Status of ECAP Simulations for the KM3NeT TDR KM3NeT WP2 meeting Rezo Shanidze Paris, 10-11 December 2008.

Slides:



Advertisements
Similar presentations
Apostolos Tsirigotis KM3NeT Design Study: Detector Architecture, Event Filtering and Reconstruction Algorithms XXV Workshop on recent developments in High.
Advertisements

Update on effective volumes and energy reconstruction A. Trovato, INFN - LNS.
R.Shanidze, B. Herold, Th. Seitz ECAP, University of Erlangen (for the KM3NeT consortium) 15 October 2009 Athens, Greece Study of data filtering algorithms.
Trigger issues for KM3NeT the large scale underwater neutrino telescope the project objectives design aspects from the KM3NeT TDR trigger issues outlook.
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.
Use of floating surface detector stations for the calibration of a deep-sea neutrino telescope G. Bourlis, N. A. B. Gizani, A. Leisos, A. G. Tsirigotis,
PROGRESS ON WATER PROPERTIES ON TRACKS RECONSTRUCTION Harold Yepes-Ramirez 09/11/2011.
IMPACT OF WATER OPTICAL PROPERTIES ON RECONSTRUCTION: HINTS FROM THE OB DATA. A PRELIMINARY STUDY ANTARES Collaboration Meeting CERN, February 07 th -10.
PROGRESS ON WATER PROPERTIES ON TRACKS RECONSTRUCTION H Yepes -Ramirez IFIC (CSIC – Universitat de València) ANTARES Collaboration Meeting Strasbourg,
WATER PROPERTIES ON TRACKS RECONSTRUCTION AND DETECTOR PERFORMANCE H Yepes -Ramirez IFIC (CSIC – Universitat de València) ANTARES Collaboration Meeting.
PROGRESS ON WATER PROPERTIES ON TRACKS RECONSTRUCTION H Yepes -Ramirez IFIC (CSIC – Universitat de València) ANTARES Collaboration Meeting Strasbourg,
A feasibility study for the detection of SuperNova explosions with an Undersea Neutrino Telescope A. Leisos, A. G. Tsirigotis, S. E. Tzamarias Physics.
Special Issues on Neutrino Telescopy Apostolos G. Tsirigotis Hellenic Open University School of Science & Technology Particle and Astroparticle Physics.
Antares/KM3NeT M. de Jong. neutrinos  p Scientific motivation: – origin cosmic rays – birth & composition relativistic jets – mechanism of cosmic particle.
KM3NeT detector optimization with HOU simulation and reconstruction software A. G. Tsirigotis In the framework of the KM3NeT Design Study WP2 - Paris,
Coincidence analysis in ANTARES: Potassium-40 and muons  Brief overview of ANTARES experiment  Potassium-40 calibration technique  Adjacent floor coincidences.
J. Barrios, S. Schulte, J.P. Gómez-González. Outline Introduction Data selection and processing MC production Data/MC comparison Event selection Detector.
Apostolos Tsirigotis Simulation Studies of km3 Architectures KM3NeT Collaboration Meeting April 2007, Pylos, Greece The project is co-funded by the.
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.
Status of KM3NeT (Detector Design Optimisations) Christopher Naumann, CEA Saclay – IRFU / SPP for the KM3NeT consortium 44 th Reconcontres de Moriond,
Piera Sapienza – VLVNT Workshop, 5-8 october 2003, Amsterdam Introduction and framework Simulation of atmospheric  (HEMAS and MUSIC) Response of a km.
WP2 meeting, Oct 2006, CPPM Claudine Colnard - NIKHEF Claudine Colnard, Ronald Bruijn, Eleonora Presani, Siemen Meester, Paul Kooijman (presented by Maarten.
Special Issues on Neutrino Telescopy Apostolos G. Tsirigotis Hellenic Open University School of Science & Technology Particle and Astroparticle Physics.
Preliminary MC study on the GRAND prototype scintillator array Feng Zhaoyang Institute of High Energy Physics, CAS, China GRAND Workshop, Paris, Feb. 015.
Why Neutrino ? High energy photons are absorbed beyond ~ 150Mpc   HE  LE  e - e + HE s are unique to probe HE processes in the vicinity of cosmic.
ANTARES  Physics motivation  Recent results  Outlook 4 senior physicists, ~5 PhD students, ~5 technicians M. de Jong RECFA 23 September 2005.
Neutrino Diffuse Fluxes in KM3NeT Rezo Shanidze, Thomas Seitz ECAP, University of Erlangen (for the KM3NeT consortium) 15 October 2009 Athens, Greece.
