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Articles 1 - 28 of 28
Full-Text Articles in Physics
Migmatite Gneiss Of The Jættedal Complex, Liverpool Land, East Greenland: Protracted High-T Metamorphism In The Overriding Plate Of The Caledonian Orogen, S. M. Johnston, A. Kylander-Clark, H. K. Brueckner
Migmatite Gneiss Of The Jættedal Complex, Liverpool Land, East Greenland: Protracted High-T Metamorphism In The Overriding Plate Of The Caledonian Orogen, S. M. Johnston, A. Kylander-Clark, H. K. Brueckner
Physics
The Greenland Caledonides (GC) formed in the overriding Laurentian plate during the closure of the Iapetus Ocean and the subduction of Baltica, and offer a unique opportunity to study metamorphic patterns, regional structures and the kinematic evolution of the overriding plate of a continental collision. We present new metamorphic petrology and coupled zircon geochronology and geochemistry data from the Jættedal complex in southern Liverpool Land to document the thermal evolution of the orogenic core of the southern GC. Pelitic migmatite gneisses from the Jættedal complex document metamorphic conditions of 850–730 °C at pressures of 11–9.5 kbar. Zircon from these samples …
The Muse View Of Qso Pg 1307+085: An Elliptical Galaxy On The MBh–Σ* Relation Interacting With Its Group Environment, Bernd Husemann, Vardha Nicola Bennert, Julia Scharwächter, J.-H. Woo, O. S. Choundhury
The Muse View Of Qso Pg 1307+085: An Elliptical Galaxy On The MBh–Σ* Relation Interacting With Its Group Environment, Bernd Husemann, Vardha Nicola Bennert, Julia Scharwächter, J.-H. Woo, O. S. Choundhury
Physics
We report deep optical integral-field spectroscopy with the Multi-Unit Spectroscopic Explorer (MUSE) at the Very Large Telescope of the luminous radio-quiet quasi-stellar object (QSO) PG 1307+085 obtained during commissioning. Given the high sensitivity and spatial resolution delivered by MUSE, we are able to resolve the compact (re ∼ 1.3 arcsec) elliptical host galaxy. After spectroscopic deblending of the QSO and host galaxy emission, we infer a stellar velocity dispersion of σ* = 155 ± 19 km s−1. This places PG 1307+085 on the local MBH–σ* relation within its intrinsic scatter but offset …
Low Intensity Gamma-Ray Spectroscopy Of The Lake Labyrinth Meteorite, Tristan C. Paul
Low Intensity Gamma-Ray Spectroscopy Of The Lake Labyrinth Meteorite, Tristan C. Paul
Physics
A 23.7g fragment of the Lake Labyrinth Meteorite (fell in 1924, collected in 1934 at Lake Labyrinth in South Australia, Australia) was re-investigated for evidence of the presence of 98Tc using a two dimensional low-intensity gamma-ray spectrometer. A new calibration technique using 26Al sources found the gamma-rays previously thought to be due to 98Tc are more likely from 166Ho. The presence of 166Ho is most likely due to activation of the stable 165Ho in the meteorite from terrestrial background sources where it was stored.
Thermodynamic Effects Of A Local Bell State Projection Interaction In A One-Dimensional Dynamic Spin System, Nickolas H. Pilgram
Thermodynamic Effects Of A Local Bell State Projection Interaction In A One-Dimensional Dynamic Spin System, Nickolas H. Pilgram
Physics
No abstract provided.
