Measurement of the [lambda]3H lifetime in Au+Au collisions at the BNL relativistic heavy ion collider

An improved measurement of the 3ΛH lifetime is presented. In this paper, the mesonic decay modes 3ΛH→3He + π− and 3ΛH→d+p+π− are used to reconstruct the 3ΛH from Au+Au collision data collected by the STAR collaboration at Relativistic Heavy Ion Collider (RHIC). A minimum χ2 estimation is used to det...

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Bibliographic Details
Main Authors: Adamczyk, Leszek (Author) , Deppner, Ingo Martin (Author) , Herrmann, Norbert (Author)
Corporate Author: STAR Collaboration (Author)
Format: Article (Journal)
Language:English
Published: 22 May 2018
In: Physical review
Year: 2018, Volume: 97, Issue: 5
ISSN:2469-9993
DOI:10.1103/PhysRevC.97.054909
Online Access:Verlag, Volltext: https://doi.org/10.1103/PhysRevC.97.054909
Verlag, Volltext: https://link.aps.org/doi/10.1103/PhysRevC.97.054909
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Author Notes:L. Adamczyk, I.M. Deppner, N. Herrmann [und 347 weitere] (STAR Collaboration)
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Summary:An improved measurement of the 3ΛH lifetime is presented. In this paper, the mesonic decay modes 3ΛH→3He + π− and 3ΛH→d+p+π− are used to reconstruct the 3ΛH from Au+Au collision data collected by the STAR collaboration at Relativistic Heavy Ion Collider (RHIC). A minimum χ2 estimation is used to determine the lifetime of τ=142+24−21(stat.)±29(syst.) ps. This lifetime is about 50% shorter than the lifetime τ=263±2 ps of a free Λ, indicating strong hyperon-nucleon interaction in the hypernucleus system. The branching ratios of the mesonic decay channels are also determined to satisfy B.R.(3He+π−)/(B.R.(3He+π−)+B.R.(d+p+π−))=0.32±0.05(stat.)±0.08(syst.). Our ratio result favors the assignment J(3ΛH)=12 over J(3ΛH)=32. These measurements will help to constrain models of hyperon-baryon interactions.
Item Description:Im Titel sind "3" und "Lambda" untereinander geschrieben: "3" hochgestellt, "Lambda" tiefgestellt
Im Titel wird Lambda als griechischer Buchstabe dargestellt
Gesehen am 05.07.2019
Physical Description:Online Resource
ISSN:2469-9993
DOI:10.1103/PhysRevC.97.054909