The Corbino approach, where the sample of interest terminates a coaxial cable, is a well-established method for microwave spectroscopy. If the sample is dielectric and if the probe geometry basically forms a conductive cavity, this combination can sustain well-defined microwave resonances that are detrimental for broadband measurements. Here, we present detailed simulations and measurements to investigate the resonance frequencies as a function of sample and probe size and of sample permittivity. This allows a quantitative optimization to increase the frequency of the lowest-lying resonance.

1.
S. J.
Fiedziuszko
,
I. C.
Hunter
,
T.
Itoh
,
Y.
Kobayashi
,
T.
Nishikawa
,
S. N.
Stitzer
, and
K.
Wakino
,
IEEE Trans. Microwave Theory
50
,
706
(
2002
).
2.
J. R.
Mosig
,
J.-C. E.
Besson
,
M.
Gex-Fabry
, and
F. E.
Gardiol
,
IEEE Trans. Instrum. Meas.
IM-30
,
46
(
1981
).
3.
H. C. F.
Martens
,
J. A.
Reedijk
, and
H. B.
Brom
,
Rev. Sci. Instrum.
71
,
473
(
2000
).
4.
J.
Krupka
,
Meas. Sci. Technol.
17
,
R55
(
2006
).
5.
U.
Kaatze
,
Meas. Sci. Technol.
24
,
012005
(
2013
).
6.
O. M.
Corbino
,
Nuovo Cimento
1
,
397
(
1911
).
7.
J. C.
Booth
,
D. H.
Wu
, and
S. M.
Anlage
,
Rev. Sci. Instrum.
65
,
2082
(
1994
).
8.
N.
Tosoratti
,
R.
Fastampa
,
M.
Giura
,
V.
Lenzi
,
S.
Sarti
, and
E.
Silva
,
Int. J. Mod. Phys. B
14
,
2926
(
2000
).
9.
M. L.
Stutzman
,
M.
Lee
, and
R. F.
Bradley
,
Rev. Sci. Instrum.
71
,
4596
(
2000
).
10.
F.
Hohls
,
U.
Zeitler
,
R. J.
Haug
,
R.
Meisels
,
K.
Dybko
, and
F.
Kuchar
,
Phys. Rev. Lett.
89
,
276801
(
2002
).
11.
M.
Scheffler
and
M.
Dressel
,
Rev. Sci. Instrum.
76
,
074702
(
2005
).
12.
H.
Xu
,
S. M.
Anlage
,
L.
Hu
, and
G.
Gruner
,
Appl. Phys. Lett.
90
,
183119
(
2007
).
13.
S. T.
Ahmad
and
D. G.
Hasko
,
Microelectron. J.
39
,
1516
(
2008
).
14.
K.
Steinberg
,
M.
Scheffler
, and
M.
Dressel
,
Rev. Sci. Instrum.
83
,
024704
(
2012
).
15.
M.
Scheffler
,
K.
Schlegel
,
C.
Clauss
,
D.
Hafner
,
C.
Fella
,
M.
Dressel
,
M.
Jourdan
,
J.
Sichelschmidt
,
C.
Krellner
,
C.
Geibel
, and
F.
Steglich
,
Phys. Status Solidi B
250
,
439
(
2013
).
16.
H.
Kitano
,
T.
Ohashi
,
H.
Ryuzaki
,
A.
Maeda
, and
I.
Tsukada
,
Physica C
412–414
,
130
(
2004
).
17.
M.
Scheffler
,
M.
Dressel
,
M.
Jourdan
, and
H.
Adrian
,
Nature (London)
438
,
1135
(
2005
).
18.
H.
Kitano
,
T.
Ohashi
, and
A.
Maeda
,
Rev. Sci. Instrum.
79
,
074701
(
2008
).
19.
M.
Scheffler
,
M.
Dressel
, and
M.
Jourdan
,
J. Phys.: Conf. Ser.
200
,
012175
(
2010
).
20.
M.
Scheffler
,
M.
Dressel
, and
M.
Jourdan
,
Eur. Phys. J. B
74
,
331
(
2010
).
21.
K.
Steinberg
,
M.
Scheffler
, and
M.
Dressel
,
J. Appl. Phys.
108
,
096102
(
2010
).
22.
D.
Geiger
,
M.
Scheffler
,
M.
Dressel
,
M.
Schneider
, and
P.
