Philippe PARENT

Dr. Philippe PARENT

orcid

Research Focus & Metrics

Academic Career Length

35Years (1992-Present)

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

Representative Publications

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1 November 2016 in Journal of Aerosol Science
Verified
Journal Article
Closed access
ABA. Bescond
A. Bescond
JYJ. Yon
J. Yon
FOF.-X. Ouf
F.-X. Ouf
CRC. Rozé
C. Rozé
ACA. Coppalle
A. Coppalle
CLC. Laffon
C. Laffon

25 August 2016 in ACS Applied Materials & Interfaces
Verified
Journal Article
Closed access
IMIevgen Mazurenko
Ievgen Mazurenko
KMKaren Monsalve
Karen Monsalve
JRJad Rouhana
Jad Rouhana
PPPhilippe PARENT
Philippe PARENT
CLCarine Laffon
Carine Laffon
ELElisabeth Lojou
Elisabeth Lojou

1 July 2002 in Topics in Catalysis
Verified
Journal Article
Closed access
PDF file
LGL. Guczi
L. Guczi
DBD. Bazin
D. Bazin
Imre KovácsImre Kovács
Imre Kovács
LBL. Borkó
L. Borkó
ZSZ. Schay
Z. Schay
ISI. Sajó
I. Sajó

1 June 1998 in Physical Review B
Verified
Journal Article
Closed access
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LFL. Fayette
L. Fayette
BMB. Marcus
B. Marcus
MMM. Mermoux
M. Mermoux
GTG. Tourillon
G. Tourillon
KLK. Laffon
K. Laffon
FNF. Le Normand
F. Le Normand
We investigated the structural changes of carbon in diamond films deposited by microwave plasma-assisted chemical vapor deposition with various methane concentrations and substrate temperatures. They were studied by x-ray-absorption near-edge structure (XANES) at the C K edge. The results on composition and structure were compared to those given by Raman spectra, x-ray-diffraction patterns, and scanning electron microscopy. Unlike Raman spectroscopy, XANES at the C K edge is nearly equally sensitive whatever the nature of the carbon (diamond, graphite, amorphous,…) involved in these deposits. At T<950°C and [CH4]<2%, the C K edge spectra and the diffraction measurements both show that the films mainly consist of diamond, despite strong morphological modifications of the films. They all display the diamond characteristics. However a small amount of amorphous component (≅10%) is incorporated, while increasing the methane concentration and/or the substrate temperature. The presence of this amorphous carbon induces a drastic change in the Raman spectra with the appearance of new lines. At substrate temperatures higher than 900 °C and methane concentrations equal to 2%, a second characteristic modification of the Raman spectra then stems from the presence of a disordered graphitic phase. These amorphous and graphitic components exhibit quite characteristic Raman and XANES spectra. The nature of these amorphous and graphitic phases included into the diamond films is discussed.

12 April 2012 in The Astrophysical Journal Letters
Verified
Journal Article
Closed access
ECEmanuele Congiu
Emanuele Congiu
GFGleb Fedoseev
Gleb Fedoseev
SISergio Ioppolo
Sergio Ioppolo
FDFrançois Dulieu
François Dulieu
HCHenda Chaabouni
Henda Chaabouni
HLHarold Linnartz
Harold Linnartz