Ultrafast Optics Used to Study Carrier Dynamics of High Quality Silicon on Glass Sample

2010 ◽  
Author(s):  
O.S Magaña-Loaiza ◽  
R. Sobolewski ◽  
J.J Sanchez Mondragon ◽  
C. Kosik-Williams ◽  
J. Zhang.
Keyword(s):  
Glass Sample ◽  
Ultrafast Optics ◽  
Carrier Dynamics ◽  
High Quality

Ultrafast Optics Used to Generate and Detect Longitudinal Acoustic Phonons in High Quality Silicon on Glass Sample

2010 ◽  
Author(s):  
O. S Magaña-Loaiza ◽  
R. Sobolewski ◽  
J. J Sánchez-Mondragón ◽  
J. Zhang ◽  
C. Kosik-Williams ◽  
...  
Keyword(s):  
Glass Sample ◽  
Ultrafast Optics ◽  
Acoustic Phonons ◽  
High Quality ◽  
Longitudinal Acoustic

Experimental Ultrafast Spectroscopy Used to Study Carrier Dynamics of High Quality Silicon on Glass Sample.

2010 ◽  
Author(s):  
Omar S. Magaña-Loaiza ◽  
Roman Sobolewski ◽  
Javier J. Sanchez-Mondragon ◽  
Carlo Kosik-Williams ◽  
Jie Zhang
Keyword(s):  
Glass Sample ◽  
Ultrafast Spectroscopy ◽  
Carrier Dynamics ◽  
High Quality

Comparison of carrier dynamics in high quality 1D/0D GaAs/AlGaAs structures

1994 ◽  
Vol 23 (1-4) ◽  
pp. 433-436
Author(s):  
F. Adler ◽  
M. Burkard ◽  
F.E. Prins ◽  
G. Lehr ◽  
H. Schweizer ◽  
...  
Keyword(s):  
Carrier Dynamics ◽  
High Quality

Vapor growth and interfacial carrier dynamics of high-quality CdS-CdSSe-CdS axial nanowire heterostructures

Nano Energy ◽  
2017 ◽  
Vol 32 ◽  
pp. 28-35 ◽  
Author(s):  
Qinglin Zhang ◽  
Huawei Liu ◽  
Pengfei Guo ◽  
Dan Li ◽  
Peng Fan ◽  
...  
Keyword(s):  
Carrier Dynamics ◽  
High Quality ◽  
Vapor Growth ◽  
Nanowire Heterostructures

Intrinsic charge carrier dynamics and device stability of perovskite/ZnO mesostructured solar cells in moisture

2016 ◽  
Vol 4 (15) ◽  
pp. 5474-5481 ◽  
Author(s):  
Yan Lei ◽  
Longyan Gu ◽  
Weiwei He ◽  
Zuxiao Jia ◽  
Xiaogang Yang ◽  
...  
Keyword(s):  
Solar Cells ◽  
Charge Carrier ◽  
Carrier Dynamics ◽  
High Quality ◽  
Charge Carrier Dynamics ◽  
Device Stability

High quality CH3NH3PbI3/PbI2/ZnO p–i–n junction solar cells fabricated in moisture maintained more than 72% of their initial PCE after 250 days storage.

Analysis of traps in high quality CVD diamond films through the temperature dependence of carrier dynamics

2003 ◽  
Vol 12 (10-11) ◽  
pp. 1733-1737 ◽  
Author(s):  
Marco Marinelli ◽  
E Milani ◽  
A Paoletti ◽  
G Pucella ◽  
A Tucciarone ◽  
...  
Keyword(s):  
Temperature Dependence ◽  
Diamond Films ◽  
Cvd Diamond ◽  
Carrier Dynamics ◽  
High Quality

Ultrafast Spectroscopy Used to Generate and Detect Longitudinal Acoustic Phonons in High Quality Silicon on Glass Sample

2010 ◽  
Author(s):  
Omar S. Magaña-Loaiza ◽  
Roman Sobolewski ◽  
Adalberto Alejo-Molina ◽  
Jie Zhang ◽  
Carlo Kosik-Williams ◽  
...  
Keyword(s):  
Glass Sample ◽  
Ultrafast Spectroscopy ◽  
Acoustic Phonons ◽  
High Quality ◽  
Longitudinal Acoustic

Influence of Preparation Conditions on Charge Carrier Dynamics In a-Si:H Determined By An In-Siju Technique

1986 ◽  
Vol 70 ◽  
Author(s):  
A. Werner ◽  
M. Kunst
Keyword(s):  
Thin Films ◽  
Hydrogenated Amorphous Silicon ◽  
Carrier Dynamics ◽  
Discharge Process ◽  
High Quality ◽  
Time Resolved ◽  
Preparation Conditions ◽  
Charge Carrier Dynamics ◽  
Hydrogenated Amorphous

ABSTRACTContactless photoconductivity measurements with the time-resolved microwave conductivity technique have been performed during the growth of hydrogenated amorphous silicon films. it has been shown that low substrate temperature and thin films lead to a larger electron decay rate and to an increased infrared absorption compared with high quality films. Addition of H2S to SiH4 during the glow discharge process leads to a worse fi1m quality which can be detected in-situ.

Some problems of objective-prism spectra classification

1966 ◽  
Vol 24 ◽  
pp. 51-52
Author(s):  
E. K. Kharadze ◽  
R. A. Bartaya
Keyword(s):  
Short Wave ◽  
High Quality ◽  
Stellar Spectra ◽  
Objective Prism

The unique 70-cm meniscus-type telescope of the Abastumani Astrophysical Observatory supplied with two objective prisms and the seeing conditions characteristic at Mount Kanobili (Abastumani) permit us to obtain stellar spectra of a high quality. No additional design to improve the “climate” immediately around the telescope itself is being applied. The dispersions and photographic magnitude limits are 160 and 660Å/mm, and 12–13, respectively. The short-wave end of spectra reaches 3500–3400Å.

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