News and Events

×

Bard College Assistant Professor of Physics Antonios Kontos Receives $210,000 Grant from the National Science Foundation to Support Research in Measuring Gravitational Waves

Bard College has received a $210,000 grant from the National Science Foundation (NSF) in support of Assistant Professor of Physics Antonios Kontos’s proposal “Research in Light Scattering Metrology for Gravitational Wave Optics.” The three-year NSF grant supports his continuing research, summer research assistants, and equipment. All research projects are to be carried out with the engagement of Bard undergraduate and local area high school students, who will be hired as summer research assistants, and provide opportunities to gain invaluable experience in pursuing careers in technology and academia.

“This NSF grant will ensure that Bard continues to contribute to the fascinating new field of gravitational wave astronomy and that our students will continue to engage in cutting edge research in optics,” says Kontos.

The NSF award supports Kontos’s research in gravitational wave (GW) detector instrumentation, one of the most important leaps in scientific progress in recent years. The Laser Interferometer Gravitational-wave Antenna (LIGO) project has given scientists the ability to observe the universe in a completely new way. Unlike conventional telescopes which use the light emitted by stars and galaxies to learn their properties and their place in the universe, GW detectors use gravitational waves which are similarly emitted by many astrophysical objects.

Gravitational-waves are ripples in spacetime that travel to Earth, and cause the detectors to essentially change in size. To do that, the LIGO detectors require state-of-the-art mirrors, which are used to sense the stretching of space. Improvements in mirror design will allow observers to look further into space, and detect more of these GW signals. 

Kontos’s proposed project will aid in pushing the mirror technology, by utilizing light scattering as a tool to study mirror coatings. Specifically, an important aspect of mirror quality is the presence of defects which scatter light and inhibit the operation of the LIGO detectors. Defects may sometimes develop on the mirror surface with time, but the process is not always understood. This research project is designed to study defects on mirrors so that we can ultimately improve LIGO’s sensitivity and improve our understanding of space, time, matter, energy, and their interactions. 

Post Date: 06-07-2022

×

Bard College Appoints Beate Liepert as Visiting Professor of Environmental and Urban Studies and Physics in the Division of Science, Mathematics, and Computing

Bard College’s Division of Science, Mathematics, and Computing is pleased to announce the appointment of Beate Liepert as Visiting Professor of Environmental and Urban Studies and Physics. Professor Liepert, who joined the Bard faculty in January 2022, focuses on environmental physics, with a specific research goal of pursuing local solutions to the global issue of climate change. Her research interests include micrometeorology, air pollution, and community-based science.

Dr. Beate Liepert is a climate scientist who pioneered research on the phenomenon of “global dimming,” a decline in the amount of sun reaching the Earth’s surface, which has implications on the planet’s water and carbon cycles. She comes to Bard from the Seattle area, where she worked for and founded start-ups in the clean tech and insure tech fields, and was a lecturer in the Department of Civil and Environmental Engineering at Seattle University. The start-ups included CLIWEN LLC, a climate, energy, and weather consulting concern; and Lumen LLC, a company that developed design solutions for solar cells. She also served as a research scientist at True Flood Risk LLC in New York, NorthWest Research Associates in Seattle, and the Lamont-Doherty Earth Observatory of Columbia University. Her work centers on basic questions of climate variability, from interannual to centennial time scales. Research interests also include taking measurements of aerosols and solar radiation and investigating climate effects on ecosystems.

Additional activities have included serving as editor for Environmental Research Letters, a UK-based journal; proposal review panelist and proposal reviewer for the National Science Foundation; presenting at more than 50 international conferences and university colloquia; and authoring reviews and articles for journals including Bulletin of the American Meteorological Society, Climate, Frontiers, International Journal of Climatology, Nature, Science, Quarterly Journal of the Royal Meteorological Society, and Global and Planetary Change, among many others. She has been interviewed on CNN and numerous international TV broadcasts; was a featured scientist in the BBC documentary Dimming the Sun, which also aired on PBS; and was profiled in a “Talk of the Town” essay in the New Yorker. Professor Liepert is the recipient of the 2016 WINGS World Quest “Women of Discovery” Earth Award and in 2015 she delivered a Distinguished Scientist Lecture at Bard on “Dimming the Sun: How Clouds and Air Pollution Affect Global Climate.”