Simulations Of Hl-Lhc Crab Cavity Noise Using Headtail, Stanley Steeper
Simulations Of Hl-Lhc Crab Cavity Noise Using Headtail, Stanley Steeper
Physics
The High Luminosity Large Hadron Collider (Hi-Lumi LHC) upgrade -- scheduled to be completed by 2025 -- will improve the existing LHC in many ways. One such upgrade is the addition of Crab Cavities (CCs). The CCs are resonant structures that provide strong transverse kicks to the circulating clouds of particles around each interaction region. As such, the CCs result in a head-on collision of the clouds and a large increase in event rate, leading to reduced statistical uncertainty and potentially faster discoveries. However, the CC field will be modulated by phase and amplitude noise which can have detrimental effects …
A Local Baseline Of The Black Hole Mass Scaling Relations For Active Galaxies. Iii. The Mbh-Σ Relation, Vardha Nicola Bennert, Tommaso Treu, Matthew W. Auger, Maren Cosens, Daeseong Park, Rebecca Rosen, Chelsea E. Harris, Matthew A. Malkan, Jong-Hak Woo
A Local Baseline Of The Black Hole Mass Scaling Relations For Active Galaxies. Iii. The Mbh-Σ Relation, Vardha Nicola Bennert, Tommaso Treu, Matthew W. Auger, Maren Cosens, Daeseong Park, Rebecca Rosen, Chelsea E. Harris, Matthew A. Malkan, Jong-Hak Woo
Physics
We create a baseline of the black hole (BH) mass ()—stellar-velocity dispersion (σ) relation for active galaxies, using a sample of 66 local () Seyfert-1 galaxies, selected from the Sloan Digital Sky Survey (SDSS). Analysis of SDSS images yields AGN luminosities free of host-galaxy contamination, and morphological classification. 51/66 galaxies have spiral morphology. Out of these, 28 bulges have Sérsic index and are considered candidate pseudo-bulges, with eight being definite pseudo-bulges based on multiple classification criteria met. Only 4/66 galaxies show signs of interaction/merging. High signal-to-noise ratio Keck spectra provide the width of the broad Hβ emission …
Yielding And Microstructure In A 2d Jammed Material Under Shear Deformation, Nathan C, Keim, Paulo E. Arratia
Yielding And Microstructure In A 2d Jammed Material Under Shear Deformation, Nathan C, Keim, Paulo E. Arratia
Physics
The question of how a disordered material's microstructure translates into macroscopic mechanical response is central to understanding and designing materials like pastes, foams and metallic glasses. Here, we examine a 2D soft jammed material under cyclic shear, imaging the structure of ∼5 × 104 particles. Below a certain strain amplitude, the structure becomes conserved at long times, while above, it continually rearranges. We identify the boundary between these regimes as a yield strain, defined without rheological measurement. Its value is consistent with a simultaneous but independent measurement of yielding by stress-controlled bulk rheometry. While there are virtually no irreversible …
A Lego® Brewster Angle Microscope For Quantitative Monolayer Film Analysis, Nicholas Benz
A Lego® Brewster Angle Microscope For Quantitative Monolayer Film Analysis, Nicholas Benz
Physics
In order to study single-molecule thick films and their phase behavior we built a Brewster Angle Microscope (BAM). BAM’s are inherently expensive due to their accuracy and precision. We built a fully functional BAM using Lego® Mindstorm® kits for the fraction of the price of a commercial BAM. And by utilizing the 10µm patented Lego® tolerance, comparable accuracy was attained. The BAM was mounted to a Langmuir-trough and will be used for laboratory experiments for optics and physical chemistry along with research on lung surfactant and on liquid crystals.
Transient Reflectance Of Photoexcited Cd3As2, Christopher P. Weber, Ernest Arushanov, Bryan S. Berggren, Tahereh Hosseini, Nikolai Kouklin, Alex Nateprov
Transient Reflectance Of Photoexcited Cd3As2, Christopher P. Weber, Ernest Arushanov, Bryan S. Berggren, Tahereh Hosseini, Nikolai Kouklin, Alex Nateprov
Physics
We report ultrafast transient-grating measurements of crystals of the three-dimensional Dirac semimetal cadmium arsenide, Cd3As2, at both room temperature and 80 K. After photoexcitation with 1.5-eV photons, charge-carriers relax by two processes, one of duration 500 fs and the other of duration 3.1 ps. By measuring the complex phase of the change in reflectance, we determine that the faster signal corresponds to a decrease in absorption, and the slower signal to a decrease in the light's phase velocity, at the probe energy. We attribute these signals to electrons' filling of phase space, first near the photon …
Transition Orbits Of Walking Droplets, Joshua Parker
Transition Orbits Of Walking Droplets, Joshua Parker
Physics
It was recently discovered that millimeter-sized droplets bouncing on the surface of an oscillating bath of the same fluid can couple with the surface waves it produces and begin walking across the fluid bath. These walkers have been shown to behave similarly to quantum particles; a few examples include single-particle diffraction, tunneling, and quantized orbits. Such behavior occurs because the drop and surface waves depend on each other to exist, making this the first and only known macroscopic pilot-wave system. In this paper, the quantized orbits between two identical drops are explored. By sending a perturbation to a pair of …
Critical Point Pairs For Smectic-A* - Smectic-C* Phase Transitions., Ted Cassirer
Critical Point Pairs For Smectic-A* - Smectic-C* Phase Transitions., Ted Cassirer
Physics
Liquid crystals is a class of materials possessing properties from both solids and fluids. Similar to solids the molecules arrange themselves in some sort of order. In the liquid crystal state there are multiple phases, smectic being one of them. In a smectic liquid crystal the molecules are aranged (along $z$) in layers. Of the smectic liquid crystals there exists different phases. In the smectic-A (Sm-A) phase the avarage tilt is $0$ relative to $z$ and in the Smectic-C (Sm-A) phase the avarage tilt is non-zero relative to $z$. Normally the liquid crystal will transition between the two phases by …
Saddle Force Mapping, Molly Totten
Saddle Force Mapping, Molly Totten
Physics
In horseback riding, the size and shape of a saddle can drastically effect the comfort, attitude and performance of the horse as well as the effectiveness of the rider. In an effort to create an accurate means of fitting the saddle to the horse, I have created a pressure sensing device that maps the force differences along critical areas of the horse's back during motion. Using an Arduino microprocessor and appropriate circuits, data was collected about the pressure levels between the saddle and the horse's back and a graphic representation of the findings was created.
