X(3872) production and absorption in a hot hadron gas

We calculate the time evolution of the X(3872) abundance in the hot hadron gas produced in the late stage of heavy ion collisions. We use effective field Lagrangians to obtain the production and dissociation cross sections of X(3872). In this evaluation we include diagrams involving the anomalous co...

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Main Authors: L.M. Abreu, K.P. Khemchandani, A. Martínez Torres, F.S. Navarra, M. Nielsen
Format: Article
Language:English
Published: Elsevier 2016-10-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269316304701
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spelling doaj-5172b0cfd31e4ca18d20e534644eab222020-11-24T22:17:44ZengElsevierPhysics Letters B0370-26931873-24452016-10-01761C30330910.1016/j.physletb.2016.08.050X(3872) production and absorption in a hot hadron gasL.M. Abreu0K.P. Khemchandani1A. Martínez Torres2F.S. Navarra3M. Nielsen4Instituto de Física, Universidade Federal da Bahia, 40210-340, Salvador, BA, BrazilFaculdade de Tecnologia, Universidade do Estado do Rio de Janeiro, Rod. Presidente Dutra Km 298, Pólo Industrial, 27537-000, Resende, RJ, BrazilInstituto de Física, Universidade de São Paulo, Caixa Postal 66318, 05315-970, São Paulo, SP, BrazilInstituto de Física, Universidade de São Paulo, Caixa Postal 66318, 05315-970, São Paulo, SP, BrazilInstituto de Física, Universidade de São Paulo, Caixa Postal 66318, 05315-970, São Paulo, SP, BrazilWe calculate the time evolution of the X(3872) abundance in the hot hadron gas produced in the late stage of heavy ion collisions. We use effective field Lagrangians to obtain the production and dissociation cross sections of X(3872). In this evaluation we include diagrams involving the anomalous couplings πD⁎D¯⁎ and XD¯⁎D⁎ and also the couplings of the X(3872) with charged D and D⁎ mesons. With these new terms the X(3872) interaction cross sections are much larger than those found in previous works. Using these cross sections as input in rate equations, we conclude that during the expansion and cooling of the hadronic gas, the number of X(3872), originally produced at the end of the mixed QGP/hadron gas phase, is reduced by a factor of 4.http://www.sciencedirect.com/science/article/pii/S0370269316304701
collection DOAJ
language English
format Article
sources DOAJ
author L.M. Abreu
K.P. Khemchandani
A. Martínez Torres
F.S. Navarra
M. Nielsen
spellingShingle L.M. Abreu
K.P. Khemchandani
A. Martínez Torres
F.S. Navarra
M. Nielsen
X(3872) production and absorption in a hot hadron gas
Physics Letters B
author_facet L.M. Abreu
K.P. Khemchandani
A. Martínez Torres
F.S. Navarra
M. Nielsen
author_sort L.M. Abreu
title X(3872) production and absorption in a hot hadron gas
title_short X(3872) production and absorption in a hot hadron gas
title_full X(3872) production and absorption in a hot hadron gas
title_fullStr X(3872) production and absorption in a hot hadron gas
title_full_unstemmed X(3872) production and absorption in a hot hadron gas
title_sort x(3872) production and absorption in a hot hadron gas
publisher Elsevier
series Physics Letters B
issn 0370-2693
1873-2445
publishDate 2016-10-01
description We calculate the time evolution of the X(3872) abundance in the hot hadron gas produced in the late stage of heavy ion collisions. We use effective field Lagrangians to obtain the production and dissociation cross sections of X(3872). In this evaluation we include diagrams involving the anomalous couplings πD⁎D¯⁎ and XD¯⁎D⁎ and also the couplings of the X(3872) with charged D and D⁎ mesons. With these new terms the X(3872) interaction cross sections are much larger than those found in previous works. Using these cross sections as input in rate equations, we conclude that during the expansion and cooling of the hadronic gas, the number of X(3872), originally produced at the end of the mixed QGP/hadron gas phase, is reduced by a factor of 4.
url http://www.sciencedirect.com/science/article/pii/S0370269316304701
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AT kpkhemchandani x3872productionandabsorptioninahothadrongas
AT amartineztorres x3872productionandabsorptioninahothadrongas
AT fsnavarra x3872productionandabsorptioninahothadrongas
AT mnielsen x3872productionandabsorptioninahothadrongas
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