2002
DOI: 10.1002/1521-3951(200211)234:1<155::aid-pssb155>3.0.co;2-r
|View full text |Cite
|
Sign up to set email alerts
|

Light Propagation- and Many-particle-induced Non-Lorentzian Lineshapes in Semiconductor Nanooptics

Abstract: Dedicated to Professor Dr. Roland Zimmermann on the occasion of his 60th birthdayThe occurrence of non-Lorentzian lineshapes is analyzed for a variety of nanooptical semiconductor systems such as quantum wells and quantum dots. Their origin is traced back to light-matter interaction (light propagation) and many-particle correlations (electron-electron and electronphonon interaction). 157

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1

Citation Types

0
9
0

Year Published

2003
2003
2018
2018

Publication Types

Select...
8
1

Relationship

2
7

Authors

Journals

citations
Cited by 27 publications
(9 citation statements)
references
References 31 publications
(39 reference statements)
0
9
0
Order By: Relevance
“…12,13 The decay time of this superradiant response inversely scales with the QW number N. The reflection from MQW Bragg structures is characterized by a Lorentzian line which grows in peak reflectivity and linewidth with increasing N. 14 In the limit of large N, the reflectivity reaches unity and a square profile characteristic for the reflection of a photonic band gap is formed. 15 Time-resolved reflection experiments and microscopic calculations have shown enhanced emission along with accelerated decay of the coherent optical polarization. 16 At higher excitation intensities, the radiative coupling gradually disappeared, which was attributed to excitation-induced dephasing due to carriercarrier interaction in the individual QWs.…”
Section: Introductionmentioning
confidence: 99%
“…12,13 The decay time of this superradiant response inversely scales with the QW number N. The reflection from MQW Bragg structures is characterized by a Lorentzian line which grows in peak reflectivity and linewidth with increasing N. 14 In the limit of large N, the reflectivity reaches unity and a square profile characteristic for the reflection of a photonic band gap is formed. 15 Time-resolved reflection experiments and microscopic calculations have shown enhanced emission along with accelerated decay of the coherent optical polarization. 16 At higher excitation intensities, the radiative coupling gradually disappeared, which was attributed to excitation-induced dephasing due to carriercarrier interaction in the individual QWs.…”
Section: Introductionmentioning
confidence: 99%
“…Contrary to light emission in Figure , the high-energy side of the excitonic resonance is more pronounced in absorption. This is because the phonon creation processes appear at higher energies in absorption . For the light emission spectra, this broadening appears on the low-energy side, because of its photon-emission character (see Supporting Information Figure S4).…”
mentioning
confidence: 99%
“…We find a polaron red-shift of approximately 29 meV with respect to the unshifted exciton main line (gray). Furthermore, the spectrum exhibits asymmetric phonon sidebands, in particular at the high-energy side of the main resonance [30][31][32] . Subtracting the homogeneous linewidth shows that we observe multiple sidebands above the main resonance originating from emission and absorption of acoustic and optical phonons, inset: Fig.…”
mentioning
confidence: 99%