Search for Dark Neutrino via Vacuum Magnetic Birefringence Experiment - - PowerPoint PPT Presentation

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Search for Dark Neutrino via Vacuum Magnetic Birefringence Experiment - - PowerPoint PPT Presentation

Search for Dark Neutrino via Vacuum Magnetic Birefringence Experiment Kimiko Yamashita (Ochanomizu Univ.) Collaborators: X. Fan (Harvard Univ.), S. Kamioka, S. Asai (Tokyo Univ.) experiment A. Sugamoto (Ochanomizu Univ., OUJ) theory PTEP


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SLIDE 1

Search for Dark Neutrino via Vacuum Magnetic Birefringence Experiment

KEK-PH 2018

  • Feb. 16th 2018

KEK, Tsukuba

Collaborators:

  • X. Fan (Harvard Univ.), S. Kamioka, S. Asai (Tokyo Univ.) experiment
  • A. Sugamoto (Ochanomizu Univ., OUJ) theory

Kimiko Yamashita (Ochanomizu Univ.)

PTEP 2017 no. 12, 123B03 (2017), arXiv:1707.03609 (arXiv:1707.03308)

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SLIDE 2

Dark Matter Search

1

SM SM SM SM Dark fermion loop

Including Dark Matter as New Physics

DM:

  • ψ×1
  • P with

t

Including P Interaction

V-A interaction

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SLIDE 3

QED interaction

2

SM SM SM SM electron loop

Parity Conserving Interaction

  • M. Aaboud et al. [ATLAS Collaboration],

``Evidence for light-by-light scattering in heavy-ion collisions with the ATLAS detector at the LHC’’ Nature Phys.13, no. 9, 852 (2017)

t

cf.

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SLIDE 4

QED Case

3

  • W. Heisenberg, H. Euler, Z. Phys. 98, 714 (1936)

Heisenberg-Euler Lagrangian:

  • constant background

electromagnetic field Fµν

  • electron 1-loop diagrams

already known

related to this

・・・

Need to Calculate Effective Lagrangian → Vacuum Birefringence Experiment

from J. Schwinger,

  • Phys. Rev. 82, 664 (1951)
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SLIDE 5

4

Photon Energy Dark Fermion Mass << We calculated here including coefficients a,b,c

~ g4/m4

Eγ << mDM

Dark Sector Case (1/3)

+ ・・・

ignore higher dimensional terms

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SLIDE 6

5

Dark Sector Case (2/3)

extra U(1)

photon in our theory (massless) extra U(1) gauge boson

  • rdinary

photon in SM

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SLIDE 7

・Effective Lagrangian of Fourth Order

6

We followed a method developed by Schwinger

  • J. Schwinger,
  • Phys. Rev.82, 664 (1951)

P

c=0 when gA or gV is 0

Dark Sector Case (3/3)

Our work: PTEP 2017 no. 12, 123B03 (2017)

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SLIDE 8

7

・OVAL (Observing Vacuum with Laser) experiment ・BMV experiment ・PVLAS experiment

  • X. Fan etal. Eur. Phys. J. D 71, no. 11, 308 (2017)
  • Eur. Phys. J. D (2014) 68: 16
  • Eur. Phys. J. C (2016) 76: 24

laser laser Input laser

  • utput

laser

Vacuum Magnetic Birefringence Experiment (1/5)

Tabletop experiment

mirror mirror To see QED

1-loop effect (not yet observed)

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SLIDE 9

8

refringence: changing phase velocity of the light birefringence: changing phase velocity of 2 light polarizations in different ways

  • 1 2

Vacuum Magnetic Birefringence Experiment (2/5)

medium A medium B medium A medium B

・refractive index: n ・phase velocity: v → n = 1/v

v1 v2 v1 v1

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SLIDE 10

9

To detect birefringence, we observe a difference of polarization state

1) Ellipticity

Polarization Rotation Elliptically polarized 2) Direction of the long axis

  • f an ellipse

ex)

  • QED
  • dark sector in our model

1 2 1 2 ex) dark sector in our model with P

Vacuum Magnetic Birefringence Experiment (3/5)

initial polarization final polarization initial polarization final polarization

birefringence birefringence

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SLIDE 11

10

To detect P interaction, we propose a new method

Vacuum Magnetic Birefringence Experiment (4/5)

P example: ・refractions are occurred for 45 degree or -45 degree polarization modes in different ways ・Polarization with parallel includes both modes.

