GERDA Meeting, September 2009, LNGS. News from Low-Level-Lab: Attempt to Reduce Neutron Background at Shallow Depths

Similar documents
- The CONUS Experiment - COherent elastic NeUtrino nucleus Scattering

Simulation and verification of the cosmogenic background at the shallow depth GIOVE detector

Neutron Activation of 74 Ge and 76 Ge

Shielding Strategies. Karl Tasso Knöpfle MPI Kernphysik, Heidelberg

Measurement of 39 Ar in Underground Argon for Dark Matter Experiments

Background simulations and shielding calculations

First tests of the big volume ultra low background gamma spectrometer

Compton suppression spectrometry

Design, Construction, Operation, and Simulation of a Radioactivity Assay Chamber

Status of the GERDA experiment

David Reyna Belkis Cabrera-Palmer AAP2010, Japan

Neutrinos. Why measure them? Why are they difficult to observe?

PHYS 3650L - Modern Physics Laboratory

The Very-Near-Site at Chooz a New Experimental Hall to Study CEnNS

GERDA: The GERmanium Detector Array for the search for neutrinoless decays of 76 Ge. Allen Caldwell Max-Planck-Institut für Physik

Neutron Activation of 76Ge

cosmic rays plus interaction with neutrons from fission and (α,n) reactions interaction with cosmic muons and neutrons direct activation

Overview about the Work with Liquid Scintillators

Background by Neutron Activation in GERDA

Results on geoneutrinos at Borexino experiment. Heavy Quarks and Leptons Yamagata Davide Basilico

W. Udo Schröder Departments of Chemistry & of Physics and Astronomy

Neutrino nucleus coherent scattering - Prospects of future reactor experiments with germanium detectors

The Ones That Got Away: Neutron Leakage Spectra

Cosmogenic background for the GERDA experiment. Luciano Pandola INFN, Laboratori del Gran Sasso, Italy

D. Medvedev GEMMA and vgen Nalchik, June 6, Investigation of neutrino properties with Ge detectors on KNPP

Low Background NAA: A powerful tool for Physics of Rare Experiments and Environmental Sciences

arxiv: v1 [physics.ins-det] 26 May 2015

The GERmanium Detector Array

Background Modeling and Materials Screening for the LUX and LZ Detectors. David Malling Brown University LUX Collaboration AARM Meeting February 2011

Studies of the XENON100 Electromagnetic Background

ON THE OMNIPRESENT BACKGROUND GAMMA RADIATION OF THE CONTINUOUS SPECTRUM

Search for 0νββ-decay with GERDA Phase II

Background Studies for the XENON100 Experiment. Alexander Kish Physics Institute, University of Zürich Doktorandenseminar August 30, 2010 UZH

Background Characterization and Rejection in the LZ Detector. David Malling Brown University IDM 2012 July 25, 2012

Low Background Experiments and Material Assay. Tessa Johnson NSSC Summer School July 2016

Rivelazione di neutrini solari - Borexino Lino Miramonti 6 Giugno 2006 Gran Sasso

Experimental Nuclear Astrophysics: Lecture 1. Chris Wrede National Nuclear Physics Summer School June 19 th, 2018

Applied Nuclear Physics (Fall 2006) Lecture 21 (11/29/06) Detection of Nuclear Radiation: Pulse Height Spectra

SuperCDMS SNOLAB: A G2 Dark Matter Search. Ben Loer, Fermilab Center for Particle Astrophysics On behalf of the SuperCDMS Collaboration

Measurements of liquid xenon s response to low-energy particle interactions

Interactive Web Accessible Gamma-Spectrum Generator & EasyMonteCarlo Tools

Setup for an in-situ measurement of the total light extinction of Liquid Argon in GERDA

Neutron flux measurement using fast-neutron activation of 12 B and 12 N isotopes in hydrocarbonate scintillators

GERDA experiment A search for neutrinoless double beta decay. Roberto Santorelli (Physik-Institut der Universität Zürich)

Low Background Counting At SNOLAB

HEROICA: a test facility for the characterization of BEGe detectors for the GERDA experiment

Background rejection techniques in Germanium 0νββ-decay experiments. ν=v

Technical Specifications and Requirements on Direct detection for Dark Matter Searches

