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7 results on '"Daniel Swetz"'

1. The status of the HOLMES experiment

Author

Luca Origo, Bradley Alpert, Marco Balata, Daniel Becker, Douglas Bennett, Adriano Bevilacqua, Matteo Borghesi, Noemi Cerboni, Giancarlo Ceruti, Edvige Celasco, Matteo De Gerone, Rugard Dressler, Marco Faverzani, Elena Ferri, Joseph Fowler, Giovanni Gallucci, John Gard, Flavio Gatti, Andrea Giachero, Gene Hilton, Ulli Köster, Danilo Labranca, Maurizio Lusignoli, John Mates, Emilio Maugeri, Roberto Moretti, Stefano Nisi, Angelo Nucciotti, Luigi Parodi, Gianluigi Pessina, Stefano Ragazzi, Carl Reintsema, Dan Schmidt, Dorothea Schumann, Fabio Siccardi, Daniel Swetz, Joel Ullom, and Leila Vale

Published
2023
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2. Status of HOLMES, an experiment for measuring the nu mass

Author

Elena Ferri, Bradley Alpert, Marco Balata, Daniel Becker, Douglas Bennett, Matteo Borghesi, Noemi Cerboni, Matteo De Gerone, Rugard Dressler, Marco Faverzani, Mariia Fedkevych, Joseph Fowler, Giovanni Gallucci, John Gard, Flavio Gatti, Andrea Giachero, Gene Hilton, Ulli Köster, Danilo Labranca, Maurizio Lusignoli, John Mates, Emilio Maugeri, Stefano Nisi, Angelo Nucciotti, Luca Origo, Gianluigi Pessina, Stefano Ragazzi, Carl Reintsema, Dan Schmidt, Dorothea Schumann, Daniel Swetz, Joel Ullom, and Leila Vale

Published
2022
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3. A Tabletop X-Ray Tomography Instrument for Nanometer-Scale Imaging: Reconstructions

Author

Zachary Levine, Bradley Alpert, Amber Dagel, Joseph Fowler, Edward Jiminez, Nathan Nakamura, Daniel Swetz, Paul Szypryt, Kyle Thompson, and Joel Ullom

Abstract

We show three-dimensional reconstructions of a region of an integrated circuit from a 130 nm copper process. The reconstructions employ x-ray computed tomography, measured with a new and innovative high-magnification x-ray microscope. The instrument uses a focused electron beam to generate x rays in a 100 nm spot and energy-resolving x-ray detectors that minimize backgrounds and hold promise for identification of materials within the sample. The x-ray generation target, a layer of platinum, is fabricated on the circuit wafer itself. A region of interest is imaged from a limited range of angles and without physically removing the region from the larger circuit. The reconstruction is consistent with the circuit’s design file.

Published
2022
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4. A metastable brominated nanodiamond surface enables room temperature and catalysis-free amine chemistry

Author

Cynthia Melendrez, Jorge Lopez-Rosas, Camron Stokes, Tsz Cheung, Sang-Jun Lee, Charles Titus, Jocelyn Valenzuela, Grace Jeanpierre, Halim Muhammad, Polo Tran, Perla Sandoval, Tyanna Supreme, Virginia Altoe, Jan Vavra, Helena Raabova, Vaclav Vanek, Sami Sainio, William Doriese, Galen O'Neil, Daniel Swetz, Joel Ullom, Kent Irwin, Dennis Nordlund, Petr Cigler, and Abraham Wolcott

Abstract

Bromination of high-pressure high-temperature (HPHT) nanodiamond (ND) surfaces has not been explored and can open new avenues for increased chemical reactivity and diamond lattice covalent bond formation. The large bond dissociation energy of the diamond lattice-oxygen bond is a challenge that prevents new bonds from forming and most researchers simply use oxygen-terminated ND (alcohols and acids) as a reactive species. In this work, we transformed a tertiary alcohol-rich ND surface to an amine surface with 50% surface coverage and was limited by the initial rate of bromination. We observed that alkyl-bromide moieties are highly labile on NDs and are metastable as previously found using density functional theory. The instability of the bromine terminated ND is explained by steric hindrance and poor surface energy stabilization. The strong leaving group properties of the alkyl-bromide intermediate were found to form diamond-nitrogen bonds at room temperature and without catalysts. The chemical lability of the brominated ND surface led to efficient amination with NH3•THF at 298 K, and a catalyst-free Sonogashira-type reaction with an alkyne-amine produced an 11-fold increase in amination rate. Overlapping spectroscopies under inert, temperature-dependent and open-air conditions provided unambiguous chemical assignments. Amine-terminated NDs and folic acid were conjugated using sulfo-NHS/EDC coupling reagents to form amide bonds, confirming that standard amine chemistry remains viable. This work supports that a robust pathway exists to activate a chemically inert diamond surface at room temperature, which broadens the pathways of bond formation when a reactive alkyl-bromide surface is prepared. The unique surface properties of brominated and aminated nanodiamond reported here are impactful to researchers who wish to chemically tune diamond for quantum sensing applications or as an electron source for chemical transformations.

