Overview of GERDA simulation activities with MaGe

Slides:



Advertisements
Similar presentations
Advanced GAmma Tracking Array
Advertisements

Activity for the Gerda-specific part Description of the Gerda setup including shielding (water tank, Cu tank, liquid Nitrogen), crystals array and kapton.
September 14, 2007Hardy Simgen, TAUP 2007 / Sendai1 Status of the GERDA experiment Hardy Simgen Max-Planck-Institut für Kernphysik Heidelberg on behalf.
M. Di Marco, P. Peiffer, S. Schönert
Results from M. Di Marco, P. Peiffer, S. Schönert Thanks to Davide Franco and Marik Barnabe Heider Gerda collaboration meeting, Tübingen 9th-11th.
WP2 Background simulations Outline Execution plan for the third year Progress of the work Activities and news.
GERDA: GERmanium Detector Array
CUORICINO and CUORE Chiara Brofferio Università di Milano – Bicocca and INFN, Sez. di Milano NOW 2004 – Otranto 12 – 17 September 2004 On behalf of the.
GERmanium Detector Array – a Search for Neutrinoless Double Beta Decay X. Liu - MPI für Physik, München Symposium – symmetries and phases in the universe,
Activity report of TG10 L. Pandola (LNGS) for the TG10 group Gerda Collaboration Meeting, February 3-5, 2005 (simulations and background studies)
CRESST Cryogenic Rare Event Search with Superconducting Thermometers Max-Planck-Institut für Physik University of Oxford Technische Universität München.
Topical Workshop in Low Radioactivity Techniques, Sudbury, Canada, August 28-29, 2010 Surface cleaning techniques B. Majorowits a, M. Wójcik b, G. Zuzel.
Planned Transregional Collaborative Research Center TR27: Neutrinos and Beyond Project A4: Development of segmented germanium detectors for the investigation.
C.Vigorito, University & INFN Torino, Italy 30 th International Cosmic Ray Conference Merida, Mexico Search for neutrino bursts from Gravitational stellar.
1 IDM2004 Edinburgh, 9 september 2004 Helenia Menghetti Bologna University and INFN Study of the muon-induced neutron background with the LVD detector.
Monte Carlo Studies on Possible Calibration Sources Kevin Kröninger, MPI für Physik GERDA Collaboration Meeting, DUBNA, 06/27 – 06/29/2005.
M. Wójcik for the GERDA Collaboration Institute of Physics, Jagellonian University Epiphany 2006, Kraków, Poland, 6-7 January 2006.
TG10 status report L. Pandola INFN, Gran Sasso National Laboratories for the TG10 Task Group Gerda Collaboration Meeting, Tuebingen November 9th – 11th,
What is MaGe? MJ outputGERDA output MaGe is a Monte Carlo simulation package dedicated to experiments searching for 0 2  decay in 76 Ge. Created by the.
Half Day IoP Meeting: Neutrinoless Double Beta Decay, University College London, Great Britain The GERDA Experiment at Gran Sasso Grzegorz Zuzel.
Data Processing for the Sudbury Neutrino Observatory Aksel Hallin Queen’s, October 2006.
Results from particle beam tests of the ATLAS liquid argon endcap calorimeters Beam test setup Signal reconstruction Response to electrons  Electromagnetic.
M. Wójcik Instytut Fizyki, Uniwersytet Jagielloński Instytut Fizyki Doświadczalnej, Uniwersytet Warszawski Warszawa, 10 Marca 2006.
The GERDA experiment L. Pandola INFN, Gran Sasso National Laboratory for the GERDA Collaboration WIN2009, Perugia, September 17 th 2009.
MaGe framework for Monte Carlo simulations MaGe is a Geant4-based Monte Carlo simulation package dedicated to experiments searching for 0 2  decay of.
MaGe: a Monte Carlo framework for the GERDA and Majorana experiments Luciano Pandola INFN, Laboratori Nazionali del Gran Sasso for the MaGe development.
Muon and Neutron Backgrounds at Yangyang underground lab Muju Workshop Kwak, Jungwon Seoul National University 1.External Backgrounds 2.Muon.
