Update on Corsika Simulation 15 June 2015

Slides:

Advertisements

Similar presentations

Masterclass Introduction to hands-on Exercise Aim of the exercise Find out what happens in proton-proton collisions at the LHC as seen by the ATLAS.

Advertisements

E. Mocchiutti, INFN Trieste - CALOR th June 2006, Chicago E. Mocchiutti 1, M. Albi 1, M. Boezio 1, V. Bonvicini 1, J. Lund 2, J. Lundquist 1, M.

Using HOURS to evaluate KM3NeT designs A.Leisos, A. G. Tsirigotis, S.E.Tzamarias In the framework of the KM3NeT Design Study VLVnT Athens, 15 October.

MARS flux simulations - update Sergei Striganov Fermilab June 3, 2009.

Update on Corsika Simulation 29 June 2015 Fabrizio Coccetti 1.

Report of the HOU contribution to KM3NeT TDR (WP2) A. G. Tsirigotis In the framework of the KM3NeT Design Study WP2 Meeting - Marseilles, 29June-3 July.

I3PropagatorMMC module Dmitry Chirkin, LBNL IceCube meeting, Uppsala, 2004.

Atmospheric shower simulation studies with CORSIKA Physics Department Atreidis George ARISTOTLE UNIVERSITY OF THESSALONIKI.

CHEP06, Mumbai-India, Feb 2006V. Daniel Elvira 1 The CMS Simulation Validation Suite V. Daniel Elvira (Fermilab) for the CMS Collaboration.

MMC and UCR icetray modules Dima Chirkin, LBNL Presented by Spencer Klein Tau 2-bang Coincident showers.

Ronald Bruijn – 10 th APP Symposium Antares results and status Ronald Bruijn.

Beam Background Simulations for HL-LHC at IR1 Regina Kwee-Hinzmann, R.Bruce, A.Lechner, N.V.Shetty, L.S.Esposito, F.Cerutti, G.Bregliozzi, R.Kersevan,

Alexander Richards, UCL 1 Atlfast and RTT (plus DCube) Christmas Meeting 18/12/2007.

XXXI International Cosmic Ray Conference, ICRC 2009 Lodz, Poland, July 7-15, 2009 Time structure of the Extensive Air Shower front with the ARGO-YBJ experiment.

Detection of electromagnetic showers along muon tracks Salvatore Mangano (IFIC)

Detector Monte-Carlo ● Goal: Develop software tools to: – Model detector performance – Study background issues – Calculate event rates – Determine feasibility.

Cosmic rays at sea level. There is in nearby interstellar space a flux of particles—mostly protons and atomic nuclei— travelling at almost the speed of.

CBM Software Meeting 1 CBM Simulation & Analysis Framework Geant3 / Gean4 configuration M. Al-Turany, D. Bertini.

Hadronic interaction studies with the ARGO-YBJ experiment (5,800 m 2 ) 10 Pads (56 x 62 cm 2 ) for each RPC 8 Strips (6.5 x 62 cm 2 ) for each Pad ( 

Hybrid measurement of CR light component spectrum by using ARGO-YBJ and WFCTA Shoushan Zhang on behalf of LHAASO collaboration and ARGO-YBJ collaboration.

SIGNAL AND BACKGROUND SIMULATION AT THE RECOMBINATION CHAMBER Vadim TALANOV CERN and IHEP, Protvino Joint LHC Machine-Experiments Workshop on Very Forward.

Particle Production of Carbon Target with 20Tto2T5m Configuration at 6.75 GeV (Updated) X. Ding, UCLA Target Studies April 3, /3/14.

Temporal and spatial structure of the Extensive Air Shower front with the ARGO- YBJ experiment 1 - INFN-CNAF, Bologna, Italy 2 - Università del Salento.

Edouard Kistenev for the PHENIX Collaboration Calorimetry based upgrade to PHENIX at RHIC CALOR 2012 Santa Fe, NM, June 4-8, 2012.

Meson Production at Low Proton Beam Energy (Update) X. Ding, UCLA Target Studies May 9, /9/113.

OUTGOING NEUTRONS IN CALET CALET AIMS AT DETECTING UHE CR ELECTRONS HIGH REJECTION FACTOR FOR PROTONS/NUCLEI NEEDED POSSIBLE IMPROVEMENT RESPECT ‘STANDARD’

Reduction of Background in Observation of W Decay Using the Forward Vertex (FVTX) detector at PHENIX Abraham Meles New Mexico State University APS April.

The Performance of the ALICE experiment for cosmic ray physics B. Alessandro, V. Canoa, A. Fernández, M. Rodríguez, M. Subieta for the ALICE Collaboration.