Published
2022
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7. Observing the Evolution of the Universe

Author

James Aguirre, Alexandre Amblard, Amjad Ashoorioon, Carlo Baccigalupi, Amedeo Balbi, Bartlett, J. G., Nicola Bartolo, Dominic Benford, Mark Birkinshaw, Jamie Bock, Dick Bond, Julian Borrill, Franois Bouchet, Michael Bridges, Emory Bunn, Erminia Calabrese, Christopher Cantalupo, Ana Caramete, Carmelita Carbone, Suchetana Chatterjee, Sarah Church, David Chuss, Carlo Contaldi, Asantha Cooray, Sudeep Das, Francesco de Bernardis, Paolo de Bernardis, Gianfranco de Zotti, Delabrouille, J., Xavier Dsert, F., Mark Devlin, Clive Dickinson, Simon Dicker, Matt Dobbs, Scott Dodelson, Olivier Dore, Jessie Dotson, Joanna Dunkley, Maria Cristina Falvella, Dale Fixsen, Pablo Fosalba, Joseph Fowler, Evalyn Gates, Walter Gear, Sunil Golwala, Krzysztof Gorski, Alessandro Gruppuso, Josh Gundersen, Mark Halpern, Shaul Hanany, Masashi Hazumi, Carlos Hernandez-Monteagudo, Mark Hertzberg, Gary Hinshaw, Christopher Hirata, Eric Hivon, Warren Holmes, William Holzapfel, Wayne Hu, Johannes Hubmayr, Kevin Huffenberger, Kent Irwin, Mark Jackson, Andrew Jaffe, Bradley Johnson, William Jones, Manoj Kaplinghat, Brian Keating, Reijo Keskitalo, Justin Khoury, Will Kinney, Theodore Kisner, Lloyd Knox, Alan Kogut, Eiichiro Komatsu, Arthur Kosowsky, John Kovac, Lawrence Krauss, Hannu Kurki-Suonio, Susana Landau, Charles Lawrence, Samuel Leach, Adrian Lee, Erik Leitch, Rodrigo Leonardi, Julien Lesgourgues, Andrew Liddle, Eugene Lim, Michele Limon, Marilena Loverde, Philip Lubin, Antonio Magalhaes, Davide Maino, Tobias Marriage, Victoria Martin, Sabino Matarrese, John Mather, Harsh Mathur, Tomotake Matsumura, Pieter Meerburg, Alessandro Melchiorri, Stephan Meyer, Amber Miller, Michael Milligan, Kavilan Moodley, Michael Neimack, Hogan Nguyen, Dwyer, Ian O., Angiola Orlando, Luca Pagano, Lyman Page, Bruce Partridge, Timothy Pearson, Hiranya Peiris, Francesco Piacentini, Lucio Piccirillo, Elena Pierpaoli, Davide Pietrobon, Giampaolo Pisano, Levon Pogosian, Dmitri Pogosyan, Nicolas Ponthieu, Lucia Popa, Clement Pryke, Christoph Raeth, Subharthi Ray, Christian Reichardt, Sara Ricciardi, Paul Richards, Graca Rocha, Lawrence Rudnick, John Ruhl, Benjamin Rusholme, Claudia Scoccola, Douglas Scott, Carolyn Sealfon, Neelima Sehgal, Michael Seiffert, Leonardo Senatore, Paolo Serra, Sarah Shandera, Meir Shimon, Peter Shirron, Jonathan Sievers, Kris Sigurdson, Joe Silk, Robert Silverberg, Eva Silverstein, Suzanne Staggs, Albert Stebbins, Federico Stivoli, Radek Stompor, Naoshi Sugiyama, Daniel Swetz, Andria Tartari, Max Tegmark, Peter Timbie, Matthieu Tristram, Gregory Tucker, Jon Urrestilla, John Vaillancourt, Veneziani, M., Licia Verde, Joaquin Vieira, Scott Watson, Benjamin Wandelt, Grant Wilson, Edward Wollack, Mark Wyman, Amit Yadav, Giraud-Héraud, Y., Olivier Zahn, Matias Zaldarriaga, Michael Zemcov, Jonathan Zwart, APC - Cosmologie, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), APC - Gravitation (APC-Gravitation), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), and Bartlett, James

Subjects
[SDU.ASTR.CO] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Cosmology and Nongalactic Astrophysics (astro-ph.CO), [PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], [SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astrophysics::Earth and Planetary Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Cosmology and Extragalactic Astrophysics, Astrophysics, Astrophysics::Galaxy Astrophysics, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

How did the universe evolve? The fine angular scale (l>1000) temperature and polarization anisotropies in the CMB are a Rosetta stone for understanding the evolution of the universe. Through detailed measurements one may address everything from the physics of the birth of the universe to the history of star formation and the process by which galaxies formed. One may in addition track the evolution of the dark energy and discover the net neutrino mass. We are at the dawn of a new era in which hundreds of square degrees of sky can be mapped with arcminute resolution and sensitivities measured in microKelvin. Acquiring these data requires the use of special purpose telescopes such as the Atacama Cosmology Telescope (ACT), located in Chile, and the South Pole Telescope (SPT). These new telescopes are outfitted with a new generation of custom mm-wave kilo-pixel arrays. Additional instruments are in the planning stages., Science White Paper submitted to the US Astro2010 Decadal Survey. Full list of 177 author available at http://cmbpol.uchicago.edu

Published
2009

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