Cracow Epiphany Conference on Physics in Underground Laboratories and its Connection with LHC Cracow, Poland The GERDA Experiment at Gran.
BACKGROUND REJECTION AND SENSITIVITY FOR NEW GENERATION Ge DETECTORS EXPERIMENTS. Héctor Gómez Maluenda University of Zaragoza (SPAIN)
1 Muon Veto System and Expected Backgrounds at Dayabay Hongshan (Kevin) Zhang, BNL DayaBay Collaboration DNP08, Oakland.
The COBRA Experiment Jeanne Wilson University of Sussex, UK On behalf of the COBRA Collaboration TAUP 2007, Sendai, Japan.
1 LTR 2004 Sudbury, December 2004 Helenia Menghetti, Marco Selvi Bologna University and INFN Large Volume Detector The Large Volume Detector (LVD)
Luciano Pandola, INFN Gran Sasso Luciano Pandola INFN Gran Sasso Genova, July 18 th, 2005 Geant4 and the underground physics community.
GERDA – a Search for Neutrinoless Double Beta Decay MPI für Physik, München Neutrinoless double beta decay and the GERDA experimentThe detector array and.
M.Altmann, GERDA Status Report SNOLAB Workshop IV, Investigating Neutrinoless Double Beta Decay Status of the GERDA Experiment Michael Altmann.
PMN07 Blaubeuren Segmented germanium detectors in 0νββ-decay experiments Kevin Kröninger (Max-Planck-Institut für Physik, München)
Phase I: Use available 76 Ge diodes from Heidelberg- Moscow and IGEX experiments (~18 kg). Scrutinize with high siginificance current evidence. Phase II:
November 19, 2007Hardy Simgen, IDEA-Meeting Paris Status of the GERDA experiment Hardy Simgen Max-Planck-Institut für Kernphysik Heidelberg on behalf.
MPI für Physik, Fachbeirat, Béla Majorovits The GERDA experiment Béla Majorovits.
SIMULATION OF BACKGROUND REDUCTION TECHNIQUES FOR Ge DBD DETECTORS Héctor Gómez Maluenda. University of Zaragoza. GERDA/Majorana MC Meeting.
Double Chooz Experiment Status Jelena Maricic, Drexel University (for the Double Chooz Collaboration) September, 27 th, SNAC11.
Alex Howard, Imperial College Slide 1 July 2 nd 2001 Underground Project UNDERGROUND PROJECT – Overview and Goals Alex Howard Imperial College, London.
AlCap Analysis Discussion Analysis Steps  Protons: BG, response, unfolding Question: perform alternative fast signal analysis  Muons: BG, efficiency.
Towards pulse shape calculation and analysis for the GERDA experiment Kevin Kröninger, MPI für Physik International School of Nuclear Physics, Erice 2005.
ICARUS T600: low energy electrons
From Edelweiss I to Edelweiss II
Status of ULE-HPGe Experiment for WIMP Search in YangYang
B. Majorovits (MPI für Physik) for the collaboration
The MiniBooNE Little Muon Counter Detector
The COBRA Experiment: Future Prospects
On behalf of TEXONO collaboration
L. Pandola INFN, Gran Sasso National Laboratories
Prompt Gamma Activation Analysis on 76Ge
GERDA Collaboration Meeting,
The Heidelberg Dark Matter Search Experiment
Status of 100Mo based DBD experiment
Simulation for DayaBay Detectors
Muon stopping target optimization
Deep learning possibilities for GERDA
Systematic uncertainties in MonteCarlo simulations of the atmospheric muon flux in the 5-lines ANTARES detector VLVnT08 - Toulon April 2008 Annarita.
Simulations of UAr dark matter detectors shielded by LAr vetoes
Pre-Test-stands at MPI Munich
MaGe workshop – summary (my collection!)
Sr-84 0n EC/b+ decay search with SrCl2 crystal
MUPAGE: A fast muon generator
Neutrino Telescope Stefan Schönert (TUM)
Status of Neutron flux Analysis in KIMS experiment
Davide Franco for the Borexino Collaboration Milano University & INFN
西村美紀(東大) 他 MEGIIコラボレーション 日本物理学会 第73回年次大会(2018年) 東京理科大学(野田キャンパス)
GERDA Test Stands for Segmented Germanium Detectors
Presentation transcript:

