# Recent Developments in CMS Fast Simulation

**Authors:** Sezen Sekmen (for the CMS Collaboration)

arXiv: 1701.03850 · 2019-08-13

## TL;DR

CMS's fast simulation framework offers a quick, reliable alternative to detailed simulation, improving efficiency and accuracy for large-scale physics event analysis at the LHC.

## Contribution

The paper introduces recent improvements in CMS fast simulation, especially in tracking and geometry, enhancing performance and synchronization with full simulation.

## Key findings

- Enhanced agreement between fast and full simulation results.
- Improved flexibility and performance in detector component emulation.
- Better synchronization with detailed GEANT4-based simulation.

## Abstract

CMS has developed a fast detector simulation package, which serves as a fast and reliable alternative to the detailed GEANT4-based (full) simulation, and enables efficient simulation of large numbers of standard model and new physics events. Fast simulation becomes particularly important with the current increase in the LHC luminosity. Here, I will discuss the basic principles behind the CMS fast simulation framework, and how they are implemented in the different detector components in order to simulate and reconstruct sufficiently accurate physics objects for analysis. I will focus on recent developments in tracking and geometry interface, which improve the flexibility and emulation performance of the framework, and allow a better synchronization with the full simulation. I will then show how these developments have led to an improved agreement of basic analysis objects and event variables between fast and full simulation.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1701.03850/full.md

## Figures

17 figures with captions in the complete paper: https://tomesphere.com/paper/1701.03850/full.md

## References

3 references — full list in the complete paper: https://tomesphere.com/paper/1701.03850/full.md

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Source: https://tomesphere.com/paper/1701.03850