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College of Sciences Welcomes Seven Faculty Members

Friday, September 6, 2019

The College of Sciences welcomes seven members of faculty who joined in 2019. They include Susan Lozier, the new dean, Betsy Middleton and John Clark Sutherland Chair, and professor in the School of Earth and Atmospheric Sciences. Six others joined the Schools of Chemistry and Biochemistry, Physics, and Psychology, as well as the Undergraduate Program in Neuroscience. 

Meghan Babcock, Academic Professional, School of Psychology
Meghan Babcock earned her Ph.D. in experimental psychology from the University of Texas, Arlington, with an emphasis in social and personality psychology. As an academic professional, she is responsible for supporting undergraduate education through teaching and academic advising for all undergraduate psychology majors. She teaches undergraduate courses in psychology – including Research Methods in Psychology and Social Psychology – and manages the laboratory sections for the Research Methods course. In addition, she serves as a supervisor for undergraduate senior theses.

Marcus Cicerone, Professor, School of Chemistry and Biochemistry
Marcus Cicerone was a former group and project leader for the National Institute of Standards and Technology. His research centers on the development and application of Raman imaging approaches and the dynamics of amorphous condensed matter. His research group has logged many imaging firsts, including the first to obtain quantitative vibrational fingerprint spectra from mammalian cells using coherent Raman imaging and the first to identify specific structural proteins from coherent Raman imaging.

Glen Evenbly, Assistant Professor, School of Physics
Born in New Zealand, Evenbly earned physics degrees from the University of Auckland, in New Zealand (B.S.), and the University of Queensland, in Australia (Ph.D.). After postdoctoral work in California Institute of Technology and the University of California, Irvine, he served as an assistant professor in the University of Sherbrooke, in Canada. He researches the development and implementation of tensor network approaches for the efficient simulation of many-body systems, with additional applications to data compression and machine learning. He received the 2017 Young Scientist Prize in Computational Physics from the International Union of Pure and Applied Physics for developing new renormalization methods to study quantum systems.

Keaton Fletcher, Assistant Professor, School of Psychology
Keaton Fletcher is an industrial-organizational psychologist who studies work team leadership and associated outcomes for individuals, teams, and organizations. Specifically, he explores how a leader's differential treatment of team members can alter team dynamics, such as information sharing, trust, conflict, and cooperation, as well as individual outcomes such as health behaviors, job attitudes, and psychological and physical well-being. He examines these dynamics and implications in the field of healthcare, given the unique challenges healthcare teams face (e.g., interruptions, membership change). He also explores ways to improve leadership behaviors and workers’ well-being through training and intervention.

Joshua Kretchmer, Assistant Professor, School of Chemistry and Biochemistry
Joshua Kretchmer joined Georgia Tech after graduate and postdoctoral studies at the California Institute of Technology. He is a theoretical and computational chemist with the rare ability to combine the two important areas of electronic structure and quantum dynamics for large systems. His research focuses on developing new techniques to understand and predict the transport of charge and energy in complex environments and materials. He will apply his new techniques and insights to various applications, from chemical control in optical cavities, to light-harvesting materials, to surface catalysis.

Susan Lozier, Professor, School of Earth and Atmospheric Sciences
Susan Lozier is also the new dean and Betsy Middleton and John Clark Sutherland Chair of the College of Sciences. As dean, she will continue her research, studying the large-scale overturning circulation of the ocean, which impacts regional and global climate through the redistribution of heat. Overturning circulation – also known as the ocean conveyor belt – is also responsible for taking anthropogenic CO2 from the atmosphere and sequestering it in the deep ocean. Lozier leads the Overturning in the Subpolar North Atlantic Program (OSNAP), a National Science Foundation (NSF)-funded, international collaboration that aims “to provide a continuous record of the full-water column, trans-basin fluxes of heat, mass and freshwater in the subpolar North Atlantic.”

