We present a detailed experimental study of the direct detection effect in a small volume (0.15μm×1μm×3.5nm) quasioptical NbN phonon cooled hot electron bolometer mixer at 673GHz. We find that the small signal noise temperature, relevant for an astronomical observation, is 20% lower than the noise temperature obtained using 300 and 77K calibration loads. In a separate set of experiments we show that the direct detection effect is caused by a combination of bias current reduction when switching from the 77 to the 300K load in combination with the bias current dependence of the receiver gain. The bias current dependence of the receiver gain is shown to be mainly caused by the current dependence of the mixer gain.

1.
E. M.
Gershenzon
,
G. N.
Gol’tsman
,
I. G.
Gogidze
,
A. I.
Eliantev
,
B. S.
Karasik
, and
A. D.
Semenov
, Sverkhprovodimost (KIAE) 3(10),
2143
(
1990
); 
E. M.
Gershenzon
,
G. N.
Gol’tsman
,
I. G.
Gogidze
,
A. I.
Eliantev
,
B. S.
Karasik
, and
A. D.
Semenov
,Superconductivity 3,
1582
(
1991
).
2.
D. E.
Prober
,
Appl. Phys. Lett.
62
,
2119
(
1993
).
3.
D. P.
Marrone
,
R.
Blundell
,
E.
Tong
,
S. N.
Paine
,
D.
Loudkov
,
J. H.
Kawamura
,
D.
Lühr
, and
C.
Barrientos
, in
Proceedings of the 16th International Symposium on Space THz Technology
, edited by
M.
Yngvarson
,
J.
Stake
, and
H.
Merkel
(
Chalmers University of Technology
,
Chalmers, Sweden
,
2005
), p.
64
.
6.
G.
Chattopadhyay
,
E.
Schlecht
,
J.
Ward
,
J.
Gill
,
H.
Javadi
,
F.
Maiwald
, and
I.
Mehdi
,
IEEE Trans. Microwave Theory Tech.
52
,
1538
(
2004
).
7.
M.
Hajenius
,
J. J. A.
Baselmans
,
A.
Baryshev
,
J. R.
Gao
,
T. M.
Klapwijk
,
J. W.
Kooi
,
W.
Jellema
, and
Z. Q.
Yang
,
J. Appl. Phys.
(in press).
8.
A. R.
Kerr
,
IEEE Trans. Microwave Theory Tech.
3.1
,
325
(
1999
).
9.
S.
Svechnokov
,
A.
Verevkin
,
B.
Voronov
,
E.
Menschikov
,
E.
Gershenzon
, and
G.
Gol’tsman
, in
Proceedings of the 9th International Symposium On Space THz Technology
, edited by
R.
McGrath
(
University of Virginia
,
Charlottesville
,
1993
), p.
45
.
10.
J.
Kawamura
,
C.-Y.
Edward Tong
,
R.
Blundell
,
D.
Cosmo Papa
,
T. R.
Hunter
,
F.
Patt
,
G.
Gol’tsman
, and
E.
Gershenzon
,
IEEE Trans. Appl. Supercond.
11
,
952
(
2001
).
11.
A. D.
Semenov
 et al., in
Proceedings of the 13th International Symposium On Space THz Technology
, edited by
R.
Blundell
and
E.
Tong
(
Harvard University
,
Cambridge, MA
,
2002
), p.
229
.
12.
Yu. B.
Vachtomin
 et al., in
Proceedings of the 15th International Symposium On Space THz Technology
, edited by
G.
Narayanan
(
University of Massachusetts
,
Boston, MA
,
2000
), p.
236
.
13.
J. J. A.
Baselmans
 et al.,
Appl. Phys. Lett.
86
,
163503
(
2005
).
14.

The data is taken at the optimally pumped IV curve of the device discussed in Ref. 13.

15.

Note that the current bias of the mixer in the presence of the direct detection effect is determined by the LO power and the load temperature. The usual approach that G and TN are a function of LO power alone is no longer valid. Hence in the presence of the direct detection effectG=G(V,I)=G(V,[PLO,Tload]) and TN=TN(V,[PLO,Tload]). This also implies that the definition of the Y factor is strictly speaking invalid in the presence of a direct detection effect since the Y factor definition requires that Ghot=Gcold. Hence only the small signal Y factor is a correct parameter, and the normal, conventional Y factor is not. This is due to the bias current change associated with the direct detection effect, which results in GhotGcold because IhotIcold and G depends on the bias current (which is a combination of LO power and load temperature). This is, however, a small effect that is ignored in the paper.

16.
H. F.
Merkel
,
P.
Khosropanah
,
D.
Wilms-Floet
,
P. A.
Yagoubov
, and
E.
Kollberg
,
IEEE Trans. Microwave Theory Tech.
48
,
690
(
2000
).
17.

We use a low frequency mixer to be able to use a LO and a signal source, since 2THz sources were not available.

18.
H.
Ekström
,
B. S.
Karasik
,
E. L.
Kollberg
, and
K. S.
Yngvesson
,
IEEE Trans. Microwave Theory Tech.
43
,
938
(
1995
).
19.

The relation T=1R relies on the assumption that the characteristic impedance of the directional coupler is identical to the impedance of the isolator in front of the amplifier. Hence the use of an isolator is crucial in this experiment, since the input match of a typical low noise amplifier can in general not be described by a 50Ω real impedance.

20.

The bias current as shown in Figs. 3–6 is given by Ihot, which is chosen arbitrarily. Note however that IDDIhot, so using Icold in stead of Ihot would not change the graphs appreciably.

21.
J. W.
Kooi
,
J. J. A.
Baselmans
,
J. R.
Gao
,
T. M.
Klapwijk
,
P.
Dieleman
,
A.
Baryshev
,
M.
Hajenius
, and
G.
de Lange
(submitted).
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