Status of the KATRIN Experiment and commissioning of the spectrometer - - PowerPoint PPT Presentation

status of the katrin experiment and commissioning of the
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Status of the KATRIN Experiment and commissioning of the spectrometer - - PowerPoint PPT Presentation

Status of the KATRIN Experiment and commissioning of the spectrometer and detector section Thomas Thmmler for the KATRIN collaboration DESY-Physikseminar, June 2013, Hamburg & Zeuthen KIT Center Elementary Particle and Astroparticle Physics


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SLIDE 1

KIT Center Elementary Particle and Astroparticle Physics (KCETA) Institute for Nuclear Physics (IKP)

KIT – University of the State of Baden-Württemberg and National Research Center of the Helmholtz Association

Status of the KATRIN Experiment and commissioning

  • f the spectrometer and detector section

Thomas Thümmler for the KATRIN collaboration DESY-Physikseminar, June 2013, Hamburg & Zeuthen

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2

  • T. Thümmler - Status and commissioning of KATRIN

! "

Introduction and KATRIN setup!

! "

Spectrometer-, Detector-Section!

! "

Status and Commissioning runs!

! "

Summary and Outlook!

Goal of KATRIN

! "

model-independent neutrino mass determination!

! "

precise spectroscopy of Tritium !-decay!

! "

unprecedented sensitivity of" ! ! ! !200 meV/c2 (90% C.L.)!

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3

  • T. Thümmler - Status and commissioning of KATRIN

cosmology cosmology: role of ! !´s as hot (warm?) dark matter? particle physics: origin and hierarchy of the ! !-mass? Millennium Simulation particle physics

fermions bosons massless bosons

neutrinos

Motivation: Neutrinos in Astroparticle Physics

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4

  • T. Thümmler - Status and commissioning of KATRIN

! "

Clear evidence for neutrino flavour oscillations:!

! "

Atmospheric neutrinos: !(!m32)2 2.4 # 10-3 eV2/c4 ! !

! "

Solar neutrinos: ! !(!m21)2 7.6 # 10-5 eV2/c4!

!" Well established fact: m" 0!

!

! "

measures #mi and HDM $"!

! "

very sensitive, but model dependent!!

! "

Planck: #mi < 0.98 eV"

(Planck 2013 results. XVI. Cosm. param.)!

! "

potential: #mi = 20-50 meV" (Planck, LSST, weak lensing)! Experiments on Neutrino Oscillations: Input from Cosmology:

Neutrino Mass: Status and Perspectives

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5

  • T. Thümmler - Status and commissioning of KATRIN

neutrino masses in lab. experiments

Neutrino Mass: Status and Perspectives

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6

  • T. Thümmler - Status and commissioning of KATRIN

neutrino masses in lab. experiments

! model-dependent (CP-phases)! ! effective Majorana mass:! ! !

!" probe " as Majorana particle: ? ! ! status: mßß < 0.35 eV, evidence?! !" potential: mßß = 20-50 meV! !" GERDA, EXO, SNO+, MAJORANA,"

Cuore, KamLAND-Zen, ...!

search for 0!ßß

  • eff. Majorana mass mßß

ν = ¯ ν

mββ =

  • i

U 2

ei · mνi

  • Neutrino Mass: Status and Perspectives
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7

  • T. Thümmler - Status and commissioning of KATRIN

neutrino masses in lab. experiments

! model-dependent (CP-phases)! ! effective Majorana mass:! ! !

!" probe " as Majorana particle: ? ! ! status: mßß < 0.35 eV, evidence?! !" potential: mßß = 20-50 meV! !" GERDA, EXO, SNO+, MAJORANA,"

Cuore, KamLAND-Zen, ...!

search for 0!ßß

  • eff. Majorana mass mßß

ν = ¯ ν

mββ =

  • i

U 2

ei · mνi

  • kinematics of ß-decay

absolute ! !e-mass: m!

! model-independent! ! squared neutrino mass:! ! ! !

