Emilio A. Nanni
Massachusetts Institute of Technology
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Featured researches published by Emilio A. Nanni.
Nature Communications | 2015
Emilio A. Nanni; Wenqian Ronny Huang; Kyung-Han Hong; Koustuban Ravi; Arya Fallahi; Gustavo Moriena; R. J. Dwayne Miller; Franz X. Kärtner
The cost, size and availability of electron accelerators are dominated by the achievable accelerating gradient. Conventional high-brightness radio-frequency accelerating structures operate with 30–50 MeV m−1 gradients. Electron accelerators driven with optical or infrared sources have demonstrated accelerating gradients orders of magnitude above that achievable with conventional radio-frequency structures. However, laser-driven wakefield accelerators require intense femtosecond sources and direct laser-driven accelerators suffer from low bunch charge, sub-micron tolerances and sub-femtosecond timing requirements due to the short wavelength of operation. Here we demonstrate linear acceleration of electrons with keV energy gain using optically generated terahertz pulses. Terahertz-driven accelerating structures enable high-gradient electron/proton accelerators with simple accelerating structures, high repetition rates and significant charge per bunch. These ultra-compact terahertz accelerators with extremely short electron bunches hold great potential to have a transformative impact for free electron lasers, linear colliders, ultrafast electron diffraction, X-ray science and medical therapy with X-rays and electron beams.
Journal of Magnetic Resonance | 2012
Alexander B. Barnes; Evgeny Markhasin; Eugenio Daviso; Vladimir K. Michaelis; Emilio A. Nanni; Sudheer Jawla; Elijah L. Mena; Ronald DeRocher; Ajay Thakkar; Paul P. Woskov; Judith Herzfeld; Richard J. Temkin; Robert G. Griffin
We describe the design and implementation of the instrumentation required to perform DNP-NMR at higher field strengths than previously demonstrated, and report the first magic-angle spinning (MAS) DNP-NMR experiments performed at (1)H/e(-) frequencies of 700 MHz/460 GHz. The extension of DNP-NMR to 16.4 T has required the development of probe technology, cryogenics, gyrotrons, and microwave transmission lines. The probe contains a 460 GHz microwave channel, with corrugated waveguide, tapers, and miter-bends that couple microwave power to the sample. Experimental efficiency is increased by a cryogenic exchange system for 3.2 mm rotors within the 89 mm bore. Sample temperatures ≤85 K, resulting in improved DNP enhancements, are achieved by a novel heat exchanger design, stainless steel and brass vacuum jacketed transfer lines, and a bronze probe dewar. In addition, the heat exchanger is preceded with a nitrogen drying and generation system in series with a pre-cooling refrigerator. This reduces liquid nitrogen usage from >700 l per day to <200 l per day and allows for continuous (>7 days) cryogenic spinning without detrimental frost or ice formation. Initial enhancements, ε=-40, and a strong microwave power dependence suggests the possibility for considerable improvement. Finally, two-dimensional spectra of a model system demonstrate that the higher field provides excellent resolution, even in a glassy, cryoprotecting matrix.
Journal of Magnetic Resonance | 2011
Emilio A. Nanni; Alexander B. Barnes; Yoh Matsuki; Paul P. Woskov; Björn Corzilius; Robert G. Griffin; Richard J. Temkin
We present a calculation of the microwave field distribution in a magic angle spinning (MAS) probe utilized in dynamic nuclear polarization (DNP) experiments. The microwave magnetic field (B(1S)) profile was obtained from simulations performed with the High Frequency Structure Simulator (HFSS) software suite, using a model that includes the launching antenna, the outer Kel-F stator housing coated with Ag, the RF coil, and the 4mm diameter sapphire rotor containing the sample. The predicted average B(1S) field is 13μT/W(1/2), where S denotes the electron spin. For a routinely achievable input power of 5W the corresponding value is γ(S)B(1S)=0.84MHz. The calculations provide insights into the coupling of the microwave power to the sample, including reflections from the RF coil and diffraction of the power transmitted through the coil. The variation of enhancement with rotor wall thickness was also successfully simulated. A second, simplified calculation was performed using a single pass model based on Gaussian beam propagation and Fresnel diffraction. This model provided additional physical insight and was in good agreement with the full HFSS simulation. These calculations indicate approaches to increasing the coupling of the microwave power to the sample, including the use of a converging lens and fine adjustment of the spacing of the windings of the RF coil. The present results should prove useful in optimizing the coupling of microwave power to the sample in future DNP experiments. Finally, the results of the simulation were used to predict the cross effect DNP enhancement (ϵ) vs. ω(1S)/(2π) for a sample of (13)C-urea dissolved in a 60:40 glycerol/water mixture containing the polarizing agent TOTAPOL; very good agreement was obtained between theory and experiment.
