2000
DOI: 10.1007/s100500070076
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Inclusive meson production in peripheral collisions of ultrarelativistic heavy ions

Abstract: There exist several proposals to use Weizsäcker-Williams photons generated by ultrarelativistic heavy ions to produce exotic particles in γγ fusion reactions. To estimate the background conditions for such reactions we analyze various mechanisms of meson production in very peripheral collisions of ultrarelativistic heavy ions at RHIC and LHC energies. Besides γγ fusion they include also electromagnetic γA interactions and strong nucleon-nucleon interactions in grazing AA collisions. All these processes are cha… Show more

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Cited by 9 publications
(7 citation statements)
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“…Several earlier papers considered uranium beams at RHIC with γ = 100. These papers found η ′ production cross-sections of 2.9 mb [35] to 3.6 mb [30]. For lead at the LHC, with γ = 4000 (rather than the planned γ = 2940 which is used here), they find η ′ cross-sections of 30 and 32 mb respectively, compared to the 22 mb found here.…”
Section: Cross Sections Rapidity and Mass Distributionsmentioning
confidence: 64%
“…Several earlier papers considered uranium beams at RHIC with γ = 100. These papers found η ′ production cross-sections of 2.9 mb [35] to 3.6 mb [30]. For lead at the LHC, with γ = 4000 (rather than the planned γ = 2940 which is used here), they find η ′ cross-sections of 30 and 32 mb respectively, compared to the 22 mb found here.…”
Section: Cross Sections Rapidity and Mass Distributionsmentioning
confidence: 64%
“…Usually such kind of interactions are considered in the context of QCD physics [4,5]. An important advantage of this reaction is the low multiplicity in γγ interaction.…”
Section: Introductionmentioning
confidence: 99%
“…During the past years a great deal of attention has been given to the experimental and the theoretical studies of hadronnucleus (h-A) and nucleus-nucleus (A-A) collisions at high energies [1][2][3][4][5][6][7][8]. The aim of this work is to study the space-time development [9] of hadronic interaction under extreme conditions of high energy and baryon densities within nuclear dimensions, which are otherwise available only in the hot early Universe.…”
Section: Introductionmentioning
confidence: 99%