the search of dark matter with ardm detector

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The search of dark matter with ArDM detector Piotr Mijakowski The Andrzej Sołtan Institute For Nuclear Studies (IPJ), Warsaw, Świerk CRACOW EPIPHANY CONFERENCE ON NEUTRINOS AND DARK MATTER 5 - 8 January 2006, Cracow, Poland

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CRACOW EPIPHANY CONFERENCE ON NEUTRINOS AND DARK MATTER 5 - 8 January 2006, Cracow, Poland. The search of dark matter with ArDM detector. Piotr Mijakowski The Andrzej Sołtan Institute For Nuclear Studies (IPJ), Warsaw, Świerk. OUTLINE. I ArDM ( Ar gon D ark M atter) - PowerPoint PPT Presentation

TRANSCRIPT

Page 1: The search of dark matter with ArDM detector

The search of dark matter with ArDM detector

Piotr MijakowskiThe Andrzej Sołtan Institute For Nuclear Studies (IPJ) Warsaw Świerk

CRACOW EPIPHANY CONFERENCE ON NEUTRINOS AND DARK MATTER5 - 8 January 2006 Cracow Poland

PMijakowski Young Researchers Session 8 January 2006 Cracow 2

OUTLINE

I ArDM (Argon Dark Matter)

II Neutron background in dark matter underground searches

III Geant4 neutron background studies

PMijakowski Young Researchers Session 8 January 2006 Cracow 3

part I ndash ArDM

httpneutrinoethzchArDM

ArDM a proposed ton-scale liquid Argon experiment for direct detection of Dark Matter as WIMPs (Weakly Interacting Massive

Particle )

ABadertscher RChandrasekharan LKaufmann AKnecht LKnechtMLaffranchi MMessina GNatterer POtiougova ARubbia JUlbricht

ETH Zurich Switzerland

CAmsler CRegenfus ABuechler-GermannZurich University Switzerland

ABueno MCCarmona-Benitez JLozano-Bahilo SNavas-ConchaUniversity of Granada Spain

IGil-Botella PLadron de Guevara LRomeroCIEMAT Spain

TKozłowski PMijakowski ERondioSoltan Institute (IPJ) Warsaw-Świerk Poland

HChagani EDaw PMajewski VKudryavtsev NSpoonerUniversity of Sheffield England

PMijakowski Young Researchers Session 8 January 2006 Cracow 4

ArDM (cont)

Elastic scattering reaction

+ Arat rest + Arrecoil

ArDMCERN

170

cm

LEM

PMTs

Ar

(10 cm)

LAr(120 cm)

detector design

drift field asymp 4 kVcm

bull Measurement of the recoils of target nuclei [10-100 keV]bull Recoil energy scintillation amp ionization of Argon

GOAL independently detect the light (PMTs) and the charge (Large Electron Multiplier)

bull lightcharge ratio allows to discriminate background events (e vs nuclear recoils)

PMijakowski Young Researchers Session 8 January 2006 Cracow 5

ArDM status

RampD CERN (1 ton prototype)

bull High voltage systembull LEM based charge readoutbull Light detection system (PMTs + VUV reflecting mirrors)bull CAD design and assemby of the detector

KEY POINT UNDERSTAND THE DETECTOR PERFORMANCE

FIRST GOAL proof of principle 39Ar rejection (intrinsic background beta-emitter with decay rate of asymp 1 kHz in a 1 ton detector)

Simulations full detector geom experimental background

PMijakowski Young Researchers Session 8 January 2006 Cracow 6

ArDM prospects

pictures ECocciaTAUP05

TIME SCALE

2006 assembly of detector at CERN test on surface

2007 transport to the Underground Laboratory (Canfranc Spain) installation in experimental hall and mounting of infrastructure + neutron shield

2007 first data taking

CANFRANC LAB (2450 m we)

PMijakowski Young Researchers Session 8 January 2006 Cracow 7

Estimated event rates

asymp 100 eventtonday

asymp 1 eventtonday

for = 10-46asymp 1 eventton100 day

Assuming 30 keV recoil energy threshold M = 100 GeVc2

PMijakowski Young Researchers Session 8 January 2006 Cracow 8

part II ndash Neutron background

Background events

nuclear eventse-like eventspossible to discriminate

bull the same signal from WIMP amp neutron interactions

bull only possible way to distinguish neutron multiple scattering

NEUTRON BACKGROUND SOURCES

local radioactivity (surrounding rock detector components)

muon-induced neutrons

- spontaneous fission 238U

- (n) reactions rsquos from radioactive chains of UTh

MOTIVATION neutron background limits detector sensitivity to WIMPs

PMijakowski Young Researchers Session 8 January 2006 Cracow 9

Neutron background sources

1 neutrons from surrounding rock - 238U and (n) reactionsflux rock ~ 38 times 10-6 n(scm2) CANFRANC ArDM input (preliminary) ~ 13200 ndaysupression neutron shielding

2 neutrons from det components - 238U and (n) reactions flux bdquodetector dependentrdquo ArDM input (preliminary) ~ 74 ndaysupression high-purity materials

3 muon-induced neutrons ndash production in hadronic amp e-m cascades init by rsquos flux -ind ~ 17 times 10-9 n(scm2) CANFRANCArDM input (preliminary) ~ 6 ndaysupression active veto

PMijakowski Young Researchers Session 8 January 2006 Cracow 10

Neutron background energy spectra

only fission spectrum

[1] rock

[2] detector components[3] -ind

plots 1 amp 3 MJ Carson JC Davies et al Astroparticle Physics 21(2004) 667-687

PMijakowski Young Researchers Session 8 January 2006 Cracow 11

part III ndash Geant4 neutron background studies

How many neutron recoils we will have in our experiment

(how many neutrons will enter the detector what energy spectrum how many would interact and produce visible recoils how many would undergo multiple scattering)

ArDM simulation tasks

detailed detector geom (Geant4) verifiaction of sim processes

(elastic scattering neutron capture)

rock neutrons neutrons from det components muon-induced neutrons

other background sources rsquos 39Ar

full detector sim (GRANADA)

PMijakowski Young Researchers Session 8 January 2006 Cracow 12

Geant4 neutron background studies ndash elastic scattering in liquid Argon

coscos

cos~d

ddT

d

dddN ArAr

)cos1(

2)(sincos1 2

2

22

2

2

2

Arn

nArnnAr

n

Ar

Arn

nnAr

Mm

mMTmM

m

M

Mm

mTT

TnltltMn

non relativistic

Argon recoil

spectra from G4

simulation

Tn = 5 keV

Tn = 15 MeV

Tn = 2 MeV

PMijakowski Young Researchers Session 8 January 2006 Cracow 13

SIMULATION- neutron source placed randomly on the walls of fiducial volume

- neutrons going out of the detector are neglected

INPUT

neutrons from rock input energy

spectrum

Geant4 neutron background studies ndash rock neutrons analysis example

n = 38bull10-6 n(scm2)assumed total neutron flux at the

walls of fiducial volume

IN OUR GEOMETRY1 neutron per ~ 65 sec13200 neutrons per day

10 keV threshold

OUTPUT

PMijakowski Young Researchers Session 8 January 2006 Cracow 14

Geant4 neutron background studies ndash rock neutrons analysis example

no of incoming neutrons

13200 nday

- correction for interacting neutrons

Pint~ 577500 nday

- correction for multiplicity

Pmulti~ 537500 ndash 4000= 3500 nday

+ correction for spatial resolution (2 cm)

3700nday

Pinter~57 Pmulti~53

assumed 2cm spatial resolution

visible95

- shielding (CH2) reduction factor 104-106

1-135 events per year

PMijakowski Young Researchers Session 8 January 2006 Cracow 15

Summary amp Outlook

bull ArDM a new project aiming at developing and operating a 1 ton-scale liquid Argon detector for direct detection of WIMPs

bull With a 1 ton prototype we want to show the validity of this design (in particular 39Ar rejection)

bull Neutron shieldings will be addressed in a second phase

bull Investigations on neutron background sources and their interactions inside the detector are also performed (simulations in Geant4)ndash evaluation of expected number of neutron events (data analysis)ndash simulations will help to specify requirements for detector veto and

shielding

SIMULATIONS OUTLOOKbull Energy spectra and flux of incoming neutronsbull Detailed detector geometry in Geant4

BACKUP

PMijakowski Young Researchers Session 8 January 2006 Cracow 17

Geant4 neutron background studies ndash neutron capture in liquid Argon

capture on natural Argon(40Ar - 996 36Ar - 0337 38Ar - 0063)

Initial neutron energy = 10 eV

Average number of rsquos produced = 35

6099 MeV

8788 MeV

6598 MeV

Page 2: The search of dark matter with ArDM detector

PMijakowski Young Researchers Session 8 January 2006 Cracow 2

OUTLINE

I ArDM (Argon Dark Matter)

