|
0
|
1 \documentclass[a4paper,11pt]{article}
|
|
|
2 \usepackage[T1]{fontenc}
|
|
7
|
3 \usepackage[utf8]{inputenc}
|
|
0
|
4 \usepackage{cv}
|
|
7
|
5 % \usepackage{parskip}
|
|
0
|
6
|
|
|
7 \newcommand{\utn}{Universit\`{a} degli Studi di Trento}
|
|
|
8
|
|
|
9 \name{Daniele Nicolodi}
|
|
|
10 \address{%
|
|
11
|
11 National Institute of Standards and Technology \\
|
|
|
12 325 Broadway \\
|
|
|
13 Boulder, CO 80305, USA}
|
|
0
|
14 \info{%
|
|
11
|
15 Phone: & +1 303 497 6801 \\
|
|
|
16 & +1 720 416 7395 \\
|
|
|
17 Email: & \mailto{daniele.nicolodi@nist.gov}}
|
|
0
|
18
|
|
|
19 \bibliography{publications}
|
|
|
20
|
|
11
|
21 % \DeclareBibliographyCategory{selected}
|
|
|
22 % \addtocategory{selected}{natcomms-2016,metrologia-2016,natphot-2015,natphot-2014,prl-2009}
|
|
|
23 % \printbibliography[heading=bibnumbered,category=selected,title={Selected publications}]
|
|
|
24
|
|
0
|
25 \begin{document}
|
|
|
26 \maketitle
|
|
|
27
|
|
|
28 \section{Education}
|
|
|
29 \begin{description}
|
|
|
30 \item[2011 \enspace Ph.D. in Physics] \utn, Trento, Italy. Degree
|
|
|
31 obtained with grade Excellent -- highest honours. Dissertation:
|
|
|
32 <<Femto Newton level testing of free fall on ground>>. Supervisor:
|
|
|
33 William Joseph Weber.
|
|
|
34 \item[2007 \enspace Master Degree in Physics] Laurea Magistrale, \utn,
|
|
|
35 Trento, Italy. Degree obtained with grade 110/110 cum laude -- highest
|
|
|
36 honours. Thesis: <<Toward a third generation torsion pendulum for
|
|
|
37 the femto-Newton level testing of free fall in the laboratory>>.
|
|
|
38 \item[2004 \enspace Bachelor Degree in Applied Physics] Laurea, \utn, Trento,
|
|
|
39 Italy. Degree obtained with grade 110/110. Thesis:
|
|
|
40 <<Calibration system for the scintillators employed in the CRESST-II
|
|
|
41 dark matter research experiment>>.
|
|
|
42 \end{description}
|
|
|
43
|
|
|
44 \section{Relevant work experiences}
|
|
|
45 \begin{description}
|
|
11
|
46 \item[February 2016 - present] Post-doc fellow. Optical Frequency
|
|
|
47 Measurements Group, Time and Frequency Division, National Institute of
|
|
|
48 Standards and Technology, Boulder, Colorado, USA.
|
|
|
49 \item[May 2012 - December 2015] Post-doc fellow. Optical Frequency Metrology
|
|
7
|
50 Group, SYRTE -- Observatoire de Paris, Paris, France.
|
|
3
|
51 \item[November 2007 - April 2012] Research Assistant. Experimental
|
|
0
|
52 Gravitation Laboratory, University of Trento, Trento, Italy.
|
|
|
53 \item[February 2010 - October 2011] Assistant Lecturer for the course
|
|
|
54 <<Fisica 1>> -- Newtonian physics for 1st year students -- at the
|
|
|
55 Faculty of Engineering, University of Trento, Trento, Italy.
|
|
|
56 \item[February 2009 - October 2009] Assistant Lecturer for the course
|
|
|
57 <<Laboratorio di Fisica 1>> -- introductory physics laboratory for
|
|
|
58 1st year Physics students -- at the Faculty of Science, University
|
|
|
59 of Trento, Trento, Italy.