Frequency Of Seyfert Type Transitions In A Sample Of 102 Local Active Galactic Nuclei, Jordan Runco
Frequency Of Seyfert Type Transitions In A Sample Of 102 Local Active Galactic Nuclei, Jordan Runco
Physics
A sample of ∼100 type-1 local (0.02 ≤ z ≤ 0.1) active galaxies (AGNs) was selected from the Sloan Digital Sky Survey with black hole masses MBH > 107 Mʘ and re-observed using the Keck 10-m telescope to study the local scaling relations between MBH and the host galaxy properties. As a side product, the data provides insight into any changes of the broad-line region within the 3-9 year time-frame covered by the two sets of spectra. The variability of the broad Hβ emission line is of particular interest to us, not only because it is used …
Cuore Image Analysis And Cuore-0 Shifting: A Contribution To The Search For Neutrinoless Double Beta Decay, Dakota Christopher Rose
Cuore Image Analysis And Cuore-0 Shifting: A Contribution To The Search For Neutrinoless Double Beta Decay, Dakota Christopher Rose
Physics
In an effort to aid in the work of the Cryogenic Underground Observatory of Rare Events (CUORE) in moving towards confirming the existence of Neutrinoless Double Beta Decay, a six week trip was made to Assergi, Italy to work as an Onsite Shifter for the previous generation of the experiment, CUORE-0, as well as to aid in construction of the full CUORE detector. Furthermore, to help in understanding possible sources of experimental error, work was done analyzing images taken of the glue spots on the faces of each Tellurium Oxide detector crystals (also containing the source of the decay, Tellurium-130). …
The Van Der Pol Oscillator As A Model Of The Hair Cell Auditory Response: A Numerical Study, Thomas Yocono
The Van Der Pol Oscillator As A Model Of The Hair Cell Auditory Response: A Numerical Study, Thomas Yocono
Physics
Hair cells, which detect and encode sound stimuli, have been shown to have a non-linear response and self sustaining oscillations. Here, we look at the Van der Pol oscillator, which has these properties, and numerically calculate its response to multiple driving frequencies. Any nonlinear system's response to multiple driving frequencies will have not just the driving frequencies present, but also combination tones, or heterodyne frequencies, which have order defined by the number of driving frequency combinations. This phenomenon has been experimentally confirmed in the human auditory response [1]. In the frequency specture of the Van der Pol steady state response …
Hst Imaging Of Fading Agn Candidates. I. Host-Galaxy Properties And Origin Of The Extended Gas*, William Keel, W. Peter Maksym, Vardha Nicola Bennert, Chris J. Lintott, S. Drew Chojnowski, Alexei Moiseev, Aleksandrina Smirnova, Kevin Schawinski, C. Megan Urry, Daniel A. Evans
Hst Imaging Of Fading Agn Candidates. I. Host-Galaxy Properties And Origin Of The Extended Gas*, William Keel, W. Peter Maksym, Vardha Nicola Bennert, Chris J. Lintott, S. Drew Chojnowski, Alexei Moiseev, Aleksandrina Smirnova, Kevin Schawinski, C. Megan Urry, Daniel A. Evans
Physics