II Neutron background in dark matter underground searches

III Geant4 neutron background studies

PMijakowski Young Researchers Session 8 January 2006 Cracow 3

part I ndash ArDM

httpneutrinoethzchArDM

ArDM a proposed ton-scale liquid Argon experiment for direct detection of Dark Matter as WIMPs (Weakly Interacting Massive

Particle )

ABadertscher RChandrasekharan LKaufmann AKnecht LKnechtMLaffranchi MMessina GNatterer POtiougova ARubbia JUlbricht

ETH Zurich Switzerland

CAmsler CRegenfus ABuechler-GermannZurich University Switzerland

ABueno MCCarmona-Benitez JLozano-Bahilo SNavas-ConchaUniversity of Granada Spain

IGil-Botella PLadron de Guevara LRomeroCIEMAT Spain

TKozłowski PMijakowski ERondioSoltan Institute (IPJ) Warsaw-Świerk Poland

HChagani EDaw PMajewski VKudryavtsev NSpoonerUniversity of Sheffield England

PMijakowski Young Researchers Session 8 January 2006 Cracow 4

ArDM (cont)

Elastic scattering reaction

+ Arat rest + Arrecoil

ArDMCERN

170

cm

LEM

PMTs

Ar

(10 cm)

LAr(120 cm)

detector design

drift field asymp 4 kVcm

bull Measurement of the recoils of target nuclei [10-100 keV]bull Recoil energy scintillation amp ionization of Argon

GOAL independently detect the light (PMTs) and the charge (Large Electron Multiplier)

bull lightcharge ratio allows to discriminate background events (e vs nuclear recoils)

PMijakowski Young Researchers Session 8 January 2006 Cracow 5

ArDM status

RampD CERN (1 ton prototype)

bull High voltage systembull LEM based charge readoutbull Light detection system (PMTs + VUV reflecting mirrors)bull CAD design and assemby of the detector

KEY POINT UNDERSTAND THE DETECTOR PERFORMANCE

FIRST GOAL proof of principle 39Ar rejection (intrinsic background beta-emitter with decay rate of asymp 1 kHz in a 1 ton detector)

Simulations full detector geom experimental background

PMijakowski Young Researchers Session 8 January 2006 Cracow 6

ArDM prospects

pictures ECocciaTAUP05

TIME SCALE

2006 assembly of detector at CERN test on surface

2007 transport to the Underground Laboratory (Canfranc Spain) installation in experimental hall and mounting of infrastructure + neutron shield

2007 first data taking

CANFRANC LAB (2450 m we)

PMijakowski Young Researchers Session 8 January 2006 Cracow 7

Estimated event rates

asymp 100 eventtonday

asymp 1 eventtonday

for = 10-46asymp 1 eventton100 day

Assuming 30 keV recoil energy threshold M = 100 GeVc2

PMijakowski Young Researchers Session 8 January 2006 Cracow 8

part II ndash Neutron background

Background events

nuclear eventse-like eventspossible to discriminate

bull the same signal from WIMP amp neutron interactions

bull only possible way to distinguish neutron multiple scattering

NEUTRON BACKGROUND SOURCES

local radioactivity (surrounding rock detector components)

muon-induced neutrons

- spontaneous fission 238U

- (n) reactions rsquos from radioactive chains of UTh

MOTIVATION neutron background limits detector sensitivity to WIMPs

PMijakowski Young Researchers Session 8 January 2006 Cracow 9

Neutron background sources

1 neutrons from surrounding rock - 238U and (n) reactionsflux rock ~ 38 times 10-6 n(scm2) CANFRANC ArDM input (preliminary) ~ 13200 ndaysupression neutron shielding

2 neutrons from det components - 238U and (n) reactions flux bdquodetector dependentrdquo ArDM input (preliminary) ~ 74 ndaysupression high-purity materials

3 muon-induced neutrons ndash production in hadronic amp e-m cascades init by rsquos flux -ind ~ 17 times 10-9 n(scm2) CANFRANCArDM input (preliminary) ~ 6 ndaysupression active veto

PMijakowski Young Researchers Session 8 January 2006 Cracow 10

Neutron background energy spectra

only fission spectrum

[1] rock

[2] detector components[3] -ind

plots 1 amp 3 MJ Carson JC Davies et al Astroparticle Physics 21(2004) 667-687

PMijakowski Young Researchers Session 8 January 2006 Cracow 11

part III ndash Geant4 neutron background studies

How many neutron recoils we will have in our experiment

(how many neutrons will enter the detector what energy spectrum how many would interact and produce visible recoils how many would undergo multiple scattering)

ArDM simulation tasks

detailed detector geom (Geant4) verifiaction of sim processes

(elastic scattering neutron capture)

rock neutrons neutrons from det components muon-induced neutrons

other background sources rsquos 39Ar

full detector sim (GRANADA)

PMijakowski Young Researchers Session 8 January 2006 Cracow 12

Geant4 neutron background studies ndash elastic scattering in liquid Argon

coscos

cos~d

ddT

d

dddN ArAr

)cos1(

2)(sincos1 2

2

22

2

2

2

Arn

nArnnAr

n

Ar

Arn

nnAr

Mm

mMTmM

m

M

Mm

mTT

TnltltMn

non relativistic

Argon recoil

spectra from G4

simulation

Tn = 5 keV

Tn = 15 MeV

Tn = 2 MeV

PMijakowski Young Researchers Session 8 January 2006 Cracow 13

SIMULATION- neutron source placed randomly on the walls of fiducial volume

- neutrons going out of the detector are neglected

INPUT

neutrons from rock input energy

spectrum

Geant4 neutron background studies ndash rock neutrons analysis example

n = 38bull10-6 n(scm2)assumed total neutron flux at the

walls of fiducial volume

IN OUR GEOMETRY1 neutron per ~ 65 sec13200 neutrons per day

10 keV threshold

OUTPUT

PMijakowski Young Researchers Session 8 January 2006 Cracow 14

Geant4 neutron background studies ndash rock neutrons analysis example

no of incoming neutrons

13200 nday

- correction for interacting neutrons

Pint~ 577500 nday

- correction for multiplicity

Pmulti~ 537500 ndash 4000= 3500 nday

+ correction for spatial resolution (2 cm)

3700nday

Pinter~57 Pmulti~53

assumed 2cm spatial resolution

visible95

- shielding (CH2) reduction factor 104-106

1-135 events per year

PMijakowski Young Researchers Session 8 January 2006 Cracow 15

Summary amp Outlook

bull ArDM a new project aiming at developing and operating a 1 ton-scale liquid Argon detector for direct detection of WIMPs

bull With a 1 ton prototype we want to show the validity of this design (in particular 39Ar rejection)

bull Neutron shieldings will be addressed in a second phase

bull Investigations on neutron background sources and their interactions inside the detector are also performed (simulations in Geant4)ndash evaluation of expected number of neutron events (data analysis)ndash simulations will help to specify requirements for detector veto and

shielding

SIMULATIONS OUTLOOKbull Energy spectra and flux of incoming neutronsbull Detailed detector geometry in Geant4

BACKUP

PMijakowski Young Researchers Session 8 January 2006 Cracow 17

Geant4 neutron background studies ndash neutron capture in liquid Argon

capture on natural Argon(40Ar - 996 36Ar - 0337 38Ar - 0063)

Initial neutron energy = 10 eV

Average number of rsquos produced = 35

6099 MeV

8788 MeV

6598 MeV

Page 3: The search of dark matter with ArDM detector

PMijakowski Young Researchers Session 8 January 2006 Cracow 3

part I ndash ArDM

httpneutrinoethzchArDM

ArDM a proposed ton-scale liquid Argon experiment for direct detection of Dark Matter as WIMPs (Weakly Interacting Massive

Particle )

ABadertscher RChandrasekharan LKaufmann AKnecht LKnechtMLaffranchi MMessina GNatterer POtiougova ARubbia JUlbricht

ETH Zurich Switzerland

CAmsler CRegenfus ABuechler-GermannZurich University Switzerland

ABueno MCCarmona-Benitez JLozano-Bahilo SNavas-ConchaUniversity of Granada Spain

IGil-Botella PLadron de Guevara LRomeroCIEMAT Spain

TKozłowski PMijakowski ERondioSoltan Institute (IPJ) Warsaw-Świerk Poland

HChagani EDaw PMajewski VKudryavtsev NSpoonerUniversity of Sheffield England

PMijakowski Young Researchers Session 8 January 2006 Cracow 4

ArDM (cont)

Elastic scattering reaction

+ Arat rest + Arrecoil

ArDMCERN

170

cm

LEM

PMTs

Ar

(10 cm)

