Kengo Hamada

Dr. Kengo Hamada

Kanagawa Institute of Industrial Science and Technology (KISTEC), Ebina, Japan
orcid

Research Focus & Metrics

Academic Career Length

9Years (2018-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

View All Publications
1 August 2020 in Nano Energy
Verified
Journal Article
Closed access
KNKohei Nishimura
Kohei Nishimura
MKMuhammad Akmal Kamarudin
Muhammad Akmal Kamarudin
DHDaisuke Hirotani
Daisuke Hirotani
Kengo HamadaKengo Hamada
Kengo Hamada
QSQing Shen
Qing Shen
SHShuzi Hayase
Shuzi Hayase

18 August 2019 in The Journal of Physical Chemistry Letters
Verified
Journal Article
Closed access
MKMuhammad Akmal Kamarudin
Muhammad Akmal Kamarudin
DHDaisuke Hirotani
Daisuke Hirotani
ZWZhen Wang
Zhen Wang
Kengo HamadaKengo Hamada
Kengo Hamada
KNKohei Nishimura
Kohei Nishimura
SHShuzi Hayase
Shuzi Hayase

17 July 2019 in ACS Energy Letters
Verified
Journal Article
Closed access
GKGaurav Kapil
Gaurav Kapil
TBTakeru Bessho
Takeru Bessho
CNChi Huey Ng
Chi Huey Ng
Kengo HamadaKengo Hamada
Kengo Hamada
MPManish Pandey
Manish Pandey
SHShuzi Hayase
Shuzi Hayase

1 April 2019 in Nano Energy
Verified
Journal Article
Closed access
CNChi Huey Ng
Chi Huey Ng
KNKohei Nishimura
Kohei Nishimura
NINozomi Ito
Nozomi Ito
Kengo HamadaKengo Hamada
Kengo Hamada
DHDaisuke Hirotani
Daisuke Hirotani
SHShuzi Hayase
Shuzi Hayase

27 April 2018 in Nano Letters
Verified
Journal Article
Closed access
GKGaurav Kapil
Gaurav Kapil
TRTERESA RIPOLLES-SANCHIS
TERESA RIPOLLES-SANCHIS
Kengo HamadaKengo Hamada
Kengo Hamada
YOYuhei Ogomi
Yuhei Ogomi
TBTakeru Bessho
Takeru Bessho
SHShuzi Hayase
Shuzi Hayase

6 February 2018 in Scientific Reports
Verified
Journal Article
Open access
PDF file
CNChi Huey Ng
Chi Huey Ng
TRTERESA RIPOLLES-SANCHIS
TERESA RIPOLLES-SANCHIS
Kengo HamadaKengo Hamada
Kengo Hamada
Siow Hwa TeoSiow Hwa Teo
Siow Hwa Teo
HLHong Ngee Lim
Hong Ngee Lim
SHShuzi Hayase
Shuzi Hayase
Perovskite solar cells based on series of inorganic cesium lead bromide and iodide mixture, CsPbBr3-xI x , where x varies between 0, 0.1, 0.2, and 0.3 molar ratio were synthesized by two step-sequential deposition at ambient condition to design the variations of wide band gap light absorbers. A device with high overall photoconversion efficiency of 3.98 % was obtained when small amount of iodide (CsPbBr2.9I0.1) was used as the perovskite and spiro-OMeTAD as the hole transport material (HTM). We investigated the origin of variation in open circuit voltage, Voc which was shown to be mainly dependent on two factors, which are the band gap of the perovskite and the work function of the HTM. An increment in Voc was observed for the device with larger perovskite band gap, while keeping the electron and hole extraction contacts the same. Besides, the usage of bilayer P3HT/MoO3 with deeper HOMO level as HTM instead of spiro-OMeTAD, thus increased the Voc from 1.16 V to 1.3 V for CsPbBr3 solar cell, although the photocurrent is lowered due to charge extraction issues. The stability studies confirmed that the addition of small amount of iodide into the CsPbBr3 is necessarily to stabilize the cell performance over time.