We present narrow- and medium-band Hubble Space Telescope imaging, with additional supporting ground-based imaging, spectrophotometry, and Fabry–Perot interferometric data, for eight galaxies identified as hosting a fading active galactic nucleus (AGN). These are selected to have AGN-ionized gas projected kpc from the nucleus and energy budgets with a significant shortfall of ionizing radiation between the requirement to ionize the distant gas and the AGN as observed directly, indicating fading of the AGN on ≈50,000 yr timescales. This paper focuses on the host-galaxy properties and origin of the gas. In every galaxy, we identify evidence of ongoing or past interactions, including …
The Lick Agn Monitoring Project 2011: Spectroscopic Campaign And Emission-Line Light Curves, Aaron J. Barth, Vardha N. Bennert, Gabriela Canalizo, Alexei V. Filippenko, Elinor L. Gates, Jenny E. Greene, Weidong Li, Matthew A. Malkan, Anna Pancoast, David J. Sand, Daniel Stern, Tommaso Treu, Jong-Hak Woo, Roberto J. Assef, Hyun-Jin Bae, Brendon J. Brewer, S. Bradley Cenko, Kelsey I. Clubb, Michael C. Cooper, Aleksandar M. Diamond-Stanic, Kyle D. Hiner, Sebastian F. Honig, Eric Hsiao, Michael T. Kandrashoff, Mariana S. Lazarova, A.M. Nierenberg, Jacob Rex, Jeffrey M. Silverman, Erik J. Tollerud, Jonelle L. Walsh
The Lick Agn Monitoring Project 2011: Spectroscopic Campaign And Emission-Line Light Curves, Aaron J. Barth, Vardha N. Bennert, Gabriela Canalizo, Alexei V. Filippenko, Elinor L. Gates, Jenny E. Greene, Weidong Li, Matthew A. Malkan, Anna Pancoast, David J. Sand, Daniel Stern, Tommaso Treu, Jong-Hak Woo, Roberto J. Assef, Hyun-Jin Bae, Brendon J. Brewer, S. Bradley Cenko, Kelsey I. Clubb, Michael C. Cooper, Aleksandar M. Diamond-Stanic, Kyle D. Hiner, Sebastian F. Honig, Eric Hsiao, Michael T. Kandrashoff, Mariana S. Lazarova, A.M. Nierenberg, Jacob Rex, Jeffrey M. Silverman, Erik J. Tollerud, Jonelle L. Walsh
Physics
In the Spring of 2011 we carried out a 2.5 month reverberation mapping campaign using the 3 m Shane telescope at Lick Observatory, monitoring 15 low-redshift Seyfert 1 galaxies. This paper describes the observations, reductions and measurements, and data products from the spectroscopic campaign. The reduced spectra were fitted with a multicomponent model in order to isolate the contributions of various continuum and emission-line components. We present light curves of broad emission lines and the active galactic nucleus (AGN) continuum, and measurements of the broad Hβ line widths in mean and rms spectra. For the most highly variable AGNs we …
Neutrinoless Double-Beta Decay Search With Cuore And Cuore-0 Experiments, N. Moggi, D.R. Artusa, F. T. Avignone Iii, O. Azzolini, M Balata, T.I. Banks, G. Bari, J. Beeman, F. Bellini, A. Bersani, M. Biassoni, C. Brofferio, C. Bucci, X. Z. Cai, A. Camacho, A. Caminata, L. Canonica, X.G. Cao, S Capelli, L. Capelli, L. Carbone, L. Cardani, N. Casali, L. Cassina, D. Chiesa, N. Chott, M Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R.J. Creswick, J.S. Cushman, I. Dafinei, A. Dally, V. Datskov, S. Dell'oro, M. M. Deninno, S Di Domizio, M.L. Di Vacri, A. Drobizhev, L. Ejzak, D.Q. Fang, H.A. Farach, M. Faverzani, G. Fernandes, E. Ferri, F. Ferroni, E. Fiorini, M.A. Franceschi, S.J. Freedman, B.K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, Thomas