LAr(120 cm)

detector design

drift field asymp 4 kVcm

bull Measurement of the recoils of target nuclei [10-100 keV]bull Recoil energy scintillation amp ionization of Argon

GOAL independently detect the light (PMTs) and the charge (Large Electron Multiplier)

bull lightcharge ratio allows to discriminate background events (e vs nuclear recoils)

PMijakowski Young Researchers Session 8 January 2006 Cracow 5

ArDM status

RampD CERN (1 ton prototype)

bull High voltage systembull LEM based charge readoutbull Light detection system (PMTs + VUV reflecting mirrors)bull CAD design and assemby of the detector

KEY POINT UNDERSTAND THE DETECTOR PERFORMANCE

FIRST GOAL proof of principle 39Ar rejection (intrinsic background beta-emitter with decay rate of asymp 1 kHz in a 1 ton detector)

Simulations full detector geom experimental background

PMijakowski Young Researchers Session 8 January 2006 Cracow 6

ArDM prospects

pictures ECocciaTAUP05

TIME SCALE

2006 assembly of detector at CERN test on surface

2007 transport to the Underground Laboratory (Canfranc Spain) installation in experimental hall and mounting of infrastructure + neutron shield

2007 first data taking

CANFRANC LAB (2450 m we)

PMijakowski Young Researchers Session 8 January 2006 Cracow 7

Estimated event rates

asymp 100 eventtonday

asymp 1 eventtonday

for = 10-46asymp 1 eventton100 day

Assuming 30 keV recoil energy threshold M = 100 GeVc2

PMijakowski Young Researchers Session 8 January 2006 Cracow 8

part II ndash Neutron background

Background events

nuclear eventse-like eventspossible to discriminate

bull the same signal from WIMP amp neutron interactions

bull only possible way to distinguish neutron multiple scattering

NEUTRON BACKGROUND SOURCES

local radioactivity (surrounding rock detector components)

muon-induced neutrons

- spontaneous fission 238U

- (n) reactions rsquos from radioactive chains of UTh

MOTIVATION neutron background limits detector sensitivity to WIMPs

PMijakowski Young Researchers Session 8 January 2006 Cracow 9

Neutron background sources

1 neutrons from surrounding rock - 238U and (n) reactionsflux rock ~ 38 times 10-6 n(scm2) CANFRANC ArDM input (preliminary) ~ 13200 ndaysupression neutron shielding

2 neutrons from det components - 238U and (n) reactions flux bdquodetector dependentrdquo ArDM input (preliminary) ~ 74 ndaysupression high-purity materials

3 muon-induced neutrons ndash production in hadronic amp e-m cascades init by rsquos flux -ind ~ 17 times 10-9 n(scm2) CANFRANCArDM input (preliminary) ~ 6 ndaysupression active veto

PMijakowski Young Researchers Session 8 January 2006 Cracow 10

Neutron background energy spectra

only fission spectrum

[1] rock

[2] detector components[3] -ind

plots 1 amp 3 MJ Carson JC Davies et al Astroparticle Physics 21(2004) 667-687

PMijakowski Young Researchers Session 8 January 2006 Cracow 11

part III ndash Geant4 neutron background studies

How many neutron recoils we will have in our experiment

(how many neutrons will enter the detector what energy spectrum how many would interact and produce visible recoils how many would undergo multiple scattering)

ArDM simulation tasks

detailed detector geom (Geant4) verifiaction of sim processes

(elastic scattering neutron capture)

rock neutrons neutrons from det components muon-induced neutrons

other background sources rsquos 39Ar

full detector sim (GRANADA)

PMijakowski Young Researchers Session 8 January 2006 Cracow 12

Geant4 neutron background studies ndash elastic scattering in liquid Argon

coscos

cos~d

ddT

d

dddN ArAr

)cos1(

2)(sincos1 2

2

22

2

2

2

Arn

nArnnAr

n

Ar

Arn

nnAr

Mm

mMTmM

m

M

Mm

mTT

TnltltMn

non relativistic

Argon recoil

spectra from G4

simulation

Tn = 5 keV

Tn = 15 MeV

Tn = 2 MeV

PMijakowski Young Researchers Session 8 January 2006 Cracow 13

SIMULATION- neutron source placed randomly on the walls of fiducial volume

- neutrons going out of the detector are neglected

INPUT

neutrons from rock input energy

spectrum

Geant4 neutron background studies ndash rock neutrons analysis example

n = 38bull10-6 n(scm2)assumed total neutron flux at the

walls of fiducial volume

IN OUR GEOMETRY1 neutron per ~ 65 sec13200 neutrons per day

10 keV threshold

OUTPUT

PMijakowski Young Researchers Session 8 January 2006 Cracow 14

Geant4 neutron background studies ndash rock neutrons analysis example

no of incoming neutrons

13200 nday

- correction for interacting neutrons

Pint~ 577500 nday

- correction for multiplicity

Pmulti~ 537500 ndash 4000= 3500 nday

+ correction for spatial resolution (2 cm)

3700nday

Pinter~57 Pmulti~53

assumed 2cm spatial resolution

visible95

- shielding (CH2) reduction factor 104-106

1-135 events per year

PMijakowski Young Researchers Session 8 January 2006 Cracow 15

Summary amp Outlook

bull ArDM a new project aiming at developing and operating a 1 ton-scale liquid Argon detector for direct detection of WIMPs

bull With a 1 ton prototype we want to show the validity of this design (in particular 39Ar rejection)

bull Neutron shieldings will be addressed in a second phase

bull Investigations on neutron background sources and their interactions inside the detector are also performed (simulations in Geant4)ndash evaluation of expected number of neutron events (data analysis)ndash simulations will help to specify requirements for detector veto and

shielding

SIMULATIONS OUTLOOKbull Energy spectra and flux of incoming neutronsbull Detailed detector geometry in Geant4

BACKUP

PMijakowski Young Researchers Session 8 January 2006 Cracow 17

Geant4 neutron background studies ndash neutron capture in liquid Argon

capture on natural Argon(40Ar - 996 36Ar - 0337 38Ar - 0063)

Initial neutron energy = 10 eV

Average number of rsquos produced = 35

6099 MeV

8788 MeV

6598 MeV

Page 4: The search of dark matter with ArDM detector

PMijakowski Young Researchers Session 8 January 2006 Cracow 4

ArDM (cont)

Elastic scattering reaction

+ Arat rest + Arrecoil

ArDMCERN

170

cm

LEM

PMTs

Ar

(10 cm)

LAr(120 cm)

detector design

drift field asymp 4 kVcm

bull Measurement of the recoils of target nuclei [10-100 keV]bull Recoil energy scintillation amp ionization of Argon

GOAL independently detect the light (PMTs) and the charge (Large Electron Multiplier)

bull lightcharge ratio allows to discriminate background events (e vs nuclear recoils)

PMijakowski Young Researchers Session 8 January 2006 Cracow 5

ArDM status

RampD CERN (1 ton prototype)

bull High voltage systembull LEM based charge readoutbull Light detection system (PMTs + VUV reflecting mirrors)bull CAD design and assemby of the detector

KEY POINT UNDERSTAND THE DETECTOR PERFORMANCE

FIRST GOAL proof of principle 39Ar rejection (intrinsic background beta-emitter with decay rate of asymp 1 kHz in a 1 ton detector)

Simulations full detector geom experimental background

PMijakowski Young Researchers Session 8 January 2006 Cracow 6

ArDM prospects

pictures ECocciaTAUP05

TIME SCALE

2006 assembly of detector at CERN test on surface

2007 transport to the Underground Laboratory (Canfranc Spain) installation in experimental hall and mounting of infrastructure + neutron shield

2007 first data taking

CANFRANC LAB (2450 m we)

PMijakowski Young Researchers Session 8 January 2006 Cracow 7

Estimated event rates

asymp 100 eventtonday

asymp 1 eventtonday

for = 10-46asymp 1 eventton100 day

Assuming 30 keV recoil energy threshold M = 100 GeVc2

PMijakowski Young Researchers Session 8 January 2006 Cracow 8

part II ndash Neutron background

Background events

nuclear eventse-like eventspossible to discriminate

bull the same signal from WIMP amp neutron interactions

bull only possible way to distinguish neutron multiple scattering

NEUTRON BACKGROUND SOURCES

local radioactivity (surrounding rock detector components)

muon-induced neutrons

- spontaneous fission 238U

- (n) reactions rsquos from radioactive chains of UTh

MOTIVATION neutron background limits detector sensitivity to WIMPs

PMijakowski Young Researchers Session 8 January 2006 Cracow 9

Neutron background sources

1 neutrons from surrounding rock - 238U and (n) reactionsflux rock ~ 38 times 10-6 n(scm2) CANFRANC ArDM input (preliminary) ~ 13200 ndaysupression neutron shielding

