High-Q 3D Photonic Bandgap Cavities for Axion Detection LLNL Axion - - PowerPoint PPT Presentation

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High-Q 3D Photonic Bandgap Cavities for Axion Detection LLNL Axion n Cavit ity Worksho hop p 2018 18 Ankur ur Agrawa wal, Akash Dixit, Aaron Chou, David I. Schuster The University of Chicago Outline Introduction to Photonic Band-gap


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SLIDE 1

High-Q 3D Photonic Bandgap Cavities for Axion Detection

LLNL Axion n Cavit ity Worksho hop p 2018 18 The University of Chicago Ankur ur Agrawa wal, Akash Dixit, Aaron Chou, David I. Schuster

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SLIDE 2

Outline

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  • Introduction to Photonic Band-gap (PBG) cavities
  • Motivation in the context of dark matter axion detection
  • Omni-directional PBG cavity
  • Simulation results

Ankur Agrawal | LLNL Cavity Workshop 2018

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SLIDE 3

Photonic Band-gap Material

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  • Band-structure for photons similar to

electrons in semiconducting materials

  • Created by periodic arrangement of

contrasting dielectric objects (atoms)

  • Simplest example is a Bragg reflector

in 1-D

  • Band-gap size,

ฮ”๐œ• ๐œ•๐‘› ~ ฮ”๐œ ๐œ

Ankur Agrawal | LLNL Cavity Workshop 2018

๐œ ๐œ = 13 = 1

The width of the ๐œ = 13 layer is 0.2a, and the width of ๐œ = 1 layer is 0.8a

Joannopoulos, John D., et al. Photonic crystals: molding the flow of light. Princeton university press, 2011.

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SLIDE 4

Photonic Band-gap Cavity

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  • Created by introducing a defect site in the

lattice

  • If defect mode frequency lies in the band-

gap, then it must exponentially decay

  • nce it enters the crystal
  • Q-values fundamentally limited by the

dielectric loss and surface loss at the boundary

Ankur Agrawal | LLNL Cavity Workshop 2018

Defect

The red curve is the electric field strength of the defect state associated with this structure เต— ๐œ‡ 2

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SLIDE 5
  • Cold microwave cavity immersed in a strong static

magnetic field (~ 8 Tesla)

Axion Dark Matter Haloscope

5 Ankur Agrawal | LLNL Cavity Workshop 2018

Microwave rowave Cavit ity 8-Tes esla la Magne gnet SQUID ID Amplifie plifier

โ…†๐‘‚๐‘ โ…†๐‘ข โˆ ๐ถ0

2๐‘…๐‘‘๐‘๐‘ค๐‘Š โˆ ๐‘”โˆ’11 3

  • Superconducting Nb RF cavities with Q~ 1010 ๏Œ
  • Copper cavities @ 10 GHz, Q ~ 104
  • High-Q cavities will allow us to
  • Match the readout cadence to the expected signal photon rate
  • Cavity Q in excess of the axion Q can be further used for

stimulated emission

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SLIDE 6

Omni-directional PBG Cavity

6 Ankur Agrawal | LLNL Cavity Workshop 2018

  • FCC-type lattice constructed with Rutile rods

(TiO2) in Sapphire

  • Complete confinement of a defect mode in all

directions

  • Dielectric loss tangent of Rutile and Sapphire is

< 10-6 thus, Q of 106 can be achieved

  • Compact

structures can be fit into small magnet bores

Johnson, S. G., & Joannopoulos, J. D. (2000). Applied Physics Letters, 77(22), 3490-3492.

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SLIDE 7

Simulation Results

7 Ankur Agrawal | LLNL Cavity Workshop 2018

0.05 0.1 0.15 0.2 0.25

  • 1.5
  • 1
  • 0.5

0.5 1 1.5 Frequen quency y (c/2a) Wave ve vector tor (k/2๐œŒ)

ฮ”๐œ• ๐œ•๐‘›~ 31%

MIT MPB simulation package For band-center @ 10GHz, a ~ 4.11 mm r ~ 0.293a ~ 1.26 mm and h ~ 0.93a ~ 4.0 mm Dielectric constant (๐œ): Rutile ~ 225 and Sapphire ~ 10 Rutile rods arranged in a trigonal pattern in Sapphire slab 4-5 periods on each side would be sufficient to exponentially suppress the losses at copper walls

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SLIDE 8

Simulation Results

8 Ankur Agrawal | LLNL Cavity Workshop 2018

A B C ANSYS HFSS package Defec fect Air rods in Sapphire substrate Defec efect

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SLIDE 9

Future ure Work: โ–ช Test powdered form

  • f

dielectric materials to estimate the enhancement in Q โ–ช Simulate a woodpile structure (Rutile-Sapphire) to get an idea of Q

Summary

9 Ankur Agrawal | LLNL Cavity Workshop 2018

โ–ช PBG Cavities made out of low-loss dielectric material may achieve high Q-values โ–ช High contrast dielectric materials allows compact structure to fit in small magnet bores โ–ช Cavity Q in excess of axion Q will further help in QND measurement using Qubits