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Towards Majorana neutrino spectroscopy M. Yoshimura

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Presentation on theme: "Towards Majorana neutrino spectroscopy M. Yoshimura"— Presentation transcript:

1 Towards Majorana neutrino spectroscopy M. Yoshimura
Why atoms ? Another or perhaps a unique way of Majorana detection  Measurement of absolute mass scale hep-ph/ Possibility of detecting relic neutrino hep-ph/

2 Significance of discovering Majorana neutrino
Neutral fermions follow economic Majorana eq or the same Dirac eq as charged ? Leading to lepton number violation and lepto-genesis    particle = anti-particle missing partner for leptogenesis Contributing to better understanding of seesaw mechanism and GUT

3 M vs D

4 Merits and demerits of atomic process
Infinitely many small energies Small pair emission rate How to enhance; resonance by energy input strong field

5 Majorana vs Dirac equations: chirally projected solutions

6 Unique signature of Majorana = interference of identical fermions
Effective only for pair emission Appear only (ii) threshold; proportional to m_i^2 Can be positive or negative Direct test of Majorana nature  cf LV in

7 2 promissing atomic processes
Low level metastable atoms laser irradiated Rydberg atoms microwave irradiated (not discussed here)

8 Neutrino pair emission from laser irradiated metastable state

9 Rough estimate of rate

10 Refinement

11 Threshold behavior 6 channels

12 Numerical estimate w.Y. Okabayashi
Input angles and masses

13

14 Total rate / rate for massless
Several % mass effects for 0.5 eV

15 Large mass effects

16 Theta_12 effect

17 Observability of relic neutrino w. T. Takahashi hep-ph/0703019
Pauli blocking effect

18 Magnitude of Pauli blocking

19 m_1 dependence for standard 1.9 K

20 Temperature measurement possible ?

21 12 threhold

22 Early universe probed by relic neutrino
Decoupling temperature Early universe after neutrino decoupling and before e^+ annihilation Large lepton asymmetry Constraint on sterile neutrino Surprizes ?

23 Measuring the lepton asymmetry
Definitive test of leptogenesis Extremely difficult, (12) or (13) threshold most promissing

24 Experiments are not easy
Discovery of atomic pair emission Mass measurement M/D distinction Relic detection

25 Summary Discussed laser irradiated pair emission to determine the magnitude and the nature of neutrino masses Identical particle effect of Majorana particles Neutrino mass spectroscopy towards 1 meV range Relic neutrino search


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