2 neutrons from det components - 238U and (n) reactions flux bdquodetector dependentrdquo ArDM input (preliminary) ~ 74 ndaysupression high-purity materials

3 muon-induced neutrons ndash production in hadronic amp e-m cascades init by rsquos flux -ind ~ 17 times 10-9 n(scm2) CANFRANCArDM input (preliminary) ~ 6 ndaysupression active veto

PMijakowski Young Researchers Session 8 January 2006 Cracow 10

Neutron background energy spectra

only fission spectrum

[1] rock

[2] detector components[3] -ind

plots 1 amp 3 MJ Carson JC Davies et al Astroparticle Physics 21(2004) 667-687

PMijakowski Young Researchers Session 8 January 2006 Cracow 11

part III ndash Geant4 neutron background studies

How many neutron recoils we will have in our experiment

(how many neutrons will enter the detector what energy spectrum how many would interact and produce visible recoils how many would undergo multiple scattering)

ArDM simulation tasks

detailed detector geom (Geant4) verifiaction of sim processes

(elastic scattering neutron capture)

rock neutrons neutrons from det components muon-induced neutrons

other background sources rsquos 39Ar

full detector sim (GRANADA)

PMijakowski Young Researchers Session 8 January 2006 Cracow 12

Geant4 neutron background studies ndash elastic scattering in liquid Argon

coscos

cos~d

ddT

d

dddN ArAr

)cos1(

2)(sincos1 2

2

22

2

2

2

Arn

nArnnAr

n

Ar

Arn

nnAr

Mm

mMTmM

m

M

Mm

mTT

TnltltMn

non relativistic

Argon recoil

spectra from G4

simulation

Tn = 5 keV

Tn = 15 MeV

Tn = 2 MeV

PMijakowski Young Researchers Session 8 January 2006 Cracow 13

SIMULATION- neutron source placed randomly on the walls of fiducial volume

- neutrons going out of the detector are neglected

INPUT

neutrons from rock input energy

spectrum

Geant4 neutron background studies ndash rock neutrons analysis example

n = 38bull10-6 n(scm2)assumed total neutron flux at the

walls of fiducial volume

IN OUR GEOMETRY1 neutron per ~ 65 sec13200 neutrons per day

10 keV threshold

OUTPUT

PMijakowski Young Researchers Session 8 January 2006 Cracow 14

Geant4 neutron background studies ndash rock neutrons analysis example

no of incoming neutrons

13200 nday

- correction for interacting neutrons

Pint~ 577500 nday

- correction for multiplicity

Pmulti~ 537500 ndash 4000= 3500 nday

+ correction for spatial resolution (2 cm)

3700nday

Pinter~57 Pmulti~53

assumed 2cm spatial resolution

visible95

- shielding (CH2) reduction factor 104-106

1-135 events per year

PMijakowski Young Researchers Session 8 January 2006 Cracow 15

Summary amp Outlook

bull ArDM a new project aiming at developing and operating a 1 ton-scale liquid Argon detector for direct detection of WIMPs

bull With a 1 ton prototype we want to show the validity of this design (in particular 39Ar rejection)

bull Neutron shieldings will be addressed in a second phase

bull Investigations on neutron background sources and their interactions inside the detector are also performed (simulations in Geant4)ndash evaluation of expected number of neutron events (data analysis)ndash simulations will help to specify requirements for detector veto and

shielding

SIMULATIONS OUTLOOKbull Energy spectra and flux of incoming neutronsbull Detailed detector geometry in Geant4

BACKUP

PMijakowski Young Researchers Session 8 January 2006 Cracow 17

Geant4 neutron background studies ndash neutron capture in liquid Argon

capture on natural Argon(40Ar - 996 36Ar - 0337 38Ar - 0063)

Initial neutron energy = 10 eV

Average number of rsquos produced = 35

6099 MeV

8788 MeV

6598 MeV

Page 5: The search of dark matter with ArDM detector

PMijakowski Young Researchers Session 8 January 2006 Cracow 5

ArDM status

RampD CERN (1 ton prototype)

bull High voltage systembull LEM based charge readoutbull Light detection system (PMTs + VUV reflecting mirrors)bull CAD design and assemby of the detector

KEY POINT UNDERSTAND THE DETECTOR PERFORMANCE

FIRST GOAL proof of principle 39Ar rejection (intrinsic background beta-emitter with decay rate of asymp 1 kHz in a 1 ton detector)

Simulations full detector geom experimental background

PMijakowski Young Researchers Session 8 January 2006 Cracow 6

ArDM prospects

pictures ECocciaTAUP05

TIME SCALE

2006 assembly of detector at CERN test on surface

2007 transport to the Underground Laboratory (Canfranc Spain) installation in experimental hall and mounting of infrastructure + neutron shield

2007 first data taking

CANFRANC LAB (2450 m we)

PMijakowski Young Researchers Session 8 January 2006 Cracow 7

Estimated event rates

asymp 100 eventtonday

asymp 1 eventtonday

for = 10-46asymp 1 eventton100 day

Assuming 30 keV recoil energy threshold M = 100 GeVc2

PMijakowski Young Researchers Session 8 January 2006 Cracow 8

part II ndash Neutron background

Background events

nuclear eventse-like eventspossible to discriminate

bull the same signal from WIMP amp neutron interactions

bull only possible way to distinguish neutron multiple scattering

NEUTRON BACKGROUND SOURCES

local radioactivity (surrounding rock detector components)

muon-induced neutrons

- spontaneous fission 238U

- (n) reactions rsquos from radioactive chains of UTh

MOTIVATION neutron background limits detector sensitivity to WIMPs

PMijakowski Young Researchers Session 8 January 2006 Cracow 9

Neutron background sources

1 neutrons from surrounding rock - 238U and (n) reactionsflux rock ~ 38 times 10-6 n(scm2) CANFRANC ArDM input (preliminary) ~ 13200 ndaysupression neutron shielding

2 neutrons from det components - 238U and (n) reactions flux bdquodetector dependentrdquo ArDM input (preliminary) ~ 74 ndaysupression high-purity materials

3 muon-induced neutrons ndash production in hadronic amp e-m cascades init by rsquos flux -ind ~ 17 times 10-9 n(scm2) CANFRANCArDM input (preliminary) ~ 6 ndaysupression active veto

PMijakowski Young Researchers Session 8 January 2006 Cracow 10

Neutron background energy spectra

only fission spectrum

[1] rock

[2] detector components[3] -ind

plots 1 amp 3 MJ Carson JC Davies et al Astroparticle Physics 21(2004) 667-687

PMijakowski Young Researchers Session 8 January 2006 Cracow 11

part III ndash Geant4 neutron background studies

How many neutron recoils we will have in our experiment

(how many neutrons will enter the detector what energy spectrum how many would interact and produce visible recoils how many would undergo multiple scattering)

ArDM simulation tasks

detailed detector geom (Geant4) verifiaction of sim processes

(elastic scattering neutron capture)

rock neutrons neutrons from det components muon-induced neutrons

other background sources rsquos 39Ar

full detector sim (GRANADA)

PMijakowski Young Researchers Session 8 January 2006 Cracow 12

Geant4 neutron background studies ndash elastic scattering in liquid Argon

coscos

cos~d

ddT

d

dddN ArAr

)cos1(

2)(sincos1 2

2

22

2

2

2

Arn

nArnnAr

n

Ar

Arn

nnAr

Mm

mMTmM

m

M

Mm

mTT

TnltltMn

non relativistic

Argon recoil

spectra from G4

simulation

Tn = 5 keV

Tn = 15 MeV

Tn = 2 MeV

PMijakowski Young Researchers Session 8 January 2006 Cracow 13

SIMULATION- neutron source placed randomly on the walls of fiducial volume

- neutrons going out of the detector are neglected

INPUT

neutrons from rock input energy

spectrum

Geant4 neutron background studies ndash rock neutrons analysis example

n = 38bull10-6 n(scm2)assumed total neutron flux at the

walls of fiducial volume

IN OUR GEOMETRY1 neutron per ~ 65 sec13200 neutrons per day

10 keV threshold

OUTPUT

PMijakowski Young Researchers Session 8 January 2006 Cracow 14

Geant4 neutron background studies ndash rock neutrons analysis example

no of incoming neutrons

13200 nday

- correction for interacting neutrons

Pint~ 577500 nday

- correction for multiplicity

Pmulti~ 537500 ndash 4000= 3500 nday

+ correction for spatial resolution (2 cm)