Gegenwart
,
J. Phys.: Conf. Ser.
391
,
012091
(
2012
).
23.
J. C.
Booth
, Ph.D. thesis,
University of Maryland
, College Park,
1996
.
24.
J. C.
Booth
,
D.-H.
Wu
, and
S. M.
Anlage
, in
Fluctuation Phenomena in High Temperature Superconductors
,
NATO ASI Series 3: High Technology
Vol.
32
, edited by
M.
Ausloos
and
A. A.
Varlamov
(
Kluwer
,
Dordrecht
,
1997
), p.
151
.
25.
M.
Scheffler
,
S.
Kilic
, and
M.
Dressel
,
Rev. Sci. Instrum.
78
,
086106
(
2007
).
26.
CST STUDIO SUITE (TM) 2011, Release Version 2011.03, CST AG.
27.
2.4 mm Calibration Kit HP 85056A (Hewlett-Packard) (now Agilent).
28.
This commercial calibration is not designed for Corbino measurements, but for devices under test with conventional connectors. This calibration procedure leads to systematic errors in our Corbino data, such as off-resonance values of S11 that differ from or even exceed unity in Figs. 2, 5, and 6, but these do not affect our conclusions concerning the resonances. Here, we prefer this commercial calibration to a dedicated three-standard Corbino procedure9,11,18 because the open and load standards of the latter can introduce errors due to resonances of exactly the type we address in the present study.11 
29.
T.
Konaka
,
M.
Sato
,
H.
Asano
, and
S.
Kubo
,
J. Supercond.
4
,
283
(
1991
).
30.
V. E.
Bottom
,
J. Appl. Phys.
43
,
1493
(
1972
).
31.
Material library of CST Microwave Studio, Release Version 2011,
2011
.
32.
The reasons for the mismatch between simulation and experiment are not completely clear. They could be due to discrepancies between experiment and simulation either in the material parameters or in the sample geometry. This would explain the larger discrepancies at higher frequencies and higher permittivities. This does not hold for the two dips in the spectra at about 30 GHz and 33 GHz, which are observable in all three measured spectra and can therefore be identified as experimental artifacts.
33.
Z.-Y.
Shen
,
C.
Wilker
,
P.
Pang
,
W. L.
Holstein
,
D.
Face
, and
D. J.
Kountz
,
IEEE Trans. Microwave Theory
40
,
2424
(
1992
).
34.
J.
Mazierska
,
J. Supercond.
10
,
73
(
1997
).
35.
W. A.
Huttema
,
B.
Morgan
,
P. J.
Turner
,
W. N.
Hardy
,
X.
Zhou
,
D. A.
Bonn
,
R.
Liang
, and
D. M.
Broun
,
Rev. Sci. Instrum.
77
,
023901
(
2006
).
36.
N.
Pompeo
,
R.
Marcon
, and
E.
Silva
,
J. Supercond.
20
,
71
(
2007
).
37.
S.
Donovan
,
O.
Klein
,
M.
Dressel
,
K.
Holczer
, and
G.
Grüner
,
Int. J. Infrared Millim. Waves
14
,
2459
(
1993
).
38.
M.
Göppl
,
A.
Fragner
,
M.
Baur
,
R.
Bianchetti
,
S.
Filipp
,
J. M.
Fink
,
P. J.
Leek
,
G.
Puebla
,
L.
Steffen
, and
A.
Wallraff
,
J. Appl. Phys.
104
,
113904
(
2008
).
39.
The lowest resonance can be compared to that of a cylindrical cavity with well-known resonance frequency for a TMmnp mode:41
$\omega _{mnp}\break = \frac{[c]}{\sqrt{\mu \epsilon }} \sqrt{\frac{x_{mn}^2}{R^2} + \frac{p^2\pi ^2}{d^2}}$
ωmnp=[c]μεxmn2R2+p2π2d2
Here, R is the radius and d the height of the cylindrical cavity, and xmn is the nth root of the Bessel function of order m. [c] stands for the velocity of light and μ and ε stand for the permeability and the permittivity. For a TM0n0 mode, i.e., p = 0, this frequency does not depend on d.
40.
J. D.
Jackson
,
Classical Electrodynamics
(
Wiley
,
New York
,
1962
), p.
254
.
41.
We find the same trend also for materials with higher permittivity, though with somewhat larger discrepancies between simulation and experiment.
You do not currently have access to this content.