High Energy Particle Spectra From Peroton Interactions At 192 Gev C PDF Download

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Nuclear Science Abstracts

Nuclear Science Abstracts
Author:
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Total Pages: 722
Release: 1976-02
Genre: Nuclear energy
ISBN:

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Charged Particle Spectra in 32S + 32S Interactions at 200 GeV/nucleon from CCD-imaged Nuclear Collisions in a Streamer Chamber

Charged Particle Spectra in 32S + 32S Interactions at 200 GeV/nucleon from CCD-imaged Nuclear Collisions in a Streamer Chamber
Author:
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Total Pages: 208
Release: 1992
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ISBN:

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We have measured the transverse momentum spectra 1/p[sub T] dN/dp[sub T] and rapidity distributions dN/dy of negatively charged hadrons and protons for central [sup 32]S + [sup 32]S interactions at 200 GeV/nucleon incident energy. The negative hadron dN/dy distribution is too broad to be accounted for by thermal models which demand isotropic particle emission. It is compatible with models which emphasize longitudinal dynamics, by either a particle production mechanism, as in the Lund fragmentation model, or by introducing one-dimensional hydrodynamic expansion, as in the Landau model. The proton dN/dy distribution, although showing no evidence for a peak in the target fragmentation region, exhibits limited nuclear stopping power. We estimate the mean rapidity shift of participant target protons to be [Delta]y [approximately] 1.5, greater than observed for pp collisions, less than measured in central pA collisions, and much less than would be observed for a single equilibrated fireball at midrapidity. Both the negative hadron and proton dN/dy distributions can be fit by a symmetric Landau two-fireball model. Although the spectrum possesses a two-component structure, a comparison to pp data at comparable center-of-mass energy shows no evidence for enhanced production at low p[sub T]. The two-component structure can be explained by a thermal and chemical equilibrium model which takes into account the kinematics of resonance decay. Using an expression motivated by longitudinal expansion we find the same temperature for both the protons and negative hadrons at freezeout, T[sub f] [approximately] 170 MeV. We conclude that the charged particle spectra of negative hadrons and protons can be accommodated in a simple collision picture of limited nuclear stopping, evolution through a state of thermal equilibrium, followed by longitudinal hydrodynamic expansion until freezeout.


Up-to-date P-p Interaction Modeling and Secondarygamma, E+/- and Neutrino Spectra in Astronomical Environment

Up-to-date P-p Interaction Modeling and Secondarygamma, E+/- and Neutrino Spectra in Astronomical Environment
Author: T. Abe
Publisher:
Total Pages:
Release: 2005
Genre:
ISBN:

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We have calculated spectra of stable secondary particles ({gamma}, e{sup {+-}}, {nu}{sub e}, {bar {nu}}{sub e}, {nu}{sub {mu}}{bar {nu}}{sub {mu}}) produced in high energy p-p interactions in astrophysical environment. The calculation has incorporated the up-to-date rising inelastic cross-sections, the diffraction dissociation process, and the Feynman scaling violation for the first time. We then found that the diffractive process makes secondary particle spectra harder than that of the incident proton; that the rising inelastic cross-section and the scaling violation produces significantly more secondary particles than previous calculations. Combination of the three features explain about a half of the ''GeV Excess'' in the EGRET Galactic diffuse {gamma}-ray spectrum with the local cosmic proton spectrum (power-law index around 2.7). The excess can be fully explained if the proton spectral index in the Galactic ridge is harder by 0.2 than above. As an extension of the calculation, we have parameterized the inclusive secondary particle spectra as functions of the incident proton kinetic energy: we predict {approx} 30% more e{sup +} and {nu}{sub e} than e{sup -} and {bar {nu}}{sub e} to be produced in the GeV range by p-p interactions.