3700nday

Pinter~57 Pmulti~53

assumed 2cm spatial resolution

visible95

- shielding (CH2) reduction factor 104-106

1-135 events per year

PMijakowski Young Researchers Session 8 January 2006 Cracow 15

Summary amp Outlook

bull ArDM a new project aiming at developing and operating a 1 ton-scale liquid Argon detector for direct detection of WIMPs

bull With a 1 ton prototype we want to show the validity of this design (in particular 39Ar rejection)

bull Neutron shieldings will be addressed in a second phase

bull Investigations on neutron background sources and their interactions inside the detector are also performed (simulations in Geant4)ndash evaluation of expected number of neutron events (data analysis)ndash simulations will help to specify requirements for detector veto and

shielding

SIMULATIONS OUTLOOKbull Energy spectra and flux of incoming neutronsbull Detailed detector geometry in Geant4

BACKUP

PMijakowski Young Researchers Session 8 January 2006 Cracow 17

Geant4 neutron background studies ndash neutron capture in liquid Argon

capture on natural Argon(40Ar - 996 36Ar - 0337 38Ar - 0063)

Initial neutron energy = 10 eV

Average number of rsquos produced = 35

6099 MeV

8788 MeV

6598 MeV

Page 6: The search of dark matter with ArDM detector

PMijakowski Young Researchers Session 8 January 2006 Cracow 6

ArDM prospects

pictures ECocciaTAUP05

TIME SCALE

2006 assembly of detector at CERN test on surface

2007 transport to the Underground Laboratory (Canfranc Spain) installation in experimental hall and mounting of infrastructure + neutron shield

2007 first data taking

CANFRANC LAB (2450 m we)

PMijakowski Young Researchers Session 8 January 2006 Cracow 7

Estimated event rates

asymp 100 eventtonday

asymp 1 eventtonday

for = 10-46asymp 1 eventton100 day

Assuming 30 keV recoil energy threshold M = 100 GeVc2

PMijakowski Young Researchers Session 8 January 2006 Cracow 8

part II ndash Neutron background

Background events

nuclear eventse-like eventspossible to discriminate

bull the same signal from WIMP amp neutron interactions

bull only possible way to distinguish neutron multiple scattering

NEUTRON BACKGROUND SOURCES

local radioactivity (surrounding rock detector components)

muon-induced neutrons

- spontaneous fission 238U

- (n) reactions rsquos from radioactive chains of UTh

MOTIVATION neutron background limits detector sensitivity to WIMPs

PMijakowski Young Researchers Session 8 January 2006 Cracow 9

Neutron background sources

1 neutrons from surrounding rock - 238U and (n) reactionsflux rock ~ 38 times 10-6 n(scm2) CANFRANC ArDM input (preliminary) ~ 13200 ndaysupression neutron shielding

2 neutrons from det components - 238U and (n) reactions flux bdquodetector dependentrdquo ArDM input (preliminary) ~ 74 ndaysupression high-purity materials

3 muon-induced neutrons ndash production in hadronic amp e-m cascades init by rsquos flux -ind ~ 17 times 10-9 n(scm2) CANFRANCArDM input (preliminary) ~ 6 ndaysupression active veto

PMijakowski Young Researchers Session 8 January 2006 Cracow 10

Neutron background energy spectra

only fission spectrum

[1] rock

[2] detector components[3] -ind

plots 1 amp 3 MJ Carson JC Davies et al Astroparticle Physics 21(2004) 667-687

PMijakowski Young Researchers Session 8 January 2006 Cracow 11

part III ndash Geant4 neutron background studies

How many neutron recoils we will have in our experiment

(how many neutrons will enter the detector what energy spectrum how many would interact and produce visible recoils how many would undergo multiple scattering)

ArDM simulation tasks

detailed detector geom (Geant4) verifiaction of sim processes

(elastic scattering neutron capture)

rock neutrons neutrons from det components muon-induced neutrons

other background sources rsquos 39Ar

full detector sim (GRANADA)

PMijakowski Young Researchers Session 8 January 2006 Cracow 12

Geant4 neutron background studies ndash elastic scattering in liquid Argon

coscos

cos~d

ddT

d

dddN ArAr

)cos1(

2)(sincos1 2

2

22

2

2

2

Arn

nArnnAr

n

Ar

Arn

nnAr

Mm

mMTmM

m

M

Mm

mTT

TnltltMn

non relativistic

Argon recoil

spectra from G4

simulation

Tn = 5 keV

Tn = 15 MeV

Tn = 2 MeV

PMijakowski Young Researchers Session 8 January 2006 Cracow 13

SIMULATION- neutron source placed randomly on the walls of fiducial volume

- neutrons going out of the detector are neglected

INPUT

neutrons from rock input energy

spectrum

Geant4 neutron background studies ndash rock neutrons analysis example

n = 38bull10-6 n(scm2)assumed total neutron flux at the

walls of fiducial volume

IN OUR GEOMETRY1 neutron per ~ 65 sec13200 neutrons per day

10 keV threshold

OUTPUT

PMijakowski Young Researchers Session 8 January 2006 Cracow 14

Geant4 neutron background studies ndash rock neutrons analysis example

no of incoming neutrons

13200 nday

- correction for interacting neutrons

Pint~ 577500 nday

- correction for multiplicity

Pmulti~ 537500 ndash 4000= 3500 nday

+ correction for spatial resolution (2 cm)

3700nday

Pinter~57 Pmulti~53

assumed 2cm spatial resolution

visible95

- shielding (CH2) reduction factor 104-106

1-135 events per year

PMijakowski Young Researchers Session 8 January 2006 Cracow 15

Summary amp Outlook

bull ArDM a new project aiming at developing and operating a 1 ton-scale liquid Argon detector for direct detection of WIMPs

bull With a 1 ton prototype we want to show the validity of this design (in particular 39Ar rejection)

bull Neutron shieldings will be addressed in a second phase

bull Investigations on neutron background sources and their interactions inside the detector are also performed (simulations in Geant4)ndash evaluation of expected number of neutron events (data analysis)ndash simulations will help to specify requirements for detector veto and

shielding

SIMULATIONS OUTLOOKbull Energy spectra and flux of incoming neutronsbull Detailed detector geometry in Geant4

BACKUP

PMijakowski Young Researchers Session 8 January 2006 Cracow 17

Geant4 neutron background studies ndash neutron capture in liquid Argon

capture on natural Argon(40Ar - 996 36Ar - 0337 38Ar - 0063)

Initial neutron energy = 10 eV

Average number of rsquos produced = 35

6099 MeV

8788 MeV

6598 MeV

Page 7: The search of dark matter with ArDM detector

PMijakowski Young Researchers Session 8 January 2006 Cracow 7

Estimated event rates

asymp 100 eventtonday

asymp 1 eventtonday

for = 10-46asymp 1 eventton100 day

Assuming 30 keV recoil energy threshold M = 100 GeVc2

PMijakowski Young Researchers Session 8 January 2006 Cracow 8

part II ndash Neutron background

Background events

nuclear eventse-like eventspossible to discriminate

bull the same signal from WIMP amp neutron interactions

bull only possible way to distinguish neutron multiple scattering

NEUTRON BACKGROUND SOURCES

local radioactivity (surrounding rock detector components)

muon-induced neutrons

- spontaneous fission 238U

- (n) reactions rsquos from radioactive chains of UTh

MOTIVATION neutron background limits detector sensitivity to WIMPs

PMijakowski Young Researchers Session 8 January 2006 Cracow 9

Neutron background sources

1 neutrons from surrounding rock - 238U and (n) reactionsflux rock ~ 38 times 10-6 n(scm2) CANFRANC ArDM input (preliminary) ~ 13200 ndaysupression neutron shielding

2 neutrons from det components - 238U and (n) reactions flux bdquodetector dependentrdquo ArDM input (preliminary) ~ 74 ndaysupression high-purity materials

3 muon-induced neutrons ndash production in hadronic amp e-m cascades init by rsquos flux -ind ~ 17 times 10-9 n(scm2) CANFRANCArDM input (preliminary) ~ 6 ndaysupression active veto

PMijakowski Young Researchers Session 8 January 2006 Cracow 10

Neutron background energy spectra

only fission spectrum

[1] rock

[2] detector components[3] -ind

plots 1 amp 3 MJ Carson JC Davies et al Astroparticle Physics 21(2004) 667-687

PMijakowski Young Researchers Session 8 January 2006 Cracow 11

part III ndash Geant4 neutron background studies

How many neutron recoils we will have in our experiment

(how many neutrons will enter the detector what energy spectrum how many would interact and produce visible recoils how many would undergo multiple scattering)

ArDM simulation tasks

detailed detector geom (Geant4) verifiaction of sim processes

(elastic scattering neutron capture)

rock neutrons neutrons from det components muon-induced neutrons

other background sources rsquos 39Ar

full detector sim (GRANADA)

