Mirko Prato

Dr. Mirko Prato

orcid

Research Focus & Metrics

Academic Career Length

23Years (2004-Present)

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

Representative Publications

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21 September 2010 in Classical and Quantum Gravity
Verified
Journal Article
Closed access
MPM Punturo
M Punturo
MAM Abernathy
M Abernathy
FAF Acernese
F Acernese
BAB Allen
B Allen
NANils Andersson
Nils Andersson
KYK Yamamoto
K Yamamoto

27 July 2015 in Journal of the American Chemical Society
Verified
Journal Article
Open access
QAQuinten A. Akkerman
Quinten A. Akkerman
VDValerio D’iNnocenzo
Valerio D’iNnocenzo
SASara Accornero
Sara Accornero
ASAlice Scarpellini
Alice Scarpellini
APAnnamaria Petrozza
Annamaria Petrozza
LMLiberato Manna
Liberato Manna
We demonstrate that, via controlled anion exchange reactions using a range of different halide precursors, we can finely tune the chemical composition and the optical properties of presynthesized colloidal cesium lead halide perovskite nanocrystals (NCs), from green emitting CsPbBr3 to bright emitters in any other region of the visible spectrum, and back, by displacement of Cl– or I– ions and reinsertion of Br– ions. This approach gives access to perovskite semiconductor NCs with both structural and optical qualities comparable to those of directly synthesized NCs. We also show that anion exchange is a dynamic process that takes place in solution between NCs. Therefore, by mixing solutions containing perovskite NCs emitting in different spectral ranges (due to different halide compositions) their mutual fast exchange dynamics leads to homogenization in their composition, resulting in NCs emitting in a narrow spectral region that is intermediate between those of the parent nanoparticles.

19 April 2011 in Classical and Quantum Gravity
Verified
Journal Article
Closed access
SHS Hild
S Hild
MAM Abernathy
M Abernathy
FAF Acernese
F Acernese
PSPau Amaro Seoane
Pau Amaro Seoane
NAN Andersson
N Andersson
KYK Yamamoto
K Yamamoto
Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope, a third-generation gravitational wave detector, has been proposed in order to fully open up the emerging field of gravitational wave astronomy. In this article we describe sensitivity models for the Einstein Telescope and investigate potential limits imposed by fundamental noise sources. A special focus is set on evaluating the frequency band below 10Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates. We develop the most accurate sensitivity model, referred to as ET-D, for a third-generation detector so far, including the most relevant fundamental noise contributions.

16 July 2010 in Classical and Quantum Gravity
Verified
Journal Article
Open access
JAJ Abadie
J Abadie
BAB P Abbott
B P Abbott
RAR Abbott
R Abbott
MAM Abernathy
M Abernathy
TAT Accadia
T Accadia
KBK Belczynski
K Belczynski

1 June 2012 in Classical and Quantum Gravity
Verified
Journal Article
Closed access
BSB Sathyaprakash
B Sathyaprakash
MAM Abernathy
M Abernathy
FAF Acernese
F Acernese
PAP Ajith
P Ajith
BAB Allen
B Allen
KYK Yamamoto
K Yamamoto

14 January 2016 in Journal of the American Chemical Society
Verified
Journal Article
Open access
QAQuinten A. Akkerman
Quinten A. Akkerman
SMSilvia Genaro Motti
Silvia Genaro Motti
AKAjay Ram Srimath Kandada
Ajay Ram Srimath Kandada
EMEdoardo Mosconi
Edoardo Mosconi
VDValerio D’innocenzo
Valerio D’innocenzo
LMLiberato Manna
Liberato Manna
We report a colloidal synthesis approach to CsPbBr3 nanoplatelets. The nucleation and growth of the platelets, which takes place at room temperature, is triggered by the injection of acetone in a mixture of precursors that would remain unreactive otherwise. The low growth temperature enables the control of the plate thickness, which can be precisely tuned from 3 to 5 monolayers. The strong two-dimensional confinement of the carriers at such small vertical sizes is responsible for the narrow PL, the strong excitonic absorption and the blue shift of the optical band gap of more than 0.47 eV compared to that of bulk CsPbBr3. We also show that the composition of the platelets can be varied all the way to CsPbCl3 or to CsPbI3 by anion exchange, with preservation of size and shape of the starting particles. The blue fluorescent CsPbCl3 nanoplatelets represent a new member of the scarcely populated group of blue emitting colloidal nanocrystals. The exciton dynamics were found to be independent of the extent of 2D confinement in these platelets, and this was supported by band structure calculations.