A Liquid Argon Scintillation Veto for the GERDA Experiment

Motivation Electron-Tracking Compton Telescope 1 st Flight of SMILE Preparation for next step summary

STATUS OF THE CALIBRATION

Double Beta Present Activities in Europe

Y2 Neutrino Physics (spring term 2017)

Search for Oscillation with Lithium-6 Detector at BR2 Prototype Update and short perspectives

The Dortmund Low Background Facility Low-Background Gamma Ray Spectrometry with an Artificial Overburden

LOW ENERGY SOLAR NEUTRINOS WITH BOREXINO. Lea Di Noto on behalf of the Borexino collaboration

Week 7: Ch. 10 Spec. w/ Scintillation Ctrs. Photomultiplier Devices

The XENON Project. M. Selvi The XENON project

Two Neutrino Double Beta (2νββ) Decays into Excited States

A NEW GENERATION OF GAMMA-RAY TELESCOPE

The Search for θ13 : First Results from Double Chooz. Jaime Dawson, APC

The intense, pulsed positron source EPOS at the Research Centre Dresden-Rossendorf

Flux Studies: Muons & Gamma Rays. By: Akkshay Khoslaa & Duncan Wilmot

Testing Dynamical Reduction Models at the Gran Sasso underground laboratory

Neutrino Physics. Neutron Detector in the Aberdeen Tunnel Underground Laboratory. The Daya Bay Experiment. Significance of θ 13

Half-life measurements using SCEPTAR at ISAC-I

Backgrounds and Sensitivity Expectations for XENON100

Chapter 11: Neutrons detectors

Neutron background and possibility for shallow experiments

Muons in Borexino. SFB Block Meeting. Daniel Bick Universität Hamburg. D. Bick (Uni HH) Muons in Borexino

PANDA-X A New Detector for Dark Matter Search. Karl Giboni Shanghai Jiao Tong University

The DarkSide-50 Outer Detectors

PoS(EPS-HEP2017)074. Darkside Status and Prospects. Charles Jeff Martoff Temple University

A Study of Neutron Shielding Methods for. Experimental Astrophysics

Beam Dump Experiments at JLab and SLAC

Testing Dynamical Reduction Models at the underground Gran Sasso Laboratory

Select Assay Capabilities at PNNL

arxiv: v1 [physics.ins-det] 4 Nov 2017

Synthesis of plastic scintillator. Ildefonso León Monzón Universidad Autónoma de Sinaloa

Gamma-Spectrum Generator

1 Introduction. KOPIO charged-particle vetos. K - RARE Meeting (Frascati) May Purpose of CPV: veto Kl

DarkSide-50: performance and results from the first atmospheric argon run

XENONNT AND BEYOND. Hardy Simgen. WIN 2015 MPIK Heidelberg. Max-Planck-Institut für Kernphysik Heidelberg

Neutron background studies for

arxiv:hep-ex/ v1 15 Aug 2006

Status of the AMoRE experiment searching for neutrinoless double beta decay of 100 Mo

Status of CUORE and Results from CUORICINO. SERGIO DI DOMIZIO UNIVERSITÀ & INFN GENOVA On behalf of the CUORE Collaboration

Introduction to Radiological Sciences Neutron Detectors. Theory of operation. Types of detectors Source calibration Survey for Dose

DARK MATTER SEARCHES AT CANFRANC: ANAIS AND ROSEBUD: an update INTRODUCTION AND EXPERIMENTAL GOALS SUMMARY OF RECENT ACHIEVEMENTS AND EFFORTS

Results from 730 kg days of the CRESST-II Dark Matter Search

Correlated Background measurement in Double Chooz experiment

Detectors for astroparticle physics

The NEXT-100 experiment for Neutrino-less Double Beta decay: Main features, Results from Prototypes and Radiopurity issues.