D. Gutierrez, E.E. Haller, K. Han, K.M. Heeger, R. Hennings-Yeomans, K.P. Hickerson, H. Z. Huang, R. Kadel, G. Keppel, Yu. G. Kolomensky, Y. L. Li, C. Ligi, K.E. Lim, X Liu, Y. G. Ma, C. Maiano, M. Maino, M. Martinez, R.H. Maruyama, Y. Mei, S. Morganti, T. Napolitano, S. Nisi, C. Nones, E.B. Norman, A. Nucciotti, T. O'Donnell, F. Orio, D. Orlandi, J.L. Ouellet, C.E. Pagliarone, M Pallavicini, M. Pallavicini, V. Palmieri, L. Pattavina, M Pavan, G Pessina, V. Pettinacci, G. Piperno, C. Pira, S Pirro, S. Pozzi, E Previtali, C. Rosenfeld, C. Rusconi, E. Sala, S Sangiorgio, D. Santone, N.D. Scielzo, M Sisti, A. R. Smith, L. Taffarello, M. Tenconi, F. Terranova, W.D. Tian, C. Tomei, S. Trentalange, G. Ventura, M Vignati, B. S. Wang, H. W. Wang, L. Wielgus, J. Wilson, L.A. Winslow, T. Wise, A. Woodcraft, L Zanotti, C. Zarra, G. Q. Zhang, B. X. Zhu, S. Zucchelli
Neutrinoless Double-Beta Decay Search With Cuore And Cuore-0 Experiments, N. Moggi, D.R. Artusa, F. T. Avignone Iii, O. Azzolini, M Balata, T.I. Banks, G. Bari, J. Beeman, F. Bellini, A. Bersani, M. Biassoni, C. Brofferio, C. Bucci, X. Z. Cai, A. Camacho, A. Caminata, L. Canonica, X.G. Cao, S Capelli, L. Capelli, L. Carbone, L. Cardani, N. Casali, L. Cassina, D. Chiesa, N. Chott, M Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R.J. Creswick, J.S. Cushman, I. Dafinei, A. Dally, V. Datskov, S. Dell'oro, M. M. Deninno, S Di Domizio, M.L. Di Vacri, A. Drobizhev, L. Ejzak, D.Q. Fang, H.A. Farach, M. Faverzani, G. Fernandes, E. Ferri, F. Ferroni, E. Fiorini, M.A. Franceschi, S.J. Freedman, B.K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, P. Gorla, C. Gotti, Thomas D. Gutierrez, E.E. Haller, K. Han, K.M. Heeger, R. Hennings-Yeomans, K.P. Hickerson, H. Z. Huang, R. Kadel, G. Keppel, Yu. G. Kolomensky, Y. L. Li, C. Ligi, K.E. Lim, X Liu, Y. G. Ma, C. Maiano, M. Maino, M. Martinez, R.H. Maruyama, Y. Mei, S. Morganti, T. Napolitano, S. Nisi, C. Nones, E.B. Norman, A. Nucciotti, T. O'Donnell, F. Orio, D. Orlandi, J.L. Ouellet, C.E. Pagliarone, M Pallavicini, M. Pallavicini, V. Palmieri, L. Pattavina, M Pavan, G Pessina, V. Pettinacci, G. Piperno, C. Pira, S Pirro, S. Pozzi, E Previtali, C. Rosenfeld, C. Rusconi, E. Sala, S Sangiorgio, D. Santone, N.D. Scielzo, M Sisti, A. R. Smith, L. Taffarello, M. Tenconi, F. Terranova, W.D. Tian, C. Tomei, S. Trentalange, G. Ventura, M Vignati, B. S. Wang, H. W. Wang, L. Wielgus, J. Wilson, L.A. Winslow, T. Wise, A. Woodcraft, L Zanotti, C. Zarra, G. Q. Zhang, B. X. Zhu, S. Zucchelli
Physics
The Cryogenic Underground Observatory for Rare Events (CUORE) is an upcoming experiment designed to search for the neutrinoless double-beta decays. Observation of the process would unambiguously establish that neutrinos are Majorana particles and provide information on their absolute mass scale hierarchy. CUORE is now under construction and will consist of an array of 988 TeO2 crystal bolometers operated at 10 mK, but the first tower (CUORE-0) is already taking data. The experimental techniques used will be presented as well as the preliminary CUORE-0 results. The current status of the full-mass experiment and its expected sensitivity will then be discussed.