Report of the HOU contribution to KM3NeT TDR (WP2) A. G. Tsirigotis In the framework of the KM3NeT Design Study WP2 Meeting - Erlangen, May 2009.
Ronald Bruijn – 10 th APP Symposium Antares results and status Ronald Bruijn.
Online Reconstruction used in the Antares-Tarot alert system J ü rgen Brunner The online reconstruction concept Performance Neutrino doublets and high.
NESTOR SIMULATION TOOLS AND METHODS Antonis Leisos Hellenic Open University Vlvnt Workhop.
The ORCA Letter of Intent Oscillation Research with Cosmics in the Abyss ORCA Antoine Kouchner University Paris 7 Diderot- AstroParticle and Cosmology.
R. Coniglione, VLVnT08, Toulon April ‘08 KM3NeT: optimization studies for a cubic kilometer neutrino detector R. Coniglione P. Sapienza Istituto.
Astroparticle physics with large neutrino detectors  Existing detectors  Physics motivation  Antares project  KM3NeT proposal M. de Jong.
Sebastian Kuch, Rezo Shanidze Summary of the Detector Simulation Studies in Erlangen KM3NeT Collaboration Meeting Pylos, Greece, April 2007.
Sebastian Kuch, Rezo Shanidze Preliminary Studies of the KM3NeT Physics Sensitivity KM3NeT Collaboration Meeting Pylos, Greece, April 2007.
Status of Sirene Maarten de Jong. What?  Sirene is yet another program that simulates the detector response to muons and showers  It uses a general.
Comparison of different km3 designs using Antares tools Three kinds of detector geometry Incoming muons within TeV energy range Detector efficiency.
PMT measurements in Antares Oleg Kalekin on behalf of Antares collaboration VLVnT 2011 Erlangen
Parallel session WP2 - Physics analysis and simulation (9:30 ->12:30) 09:30 Diffuse Galactic Flux -Andrew Taylor (DIAS) 09:55 MUPAGE status– Giada Carminati.
C.Distefano KM3NET ‘Physics and Simulation (WP2)’ Oct 24 – 25, 2006 LNS NEMO software Carla Distefano for the NEMO Collaboration KM3NET ‘Physics and Simulation.
Update on neutrino simulation with GENIE Carla Distefano.
MC study of TREND Ground array Feng Zhaoyang Institute of High Energy Physics,CAS
Low energy option for KM3NeT Phase 1? KM3NeT-ORCA (Oscillation Research with Cosmics in the Abyss) P. Coyle, Erlangen 23 June 2012.
Reconstruction code and comparison between Genie and Genhen A. Trovato, C. Distefano, R. Coniglione and P. Sapienza Kick-off ORCA meeting: 6 September.
Update on km3 Clancy James & MC Working Group KM3NeT General Meeting Catania, 21/02/2012.
A proposal for the KM3NeT Computing Model Pasquale Migliozzi INFN - Napoli 1.
Geant4 Simulation for KM3 Georgios Stavropoulos NESTOR Institute WP2 meeting, Paris December 2008.
Towards the TDR KM3NeT-DS WPx Meeting, Paris, Feb , 2009 Uli Katz ECAP / Univ. Erlangen  My private views  Basis for discussion  Decisions taken.
Status of Sirene Maarten de Jong. What?  Sirene is a program that simulates the detector response to muons and showers  It is based on the formalism.
KM3NeT P.Kooijman Universities of Amsterdam & Utrecht for the consortium.
Optical Modules in the KM3NeT optimization studies in Erlangen
Update on the GRB Triggered Shower Analysis
Performance of flexible tower with horizontal extent
Sebastian Kuch University Erlangen-Nürnberg
Pasquale Migliozzi INFN Napoli
Systematic uncertainties in MonteCarlo simulations of the atmospheric muon flux in the 5-lines ANTARES detector VLVnT08 - Toulon April 2008 Annarita.
Astronomy session: a summary
Calculation of detector characteristics for KM3NeT
discovery potential of Galactic sources
Optimization studies of a tower based km3 detector
MUPAGE: A fast muon generator
Karen Andeena, Katherine Rawlinsb, Chihwa Song*a
on behalf of the NEMO Collaboration
MC studies of the KM3NeT physics performance Rezo Shanidze
Search for coincidences and study of cosmic rays spectrum
P. Sapienza, R. Coniglione and C. Distefano
Optimization of tower design
KM3NeT Detector optimisation with FAST-CAL*
Hellenic Open University
Presentation transcript:

