Mass dependence of light-nucleus production in ultrarelativistic heavy-ion collisions

T. A. Armstrong, K. N. Barish, S. Batsouli, S. J. Bennett, A. Chikanian, S. D. Coe, T. M. Cormier, R. Davies, C. B. Dover, P. Fachini, B. Fadem, L. E. Finch, N. K. George, S. V. Greene, P. Haridas, J. C. Hill, A. S. Hirsch, R. Hoversten, H. Z. Huang, H. JaradatB. S. Kumar, T. Lainis, J. G. Lajoie, R. A. Lewis, Q. Li, B. Libby, R. D. Majka, T. E. Miller, M. G. Munhoz, J. L. Nagle, I. A. Pless, J. K. Pope, N. T. Porile, C. A. Pruneau, M. S.Z. Rabin, J. D. Reid, A. Rimai, A. Rose, F. S. Rotondo, J. Sandweiss, R. P. Scharenberg, A. J. Slaughter, G. A. Smith, M. L. Tincknell, W. S. Toothacker, G. Van Buren, F. K. Wohn, Z. Xu

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Abstract

Light nuclei can be produced in the central reaction zone via coalescence in relativistic heavy-ion collisions. Experiment 864 at BNL has measured the production of ten light nuclei with nuclear number A = 1 to A = 7 at rapidity y ≃ 1.9 and pT/A ≤ 300 MeV/c. Data were taken with a Au beam of momentum of 11.5AGeV/c on a Pb or Pt target with different experimental settings. The invariant yields show a striking exponential dependence on nuclear number with a penalty factor of about 50 per additional nucleon. Detailed analysis reveals that the production may depend on the spin factor of the nucleus and the nuclear binding energy as well.

Original languageEnglish
Pages (from-to)5431-5434
Number of pages4
JournalPhysical Review Letters
Volume83
Issue number26
DOIs
StatePublished - Jan 1 1999
Externally publishedYes

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