2000
DOI: 10.1103/physrevb.61.15614
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Photoluminescence of InAs quantum dots inn-i-p-iGaAs superlattice

Abstract: Large blueshift and linewidth increase in photoluminescence ͑PL͒ spectra of InAs quantum dots ͑QD's͒ in n-i-p-i GaAs superlattice were observed. By increasing the excitation intensity from 0.5 to 32 W/cm 2 , the PL peak position blueshifted 18 meV, and the linewidth increased by 20 meV. Such large changes are due to the state-filling effects of the QD's resulted from the separation of photogenerated electrons and holes caused by the doping potential.The optical properties of InAs self-assembled quantum dots ͑Q… Show more

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Cited by 9 publications
(10 citation statements)
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“…In Table I we report the FWHM values of the ground state and the first excited state of ͑S1, S2, and S3͒ samples. 31 Similar behavior is observed by Kumagai et al 32 on InAs/ GaAs QDs with modulation doped ͑p-doped with beryllium͒, they explained the increase in FWHM by the interdiffusion of beryllium atoms from the GaAs to the QDs layer. In fact, when QDs are placed near the channel, they behave like doped-QDs, because doping atoms are supposed to introduce radiative recombination centers which will increase the FWHM.…”
Section: Resultssupporting
confidence: 77%
“…In Table I we report the FWHM values of the ground state and the first excited state of ͑S1, S2, and S3͒ samples. 31 Similar behavior is observed by Kumagai et al 32 on InAs/ GaAs QDs with modulation doped ͑p-doped with beryllium͒, they explained the increase in FWHM by the interdiffusion of beryllium atoms from the GaAs to the QDs layer. In fact, when QDs are placed near the channel, they behave like doped-QDs, because doping atoms are supposed to introduce radiative recombination centers which will increase the FWHM.…”
Section: Resultssupporting
confidence: 77%
“…In several works [14,19,49] that also investigated the finite temperature properties of nuclear matter, the entire interaction involves temperature dependence. However, similar to [3,5,6,18,50,16,9], in [20] the temperature effects were invoked through the kinetic part of the interaction which also successfully explained the finite temperature properties of nuclear matter at low density. In the present work I consider same approach with the same model as [20] to examine the thermal properties of nuclear matter more rigorously at different density domains.…”
Section: Introductionmentioning
confidence: 73%
“…It is therefore that one rely on theoretical modeling of proto-neutron star matter (PNSM) to understand its composition and compute the EoS on its basis. A lot of work has been done in this regard to comprehend successfully the temperature dependence of nuclear matter properties [3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23] using a wide variety of approaches. Based on microscopic treatments, two and three body nuclear potentials were constructed using chiral effective theory [24,25] to compute the nuclear matter properties at finite temperature while nuclear dipolar strength was successfully calculated by adopting finite-temperature relativistic time blocking approximation [26].…”
Section: Introductionmentioning
confidence: 99%
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