The department offers a physics colloquium every Friday. Researchers from outside the College are invited to talk about their work, students discuss their summer research projects and their senior-exercise topics, and alumni share their latest exploits. Check regularly for upcoming talks.
Fall 2021 Physics Colloquiums
Professor of Physics David Weiss of Eberly College of Science will be presenting on the role of atoms in quantum computing. You can join us for this presentation from 12 to 1 p.m. in Hayes Hall 211/213.
I will first explain how we use lattices made from light to trap 3D arrays of single neutral atoms. Then I will show how these atoms can be used as the quantum bits (qubits) in a quantum computer. Among the tools we have developed to this end, I will focus on how we sort 50 atoms in the 3D lattice, in a real world demonstration of a Maxwell's demon, arguably the first such demonstration with more than a couple of particles.
In this exciting combination of biology and physics, assistant professor of Physics and Astronomy, Srividya Iyer-Biswas, of Purdue University will explain her research in defining quantitative laws for understanding cell division and biological systems.
There has been a longstanding quest for uncovering the quantitative laws governing the stochastic growth and division of individual cells. While great strides have been made in unravelling and modeling the details of the gene regulatory networks which dictate growth and division for different organisms, there is a regrettable paucity of quantitative physical laws derived from the complementary “top down” perspective. Introducing the unique combination of technologies that facilitated probing stochastic cellular dynamics with unprecedented precision, I will first summarize the "scaling laws" that govern fluctuations in growth and division of individual cells under steady-state growth conditions. Taking a minimalist perspective, I will argue for how these scaling laws reveal an elegant physical principle governing these complex biological processes: a single cellular unit of time, which scales with external conditions, governs all aspects of stochastic cell growth and division at a given condition. I will then focus on applications of the technology to probe more complex growth conditions, the corresponding generalizations of the physical principle, and the implications for the underlying biological systems design. Finally, I propose an integrative perspective of microbial growth dynamics under balanced conditions, by introducing a multi-scale theoretical framework that takes observables at both scales, single-cell and population, into account. Time permitting, I will make connections with stochastic intergenerational homeostasis of bacterial growth and form.
Join us in Hayes 211/213 from 12:10 to 1 p.m. to hear the presentation. Food will be served after the meeting.
Professor of Physics Nicole Zellner of Albion College will be presenting on astrobiology and the search of life in space. You can join us for this presentation from 12 to 1 p.m. in Hayes Hall 211/213. If you cannot join us in person, feel free to join us virtually by following this Zoom link.
Astrobiology is defined as the study of life in the universe. But, then, how can you define life itself? There are three main requirements of life known to us: energy, water and organic molecules. Formed in molecular clouds, on dust grains, are the building blocks of life: biomolecules. Energy changes simple molecules into more complicated ones and these are used in DNA. The identification of these prerequisites of life has opened a greater question: is there life in space? Specifically, we talk about the detection of water, energy and organic molecules from space debris on Mars, thus leading to the conclusion that with all the right elements present maybe it is a matter of time till a discovery of life.
Similarly, on Europa, Titan and Enceladus, there is a distinct possibility of the presence of life. However, it may not be the kind of life you imagine. To find life as we know it, we look towards the stars at the Galactic Habitable Zone, Stellar Habitable Zones and Extrasolar Planets. The likelihood of finding intelligent life is explored by the Drake equation, Seager equation and practically, using SETI for the observation of radio signals. This talk will carry you on a cosmic journey to uncover the meaning of life in astrobiological terms, a new kind of life and perhaps, a familiar one in an unfamiliar place.
Professor of Physics Susan Lehman of the College of Wooster will be presenting on experiments in the study of critical systems. You can join us for this presentation from 12 to 1 p.m. in Hayes Hall 211/213. If you cannot join us in person, feel free to join us virtually by following this Zoom link.
A granular system behaves in some ways like a liquid with an ability to flow, and in some ways like a solid with a stable fixed structure if undisturbed. A tiny stimulus to the pile most often results in only a small response, but the same small stimulus can also create an unpredictable and catastrophic collapse of the pile. These collapses occur both in natural settings, with hazards such as landslides and snow avalanches, and in industrial situations, where granular materials like sand or agricultural grains need to flow freely. We use a simple experimental system — a 3D conical pile of uniform beads — in order to model these real-world physical systems. We investigate the dynamic response of the pile by recording avalanches from the pile over the course of tens of thousands of bead drops. The resulting behavior is well-characterized by universal power laws and scaling functions, relating this work to the broader study of critical systems.
For Family Weekend, Professor Benjamin Schumacher will discuss various impossibilities in physics and what they mean regarding our understanding of the world. Join us in Hayes Hall 211/213 at 12 p.m. for this exciting presentation on the impossible. If you cannot join us in person, feel free to join us virtually by following this Zoom link.
Some things are possible and some are not. That line between the possible and the impossible can tell us a lot about the way nature works. In this talk we will ponder a few impossibilities, from the famous (time travel) to the obscure (quantum cloning), using them to discover some of the physical principles that govern information in our quantum universe. As one might expect upon a journey into wonderland, our constant companion will be Alice — thanks to her creator Lewis Carroll and her most famous illustrator Sir John Tenniel. Many surprises will await us through the looking-glass of the impossible.
Michael Lisa will be offering a look at the unique applications of physics in the world of sports, encompassed in a semester course at Ohio State University. Join us in Hayes Hall 211/213 at 12 p.m. to learn more.
