Nanocrystalline silicon, amorphous silicon, semiconductor nanowires

This has been a long standing project simulating nanocrystalline and amorphous silicon thin films. The objective of the research is to identify, explore, evaluate and model new heterogeneous thin film materials capable of making a breakthrough in the production of low cost electricity from sunlight. This project has been part of the NREL national thin film solar cell team effort.

Our approach has been to use molecular dynamics simulations using both classical and tight binding methods to obtain insight into mechanisms of metastability and the structure of nanocrystaline silicon.

Metastability

The Staebler-Wronski effect or the degradation of thin film silicon solar cells when they are placed in sunlight is a mystery that has plagued the research community for more than 20 years. When such solar cells are kept in sunlight their efficiency drops by 15-20% over a period of several days. Intensive studies have established that these changes are due to creating of mid-gap defect states from silicon dangling bonds in the amorphous silicon films.  From an annealed defect density of 1015 cm-3, the defect density rises to 1016-1017 cm-3 after light-soaking. The metastable changes are reversible and can be removed by annealing the material at 180-200 C. The metastable defects are indistinguishable from native dangling bond defects. Significantly the metastable defects are at least 4 Å distant from hydrogen sites- indicating an anti-correlation with H.

We proposed a new mechanism explaining many features of the Staebler-Wronski effect [1,2]. In the first step sunlight creates an excess density of electrons and holes. The electrons recombine with holes on weak silicon bonds in the material.  The recombination energy causes the weak silicon bonds to break, generating silicon dangling bond – floating bond pairs.  Accurate tight-binding molecular dynamics simulations have established the lowering oif energy barriers for bond-breaking when excited e-h pairs are present. During the second step, the floating bonds (over-coordinated silicon atoms) diffuse away from the dangling bonds and move freely throughout the material since they are a mobile species. In the third step the floating bonds recombine with themselves or with H in the network, and the network is left with primarily dangling bonds. An interesting caveat is that because of charge neutrality charged dangling bond defects are formed in addition to the neutral species. Many features of the Staebler-Wronski are explained well by this model (Phys. Rev. Lett. paper, book chapter). The model has been featured in news releases (Ames Lab Inquiry article, Hindu).

 

Weak Si bond (WB) breaking into a dangling bond (DB) and a floating bond  (FB) afer e-h recombination

 

 
 

 

 

 

 

 


Nanocrystalline silicon

Nanocrystalline silicon was simulated consisting of nanocrystallites embedded in an amorphous matrix. The presence of the nanocrystallite improves the ordering of the amorphous matrix which may account for the higher stability of nanocrystalline silicon towards light soaking. The nanoscale structure can inhibit the instability and breaking of weak bonds.

There is a thin disordered region around the nanocrystal containing an excess density of H where the H density is about twice the background H density. By performing simulations at various temperatures and monitoring the motion of H, we found that the excess grain boundary H is responsible for the anomalous low-temperature H evolution peak that occurs near 400C in addition to the high temperature H evolution peak at 600C.

 Powerpoint  presentation on nanocrystalline silicon

 

 

 


Semiconductor Nanowires

Present work is investigating the structure of semiconductor nanowires, including the structure and orientation of crystalline core nanowires. There are many similarities to microcrystalline silicon.

 

Faculty: Rana Biswas

Collaborators: Bicai Pan, Y. Ye

Students: Venkatesh Selvaraj

Funding: NREL, PRF(ACS)


Research Programs

MRC Homepage