Abstract

An infrared detector using a photoeffect in mercury selenide is described which responds from the visible to 15 μ. Although the detector construction and sample geometry are similar to that employed in the photoelectromagnetic (PEM) effect, performance differs from that expected of the PEM effect. The spectral response for constant power input per unit wavelength interval peaks in the visible and is wavelength independent in the interval from 3 to 15 μ. The frequency response indicates a detector response time of 150 μsec. A thermal response mechanism is proposed.

© 1961 Optical Society of America

Full Article  |  PDF Article

References

  • View by:
  • |
  • |
  • |

  1. M. D. Blue and P. W. Kruse (to be published).
  2. P. W. Kruse, J. Appl. Phys. 30, 770 (1959); Electronics 33, 62 (1960).
    [Crossref]
  3. D*(500°K, f, 1), the detectivity, is a figure of merit relating the extrapolated signal-to-noise ratio in a 1 cps bandwidth centered at frequency f per watt of radiant flux from a 500°K blackbody for a detector of 1 cm2 area.
  4. I. I. Sochard and J. H. Becker, Bull. Am. Phys. Soc. 3, 114 (1958); Bull. Am. Phys. Soc. 4, 134 (1959); NBS Rept. No. 6437 (June, 1959); J. H. Becker, J. Appl. Phys. 31, 612 (1960).
    [Crossref]
  5. E. H. Putley, Proc. Phys. Soc. (London) B68, 35 (1955).
  6. W. W. Gärtner, Phys. Rev. 122, 419 (1961).
    [Crossref]
  7. P. J. Price, Phil. Mag. 46, 1252 (1955).

1961 (1)

W. W. Gärtner, Phys. Rev. 122, 419 (1961).
[Crossref]

1959 (1)

P. W. Kruse, J. Appl. Phys. 30, 770 (1959); Electronics 33, 62 (1960).
[Crossref]

1958 (1)

I. I. Sochard and J. H. Becker, Bull. Am. Phys. Soc. 3, 114 (1958); Bull. Am. Phys. Soc. 4, 134 (1959); NBS Rept. No. 6437 (June, 1959); J. H. Becker, J. Appl. Phys. 31, 612 (1960).
[Crossref]

1955 (2)

E. H. Putley, Proc. Phys. Soc. (London) B68, 35 (1955).

P. J. Price, Phil. Mag. 46, 1252 (1955).

Becker, J. H.

I. I. Sochard and J. H. Becker, Bull. Am. Phys. Soc. 3, 114 (1958); Bull. Am. Phys. Soc. 4, 134 (1959); NBS Rept. No. 6437 (June, 1959); J. H. Becker, J. Appl. Phys. 31, 612 (1960).
[Crossref]

Blue, M. D.

M. D. Blue and P. W. Kruse (to be published).

Gärtner, W. W.

W. W. Gärtner, Phys. Rev. 122, 419 (1961).
[Crossref]

Kruse, P. W.

P. W. Kruse, J. Appl. Phys. 30, 770 (1959); Electronics 33, 62 (1960).
[Crossref]

M. D. Blue and P. W. Kruse (to be published).

Price, P. J.

P. J. Price, Phil. Mag. 46, 1252 (1955).

Putley, E. H.

E. H. Putley, Proc. Phys. Soc. (London) B68, 35 (1955).

Sochard, I. I.

I. I. Sochard and J. H. Becker, Bull. Am. Phys. Soc. 3, 114 (1958); Bull. Am. Phys. Soc. 4, 134 (1959); NBS Rept. No. 6437 (June, 1959); J. H. Becker, J. Appl. Phys. 31, 612 (1960).
[Crossref]

Bull. Am. Phys. Soc. (1)

I. I. Sochard and J. H. Becker, Bull. Am. Phys. Soc. 3, 114 (1958); Bull. Am. Phys. Soc. 4, 134 (1959); NBS Rept. No. 6437 (June, 1959); J. H. Becker, J. Appl. Phys. 31, 612 (1960).
[Crossref]

J. Appl. Phys. (1)

P. W. Kruse, J. Appl. Phys. 30, 770 (1959); Electronics 33, 62 (1960).
[Crossref]

Phil. Mag. (1)

P. J. Price, Phil. Mag. 46, 1252 (1955).

Phys. Rev. (1)

W. W. Gärtner, Phys. Rev. 122, 419 (1961).
[Crossref]

Proc. Phys. Soc. (London) (1)

E. H. Putley, Proc. Phys. Soc. (London) B68, 35 (1955).

Other (2)

D*(500°K, f, 1), the detectivity, is a figure of merit relating the extrapolated signal-to-noise ratio in a 1 cps bandwidth centered at frequency f per watt of radiant flux from a 500°K blackbody for a detector of 1 cm2 area.

M. D. Blue and P. W. Kruse (to be published).

Cited By

OSA participates in Crossref's Cited-By Linking service. Citing articles from OSA journals and other participating publishers are listed here.

Alert me when this article is cited.


Figures (2)

Fig. 1
Fig. 1

Relative spectral response of HgSe detector 6A-223 for constant power input per unit wavelength interval.

Fig. 2
Fig. 2

Relative frequency response of HgSe detector 6A-223.