Investigation and development of the suppression methods of the 42 K background in LArGe

The Nucifer Experiment: Non-Proliferation with Reactor Antineutrinos

An underground cosmic-ray detector made of RPC

UCLA Dark Matter 2014 Symposium. Origins and Distributions of the Backgrounds. 15 min

章飞虹 ZHANG FeiHong INTERNATIONAL SCHOOL OF SUBNUCLEAR PHYSICS Ph.D. student from Institute of High Energy Physics, Beijing

MC Benchmarks for LAr Instrumentation in GERDA

Neutrino Experiments: Lecture 2 M. Shaevitz Columbia University

Transcription:

GERDA Meeting, September 2009, LNGS News from Low-Level-Lab: Attempt to Reduce Neutron Background at Shallow Depths

1. Motivation 1.1 Gamma Spectroscopy at MPI-K Gentner Building Bruno Corrado Low-level-laboratory under 15 m we. overburden 2 detectors with active muon veto (proportional counting chambers)

1. Motivation 1.2 Comparison to GeMPI Corrado at MPI-K GeMPI at LNGS Overburden (mwe.) 15 3800 Active mass (kg) 0.94 2.15 Counts/day/mass [40-2700 kev] (1/d/kg) 3830 30 Sensitivity U/Th (mbq/kg) ~ 1 ~ 0.01 2 orders of magnitude discrepancy in sensitivity

1. Motivation 1.3 Background Components Gerd Heusser, 1993

1. Motivation 1.3 Background Components proportional counters lead Ge N2 copper

1. Motivation 1.3 Background Components cosmic ray μ proportional counters proportional chambers provide anti-coincidence veto for e.m. components lead γ e Ge n N2 copper but delayed neutrons from nuclear interactions difficult to detect

1. Motivation 1.3 Background Components γ-lines from neutron interaction Ge-73m Ge-75m annihilation peak Ge-71m Bremstrahlung & Compton neutron activation of surrounding copper Co-60

1. Motivation 1.4 GIOVE: a New Detector Preliminary design study! Goal: increase of sensitivity by a factor of 5-10 by efficient neutron background reduction GeMPI-oriented construction plus Inner and outer veto system Use of plastic scintillators Borated polyethylene as a neutron shield designed by G.Heusser, B.Mörk

2. Experiments 2.1 Investigation of Neutron Flux Reduction by Borated PE (Geiger, K.W. and Hargrove, C.K.)

2. Experiments 2.1 Investigation of Neutron Flux Reduction by Borated PE No PE 5 cm borated PE 15 cm borated PE 8 cm unborated PE

2. Experiments 2.1 Investigation of Neutron Flux Reduction by Borated PE Ge(n,γ) capture reactions Ge(n,n ) scattering reactions mostly induced by thermal neutrons mostly induced by fast neutrons No PE 5 cm borated PE 15 cm borated PE 8 cm unborated PE

2. Experiments 2.1 Investigation of Neutron Flux Reduction by Borated PE borated (10% mass) unborated Relative reduction (a.u.) integral flux moderated neutrons fast neutrons Absorber thickness (cm)

2. Experiments 2.1 Investigation of Neutron Flux Reduction by Borated PE borated PE (10% mass) Relative reduction (a.u.) Best fit with correction for pedestal due to experimental setup yields mean attenuation length of λ= (6.2 ± 0.6) cm integral flux (data) exp() - fit with pedestal exp() - fit Absorber thickness (cm)

2. Experiments 2.2 Current Test Stand for PE/Lead Configurations varying sequence of borated PE and lead layers pure PE for neutron signal creation (2223 kev gamma line from 1 H(n,γ)reaction)

2. Experiments 2.2 Current Test Stand for PE/Lead Configurations Sequence on top Peak Area at 2223 kev (counts/day) Ratio (%) lead 90±6 100 lead PE 68±4 76 lead PE 67±4 74 lead PE 69±3 77

Attempt to Neutron Background Reduction at Shallow Depths 2. Experiments 2.3 Radio-Purity detector chamber filled with PE Ge PE Activity (mb/kg) Pure PE 5% B-PE 10% B-PE B 2 O 3 Ra-226 < 4 130 ± 3 53 ± 3 573 ± 18 Th-228 < 203 12 ± 2 9 ± 2 50 ± 9 K-40 < 17 22 ± 7 33 ± 8 70 ± 32 about 7 cm of inner copper layer needed for sufficient gamma suppression

3. Conclusions 3.1 The Giove Design Preliminary design study! GeMPI-oriented construction plus Inner and outer veto system Use of plastic scintillators Borated polyethylene as a neutron shield designed by G.Heusser, B.Mörk