The core photoluminescence emission of MOVPE-grown GaAs-Al0.33Ga0.67As core-shell nanowires is studied as function of the relevant geometrical parameter of these nanostructures, namely the shell-thickness to core-radius ratio h(s)/R-c. The energy of the dominant emission peak was compared with values of the GaAs heavy- and light-hole excitons redshifted by a uniaxial tensile strain, the latter calculated assuming perfect coherence at the core/shell interface and elastic energy equilibrium within the nanowires. Good agreement is obtained for h(s)/R-c < 1, the intrinsic strain-free excitonic emission being identified at 1.510 eV, and further ascribed to bound heavy-hole excitons. For h(s)/R-c > 1 increasingly larger redshifts (up to similar to 9 meV in excess of values calculated based on our elastic strain model) are observed, and tentatively ascribed to shell-dependent exciton localization effects. [GRAPHICS] Experimental and calculated bound exciton peak energies for GaAs-Al0.33Ga0.67As core-shell nanowires as function of their shell-thickness to core-radius ratio h(s)/R-c.
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James Madison Univ, Dept Phys & Astron, Harrisonburg, VA 22807 USAJames Madison Univ, Dept Phys & Astron, Harrisonburg, VA 22807 USA
Kaveh, M.
Gao, Q.
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Australian Natl Univ, Dept Elect Mat Engn, Res Sch Phys & Engn, Canberra, ACT 2601, AustraliaJames Madison Univ, Dept Phys & Astron, Harrisonburg, VA 22807 USA
Gao, Q.
Jagadish, C.
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Australian Natl Univ, Dept Elect Mat Engn, Res Sch Phys & Engn, Canberra, ACT 2601, AustraliaJames Madison Univ, Dept Phys & Astron, Harrisonburg, VA 22807 USA
Jagadish, C.
Ge, J.
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Univ Tennessee, Dept Mat Sci & Engn, Knoxville, TN 37996 USAJames Madison Univ, Dept Phys & Astron, Harrisonburg, VA 22807 USA
Ge, J.
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Duscher, G.
Wagner, H. P.
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Univ Cincinnati, Dept Phys, Cincinnati, OH 45220 USAJames Madison Univ, Dept Phys & Astron, Harrisonburg, VA 22807 USA