Methods and Results for Standard Model Event Generation at $$\sqrt{s}$$ = 14 TeV, 33 TeV and 100 TeV Proton Colliders (A Snowmass Whitepaper)
Abstract
This document describes the novel techniques used to simulate the common Snowmass 2013 En- ergy Frontier Standard Model backgrounds for future hadron colliders. The purpose of many Energy Frontier studies is to explore the reach of high luminosity data sets at a variety of high energy collid- ers. The generation of high statistics samples which accurately model large integrated luminosities for multiple center-of-mass energies and pile-up environments is not possible using an unweighted event generation strategy | an approach which relies on event weighting was necessary. Even with these improvements in e ciency, extensive computing resources were required. This document de- scribes the speci c approach to event generation using Madgraph5 to produce parton-level processes, followed by parton showering and hadronization with Pythia6, and pile-up and detector simulation with Delphes3. The majority of Standard Model processes for pp interactions at √s = 14, 33, and 100 TeV with 0, 50, and 140 additional pile-up interactions are publicly available.
- Authors:
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States). et al.
- Publication Date:
- Research Org.:
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
- OSTI Identifier:
- 1128125
- Report Number(s):
- SNOW13-00167
arXiv eprint number arXiv:1308.1636
- DOE Contract Number:
- AC02-07CH11359
- Resource Type:
- Technical Report
- Resource Relation:
- Conference: Community Summer Study 2013, Minneapolis, MN (United States), 29 Jul-06 Aug 2013
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
Citation Formats
Avetisyan, Aram. Methods and Results for Standard Model Event Generation at $\sqrt{s}$ = 14 TeV, 33 TeV and 100 TeV Proton Colliders (A Snowmass Whitepaper). United States: N. p., 2013.
Web. doi:10.2172/1128125.
Avetisyan, Aram. Methods and Results for Standard Model Event Generation at $\sqrt{s}$ = 14 TeV, 33 TeV and 100 TeV Proton Colliders (A Snowmass Whitepaper). United States. doi:10.2172/1128125.
Avetisyan, Aram. Wed .
"Methods and Results for Standard Model Event Generation at $\sqrt{s}$ = 14 TeV, 33 TeV and 100 TeV Proton Colliders (A Snowmass Whitepaper)". United States.
doi:10.2172/1128125. https://www.osti.gov/servlets/purl/1128125.
@article{osti_1128125,
title = {Methods and Results for Standard Model Event Generation at $\sqrt{s}$ = 14 TeV, 33 TeV and 100 TeV Proton Colliders (A Snowmass Whitepaper)},
author = {Avetisyan, Aram},
abstractNote = {This document describes the novel techniques used to simulate the common Snowmass 2013 En- ergy Frontier Standard Model backgrounds for future hadron colliders. The purpose of many Energy Frontier studies is to explore the reach of high luminosity data sets at a variety of high energy collid- ers. The generation of high statistics samples which accurately model large integrated luminosities for multiple center-of-mass energies and pile-up environments is not possible using an unweighted event generation strategy | an approach which relies on event weighting was necessary. Even with these improvements in e ciency, extensive computing resources were required. This document de- scribes the speci c approach to event generation using Madgraph5 to produce parton-level processes, followed by parton showering and hadronization with Pythia6, and pile-up and detector simulation with Delphes3. The majority of Standard Model processes for pp interactions at √s = 14, 33, and 100 TeV with 0, 50, and 140 additional pile-up interactions are publicly available.},
doi = {10.2172/1128125},
journal = {},
number = ,
volume = ,
place = {United States},
year = {Wed Aug 07 00:00:00 EDT 2013},
month = {Wed Aug 07 00:00:00 EDT 2013}
}
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