! direct, from kinematics! ! status: m! < 2.3 eV! !" potential: m! = 200 meV! !" KATRIN, MARE,"

Project 8, ECHO" !

m2

νe =

  • i

|Uei|2 · m2

νi

Neutrino Mass: Status and Perspectives

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8

  • T. Thümmler - Status and commissioning of KATRIN

d"

i

dE = C# p# (E + me)# (E0 $ E)# (E0 $ E)2 $ mi

2 # F(E,Z)# %(E0 $ E $ mi)

ß-decay – Fermi theory & !-mass

ß-decay kinematics close to endpoint E0: model independent measurement of m(!e), based solely on kinematic parameters & energy conservation m("e) = Uei

2# i=1 3

$

mi

2

  • bservable m2("e):

effective electron-"-mass

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9

∆E E0 3

  • T. Thümmler - Status and commissioning of KATRIN

d"

i

dE = C# p# (E + me)# (E0 $ E)# (E0 $ E)2 $ mi

2 # F(E,Z)# %(E0 $ E $ mi)

m("e) = Uei

2# i=1 3

$

mi

2

ß-decay – Fermi theory & !-mass

ß-decay kinematics close to endpoint E0: model independent measurement of m(!e), based solely on kinematic parameters & energy conservation

  • bservable m2("e):

effective electron-"-mass

!" small modifications by final states, radiative & recoil corrections

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10

∆E E0 3

  • T. Thümmler - Status and commissioning of KATRIN

d"

i

dE = C# p# (E + me)# (E0 $ E)# (E0 $ E)2 $ mi

2 # F(E,Z)# %(E0 $ E $ mi)

m("e) = Uei

2# i=1 3

$

mi

2

key requirements:

!" low endpoint ! source !" high count rate !" high energy resolution !" extremely low background

ß-decay – Fermi theory & !-mass

ß-decay kinematics close to endpoint E0: model independent measurement of m(!e), based solely on kinematic parameters & energy conservation

  • bservable m2("e):

effective electron-"-mass

!" small modifications by final states, radiative & recoil corrections

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11

Magnetic Adiabatic Collimation with Electrostatic Filter

! !

!" collimation:

adiabatic transport: E ! E|| due to μ = const.

!" energy analysis:

  • nly electrons with E|| > eU0 (retarding potential) can pass analysing plane

high-pass filter with a sharp transmission function, no tails!

!" energy resolution: !

!E = E ∙ Bmin / Bmax = 0.93 eV

  • T. Thümmler - Status and commissioning of KATRIN

The MAC-E filter

  • A. Picard et al., NIM B 63 (1992)

Design Facts: Bmax = 6 T Bmin = 0.3 mT Bmin / Bmax = 5∙10-5 μ = E / B = const. U0 = 18.6 kV E = 18.6 keV E = E + E||

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12

  • T. Thümmler - Status and commissioning of KATRIN

Tritium source Transport section

1 011 e- / s e-

3He

Pre spectrometer

103 e- /s e- e- e-

Spectrometer

1 e- /s e-

Detector

"E = 0.93 eV E = 18600 eV 1011 e- /s e-

3H

" decay

ve

3He 3H

E > 18.3 keV

70 m!

The KATRIN Setup - Overview

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13

  • 40 -30 -20 -10 0 +10

distance from analysing plane [m] potential [kV]

  • 20
  • 10

tritium source

1 10-1 10-2

spectrometer Bmin Bmax

magnetic field & electrostatic potential

B-field [T]

  • T. Thümmler - Status and commissioning of KATRIN
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14

" 10-3 stability of tritium source column density " "d " retention factor for molecular tritium R = 1014 " effective removal of ions "" fully adiabatic (meV scale) transport of electrons over > 50 m "" avoid particle storage in Penning-like traps "" avoid contermination by Rn in the volume

tritium-bearing components electrostatic spectrometers & detector

1011 electrons/s tritium source <10-2 cps total background

  • T. Thümmler - Status and commissioning of KATRIN

The KATRIN Setup

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15

WGTS

  • T. Thümmler - Status and commissioning of KATRIN

16 m

Design parameter luminosity! 1.7 # 1011 Bq! injection rate! 5 # 1019 T2/s 40 g/day 10 kg/y! Tritium purity! > 95%! ±0.1 %! temperature! T = 27 K ± 30 mK! ±0.1 %! pressure! pinj 10-3 mbar ! ±0.1 %! magnetic guiding! B = 3.6 T!

