Skip to main content.
Bard
  • Bard
  • Academics sub-menuAcademics

    A place to think.

    Discover Bard
    • Academics
      • Programs and Divisions
      • Structure of the Curriculum
      • Courses
      • Requirements
      • Academic Calendar
      • Faculty
      • Libraries
      • College Catalogue
      • Bard Abroad
      • Dual-Degree Programs
      • Other Study Opportunities
      • Graduate Programs
      • Early Colleges
  • Admission sub-menuAdmission

    Do you love to learn?

    Discover Bard

    Apply Now
    • Discover Bard
      • Our Students
      • Our Alumni/ae
      • Campus Tours
      • Bridge Program
      • Video Gallery
    • Applying
      • First Year
      • Transfer Students
      • Early College Transfers
      • International Students
      • Homeschooled Students
      • DACA and Undocumented
      • Bard Conservatory
      • Return to College
      • Admitted Students
      • Enroll Now!
      • New Students
      • Prospective Families
      • Familias
      • Financial Aid
      • Tuition and Payment
      • Contact Us
      • Admission Team
      • Tour Guides
      • Graduate Admission
      • Early College Admission
  • Campus Life sub-menuCampus Life
    Bard Campus Life

    Make a home in Annandale.

    • Living on Campus
      • Housing + Dining
      • Campus Resources
      • Get Involved on Campus
      • Bard Connects
      • Visiting + Transportation
      • Athletics + Recreation
      • New Students
  • Civic Engagement sub-menuCivic Engagement
    • Bard CCE The Center for Civic Engagement (CCE) at Bard College embodies the fundamental belief that education and civil society are inextricably linked.

      Take action.
      Make an impact.

      Get Involved
      • Campus + Community
      • In the Classroom
      • U.S. Network
      • International Network
      • About CCE
      • Resources
      • Support
  • Newsroom sub-menuNews + Events
    Upstreaming
    • News + Events
      • Newsroom
      • Events Calendar
      • Video Gallery
      • Press Releases
      • Office of Communications
      • COVID-19 Updates
    • Special Events
      • Commencement + Reunion Weekend
      • Family + Alumni/ae Weekend
      • Fisher Center
      • Bard SummerScape
      • Bard Athletics
  • About Bard sub-menuAbout Bard

    A private college for the public good.

    Support Bard
    • About Bard College
      • Mission Statement
      • Bard History
      • Love of Learning
      • Visiting Bard
      • Employment
      • OSUN
      • Bard Abroad
      • The Bard Network
      • Montgomery Place Campus
      • Campus Tours
      • Diversity, Equity, and Inclusion
      • Sustainability
      • Title IX
      • HEOA Disclosures
      • Institutional Support
      • Safety and Security
      • Inside Bard
      • Alumni/ae Network
      • Family Network
      • Support Bard
  • COVID-19 Response
  • Search
Bard Physics Program

News and Events

Physics Menu
  • Physics Home:
  • Prog sub-menuThe Program
    • Physics Program
    • 3+2 Programs in Engineering
  • Faculty
  • Requirements + Courses
  • Research
  • Senior Projects
  • News + Events
  • Resources

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 granular world of quantum gravity. In a new study, Haggard and colleagues use computer simulations to show that dynamical grains of space can be built up into a complete picture of a small but evolving quantum spacetime.

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.
Read more in Physical Review Letters

Post Date: 12-06-2020

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

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.

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

Bard Connects: Faculty and Staff Get Creative to Provide Protective Gear to Regional Health Workers

A broad network of Bard faculty and staff has come together to produce face shields for frontline health-care workers who are grappling with a nationwide shortage of protective gear.

Bard Connects: Faculty and Staff Get Creative to Provide Protective Gear to Regional Health Workers

“Life in the era of COVID-19, as in all times of crisis, amplifies our basic instincts. Do we become anxious or confident, selfish or generous, rigid or adaptable? The same applies to institutions. And right now, at this moment of national and global crisis, Bard College is demonstrating who we are: student-focused, innovative, entrepreneurial, and civically engaged.” —Jonathan Becker, Vice President for Academic Affairs and Director of the Center for Civic Engagement at Bard College


A broad network of Bard faculty and staff—including Ivonne Santoyo-Orozco and Ross Exo Adams in the Bard Architecture and Design Program; Maggie Hazen and Melinda Solis in Studio Arts; IT’s Doug O’Connor, Hayden Sartoris, and Christopher Ahmed; and the Philosophy Program’s Katie Tabb—has come together to produce face shields for frontline health-care workers who are grappling with a nationwide shortage of protective gear.
3D-printed face shield components.
3D-printed face shield components.


