Luminosity and luminous region calculations for the LHC
Abstract
The Luminosity and luminous region for an accelerator for bunched beams and a crossing angle are considered. Time averaged values for both are calculated based on the assumptions that the bunch length increases linearly and the intensity decreases exponentially. Specific calculations are made for the forthcoming Large Hadron Collider (LHC).
FAQs
AI
What explains the impact of crossing angle on luminosity calculations?
The analysis finds that increasing the crossing angle significantly reduces both luminosity and luminous region, highlighting its crucial role. Specifically, a change in crossing angle from 0 to 500 µrad impacts luminosity significantly more than slight variations in bunch length.
How does bunch length influence the luminous region in LHC experiments?
A linear increase in bunch length by 30% over 10 hours does not significantly alter the luminous region. This demonstrates that the luminous region remains stable even under conditions of expected bunch length growth.
What are the consequences of excluding the hourglass effect in luminosity estimations?
Neglecting the hourglass effect results in marginal loss in luminosity for the LHC scenarios, specifically for typical parameters like a bunch length of 7.7 cm and a β* of 50 cm. In scenarios where the bunch length increases to 10 cm, the hourglass effect becomes notably important.
When was the evaluation of average luminosity under time decay scenarios conducted?
The evaluation of average luminosity, considering a 30% bunch length increase and exponential intensity decay, was conducted over a simulated 10-hour period. This assessment indicated that the luminous region remains largely unchanged despite these decay patterns.
Why is the hourglass effect often neglected in luminosity calculations?
The study demonstrates that for typical LHC parameters, the hourglass effect contributes negligibly to luminosity, suggesting its exclusion simplifies calculations without significant loss of accuracy. This conclusion is reinforced by extensive numerical integrations that show minimal luminosity variation due to hourglass considerations.
References (6)
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