1999
DOI: 10.1016/s0370-2693(98)01467-1
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Inverse slope systematics in high-energy p+p and Au+Au reactions

Abstract: We employ the Monte-Carlo PYTHIA to calculate the transverse mass spectra of various hadrons and their inverse slopes T * at m T −m = 1.5−2 GeV in p+p reactions at √ s = 200 GeV. Due to (multiple) minijet production T * in general increases as a function of the hadron mass. Moreover, the T * (m) systematics has a "discontinuity" at the charm threshold, i.e. the inverse slope of D-mesons is much higher than that of non-charmed hadrons and even of the heavier Λ C baryon. The experimental observation of this char… Show more

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Cited by 18 publications
(22 citation statements)
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“…1. This explanation is in the line with the typical hydrodynamical calculations (see, for instance, [12]) -the inverse slope parameter T * of the hadron is smaller, if it decouples early, i.e., at higher temperatures T f , but smaller velocity v f T . A more careful analysis requires the combination of the hydrodynamic approach at the early stage of the expansion with cascade model calculations at the latest stage [13,14].…”
supporting
confidence: 86%
See 1 more Smart Citation
“…1. This explanation is in the line with the typical hydrodynamical calculations (see, for instance, [12]) -the inverse slope parameter T * of the hadron is smaller, if it decouples early, i.e., at higher temperatures T f , but smaller velocity v f T . A more careful analysis requires the combination of the hydrodynamic approach at the early stage of the expansion with cascade model calculations at the latest stage [13,14].…”
supporting
confidence: 86%
“…The hydrodynamic calculations of Ref. [12] [12]. In fact, the situation is even more uncertain as the dynamical transport calculations of the HSD model (Hadron String Dynamics) made for RHIC energy [28] predict a rather small inverse slope of about 225 MeV for all particle species.…”
mentioning
confidence: 99%
“…The different scenarios of 'charmonium melting' and 'hadronic comover dissociation' may clearly be distinguished at FAIR energies (of about [25][26][27][28][29][30][31][32][33][34][35], where the centrality dependence of the J/Ψ survival probability and the Ψ ′ to J/Ψ ratio are significantly lower in the 'comover absorption' model than in the 'charmonium melting' scenario. This result comes about since the average comover density decreases only moderately with lower bombarding energy, whereas the region in space-time with energy densities above critical values of e.g.…”
Section: Discussionmentioning
confidence: 99%
“…in collision energy. The dependence of the inverse slope parameter T (and therefore of the p T ) on particle mass has previously been proposed to be due to an increasing contribution to the transverse momentum spectra from minijet production in p + p and p + p collisions [35]. The contribution is expected to be even greater for higher mass particles [36].…”
Section: Mean Transverse Momentummentioning
confidence: 97%