Fission Fragment Tracking And Identification In The Neutron-Induced Fission Fragment Tracking Experiment’S Time Projection Chamber, Eric Song
Physics
The Neutron-Induced Fission Fragment Tracking Experiment (NIFFTE) built a novel Time Projection Chamber (TPC), the FissionTPC, for measuring neutron-induced fission cross-sections to unprecedented precision. We investigated data from a 2014 run (400010151) at the Los Alamos Neutron Science Center (LANSCE) with a double-sided U235/Pu239 target. Our particle identification studies will aid in the development of improved tracking algorithms.
Correlations In Intensity Fluctuations From A Quasi-Thermal Light Source: An Application Of Hanbury Brown & Twiss, Christopher Watanabe
Correlations In Intensity Fluctuations From A Quasi-Thermal Light Source: An Application Of Hanbury Brown & Twiss, Christopher Watanabe
Physics
In this experiment, the observation by Hanbury Brown and Twiss that light intensity fluctuations from an extended broadband source are spatially correlated is demonstrated with a quasi-thermal light source. Laser light is used to illuminate a ground glass screen and generate a diffraction pattern, also known as a speckle pattern. The speckle pattern is recorded using an electronic camera and analyzed. Calculated auto-correlations of the intensity fluctuations agree with theoretical results originating from speckle analysis.
Simulation Of Light Scattering From Brownian Particles, Raymond Mullen
Simulation Of Light Scattering From Brownian Particles, Raymond Mullen
Physics
This project is a computational exploration of the light scattering from Brownian particles. We simulate laser light scattering to produce fluctuating light intensity at a detector located in the far-field. By analyzing the statistical properties of this intensity fluctuation, and knowing physical parameters of the system, we can deduce the size of the scattering particles. The computer simulation is in excellent agreement with theory.
An Extremum Principle For Charged Black Holes, Shaker Von Price Funkhouser
An Extremum Principle For Charged Black Holes, Shaker Von Price Funkhouser
Physics
There is a well known static condition that characterizes how two or more charged black holes stay in place: this condition is |qi |=mi , where a black hole (labeled by i) has electric charge qi and mass mi . For nearly half a century, this static condition has eluded a simple physical interpretation, without appealing to forces. I provide the first proof that the static condition, |qi |=mi , corresponds to an extremum of the black holes’ total energy. My approach uses geometry and calculus in the context of general relativity. For the non-specialist, this work draws upon one’s …
Cosmic Evolution Of Black Holes And Spheroids. V. The Relation Between Black Hole Mass And Host Galaxy Luminosity For A Sample Of 79 Active Galaxies, Daeseong Park, Jong-Hak Woo, Vardha N. Bennert, Tommaso Treu, Matthew W. Auger, Matthew A. Malkan
Cosmic Evolution Of Black Holes And Spheroids. V. The Relation Between Black Hole Mass And Host Galaxy Luminosity For A Sample Of 79 Active Galaxies, Daeseong Park, Jong-Hak Woo, Vardha N. Bennert, Tommaso Treu, Matthew W. Auger, Matthew A. Malkan
Physics
We investigate the cosmic evolution of the black hole (BH) mass–bulge luminosity relation using a sample of 52 active galaxies at z ∼ 0.36 and z ∼ 0.57 in the BH mass range of 107.4–109.1 M0. By consistently applying multicomponent spectral and structural decomposition to high-quality Keck spectra and high-resolution Hubble Space Telescope images, BH masses (MBH) are estimated using the Hβ broad emission line combined with the 5100 Å nuclear luminosity, and bulge luminosities (Lbul ) are derived from surface photometry. Comparing the resulting MBH − Lbul relation to local active galaxies and taking into account selection effects, we …
Role Of Disorder In Finite-Amplitude Shear Of A 2d Jammed Material, Nathan C. Keim, Paulo E. Arratia
