort |
Xiao-Ze Tan |
title |
Rates of $$D^{*}_{0}(2400)$$ D0∗(2400) , $$ D_J^*(3000) $$ DJ∗(3000) as the $$D^{*}_{0}(2P)$$ D0∗(2P) and $$D^{*}_{0}(3P)$$ D0∗(3P) in B decays |
title_short |
Rates of $$D^{*}_{0}(2400)$$ D0∗(2400) , $$ D_J^*(3000) $$ DJ∗(3000) as the $$D^{*}_{0}(2P)$$ D0∗(2P) and $$D^{*}_{0}(3P)$$ D0∗(3P) in B decays |
title_full |
Rates of $$D^{*}_{0}(2400)$$ D0∗(2400) , $$ D_J^*(3000) $$ DJ∗(3000) as the $$D^{*}_{0}(2P)$$ D0∗(2P) and $$D^{*}_{0}(3P)$$ D0∗(3P) in B decays |
title_fullStr |
Rates of $$D^{*}_{0}(2400)$$ D0∗(2400) , $$ D_J^*(3000) $$ DJ∗(3000) as the $$D^{*}_{0}(2P)$$ D0∗(2P) and $$D^{*}_{0}(3P)$$ D0∗(3P) in B decays |
title_full_unstemmed |
Rates of $$D^{*}_{0}(2400)$$ D0∗(2400) , $$ D_J^*(3000) $$ DJ∗(3000) as the $$D^{*}_{0}(2P)$$ D0∗(2P) and $$D^{*}_{0}(3P)$$ D0∗(3P) in B decays |
title_sort |
rates of $$d^{*}_{0}(2400)$$ d0∗(2400) , $$ d_j^*(3000) $$ dj∗(3000) as the $$d^{*}_{0}(2p)$$ d0∗(2p) and $$d^{*}_{0}(3p)$$ d0∗(3p) in b decays |
publisher |
SpringerOpen |
series |
European Physical Journal C: Particles and Fields |
issn |
1434-6044 1434-6052 |
publishDate |
2019-09-01 |
description |
Abstract In this paper, we use the instantaneous Bethe–Salpeter method to calculate the semi-leptonic and non-leptonic production of the orbitally excited scalar $$ D_0^* $$ D0∗ in B meson decays. When the final state is 1P state $$ D_0^*(2400) $$ D0∗(2400) , our theoretical decay rate is consistent with experimental data. For $$ D_J^*(3000) $$ DJ∗(3000) final state, which was observed by LHCb collaboration recently and here treated as the orbitally excited scalar $$D^{*}_{0}(2P)$$ D0∗(2P) , its rate is in the order of $$ 10^{-4} \sim 10^{-6}$$ 10-4∼10-6 . We find the special node structure of $$D^{*}_{0}(2P)$$ D0∗(2P) wave function possibly results in the suppression of its branching ratio and the abnormal uncertainty. The 3P states production rate is in the order of $$ 10^{-5}$$ 10-5 . |
url |
http://link.springer.com/article/10.1140/epjc/s10052-019-7305-3 |
work_keys_str_mv |
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