Revisiting radiative decays of $$1^{+-}$$ 1 + - heavy quarkonia in the covariant light-front approach
Abstract We revisit the calculation of the width for the radiative decay of a $$1^{+-}$$ 1 + - heavy $$Q \bar{Q}$$ Q Q ¯ meson via the channel $$1^{+-} \rightarrow 0^{-+} +\gamma $$ 1 + - → 0 - + + γ in the covariant light-front quark model. We carry out the reduction of the light-front amplitude in...
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doaj-a170aeebcb6c4ed0931b6c21d6b354d72020-11-25T01:41:37ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522017-04-0177411210.1140/epjc/s10052-017-4818-5Revisiting radiative decays of $$1^{+-}$$ 1 + - heavy quarkonia in the covariant light-front approachYan-Liang Shi0C. N. Yang Institute for Theoretical Physics, Stony Brook UniversityAbstract We revisit the calculation of the width for the radiative decay of a $$1^{+-}$$ 1 + - heavy $$Q \bar{Q}$$ Q Q ¯ meson via the channel $$1^{+-} \rightarrow 0^{-+} +\gamma $$ 1 + - → 0 - + + γ in the covariant light-front quark model. We carry out the reduction of the light-front amplitude in the non-relativistic limit, explicitly computing the leading and next-to-leading order relativistic corrections. This shows the consistency of the light-front approach with the non-relativistic formula for this electric dipole transition. Furthermore, the theoretical uncertainty in the predicted width is studied as a function of the inputs for the heavy-quark mass and wave function structure parameter. We analyze the specific decays $$h_{\mathrm{c}}(1P) \rightarrow \eta _{\mathrm{c}}(1S) + \gamma $$ h c ( 1 P ) → η c ( 1 S ) + γ and $$h_{\mathrm{b}}(1P) \rightarrow \eta _{\mathrm{b}}(1S) + \gamma $$ h b ( 1 P ) → η b ( 1 S ) + γ . We compare our results with experimental data and with other theoretical predictions from calculations based on non-relativistic models and their extensions to include relativistic effects, finding reasonable agreement.http://link.springer.com/article/10.1140/epjc/s10052-017-4818-5 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Yan-Liang Shi |
spellingShingle |
Yan-Liang Shi Revisiting radiative decays of $$1^{+-}$$ 1 + - heavy quarkonia in the covariant light-front approach European Physical Journal C: Particles and Fields |
author_facet |
Yan-Liang Shi |
author_sort |
Yan-Liang Shi |
title |
Revisiting radiative decays of $$1^{+-}$$ 1 + - heavy quarkonia in the covariant light-front approach |
title_short |
Revisiting radiative decays of $$1^{+-}$$ 1 + - heavy quarkonia in the covariant light-front approach |
title_full |
Revisiting radiative decays of $$1^{+-}$$ 1 + - heavy quarkonia in the covariant light-front approach |
title_fullStr |
Revisiting radiative decays of $$1^{+-}$$ 1 + - heavy quarkonia in the covariant light-front approach |
title_full_unstemmed |
Revisiting radiative decays of $$1^{+-}$$ 1 + - heavy quarkonia in the covariant light-front approach |
title_sort |
revisiting radiative decays of $$1^{+-}$$ 1 + - heavy quarkonia in the covariant light-front approach |
publisher |
SpringerOpen |
series |
European Physical Journal C: Particles and Fields |
issn |
1434-6044 1434-6052 |
publishDate |
2017-04-01 |
description |
Abstract We revisit the calculation of the width for the radiative decay of a $$1^{+-}$$ 1 + - heavy $$Q \bar{Q}$$ Q Q ¯ meson via the channel $$1^{+-} \rightarrow 0^{-+} +\gamma $$ 1 + - → 0 - + + γ in the covariant light-front quark model. We carry out the reduction of the light-front amplitude in the non-relativistic limit, explicitly computing the leading and next-to-leading order relativistic corrections. This shows the consistency of the light-front approach with the non-relativistic formula for this electric dipole transition. Furthermore, the theoretical uncertainty in the predicted width is studied as a function of the inputs for the heavy-quark mass and wave function structure parameter. We analyze the specific decays $$h_{\mathrm{c}}(1P) \rightarrow \eta _{\mathrm{c}}(1S) + \gamma $$ h c ( 1 P ) → η c ( 1 S ) + γ and $$h_{\mathrm{b}}(1P) \rightarrow \eta _{\mathrm{b}}(1S) + \gamma $$ h b ( 1 P ) → η b ( 1 S ) + γ . We compare our results with experimental data and with other theoretical predictions from calculations based on non-relativistic models and their extensions to include relativistic effects, finding reasonable agreement. |
url |
http://link.springer.com/article/10.1140/epjc/s10052-017-4818-5 |
work_keys_str_mv |
AT yanliangshi revisitingradiativedecaysof11heavyquarkoniainthecovariantlightfrontapproach |
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1725040610403942400 |