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Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.)...

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Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/21 17th Lomonosov 1
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Page 1: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

Neutrino mass spectroscopy with atoms-- experimental

status--

N. Sasao and M. Yoshimura (Okayama

U.)for SPAN collaboration

2015/8/21 17th Lomonosov 1

Page 2: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

Accelerated a rare process by a huge factor >1018

2015/8/21 17th Lomonosov 2

Prepared excited states: E1 transition (single is

forbidden. Two photon life time is very long.121/ 2 10 sec

Observed two photon process: From an ensemble of coherent

states With a trigger injected for one of

the two-photon partners. Huge acceleration factor >10^18

           compared with the spontaneous

rate.

Page 3: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

Outline

Unknowns in physics and an atomic way

Macro coherent amplification and its experimental proof

Future prospects and Summary

2015/8/21 17th Lomonosov 3

Key word 1: RENP (radiative emission of neutrino pairs) Key word 2: Macro-coherent amplification

Key word 3: PSR (paired super-radiance)

Page 4: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

Experimental principle and its characteristics

Experimental principle Radiative emission of -pair Measure photon energy spectrum

Merit and demerit using atoms ( energy scale of atoms )~( neutrino mass scale )

Sensitivity to absolute mass, hierarchy, M-D, CP-phases

Small rate -> need amplification: e.g. ~1/10^26 year for Q=1 eV

「 Macro-coherent amplification mechanism 」2015/8/21 17th Lomonosov 4

RENP(Radiative Emission of Neutrino Pair)

e g

Page 5: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

Expected RENP rate

RENP spectrum calculation: Calculated reliably with the standard model.

Example of RENP rate =50 Hz for Xe 3P1 (8.4365eV). n=7x 10^20 [cm-3], V=100 cm^3, =10^-3

2015/8/21 17th Lomonosov 5

“Neutrino Spectroscopy with Atoms and Molecules”,A. Fukumi et.al : Prog. Theor. Exp. Phys. 2012, 04D002

Macro-coherent amplification  ・ N^2   ・ momentum conservation

2(1 4sin )wQw N Z

Page 6: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

impact on neutrino physics

Absolute mass and hierarchy

Example of RENP spectrum( Xe )

Similar to muon decay spectrum

2015/8/21 17th Lomonosov 6

eg

M e

E

n=7x10^20 cm^-3V=100 cm^3

Xe: 8.4365 eV

thresholds:

0 1 2 3( , , )m Min m m m

4 [eV]

Page 7: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

Amplification by coherence among atoms

Super-Radiance De-excitation via single photon

emission

Macro-coherent amplification De-excitation via multi-particle

emission

2015/8/21 17th Lomonosov

1 2 3 0k k k

7

Ba SR experiment

“Production of Ba Metastable State via Super-Radiance”,C. Ohae et.al, JPSJ 83,044301 (2014)

Page 8: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

Experimental proof of macro-coherent amplification

PSR (paired super-radiance ) QED process where -pair is replaced with a photon. A pair of strong light pulses (SR) will be emitted.

2015/8/21 17th Lomonosov 8

“Dynamics of two-photon paired superradiance”,M. Yoshimura, N. S, and M. Tanaka, PHYSICAL REVIEW A 86, 013812 (2012)

Page 9: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

PSR experiment

Para-hydrogen molecule (Spin=0) Vibrational level (v=1) to ground

level (v=0). E1 forbidden. Small 2-photon emission rate:

Excitation by adiabatic Raman Irradiation by 2 lasers from one side An external trigger laser Detect 2-photon emissions

2015/8/21 17th Lomonosov 9

“Observation of coherent two-photon emission from the first vibrationally-excited state of hydrogen molecules”, Yuki Miyamoto et. al. Prog. Theor. Exp. Phys. 2014, 113C01

121/ 2 10 sec

Page 10: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

Features of adiabatic Raman process

Why we use Raman process? Creation of coherence among two levels |e> and |g> Generation of higher side-bands

2015/8/21 17th Lomonosov 10

Eigenstates:

Density matrix

Page 11: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

Experimental setup

2015/8/21 17th Lomonosov 11

T=77K, P=60kPa D=2cm, L=15cm

Page 12: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

Wavelengths to be rememberedand comments

Important wavelengths Macro-coherent ?

Energy conservation

Momentum conservation law is equivalent to energy conservation law.

2015/8/21 17th Lomonosov 12

Phase factor added to target

684nm

532nm

4.59um (trigger)

5.05um

1 2

2

( )N

i k k xa

a

R e M

Page 13: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

Observation of Raman sidebands

2015/8/21 17th Lomonosov 13

13 sidebands observed (λ=192 - 4662nm)

Evidence for large coherence

Page 14: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

Degree of coherence

Maxwell-Bloch eq.