  • > We detect perpendicular

to see reflections QED: ・refractions are occurred for parallel (from magnetic field) or perpendicular polarization modes in different ways ・Polarization with 45 degrees includes both modes.

  • > We detect -45 degrees to see reflections

No QED background

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SLIDE 12

11

Ring Fabry-Perot resonator

Fabry-Perot resonator

mirror mirror mirror mirror mirror mirror

P is reduced if only 2 mirrors

Vacuum Magnetic Birefringence Experiment (5/5)

To detect P interaction, we propose a new method

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SLIDE 13

12

Dark neutrino

We assume gA = - gV (= |e|) to obtain the experimental constraint ↓ V – A current: Dark neutrino We examine the case, having both the electron and the lightest DS neutrino. For the DS search, QED forms the background to the DS signal.

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13

Allowed region

  • J. Jaeckel, Frascati Phys. Ser. 56, 172 (2012)

Log10 [eV]

dark photon mass GeV

At VMB experiment, the sensitivity does not depend on dark photon mass We focus

  • n this

region

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SLIDE 15

Conventional, QED/Dark neutrino

14

laser energy: 1 - 4 eV

Experimental Limit ⬇︎

QED ~100!

  • QED
  • dark

neutrino

↑Exclude region

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SLIDE 16

New set up, dark neutrino only

15

↓allowed

Experimental Limit ⬇︎

dark neutrino

P

↑Exclude region

P No QED background

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SLIDE 17

Summary

  • 1. We considered Parity violated dark sector model,

and derived generalized Heisenberg-Euler formula

  • 2. Our focus lay on light-by-light scattering effective

Lagrangian of fourth order and gave a result:

  • 3. We focused on Vacuum Magnetic Birefringence

Experiment to probe the dark sector and proposed new polarization state and the ring resonator in stead of the usual Fabry-Perot resonator to measure the Parity violated term

16

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SLIDE 18

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Backup

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Search for Dark Neutrino via Vacuum Magnetic Birefringence Experiment 20' We consider a dark matter model where a dark matter candidate couples to photons via an extra U(1) mediator and assume that this dark matter candidate is a fermion and can couple to the mediator with parity violation. We derived a low energy effective Lagrangian including a parity violated term for light-by-light scattering by integrating out the dark matter fermion. Our focus lies on Vacuum Magnetic Birefringence Experiment to probe the dark sector. We propose the ring resonator (3-4 mirrors) with an appropriate polarization state of light in stead of a usual Fabry-Perot resonator (2 mirrors) with a conventional polarization state of light to measure the Parity violated term. We assume that a dark neutrino is a dark matter, i.e. V-A current, and give constraints on model parameters from a current experimental limit. PTEP 2017 no. 12, 123B03 (2017) (arXiv: 1707.03308 [hep-ph]), arXiv:1707.03609 [hep-ph]

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SM + U’(1)Y’ + 1 Complex Scalar

spontaneously broken

Dark Matter Model (1/3)

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SLIDE 21

20

mass diagonalization We assume

Dark Matter Model (2/3)

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Dark Matter Model (3/3)

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2 conditions t

laser laser B B

1 eV 10 Tesla, (1 Tesla ~ 200 eV2)

e e e e Ψ with mass m

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SLIDE 24

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beam energy 1.16 eV @OVAL experiment

Vacuum Magnetic Birefringence Experiment: laser beam energy

For 2 mirrors system: 1 ~ 4 eV laser energy itself: m eV ~ 10 k eV are available thanks to X-ray Free Electron Laser