With two 3D printers loaned by Bard physicist Paul Cadden-Zimansky, Exo Adams and Santoyo-Orozco set up a makeshift lab in Tivoli to fabricate reusable face shields for health-care workers. When the lab is fully operational, they expect to produce up to 50 shields per week. Hazen and Solis have begun a production line as well, using 3D printers purchased with proceeds from a GoFundMe campaign established by MFA alumna Luba Drozd ’15 that has raised more than $20,000. A small batch of shields has already been distributed to Columbia Memorial Hospital in Hudson, New York, and the group is now looking for more distribution options in the Hudson Valley. Deliveries of face shields are also scheduled for Albany Medical Center and, in Dover, New Jersey, Saint Clare’s Hospital, where a Bard student’s relative works and on whose behalf the student made a request. Anyone interested in distribution or in assisting with the project should contact Doug O’Connor (oconnor@bard.edu), who is centralizing the distribution efforts with the help of CCS Bard students.

And in Annandale, members of the Fisher Center’s Costume Shop—together with Audrey Smith from Buildings and Grounds, Rosalia Reifler from Environmental Services, and Saidee Brown from the President’s Office—have sewn nearly 200 face masks for the essential College employees who remain on campus.
 
To learn more about virtual engagement opportunities at Bard, visit Bard Connects.

Post Date: 04-12-2020
More Physics News
  • Professor of Physics Hal Haggard and Colleagues Receive Buchalter Cosmology Prize for Black Hole Research

    Professor of Physics Hal Haggard and Colleagues Receive Buchalter Cosmology Prize for Black Hole Research

    Bard College Assistant Professor of Physics Hal Haggard and his fellow researchers were awarded a 2019 Buchalter Cosmology Prize at the 235th meeting of the American Astronomical Society in Honolulu, Hawaii, on January 6. The annual prize series, created by Dr. Ari Buchalter in 2014, seeks to reward new ideas or discoveries that have the potential to produce a breakthrough advance in our understanding of the origin, structure, and evolution of the universe. Professor Haggard and his colleagues were recognized for research testing the Bekenstein-Hawking entropy of black holes.

    The $5,000 Second Prize was awarded to Professor Haggard, of Bard College and the Perimeter Institute for Theoretical Physics, and colleagues from the Pennsylvania State University: Eugenio Bianchi, Anuradha Gupta, and B. S. Sathyaprakash (also of Cardiff University). The judging panel recognized their paper, “Quantum Gravity and Black Hole Spin in Gravitational Wave Observations: a Test of the Bekenstein-Hawking Entropy,” as “a remarkable test of the thermodynamic character of black holes, predicting the spin characteristics of an initial primordial population of black holes that thermalize in the early universe, and which could be detectable by current and near-future gravitational wave detectors.”

    Haggard’s work is part of an ongoing scientific revolution in the study of black holes. Last year, scientists captured the first direct image of a black hole, less than four years after measuring, for the first time, the gravitational waves created by the collision of two black holes circling one another at nearly light speed. These waves directly oscillate space and time. Contrary to initial expectations, pairs of black holes crashing into each other give rise to most of the gravitational waves we can currently measure. Advanced facilities like the Laser Interferometer Gravitational-Wave Observatory (LIGO) are now observing and measuring black hole collisions about once a week.

    Previously, scientists only knew about two main types of black holes: X-ray binary systems, which often contain one active star and a black hole, in the range of five to 15 times the mass of our sun, that “siphons off” mass from the donor star; and supermassive black holes, a class that includes the black hole imaged in 2019, which measures about 6.5 billion solar masses. 

    Prior to LIGO, physicists did not expect that the main class of binary collisions measured would be of two black holes, or that those black holes would have masses in the range of 20 to 80 solar masses. Most surprising of all, it now appears possible that most of the black holes measured through gravitational waves aren’t spinning at all before they collide. Scientists had thought that the majority of black holes were formed in the gravitational collapse of a rotating star. 

    Haggard and his colleagues’ paper shows that black holes formed in a different way, as part of the hot primordial soup of the early universe, could naturally have zero spin. The authors also find that these black holes would be expected to have masses of 10 to 100 times the mass of our sun. Their arguments are based on understanding how entropy and temperature determine the physical characteristics of a black hole, for example its spin. 

