1994
DOI: 10.1103/physrevc.50.1077
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Production of light nuclei in relativistic heavy-ion collisions

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Cited by 51 publications
(19 citation statements)
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“…The penalty factor, namely the reduction of the yield by adding one nucleon, is 307 ± 76. Such an exponential decrease has already been observed at lower incident energies starting from those provided by the AGS [16,18,19,21], yet with different slopes.…”
Section: B Spectra Of Nucleimentioning
confidence: 79%
See 1 more Smart Citation
“…The penalty factor, namely the reduction of the yield by adding one nucleon, is 307 ± 76. Such an exponential decrease has already been observed at lower incident energies starting from those provided by the AGS [16,18,19,21], yet with different slopes.…”
Section: B Spectra Of Nucleimentioning
confidence: 79%
“…The production of light nuclei has attracted attention already at lower incident energies in heavy-ion collisions at the AGS, SPS, and RHIC [16][17][18]. A study of the dependence on √ s NN is of particular interest, because different production mechanisms might dominate at various energies, e.g., a formation via spectator fragmentation at lower energies or via coalescence/thermal mechanisms at higher ones.…”
Section: Published By the American Physical Society Under The Terms Omentioning
confidence: 99%
“…For the chemical freeze-out temperature that currently best describes the LHC data (T ch = 156 MeV), the expected hypertriton yield is dN/dy= 1 ×10 −4 . For 4 Λ H a value dN/dy = 2 ×10 −7 is foreseen, and it is reasonable to assume the same value for 4 Λ He which has a similar mass. For the estimation of the number of reconstructed hypernuclei, the decay branching ratios (B.R.)…”
Section: Discussionmentioning
confidence: 99%
“…In fact, while many Λ-hypernuclei have been observed so far, the first observation of an anti-hypernucleus is rather recent and was reported in the analysis of Au-Au collisions at √ s NN = 200 GeV by the STAR Collaboration at RHIC [3]. Since light hypernuclei are weakly bound nuclear systems, they are sensitive probes of the final stages of the evolution of the fireball formed in the heavy-ion collisions [4].…”
Section: Introductionmentioning
confidence: 99%
“…Measurements of deuteron coalescence in high energy heavy ion collisions have been reported previously both at AGS energies [20][21][22][23][24] from 10 to 14.6 A·GeV/c and at SPS energies [25][26][27][28][29] at 200 or 158 A·GeV/c. Of these, the AGS results of Si+A [20] and Au+Au [22] collisions as well as the SPS results of [25] are of special importance for the present study because they also deal with the systematics of deuteron production as function of rapidity, centrality, mass and transverse mass.…”
Section: Introductionmentioning
confidence: 99%