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Mass dependence of light nucleus production in ultrarelativistic heavy ion collisions

Authors :
A. J. Slaughter
S. Bennett
Carl B. Dover
M. S. Z. Rabin
A. Chikanian
Hazim Jaradat
I. A. Pless
M. L. Tincknell
Senta Greene
L. E. Finch
T. E. Miller
R. Davies
B. Libby
J. L. Nagle
John Hill
A. Rimai
Raymond A. Lewis
R. P. Scharenberg
P. Haridas
J. G. Lajoie
M. G. Munhoz
F. K. Wohn
J. K. Pope
S. D. Coe
Claude Andre Pruneau
N. K. George
Thomas Michael Cormier
W. S. Toothacker
G. Van Buren
P. Fachini
Gerald A. Smith
H. Z. Huang
A. A. Rose
B. S. Kumar
R. Hoversten
Z. Z. Xu
S. Batsouli
T. Lainis
Andrew S. Hirsch
J. D. Reid
Q. Li
R. D. Majka
F. S. Rotondo
J. Sandweiss
N. T. Porile
T. A. Armstrong
K. N. Barish
B. Fadem
Publication Year :
1999

Abstract

Light nuclei can be produced in the central reaction zone via coalescence in relativistic heavy ion collisions. E864 at BNL has measured the production of ten light nuclei with nuclear number of A=1 to A=7 at rapidity $y\simeq1.9$ and $p_{T}/A\leq300MeV/c$. Data were taken with a Au beam of momentum of 11.5 A $GeV/c$ 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.<br />(6 pages, 3 figures), some changes on text, references and figures' lettering. To be published in PRL (13Dec1999)

Details

Language :
English
Database :
OpenAIRE
Accession number :
edsair.doi.dedup.....4e07e9aaa27ad868a02b7862f7ed38d3