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Direct Neutrino Mass Measurements 5 th International Symposium on Symmetries in Subatomic Physics, Groningen, June 17-22, 2012 Christian Weinheimer Institut fr Kernphysik, Westflische Wilhelms-Universitt Mnster weinheimer@uni-muenster.de


  1. Direct Neutrino Mass Measurements 5 th International Symposium on Symmetries in Subatomic Physics, Groningen, June 17-22, 2012 Christian Weinheimer Institut für Kernphysik, Westfälische Wilhelms-Universität Münster weinheimer@uni-muenster.de Introduction ● The KArlsruhe TRItium Neutrino experiment KATRIN ● Other direct neutrino mass approaches ● Summary ● Photo: M. Zacher Christian Weinheimer SSP 2012, Groningen, June 21, 2012 1

  2. Hot Dark Matter: neutrinos Their contribution depends on m ν Results of recent oscillation experiments: Θ 23 , Θ 12 , Θ 13 , Δ m 2 23 , Δ m 2 12 ν e ν µ ν τ ν 1 ν 2 ν 3 Relics from the hot plasma after the big bang (like CMB): 336 ν / cm 3 Ω 1 degenerated masses 0.1 cosmological relevant e.g. seesaw mechanism type 2 0.01 hierarchical masses Δ m 2 0.001 23 e.g. seesaw mechanism type 1 explains smallness of masses, Δ m 2 but not mixing 12 Christian Weinheimer SSP 2012, Groningen, June 21, 2012 2

  3. Three complementary ways to the absolute neutrino mass scale 1) Cosmology very sensitive, but model dependent compares power at different scales current sensitivity: Σ m( ν i )  0.5 eV e.g. S. Hannestad, Prog. Part. Nucl. Phys. 65 (2010) 185 Search for 0 νββ 2) Sensitive to Majorana neutrinos Evidence for m ee ( ν )  0.3 eV ? GERDA is running, EXO delivered 1 st limit ! m ββ ( ν ) = | Σ |U ei 2 | e i α (i) m( ν i )| 3) Direct neutrino mass determination: No further assumptions needed. no model dependence use E 2 = p 2 c 2 + m 2 c 4  m 2 ( ν ) is observable mostly most sensitive methode: endpoint spectrum of β -decay m 2 ( ν e ) = Σ |U ei 2 | m 2 ( ν i ) Christian Weinheimer SSP 2012, Groningen, June 21, 2012 3

  4. Direct determination of m( ν e ) from β decay  (A,Z+1) + + e- + ν e β decay: (A,Z) Complementary to 0 νββ Complementary to 0 νββ and cosmology β electron energy spectrum: and cosmology dN/dE = K F(E,Z) p E tot (E 0 -E e ) Σ |U ei | 2  (E 0 -E e ) 2 – m( ν i ) 2 (modified by electronic final states, recoil corrections, radiative corrections) averaged neutrino mass Review: Review: E.W. Otten & C. Weinheimer E.W. Otten & C. Weinheimer Rep. Prog. Phys., 71 (2008) 086201 Rep. Prog. Phys., 71 (2008) 086201 Need: low endpoint energy  Tritium 3 H, ( 187 Re) very high energy resolution & very high luminosity &  MAC-E-Filter very low background (or bolometer for 187 Re) Christian Weinheimer SSP 2012, Groningen, June 21, 2012 4

  5. Tritium experiments: source  spectrometer MAC-E-Filter ● Two supercond. solenoids compose magnetic guiding field ● adiabatic transformation: µ = E/B = const.  parallel e - beam ● Energy analysis by electrostat. retarding field Δ E = EB min /B max = 0.93 eV (KATRIN)  sharp integrating transmission function without tails  Magnetic Adiabatic Collimation + Electrostatic Filter (A. Picard et al., Nucl. Instr. Meth. 63 (1992) 345) Christian Weinheimer SSP 2012, Groningen, June 21, 2012 5

  6. The Mainz Neutrino Mass Experiment Phase 2: 1997-2001 ⇓ After all critical systematics measured by own experiment (atomic physics, surface and solid state physics: inelastic scattering, self-charging, neighbour excitation): m 2 ( ν ) = -0.6 ± 2.2 ± 2.1 eV 2  m( ν ) < 2.3 eV (95% C.L.) C. Kraus et al., Eur. Phys. J. C 40 (2005) 447 Christian Weinheimer SSP 2012, Groningen, June 21, 2012 6

  7. The Troitsk Neutrino Mass Experiment windowless gaseous T 2 source, similar to LANL MAC-E-Filter, similar to Mainz Vladimir Mikhailovich Lobashev Δ E = 3.5eV Energy resolution: Luminosity: L = 0.6cm 2 1934-2011 3 electrode system in 1.5m (L = ΔΩ /2 π * A source ) diameter UHV vessel (p<10 -9 mbar) Re-analysis of Troitsk data (better source thickness, better run selection) Aseev et al, Phys. Rev. D 84, 112003 (2011) m β < 2.2 eV, 95% CL Christian Weinheimer SSP 2012, Groningen, June 21, 2012 7

  8. The KATRIN experiment at KIT Aim: m( ν e ) sensitivity of 200 meV (currently 2 eV) ● very high energy resolution ( Δ E  1eV, i.e. σ = 0.3 eV)  source  spectrometer concept ● strong, opaque source  dN/dt ~ A source ● magnetic flux conservation (Liouville)  scaling law: A spectrometer / A source = B source / B spectrometer = E / Δ E = 20000 / 1 detector KATRIN Design Report 70 m main spectrometer Scientific Report FZKA 7090) pre tritium spectro- retention meter windowless gaseous 10m system molecular tritium source Christian Weinheimer SSP 2012, Groningen, June 21, 2012 8