CAPER facility Tritium Laboratory Karlsruhe!

  • a unique research facility in Europe!

Windowless Gaseous Tritium Source WGTS

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16

  • T. Thümmler - Status and commissioning of KATRIN

DPS1-R WGTS DPS1-F DPS2-F control system T2 injection

inner loop

T2 preparation isotope separation CMS-R

95% 5% 5% 95%

T2 retention- system batch mode, 60 days (<1 Ci)

1% 1%

KATRIN tritium loop system

ISS glove box

permeator

Up and running extremely stable!

! designed for a stability at 10-3 level ! achieved: 2 # 10-4 over 4 months

Windowless Gaseous Tritium Source WGTS

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17

Windowless Gaseous Tritium Source WGTS

conzept: 2-Phasen Neon (sied. Flüssigkeit)

2 phase Neon beam tube Cu Tritium heater s s.c . Helium vessel Kr KATRIN requirement: T = 27 K with "T < 30 mK

Temperature [K]!

WGTS Demonstrator:

! on-site and cold tested

in 2010

! "Tmax = ± 3 mK

  • T. Thümmler - Status and commissioning of KATRIN
  • S. Grohmann et al., Cryogenics,

Volume 51, Issue 8, August 2011

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18

  • T. Thümmler - Status and commissioning of KATRIN

! active pumping, 4 TMPs !" Tritium retention 105 ! magnetic field: 5.6 T ! under construction, to be installed 2014 ! pumping by cryo-sorption !" Tritium retention >107 ! magnetic field: 5.6 T ! delivery Spring 2014

ß´s Argon Frost Pump T = 3 – 4.5 K

T2

cryo-sorption stainless steel

DPS2-F CPS ß´s

  • O. Kazachenko et al., NIM A 587 (2008) 136
  • F. Eichelhardt et al, Fusion Science and

Technology 54 (2008) 615

Transport and Pumping Sections

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19

no info

  • n m(!)
  • " filter out all ß-decay

electrons without m(! !)-info

  • reduce background

from ionising collisions

tandem design: pre-filter & energy analysis 1011 electrons/s ! 10-2 electrons/s

Electrostatic Spectrometers

pre-filter option

fixed retarding potential U0 = - 18.3 kV # #E ~ 100 eV

precision filter - scanning

variable retarding potential U0 = - 18.4 … -18.6 kV # #E ~ 0.93 eV (100% transmission)

  • T. Thümmler - Status and commissioning of KATRIN
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20 PINCH MAGNET DETECTOR MAGNET DETECTOR SUPPORT STRUCTURE VACUUM, CALIBRATION SYSTEM ELECTRONICS

  • T. Thümmler - Status and commissioning of KATRIN

!" Si-PIN diode !" detection of transmitted !’s (mHz to kHz) !" low background for T2 endpoint investigation !" high energy resolution:

"E = 1.48(1) keV (FWHM) at 18.6 keV

!" 12 rings with 30° segmentation + 4-fold center = 148 pixels !" minimize bg, investigate systematic effects !" compensate field inhomogeneities

  • f spectrometer’s analyzing plane.

KATRIN Main Detector

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21

KATRIN Main Detector

  • T. Thümmler - Status and commissioning of KATRIN

!" detector commissioning completed !" first light from spectrometer – May 2013 241Am

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22

  • T. Thümmler - Status and commissioning of KATRIN

! " earth magnetic/environmental fields distort

  • magn. flux tube in low field region (0.3 mT)!

! " needs to be compensated!! ! " low field correction:! ! " optimize flux tube! ! " fine tune transmission and resolution.!