PMijakowski Young Researchers Session 8 January 2006 Cracow 12

Geant4 neutron background studies ndash elastic scattering in liquid Argon

coscos

cos~d

ddT

d

dddN ArAr

)cos1(

2)(sincos1 2

2

22

2

2

2

Arn

nArnnAr

n

Ar

Arn

nnAr

Mm

mMTmM

m

M

Mm

mTT

TnltltMn

non relativistic

Argon recoil

spectra from G4

simulation

Tn = 5 keV

Tn = 15 MeV

Tn = 2 MeV

PMijakowski Young Researchers Session 8 January 2006 Cracow 13

SIMULATION- neutron source placed randomly on the walls of fiducial volume

- neutrons going out of the detector are neglected

INPUT

neutrons from rock input energy

spectrum

Geant4 neutron background studies ndash rock neutrons analysis example

n = 38bull10-6 n(scm2)assumed total neutron flux at the

walls of fiducial volume

IN OUR GEOMETRY1 neutron per ~ 65 sec13200 neutrons per day

10 keV threshold

OUTPUT

PMijakowski Young Researchers Session 8 January 2006 Cracow 14

Geant4 neutron background studies ndash rock neutrons analysis example

no of incoming neutrons

13200 nday

- correction for interacting neutrons

Pint~ 577500 nday

- correction for multiplicity

Pmulti~ 537500 ndash 4000= 3500 nday

+ correction for spatial resolution (2 cm)

3700nday

Pinter~57 Pmulti~53

assumed 2cm spatial resolution

visible95

- shielding (CH2) reduction factor 104-106

1-135 events per year

PMijakowski Young Researchers Session 8 January 2006 Cracow 15

Summary amp Outlook

bull ArDM a new project aiming at developing and operating a 1 ton-scale liquid Argon detector for direct detection of WIMPs

bull With a 1 ton prototype we want to show the validity of this design (in particular 39Ar rejection)

bull Neutron shieldings will be addressed in a second phase

bull Investigations on neutron background sources and their interactions inside the detector are also performed (simulations in Geant4)ndash evaluation of expected number of neutron events (data analysis)ndash simulations will help to specify requirements for detector veto and

shielding

SIMULATIONS OUTLOOKbull Energy spectra and flux of incoming neutronsbull Detailed detector geometry in Geant4

BACKUP

PMijakowski Young Researchers Session 8 January 2006 Cracow 17

Geant4 neutron background studies ndash neutron capture in liquid Argon

capture on natural Argon(40Ar - 996 36Ar - 0337 38Ar - 0063)

Initial neutron energy = 10 eV

Average number of rsquos produced = 35

6099 MeV

8788 MeV

6598 MeV

Page 8: The search of dark matter with ArDM detector

PMijakowski Young Researchers Session 8 January 2006 Cracow 8

part II ndash Neutron background

Background events

nuclear eventse-like eventspossible to discriminate

bull the same signal from WIMP amp neutron interactions

bull only possible way to distinguish neutron multiple scattering

NEUTRON BACKGROUND SOURCES

local radioactivity (surrounding rock detector components)

muon-induced neutrons

- spontaneous fission 238U

- (n) reactions rsquos from radioactive chains of UTh

MOTIVATION neutron background limits detector sensitivity to WIMPs

PMijakowski Young Researchers Session 8 January 2006 Cracow 9

Neutron background sources

1 neutrons from surrounding rock - 238U and (n) reactionsflux rock ~ 38 times 10-6 n(scm2) CANFRANC ArDM input (preliminary) ~ 13200 ndaysupression neutron shielding

2 neutrons from det components - 238U and (n) reactions flux bdquodetector dependentrdquo ArDM input (preliminary) ~ 74 ndaysupression high-purity materials

3 muon-induced neutrons ndash production in hadronic amp e-m cascades init by rsquos flux -ind ~ 17 times 10-9 n(scm2) CANFRANCArDM input (preliminary) ~ 6 ndaysupression active veto

PMijakowski Young Researchers Session 8 January 2006 Cracow 10

Neutron background energy spectra

only fission spectrum

[1] rock

[2] detector components[3] -ind

plots 1 amp 3 MJ Carson JC Davies et al Astroparticle Physics 21(2004) 667-687

PMijakowski Young Researchers Session 8 January 2006 Cracow 11

part III ndash Geant4 neutron background studies

How many neutron recoils we will have in our experiment

(how many neutrons will enter the detector what energy spectrum how many would interact and produce visible recoils how many would undergo multiple scattering)

ArDM simulation tasks

detailed detector geom (Geant4) verifiaction of sim processes

(elastic scattering neutron capture)

rock neutrons neutrons from det components muon-induced neutrons

other background sources rsquos 39Ar

full detector sim (GRANADA)

PMijakowski Young Researchers Session 8 January 2006 Cracow 12

Geant4 neutron background studies ndash elastic scattering in liquid Argon

coscos

cos~d

ddT

d

dddN ArAr

)cos1(

2)(sincos1 2

2

22

2

2

2

Arn

nArnnAr

n

Ar

Arn

nnAr

Mm

mMTmM

m

M

Mm

mTT

TnltltMn

non relativistic

Argon recoil

spectra from G4

simulation

Tn = 5 keV

Tn = 15 MeV

Tn = 2 MeV

PMijakowski Young Researchers Session 8 January 2006 Cracow 13

SIMULATION- neutron source placed randomly on the walls of fiducial volume

- neutrons going out of the detector are neglected

INPUT

neutrons from rock input energy

spectrum

Geant4 neutron background studies ndash rock neutrons analysis example

n = 38bull10-6 n(scm2)assumed total neutron flux at the

walls of fiducial volume

IN OUR GEOMETRY1 neutron per ~ 65 sec13200 neutrons per day

10 keV threshold

OUTPUT

PMijakowski Young Researchers Session 8 January 2006 Cracow 14

Geant4 neutron background studies ndash rock neutrons analysis example

no of incoming neutrons

13200 nday

- correction for interacting neutrons

Pint~ 577500 nday

- correction for multiplicity

Pmulti~ 537500 ndash 4000= 3500 nday

+ correction for spatial resolution (2 cm)

3700nday

Pinter~57 Pmulti~53

assumed 2cm spatial resolution

visible95

- shielding (CH2) reduction factor 104-106

1-135 events per year

PMijakowski Young Researchers Session 8 January 2006 Cracow 15

Summary amp Outlook

bull ArDM a new project aiming at developing and operating a 1 ton-scale liquid Argon detector for direct detection of WIMPs

bull With a 1 ton prototype we want to show the validity of this design (in particular 39Ar rejection)

bull Neutron shieldings will be addressed in a second phase

bull Investigations on neutron background sources and their interactions inside the detector are also performed (simulations in Geant4)ndash evaluation of expected number of neutron events (data analysis)ndash simulations will help to specify requirements for detector veto and

shielding

SIMULATIONS OUTLOOKbull Energy spectra and flux of incoming neutronsbull Detailed detector geometry in Geant4

BACKUP

PMijakowski Young Researchers Session 8 January 2006 Cracow 17

Geant4 neutron background studies ndash neutron capture in liquid Argon

capture on natural Argon(40Ar - 996 36Ar - 0337 38Ar - 0063)

Initial neutron energy = 10 eV

Average number of rsquos produced = 35

6099 MeV

8788 MeV

6598 MeV

Page 9: The search of dark matter with ArDM detector

PMijakowski Young Researchers Session 8 January 2006 Cracow 9

Neutron background sources

1 neutrons from surrounding rock - 238U and (n) reactionsflux rock ~ 38 times 10-6 n(scm2) CANFRANC ArDM input (preliminary) ~ 13200 ndaysupression neutron shielding

2 neutrons from det components - 238U and (n) reactions flux bdquodetector dependentrdquo ArDM input (preliminary) ~ 74 ndaysupression high-purity materials

3 muon-induced neutrons ndash production in hadronic amp e-m cascades init by rsquos flux -ind ~ 17 times 10-9 n(scm2) CANFRANCArDM input (preliminary) ~ 6 ndaysupression active veto

PMijakowski Young Researchers Session 8 January 2006 Cracow 10

Neutron background energy spectra

only fission spectrum

[1] rock

[2] detector components[3] -ind

plots 1 amp 3 MJ Carson JC Davies et al Astroparticle Physics 21(2004) 667-687

PMijakowski Young Researchers Session 8 January 2006 Cracow 11

part III ndash Geant4 neutron background studies

How many neutron recoils we will have in our experiment

(how many neutrons will enter the detector what energy spectrum how many would interact and produce visible recoils how many would undergo multiple scattering)

ArDM simulation tasks

detailed detector geom (Geant4) verifiaction of sim processes

(elastic scattering neutron capture)

rock neutrons neutrons from det components muon-induced neutrons

other background sources rsquos 39Ar

full detector sim (GRANADA)