    “I’m delighted about this paper because it brings together so many of the strands of my work,” says Haggard. “Gravitational wave measurements are an exciting probe of the rich interplay between gravitational thermodynamics, black holes, and the early history of the cosmos. It is a rare point of contact between the ideas that go into a quantum theory of gravity, like black hole entropy, and experimental observations that are happening right now.”

    The $10,000 First Prize was awarded to Jahed Abedi and Niayesh Afshordi for their work entitled “Echoes from the Abyss: A Highly Spinning Black Hole Remnant for the Binary Neutron Star Merger GW170817.” The $2,500 Third Prize was awarded to José Beltrán Jiménez of Universidad de Salamanca and colleagues for their work entitled “The Geometrical Trinity of Gravity.”

    Dr. Buchalter, a former astrophysicist turned business entrepreneur, established the prize series in the belief that significant breakthroughs in the field of cosmology still lie ahead but might require challenging and breaking with accepted paradigms. “The 2019 prizewinners represent bold thinking that can help open up new frontiers in our understanding of physics and of the universe,” said Dr. Buchalter. The judging panel for the annual prizes is made up of leading theoretical physicists noted for their work in cosmology. The 2019 panel included Justin Khoury and Mark Trodden of the University of Pennsylvania and Lee Smolin of the Perimeter Institute for Theoretical Physics. Learn more at buchwaltercosmologyprize.org.
    Read the Paper in General Relativity and Quantum Cosmology
    Visit the Physics Program Website

    Post Date: 01-21-2020
  • Underwater Laser Slicing of the World’s Thinnest Material

    Underwater Laser Slicing of the World’s Thinnest Material

    Bard Faculty and Students in Chemistry and Physics Collaborate on Newly Published Research

    In recent years, scientists have developed a new set of techniques to thin down certain materials into sheets that are only a few atoms thick—the most famous example being graphene, a one-atom thin layer of graphite that holds the title of world’s thinnest material. Graphene and its thin cousins hold promise both for being implemented in new technology and in helping physicists understand the quantum properties of materials. In making prototype devices from them, researchers often need to shape these sheets into particular patterns with features measured in nanometers.

    Noting that conventional methods for doing this require multistep processes that can damage the materials, Ethan Richman ’20 led a team of undergraduates working in the labs of Bard Chemistry Professor Chris LaFratta and Physics Professor Paul Cadden-Zimansky to pioneer a potentially cleaner and faster way of slicing graphene at the nanoscale by using a high-powered laser beam focused into a microscope. While a handful of other research groups around the world have tried using lasers for graphene slicing, the Bard researchers noticed that laser cuts in air can damage the graphene at the atomic level. Taking a cue from techniques used in industrial laser cutting, Richman tried modifying the cutting technique by submerging the graphene in water and found this improved both the quality and efficiency of the cutting. Their results are published in Optics Materials Express, with Cadden-Zimansky, LaFratta, and eight student collaborators as coauthors.
    Read More in Optics Materials Express

    Post Date: 09-03-2019
  • Bard Hosts Quantum Gravity Summer School for Students and Scholars from U.S. and Abroad

    Bard Hosts Quantum Gravity Summer School for Students and Scholars from U.S. and Abroad

    With Public Lecture “What Is Time?” by Carlo Rovelli, World-Renowned Scientist and Best-Selling Author, on Thursday, June 13

    The Bard Summer School on Quantum Gravity takes place from June 9 to June 16. Fifty-two students from more than 20 countries will participate, plus Bard College students on campus for the Summer Research Institute. This program for undergraduate and graduate students features canonical and covariant approaches to quantum gravity and quantum cosmology. One unique feature of the program is an afternoon computing lab in which students learn a computational technique in cosmology or one in quantum gravity from scratch.

    The Bard Summer School on Quantum Gravity provides free tuition and housing on the Bard College campus. The school received generous support from the Center for Gravitation and the Cosmos at Pennsylvania State University; the Perimeter Institute for Theoretical Physics; the University of Waterloo; the Division of Science, Mathematics, and Computing at Bard College; the Dean of Bard College; and the Bard Physics Program.