Air Coil System

! " Earth magnetic field compensation & low field correction

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23

  • T. Thümmler - Status and commissioning of KATRIN

! " earth magnetic/environmental fields distort

  • magn. flux tube in low field region (0.3 mT)!

! " needs to be compensated!! ! " low field correction:! ! " optimize flux tube! ! " fine tune transmission and resolution.!

Air Coil System

! " Earth magnetic field compensation & low field correction

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24

  • T. Thümmler - Status and commissioning of KATRIN

Precision Energy Filter: variable retardation U0 = -18.4 … -18.6 kV # #E ~ 0.93 eV

Main Spectrometer:

!" MAC-E Filter principle # precise energy analysis !" Vacuum vessel on retarding potential !" high resolution: "E = 0.93 eV ! $ 10 m, length 23 m !" volume: 1240 m$ !" inner surface: 690 m% ! Reduce background rate: ! ultra high vacuum (UHV): p < 10-11 mbar ! induced by cosmic ray muons:

! background increase ! counter measure: wire electrode

E E0 Bmin Bmax 1 20000

KATRIN Main Spectrometer

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25

  • T. Thümmler - Status and commissioning of KATRIN

Spectrometer itself is a source of background

Wire defines electrostatic filter:

! 240 modules, 23000 wires ! precision requirement 0.2 mm ! compatible to UHV

  • K. Valerius et al., Particle and Nuclear

Physics, Volume 64, Issue 2, April 2010

KATRIN Main Spectrometer

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26

  • T. Thümmler - Status and commissioning of KATRIN

Wire Electrode Installation - completed

! "

wire installation until Jan. 2012 (7 Years)!

! "

entry electrodes mid 2012!

! "

baffle and getter pump and" complete vacuum system until Nov. 2012!

! "

next: baking / vacuum conditioning!

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27

Radon as Background Source

" 219Rn emanation from St707 NEG getter strips (3 ∙ 1 km) in pump ports

  • T. Thümmler - Status and commissioning of KATRIN
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28

Radon as Background Source

" 219Rn emanation from St707 NEG getter strips (3 ∙ 1 km) in pump ports

Auger electrons shake-off electrons conversion electrons shell reorganisation electrons

  • T. Thümmler - Status and commissioning of KATRIN
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29

Radon as Background Source

" 219Rn emanation from St707 NEG getter strips (3 ∙ 1 km) in pump ports

Auger electrons shake-off electrons conversion electrons shell reorganisation electrons

F.M. Fränkle et al.,

  • Astropart. Phys. 35 (2011) 128
  • S. Mertens et al.,
  • Astropart. Phys. 41 (2013) 52
  • T. Thümmler - Status and commissioning of KATRIN
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30

Auger electrons shake-off electrons conversion electrons shell reorganisation electrons

" passive background reduction: LN2-cooled baffles to cryocondense 219Rn

  • T. Thümmler - Status and commissioning of KATRIN

Radon as Background Source

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31

time [s]

#" 219,220Rn emanation from bulk material of vessel #" need active background suppression " stored multi-keV electrons: rapid cyclotron motion intermediate axial oscillation slow magnetron drift

Background Reduction

" " " " " "

" Background process continues:

  • " ionization of residual gas secondary electrons
  • " primary electron energies: 100 eV < E < 500 keV
  • " up to 5000 secondary electrons per stored primary
  • " significant background increase for hours
  • T. Thümmler - Status and commissioning of KATRIN
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32

" ExB drifts: electrons hit wall (works for E < 2 keV) " 1 kV between dipole halves, vessel Ø 10m E=100 V/m

electric dipole

energy [eV]

  • T. Thümmler - Status and commissioning of KATRIN

Background Reduction Methods

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33

" ExB drifts: electrons hit wall (works for E < 2 keV) " 1 kV between dipole halves, vessel Ø 10m E=100 V/m

electric dipole magnetic pulse

drift into flux tube drift out of flux tube t B E rot ! ! " = t B r E ! ! " = 2

< ! ! t B

> ! ! t B

# Maxwell law

  • f induction:

# Reduction of field strength increased cyclotron radius electrons hits the wall (works for all energies, but reversible) energy [eV]

