Marco Fronzi

Dr. Marco Fronzi

School of Physics, The University of Sydney, Sydney, New South Wales, Australia
+1
orcid

Research Focus & Metrics

Academic Career Length

21Years (2006-Present)

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

Representative Publications

View All Publications
16 August 2017 in Nanoscale
Verified
Journal Article
Closed access
PDF file
Sherif Abdulkader TawfikSherif Abdulkader Tawfik
Sherif Abdulkader Tawfik
SASajid Ali
Sajid Ali
Marco FronziMarco Fronzi
Marco Fronzi
MKMehran Kianinia
Mehran Kianinia
TTToan Trong Tran
Toan Trong Tran
MFMichael J. Ford
Michael J. Ford
Hexagonal boron nitride (hBN) has recently emerged as a fascinating platform for room-temperature quantum photonics due to the discovery of robust visible light single-photon emitters. In order to utilize these emitters, it is necessary to have a clear understanding of their atomic structure and the associated excitation processes that give rise to this single photon emission. Here, we performed density-functional theory (DFT) and constrained DFT calculations for a range of hBN point defects in order to identify potential emission candidates. By applying a number of criteria on the electronic structure of the ground state and the atomic structure of the excited states of the considered defects, and then calculating the Huang–Rhys (HR) factor, we found that the CBVN defect, in which a carbon atom substitutes a boron atom and the opposite nitrogen atom is removed, is a potential emission source with a HR factor of 1.66, in good agreement with the experimental HR factor. We calculated the photoluminescence (PL) line shape for this defect and found that it reproduces a number of key features in the experimental PL lineshape.

15 August 2009 in Physical Chemistry Chemical Physics
Verified
Journal Article
Closed access
PDF file
Marco FronziMarco Fronzi
Marco Fronzi
SPSimone Piccinin
Simone Piccinin
BDBernard Delley
Bernard Delley
ETEnrico Traversa
Enrico Traversa
Catherine StampflCatherine Stampfl
Catherine Stampfl
We present a density functional theory investigation of the interaction between water and cerium oxide surfaces, considering both the stoichiometric and the reduced surfaces. We study the atomic structure and energetics of various configurations of water adsorption (for a water coverage of 0.25 ML) and account for the effect of temperature and pressure of the environment, containing both oxygen and water vapor, employing the ab initio atomistic thermodynamics approach. Through our investigation, we obtain the phase diagram of the water–ceria system, which enables us to discuss the stability of various surface structures as a function of the ambient conditions. For the stoichiometric surface, we find that the most stable configuration for water is when it is bonded at the cerium site, involving two O–H bonds of hydrogen and oxygen atoms at the surface. If oxygen vacancies are introduced at the surface, which is predicted under more reducing conditions, the binding energy of water is stronger, indicating an effective attractive interaction between water molecules and oxygen vacancies. Water dissociation, and the associated activation energies, are studied, and the role of oxygen vacancies is found to be crucial to stabilize the dissociated fragments. We present a detailed analysis of the stability of the water–ceria system as a function of the ambient conditions, and focus on two important surface processes: water adsorption/desorption on the stoichiometric surface and oxygen vacancy formation in the presence of water vapor. A study of the vibrational contribution to the free energy allows us to estimate the effect of this term on the stability range of adsorbed water.

2 February 2016 in Advanced Materials
Verified
Journal Article
Closed access
PDF file
MNMichael Nolan
Michael Nolan
AIAnna Iwaszuk
Anna Iwaszuk
ALAoife K. Lucid
Aoife K. Lucid
JCJohn J. Carey
John J. Carey
Marco FronziMarco Fronzi
Marco Fronzi

31 July 2019 in Journal of Materials Chemistry A
Verified
Journal Article
Closed access
PDF file
XXXi Xu
Xi Xu
HWHuiqiang Wang
Huiqiang Wang
Marco FronziMarco Fronzi
Marco Fronzi
XWXianfen Wang
Xianfen Wang
LBLei Bi
Lei Bi
ETEnrico Traversa
Enrico Traversa
A rational design of a high-performance cathode for proton-conducting solid oxide fuel cells (SOFCs) is proposed in this study with the aim of improving the hydration properties of conventional perovskite cathode materials, thus leading to the development of new materials with enhanced proton migration. Herein, potassium is used to dope traditional Ba0.5Sr0.5Co0.8Fe0.2O3−δ (BSCF), which is demonstrated to be a beneficial way for improving hydration, both experimentally and theoretically. The theoretical study was needed to overcome practical limits that hindered direct hydrogen mobility measurements. The novel material Ba0.4K0.1Sr0.5Co0.8Fe0.2O3−δ (BKSCF) shows a lower overall proton migration energy compared with that of the sample without K, suggesting that K-doping enhances proton conduction, which shows an improved performance by extending the catalytic sites to the whole cathode area. As a result, a fuel cell built with the novel BKSCF cathode shows an encouraging fuel cell performance of 441 and 1275 mW cm−2 at 600 and 700 °C, respectively, which is significantly higher than that of the cell using the pristine BSCF cathode. This study provides a new and rational way to design a perovskite cathode for proton-conducting SOFCs with high performance.

8 September 2009 in The Journal of Chemical Physics
Verified
Journal Article
Closed access
Marco FronziMarco Fronzi
Marco Fronzi
Aloysius SoonAloysius Soon
Aloysius Soon
BDBernard Delley
Bernard Delley
ETEnrico Traversa
Enrico Traversa
Catherine StampflCatherine Stampfl
Catherine Stampfl
We present density functional theory investigations of the bulk properties of cerium oxides (CeO2 and Ce2O3) and the three low index surfaces of CeO2, namely, (100), (110), and (111). For the surfaces, we consider various terminations including surface defects. Using the approach of “ab initio atomistic thermodynamics,” we find that the most stable surface structure considered is the stoichiometric (111) surface under “oxygen-rich” conditions, while for a more reducing environment, the same (111) surface, but with subsurface oxygen vacancies, is found to be the most stable one, and for a highly reducing environment, the (111) Ce-terminated surface becomes energetically favored. Interestingly, this latter surface exhibits a significant reconstruction in that it becomes oxygen terminated and the upper layers resemble the Ce2O3(0001) surface. This structure could represent a precursor to the phase transition of CeO2 to Ce2O3.

1 March 2021 in Journal of Power Sources
Verified
Journal Article
Closed access
XXXi Xu
Xi Xu
YXYangsen Xu
Yangsen Xu
JMJinming Ma
Jinming Ma
YYYanru Yin
Yanru Yin
Marco FronziMarco Fronzi
Marco Fronzi
LBLei Bi
Lei Bi