|
|
|
60 \item[1999 - 2007] Freelance in the Information Technology field with
|
|
|
61 particular, but not limited to, experience in the design,
|
|
|
62 development and integration of custom GNU-Linux solutions, design
|
|
|
63 and development of desktop and web-based applications, network
|
|
|
64 protocol analysis and implementation.
|
|
|
65 \end{description}
|
|
|
66
|
|
|
67 \section{Current research activity and interests}
|
|
|
68 \begin{dottedlist}
|
|
7
|
69 High precision frequency metrology \and Optical frequency combs \and
|
|
|
70 Low phase-noise photonic microwave generation \and Ultra-stable
|
|
|
71 lasers \and Laser frequency stabilization techniques \and Optical
|
|
|
72 clocks
|
|
0
|
73 \end{dottedlist}
|
|
|
74
|
|
|
75 \noindent
|
|
7
|
76 My research activity focuses on the exploitation fiber-based optical
|
|
|
77 frequency combs systems for the transfer of the frequency stability of
|
|
|
78 ultra-stable lasers to other wavelengths in the optical domain and to
|
|
|
79 the microwave domain. Amnong other applications, the aim is to
|
|
|
80 generate high stability optical and microwave signals to probe the
|
|
|
81 atomic fountan clocks and the optical lattice clocks at SYRTE.
|
|
3
|
82
|
|
7
|
83 In the optical domain we recently realized and an optical frequency
|
|
|
84 stability transfer scheme based on an optical frequency comb capable
|
|
|
85 of transferring frequency stability exceeding the thermal noise limit
|
|
|
86 of state-of-the-art high-finesse optical cavities. In the microwave
|
|
|
87 domain the solution implemented in my laboraotry is already capable to
|
|
|
88 compete with the stability of state-of-the-art cryogenic sapphire
|
|
|
89 oscillators. My research aims at further improving the phase noise of
|
|
|
90 the generated microwave signal by exploring new optical frequency comb
|
|
|
91 and photo-detection technologies.
|
|
|
92
|
|
|
93 I am also responsible for the operation of the femtosecond combs for
|
|
|
94 the characterization the ultra-stable laser developed at SYRTE and for
|
|
|
95 the comparison of the different optical and microwave clocks operated
|
|
|
96 at SYRTE with stability and accuracy not limited by the stability of
|
|
|
97 the optical frequency comb setup.
|
|
|
98
|
|
|
99 \section{Previous research activity}
|
|
3
|
100 \begin{dottedlist}
|
|
|
101 High precision force metrology \and High sensitivity torsion
|
|
|
102 pendulums \and Sources of force noise on geodesic reference
|
|
|
103 macroscopic test masses \and Dissipation mechanisms in mechanical
|
|
|
104 experiments \and Optical interferometry
|
|
|
105 \end{dottedlist}
|
|
|
106
|
|
|
107 \noindent
|
|
|
108 My previous research activity focused on the study of the limits for
|
|
|
109 achieving near perfect free-fall of macroscopic test masses for the
|
|
|
110 observation of gravitational waves. In particular, I contributed to
|
|
|
111 the on-ground measurement of small force disturbances on the test
|
|
|
112 masses of the Laser Interferometer Space Antenna space low-frequency
|
|
7
|
113 gravitational wave detector -- LISA -- and its precursor mission LISA
|
|
3
|
114 Pathfinder, exploiting the femto-Newton level sensitivity of a torsion
|
|
7
|
115 pendulum.
|
|
|
116
|
|
|
117 My work work included the experimental activity, the development of
|
|
|
118 data analysis routines for the extraction of stochastic and coherent
|
|
|
119 small force signals, and, concurrently it also aimed at improving the
|
|
|
120 sensitivity of the torsion pendulum apparatus itself, pushing the
|
|
|
121 current limits for small force metrology. I lead the initial effort
|
|
|
122 for the realisation of a low-noise torsion pendulum angular position
|
|
|
123 read-out based on an heterodyne wavefront-sensing interferometer with
|
|
|
124 nanoradian sensitivity, applying some of the LISA Pathfinder
|
|
|
125 interferometer techniques. I collaborated to the development of the
|
|
|
126 LTPDA Matlab Toolbox for the LISA Pathfinder data analysis, with
|
|
|
127 particular attention to the relational database data storage
|
|
|
128 component.