    The eight faculty members are scholars at the top of their fields: Ivan Agullo, Louisiana State University; Boris Bolliet, Jodrell Bank Center for Astrophysics, The University of Manchester; Pietro Doná, Pennsylvania State University; Edward Wilson-Ewing, University of New Brunswick; Maïté Dupuis, University of Waterloo and Perimeter Institute for Theoretical Physics; Laurent Freidel, Perimeter Institute for Theoretical Physics; Carlo Rovelli, Centre de Physique Théorique, Aix-Marseille Université and Université de Toulon; and Sebastian Steinhaus, Perimeter Institute for Theoretical Physics.
    Students in the Quantum Gravity Summer School at Bard College.
    Students in the Quantum Gravity Summer School at Bard College.

    Carlo Rovelli, world-renowned scientist and best-selling author, will give a public lecture, “What Is Time?,” in Olin Hall on Thursday, June 13, at 7:00 p.m. as part of the weeklong program. Rovelli is a member of the faculty at Centre de Physique Théorique de Aix-Marseille Université et Université de Toulon, France. Rovelli writes of his upcoming lecture:
    Time is a mystery that does not cease to puzzle us. Philosophers, artists and poets have long explored its meaning while scientists have found that its structure is different from the simple intuition we have of it. From Boltzmann to quantum theory, from Einstein to loop quantum gravity, our understanding of time has been undergoing radical transformations. Time flows at a different speed in different places, the past and the future differ far less than we might think, and the very notion of the present evaporates in the vast universe.
    The event is free and open to the public, but reservations are required. Reserve a seat by emailing Hal Haggard (hhaggard@bard.edu). Doors open at 6:30 p.m. This event is sponsored by the Physics Program.


    — Further Reading —

    Jim Bardeen, Hal Haggard, and Carlo Rovelli, faculty members in the Bard Summer School on Quantum Gravity, weigh in on “White Holes: Black Holes’ Neglected Twins,” in Space.

     
    Read More

    Post Date: 06-09-2019
  • Bard Alum, Physics PhD Candidate Ingrid Stolt ’15 on the Magic of Magnets

    Bard Alum, Physics PhD Candidate Ingrid Stolt ’15 on the Magic of Magnets

    At age seven, Bard alum Ingrid Stolt ’15 fell in love with the magnets on her parents’ refrigerator: “I used to pretend that one magnet was a magic wand that was causing the other to move back and forth and rotate through supernatural powers. Magnetism seemed magical because it was so mysterious, yet I wanted to understand how it worked.” Today, she's a fourth-year doctoral student in physics, helping to develop practical uses for superconductivity at Northwestern's Nuclear Magnetic Resonance Laboratory.
    Full story at Helix Magazine

    Post Date: 02-28-2019
  • Early College Alumna Raspberry Simpson Is Developing the Fuel of the Future at MIT

    Early College Alumna Raspberry Simpson Is Developing the Fuel of the Future at MIT

    Raspberry Simpson, Bard College at Simon’s Rock alumna, Class of 2008, is pursuing her PhD at MIT and working on the development of fusion power.
    Full story at MIT News

    Post Date: 02-19-2019
  • Bard Physicist Hal Haggard Coauthors Study on the Holographic Description of 4-D Spacetime

    Bard Physicist Hal Haggard Coauthors Study on the Holographic Description of 4-D Spacetime

    Building on previous work in three dimensions, the study provides a new route to a complete boundary description of four-dimensional spacetime.
    Read article in the Journal of High Energy Physics

    Post Date: 01-29-2019

Physics Events

There are no events to display.
2020
  
2019
  
2018
  
2017
  
View Full Archive


2017

Tuesday, December 19, 2017
Reem-Kayden Center  6:30 pm EST/GMT-5
Join our December graduating seniors in presenting their senior projects


Friday, December 15, 2017
Kim K. McLeod, Wellesley College
Hegeman 107  12:00 pm EST/GMT-5
With over 3500 planets now detected around other stars, you might think that we’ve seen it all.  However, each new exoplanet survey turns up exotic worlds that challenge our notions of how solar systems form and evolve.  One such survey is the Kilodegree Extremely Little Telescope (KELT) survey, which has a knack for finding giant planets very close to their hot host stars.  I will describe recent KELT discoveries, including one giant planet that is hotter than most stars, and will explain how new kinds of analyses are uncovering a population of giant planets on highly-tilted orbits that suggest we have much yet to learn about the dynamical evolution of planetary systems.  I’ll also offer a glimpse into the workings of a modestly-sized telescope at a small college and will describe how my own crew of Wellesley undergraduates contributes to KELT discoveries.