PMijakowski Young Researchers Session 8 January 2006 Cracow 12

Geant4 neutron background studies ndash elastic scattering in liquid Argon

coscos

cos~d

ddT

d

dddN ArAr

)cos1(

2)(sincos1 2

2

22

2

2

2

Arn

nArnnAr

n

Ar

Arn

nnAr

Mm

mMTmM

m

M

Mm

mTT

TnltltMn

non relativistic

Argon recoil

spectra from G4

simulation

Tn = 5 keV

Tn = 15 MeV

Tn = 2 MeV

PMijakowski Young Researchers Session 8 January 2006 Cracow 13

SIMULATION- neutron source placed randomly on the walls of fiducial volume

- neutrons going out of the detector are neglected

INPUT

neutrons from rock input energy

spectrum

Geant4 neutron background studies ndash rock neutrons analysis example

n = 38bull10-6 n(scm2)assumed total neutron flux at the

walls of fiducial volume

IN OUR GEOMETRY1 neutron per ~ 65 sec13200 neutrons per day

10 keV threshold

OUTPUT

PMijakowski Young Researchers Session 8 January 2006 Cracow 14

Geant4 neutron background studies ndash rock neutrons analysis example

no of incoming neutrons

13200 nday

- correction for interacting neutrons

Pint~ 577500 nday

- correction for multiplicity

Pmulti~ 537500 ndash 4000= 3500 nday

+ correction for spatial resolution (2 cm)

3700nday

Pinter~57 Pmulti~53

assumed 2cm spatial resolution

visible95

- shielding (CH2) reduction factor 104-106

1-135 events per year

PMijakowski Young Researchers Session 8 January 2006 Cracow 15

Summary amp Outlook

bull ArDM a new project aiming at developing and operating a 1 ton-scale liquid Argon detector for direct detection of WIMPs

bull With a 1 ton prototype we want to show the validity of this design (in particular 39Ar rejection)

bull Neutron shieldings will be addressed in a second phase

bull Investigations on neutron background sources and their interactions inside the detector are also performed (simulations in Geant4)ndash evaluation of expected number of neutron events (data analysis)ndash simulations will help to specify requirements for detector veto and

shielding

SIMULATIONS OUTLOOKbull Energy spectra and flux of incoming neutronsbull Detailed detector geometry in Geant4

BACKUP

PMijakowski Young Researchers Session 8 January 2006 Cracow 17

Geant4 neutron background studies ndash neutron capture in liquid Argon

capture on natural Argon(40Ar - 996 36Ar - 0337 38Ar - 0063)

Initial neutron energy = 10 eV

Average number of rsquos produced = 35

6099 MeV

8788 MeV

6598 MeV

Page 10: The search of dark matter with ArDM detector

PMijakowski Young Researchers Session 8 January 2006 Cracow 10

Neutron background energy spectra

only fission spectrum

[1] rock

[2] detector components[3] -ind

plots 1 amp 3 MJ Carson JC Davies et al Astroparticle Physics 21(2004) 667-687

PMijakowski Young Researchers Session 8 January 2006 Cracow 11

part III ndash Geant4 neutron background studies

How many neutron recoils we will have in our experiment

(how many neutrons will enter the detector what energy spectrum how many would interact and produce visible recoils how many would undergo multiple scattering)

ArDM simulation tasks

detailed detector geom (Geant4) verifiaction of sim processes

(elastic scattering neutron capture)

rock neutrons neutrons from det components muon-induced neutrons

other background sources rsquos 39Ar

full detector sim (GRANADA)

PMijakowski Young Researchers Session 8 January 2006 Cracow 12

Geant4 neutron background studies ndash elastic scattering in liquid Argon

coscos

cos~d

ddT

d

dddN ArAr

)cos1(

2)(sincos1 2

2

22

2

2

2

Arn

nArnnAr

n

Ar

Arn

nnAr

Mm

mMTmM

m

M

Mm

mTT

TnltltMn

non relativistic

Argon recoil

spectra from G4

simulation

Tn = 5 keV

Tn = 15 MeV

Tn = 2 MeV

PMijakowski Young Researchers Session 8 January 2006 Cracow 13

SIMULATION- neutron source placed randomly on the walls of fiducial volume

- neutrons going out of the detector are neglected

INPUT

neutrons from rock input energy

spectrum

Geant4 neutron background studies ndash rock neutrons analysis example

n = 38bull10-6 n(scm2)assumed total neutron flux at the

walls of fiducial volume

IN OUR GEOMETRY1 neutron per ~ 65 sec13200 neutrons per day

10 keV threshold

OUTPUT

PMijakowski Young Researchers Session 8 January 2006 Cracow 14

Geant4 neutron background studies ndash rock neutrons analysis example

no of incoming neutrons

13200 nday

- correction for interacting neutrons

Pint~ 577500 nday

- correction for multiplicity

Pmulti~ 537500 ndash 4000= 3500 nday

+ correction for spatial resolution (2 cm)

3700nday

Pinter~57 Pmulti~53

assumed 2cm spatial resolution

visible95

- shielding (CH2) reduction factor 104-106

1-135 events per year

PMijakowski Young Researchers Session 8 January 2006 Cracow 15

Summary amp Outlook

bull ArDM a new project aiming at developing and operating a 1 ton-scale liquid Argon detector for direct detection of WIMPs

bull With a 1 ton prototype we want to show the validity of this design (in particular 39Ar rejection)

bull Neutron shieldings will be addressed in a second phase

bull Investigations on neutron background sources and their interactions inside the detector are also performed (simulations in Geant4)ndash evaluation of expected number of neutron events (data analysis)ndash simulations will help to specify requirements for detector veto and

shielding

SIMULATIONS OUTLOOKbull Energy spectra and flux of incoming neutronsbull Detailed detector geometry in Geant4

BACKUP

PMijakowski Young Researchers Session 8 January 2006 Cracow 17

Geant4 neutron background studies ndash neutron capture in liquid Argon

capture on natural Argon(40Ar - 996 36Ar - 0337 38Ar - 0063)

Initial neutron energy = 10 eV

Average number of rsquos produced = 35

6099 MeV

8788 MeV

6598 MeV

Page 11: The search of dark matter with ArDM detector

PMijakowski Young Researchers Session 8 January 2006 Cracow 11

part III ndash Geant4 neutron background studies

How many neutron recoils we will have in our experiment

(how many neutrons will enter the detector what energy spectrum how many would interact and produce visible recoils how many would undergo multiple scattering)

ArDM simulation tasks

detailed detector geom (Geant4) verifiaction of sim processes

(elastic scattering neutron capture)

rock neutrons neutrons from det components muon-induced neutrons

other background sources rsquos 39Ar

full detector sim (GRANADA)

PMijakowski Young Researchers Session 8 January 2006 Cracow 12

Geant4 neutron background studies ndash elastic scattering in liquid Argon

coscos

cos~d

ddT

d

dddN ArAr

)cos1(

2)(sincos1 2

2

22

2

2

2

Arn

nArnnAr

n

Ar

Arn

nnAr

Mm

mMTmM

m

M

Mm

mTT

TnltltMn

non relativistic

Argon recoil

spectra from G4

simulation

Tn = 5 keV

Tn = 15 MeV

Tn = 2 MeV

PMijakowski Young Researchers Session 8 January 2006 Cracow 13

SIMULATION- neutron source placed randomly on the walls of fiducial volume

- neutrons going out of the detector are neglected

INPUT

neutrons from rock input energy

spectrum

Geant4 neutron background studies ndash rock neutrons analysis example

n = 38bull10-6 n(scm2)assumed total neutron flux at the

walls of fiducial volume

IN OUR GEOMETRY1 neutron per ~ 65 sec13200 neutrons per day

10 keV threshold

OUTPUT

PMijakowski Young Researchers Session 8 January 2006 Cracow 14

Geant4 neutron background studies ndash rock neutrons analysis example

no of incoming neutrons

13200 nday

- correction for interacting neutrons

Pint~ 577500 nday

- correction for multiplicity

Pmulti~ 537500 ndash 4000= 3500 nday

+ correction for spatial resolution (2 cm)

3700nday

Pinter~57 Pmulti~53

assumed 2cm spatial resolution

visible95

- shielding (CH2) reduction factor 104-106

1-135 events per year

PMijakowski Young Researchers Session 8 January 2006 Cracow 15

Summary amp Outlook

bull ArDM a new project aiming at developing and operating a 1 ton-scale liquid Argon detector for direct detection of WIMPs

bull With a 1 ton prototype we want to show the validity of this design (in particular 39Ar rejection)

bull Neutron shieldings will be addressed in a second phase

bull Investigations on neutron background sources and their interactions inside the detector are also performed (simulations in Geant4)ndash evaluation of expected number of neutron events (data analysis)ndash simulations will help to specify requirements for detector veto and

shielding

SIMULATIONS OUTLOOKbull Energy spectra and flux of incoming neutronsbull Detailed detector geometry in Geant4