MC study of TREND Ground array Feng Zhaoyang Institute of High Energy Physics,CAS

Space-time structure of signals in scintillation detectors of EAS L.G. Dedenko, G.F. Fedorova, T.M. Roganova and D.A. Podgrudkov.

MDI Simulations at SLAC Takashi Maruyama, Lew Keller, Thomas Markiewicz, Uli Wienands, SLAC MAP Collaboration Meeting, FNAL June 21, 2013.

A Short Course on Geant4 Simulation Toolkit Introduction

Generator status Akiya Miyamoto KEK 23 February 2016.

LHCf Collaboration Meeting, Catania, 4-6 July 2009 MC comparison: Fluka vs Epics Oscar Adriani.

Multi-Strange Hyperons Triggering at SIS 100

R.W. Assmann, V. Boccone, F. Cerutti, M. Huhtinen, A. Mereghetti

Future Imaging Atmospheric Cherenkov Telescopes:

Cosmogenic Muon Background

Measurement of high energy cosmic rays by the new Tibet hybrid experiment J. Huang for the Tibet ASγCollaboration a a Institute of high energy physics,

The ALICE Cosmic Ray Physics Program

Energy Dependence of the UE

Introduction to hands-on Exercise

Kilohertz Decision Making on Petabytes

Methods of Experimental Particle Physics

Is Strangeness production different in the Bulk and in Jets ?

Simulation Project Structure and tasks

Systematic uncertainties in MonteCarlo simulations of the atmospheric muon flux in the 5-lines ANTARES detector VLVnT08 - Toulon April 2008 Annarita.

Pierre Auger Observatory Present and Future

GPAMELA Alessandro Bruno.

B. Hariharan Tata Institute of Fundamental Research, India

Update on coincidences

(CMS GEANT4 simulation)

Litao Zhao Liaoning University&IHEP

Open heavy flavor analysis with the ALICE experiment at LHC

HADRONIC INTERACTION MODELS AND DPMJET-CHARM MODEL

Update on Data Analysis

Pedro Arce (CERN/CIEMAT)

Beam Dump Experiments with Photon and Electron Beams

High Granularity Calorimeter Upgrade Studies

A Short Course on Geant4 Simulation Toolkit Introduction

EEE telescope simulation

Detector Optimization using Particle Flow Algorithm

Search for coincidences and study of cosmic rays spectrum

Low mass dimuon acceptance

ICRC2011, 32ND INTERNATIONAL COSMIC RAY CONFERENCE, BEIJING 2011

“Min-Bias” and the “Underlying Event”

Hit density at scoring planes at r=10, 30, and 50 cm.

Background Simulations at Fermilab

PHYS 3446 – Lecture #18 Monday ,April 9, 2012 Dr. Brandt Calorimeter

Main Design Parameters RHIC Magnets for MEIC Ion Collider Ring

Presentation transcript:

Update on Corsika Simulation 15 June 2015 Fabrizio Coccetti

Choice of Models for Hadronic Interactions After talking with experts (Lorenzo Perrone and Daniele Martello), we decided which models should be used to generate showers for EEE: High-energy Hadronic Interactions: EPOS (this is the only model available in Corsika which reproduces heavy ion data from RHIC *and* LHC ) Low-energy Hadronic Interactions: FLUKA (standard choice)

Configuration EPOS Parameters EPOPAR input ../epos/epos.param !initialization input file for epos EPOPAR fname inics ../epos/epos.inics !initialization input file for epos EPOPAR fname iniev ../epos/epos.iniev !initialization input file for epos EPOPAR fname initl ../epos/epos.initl !initialization input file for epos EPOPAR fname inirj ../epos/epos.inirj !initialization input file for epos EPOPAR fname inihy ../epos/epos.ini1b !initialization input file for epos EPOPAR fname check none EPOPAR fname histo none EPOPAR fname data none EPOPAR fname copy none

Configuration Energy Cuts (Same as ARGO) ECUTS 0.05 0.05 0.00005 0.00005 (GeV) Hadrons, Muons, Electrons, Photons The low energy cut-off of the particle kinetic energy

Configuration Observation Level (Sea level) OBSLEV 0.E2 (cm)

Configuration magnetic field (Rome) MAGNET 24.5 39.4 24.5: is the horizontal component of the Earth’s magnetic field (in μT) to the x-direction of the detector (North) 39.4: is the vertical component of the Earth’s magnetic field (in μT) downwards.

A python package to use Corsika to generate showers on multiple CPUs e3sim is a python package written to perform simulations for the (Extreme Energy Events) EEE experiment. Available on: github.com/centrofermi Multithreading is supported: You have just to specify the number of cores you want to use and the software take care of generating different threads in different cores/CPUs.