How much gallium do we need for a p-type Cu(In,Ga)Se2?

Documenti analoghi

• The impact of Kelvin probe force microscopy operation modes and environment on grain boundary band bending in perovskite and Cu(In,Ga)Se2 solar cells
  di: Lanzoni, Evandro Martin, et al.
  Pubblicazione: (2021)
• CuIn(Se,Te)2 absorbers with bandgaps < 1 eV for bottom cells in tandem applications
  di: Weiss, Thomas Paul, et al.
  Pubblicazione: (2023)
• Improved sequentially processed Cu(In,Ga)(S,Se)2 by Ag alloying
  di: Prot, Aubin JC. M., et al.
  Pubblicazione: (2024)
• On the origin of tail states and VOC losses in Cu(In,Ga)Se2
  di: Ramírez, Omar, et al.
  Pubblicazione: (2022)
• Improved Sequentially Processed Cu(In,Ga)(S,Se)2 by Ag Alloying
  di: Aubin Jean‐Claude Mireille Prot, et al.
  Pubblicazione: (2024)