Friday, December 8, 2017
Cecilia Levy, SUNY Albany

 

Hegeman 107  12:00 pm EST/GMT-5
The quest for dark matter is one of particle physics most active research areas today. Despite the overwhelming amount of evidence that it exists and makes up to 25% of the universe, a dark matter particle has yet to be detected. While over the years, many different experiments using many different technologies have emerged, liquid xenon detectors have now proven their superiority in leading the field of direct dark matter detection. However, as they need to become bigger and bigger to be more and more sensitive, the current detectors are reaching the limit of irreducible backgrounds, and thus are reaching the end of their detection ability. Therefore new, improved detectors must be invented which will not only address the background issues that current detectors face but also probe new, until now inaccessible, search areas, thus opening a new era for DM detection.


Friday, December 1, 2017
David Kagan, University of Massachusetts-Dartmouth
Hegeman 107  12:00 pm EST/GMT-5
String theory's roots date back to the 1960's in attempts to determine the nature of the strong interaction using S-matrix techniques. The goal was to "bootstrap" to a nearly unique theory using a small, simple set of physical principles, and avoiding the use of quantum fields entirely. Many beautiful results emerged, but the program ultimately fizzled with the success of quantum chromodynamics (QCD). String theory however, has always remained deeply connected to the S-matrix approach and recent developments have inspired a renewed interest in the S-matrix, particularly as a tool for constraining the possible quantum field theories that might be consistently completed into a theory of quantum gravity at high enough energies. In this talk, I will provide an overview of key developments early in the formulation of string theory and describe some exciting new no-go results that have emerged hinting that string theory may indeed be "the only game in town" (modulo important assumptions!).


Friday, November 17, 2017
Matthew Deady & Paul Cadden-Zimansky
Physics Program, Bard College

Hegeman 107  12:00 pm EST/GMT-5
Where does Bard get its energy from now, and where will it come from in the future?  This seminar features two short presentations examining both near-term, small-scale changes (microhydroelectric power from the Sawkill) and constraints on long-term planning (how could Bard become carbon neutral by 2035?).  An informal discussion over pizza of prospects and challenges concerning energy production follows the presentations.


Friday, November 3, 2017
David Helfand, Columbia University
Hegeman 107  12:00 pm EST/GMT-5
Over the past ten years, my colleagues and I have been using the Very Large Array radio telescope to construct by the far highest resolution survey yet made of our Galaxy at centimeter wavelengths. The images reveal thousands of Galactic radio emitters which mark the places of stellar birth in cold clouds of  gas and dust, and stellar death in the violent explosions of supernove. Combining this survey with data from other wavelengths, particularly the Spitzer Space Observatory's Infrared survey of the Galaxy provides a spectacular new multi-colored view of the Milky Way and reveals a number of unexpected surprises.

 


Friday, October 13, 2017
Peter J. Collings
Department of Physics & Astronomy, Swarthmore College

 

Hegeman 107  12:00 pm EST/GMT-5
The liquid crystals used in displays are oily fluids in which the molecules possess orientational order.  Another class of liquid crystals relies on the spontaneous formation of molecular assemblies when certain dyes and drugs are dissolved in water.  These aqueous systems are the subject of significant scientific research, due to the possibility of applications in biology and medicine.  This research reveals that water-based liquid crystals behave quite differently from their oily counterparts, thus creating the understanding necessary to develop new techniques and devices in an area where liquid crystals have had little impact.

 


Friday, October 6, 2017
Antonios Kontos
Physics Program

Hegeman 107  12:00 pm EST/GMT-5
The 2017 Nobel Prize in Physics was awarded to Rainer Weiss, Kip Thorne and Barry Barish for the conception, construction and operation of the LIGO detector that detected Gravitational Waves for the first time. Considering the impossibly weak nature of gravitational waves, this was a monumental achievement of experimental ingenuity which has now opened a new type of window to the Universe (a microphone really). I will go through how the detectors work, what Gravitational Waves tell us about the universe and some personal experiences from being part of the collaboration.


Friday, September 29, 2017
  Gravitational lensing, hydroelectric generators, and better electric guitars. 
Hegeman 107  12:00 pm EST/GMT-5
Come check out what physics senior projects are in the works for this year over a pizza lunch.