|
|
0
|
129
|
|
|
130 \section{Skills and competences}
|
|
|
131
|
|
7
|
132 I have experience in designing and analysing experiments and
|
|
0
|
133 measurement techniques, with the particular attention to detail and
|
|
|
134 sources of uncertainty required in high precision measurements. I have
|
|
|
135 experience with the design, setup and operation of precise mechanical
|
|
|
136 apparatuses, low noise electronics, high precision optical systems,
|
|
|
137 data acquisition hardware and software, computer controlled
|
|
|
138 experiments, and high vacuum systems, as well as with the development
|
|
3
|
139 of data analysis methods and numerical simulations. More recently I
|
|
|
140 acquired competences in the operation of fiber-based optical frequency
|
|
|
141 combs, ultra-stable laser stabilised on high-finesse optical cavities,
|
|
7
|
142 frequency and phase noise characterization, radio-frequency and
|
|
|
143 microwave electronics, and software-defined radio.
|
|
0
|
144
|
|
7
|
145 I am proficient programming in C, C\texttt{++}, Python, Perl, Matlab,
|
|
|
146 and LabView, with specific experience in scientific computing and data
|
|
0
|
147 analysis. I have experience in real-time data acquisition and
|
|
7
|
148 processing, and I have knowledge of real-time programming techniques.
|
|
|
149 I master and routinely take advantage of modern software development
|
|
|
150 techniques and version control systems. I'm passionate about Free
|
|
|
151 Software and I contribute to several Free Software projects. I have
|
|
|
152 experience in system administration of GNU-Linux systems and I'm
|
|
|
153 comfortable working in Unix, Mac~OS~X, and Microsoft Windows computing
|
|
|
154 environments. I have good knowledge of the LaTeX typesetting system.
|
|
0
|
155
|
|
|
156 \section{Other relevant experiences}
|
|
|
157 \begin{description}
|
|
|
158 \item[October 4th - 8th 2010]
|
|
|
159 Advanced Scientific Programming in Python Autumn School, Trento, Italy.
|
|
|
160 \item[May 5th - 9th 2008]
|
|
|
161 3rd VESF School on Gravitational Waves Summer School, Virgo, Cascina, Italy.
|
|
|
162 \item[August 2005 - July 2006]
|
|
|
163 Erasmus student at the Lunds Universitet, Lund, Sweden.
|
|
|
164 \item[April 2005 - June 2005]
|
|
|
165 Visiting student at the Physics department of the
|
|
|
166 T\"{u}binghen Universit\"{a}t, T\"{u}binghen, Germany.
|
|
|
167 \end{description}
|
|
|
168
|
|
|
169 %\section{Languages}
|
|
|
170 %\begin{description}[style=sameline]
|
|
|
171 %\item[Italian:]
|
|
|
172 % mother tongue.
|
|
|
173 %\item[English:]
|
|
|
174 % good spoken and written.
|
|
|
175 %\end{description}
|
|
|
176
|
|
|
177 % publications
|
|
11
|
178 \printbibliography[heading=bibnumbered,title={Publications}]
|
|
0
|
179
|
|
|
180 \section{Conference contributions}
|
|
|
181
|
|
|
182 \newcommand{\litem}[1]{\item{\it #1.}}
|
|
|
183 \begin{enumerate}
|
|
11
|
184 \litem{Ultra-low phase noise frequency-comb-based microwave generation
|
|
|
185 and characterization} Talk. IEEE International Frequency Control
|
|
|
186 Symposium, New Orleans, Louisiana, USA. May 9-12, \textbf{2016}.
|
|
|
187
|
|
7
|
188 \litem{Automatic control of amplitude-to-phase conversion in
|
|
|
189 photo-detection of femto-second pulses for low phase-noise microwave
|
|
11
|
190 generation} Poster. IFCS-EFTF Conference, Denver, Colorado, USA. April
|
|
7
|
191 12-16, \textbf{2015}.
