Double beta decay status and future
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Double Beta Decay - status and future. Double beta decay basics Experimental challenges Current experimental status HM(HKK) result Future experimental programmes Dark matter and bb0n.

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Double beta decay status and future

Double Beta Decay - status and future

Double beta decay basics

Experimental challenges

Current experimental status

HM(HKK) result

Future experimental programmes

Dark matter and bb0n

Based on talks at ApPEC Peer Review of bb0n, Nu2002 (heavily) ….and a night in the Lamb with Kai Züber and Roland


Double beta decay
Double Beta Decay

Cremonesi Nu2002


Bb0n rates
bb0n Rates

Cremonesi Nu2002


Why do bb0n
Why do bb0n?

Cremonesi Nu2002


Experimental considerations
Experimental Considerations

Measure this

Cremonesi Nu2002


Key issues
Key Issues

  • Multi-isotopic targets

    • “Redundancy, redundancy, redundancy” (J. Bahcall)

    • Background removal by different peak positions (ie noise peak at Q)

  • Enrichment

  • Radio-isotopic backgrounds

  • Energy Resolution

  • Discrimination

    • Removal of gamma, beta, neutron backgrounds

    • bb(2n) background irremovable (separate peaks)

    • Co-location of daughter ion

  • Theory

    • Matrix elements

  • Analysis techniques

    • Esp. in light of H-M claim


Current experimental limits
Current Experimental Limits

Cremonesi Nu2002


Current experimental limits1
Current Experimental Limits

Cremonesi Nu2002



Hm hvkk result
HM(HVKK) Result

Cremonesi Nu2002


Hm hvkk result1
HM(HVKK) Result

Cremonesi Nu2002


Comments on hm hvkk
Comments on HM(HVKK)

Cremonesi Nu2002



Igex canfranc
IGEX: Canfranc

hep-ex 0202026



Milano dbd ii
Milano DBD-II

Cremonesi Nu2002


Mdbd ii results
MDBD-II: Results

Cremonesi Nu2002


Mdbd ii background
MDBD-II: Background

Cremonesi Nu2002


Proposed experiments
Proposed Experiments

Cremonesi Nu2002


Proposed experiments1
Proposed Experiments

  • Half life normalised to 5 years operation

10’s kg scale

Tonne scale

  • Matrix element range. Half life for 50meV mass (in 1026y)

Elliott and Vogel Ann. Rev. Nucl. Part. Sci. 52 (2002)


Modularity and prototyping
Modularity and prototyping

  • Modularity

    • Discrimination through segmentation

    • Increase in support materials

      • GENIUS vs. Majorana

    • Systematics checks

  • Prototyping

    • Direct scale-up of current technology won’t require prototyping - too expensive?

    • Prototype is first module

    • All experiments involved in prototyping

      • Handling scale up issues (cryostats, mass, etc)

      • Handling readout options (laser tag, WLS fibres)

      • Cross check against Monte Carlo


Nemo iii
NEMO-III

Cremonesi Nu2002


Nemo iii1
NEMO-III

Cremonesi Nu2002


Cuore
CUORE

Cremonesi Nu2002


Cuoricino
CUORicino

Cremonesi Nu2002


Exo xenon
EXO - Xenon

Cremonesi Nu2002


Exo two approaches
EXO - two approaches

Cremonesi Nu2002


Majorana
Majorana

Cremonesi Nu2002


Genius
GENIUS

Cremonesi Nu2002


Genius tf
GENIUS-TF

Cremonesi Nu2002


GEM

Cremonesi Nu2002


Dcba cobra
DCBA/COBRA

Cremonesi Nu2002



Bb0n and dark matter
bb0n and dark matter

  • Many common elements for rare event searches

    • Theoretically prejudice for max sensitivity required

      • DM: 10-10pb covers most of SUSY models

      • bb: >10 meV from oscillations

      • Both require large mass targets (~1 tonne)

    • Low backgrounds required

      • High radio-purity materials

      • Good shielding

    • Discrimination required

      • DM: nuclear vs. electron recoil, spatial

      • bb: spatial (co-location of daughter)

    • Good resolution/threshold (high light yield, etc.)

      • DM: keV range - bite into DM spectrum

      • bb: MeV range - separate peaks at Q

  • Can we do both in one detector?

    • Xenon is an obvious candidate to consider within U.K.

Beware!


Xenon experience in uk ral
Xenon experience in UK/RAL

Gotthard Xe TPC DB experiment (Roland)

ZEPLIN dark matter programme

(RAL, IC, Shef)


Zeplin as bb0n experiment
ZEPLIN as bb0n experiment

  • Developing ideas for combining dark matter and bb0n experiments

    Key issues are

    • Energy scales of interest

      • Primarily a DAQ issue, saturation of readouts, etc.

    • Discrimination of backgrounds

      • Can position sensitivity in ZEPLIN be improved to check co-locality in DB?

    • Resolution at MeV scales

      • Looks OK in second generation DM targets

  • There is also b+b+ capability

    • 124Xe (0.1% in nat. Xe) is one of seven known b+b+ emitters

    • 2nb+ b+ gives 4x 511keV photon signal

    • 2nb+ECgives X-ray (30keV) and 2x 511keV photon signal (

    • 2nECECgives 2x X-ray (30keV) signal

      • Current limits for 124Xe are T0.52n > 2x1014 years, T0.50n > 4x1017 years


Conclusions
Conclusions

  • The bb0n decay search has the promise of illuminating

    • Absolute mass scale of neutrinos

      (note this is effective mass, unlike beta end point: KATRIN)

    • Lepton number violation

    • Majorana vs. Dirac description

  • Current limits/claims 300meV

    • H-M (HVKK) Claim contested

  • Oscillation results encourage meV searches

  • Several programmes suggested on Ge, Xe, Te, Mo

    • Need large scale, good resolution, discrimination, enrichment

  • Possibility of DM detectors as DB

    • ZEPLIN programme?

    • One man’s background….


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