1990
DOI: 10.1007/bf01549679
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Energy distributions of dimuons and diphotons in relativistic heavy ion collisions

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Cited by 5 publications
(8 citation statements)
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“….. 20). Namely, the emission of pairs from the QGP with large invariant mass of about 5GeV is more active than that from the RG; furthermore in this region the dimuon emission from the RG is strongly suppressed because of the presence of the pion form-factor 22 ) (2'6).…”
Section: The /S-to-angular Distribution Of Pairsmentioning
confidence: 98%
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“….. 20). Namely, the emission of pairs from the QGP with large invariant mass of about 5GeV is more active than that from the RG; furthermore in this region the dimuon emission from the RG is strongly suppressed because of the presence of the pion form-factor 22 ) (2'6).…”
Section: The /S-to-angular Distribution Of Pairsmentioning
confidence: 98%
“…20) replacing the variables (El , E 2) by (Cl, C2). It owes the rapidity-independence in the energy-tof) distribution.…”
Section: Conclusion and Commentsmentioning
confidence: 99%
“…From Ref. [12] we get the following relations (Q=QGP, H = H R G , MP=muon pairs, and P P = photon pairs):…”
Section: I~ ( M~) /~= R N ; / [ ( M~-m I )~+ M ; R I ]mentioning
confidence: 99%
“…2 ~e V / f m~) are taken from our earlier papers [9,13]. The total contribution to the pair production rate is given by Following Yoshida [12], we also consider the pairs of particles which are collinearly produced in the transverse direction. In other words, the detectors are assumed to be opposite to each other in the plane perpendicular to the ion-beam axis in the center of the ion-momentum frame.…”
Section: I~ ( M~) /~= R N ; / [ ( M~-m I )~+ M ; R I ]mentioning
confidence: 99%
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