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| author | Daniele Nicolodi <daniele@grinta.net> |
|---|---|
| date | Sun, 17 Oct 2021 16:52:37 +0200 |
| parents | 6396966cca25 |
| children | 86a6ab1746e4 |
| rev | line source |
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| 0 | 1 \documentclass[a4paper,11pt]{article} |
| 2 \usepackage[T1]{fontenc} | |
| 7 | 3 \usepackage[utf8]{inputenc} |
| 0 | 4 \usepackage{cv} |
| 23 | 5 \usepackage{graphicx} |
| 0 | 6 |
| 7 \newcommand{\utn}{Universit\`{a} degli Studi di Trento} | |
| 8 | |
| 9 \name{Daniele Nicolodi} | |
| 10 \address{% | |
| 23 | 11 Physikalisch-Technische Bundesanstalt\\ |
| 12 Bundesallee 100\\ | |
| 13 Braunschweig, D-38116, Germany} | |
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14 \info{% |
| 23 | 15 Phone: & +49 531 5924315 \\ |
| 16 & +49 1520 7178926 \\ | |
| 17 Email: & \mailto{daniele.nicolodi@ptb.de}\\ | |
| 18 \raisebox{-0.3em}{\includegraphics[width=1.3em]{orcid.pdf}} & \orcid{0000-0003-1467-1756}} | |
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19 |
| 0 | 20 \bibliography{publications} |
| 21 | |
| 11 | 22 % \DeclareBibliographyCategory{selected} |
| 23 % \addtocategory{selected}{natcomms-2016,metrologia-2016,natphot-2015,natphot-2014,prl-2009} | |
| 24 % \printbibliography[heading=bibnumbered,category=selected,title={Selected publications}] | |
| 25 | |
| 0 | 26 \begin{document} |
| 27 \maketitle | |
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28 |
| 0 | 29 \section{Education} |
| 30 \begin{description} | |
| 31 \item[2011 \enspace Ph.D. in Physics] \utn, Trento, Italy. Degree | |
| 23 | 32 obtained with grade Excellent, highest honours. Dissertation: |
| 33 \textit{``Femto Newton level testing of free-fall on | |
| 34 ground''}. Supervisor: William Joseph Weber. | |
| 0 | 35 \item[2007 \enspace Master Degree in Physics] Laurea Magistrale, \utn, |
| 23 | 36 Trento, Italy. Degree obtained with grade 110/110 cum laude, highest |
| 37 honours. Thesis: \textit{``Toward a third generation torsion | |
| 38 pendulum for the femto-Newton level testing of free fall in the | |
| 39 laboratory''}. Supervisor: Stefano Vitale. | |
| 40 \item[2004 \enspace Bachelor Degree in Applied Physics] Laurea, \utn, | |
| 41 Trento, Italy. Degree obtained with grade 110/110. Thesis: | |
| 42 \textit{``Calibration system for the scintillators employed in the | |
| 43 CRESST-II dark matter research experiment''}. | |
| 0 | 44 \end{description} |
| 45 | |
| 46 \section{Relevant work experiences} | |
| 47 \begin{description} | |
| 23 | 48 \item[September 2020 - present] Junior Group Leader. Quantum Optics |
| 49 and Unit of Length Department, Optics Division, | |
| 50 Physikalisch-Technische Bundesanstalt, Braunschweig, Germany. | |
| 51 \item[February 2016 - August 2020] Research associate. Optical Frequency | |
| 11 | 52 Measurements Group, Time and Frequency Division, National Institute of |
| 53 Standards and Technology, Boulder, Colorado, USA. | |
| 54 \item[May 2012 - December 2015] Post-doc fellow. Optical Frequency Metrology | |
| 7 | 55 Group, SYRTE -- Observatoire de Paris, Paris, France. |
| 3 | 56 \item[November 2007 - April 2012] Research Assistant. Experimental |
| 0 | 57 Gravitation Laboratory, University of Trento, Trento, Italy. |
| 58 \item[February 2010 - October 2011] Assistant Lecturer for the course | |
| 23 | 59 \textit{``Fisica 1''} -- Newtonian physics for 1st year students -- |
| 60 at the Faculty of Engineering, University of Trento, Trento, Italy. | |
| 0 | 61 \item[February 2009 - October 2009] Assistant Lecturer for the course |
| 23 | 62 \textit{``Laboratorio di Fisica 1''} -- introductory physics |
| 63 laboratory for 1st year Physics students -- at the Faculty of | |
| 64 Science, University of Trento, Trento, Italy. | |
| 65 % \item[1999 - 2007] Freelance in the Information Technology field with | |
| 66 % particular, but not limited to, experience in the design, | |
| 67 % development and integration of custom GNU-Linux solutions, design | |
| 68 % and development of desktop and web-based applications, network | |
| 69 % protocol analysis and implementation. | |
| 0 | 70 \end{description} |
| 71 | |
| 26 | 72 \section{Research activity} |
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73 \begin{dottedlist} |
