Category: News

Douglas Banyai Research

Doug Banyai Computer Model
Computer model of a nanoparticle based transistor. The conduction channel consists of a disordered array of nanoparticles. This model is used with the finite element method to investigate capacitances.

Mutli-scale modeling of nanoparticle based transistors

For half a century the integrated circuits (ICs) that make up the heart of electronic devices have been steadily improving by shrinking at an exponential rate. However, as the current crop of ICs get smaller and the insulating layers involved become thinner, electrons leak through due to quantum mechanical tunneling. This is one of several issues which will bring an end to the party, after which future improvements will have to come from employing fundamentally different transistor architecture rather than fine tuning and miniaturizing the field effect transistors in use today.

Several new transistor designs, some designed and built here at Tech, involve electrons tunneling their way through arrays of nanoparticles. We use a multi-scale approach to model these devices and study their behavior. For the smallest details of how often electrons jump from one particular nanoparticle to another, we use a first principles approach (density functional theory) to study the quantum mechanics involved. To estimate the change in energy due to the movement of a single electron, we use the finite element method to calculate electrostatic capacitances. The kinetic Monte Carlo method allows us to use our knowledge of these details to simulate an entire device — sometimes consisting of hundreds of individual particles — and watch as a device ‘turns on’ and starts conducting an electric current. Finally, we are developing new algorithms that will allow us to simulate the collective behavior of thousands of devices.

This work is ongoing under the advisement of Dr. John Jaszczak, in collaboration with the research groups of Dr. Pandey, Dr. Bergstrom, and Dr. Yap, and with support from the Miles fellowship.

Doug Banyai 2 Clusters
Model of of two gold nanoparticles at atomic resolution. This model is used to investigate tunneling between nanoparticles.

Ravi Joshi Research

Ravi Joshi
Ravi Joshi

How would negative energy density affect a classic Friedmann cosmology? Although never measured and possibly unphysical, the evolution of a universe containing a significant cosmological abundance of any of a number of hypothetical stable negative energy components is explored. These negative energy (Omega < 0) forms include negative phantom energy (w<-1), negative cosmological constant w=-1, negative domain walls w=-2/3, negative cosmic strings (w=-1/3), negative mass w=0, negative radiation (w=1/3), and negative ultra light (w > 1/3). Assuming that such universe components generate pressures as perfect fluids, the attractive or repulsive nature of each negative energy component is reviewed.

The Friedmann equations can only be balanced when negative energies are coupled to a greater magnitude of positive energy or positive curvature, and minimal cases of both of these are reviewed. The future and fate of such universes in terms of curvature, temperature, acceleration, and energy density are reviewed including endings categorized as a Big Crunch, Big Void, or Big Rip and further qualified as “Warped”, “Curved”, or “Flat”, “Hot” versus “Cold”, “Accelerating” versus “Decelerating” versus “Coasting”. A universe that ends by contracting to zero energy density is termed a Big Poof. Which contracting universes “bounce” in expansion and which expanding universes “turnover” and contract are also reviewed.

Hao Zhou Research

HAWC Experiment
Figure 1: The HAWC experiment as of July 26, 2013. The full array will cover the whole plane in the center of the picture.

I am working with Dr. Petra Huentemeyer on the HAWC (short for High Altitude Water Cherenkov) experiment, a very high energy (VHE) gamma-ray observatory currently being built in Mexico. In contrast to optical or radio waves, gamma-ray photons cannot penetrate the Earth’s atmosphere. Instead they collide with particles in the atmosphere and create showers of secondary particles through electromagnetic and hadronic interactions. Once completed the HAWC experiment will consist of 300 water Cherenkov detectors (WCDs), that will measure these secondary particles as they sweep through the array. The directions of the primary gamma-ray photons are reconstructed using the time between the signals in each WCD. Thus timing calibration, which is what I am currently working on, is crucial for good angular resolution. As of now, more than one third of the array is finished and operational. At the moment, I am doing a preliminary analysis of data collected with this sub-array. Figure 1 shows a picture of HAWC on July 26, 2013. My research is focusing on pulsar wind nebulae (PWNe), the largest class of galactic VHE gamma-ray sources. PWNe produce electromagnetic radiation in a very broad energy range from radio to VHE gamma rays, and thereby provide an excellent laboratory to study the physical processes at very high energy. Figure 2 shows the crab nebula at different wavelengths. Using data collected with the complete HAWC array, I will reconstruct the energy spectrum of gamma rays emitted by PWNe. I will combine my analysis results with data from other experiments that take measurements at lower energies, to reveal the physics processes occurring in PWNe.

by Hao Zhou

Crab Nebula
Figure 2: Crab nebula in radio (red), optical (green) and X-ray (blue) from APOD (Astronomy Picture of the Day) on September 20, 2002. Credit: J. Hester (ASU), CXC, HST, NRAO, NSF, NASA

SURF Presentations August 12 and 13, 2013

Recipients of Summer Undergraduate Research Fellowships (SURFs) will present end-of-summer project updates Monday and Tuesday (Aug. 12 and 13), from 9 to 11 a.m., in Fisher 139.

