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1 CUORE and Backgrounds in Undeground Physics Sachi Wagaarachchi UC Berkeley

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Page 1: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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CUORE and Backgrounds in Undeground Physics

Sachi WagaarachchiUC Berkeley

Page 2: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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Outline...Outline...

● CUORE– Backgrounds and sources– Reducing backgrounds– Expected backgounds for CUORE/CUPID

● Overview of backgrounds,

Natural radioactive chains, cosmic rays, etc

Page 3: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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CUORECUORE

● Super brief overview, – What is 0νββ, why is it important,– How cuore is trying to measure it,– History and results

● Results → backgrounds,– Discuss sources– Methods of reduction,– Expected results from reduction methods

Page 4: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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Neutrinoless Double Beta DecayNeutrinoless Double Beta Decay

● 2νββ → one of the most rare processes observed– Only observable in nuclei whose structure prohibits beta decay

● 0νββ → prohibited by the Standard Model due to lepton number violation– Observation → Majorana nature of neutrino! New physics!

● Current limits >10e25 yrs

Page 5: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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Search for 0nubbSearch for 0nubb

● Peak at the endpoint of 2νββ spectrum

● At the Q value

● Needs good energy resolution,

● Very low background

Page 6: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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CUORE: Bolometric techniqueCUORE: Bolometric technique

Crystal Absorber (TeO2): E → ΔT Biased T sensor (NTD-Ge): ΔT → ΔV Thermal link (PTFE+gold wires): T0~10 mK

Particle energy is converted into phononsby dielectric and diamagnetic absorbers

whose heat capacity (C∝T3) is very low at low T. (At T~10 mK DT ~300 mK @ 1 MeV)ΔT=

EC (T )

Δt=CG

Page 7: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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CUORE UndergroundCUORE Underground

● Average Depth: ~1400m of rock

● Water Equivalent: 3650 m● Reduces mu flux by a

factor of 106

Located in the Gran Sasso National Lab, Italy.

In Hall A, (Same hall as CRESST and GERDA)

Page 8: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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CUORE ProgramCUORE Program

MiDBD1.8 kg 130Te

1997-2001

Cuoricino11.3 kg 130Te

2003-2009

T1/20ν > 2.8 x 1024 y T1/2

0ν > 2.1 x 1023 y

2013-2015 Begin 2016

CUORE-010.9 kg 130Te

CUORE209 kg 130Te

T1/20ν > 4.0x 1024 y

Page 9: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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CUORE● 19 Towers, 988 TeO2 Crystals. 5x5x5cm each

● Total Active Mass: 741kg (~200kg 130Te)● Energy resolution: 5keV @2615 keV (FWHM)● Background Aim: 10-2 counts/keV/kg/year

DetectorsDetectors

CUORE - 0● One Tower of 52 130Te Crystals. 5x5x5cm3 each

● Total Active Mass: 39kg TeO2 (~11kg 130Te)

● Energy resolution: 5keV @2615 keV (FWHM)● Background: ~0.06 counts/keV/kg/year

Page 10: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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CUORE-0 resultsCUORE-0 results

Cuorecino CUORE-0

0vbb Half life 2.8x1024 yr 2.7x1024 yr

Combined with Cuorecino 4.0x1024 yr

Resolution 5.8keV 4.9keV

Selection Efficiency ~83% ~81.3%

1. e+/e-

2. 214Bi, 3. 40K4. 208Tl, 5. 60Co, 6. 228Ac

Page 11: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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Backgrounds: OverviewBackgrounds: Overview

● Cosmic Background● 238U Chain● 232Th Chain● 40K● Intrinsic detector material● Other radioactive sources

Nuclear fallout material, cosmogenically activated detector and construction material

Page 12: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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Cosmic BackgroundCosmic Background

● Cosmic ray primaries and secondaries● Cosmic muons

Page 13: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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● Mainly n,p, π, e ● Do not travel far due to higher interaction cross sections

– Not a problem for underground detector experiments

Cosmic backgroundsCosmic backgrounds

Page 14: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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Cosmic Muon backgroundCosmic Muon background

● Cosmic rays that hit earth are mostly p and α ~99%, – collisions of which produce cascade events producing muons, neutrinos,

e, e+ and γ s● Muons interact much less, and hence make up most of the cosmic

ray products that reach the surface.● These are mostly produced high in the atmosphere (~15km) with

an average energy of 6GeV● With contributions from pion and kaon decay, the intensity fit is

approximately, (for E > 100/Cosθ GeV)

● Intensity of muons on the surface ~70 m-2s-1sr-1 Or 1 min-1.cm-2 for a horizontal detector

Page 15: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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Muon InteractionsMuon Interactions

● Muons loose energy by bremsstrahlung, pair production and photonuclear interactions,

a. Scattering,b. Bremsstrahlungc. Pair productiond. Photonuclear interaction

Page 16: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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Muons...Muons...

● Reduced flux underground, by factor of 10-6

● Still a decent background, 2 counts/year/kg (??)

Page 17: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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232Th Chain232Th Chain

● One of the two main contributors for backgrounds

Page 18: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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CUORE Background from 232ThCUORE Background from 232Th

Page 19: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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238U Chain238U Chain

Page 20: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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Detector radioactivityDetector radioactivity

● Intrinsic radioactivity from the detector materials

● Construction materials, Fe, Cu etc

Page 21: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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Reducing backgroundsReducing backgrounds

● Removing the radioactive materials,– Using cleaner materials, cleaning– Cleaner assembly, construction methods

● Shield– External shields,– Detector materials as shields

● Tag and veto,– External tagging– Rejecting events using detector data

Page 22: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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Background sources in CUOREBackground sources in CUORE

Page 23: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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Background sources in CUORE...Background sources in CUORE...

● Breakdown by MC methods and real data...

Page 24: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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Cleaning...Cleaning...

● Choosing cleaner construction materials● Most of the background was due to

surface contamination– Thourough cleaning methods– Assembling in clean room

● Radon free air system● Lead shields● Muon veto system

Page 25: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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CUORE-0 comparisonCUORE-0 comparison

208Tl

Page 26: CUORE and Backgrounds in Undeground Physics · CUORE Program MiDBD 1.8 kg 130Te 1997-2001 Cuoricino 11.3 kg 130Te 2003-2009 T1/2 T 0ν > 2.8 x 1024 y 1/2 0ν > 2.1 x 1023 y 2013-2015

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ConclusionConclusion

● Main background channels for underground physics,

● Go underground,● Clean and Veto