Alonzo Whyte, Academic Professional, Undergraduate Program in Neuroscience
After Alonzo Whyte earned his Ph.D. in from the University of St. Andrews, in Scotland, he completed an NIH-funded Fellowship in Research and Science Teaching (FIRST) at Emory University, focusing on developmental factors during adolescence that increase vulnerability to drug addiction and maladaptive decision-making. He teaches in the Principles of Neuroscience course and several upper-level neuroscience courses, in addition to coordinating the development of new experiments for the NEUR 2001 lab sections. He also provides academic advising to undergraduate neuroscience majors and serves on the Neuroscience Curriculum Committee for the management and development of neuroscience core and elective courses. 

Media Contact: 

A. Maureen Rouhi, Ph.D.
Director of Communications
College of Sciences

Summary: 

The College of Sciences welcomes seven members of faculty who joined in 2019. They include Susan Lozier, the new dean, Betsy Middleton and John Clark Sutherland Chair, and professor in the School of Earth and Atmospheric Sciences. Six others joined the Schools of Chemistry and Biochemistry, Physics, and Psychology, as well as the Undergraduate Program in Neuroscience. 

Intro: 

The College of Sciences welcomes seven members of faculty who joined in 2019. They include Susan Lozier, the new dean, Betsy Middleton and John Clark Sutherland Chair, and professor in the School of Earth and Atmospheric Sciences. Six others joined the Schools of Chemistry and Biochemistry, Physics, and Psychology, as well as the Undergraduate Program in Neuroscience. 

Alumni: 

Abstract:

Recently, the study of ultracold quantum gases of alkaline-earth-like atoms attracts great attention. Owing to the unique properties of these atoms, the system provides a perfect platform to study the non-trivial effects induced by orbital degree of freedom, spin-exchange interaction, and large-spin symmetry. In this talk, I will give some examples about simulating interesting quantum systems using alkaline-earth-like atomic gases. I hope this concise introduction can reveal at least some part of the talent of alkaline-earth-line atoms in the field of quantum simulation.

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Renovated Science Labs in Boggs

Tuesday, September 10, 2019

Editor's note: Here is an update on the information at minute 1:36 in the video: The Center for Relativistic Astrophysics, which currently occupies the next space to be renovated, is now slated to move into the Klaus Building to form a new interdisciplinary research neighborhood focusing on astrophysics and planetary sciences. 

Relentless construction in Georgia Tech makes it hard to keep track of what’s done and what’s just started. Earlier this year, the renovated first floor of the Gilbert Hillhouse Boggs building opened for business without fanfare. In the spring 2019 semester, upper-level laboratory courses in physics and biology quietly moved to spaces fashioned out of old offices and research labs.

On the outside, Boggs looks the same as it was in the 1970s, when it was built. But come in and you might exclaim, “Wow! I had no idea Boggs could look like this,” as Juan Archila says he has heard many people say. As the College of Sciences’ director of facilities and capital planning, Archila was heavily involved in the building’s makeover. 

Repurposed Mingles with State-of-the-Art

The main drivers of the Boggs first-floor upgrade are safety, accessibility, and sustainability. “We now have windows between the biology labs,” Archila says. All door also have windows, “to create transparency and to promote safety and accountability.” For students with disabilities, labs now have benches that are shorter than standard.

Budget for the project was tight, Archila says. In the spirit of sustainability and economy, usable materials were reused. “We didn’t completely gut the old spaces,” Archila says. “We repurposed and moved a lot of the cabinetry.”

Amid the repurposed cabinets are state-of-the-art equipment.

“Last year we received Tech Fee Funds to purchase nine Class II Biological Safety Cabinets,” says Alison Onstine, laboratory manager in the School of Biological Sciences. Each cabinet is six feet long and can accommodate two students working side by side. These equipment expand the hands on experience for students in handling cells, as well as organisms that require Biosafety Level 2.

More equipment is forthcoming, including an ultra-low-temperature freezer for specimen preservation, fluorescent microscopes, incubators for microbial work, and additional physiology equipment. 

Improvements in Learning and Instruction

Upper-level biology lab courses are now in Boggs, including genetics, microbiology, cell and molecular biology, anatomy, and physiology. Labs for advanced physics courses, as well as electronics and optics, also have moved to Boggs.

The advanced physics labs were previously taught in two small rooms in the Howey Building, says Claire Berger, a professor of the practice in the School of Physics who teaches the lab courses. In Boggs, “we have so much more space! It is clean and well-organized.