| 26 | 74 optical frequency metrology \and ultra-stable lasers \and optical |
| 75 atomic clocks \and optical frequency combs \and photonic microwave | |
| 76 generation \and spectral purity transfer \and fiber and free-space | |
| 77 optical frequency transfer \and gravitational waves detection \and | |
| 78 torsion balances | |
| 3 | 79 \end{dottedlist} |
| 80 | |
| 81 \noindent | |
| 26 | 82 Ultra-stable lasers are essential optical atomic clocks, quantum |
| 83 devices based on cold atoms, and quantum communications. Better laser | |
| 84 frequency stability will improve optical atomic clocks timekeeping | |
| 85 stability and will enable more stringent fundamental physics tests | |
| 86 that will challenge our understanding of the universe. Cryogenic | |
| 87 high-finesse optical cavities allow to overcome the thermal noise | |
| 88 limit of room-temperature optical cavities and represent the | |
| 89 state-of-the-art in laser frequency stabilization. I develop | |
| 90 cryogenic optical cavities targeting even better laser frequency | |
| 91 stability by operating at lower temperatures and employing new | |
| 92 designs, novel mirror technologies, and different materials. | |
| 93 | |
| 94 Optical atomic clocks are the most accurate measurement devices ever | |
| 95 realized and are set to replace microwave Cs clocks as definition of | |
| 96 the second. I contributed to the development and systematic | |
| 97 uncertainty evaluation of NIST's Yb optical lattice clocks that made | |
| 98 these clocks the world's most accurate optical clocks. I contributed | |
| 99 to the measurement campaigns that compared NIST's Yb optical lattice | |
| 100 clocks with other optical atomic clocks and with microwave primary and | |
| 101 secondary frequency standards via optical fiber links and satellite | |
| 102 microwave links. The unprecedented accuracy and the agreement | |
| 103 demonstrated between the clocks realized an important milestone toward | |
| 104 the future redefinition of the second. | |
| 0 | 105 |
| 26 | 106 Exploiting ultra-stable lasers for scientific and technological |
| 107 applications most often requires transferring their exquisite | |
| 108 frequency stability to oscillators operating at a different | |
| 109 frequency. I developed a fiber-based optical frequency comb system | |
| 110 that realized optical frequency stability transfer between lasers | |
| 111 widely different wavelength with unprecedented and unsurpassed | |
| 112 frequency stability. Low phase noise microwaves sources are paramount | |
| 113 for many applications, including precision metrology, deep-space | |
| 114 navigation, coherent radar, and wireless communications. In | |
| 115 collaboration with industrial partners, I developed a fiber-based | |
| 116 optical frequency comb system for photonic microwave generation with | |
| 117 unprecedented and unsurpassed low phase noise and zeptosecond-level | |
| 118 absolute timing noise. This system has then been commercialized. | |
| 119 | |
| 120 Gravitational waves observations are revolutionizing astronomy and | |
| 121 astrophysics. Detecting gravitational waves relies on | |
| 122 interferometrically measuring the distance between test-masses in near | |
| 123 perfect free-fall. I conducted on-ground measurement of the small | |
| 124 force disturbances acting on the test-masses of the LISA space | |
| 125 gravitational waves detector exploiting the femto-Newton level | |
| 126 sensitivity of a torsion balance. I identified and modelled an | |
| 127 unexpected increase of Brownian noise from residual gas molecules | |
| 128 collisions in constrained geometries, with repercussions on the design | |
| 129 of LISA and second generation ground-based gravitational wave | |
| 130 detectors. I contributed to the design of the LISA Pathfinder mission | |
| 131 for the in-flight testing of the concept of low-frequency | |
| 132 gravitational waves detection in space and that validated the | |
| 133 disturbance model developed from the on-ground measurements. | |
| 23 | 134 |
| 0 | 135 \section{Skills and competences} |
| 136 | |
| 26 | 137 I developed experiments that advanced the state-of-the-art in the |
| 138 respective domains by realizing unprecedented performances. I designed | |