From Tech Today.

SURF award recipients in physics include:

Joseph Charnawskas
Advisor: Raymond Shaw
The Effects of the Gravitational Force on Water Particles in a Turbulent Flow

Mick Small
Advisor: Yoke Khin Yap
Photovoltaic Responses of Quantum Dot Sensitized ZnO Nanowires

Angela Small (Honor’s Institute)
Advisor: Jacek Borysow
Analysis of Artificial Breath Samples Using Raman Spectroscopy for Medical Diagnosis

Kevin Rocheleau (Honor’s Institute)
Advisor: Petra Huentemeyer
Analysis and Modeling of Diffuse Gamma-Ray Emission from the Cygnus Region using FERMI and HAWC Data

Jaszczak Publishes on Nanotech Innovations

Journal of Nano EducationProfessor John Jaszczak (Physics), former undergraduate student Echoe Bouta, and Professor of Practice Mary Raber (Institution for Interdisciplinary Studies) published a paper “Nanotech Innovations Enterprise at Michigan Technological University” in the latest edition of Journal of Nano Education, which is a special issue commemorating ten years of National Science Foundation funding of Nanotechnology Undergraduate Education programs.

From Tech Today.

Visit Nanotech Innovations

Fan Yang Research

Fan Yang - Nucleation Rates
Figure 1. wi and ni relationship for two ice nucleation rates. Blue points are from LES with lower ice nucleation rate and red points are higher ice nucleation rate. Solid and dashed lines are best fitted 2.5 slope lines.

Minimalist model of ice microphysics in mixed-phase stratiform clouds

Fan Yang

Advisor: Raymond Shaw

Mixed-phase clouds, which can exist days even weeks, are frequently observed in the Arctic region where they play an important role in the radiation balance. Observations also show that ice particles precipitate from these clouds nearly all time. The question of whether persistent ice crystal precipitation from supercooled layer clouds can be explained by time-dependent, stochastic ice nucleation is explored using an approximate, analytical model, and a large-eddy simulation (LES) cloud model. The updraft velocity in the cloud defines an accumulation zone, where small ice particles cannot fall out until they are large enough, which will increase the residence time of ice particles in the cloud. Ice particles reach a quasi-steady state between growth by vapor deposition and fall speed at cloud base. The analytical model predicts that ice water content (wi) has a 2.5 power law relationship with ice number concentration (ni). wi and ni from a LES cloud model with stochastic ice nucleation also confirm the 2.5 power law relationship. The prefactor of the power law is proportional to the ice nucleation rate, and therefore provides a quantitative link to observations of ice microphysical properties. Figure 1 shows LES results for two ice nucleation rates: Blue points correspond to low ice nucleation rate and red points to high ice nucleation rate. It’s clearly to see that points follow the 2.5 power law as our analytical model expected. The intercept shift predicted by the minimalist model is 1.05, which is very close to the best fitted line shift in Figure 1, 5.77-4.75=1.03. This provides a compelling link between ice microphysical properties and the ice nucleation rate within the cloud, which may be used in future analysis of cloud observation.

Reference

Yang, F., M. Ovchinnikov, R.A. Shaw (2013), Minimalist model of ice microphysics in mixed-phase stratiform clouds, Geophys. Res. Lett. doi: 10.1002/grl.50700 (accepted)

Alum Bhabana Pati Visited on Friday

Jacek Borysow and Bhabna Pati
Jacek Borysow and Bhabana Pati

Dr. Bhabana Pati visited the department on Friday, July 12, 2013. Bhabna graduated in 1997 with a Ph.D. after working with Dr. Jacek Borysow as a “laser junkie.” She developed the single mode tunable titanium sapphire laser and subsequently tunable ultraviolet laser via sum frequency generation in a non-linear crystal.

Today she is a principal scientist at Q-Peak Co. and still a “laser junkie,” trying among many other things to shoot lasers at the Moon to find out its composition via Laser Induced Breakdown Spectroscopy.