Coherence estimated by simulation:

2015/8/21 17th Lomonosov 14

Page 15: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

Observation of two-photon process

2015/8/21 17th Lomonosov 15

4.59μm( External trigger )

|e> v=1

|g> v=05.05μm

“Externally triggered coherent two-photon emission from hydrogen molecules”, Yuki Miyamoto et. al. arXiv:1505.07663, accepted for publication in in Prog. Theor. Exp. Phys.

Page 16: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

Comparison with spontaneous emission

# of observed photons=6 x 10^11/pulse # of expected photons due to spontaneous

emission

Huge amplification factor of >10^(18). It can only be understood by macro-coherent

amplification mechanism.

2015/8/21 17th Lomonosov 16

2 70 0 0Expected photons=R 10 / pulse

Ew Ln A t

E

Page 17: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

How far have we reached?

RENP rate example =50 Hz for Xe 3P1

(8.4365eV). n=7x 10^20 [cm-3] V=100 cm^3, =10^-3

PSR experiment P-H2 (0.52eV). n=6x 10^19 [cm-3], V=1.5x10^-2 cm^3, =10^-3

2015/8/21 17th Lomonosov 17

n^3 V (Spectrum function)=(average coherence eg)x (stored field energy)/(n eg)

Caution: Direct comparison is not allowed because different atoms/molecules and/or different interactions (EM-Weak) are involved.

Page 18: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

Road map

Study and control PSR. PSR detailed study

Counter propagating PSR PSR control

Mode switching method

RENP basic study High density target with

coherence Soliton formations Control of background

RENP experiment

2015/8/21 17th Lomonosov 18

2~3 years

2~3 years

Page 19: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

summary

RENP Systematic way to measure neutrino’s undetermined parameters. Absolute mass, M-D distinction, CP-phases

Macro-coherent amplification Amplification due to coherence among particles

PSR Huge amplification >10^18 was observed using two-photon process from p-H2 vibrational levels.

Future prospect PSR Study in more detail RENP basic study RENP experiment

2015/8/21 17th Lomonosov 19

4~6 years

proves basic part of macro-coherence amplification

Page 20: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

Thank you for your attention

SPAN group (Spectroscopy with Atomic Neutrino) K.Yoshimura, A.Yoshimi, S. Uetake, M. Yoshimura, I. Nakano, Y. Miyamoto. T. Masuda, H.Hara, K. Kawaguchi, J. Tang  ( Okayama U. ) M.Tanaka (Osaka U) 、 T. Wakabayashi(Kinki U) 、 A.Fukumi (Kawasaki) S. Kuma(Riken), C. Ohae(UEC) 、 K.Nakajima(KEK) 、 H.Nanjo (Kyoto)

2015/8/21 17th Lomonosov 20

Page 21: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

Backups BG free RENP Physics goals: Majorana-Dirac and CP-phases Properties of observed signal Soliton

2015/6/30-7/6 China 21

Page 22: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

BG free RENP Electro-magnetic waves in waveguide

EM waves have “an effective mass” RENP is allowed but 3is forbidden

2015/6/30-7/6 China 22

“Radiative emission of neutrino pair free of quantum electrodynamic backgrounds” M. Yoshimura, N. Sasao, and M. Tanaka, http://arxiv.org/abs/1501.05713v1

Page 23: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

impact on neutrino physics (2)

Majorana-Dirac & CP -phases

Majorana-Dirac distinction Identical particle effect

CP-phase measurements Difference in spectrum

2015/8/21 17th Lomonosov 23

“Observables in Neutrino Mass Spectroscopy Using Atoms”, D.N. Dinh, S.T. Petcov, N.S, M.Tanaka, M.Yoshimura, Phys. Lett. B 719 (2013) 154–163

M(IH)

D(NH)

0

( ) / 5 0.428 [eV],

2 [meV]

eg egE E Yb

m

Page 24: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

Properties of observed signal

2015/8/21 17th Lomonosov 24

Page 25: Neutrino mass spectroscopy with atoms-- experimental status-- N. Sasao and M. Yoshimura (Okayama U.) for SPAN collaboration 2015/8/2117th Lomonosov1.

Soliton

”Stopped-light” Control transparency between p-g by

irradiating laser lights (control) between p-e Input signal light between p-g, and store

information in atomic coherence Retrieve information by control laser

Two-photon version of ”Stopped-light” Energy condensed state between light field and

matter (medium) Existence expected theoretically Created only in counter-propagating PSR

Need experimental studies Planning to create soliton by irradiating counter

propagating lasers with an appropriate intensity structure predicted by theory.

2015/8/21 17th Lomonosov 25

red: field strengthblack: coherenceblue: population difference


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