| 139 and implemented innovative measurement techniques. I have experience | |
| 140 in experiment design and optimization. I have redacted of research | |
| 141 project and funding applications. I have been working with outstanding | |
| 142 results in large international collaborations and in smaller focused | |
| 143 collaborations both with industrial and academic partners. I have | |
| 144 experience in the interaction with the aerospace industry. I have | |
| 145 co-supervised master and PhD students. | |
| 0 | 146 |
| 26 | 147 I have extensive experience with optical frequency combs, ultra-stable |
| 148 lasers, high-finesse optical cavities, free-space and fiber optical | |
| 149 systems, very low noise audio-frequency, radio-frequency, and | |
| 150 microwave electronics, software-defined radios, ultra-high vacuum | |
| 151 systems, cryogenics and close-cycle cryostats, data acquisition | |
| 152 hardware and software. | |
| 17 | 153 |
| 154 I developed data analysis methods and numerical simulations. I am | |
| 23 | 155 proficient programming in C, C\texttt{++}, Python, Perl, Matlab, |
| 26 | 156 LabVIEW, and Lisp. I have designed and implemented real-time data |
| 157 acquisition and processing. I master modern software development | |
| 158 techniques and version control systems. I am passionate about Free | |
| 159 Software and I contribute to Free Software projects. | |
| 0 | 160 |
| 23 | 161 % \section{Other relevant experiences} |
| 162 % \begin{description}[style=sameline] | |
| 163 % \item[February - August 2018:] | |
| 164 % Mentor for the Google Summer of Code program for the Debian organization. | |
| 165 % \item[October 4th-8th 2010:] | |
| 166 % Advanced Scientific Programming in Python Autumn School, Trento, Italy. | |
| 167 % \item[May 5th-9th 2008:] | |
| 168 % 3rd VESF School on Gravitational Waves Summer School, Virgo, Cascina, Italy. | |
| 169 % \item[August 2005 - July 2006:] | |
| 170 % Erasmus student at the Lunds Universitet, Lund, Sweden. | |
| 171 % \item[April - June 2005:] | |
| 172 % Visiting student at the T\"{u}binghen Universit\"{a}t, T\"{u}binghen, Germany. | |
| 173 % \end{description} | |
| 0 | 174 |
| 20 | 175 \section{Languages} |
| 176 \begin{description}[style=sameline] | |
| 177 \item[Italian:] | |
| 178 native speaker. | |
| 179 \item[English:] | |
| 180 highly proficient. | |
| 181 \item[French:] | |
| 182 basic communication skills, good understanding. | |
| 183 \end{description} | |
| 0 | 184 |
| 26 | 185 \section{Awards} |
| 186 \begin{description} | |
| 187 \item[2019 \enspace PML Distinguished Associate Award, NIST] For | |
| 188 creating and networking the world's best optical atomic clocks for | |
| 189 a 100-fold improvement in precision timekeeping over state of the | |
| 190 art. | |
| 191 \end{description} | |
| 192 | |
| 17 | 193 \section{Publications} |
| 23 | 194 35 articles in peer-reviewed international journals: Nature, Science, |
| 26 | 195 Nature Photonics, Physical Review Letters, Optica, Classical and |
| 196 Quantum Gravity, and others. Cited 1350 times. H index 24. Two | |
| 197 invited and 8 more talks at international conferences. | |
| 17 | 198 |
| 199 \printbibliography[heading=none] | |
| 0 | 200 |
| 201 \section{Conference contributions} | |
| 202 | |
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203 \newcommand{\litem}[1]{\item{\it #1.}} |
| 0 | 204 \begin{enumerate} |
| 23 | 205 \litem{Optical clock frequency ratios at the 18th decimal place} |
| 206 Talk. EFTF: European Time and Frequency Forum, Noordwijk, The | |
| 207 Netherlands. April 21-23, \textbf{2020}. | |
| 208 | |
| 209 \litem{Toward optical lattice clocks at the $\mathit{10^{-19}}$ level} | |
| 210 Invited talk. IFCS-EFTF Conference, Oralndo, Florida, USA. April | |
| 211 14-18, \textbf{2019}. | |
| 212 | |
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213 \litem{Cryogenic high-finesse optical cavity to improve the stability |
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214 of Yb optical lattice clocks} Talk. 2018 IEEE International |
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215 Frequency Control Symposium, Olympic Valley, California, USA. May |
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216 22-24, \textbf{2018}. |