  9. Molecular Windowless Gaseous Tritium Source WGTS T 2 WGTS: tub in long superconducting solenoids  9cm, length: 10m, T = 30 K Tritium recirculation (and purification) p inj = 0.003 mbar, q inj = 4.7Ci/s allows to measure with near to maximum count rate using ρ d = 5  10 17 /cm 2 with small systematics check column density by e-gun, T 2 purity by laser Raman Christian Weinheimer SSP 2012, Groningen, June 21, 2012 9

  10. Very successful cool-down and stability tests of the WGTS demonstrator cooling concept of WGTS: beam tube pressurized 2-phase Ne Ø=90mm arrival of WGTS demonstrator at KIT: April 2010 p r e l i m i n a r y S. Grohmann, S. Grohmann, Cryogenics 49, Cryogenics 49, No. 8 (2009) 413 No. 8 (2009) 413 Currently: tests of sc magnets, constructing of WGTS out of demonstrator Christian Weinheimer SSP 2012, Groningen, June 21, 2012 10

  11. Transport and differential & cryo pumping sections Cryogenic Differential Molecular windowless pumping pumping gaseous tritium source with Argon snow at LHe temperatures (successfully tested with the TRAP experiment)  10 -7 mbar l/s FT-ICR Penning traps to FT-ICR Penning traps to T 2 -injection 1.8 mbar l/s (STP) measure ions from WGTS measure ions from WGTS = 1.7*10 11 Bq/s = 40 g/d < 2.5 10 -14 mbar l/s  adiabatic electron guiding & T 2 reduction factor of ~10 14 Christian Weinheimer SSP 2012, Groningen, June 21, 2012 11

  12. Commissioning of DPS2-F Ion test source: Ion test source: S. Lukic et al., S. Lukic et al., Rev. Scient. Instr. Rev. Scient. Instr. 82 (2011) 013303 82 (2011) 013303 FT-ICR Penning traps: FT-ICR Penning traps: M. Ubieto-Diaz et al., M. Ubieto-Diaz et al., Int. J. Mass. Spectrom. Int. J. Mass. Spectrom. 288 (2009) 1-5 288 (2009) 1-5 gas inlet outgoing gas flow ≈ 3 × 10 17 ≈ 3 × 10 12 molecules/s molecules/s First gas flow reduction measurements with Ar Currently: Problem of a broken diode S. Lukic et al., from the safety system Vacuum 86 (2012) 1126 of a superconducting coil Christian Weinheimer SSP 2012, Groningen, June 21, 2012 12

  13. Electromagnetic design: magnetic fields B-field [T] 1:20000  Δ E = E  B min / B max = E  1 / 20000 = 0.93 eV -40 -30 -20 -10 0 +10 aircoils: distance from analysing plane [m] axial field shaping + earth field compensatio n Christian Weinheimer SSP 2012, Groningen, June 21, 2012 13

  14. The detector Requirements VACUUM, CALIBRATION SYSTEM ● detection of β -electrons (mHz to kHz) ● high efficiency (> 90%) ● low background (< 1 mHz) ELECTRONICS (passive and active shielding) DETECTOR PINCH MAGNET DETECTOR ● good energy resolution (< 1 keV) MAGNET Properties electrons    ● 90 mm Ø Si PIN diode SUPPORT STRUCTURE ● thin entry window (50nm) ● detector magnet 3 - 6 T ● post acceleration (30kV) (to lower background in signal region) ● segmented wafer (145 pixels) → record azimuthal and radial profile of the flux tube → investigate systematic effects → compensate field inhomogeneities Christian Weinheimer SSP 2012, Groningen, June 21, 2012 14

  15. KATRIN detector is being commissioned at KIT Christian Weinheimer SSP 2012, Groningen, June 21, 2012 15

  16. Main Spectrometer – Transport to Karlsruhe Institute of Technology 8800 km Leopoldshafen, 25.11.06 Christian Weinheimer SSP 2012, Groningen, June 21, 2012 16

  17. KATRIN has a 100-times larger surface, but requests same bg → something new e - Secondary electrons from wall/electrode  µ  by cosmic rays, environmental radioactivity, ...  New: wire electrode on slightly more negative potential  γ    U- Δ U U Mainz V (2004) Mainz 2001-2004 Christian Weinheimer SSP 2012, Groningen, June 21, 2012 17

  18. Design, construction and mounting of the 690m 2 2-layer wire electrode system Requirements: - 200 µ m precision - out-bakeable 350 o C - 10 -11 mbar compatiible - 1 kV difference voltage - non magnetic - ... Foto: Peter Lessmann Christian Weinheimer SSP 2012, Groningen, June 21, 2012 18

  19. Two-layer wire electrode modules installation inside main spectrometer All 248 modules are installed, January 31, 2012 Christian Weinheimer SSP 2012, Groningen, June 21, 2012 19

  20. Background from stored electrons: methods to avoid or to eliminate them Radon suppression by LN 2 cooled baffle Stored electron by magnetic mirrors F. Fränkle et al., Astropart. Phys. 35 (2011) 128 Nulling magnetic field by magn. pulse radial E x B drift due to electric dipole pulse Mechanical eliminating stored particles: M. Beck et al, Eur. Phys. J. A44 (2010) 499 Christian Weinheimer SSP 2012, Groningen, June 21, 2012 20

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