“It allows for more experiments to be set up and in better conditions. For example, the labs now have three separate dark rooms, equipped with water sinks, for the optical experiments.

“The labs are also less cluttered, therefore better in terms of safety. Because the teaching environment is less noisy, we can have one-to-one teaching on each of the individual experiments, as well as group teaching with a large, well-lit white board.”

The biology labs now in Boggs previously were taught in spaces spread across three floors of the Cherry Emerson Building. Now they are in one floor, sharing preparation rooms and equipment. “In Boggs, we have a strong nucleus that brings together the biology teaching lab community,” Onstine says.

“We have, for the first time, office spaces for teaching assistants and instructors to meet with students in close proximity to the labs,” Onstine says. “Additional benefits include two new shared equipment labs accessible to everyone, bringing our most advanced equipment within easy reach of students – including a bench-top flow cytometer, fluorescent plate readers, real-time PCR machines. These equipment spaces located between two teaching labs have promoted an open plan which we hope will create more connectivity between our core upper-level lab courses.” 

With the advanced chemistry labs in the second-floor, Boggs has become an interdisciplinary space for upper-level science majors, Archila says. “People who are focused on different majors see each other. That’s when you realize that a lot of people are attacking the same problem, just from different angles. It makes sense for Georgia Tech to establish that culture from the very beginning.”

“We are fortunate to share the floor with a new neuroscience teaching lab and to be one floor away from the chemistry teaching labs,” Onstine says. She thinks this layout will foster interaction and interdisciplinary research among students of different majors.

Media Contact: 

A. Maureen Rouhi, Ph.D.
Director of Communications
College of Sciences

Summary: 

Relentless construction in Georgia Tech makes it hard to keep track of what’s done and what’s just started. Earlier this year, the renovated first floor of the Gilbert Hillhouse Boggs building opened for business without fanfare. In the spring 2019 semester, upper-level laboratory courses in physics and biology quietly moved to spaces fashioned out of old offices and research labs.

Intro: 

Relentless construction in Georgia Tech makes it hard to keep track of what’s done and what’s just started. Earlier this year, the renovated first floor of the Gilbert Hillhouse Boggs building opened for business without fanfare. In the spring 2019 semester, upper-level laboratory courses in physics and biology quietly moved to spaces fashioned out of old offices and research labs.

Alumni: 

ABSTRACT:

Ultracold molecules are a new addition to the family of ultracold quantum matter, offering numerous internal states and strong dipolar interactions. So far, experiments have largely concentrated on using one or two internal states -- for example the ground state and a single excited rotational states -- which allows them explore physics such as quantum magnetism. However, the vast number of stable rotational states present new opportunities for quantum matter. I will describe two directions of our group's research in this area. First, we will see how experiments can use rotational states as a "synthetic dimension" -- an effective extra spatial dimension -- in which exotic phenomena can occur, such as topological bandstructures and the emergence of quantum strings. Second, we'll explore how collisions of ultracold molecules, in strong contrast to atoms, can be chaotic, and how this influences the many-body physics of many interacting molecules. Time permitting, I will also sketch our group's recent results on other issues at the intersection of many-body physics and ultracold matter, for example the phase diagram of the SU(6) Fermi-Hubbard mode, which isl being measured in ongoing experiments, and how new Lieb-Robinson bounds can transform our understanding of quantum matter and lead to new numerical algorithms.

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Abstract

Complex life larger than a humble nematode would not be possible without a circulatory system. Plants, fungi, and animals have developed vascular systems of striking complexity to solve the problem of long distance nutrient delivery, waste removal, and information exchange. These biological flow systems are frequently not static, but dynamically alter the diameters of their vessels in order to optimally achieve their intended function. The conductance of these vessels does not have to be linear, although it is frequently treated as such. Inspired by haemodynamic oscillations in the cortex, in this talk we explore how a system of laminar flow vessels can spontaneously produce and sustain dynamic local oscillations, even in the absence of time varying boundary conditions. We will show how these non-linear conducting vessels propagate pulses, how they redirect high volumes of flow to different locations of the network, and how introducing defects in the network can modify the dynamics. Last, we will discuss how we can use network topology and fluid dynamics to control flow in unexpected ways, and what this dynamic flow network behavior can tell us about living systems.