|
|
|
192
|
|
|
193 \litem{Optical and microwave frequency synthesis with optical frequency
|
|
11
|
194 combs} Invited seminar. Sao Paulo University, Sao Carlos, Brazil.
|
|
7
|
195 September 2, \textbf{2014}.
|
|
|
196
|
|
|
197 \litem{Spectral purity transfer between optical wavelengths at the
|
|
11
|
198 $\mathit{10^{-18}}$ level} Talk. CPEM 2014, Rio de Janeiro, Brazil.
|
|
7
|
199 August 24-29, \textbf{2014}.
|
|
|
200
|
|
|
201 \litem{Spectral purity transfer between optical wavelengths at the
|
|
|
202 $\mathit{10^{-18}}$ level} Talk. French-Russian-German Laser
|
|
11
|
203 Symposium 2013, Besançon, France. November 4-7, \textbf{2013}.
|
|
7
|
204
|
|
|
205 \litem{Spectral purity transfer between optical wavelengths at the
|
|
|
206 $\mathit{10^{-18}}$ level} Talk. Joint UFFC, EFTF and PFM Symposium,
|
|
11
|
207 Prague, Czech Republic. July 21-25, \textbf{2013}.
|
|
7
|
208
|
|
0
|
209 \litem{Brownian force noise from residual gas damping and the
|
|
|
210 sensitivity of advanced gravitational wave observatories} Talk.
|
|
11
|
211 9th Amaldi Conference on Gravitational Waves, Cardiff, Wales, UK.
|
|
0
|
212 July 10-15, \textbf{2011}.
|
|
|
213
|
|
|
214 \litem{Femto-Newton level testing of free-fall on-ground} Solicited
|
|
11
|
215 talk. 38th COSPAR Scientific Assembly, Bremen, Germany. July 18-25,
|
|
0
|
216 \textbf{2010}.
|
|
|
217
|
|
|
218 \litem{Experimental investigation of GRS force disturbance sources}
|
|
11
|
219 Talk. 8th LISA Symposium, Stanford University, California, USA. June
|
|
0
|
220 28 - July 2, \textbf{2010}.
|
|
|
221
|
|
|
222 \litem{Improving torsion pendulum force sensitivity with LISA
|
|
|
223 Pathfinder like interferometric angular read-out} Poster. 8th LISA
|
|
11
|
224 Symposium, Stanford University, California, USA. June 28 - July 02,
|
|
0
|
225 \textbf{2010}.
|
|
|
226
|
|
|
227 \litem{Increased Brownian force noise from molecular impacts in a
|
|
|
228 constrained volume} Talk. From Quantum to Cosmos 4 - Q2C4, Bremen,
|
|
11
|
229 Germany. September 21-24, \textbf{2009}.
|
|
0
|
230
|
|
|
231 \litem{Gas damping in the LISA noise budget} Poster. 8th Edoardo
|
|
11
|
232 Amaldi Conference on Gravitational Waves, New York, USA. June 21-26,
|
|
0
|
233 \textbf{2009}.
|
|
|
234
|
|
|
235 \litem{An improved torsion pendulum for on-ground verification of the
|
|
|
236 LISA gravitational reference sensor} Poster. 7th LISA Symposium,
|
|
11
|
237 Barcelona, Spain. June 16-20, \textbf{2008}.
|
|
0
|
238
|
|
|
239 \litem{Characterization of the LISA gravitational reference sensor with
|
|
|
240 an upgraded torsion pendulum} Poster. 7th Edoardo Amaldi Conference
|
|
11
|
241 on Gravitational Waves, Sydney, Australia. July 8-14, \textbf{2007}.
|
|
0
|
242 \end{enumerate}
|
|
|
243
|
|
|
244 \vfill
|
|
13
|
245 \centering\fontsize{9}{12}\sf Updated \today.
|
|
0
|
246
|
|
|
247 \end{document}
|
