Toroidal Axion Haloscope Development at CAPP Harry W Themann - - PowerPoint PPT Presentation

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Toroidal Axion Haloscope Development at CAPP Harry W Themann - - PowerPoint PPT Presentation

Toroidal Axion Haloscope Development at CAPP Harry W Themann Center for Axion and Precision Physics Daejeon, ROK LLNL-Microwave Cavity Workshop 2017 1/11/2017 Harry W Themann CAPP 1 Why Toroid? 2 Axion Power


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SLIDE 1

Toroidal Axion Haloscope Development at CAPP

Harry W Themann Center for Axion and Precision Physics Daejeon, ROK LLNL-Microwave Cavity Workshop 2017

1/11/2017 Harry W Themann CAPP 1

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SLIDE 2

Why Toroid?

Axion Power 𝑄

𝑏 ∝ 𝑅𝐷𝐢2π‘Š

  • Larger cavities, higher field magnets, preserve Q & C
  • Larger cavities -> problem at higher frequencies
  • Multiple Cavities (see SW Youn)
  • What about Toroids?
  • No endcaps, can I get something for nothing?
  • With a toroidal magnet the 𝐢 field is, at least nominally, parallel

to all conductive surfaces

  • Lends itself to superconductive films?

1/11/2017 Harry W Themann CAPP 2

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SLIDE 3

Toroid Modes

  • No pure TM or TE modes
  • Inverse toroid aspect ratio 𝜍0 =

𝑠 𝑆

  • Bicycle tubes are better than

truck tubes

  • 𝐹 field lines of desired mode

similar to applied B field

  • No mode crossings

1/11/2017 Harry W Themann CAPP 3

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SLIDE 4

Analytic Modes

  • Cap and Deutsch lEEE Transactions on Microwave

Theory and Techniques Vol MTT-26,NO.7, JULY1978

  • Janaki & Dasgupta IEEE Transactions on Plasma

Science, VOL. I X . NO. I . FEBRUARY 1990

  • Inverse toroid aspect ratio 𝜍0 =

𝑠 𝑆

  • J & D expand in 𝜍0
  • π‘ˆπ‘"π‘šπ‘—π‘™π‘“" ∝ 𝑏=0

∞

𝑏𝑗 TM + 𝑐=0

∞

𝑐𝑗 TE

  • As 𝑆 β†’ ∞ 𝜍0 β†’ 0 π‘ˆπ‘"π‘šπ‘—π‘™π‘“" 𝑐𝑓𝑑𝑝𝑛𝑓𝑑 π‘ˆπ‘
  • For the dimensions contemplated there are no

degeneracies, no crossings

  • We used simulation to verify this

1/11/2017 Harry W Themann CAPP 4

r R

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SLIDE 5

1/11/2017 Harry W Themann CAPP 5

  • B. R. Ko; Axion Dark Matter Workshop, Stockholm

Effective Volume B2VC

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SLIDE 6

1/11/2017 Harry W Themann CAPP 6

Low Fringe Fields

R = 200cm R = 50cm Bavg= 5T 9 coils

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SLIDE 7

1/11/2017 Harry W Themann CAPP 7

Q Factor

  • B. R. Ko; Axion Dark Matter Workshop, Stockholm
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SLIDE 8

Assembly Concept

1/11/2017 Harry W Themann CAPP 8

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SLIDE 9

Assembly Concept

1/11/2017 Harry W Themann CAPP 9

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SLIDE 10

Assembly Concept

1/11/2017 Harry W Themann CAPP 10

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SLIDE 11

First Toroid β€œSUB”

  • Driven by a desire to be able

to mount in a cryocooler available to us

  • R=4cm r=2cm 𝜍0 = 0.5
  • Simulation verifies no mode

crossing

1/11/2017 Harry W Themann CAPP 11

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SLIDE 12

Cappuccino β€œSUB”

  • Early iteration of design
  • Simulation
  • Dimensions of SUB
  • Dimensions of tune hoop
  • Antenna sizes and shapes
  • Antenna placement (we had them

at angles in the beginning)

1/11/2017 Harry W Themann CAPP 12

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SLIDE 13

Design Challenges

  • Three sections not

necessary for this model but we decided to have a learning experience

  • One challenge was to exert

force to push ends together

1/11/2017 Harry W Themann CAPP 13

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SLIDE 14

Photo

1/11/2017 Harry W Themann CAPP 14

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SLIDE 15

CAD Pictures

1/11/2017 Harry W Themann CAPP 15

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SLIDE 16

First Look

  • Coupling issues, cross talk with each other with hoop, sim

vs data

  • Best antenna shape/size, reality vs simulation
  • Q factor
  • Calculated 20 000
  • Alignment issues, best 6000
  • Indium β€œgaskets” were a failure
  • Bagel cut achieved 20 000 w/o hoop
  • The simulations predicted that the hoop must go

upwards but doesn’t seem to matter

1/11/2017 Harry W Themann CAPP 16

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SLIDE 17

Finished Product

1/11/2017 Harry W Themann CAPP 17

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1/11/2017 Harry W Themann CAPP 18

Q = 10,700 CF = 8.159GHz

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SLIDE 19

1/11/2017 Harry W Themann CAPP 19

  • B. R. Ko; Axion Dark Matter Workshop, Stockholm
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SLIDE 20

Pictures

1/11/2017 Harry W Themann CAPP 20

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SLIDE 21

Future

1/11/2017 Harry W Themann CAPP 21

500mm Major Radius

  • Continue to develop flanging
  • Scale up tuning
  • Cryogenic ready
  • Packaging
  • Physical placement
  • Placement WRT to cooling
  • Cable routing
  • Actuation routing
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SLIDE 22

Conclusion

  • We have a working toroidal cavity
  • Learned a lot but this has also made

us realize that there are some daunting challenges in front of us.

  • CAPP LVP Hall is building

momentum rapidly

1/11/2017 Harry W Themann CAPP 22

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SLIDE 23

BACKUP

1/11/2017 Harry W Themann CAPP 23

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Assembly Concept

1/11/2017 Harry W Themann CAPP 24

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Challenges

1/11/2017 Harry W Themann CAPP 25

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SLIDE 26

1/11/2017 Harry W Themann CAPP 26

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SLIDE 27

1/11/2017 Harry W Themann CAPP 27

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SLIDE 28

1/11/2017 Harry W Themann CAPP 28

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SLIDE 29

1/11/2017 Harry W Themann CAPP 29

  • B. R. Ko; Axion Dark Matter Workshop, Stockholm