  • T. Thümmler - Status and commissioning of KATRIN

Background Reduction Methods

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34

electron cyclotron resonance

" ExB drifts: electrons hit wall (works for E < 2 keV) " 1 kV between dipole halves, vessel Ø 10m E=100 V/m

electric dipole magnetic pulse

drift into flux tube drift out of flux tube t B E rot ! ! " = t B r E ! ! " = 2

< ! ! t B

> ! ! t B

# Maxwell law

  • f induction:

# Reduction of field strength increased cyclotron radius electrons hits the wall (works for all energies, but reversible) # Stochastic heating: RF puls matched to cycl. freq. % %RF = % %cycl

! " m eB =

  • inc. cyclotron radius

electron hits the wall

(works for all energies)

energy [eV]

  • T. Thümmler - Status and commissioning of KATRIN

Background Reduction Methods

  • S. Mertens et al.,

arXiv:1205.3729

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35

  • T. Thümmler - Status and commissioning of KATRIN

"" aim: UHV in huge spectrometer: p & 10-11 mbar "" to do: spectrometer bake-out at T = 300 °C "" achieved in January 2013 !

Vacuum conditioning for the commissioning measurements

Spectrometer Commissioning

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36

  • T. Thümmler - Status and commissioning of KATRIN

Spectrometer bake-out: procedure

"" slow heating: expansion of vessel and electrode by 10 cm "" temperature breakpoints: 200°C – water vapor removal 300°C – activation of getter material

1,E-11 1,E-10 1,E-09 1,E-08 1,E-07 1,E-06 1,E-05 1,E-04 50 100 150 200 250 300 350 350 450 550 650 750 850 950

pressure in mbar temperature in °C time in hours

Baking cycle (4. - 30.1.2013) temperature pressure

leak developed pressure back at 10-11 mbar level

Spectrometer Commissioning Status

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37

  • T. Thümmler - Status and commissioning of KATRIN

Spectrometer bake-out: procedure

"" slow heating: expansion of vessel and electrode by 10 cm

Spectrometer Commissioning Status

10 cm at 20 °C at 300 °C Remember what‘s inside!

"

$$$$$$$$$$$$$$$$$$$ $$$$$$$$$$$$$$$$$$$ $$$$$$$$$$$$$$$$$$$ $$$$$$$$$$$$$$$$$$$$$$ $$$$$$$$$$$$$$$$$$$ $ $ $ $ $ $ $ $ $ $ $ $ $ $

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$$

"

$$

$

" "

$ $ $ $ $

$ $

$ $ $ $ $$

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38

  • T. Thümmler - Status and commissioning of KATRIN

Spectrometer bake-out: procedure

"" slow heating: expansion of vessel and electrode by 10 cm

Spectrometer Commissioning Status

10 cm at 20 °C at 300 °C Remember what‘s inside!

"

$$$$$$$$$$$$$$$$$$$ $$$$$$$$$$$$$$$$$$$ $$$$$$$$$$$$$$$$$$$ $$$$$$$$$$$$$$$$$$$$$$ $$$$$$$$$$$$$$$$$$$ $ $ $ $ $ $ $ $ $ $ $ $ $ $

$ $

$

$$

"

$$

"

$$

$

" "

$ $ $ $ $

$ $

$ $ $ $ $$

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39

  • T. Thümmler - Status and commissioning of KATRIN

Spectrometer – Detector Integration

Spectrometer Detector

X-rays visual

!" detector integration requires valve

inside magnet bore: beam-line valve

!" deformation of O-Ring during baking

disabled the valve’s basic function

!" challenge to attach detector without

venting / getter contamination

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40

  • T. Thümmler - Status and commissioning of KATRIN

1240 m$

Ar 6.0 Ar 9.0

XENON 1t gas purification technology

144 bottles of Argon gas N6.0 $" O-Ring exchanged under Ar over pressure $" beal-line valve leak tight $" detector section attached

Spectrometer – Detector Integration

!" replacing the O-Ring requires work

under Ar gas atmosphere

!" NEG pump requires Ar of quality N9.0

to prevent contamination

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41

!