Diploma, Institute of Meteorology and Institute of Bioclimatology and Air Pollution Research, Ludwig-Maximilians University Munich; Doctor rer. nat., Institute of Meteorology, Department of Physics, Ludwig-Maximilians University; postdoctoral research scientist, Lamont-Doherty Earth Observatory of Columbia University; certificate program in fine arts, Parsons School of Design.

Post Date: 04-13-2022

×

Bard Physics Professor Shuo Zhang Presents Research on Supermassive Black Hole at 2022 American Astronomical Society Press Conference

Bard College Assistant Professor of Physics Shuo Zhang has been invited by the American Astronomical Society (AAS) to present her most recent research on how surrounding molecular gas clouds offer insight into the activity history of Sgr A*, the now inactive supermassive black hole at the center of our Milky Way galaxy. Zhang’s talk, “Galactic Center Molecular Clouds: Storytellers of Past Outburst of the Galactic Center Supermassive Black Hole,” is being presented at a virtual AAS press conference to be held on Tuesday, January 11 from 4:15pm to 5:15pm ET via Zoom. For more information about the virtual press conference, click here.

Though inactive nowadays, traces of a glorious past of Sgr A* can be found in the surrounding molecular gas clouds, which reflect incoming X-ray emission from Sgr A* up to a few hundred years ago. Therefore, by studying X-ray emission from molecular clouds at different distances from Sgr A*, we can reconstruct the activity history of Sgr A* in the past few centuries. Shuo Zhang and her post-bac researcher Nathalie Jones ’21 have focused their study on a particular Galactic center molecular cloud, the “Bridge”. Their analysis on archival data by the NuSTAR telescope during 2012-2020, and the XMM-Newton telescope data during 2000-2020 clearly demonstrates an epic 20-year-long X-ray brightening of the “Bridge” molecular cloud, making it currently the brightest diffuse feature in the Sgr A* complex region. Continuous monitoring of this molecular cloud and capturing its peak luminosity will tell us how luminous Sgr A* used to be a couple dozen years ago, which is essential to understand the activity cycle of supermassive black holes. This project is supported by NASA NuSTAR Guest Observation grant #80NSSC20K0035.

“It is amazing to have these molecular gas clouds as storytellers of past activities of the monster black hole in the center of our Galaxy,” says Zhang. 

About the Annual Conference of the American Astronomical Society
The American Astronomical Society is the major organization of professional astronomers in North America, with a membership of 7,700 individuals with research and educational interests in astronomical sciences. The 239th meeting is the 2022 winter annual American Astronomical Society conference, which brings together the International astronomer community and shares the most recent discoveries and results in astronomy. Though the major meeting was canceled due to COVID situation, the press conference will take place virtually as planned.

Post Date: 01-11-2022

×

Bard College Appoints Astrochemist Clara Sousa-Silva to Tenure Track Faculty Position in Physics Program, Effective Spring 2022

Bard College is pleased to announce that Clara Sousa-Silva has been appointed to a tenure track faculty position in the Physics Program. Sousa-Silva will join the faculty of the College in spring 2022 as a full-time assistant professor of physics in the Division of Science, Mathematics, and Computing. Sousa-Silva is a quantum astrochemist at the Center for Astrophysics | Harvard & Smithsonian. She investigates how molecules interact with light so that they can be detected on faraway worlds. Sousa-Silva’s July 2021 TED talk, “The Fingerprints of Life Beyond Earth,” is featured on the front page of the TED website.

About Clara Sousa-Silva
Clara Sousa-Silva spends most of her time studying molecules that life can produce so that, one day, she can detect an alien biosphere. Her favorite molecular biosignature is phosphine: a terrifying gas associated with mostly unpleasant life. When she is not deciphering exoplanet atmospheres, Sousa-Silva works hard to persuade the next generation of scientists to become an active part of the astronomical community.

Sousa-Silva holds a doctoral degree in quantum chemistry from the University College London, and a masters degree in physics and astronomy from the University of Edinburgh in Scotland. Among her many achievements, Sousa-Silva is the recipient of the prestigious 51 b Pegasi Fellowship from the Heising Simons Foundation. The fellowship supports the growing field of planetary astronomy and exceptional postdoctoral scientists who make unique contributions to the field of astronomy. Her work and commentary has been featured in the BBC, WIRED, and the New York Times, among many others. Prior to joining the Center for Astrophysics, Sousa-Silva served as a research scientist at MIT.

