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Outline

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

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What explains the impact of crossing angle on luminosity calculations?add

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?add

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?add

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?add

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?add

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)

  1. T. Suzuki, "General formulae of luminosity for various types of colliding beam ma- chines". KEK-76-3, (1976).
  2. F. Ruggiero and F. Zimmerman, "Luminosity optimization near the beam-beam limit by increasing bunch length or crossing angle", CERN-SL-2002-005(AP) and PRSTAB 5, 061001, (2002).
  3. B. Muratori, All relevant programs and detailed results available in ' /afs/cern.ch/user/b/bmurator/public/lumi/', (2002).
  4. P. Baudrenghien, "Position of the LHC luminous region". Private communication.
  5. H. Grote and W. Herr, "Nominal and ultimate luminosity performance of the LHC", LHC Project Note 275 (2002).
  6. O. Brüning, Private communication.