Commissioning of the Spectrometer and Detector Sections" (= all non Tritium parts of KATRIN)" ! Monitor! Spectrometer! Main Spectrometer! Main" Detector! E-Gun!

developed! at Uni Münster!

  • T. Thümmler - Status and commissioning of KATRIN

SDS Commissioning

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42

  • T. Thümmler - Status and commissioning of KATRIN

Present Status:

!" pressure p = 7 x 10-11 mbar !" identical to situation before venting !" all subsystems operational: !" Vacuum and High Voltage !" S.C. Magnets, Air Coils !" Detector and DAQ !" Monitoring and Database !" Online-Analysis !" first light seen on May 31, 2013

SDS Commissioning

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43

SDS Commissioning & First Light

  • T. Thümmler - Status and commissioning of KATRIN

! asym. magn. field !" map electrode structure

  • nto detector
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44

SDS Commissioning & First Light

  • T. Thümmler - Status and commissioning of KATRIN

! asym. magn. field !" map electrode structure

  • nto detector

!" rate related to electrode

potential

preliminary

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45

SDS Commissioning & First Light

  • T. Thümmler - Status and commissioning of KATRIN

! asym. magn. field !" map electrode structure

  • nto detector

!" rate related to electrode

potential

!" rings identified

Preliminary

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46

SDS Commissioning & First Light

  • T. Thümmler - Status and commissioning of KATRIN

!" sym. magn. field !" MAC-E filter conditions !" rate dropped to 1.6 cps at

retarding pot. U = -600 V

!" preliminary and to be

improved!

preliminary

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47

SDS Commissioning & Next Steps

  • T. Thümmler - Status and commissioning of KATRIN

!"

Setup, DAQ, Database and Analysis working fine

!"

there is room for improvements

!"

Background rate is low, but not low enough for KATRIN

!"

1.6 cps at 146 pixels makes 10-2 cps per pixel

!"

Tritium runs requires 10-2 cps for all pixels

!"

no evidence for Penning-like traps found

!"

angular selective electron gun to be commissioned next

!"

check transmission properties of MAC-E filter

!"

commission high-voltage operation up to 35 kV

!"

check background and transmission under KATRIN conditions

!"

commission LN2 baffle system

!"

investigate Rn-related background

!"

investigate background reduction methods

!"

qualify main spectrometer for Tritium operation in 2015

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48

KATRIN Sensitivity

#" reference ! !-mass sensitivity for 3 ´full beam´ years (5y cal. time):

  • " statistical & systematic errors

contribute equally: statistics & &stat = 0.018 eV2 systematics & &syst < 0.017 eV2 sensitivity m(!) = 200 meV (90% CL) 350 meV (5&) #" plans for a later KATRIN phase II:

  • differential ß-energy spectrum:

cryo-bolometer array with #E ~ 1eV? synchrotron emission (GHz-range)?

  • precision external value end point E0
  • atomic tritium source?

10&'' 4&''

electron energy +18.5 keV [eV] 66 68 70 72 74 1 0.99 0.98 0.97 0.96 ratio of specta

  • T. Thümmler - Status and commissioning of KATRIN

full beam time [months]

1200 1000 800 600 400 200

sensitivity 90% CL [meV]

0 2 4 6 8 10

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49

  • T. Thümmler - Status and commissioning of KATRIN

Summary & Outlook

! " motivation for neutrino mass meas. from particle and astroparticle physics ! !

! decay offers a model-independent method to determine m"!

! " KATRIN is designed to reach a sensitivity of 200 meV on m"%

!

! " KATRIN continuing construction and started commissioning:! ! " Source under construction, to be delivered in early 2015! ! " Transport sections under construction,"

to be delivered Spring 2014!

! " Main Spectrometer and Detector"

commissioning just started!

! "

First Light on May 31st!

! "

Continuing with HV and Baffle"

  • peration until September.!

! "

Upgrade program in Fall 2013!