2010
DOI: 10.1103/physrevstab.13.091001
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Time evolution of the luminosity of colliding heavy-ion beams in BNL Relativistic Heavy Ion Collider and CERN Large Hadron Collider

Abstract: We have studied the time evolution of the heavy ion luminosity and bunch intensities in the Relativistic Heavy Ion Collider (RHIC), at BNL, and in the Large Hadron Collider (LHC), at CERN. First, we present measurements from a large number of RHIC stores (from Run 7), colliding 100 GeV/nucleon 197 Au 79+ beams without stochastic cooling. These are compared with two different calculation methods. The first is a simulation based on multi-particle tracking taking into account collisions, intrabeam scattering, rad… Show more

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Cited by 19 publications
(24 citation statements)
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References 28 publications
(48 reference statements)
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“…A complete luminosity model for heavy ion runs at both RHIC and LHC is presented in [3]. With tracking and/or solving ODEs (ordinary differential equations), the results agree well with the RHIC Au runs, and the model can be used to predict the luminosity of the LHC lead runs.…”
Section: Luminosity Modelmentioning
confidence: 78%
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“…A complete luminosity model for heavy ion runs at both RHIC and LHC is presented in [3]. With tracking and/or solving ODEs (ordinary differential equations), the results agree well with the RHIC Au runs, and the model can be used to predict the luminosity of the LHC lead runs.…”
Section: Luminosity Modelmentioning
confidence: 78%
“…The decay patterns of the luminosity and the beam intensity are quite different [3]. Moreover, the luminosity decays in 2007 and 2010 are different, and also the intensity decays with and without longitudinal cooling are different.…”
mentioning
confidence: 91%
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“…For example, the longitudinal and transverse damping time due to the radiation mechanism is 825 hour and 1650 hour, respectively. This is compared with LHC at store, 6.3 hour and 12.6 hour, respectively [8].…”
Section: Radiation Dampingmentioning
confidence: 99%
“…The next stage of the modelling is to look at the evolution over a fill using the Collider Time Evolution simulation program [16][17][18], a multi-particle simulation that includes the effects of IBS, luminosity burn-off, radiation damping, etc. Here again, of course, the spread in bunch parameters differentiates the rate of intensity and luminosity decay along the bunch train.…”
Section: Integrated Luminosity Projectionsmentioning
confidence: 99%