AbstractAl2O3 rear surface passivated ultra-thin Cu(In,Ga)Se2 (CIGS) solar cells with Mo nano-particles (NPs) as local rear contacts are developed to demonstrate their potential to improve optical confinement in ultra-thin CIGS solar cells. The CIGS absorber layer is 380nm thick and the Mo NPs are deposited uniformly by an up-scalable technique and have typical diameters of 150 to 200nm. The Al2O3 layer passivates the CIGS rear surface between the Mo NPs, while the rear CIGS interface in contact with the Mo NP is passivated by [Ga]/([Ga]+[In]) (GGI) grading. It is shown that photon scattering due to the Mo NP contributes to an absolute increase in short circuit current density of 3.4mA/cm2; as compared to equivalent CIGS solar cells with a ...
An innovative rear contacting structure for copper indium gallium (di) selenide (CIGS) thin-film sol...
Recently, Cu(In,Ga)Se 2 (CIGS) solar cells have achieved 21% world-record efficiency, partly due to ...
Having an absorber layer thickness below 1 micrometre for a regular copper indium gallium di-selenid...
Al2O3 rear surface passivated ultra-thin Cu(In,Ga)Se2 (CIGS) solar cells with Mo nano-particles (NP)...
AbstractAl2O3 rear surface passivated ultra-thin Cu(In,Ga)Se2 (CIGS) solar cells with Mo nano-partic...
Al2O3 rear surface passivated ultra-thin Cu(In,Ga)Se2 (CIGS) solar cellswithMo nano-particles (NPs) ...
AbstractFor the first time, a novel rear contacting structure for copper indium gallium (di)selenide...
Reducing absorber layer thickness below 500 nm in regular Cu(In,Ga)Se2 (CIGS) solar cells decreases ...
Reducing absorber layer thickness below 500 nm in regular Cu(In,Ga)Se2 (CIGS) solar cells decreases ...
Reducing absorber layer thickness below 500 nm in regular Cu(In,Ga)Se2 (CIGS) solar cells decreases ...
Reducing the absorber layer thickness below 1 μm for a regular copper indium gallium di-selenide (CI...
Reducing the absorber layer thickness below 1 μm for a regular copper indium gallium di-selenide (CI...
An innovative rear contacting structure for copper indium gallium (di) selenide (CIGS) thin-film sol...
An innovative rear contacting structure for copper indium gallium (di) selenide (CIGS) thin-film sol...
The material supply to build renewable energy conversion systems needs to be considered from both a ...
An innovative rear contacting structure for copper indium gallium (di) selenide (CIGS) thin-film sol...
Recently, Cu(In,Ga)Se 2 (CIGS) solar cells have achieved 21% world-record efficiency, partly due to ...
Having an absorber layer thickness below 1 micrometre for a regular copper indium gallium di-selenid...
Al2O3 rear surface passivated ultra-thin Cu(In,Ga)Se2 (CIGS) solar cells with Mo nano-particles (NP)...
AbstractAl2O3 rear surface passivated ultra-thin Cu(In,Ga)Se2 (CIGS) solar cells with Mo nano-partic...
Al2O3 rear surface passivated ultra-thin Cu(In,Ga)Se2 (CIGS) solar cellswithMo nano-particles (NPs) ...
AbstractFor the first time, a novel rear contacting structure for copper indium gallium (di)selenide...
Reducing absorber layer thickness below 500 nm in regular Cu(In,Ga)Se2 (CIGS) solar cells decreases ...
Reducing absorber layer thickness below 500 nm in regular Cu(In,Ga)Se2 (CIGS) solar cells decreases ...
Reducing absorber layer thickness below 500 nm in regular Cu(In,Ga)Se2 (CIGS) solar cells decreases ...
Reducing the absorber layer thickness below 1 μm for a regular copper indium gallium di-selenide (CI...
Reducing the absorber layer thickness below 1 μm for a regular copper indium gallium di-selenide (CI...
An innovative rear contacting structure for copper indium gallium (di) selenide (CIGS) thin-film sol...
An innovative rear contacting structure for copper indium gallium (di) selenide (CIGS) thin-film sol...
The material supply to build renewable energy conversion systems needs to be considered from both a ...
An innovative rear contacting structure for copper indium gallium (di) selenide (CIGS) thin-film sol...
Recently, Cu(In,Ga)Se 2 (CIGS) solar cells have achieved 21% world-record efficiency, partly due to ...
Having an absorber layer thickness below 1 micrometre for a regular copper indium gallium di-selenid...