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Abstract

The era of high-energy astrophysics with cosmic neutrinos began with the discovery of high-energy neutrinos with extraterrestrial origin in IceCube. The observation of high-energy cosmic neutrino flux revealed the prominent and larger than expected role of hadronic interactions in the high-energy universe. Neutrinos can escape dense environments, otherwise opaque to photons, and travel cosmic distances unscathed by background radiation or magnetic fields. Therefore, they can provide the smoking gun for the origin of the cosmic rays.  In this talk, I will review the status of the high-energy neutrino astrophysics, will highlight the recent developments achieved via multimessenger observations, and furthermore, discuss the power of neutrino astrophysics in probing for the problems at the intersection of astrophysics , particle physics, and cosmology.

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Abstract

Observations show that supermassive black holes can affect their environment through outflows and other feedback processes. In order to establish the exact role that supermassive black holes play for galaxy evolution, we need to determine accurately the mass of the black holes for both nearby and more distant galaxies.  Since the commonly used methods are currently capable of measuring the mass with an uncertainty of a factor of 3 to 5 only, there is a dire need to significantly improve these methods. In this seminar I will discuss some of the main challenges we are facing in order to improve the black hole mass determinations as a first step to understand the role that black holes play for galaxy evolution.  In addition, I will address some of the recent progress that has been made on this topic, including the impact of the new results coming out of the Event Horizon Telescope and the GRAVITY instrument on ESO’s Very Large Telescope.

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Abstract

The three commonly considered pathways for hot Jupiter formation are in situ formation, runaway accretion in the outer disk followed by disk migration, and tidal migration (occurring after the disk has dissipated). None of these explains the entire observed sample of hot Jupiters, suggesting that different selections of systems form via different pathways. The way forward is to use observational data to constrain the migration pathways of particular classes of systems, and subsequently assemble these results into a coherent picture of hot Jupiter formation. We present constraints on the migratory pathway for one particular type of system: hot Jupiters orbiting cool stars (T< 6200 K). Using the full observational sample, we find that the orbits of most wide planetary companions to hot Jupiters around these cool stars must be well aligned with the orbits of the hot Jupiters and the spins of the host stars. The population of systems containing both a hot Jupiter and an exterior companion around a cool star thus generally exist in roughly coplanar configurations, consistent with the idea that disk-driven migratory mechanisms have assembled most of these systems.

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Abstract

Since Einstein's quadrupole formalism, multipolar analysis has played a central role in gravitational wave theory. In particular, gravitational waves from compact sources are ubiquitously represented using spin weighted spherical harmonic multipoles. But there is good reason to expect that a more natural basis exists for representing gravitational waves from astrophysical systems with angular momentum. In this talk I will review the recent developments in gravitational wave signal models for binary black hole systems. A key limitation of many such models is that they do not account for the more natural “spheroidal” harmonic nature of the post-merger signal. In this regard, I will briefly discuss recent work at the interface of BH perturbation theory, and numerical relativity which uses spheroidal harmonic information from NR simulations to model the late post-merger for spinning but non-precessing binary black hole systems. Lastly, the spheroidal harmonics will be discussed as a potentially more appropriate basis for all of inspiral, merger and ringdown.

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Abstract

As the gravitational wave (GW) observatories get more sensitive, the number of confident detection will grow exponentially. Conventional parameter estimation (PE) algorithms have to use specifically-tuned settings with fast waveform models to estimation parameters on multiple day timescales. As more events get detected and more sophisticated (and slower) models get developed, it will be necessary to speed up the runtime of these analyses. I introduce a rapid PE algorithm: RIFT. This algorithm can  estimate parameters of GW events in a shorter time period with slower waveform models as well as with numerical relativity waveforms (NR). In this talk, I will first introduce the methodology to the algorithm as well as tests we have done to check for systematic biases. I will show examples of real and synthetic events with different types of waveforms. I will then present practical applications that the algorithm can be uniquely applied to. Lastly, I will present updates and improvements we are making to the algorithm.

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