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Can I read Urbach–Martienssen's tails in layered semiconductor GaSe on EtoBox?

Urbach–Martienssen's tails in layered semiconductor GaSe by B. Abay; H.S. Güder; Y.K. Yoğurtçu is a Physics and Astronomy article available to read on EtoBox.

What is Urbach–Martienssen's tails in layered semiconductor GaSe about?

The dependence of the absorption coefficient on photon energy and temperature near the fundamental absorption edge was measured for layered single crystal, Gallium selenide (GaSe). The exponentially increasing absorption tail was explained as an Urbach-Martienssen's (U-M's) tails in the 10-340 K temperature range. Temperature dependence of the characteristic Urbach's parameters such as steepness parameter s(T) and Urbach's energy E U k B T=s indicate that absorption is predominantly influenced by the phonon-induced microelectric fields and not compositional or structural potential fluctuations. The evaluated effective phonon energy hn p 17 meV is in good agreement with the A H 1 1 homopolar phonon mode obtained from Raman spectra and infrared (IR) measurement for this compound. The absorption process can be considered as an internal Franz-Keldysh effect, caused by the phonon-generated microelectric fields related with charged impurities or defects associated with bulk two-dimensional stacking faults, interstitial atoms, or vacancies in the GaSe lattice and can be described in the framework of the Dow and Redfield (DR) theory.

Who reads Urbach–Martienssen's tails in layered semiconductor GaSe?

It is typically read by researchers, students, and practitioners in Physics and Astronomy.

Author
B. Abay; H.S. Güder; Y.K. Yoğurtçu
Publisher
Elsevier Science; Elsevier ; Elsevier BV (ISSN 0038-1098)
Published
1999
Language
EN
Field
Physics and Astronomy (Physical Sciences)

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