2004
DOI: 10.1063/1.1795980
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Terahertz emission from p-lnAs due to the instantaneous polarization

Abstract: Terahertz radiation from differently doped n- and p-type InAs crystal surfaces was investigated by time-resolved measurement. Large increase of the emitted terahertz power has been observed for p-InAs samples with the p-doping levels of approximately 1016–1017cm−3. This increase was explained by a large surface depletion layer and an electric-field-induced optical rectification effect in this layer.

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Cited by 87 publications
(67 citation statements)
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“…2 is possibly due to a minor contribution from bulk optical rectification, although it is not possible to completely rule out other nonlinear processes-such as electric-field-induced optical rectification or surface nonlinear optical response-without further experimental evidence. 12,18 The dependence of the THz power on the temperature has been measured over the range 20-300 K. The results are shown in Fig. 4, normalized to a power of 1 at 300 K. In contrast to undoped, residual n-type ͑100͒ InAs, for which a maximum in power is observed at ϳ170 K, 9 but in agreement with data for undoped ͑111͒ InSb, 10,11 our data show a steady decrease in power with temperature.…”
supporting
confidence: 76%
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“…2 is possibly due to a minor contribution from bulk optical rectification, although it is not possible to completely rule out other nonlinear processes-such as electric-field-induced optical rectification or surface nonlinear optical response-without further experimental evidence. 12,18 The dependence of the THz power on the temperature has been measured over the range 20-300 K. The results are shown in Fig. 4, normalized to a power of 1 at 300 K. In contrast to undoped, residual n-type ͑100͒ InAs, for which a maximum in power is observed at ϳ170 K, 9 but in agreement with data for undoped ͑111͒ InSb, 10,11 our data show a steady decrease in power with temperature.…”
supporting
confidence: 76%
“…As expected from the equations governing the optical rectification, 17 the cos 2 dependence is consistent with optical rectification for ͑100͒ orientation, just as a cos 3 dependence has been noted for ͑111͒ orientation. 12 A cos 2 dependence has been observed previously for ͑100͒ orientation in, for example, n-type InAs ͑Ref. 18͒ and n-type InSb.…”
mentioning
confidence: 56%
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“…New experimental facts emerged after discovery [150] that a p-type InAs is a better THz emitter than an n-type InAs. This fact was explained in [150] as a consequence of the EFIOR effect induced by the surface field in the p-InAs.…”
Section: Inas and Other Narrow-gap Semiconductorsmentioning
confidence: 99%