Role Of Disorder In Finite-Amplitude Shear Of A 2d Jammed Material, Nathan C. Keim, Paulo E. Arratia
Physics
A material’s response to small but finite deformations can reveal the roots of its response to much larger deformations. Here, we identify commonalities in the responses of 2D soft jammed solids with different amounts of disorder. We cyclically shear the materials while tracking their constituent particles, in experiments that feature a stable population of repeated structural relaxations. Using bidisperse particle sizes creates a more amorphous material, while monodisperse sizes yield a more polycrystalline one. We find that the materials’ responses are very similar, both at the macroscopic, mechanical level and in the microscopic motions of individual particles. However, both locally …
Searching For Neutrinoless Double-Beta Decay Of 130te With Cuore, D.R. Artusa, F.T. Avignone Iii, O. Azzolini, M. Balata, T.I. Banks, G. Bari, J. Beeman, F. Bellini, A. Bersani, M. Biassoni, C. Brofferio, C. Bucci, X.Z. Cai, A. Camacho, L. Canonica, X.G. Cao, S. Capelli, L. Carbone, L. Cardani, M. Carrettoni, N. Casali, D. Chiesa, N. Chott, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R.J. Creswick, I. Dafinei, A. Dally, V. Datskov, A. De Biasi, M.M. Deninno, S. Di Domizio, M.L. Di Vacri, L. Ejzak, D.Q Fang, H.A. Farach, M. Faverzani, G. Fernandes, E. Ferri, F. Ferroni, E. Fiorini, M.A. Franceschi, S.J. Freedman, B.K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, J. Goett, P. Gorla, C. Gotti, T.D. Gutierrez, E.E. Haller, K. Han, K.M. Heeger, R. Hennings-Yeomans, H.Z. Huang, R. Kadel, K. Kazkaz, G. Keppel, Yu. G. Kolomensky, Y.L. Li, C. Ligi, X. Liu, Y.G. Ma, C. Maiano, M. Maino, M. Martinez, R.H. Maruyama, Y. Mei, N. Moggi, S. Morganti, T. Napolitano, S. Nisi, C. Nones, E.B. Norman, A. Nucciotti, T. O'Donnell, F. Orio, D. Orlandi, J.L. Ouellet, M. Pallavicini, V. Palmieri, L. Pattavina, M. Pavan, M. Pedretti, G. Pessina, V. Pettinacci, G. Piperno, C. Pira, S. Pirro, E. Previtali, V. Rampazzo, C. Rosenfeld, C. Rusconi, E. Sala, S. Sangiorgio, N.D. Scielzo, M. Sisti, A.R. Smith, L. Taffarello, M. Tenconi, F. Terranova, W.D. Tian, C. Tomei, S. Trentalange, G. Ventura, M. Vignati, B.S. Wang, H.W. Wang, L. Wielgus, J. Wilson, L.A. Winslow, T. Wise, A. Woodcraft, L. Zanotti, C. Zarra, B.X. Zhu, S. Zucchelli
Searching For Neutrinoless Double-Beta Decay Of 130te With Cuore, D.R. Artusa, F.T. Avignone Iii, O. Azzolini, M. Balata, T.I. Banks, G. Bari, J. Beeman, F. Bellini, A. Bersani, M. Biassoni, C. Brofferio, C. Bucci, X.Z. Cai, A. Camacho, L. Canonica, X.G. Cao, S. Capelli, L. Carbone, L. Cardani, M. Carrettoni, N. Casali, D. Chiesa, N. Chott, M. Clemenza, S. Copello, C. Cosmelli, O. Cremonesi, R.J. Creswick, I. Dafinei, A. Dally, V. Datskov, A. De Biasi, M.M. Deninno, S. Di Domizio, M.L. Di Vacri, L. Ejzak, D.Q Fang, H.A. Farach, M. Faverzani, G. Fernandes, E. Ferri, F. Ferroni, E. Fiorini, M.A. Franceschi, S.J. Freedman, B.K. Fujikawa, A. Giachero, L. Gironi, A. Giuliani, J. Goett, P. Gorla, C. Gotti, T.D. Gutierrez, E.E. Haller, K. Han, K.M. Heeger, R. Hennings-Yeomans, H.Z. Huang, R. Kadel, K. Kazkaz, G. Keppel, Yu. G. Kolomensky, Y.L. Li, C. Ligi, X. Liu, Y.G. Ma, C. Maiano, M. Maino, M. Martinez, R.H. Maruyama, Y. Mei, N. Moggi, S. Morganti, T. Napolitano, S. Nisi, C. Nones, E.B. Norman, A. Nucciotti, T. O'Donnell, F. Orio, D. Orlandi, J.L. Ouellet, M. Pallavicini, V. Palmieri, L. Pattavina, M. Pavan, M. Pedretti, G. Pessina, V. Pettinacci, G. Piperno, C. Pira, S. Pirro, E. Previtali, V. Rampazzo, C. Rosenfeld, C. Rusconi, E. Sala, S. Sangiorgio, N.D. Scielzo, M. Sisti, A.R. Smith, L. Taffarello, M. Tenconi, F. Terranova, W.D. Tian, C. Tomei, S. Trentalange, G. Ventura, M. Vignati, B.S. Wang, H.W. Wang, L. Wielgus, J. Wilson, L.A. Winslow, T. Wise, A. Woodcraft, L. Zanotti, C. Zarra, B.X. Zhu, S. Zucchelli
Physics