Thursday, September 28, 2017
Reem-Kayden Center  6:00 pm EST/GMT-5

Friday, September 15, 2017
Required of All Students Working or Doing Research in the Lab
Reem-Kayden Center Laszlo Z. Bito '60 Auditorium  4:00 pm EST/GMT-5
If you previously attended a lab training session this year, you do not need to attend again. If you are unsure, please contact Maureen O’Callaghan-Scholl with questions at ocalla@bard.edu.

Friday, September 8, RKC 103, 4 p.m.
Friday, September 15, RKC 103, 4 p.m.


Friday, September 15, 2017
Hegeman 107  12:00 pm EST/GMT-5
From gravitational microlensing of distant planets to microhydro power on the Sawkill, come enjoy pizza and students discussing their summer research.


Friday, September 8, 2017
Required of All Students Working or Doing Research in the Lab
Reem-Kayden Center Laszlo Z. Bito '60 Auditorium  4:00 pm EST/GMT-5
If you previously attended a lab training session this year, you do not need to attend again. If you are unsure, please contact Maureen O’Callaghan-Scholl with questions at ocalla@bard.edu.

Friday, September 8, RKC 103, 4 p.m.
Friday, September 15, RKC 103, 4 p.m.


Friday, September 8, 2017
  Come learn what's happening in the Physics Program this semester, welcome new students and faculty into the Program, and enjoy a pizza lunch.
Hegeman 107  12:00 pm EST/GMT-5

Thursday, July 20, 2017
  Ilya R. Fischhoff
Postdoctoral Associate
Cary Institute for Ecosystem Studies

Reem-Kayden Center Laszlo Z. Bito '60 Auditorium  3:00 pm EST/GMT-5
Ilya Fischhoff is a postdoctoral fellow with The Tick Project (www.tickproject.org). The Tick Project is a 5-year study to determine whether controlling ticks at the neighborhood scale reduces tick-borne diseases in people. One of the tick control methods that The Tick Project is evaluating is Met52, a biopesticide containing spores of a tick-killing fungus. In assessing Met52, it is important to evaluate not only its efficacy in reducing tick-borne disease but also its impacts on non-target organisms. Ilya will present results from an experiment he conducted last summer to assess the effects of Met52 on non-target arthropods in lawn and forest habitats typical of residential yards. Ilya sampled arthropods on treatment and control plots, before and after spray with Met52 on the treatment plots or water on the control plots. Ilya used multivariate models to analyze the data on arthropod abundance in 25 taxonomic orders. There were significant effects of plot location, period (before vs. after spray) and habitat (lawn vs. forest), but no effect of treatment (Met52 vs. water). A retrospective power analysis showed that the study had an 80% chance of detecting a reduction in arthropod abundance of 55% or greater. Based on these results, Ilya and his collaborators concluded that the use of Met52 in suburban yards is unlikely to cause meaningful reductions in the abundance of non-target arthropods. Finally, Ilya will also talk briefly about a microcosm experiment he is setting up to examine interactions among Met52, ticks, and brush-legged wolf spiders, a natural enemy of ticks.
 

Thursday, July 13, 2017
Jeremy R. Manning, Ph.D.
Assistant Professor of Psychological & Brain Sciences
Dartmouth College

Reem-Kayden Center Laszlo Z. Bito '60 Auditorium  3:00 pm EST/GMT-5
Our memory systems leverage the statistical structure of the world around us (context) to organize and store incoming information and retrieve previously stored information.  This enables us to recognize the situations we are in and to adapt our behaviors accordingly.  For example, your might choose to behave differently on a road trip with close friends versus commuting into work with your boss, even though many aspects of your perceptual experience are preserved across those two scenarios.  You might also remember different aspects of conversations from those trips when asked about them later.

In my talk, I will explore the extent to which (and the circumstances under which) these sorts of processes may be manipulated to influence memory.  I’ll begin by exploring these processes using a simple word list learning paradigm.  I’ll show how we can influence memory performance (specifically, how many words people remember and the order people remember the words in).  Then I’ll talk about how these same ideas can be applied to “naturalistic” memories, such as memories for scenes in a movie or concepts learned in the classroom.


