TY - JOUR
T1 - No extraordinary χ(3) in lead-halide perovskites
T2 - Placing an upper bound on Kerr nonlinearity by means of time-resolved interferometry
AU - Lorenc, Dusan
AU - Zhumekenov, Ayan
AU - Bakr, Osman M.
AU - Alpichshev, Zhanybek
N1 - Publisher Copyright:
© 2024 American Physical Society.
PY - 2024/8
Y1 - 2024/8
N2 - Lead halide perovskites have recently been reported to demonstrate an exceptionally high nonlinear (Kerr) refractive index n2 of up to 10-8cm2/W in CH3NH3PbBr3. Other researchers, however, observe different, substantially more conservative numbers. In order to resolve this disagreement, the nonlinear Kerr index of a bulk sample of lead halide perovskite was measured directly by means of an interferometer. This approach has many advantages as compared to the more standard z-scan technique. In particular, this method allows studying the induced changes to the refractive index in a time-resolved manner, thus enabling to separate the different contributions to n2. The extracted n2 values for CsPbBr3 and MAPbBr3 at λ≈1μm are n2=+2.1×10-14cm2/W and n2=+6×10-15cm2/W, respectively. Hence, these values are substantially lower than what has been indicated in most of the previous reports, implying the latter one should be regarded with great care.
AB - Lead halide perovskites have recently been reported to demonstrate an exceptionally high nonlinear (Kerr) refractive index n2 of up to 10-8cm2/W in CH3NH3PbBr3. Other researchers, however, observe different, substantially more conservative numbers. In order to resolve this disagreement, the nonlinear Kerr index of a bulk sample of lead halide perovskite was measured directly by means of an interferometer. This approach has many advantages as compared to the more standard z-scan technique. In particular, this method allows studying the induced changes to the refractive index in a time-resolved manner, thus enabling to separate the different contributions to n2. The extracted n2 values for CsPbBr3 and MAPbBr3 at λ≈1μm are n2=+2.1×10-14cm2/W and n2=+6×10-15cm2/W, respectively. Hence, these values are substantially lower than what has been indicated in most of the previous reports, implying the latter one should be regarded with great care.
UR - http://www.scopus.com/inward/record.url?scp=85202295476&partnerID=8YFLogxK
U2 - 10.1103/PhysRevMaterials.8.085403
DO - 10.1103/PhysRevMaterials.8.085403
M3 - Article
AN - SCOPUS:85202295476
SN - 2475-9953
VL - 8
JO - Physical Review Materials
JF - Physical Review Materials
IS - 8
M1 - 085403
ER -