Ohio State University offers a one-semester course on the physics of sports, which satisfies a GEC science requirement of all students. Scholarship athletes, business and liberal arts majors make up the majority of the ~80 students enrolled in the class, though interested sports enthusiasts from more technical fields join as well. The class is far from the "Physics for Poets" type of course that some expected, leading to some initial math- and science-anxiety. It is gratifying when some of this anxiety is replaced by a self-confidence in many students that they can, indeed, handle and appreciate a "real" mathematical science course on material they already enjoy. While the underlying physics lies of course squarely in the realm of classical mechanics, and familiar topics must be covered, the course aims to be unique, not simply a standard classical mechanics class with sports examples. I will discuss the several challenges to develop a course like this and share some specific lessons learned and insights gained over many years. This talk does not present formal physics education research.
Professor of Physics Smitha Vishveshwara from the University of Illinois Urbana-Champaign will be presenting on "Quantum Voyages, Cosmic Journeys: Exploring Physics through the Arts." This presentation takes a unique gaze at physics through the artistic spectrum. Join us in Hayes 211/213 at 12 p.m. for the presentation.
From ancient monuments to modern day films, the confluence of the arts and physics has resulted in creations that have led to a deeper understanding of nature, to friendly and enchanting ways of perceiving science in action, to giving the arts a new dimension, to technological progress, and to pure fun! In this talk, I will describe the educational power of such confluences and recount some of our experiences in this realm. In a project-based interdisciplinary course entitled Where the Arts meets Physics, we bring alive the universe and the quantum world through installation and performance — cosmic canopies housing black hole mergers, raps on radioactivity, Warhol versions of Bohr-Einstein debates, and more. Collaborations with theater, music and dance have led two original performance pieces that explore the magic and beauty of the quantum world, Quantum Voyages and Quantum Rhapsodies. I will share the science, stories, and process behind the making and performing of these pieces, and conclude with a description our latest adventure — a virtual art-science festival entitled the Illuminated Universe.
Our fourth and final honor student speaker will be Mary Gerhardinger. She will be presenting on "Modeling Relativistic Fluids in General Relativity." Join us in Hayes 211/213 at 1 p.m. for the presentation. Food will be provided before the presentation at 12:30 p.m.
Current models of cosmology predict the formation of black holes near the beginning of the Universe’s life that are not a result of stellar collapse. These black holes, called Primordial Black Holes (PBH), could help explain our currently incomplete understanding of the origin of super massive black holes and the composition of dark matter. Exactly how these PBH are formed, however, has not been studied rigorously. In this talk I will introduce my honors work examining the possible formation of PBH from primordial density fluctuations modeled through the interaction of radiation with gravity. Specifically, I will discuss the best approximations we can use to describe both radiation (as a relativistic fluid) and gravity (as Einstein’s theory of General Relativity). We will investigate both the theories of fluids and general relativity before discussing how to implement this model onto computational simulations, performed using a tool called GABERel.
The third of our honors student presentations will be Tom Yoda discussing trapped ultra-cold atoms. Join us at noon on Friday, Sept. 17.
"The Rydberg excitation blockade, or the suppression of excitation due to strong interactions, is a critical component of quantum computation and simulation using neutral atoms. However, unwanted state-mixing effects near Förster resonance cause the blockade to break down. My research group performs state selective field ionization spectroscopy on a shot-by-shot basis to observe this effect. I will introduce you to the world of trapped ultra-cold atoms. Then, I will propose my honors project of controlling unwanted state-mixing effects using different parameters, not just the principal quantum number or density of the atoms, but also pulse duration and Rabi frequency. This control will be critical in future implementations of neutral-atom quantum information."
In the second of our honors presentation series, Erika Florio '22 will be exploring the physics of black hole-scalar field interactions. This event will be virtual. Join us via Zoom.
As it stands, our best description of gravity, general relativity, is not fully consistent with our most successful physical theory ever, quantum mechanics. Examining high-energy phenomena, such as the physics of the early universe and regions of extreme spacetime curvature, is essential for determining where our theory of gravity may fail, and how we can move beyond it. This presentation will introduce Ericka's honors work examining the physics of black hole-scalar field interactions. She will perform this computation using GABERel, a numerical tool that can couple full (numerical) general relativity with scalar fields without making any assumptions, in a fully non-linear context. She will generate scalar field wave packets and a black hole, then allow the wave packet to hit a black hole. She will then examine the products of this interaction in configuration space as the frequency of the wave packet changes in order to determine which types of interactions are possible and on what scales.
This September, the Physics Department is hosting a series of presentations by our very own honor students. For Friday, Sept. 3, we welcome Quinn Curren (class of 2022) for his presentation on pulsar candidates. Due to recent changes on campus, this presentation will be a virtual event.
Pulsars are rapidly spinning neutron stars that emit electromagnetic radiation along their magnetic poles. The fastest pulsars, known as millisecond pulsars, rotate hundreds or thousands of times each second and have periods as precise as atomic clocks. Scientists can observe gravitational waves through the careful timing of a large collection of millisecond pulsars, since gravitational waves will shift the correlated arrival time of these pulses as measured on Earth. These Pulsar Timing Arrays become more sensitive as more pulsars are discovered. Pulsars are observed mainly using radio telescopes, but radio emissions from other sources are also picked up by these telescopes. Advanced software is used to find pulsar candidates from radio telescope observations across the sky. Radio Frequency Interference (RFI) and noise comprises well over 99 percent of the candidates in the PALFA survey, and can closely resemble genuine pulsar candidates. However, manually sorting through the pulsar/RFI candidates is time consuming and inefficient. One method of analyzing the candidate list is to create an algorithm that will automatically rank the candidates using machine learning algorithms (MLA). This project aims to create a novel MLA that will rank pulsars accurately and separate them from non-pulsar candidates. Machine learning aims to recreate the way that humans learn; and like MLAs, this project’s structure is based upon the methods that experts use to manually rank candidates.
Enjoy a welcome meeting to the Physics Colloquium series. Meet other students and members of the department and discuss what's happening this year in physics. Lunch will be served from 12 to 1 p.m.