Thursday, July 6, 2017
  Antonios Kontos, Physics program
Reem-Kayden Center Laszlo Z. Bito '60 Auditorium  3:00 pm EST/GMT-5
With three detections and counting, the Advanced LIGO gravitational-wave observatories have opened a new window into the Universe. For now, all the detected gravitational-waves originated from collisions of two black holes. The effect that these gravitational-waves have as they pass through space is to stretch and compress space-time, much like sound waves stretch and compress the air. To understand the challenge of detecting this effect here on Earth, imagine (if you can) that a reasonably strong gravitational wave changes the length of one kilometer by one thousandth of a proton's diameter. At this level of sensitivity, quantum mechanics and the Heisenberg uncertainty principle start playing a significant role and if we want to listen further into the Universe, we need to manipulate the quantum nature of light to our advantage. In this talk I will give an overview of gravitational waves, how LIGO detects them, and why quantum mechanics matters when measuring distances with such precision.


Thursday, June 15, 2017
  Michael Bergman
Emily H. Fisher Professor of Physics
Bard College at Simon's Rock

Reem-Kayden Center Laszlo Z. Bito '60 Auditorium  3:00 pm EST/GMT-5
Earth's iron alloy inner core was not discovered until 1936-six years after the discovery of Pluto. For many years after that little was known about this most remote part of our planet, but in the last thirty years seismologists have been revealing it has some unusual properties. The cause of these seismic inferences remains uncertain, but they provide clues about the mineral physics and dynamics of the core. This talk will review the seismic observations of the inner core, and discuss their implications for its evolution.


Friday, May 19, 2017
Eleni-Alexandra Kontou
Physics Program

Hegeman 107  12:00 pm EST/GMT-5
We can only perceive four dimensions, but several standard model extensions suggest the existence of more. If that’s true, why can't we see them? One possible explanation is that these extra dimensions are compactified, meaning they have a finite length compared to the infinite standard four. Cosmology offers a very interesting possibility of finding evidence for the existence of these extra dimensions in the Cosmic Microwave Background (CMB). The CMB is an echo from the Big Bang era, and can give us important insight to the past of our universe and whether it could have included compactified dimensions.


Thursday, May 18, 2017
Reem-Kayden Center  6:30 pm EST/GMT-5
Join Science, Mathematics & Computer graduating seniors in presenting their senior projects.


Tuesday, May 16, 2017
Montgomery Place, Mansion  8:30 pm – 10:00 pm EST/GMT-5
Join us at the Montgomery Place visitor center for a short talk by Prof. Eleni Kontou on the the latest science from NASA’s Juno probe of Jupiter, followed by telescope viewing of Jupiter and its moons, a guided tour of the night sky, and a round of Ask-a-Physicist-Anything.

Buses to the event leave from the Kline South stop at 8:15 pm and 8:30 pm.

Clear weather permitting.


Friday, May 12, 2017
Daniel Marlow, Princeton University
Hegeman 107  12:00 pm EST/GMT-5
Radio astronomy has greatly enhanced the range of observable astronomical phenomena.  Although a wide range of wavelengths are used in radio astronomy, one of the most important is 21 cm, which corresponds to the hyperfine transition in atomic hydrogen.   Although the 21 cm signal from a small collection of hydrogen atoms is exceedingly weak, and the density of hydrogen in the Milky Way is very low, the Galaxy is a big place and contains enough hydrogen to produce a signal that can be detected with a modest terrestrial apparatus.    In this talk, I will present results obtained at 21 cm with a recently refurbished cold-war-era 60-foot dish antenna.   Data from the dish will be used to measure the Sun's velocity with respect to the average velocity of nearby stars and to infer the existence of dark matter.    Time permitting, pulsar signals will be presented and schematic plans for a kit capable of detecting indirect evidence for dark matter for costing less than $1000 will be presented.


Friday, April 28, 2017
Edward Marti
Joint Institute for Laboratory Astrophysics
University of Colorado

 

Hegeman 107  12:00 pm EST/GMT-5
The accuracy of atomic clocks has improved a thousandfold over the last 15 years. The latest generation of atomic clocks, called "optical lattice clocks", can detect changes in general relativity's gravitational redshift over a few centimers. These clocks use extremely stable lasers to count the "ticks" of an optical-frequency transition in atoms cooled to the nanokelvin regime, reaching 18 digits of accuracy in a few hours. In this talk, I will discuss how we achieve this accuracy through exquisite control of the quantum mechanical state of these ultracold atoms, and how we are using these clocks to search for dark matter and test relativity.