About Bard College
Founded in 1860, Bard College is a four-year residential college of the liberal arts and sciences located 90 miles north of New York City. With the addition of the Montgomery Place estate, Bard’s campus consists of nearly 1,000 parklike acres in the Hudson River Valley. It offers bachelor of arts, bachelor of science, and bachelor of music degrees, with majors in nearly 40 academic programs; graduate degrees in 11 programs; eight early colleges; and numerous dual-degree programs nationally and internationally. Building on its 161-year history as a competitive and innovative undergraduate institution, Bard College has expanded its mission as a private institution acting in the public interest across the country and around the world to meet broader student needs and increase access to liberal arts education. The undergraduate program at our main campus in upstate New York has a reputation for scholarly excellence, a focus on the arts, and civic engagement. Bard is committed to enriching culture, public life, and democratic discourse by training tomorrow’s thought leaders. For more information about Bard College, visit bard.edu.(8/31/21)
 

Post Date: 08-30-2021

×

Bard Physicist Hal Haggard Coauthors New Study on Fast Spacetime Dynamics in Quantum Gravity

Dynamics has altered forever the once static arenas of space and time. Physicists have even measured spacetime deform and undulate as gravitational waves propagate away from colliding black holes. Regrettably, these dynamics have incompletely invaded the discrete, granular world of quantum gravity. In a new study in Physical Review Letters, Haggard, together with colleagues Seth Asante and Bianca Dittrich of the Perimeter Institute for Theoretical Physics, uses computer simulations to show that dynamical grains of space can be built up into a complete picture of a small but evolving quantum spacetime.

Post Date: 12-06-2020

×

Bard Physics Professor Shuo Zhang Discusses Her Research on Galactic Center Filaments at American Astronomical Society Press Conference

Bard College Assistant Professor of Physics Shuo Zhang discussed her current research and participated in a press briefing Tuesday, June 2, at the 236th Meeting of the American Astronomical Society. In her presentation, “Revealing the Powerful Particle Accelerator in the Galactic Center,” Zhang discussed her research exploring the nature and origin of one of the most striking phenomena in the center of the Milky Way Galaxy, the existence of dozens of filamentary structures that can be as long as hundreds of light years. In a series of papers, Zhang and her research partners propose that the supermassive black hole in the Galactic center, Sagittarius A*, is the engine producing energetic particles that eventually light up these filaments in the X-ray and radio wave bands.

Zhang says the theory is supported by recent gamma-ray and radio observations. “Using observations recently obtained by the Chandra space telescope, we see evidence for new X-ray filaments,” says Zhang. “My next goal is to conduct a systematic multi-wavelength search for Galactic center filaments and use their spatial distribution and spectral information to further test our theory.”

The American Astronomical Society is the major organization of professional astronomers in North America, with a membership of 7,700 individuals with research and educational interests in astronomical sciences. The 236th meeting is the 2020 summer annual American Astronomical Society conference, which brings together the international astronomer community and shares the most recent discoveries and results in astronomy. For more information, visit aas.org.

Shuo Zhang, assistant professor of physics at Bard, is interested in observational high-energy astrophysics, including supermassive black hole accretion and feedback, origin of Galactic cosmic-rays and dark matter searches. She studies outburst histories of the supermassive massive black hole at the center of the Milky Way galaxy and nearby galaxies, in order to understand supermassive black hole activity cycle, particle acceleration mechanism and physics under strong gravitational field. Recently, she initiated an original particle astrophysics project on probing Galactic cosmic-ray particles at MeV through PeV energy scales suing innovative methods, aiming to understand the origin of Galactic cosmic-rays and to reveal power particle accelerators at the center of the Galaxy. Zhang served previously as a NASA Einstein Fellow at Boston University, and a postdoctoral scholar and Heising-Simons Fellow at the MIT Kavli Institute for Astrophysics and Space Research. In addition to her research, she is a referee for Nature, monthly notices of the Royal Astronomical Society, and a panel reviewer for NASA’s Astrophysics Data Analysis Project. She is also a member of several scientific collaborations, including Event Horizon Telescope (EHT) collaboration, eXTP Space Telescope Observatory Science Working Group, Chandra/ACIS Instrument Team, and NuSTAR Space Telescope Science Team, among others. Her work has appeared frequently in Astrophysical Journal and Monthly Notices of the Royal Astronomical Society. Zhang earned a BS degree from Tsinghua University and a PhD from Columbia University.
 

Post Date: 06-02-2020