Journal of Magnetic Resonance | 2012
Alexander B. Barnes; Emilio A. Nanni; Judith Herzfeld; Robert G. Griffin; Richard J. Temkin
We describe the design and implementation of a novel tunable 250 GHz gyrotron oscillator with >10 W output power over most of a 3 GHz band and >35 W peak power. The tuning bandwidth and power are sufficient to generate a >1 MHz nutation frequency across the entire nitroxide EPR lineshape for cross effect DNP, as well as to excite solid effect transitions utilizing other radicals, without the need for sweeping the NMR magnetic field. Substantially improved tunability is achieved by implementing a long (23 mm) interaction cavity that can excite higher order axial modes by changing either the magnetic field of the gyrotron or the cathode potential. This interaction cavity excites the rotating TE(₅,₂,q) mode, and an internal mode converter outputs a high-quality microwave beam with >94% Gaussian content. The gyrotron was integrated into a DNP spectrometer, resulting in a measured DNP enhancement of 54 on the membrane protein bacteriorhodopsin.
Physical Review Special Topics-accelerators and Beams | 2014
W. Graves; J. Bessuille; P. Brown; Sergio Carbajo; V. Dolgashev; Kyung-Han Hong; E. Ihloff; Boris Khaykovich; Hua Lin; Krishna Murari; Emilio A. Nanni; Giacomo Resta; S. Tantawi; Luis E. Zapata; Franz X. Kärtner; D. E. Moncton
A design for a compact x-ray light source (CXLS) with flux and brilliance orders of magnitude beyond existing laboratory scale sources is presented. The source is based on inverse Compton scattering of a high brightness electron bunch on a picosecond laser pulse. The accelerator is a novel high-efficiency standing-wave linac and rf photoinjector powered by a single ultrastable rf transmitter at X-band rf frequency. The high efficiency permits operation at repetition rates up to 1 kHz, which is further boosted to 100 kHz by operating with trains of 100 bunches of 100 pC charge, each separated by 5 ns. The entire accelerator is approximately 1 meter long and produces hard x rays tunable over a wide range of photon energies. The colliding laser is a
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2016
Franz X. Kärtner; F. Ahr; A.-L. Calendron; Huseyin Cankaya; Sergio Carbajo; G. Chang; G. Cirmi; Katerina Dörner; U. Dorda; Arya Fallahi; A. Hartin; Michael Hemmer; Richard G. Hobbs; Y. Hua; W.R. Huang; R. Letrun; N. Matlis; V. Mazalova; O.D. Mücke; Emilio A. Nanni; William P. Putnam; Koustuban Ravi; F. Reichert; Iosifina Sarrou; Xiaojun Wu; A. Yahaghi; H. Ye; Luis E. Zapata; Dongfang Zhang; Chun Zhou
\mathrm{Yb}\ensuremath{\mathbin:}\mathrm{YAG}
Scientific Reports | 2015
W. Ronny Huang; Emilio A. Nanni; Koustuban Ravi; Kyung-Han Hong; Arya Fallahi; Liang Jie Wong; Phillip D. Keathley; Luis E. Zapata; Franz X. Kärtner
solid-state amplifier producing 1030 nm, 100 mJ pulses at the same 1 kHz repetition rate as the accelerator. The laser pulse is frequency-doubled and stored for many passes in a ringdown cavity to match the linac pulse structure. At a photon energy of 12.4 keV, the predicted x-ray flux is
Optics Express | 2015
Koustuban Ravi; Wenqian Ronny Huang; Sergio Carbajo; Emilio A. Nanni; Damian N. Schimpf; Erich P. Ippen; Franz X. Kärtner
5\ifmmode\times\else\texttimes\fi{}1{0}^{11}\text{ }\text{ }\mathrm{photons}/\mathrm{second}
arXiv: Accelerator Physics | 2016
W. Ronny Huang; Arya Fallahi; Xiaojun Wu; Huseyin Cankaya; Anne-Laure Calendron; Koustuban Ravi; Dongfang Zhang; Emilio A. Nanni; Kyung-Han Hong; Franz X. Kärtner
in a 5% bandwidth and the brilliance is
Physical review accelerators and beams | 2016
Sergio Carbajo; Emilio A. Nanni; Liang Jie Wong; Gustavo Moriena; Phillip D. Keathley; Guillaume Laurent; R. J. Dwayne Miller; Franz X. Kärtner
2\ifmmode\times\else\texttimes\fi{}1{0}^{12}\text{ }\text{ }\mathrm{photons}/(\mathrm{sec}\text{ }{\mathrm{mm}}^{2}\text{ }{\mathrm{mrad}}^{2}\text{ }\text{ }0.1%)