Friday, April 7, 2017
  Matthew Deady, Physics Program
Hegeman 107  12:00 pm EST/GMT-5
In the summer of 2012, two teams of scientists working on the Large Hadron Collider in Switzerland announced that they had discovered the long-awaited Higgs Boson.  What is this particle?  Why do physicists think is it so important?  How was it predicted?  How was it discovered?  What are the implications to our understanding of matter, energy, and the universe?  These and other questions will be addressed as we investigate the fundamental particles and forces that underlie all physical phenomena, culminating in the Higgs discovery and consideration of what might be beyond.


Friday, March 10, 2017
Joshua Cooperman, Physics Program

 

Hegeman 107  12:00 pm EST/GMT-5
Quantum gravity is the much sought-after synthesis of quantum mechanics and general relativity, the two pillars of contemporary physics. I will deliver an accessible introduction to the promising approach to quantum gravity called causal dynamical triangulations. Founding my presentation on the quantum mechanics of a particle, I will build an intuitive conception of the quantum mechanics of spacetime. I will survey the key results deriving from causal dynamical triangulations and broach the key question facing causal dynamical triangulations.

 


Friday, March 3, 2017
Eric L. N. Jensen
Swarthmore College

Hegeman 107  12:00 pm EST/GMT-5
Since the discovery of the first extrasolar planet a little more than 20 years ago, the list of known planets orbiting other stars has grown to more than 3,000—but we are still in the early stages of understanding the diversity of other planetary systems.  A key part of this understanding has come from studies of planets that eclipse (or “transit”) their host stars as seen from Earth.   I will explain how studies of these planets allow us to determine their radii, masses, mean densities, atmospheric composition, and the angle at which they orbit relative to the parent star’s equator, all without being able to image the planets directly.  Small telescopes (with primary mirror diameters of 0.3–1 meter) play an important role in the larger “ecosystem” of telescopes that discover and characterize these planets, and such telescopes have been instrumental in the recent discoveries of planets around very bright stars that are much hotter than the Sun, and in the just-announced discovery of seven Earth-radius planets around the ultra-cool dwarf star Trappist-1.


Friday, February 24, 2017
James Lowenthal, Smith College
Hegeman 107  12:00 pm EST/GMT-5
I’ll give an overview of observing at the 50-m Large Millimeter Telescope and will focus on the latest results on distant, dusty, massive starburst galaxies in the early universe.  Studying distant galaxies lets us peer billions of years back in time, well over halfway back to the Big Bang, to learn how galaxies form and evolve.  New infra-red and millimeter-wave images and spectra from the Planck and Herschel satellites and from the LMT have helped identify the most luminous galaxies yet known, thousands of times brighter than our own Milky Way, and churning gas into new stars at a furious rate.  Many are also strongly gravitationally lensed, their images warped and amplified by intervening massive galaxies, which lets us see more detail on fainter galaxies than usual.  Hubble Space Telescope’s sharp vision further enhances our view and can finally reveal what triggers such spectacular starburst activity. 


Thursday, February 16, 2017
Zammy Diaz
Columbia University Institute of Human Nutrition

Campus Center Lobby  11:00 am – 1:00 pm EST/GMT-5
Join Zammy Diaz, IHN Communications Center, to learn why the one-year MS Program in Nutrition Science may be a great gap or glide year for you.


Friday, February 3, 2017
Paul Cadden-Zimansky
Physics Program

Hegeman 102  12:00 pm EST/GMT-5
The development of almost all modern technology relies on a firm understanding of the concepts of electricity and magnetism, and these concepts are at the heart of fundamental explanations of most physical phenomena. The historical evolution of these concepts traces back thousands of years and took a number of surprising, unorthodox, and occasionally tragic turns before the rules governing electricity and magnetism were codified. In this talk, intended for a general audience, I'll review some of the key experiments and insights of past centuries that led to our present theories.

Physics Program Social and Lunch to Follow


Discover Physics at Bard

Hal Haggard, Director
Physics Program
Bard College | PO Box 5000
Annandale-on-Hudson, NY 12504
haggard@bard.edu | 845-758-7302
Bard College
Campus Road, PO Box 5000
Annandale-on-Hudson, New York 12504-5000
Phone: 800-BARDCOL
Admission Phone: 845-758-7472
Admission E-mail: admission@bard.edu
©2020 Bard College
Follow Us on Twitter
Like us on Facebook
Follow Us on Instagram
You Tube
Information For:
Prospective Students
Current Employees
Alumni/ae 
Families
Quick Links
Employment
Travel to Bard
Site Search
Support Bard