Contribution Oral Presentation
Production of sexaquark (uuddss) in high-energy collisions
Speakers
- Prof. Sonia KABANA
Primary authors
- Dr. Zhi-Lei et al SHE (Wuhan Textile Uiversity)
- Prof. Sonia KABANA (Universidad de Tarapaca)
Content
The sexaquark is a stable state with quark content ( u u d d s s) hypothesized by [1] which might be a candidate for dark matter in the Universe. We present results on coalescence [2] production of the sexaquark using the parton and hadron cascade model PACIAE in p+p collisions at sqrt(s) = 7 TeV. The yields, yield ratios, and dependences of the spatial parameters (the size of the diquark D 0 and the radius of the sexaquark R 0) of a (anti)sexaquark are predicted. The yields of the hadronic H-dibaryon molecule H ( Λ Λ) generated in the final hadronic state are also compared. These estimates provide references for future sexaquark searches and other exotic state studies, such as dibaryons.
[1] Stable Sexaquark, Glennys R. Farrar(New York U., CCPP), e-Print: 1708.08951 [2] Coalescence production of sexaquark with three diquarks in high-energy nuclear collisions, Zhi-Lei She(Wuhan Textile U.) et al., Phys.Rev.D 112 (2025) 3, 034002 • e-Print: 2502.17381 [hep-ph]
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