BACKUP

PMijakowski Young Researchers Session 8 January 2006 Cracow 17

Geant4 neutron background studies ndash neutron capture in liquid Argon

capture on natural Argon(40Ar - 996 36Ar - 0337 38Ar - 0063)

Initial neutron energy = 10 eV

Average number of rsquos produced = 35

6099 MeV

8788 MeV

6598 MeV

Page 12: The search of dark matter with ArDM detector

PMijakowski Young Researchers Session 8 January 2006 Cracow 12

Geant4 neutron background studies ndash elastic scattering in liquid Argon

coscos

cos~d

ddT

d

dddN ArAr

)cos1(

2)(sincos1 2

2

22

2

2

2

Arn

nArnnAr

n

Ar

Arn

nnAr

Mm

mMTmM

m

M

Mm

mTT

TnltltMn

non relativistic

Argon recoil

spectra from G4

simulation

Tn = 5 keV

Tn = 15 MeV

Tn = 2 MeV

PMijakowski Young Researchers Session 8 January 2006 Cracow 13

SIMULATION- neutron source placed randomly on the walls of fiducial volume

- neutrons going out of the detector are neglected

INPUT

neutrons from rock input energy

spectrum

Geant4 neutron background studies ndash rock neutrons analysis example

n = 38bull10-6 n(scm2)assumed total neutron flux at the

walls of fiducial volume

IN OUR GEOMETRY1 neutron per ~ 65 sec13200 neutrons per day

10 keV threshold

OUTPUT

PMijakowski Young Researchers Session 8 January 2006 Cracow 14

Geant4 neutron background studies ndash rock neutrons analysis example

no of incoming neutrons

13200 nday

- correction for interacting neutrons

Pint~ 577500 nday

- correction for multiplicity

Pmulti~ 537500 ndash 4000= 3500 nday

+ correction for spatial resolution (2 cm)

3700nday

Pinter~57 Pmulti~53

assumed 2cm spatial resolution

visible95

- shielding (CH2) reduction factor 104-106

1-135 events per year

PMijakowski Young Researchers Session 8 January 2006 Cracow 15

Summary amp Outlook

bull ArDM a new project aiming at developing and operating a 1 ton-scale liquid Argon detector for direct detection of WIMPs

bull With a 1 ton prototype we want to show the validity of this design (in particular 39Ar rejection)

bull Neutron shieldings will be addressed in a second phase

bull Investigations on neutron background sources and their interactions inside the detector are also performed (simulations in Geant4)ndash evaluation of expected number of neutron events (data analysis)ndash simulations will help to specify requirements for detector veto and

shielding

SIMULATIONS OUTLOOKbull Energy spectra and flux of incoming neutronsbull Detailed detector geometry in Geant4

BACKUP

PMijakowski Young Researchers Session 8 January 2006 Cracow 17

Geant4 neutron background studies ndash neutron capture in liquid Argon

capture on natural Argon(40Ar - 996 36Ar - 0337 38Ar - 0063)

Initial neutron energy = 10 eV

Average number of rsquos produced = 35

6099 MeV

8788 MeV

6598 MeV

Page 13: The search of dark matter with ArDM detector

PMijakowski Young Researchers Session 8 January 2006 Cracow 13

SIMULATION- neutron source placed randomly on the walls of fiducial volume

- neutrons going out of the detector are neglected

INPUT

neutrons from rock input energy

spectrum

Geant4 neutron background studies ndash rock neutrons analysis example

n = 38bull10-6 n(scm2)assumed total neutron flux at the

walls of fiducial volume

IN OUR GEOMETRY1 neutron per ~ 65 sec13200 neutrons per day

10 keV threshold

OUTPUT

PMijakowski Young Researchers Session 8 January 2006 Cracow 14

Geant4 neutron background studies ndash rock neutrons analysis example

no of incoming neutrons

13200 nday

- correction for interacting neutrons

Pint~ 577500 nday

- correction for multiplicity

Pmulti~ 537500 ndash 4000= 3500 nday

+ correction for spatial resolution (2 cm)

3700nday

Pinter~57 Pmulti~53

assumed 2cm spatial resolution

visible95

- shielding (CH2) reduction factor 104-106

1-135 events per year

PMijakowski Young Researchers Session 8 January 2006 Cracow 15

Summary amp Outlook

bull ArDM a new project aiming at developing and operating a 1 ton-scale liquid Argon detector for direct detection of WIMPs

bull With a 1 ton prototype we want to show the validity of this design (in particular 39Ar rejection)

bull Neutron shieldings will be addressed in a second phase

bull Investigations on neutron background sources and their interactions inside the detector are also performed (simulations in Geant4)ndash evaluation of expected number of neutron events (data analysis)ndash simulations will help to specify requirements for detector veto and

shielding

SIMULATIONS OUTLOOKbull Energy spectra and flux of incoming neutronsbull Detailed detector geometry in Geant4

BACKUP

PMijakowski Young Researchers Session 8 January 2006 Cracow 17

Geant4 neutron background studies ndash neutron capture in liquid Argon

capture on natural Argon(40Ar - 996 36Ar - 0337 38Ar - 0063)

Initial neutron energy = 10 eV

Average number of rsquos produced = 35

6099 MeV

8788 MeV

6598 MeV

Page 14: The search of dark matter with ArDM detector

PMijakowski Young Researchers Session 8 January 2006 Cracow 14

Geant4 neutron background studies ndash rock neutrons analysis example

no of incoming neutrons

13200 nday

- correction for interacting neutrons

Pint~ 577500 nday

- correction for multiplicity

Pmulti~ 537500 ndash 4000= 3500 nday

+ correction for spatial resolution (2 cm)

3700nday

Pinter~57 Pmulti~53

assumed 2cm spatial resolution

visible95

- shielding (CH2) reduction factor 104-106

1-135 events per year

PMijakowski Young Researchers Session 8 January 2006 Cracow 15

Summary amp Outlook

bull ArDM a new project aiming at developing and operating a 1 ton-scale liquid Argon detector for direct detection of WIMPs

bull With a 1 ton prototype we want to show the validity of this design (in particular 39Ar rejection)

bull Neutron shieldings will be addressed in a second phase

bull Investigations on neutron background sources and their interactions inside the detector are also performed (simulations in Geant4)ndash evaluation of expected number of neutron events (data analysis)ndash simulations will help to specify requirements for detector veto and

shielding

SIMULATIONS OUTLOOKbull Energy spectra and flux of incoming neutronsbull Detailed detector geometry in Geant4

BACKUP

PMijakowski Young Researchers Session 8 January 2006 Cracow 17

Geant4 neutron background studies ndash neutron capture in liquid Argon

capture on natural Argon(40Ar - 996 36Ar - 0337 38Ar - 0063)

Initial neutron energy = 10 eV

Average number of rsquos produced = 35

6099 MeV

8788 MeV

6598 MeV

Page 15: The search of dark matter with ArDM detector

PMijakowski Young Researchers Session 8 January 2006 Cracow 15

Summary amp Outlook

bull ArDM a new project aiming at developing and operating a 1 ton-scale liquid Argon detector for direct detection of WIMPs

bull With a 1 ton prototype we want to show the validity of this design (in particular 39Ar rejection)

bull Neutron shieldings will be addressed in a second phase

bull Investigations on neutron background sources and their interactions inside the detector are also performed (simulations in Geant4)ndash evaluation of expected number of neutron events (data analysis)ndash simulations will help to specify requirements for detector veto and

shielding

SIMULATIONS OUTLOOKbull Energy spectra and flux of incoming neutronsbull Detailed detector geometry in Geant4

BACKUP

PMijakowski Young Researchers Session 8 January 2006 Cracow 17

Geant4 neutron background studies ndash neutron capture in liquid Argon

capture on natural Argon(40Ar - 996 36Ar - 0337 38Ar - 0063)

Initial neutron energy = 10 eV

Average number of rsquos produced = 35

6099 MeV

8788 MeV

6598 MeV

Page 16: The search of dark matter with ArDM detector

BACKUP

PMijakowski Young Researchers Session 8 January 2006 Cracow 17

Geant4 neutron background studies ndash neutron capture in liquid Argon

capture on natural Argon(40Ar - 996 36Ar - 0337 38Ar - 0063)

Initial neutron energy = 10 eV

Average number of rsquos produced = 35

6099 MeV

8788 MeV

6598 MeV

Page 17: The search of dark matter with ArDM detector

PMijakowski Young Researchers Session 8 January 2006 Cracow 17

Geant4 neutron background studies ndash neutron capture in liquid Argon

capture on natural Argon(40Ar - 996 36Ar - 0337 38Ar - 0063)

Initial neutron energy = 10 eV

Average number of rsquos produced = 35

6099 MeV

8788 MeV

6598 MeV