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217 |
| 20 | 218 \litem{Beyond state-of-the-art laser frequency stabilization for |
| 219 improved Yb optical lattice clocks} Poster. ICOLS: International | |
| 220 Conference on Laser Spectroscopy, Arcachon, France, July 2-8, | |
| 221 \textbf{2017}. | |
| 222 | |
| 11 | 223 \litem{Ultra-low phase noise frequency-comb-based microwave generation |
| 224 and characterization} Talk. IEEE International Frequency Control | |
| 225 Symposium, New Orleans, Louisiana, USA. May 9-12, \textbf{2016}. | |
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226 |
| 23 | 227 % \litem{Phase noise measurements} Lecture. 2015 ITN-FACT Workshop, |
| 228 % LNE-SYRTE -- Observatoire de Paris, Paris, France. September 8-10, | |
| 229 % \textbf{2015}. | |
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230 |
| 23 | 231 % \litem{Software in physics experiments} Lecture. 2015 ITN-FACT |
| 232 % Workshop, LNE-SYRTE -- Observatoire de Paris, Paris, France. September | |
| 233 % 8-10, \textbf{2015}. | |
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234 |
| 7 | 235 \litem{Automatic control of amplitude-to-phase conversion in |
| 236 photo-detection of femto-second pulses for low phase-noise microwave | |
| 11 | 237 generation} Poster. IFCS-EFTF Conference, Denver, Colorado, USA. April |
| 7 | 238 12-16, \textbf{2015}. |
| 239 | |
| 240 \litem{Optical and microwave frequency synthesis with optical frequency | |
| 11 | 241 combs} Invited seminar. Sao Paulo University, Sao Carlos, Brazil. |
| 7 | 242 September 2, \textbf{2014}. |
| 243 | |
| 244 \litem{Spectral purity transfer between optical wavelengths at the | |
| 11 | 245 $\mathit{10^{-18}}$ level} Talk. CPEM 2014, Rio de Janeiro, Brazil. |
| 7 | 246 August 24-29, \textbf{2014}. |
| 247 | |
| 248 \litem{Spectral purity transfer between optical wavelengths at the | |
| 249 $\mathit{10^{-18}}$ level} Talk. French-Russian-German Laser | |
| 11 | 250 Symposium 2013, Besançon, France. November 4-7, \textbf{2013}. |
| 7 | 251 |
| 252 \litem{Spectral purity transfer between optical wavelengths at the | |
| 253 $\mathit{10^{-18}}$ level} Talk. Joint UFFC, EFTF and PFM Symposium, | |
| 11 | 254 Prague, Czech Republic. July 21-25, \textbf{2013}. |
| 7 | 255 |
| 0 | 256 \litem{Brownian force noise from residual gas damping and the |
| 257 sensitivity of advanced gravitational wave observatories} Talk. | |
| 11 | 258 9th Amaldi Conference on Gravitational Waves, Cardiff, Wales, UK. |
| 0 | 259 July 10-15, \textbf{2011}. |
| 260 | |
| 261 \litem{Femto-Newton level testing of free-fall on-ground} Solicited | |
| 11 | 262 talk. 38th COSPAR Scientific Assembly, Bremen, Germany. July 18-25, |
| 0 | 263 \textbf{2010}. |
| 264 | |
| 265 \litem{Experimental investigation of GRS force disturbance sources} | |
| 11 | 266 Talk. 8th LISA Symposium, Stanford University, California, USA. June |
| 0 | 267 28 - July 2, \textbf{2010}. |
| 268 | |
| 269 \litem{Improving torsion pendulum force sensitivity with LISA | |
| 270 Pathfinder like interferometric angular read-out} Poster. 8th LISA | |
| 11 | 271 Symposium, Stanford University, California, USA. June 28 - July 02, |
| 0 | 272 \textbf{2010}. |
| 273 | |
| 274 \litem{Increased Brownian force noise from molecular impacts in a | |
| 275 constrained volume} Talk. From Quantum to Cosmos 4 - Q2C4, Bremen, | |
| 11 | 276 Germany. September 21-24, \textbf{2009}. |
| 0 | 277 |
| 278 \litem{Gas damping in the LISA noise budget} Poster. 8th Edoardo | |
| 11 | 279 Amaldi Conference on Gravitational Waves, New York, USA. June 21-26, |
| 0 | 280 \textbf{2009}. |
| 281 | |
| 282 \litem{An improved torsion pendulum for on-ground verification of the | |
| 283 LISA gravitational reference sensor} Poster. 7th LISA Symposium, | |
| 11 | 284 Barcelona, Spain. June 16-20, \textbf{2008}. |
| 0 | 285 |
| 286 \litem{Characterization of the LISA gravitational reference sensor with | |
| 287 an upgraded torsion pendulum} Poster. 7th Edoardo Amaldi Conference | |
| 11 | 288 on Gravitational Waves, Sydney, Australia. July 8-14, \textbf{2007}. |
| 0 | 289 \end{enumerate} |
| 290 | |
| 23 | 291 \vfill{\fontsize{9}{12}\selectfont Last updated \today} |
| 0 | 292 |
| 293 \end{document} |