Overview of GERDA simulation activities with MaGe Luciano Pandola INFN, Laboratori del Gran Sasso MaGe Joint Workshop, Munich, January 2010

Main activities in GERDA that are using MaGe Simulation of the main GERDA set-up (Phase I, Phase II, with segmented/BEGes) Total expected background rate and spectrum Many contributions to be taken into account (require a coherent approach and infrastructure) Calibration system Activity and position of calibration sources Pulse shape simulation Study expected background rejection performances, provide realistic “data” to test reconstruction algorithms Test stands and prototypes Interpretation of data and validation of simulations BeGes (Hd, LNGS, Zurich) and segmented (Munich) Some topics will be described in dedicated talks

GERDA geometries selectable in MaGe - 1 Top muon veto Neck Cryostat Water tank Detector array Directory /gerdageometry Used to simulate the main GERDA setup all infrastructure in place water tank, cryostat, detector array, holders Detector array can be customized in number, type and size of crystals (can be set individually) within the 95 positions available: any combination of segmented, BeGes, non-coax, natGe, enrGe and dimensions (provide they are not too big!)

GERDA geometries selectable in MaGe - 2 Directory /munichteststand Contains about 20 geometries for test stands and screening facilities at Munich, LNGS, Heidelberg and Hades Work performed for data interpretation (e.g. with BEGes) and Monte Carlo validation (e.g. Munich prototypes)

GERDA output schemes The directory /gerdaio contains 12 GERDA specific output schemes Most of them are ROOT-based (+ possibly ASCII outputs) 3 output schemes are related to the main GERDA setup change for the amount/type information they store (radioactive isotopes, neutrons, all hits) Other schemes to be used with tests stands and other GERDA geometries some of them are general enough to be used with other geometries, e.g. file-based geometries tools to dump hit information on ASCII files  interface to external software for pulse shape simulation

MCC2 Campaign - 1 Simulations run for Phase I and Phase II arrangements Phase II array contains: 8 enrGe unsegmented detectors (HdM-IGEX), 14 enrGe 18-fold segmented detectors and 8 natGe unsegmented detectors (GTF) Phase I array has HdM-IGEX-GTF. Individual dimensions considered. Main contributions of energy depositions in crystals: Contamination of materials Neutrons-induced Muon-induced Various physics processes contributing to the energy spectrum are simulated using MaGe

MCC2 Campaign - 2 Final goal: get expectation of full energy spectrum of both phases of GERDA (rate & shape) can also be used “a posteriori” (with a fit) to evaluate contaminations of materials Assumptions: Core and segment thresholds = 10 keV Resolution: 2.5 keV FWHM at 1.332 MeV GTF detectors are considered only for anti-coincidence (not for the energy spectrum) Need to keep track of (many) individual contributions, each with parameters, as half-lifes, activities, etc. ( NEST)

Example: 0nbb decay 0nbb decay of 76Ge in the active volume and dead layer for Phase I and II arrays. Spectrum in the assumption of DBD mediated by massive Majorana neutrinos. Dead layer: 0.8 mm for p-type detectors and negligible for n-type For T1/2 = 1.2 · 1025 y (KK) active volume dead layer bck goal Signal efficiency vs. anti-coincidence cuts (Phase II array) No cuts: 92.0% Det anti-coinc: 91.3% Seg anti-coinc: 87.2%

Example: Prompt m-induced background Prompt m-induced background simulated again with MaGe in the MCC2 framework (Phase I & II). Derived info for new estimate of m-induced delayed background (e.g. 77mGe, 38Cl) Notice: the previous simulation [NIM A 570 (2007) 149] run with different geometry. Used MUSUN to simulate explicitely energy-angle correlation No cut Segment anti-c Results qualititatively consistent with the previous work. For Phase II (at Qbb): 9·10-3 counts/(keV·kg·y) without cuts and 4·10-4 counts/(keV·kg·y) with segment anti-coincidence. Cherenkov veto needed and allows for < 10-5 counts/(keV·kg·y)

Example: n-induced background Water buffer absorbs effectively all external neutrons: main contribution comes from neutrons produced in the setup (specifically, the stainless-steel cryostat!). Global limit to bck from external neutrons: 10-7 cts/(keV·kg·y) nuclear recoils (n,n’g) 1000 kg·y exposure Spectrum due to interactions of n from cryostat Prompt background at Qbb: 7·10-6 cts/(keV·kg·y) with no cut. Reduction by factor of 4 by segment anti-coincidence

Other applications: background from 222Rn in LAr Measurements of the 222Rn cryostat emanation triggered a new Monte Carlo campaign for the background estimate  simulated effect of 222Rn daughters (214Bi and 214Pb) for the Phase I & II arrays Phase II array [uniform 222Rn distribution]: 214Bi no cut 214Pb no cut segmentation segmentation Segmentation cut: factor ~2 at Qbb

Conclusions GERDA Monte Carlo group (aka TG10) uses/develops MaGe as the main simulation tool main GERDA set-up precisely coded, with proper shapes and dimensions customizable in terms of shape, number and dimensions of detectors also many test-stands and prototypes available in MaGe used for data analysis and MC validation other home-made codes used for cross-check and/or as quicker solutions for intensive jobs Ongoing simulations to produce: full background spectrum (not only at Qbb) requires infrastructure to keep track of individual contribution pulse shapes for candidate Phase II detectors