Neutrinoless double-beta (0νββ) decay is a hypothesized lepton-number-violating process that offers the only known means of asserting the possible Majorana nature of neutrino mass. The Cryogenic Underground Observatory for Rare Events (CUORE) is an upcoming experiment designed to search for 0νββ decay of 130Te using an array of 988 TeO2 crystal bolometers operated at 10 mK. The detector will contain 206 kg of 130Te and have an average energy resolution of 5 keV; the projected 0νββ decay half-life sensitivity after five years of livetime is 1.6 × 1026 y at 1σ (9.5 × 1025 y at the 90% confidence level), …
Characterizing Double And Triple Laser Beam Interference Patterns In The Context Of Trapping Atoms For Quantum Computing, Ian E. Powell
Characterizing Double And Triple Laser Beam Interference Patterns In The Context Of Trapping Atoms For Quantum Computing, Ian E. Powell
Physics
We propose two optical neutral atom traps for quantum computing involving the intersection of two or three laser beams. We simulate both the intensity and the potential energy of the interference pattern. From these simulations we create animations of how the potential energy and intensity change with varying angles of separation between the laser beams in the system. We parameterize lines through our interference pattern and fit simple harmonic oscillator potential energies to the potential energy wells calculated to characterize our interference pattern’s atom trapping capabilities. Finally, we investigate a possible quantum entanglement routine by observing how the geometry of …
Radar Absorption, Basal Reflection, Thickness And Polarization Measurements From The Ross Ice Shelf, Antarctica, Jordan C. Hanson, Steven W. Barwick, Eric C. Berg, Dave Z. Besson, Thorin J. Duffin, Spencer R. Klein, Stuart A. Kleinfelder, Corey Reed, Mahshid Roumi, Thorsten Stezelberger, Joulien Tatar, James A. Walker, Liang Zou
Radar Absorption, Basal Reflection, Thickness And Polarization Measurements From The Ross Ice Shelf, Antarctica, Jordan C. Hanson, Steven W. Barwick, Eric C. Berg, Dave Z. Besson, Thorin J. Duffin, Spencer R. Klein, Stuart A. Kleinfelder, Corey Reed, Mahshid Roumi, Thorsten Stezelberger, Joulien Tatar, James A. Walker, Liang Zou
Physics
Radio-glaciological parameters from the Moore’s Bay region of the Ross Ice Shelf, Antarctica, have been measured. The thickness of the ice shelf in Moore’s Bay was measured from reflection times of radio-frequency pulses propagating vertically through the shelf and reflecting from the ocean, and is found to be 576 ± 8 m. Introducing a baseline of 543 ± 7m between radio transmitter and receiver allowed the computation of the basal reflection coefficient, R, separately from englacial loss. The depth-averaged attenuation length of the ice column, 〈L〉 is shown to depend linearly on frequency. The best fit (95% confidence level) is …
Confocal Sputtering Of Conformal Α-Β Phase W Films On Etched Al Features, John Mark Kreikebaum, Blas Cabrera, Jeffrey J. Yen, Paul L. Brink, Matt Cherry, Astrid Tomada, Betty A. Young
Confocal Sputtering Of Conformal Α-Β Phase W Films On Etched Al Features, John Mark Kreikebaum, Blas Cabrera, Jeffrey J. Yen, Paul L. Brink, Matt Cherry, Astrid Tomada, Betty A. Young
Physics
The authors report on thin-film processing improvements in the fabrication of superconducting quasiparticle-trap-assisted electrothermal-feedback transition-edge sensors used in the design of cryogenic dark matter search detectors. The work was performed as part of a detector upgrade project that included optimization of a new confocal sputtering system and development of etch recipes compatible with patterning 40 nm-thick, α-β mixed-phase W films deposited on 300–600 nm-thick, patterned Al. The authors found that their standard exothermic Al wet etch recipes provided inadequate W/Al interfaces and led to poor device performance. The authors developed a modified Al wet-etch recipe that effectively mitigates geometrical step-coverage …