Status of ECAP Simulations for the KM3NeT TDR KM3NeT WP2 meeting Rezo Shanidze Paris, December 2008

KM3NeT simulations: from CDR to TDR String design (NIKHEF) Path to TDR : Write up for cable-based design New multi-PMT OM design (from NIKHEF)

Multi-PMT OM in cabled design 5. Optical interface 3. PMT base 2. PMT 4. Communication Concentrator 6. Cooling 1. Glass sphere  from  NIKHEF (E. de Wolf, E. Heine ) presentations  at KM3NeT WP 3/4/5 meeting, Paris, 15-16/19/2008 Multi-PMT OM configurations Reference detector vs. Write-up PMTs () () () () CDR (RefDet) 21 0 Write-up

V3.4 14/10/2008 Write-up for cabled design

KM3NeT detector simulations in ECAP  ANTARES Software: detector physics events PMT hits reconstruction  gendet genhen mupage Simulations in ECAP after CDR km3 reco  New PC-farm in ECAP Erlangen  ANTARES/KM3NeT software installation on PC-farm  mupage for atmospheric-  simulations in KM3NeT PC-farm and ANTARES/KM3NeT related software: Ralf Auer and Claudio Kopper

common disk Space ~ 25 TB ECAP PC-farm with Grid Engine queuing system Used by all ECAP groups: ANTARES, KM3NeT, H.E.S.S., Detector development 260 batch nodes 130 interactive nodes ECAP PC-farm for KM3NeT simulations

New detector configuration V = A x L DU, A = (n-1) 2 xd 2 CDR: L DU = 595 m, d = 95 m, 1.05 km 3 OMs = 225 x 37 St. = 8325; PMTs = (21x8325) New: L DU = 493 m, D= km 3 OMs = 225 x 25 St. = 5625; PMTs = (31x5625)  CDR reference detector  new detector:  same instrumented volume ( 1km 3 ), total photocathode area,  number of detection units ( n x n = 15x15=225)  Down-looking PMTS OM with 31x3” PMTs.  CDR 

Effective Area  Detector configuration: s25om31d105 Effective area of s25om31d105 configuration, calculated for the different conditions.

Detector configuration: s25om31d105 Effective Area vs neutrino angle Next step: Detailed comparison of effective area angular resolution for CDR reference detector and new configuration.

Simulation of atmospheric muons: MUPAGE Input: detector surface and physics information: detector geometry, depth Medium: water/ice zenith angle range [0 o,85 o ] max distance of  from the shower axis in a bundle [100m] Range of muon energy [20,10 5 ] GeV Range bundle multiplicity [0,1000] Output: ascii files in table format Equivalent livetime of simulated run  bundle on a can surface Example from M.Spurio (VLVnT08): R, h ~ 300 / 600 m A=1.4 km 2 depth = 2.5 km w.e. Livetime = 1 month E  > 20 GeV, m=[0,100]. 3.6  10 9 bundles 358 files (2h livetime), 600 GB (ascii) CPU: 360 h (2xIntel Xeon Quad Core, 2.33 GHz)

MUPAGE New simulations with v3.1 ( bug in v2.2, G. Carminati ANTARES PAW meeting, Rome, )  Current  event sample with  mupage v 3.1 : 10 7 events (  -bundles) at 3 different depth: 2500, 3500, 4800 m with same CAN parameters: R ≈1.2 km, h ≈ 0.8 km, A ≈ 10.3 km 2 Depth (km) Live time ( 10 7 ev sec/h)  -mult CPU / 10 6 CPU/10 5 ( km3 ) file size (MB) ( 10 6 ascii) / :29:49 2: 36: / :49:01 2: 42: / :12:31 2:48: MUPAGE ECAP PC-farm ( 10 7 events) atm-  simulation (MUPAGE ) requires large computing resources and large scale simulations could be performed for the selected TDR detector. Livetime = 1 month for KM3NeT ~ 3 x  -bundles /2500 m

MUPAGE data  Angular distribution of  -bundles at 3 different depth Detector at: m m m Solid angle for Neutrino observation  cos    is slightly larger for  4800 m  mupage simulations:  cos  <  For 2.5/3.5/4.8 km  cos  <  /-0.127/

Expected rate in KM3NeT: few x Hz ( 1  in few minutes ) Expected atm-  -rate ( > 5 hit, Hz) : 2500 / 500 / 100 ( > 10 hit, Hz) : 1750 / 360 / 70 ( > 100 hit, Hz) : 40 / 6 / 1 Expected 40 K hits/10  s : ~ 7000 ( for 4kHz/PMT, 4% of PMTs ) Expected, atm-  and 40 K rates in KM3NeT  atm-  hit rate for MultiPMT det. at 2500 m calculated with MUPAGE and KM3 ( 2.5 km ) Mean number of hits ~ 15.5 [ 2.4 / 3.5 / 4.8 km]

Reconstruction of atm-  events Reconstruction of  -events: - necessary to estimate the ate of miss-reconstructed atm-  sample. (keep < 10% for -sample) Reconstruction code in ECAP for KM3NeT: RECO/Aart strategy ( with modifications by S.Kuch ) Example of atm-   reconstruction of  mupage (v2.2) events. No quality cuts !

Summary and outlook KM3NeT detector simulation is fully operational and ECAP PC-farm ( thanks to Ralf Auer and Claudio Copper ! ) Atmospheric  simulations (MUPAGE) are included in the KM3NeT TDR studies. ECAP simulations for TDR will be performed for the cabled design option of the KM3NeT detector. Most of the tools needed for the analysis of simulated events are already developed in ECAP ( PhD of Sebastian Kuch). The results for the KM3NeT TDR simulations should be cross- checked with other groups.