Physics

News & Events

Tuesday, October 22, 2019

Chemistry Study Room 

Peed led study space for Chemistry 


Time: 5:00 pm – 10:00 pm
Location: RCK Chemistry pods
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Tuesday, October 22, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Wednesday, October 23, 2019

Chemistry Study Room 

Peed led study space for Chemistry 


Time: 5:00 pm – 10:00 pm
Location: RCK Chemistry pods
E-mail to Friend

Wednesday, October 23, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
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Friday, October 25, 2019

I Work with Magnets: Nuclear Magnetic Resonance Studies of High-temperature Superconductors

 

Ingrid StoltBard class of 2015, Northwestern University


Time: 12:00 pm – 1:00 pm
Location: Hegeman 107
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Friday, October 25, 2019

Summer Research Poster Session

Join faculty and students who participated in this year’s program in presenting their work
Time: 4:00 pm – 6:00 pm
Location: Reem-Kayden Center
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Sunday, October 27, 2019

Chemistry Study Room

Peer-led Chemistry study space


Time: 12:00 pm – 2:00 pm
Location: RCK Chemistry Pods
E-mail to Friend

Sunday, October 27, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Monday, October 28, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Tuesday, October 29, 2019

Chemistry Study Room 

Peed led study space for Chemistry 


Time: 5:00 pm – 10:00 pm
Location: RCK Chemistry pods
E-mail to Friend

Tuesday, October 29, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Wednesday, October 30, 2019

Chemistry Study Room 

Peed led study space for Chemistry 


Time: 5:00 pm – 10:00 pm
Location: RCK Chemistry pods
E-mail to Friend

Wednesday, October 30, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
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Thursday, October 31, 2019

The Jefferson Project: Integrating Science and Technology for Enduring Lake Protection

 

Rick Relyea, Director, The Jefferson ProjectRensselaer Polytechnic Institute


Time: 12:00 pm – 1:00 pm
Location: Reem-Kayden Center Laszlo Z. Bito '60 Auditorium
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Sunday, November 3, 2019

Chemistry Study Room

Peer-led Chemistry study space


Time: 12:00 pm – 2:00 pm
Location: RCK Chemistry Pods
E-mail to Friend

Sunday, November 3, 2019

Chemistry Study Room

Peer-led Chemistry study space


Time: 12:00 pm – 2:00 pm
Location: RCK Chemistry Pods
E-mail to Friend

Sunday, November 3, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Sunday, November 3, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Monday, November 4, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Tuesday, November 5, 2019

Chemistry Study Room 

Peed led study space for Chemistry 


Time: 5:00 pm – 10:00 pm
Location: RCK Chemistry pods
E-mail to Friend

Tuesday, November 5, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Wednesday, November 6, 2019

Chemistry Study Room 

Peed led study space for Chemistry 


Time: 5:00 pm – 10:00 pm
Location: RCK Chemistry pods
E-mail to Friend

Wednesday, November 6, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Thursday, November 7, 2019

DNA Repair: Why Do We Care?

 

Paula Checchi, Marist College


Time: 12:00 pm – 1:00 pm
Location: Reem-Kayden Center Laszlo Z. Bito '60 Auditorium
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Thursday, November 7, 2019

Taking a Symptom Level Approach to Depression

 

Michael MullarkeyUniversity of Texas-Austin


Time: 4:45 pm – 6:00 pm
Location: Preston Theater
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Friday, November 8, 2019

Controlling Hybrid States of Light and Matter in Atomically-thin Semiconductors

Trevor LaMountain, Northwestern University

Interactions between light and matter underlie a variety of everyday technologies. Typical examples include solar cells, where light is absorbed and converted to electronic energy, and LEDs, where the opposite occurs. By embedding semiconductors in between two mirrors, we can greatly enhance the light-matter interaction, giving rise to much more exotic effects than just absorption or emission. Under certain conditions these systems can form hybrid quantum states known as “polaritons,” which exhibit properties of both light and matter. In a different regime, off-resonant light can cause the electronic energy levels to shift with negligible absorption. Known as the optical Stark effect, this feature provides a way to precisely control the energy levels of semiconductors using only light. In this talk, I will introduce the closely-related physics that describes both polariton formation and the optical Stark effect. I will then discuss some interesting features of both of these phenomena in atomically-thin semiconductors. Finally, I will present resent results that combine both of these regimes by demonstrating the optical Stark shift of exciton-polaritons in atomically-thin semiconductors.

 
Time: 12:00 pm – 1:00 pm
Location: Hegeman 107
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Sunday, November 10, 2019

Chemistry Study Room

Peer-led Chemistry study space


Time: 12:00 pm – 2:00 pm
Location: RCK Chemistry Pods
E-mail to Friend

Sunday, November 10, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Monday, November 11, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Tuesday, November 12, 2019

Chemistry Study Room 

Peed led study space for Chemistry 


Time: 5:00 pm – 10:00 pm
Location: RCK Chemistry pods
E-mail to Friend

Tuesday, November 12, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Wednesday, November 13, 2019

Chemistry Study Room 

Peed led study space for Chemistry 


Time: 5:00 pm – 10:00 pm
Location: RCK Chemistry pods
E-mail to Friend

Wednesday, November 13, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Thursday, November 14, 2019

How to Plan a Meaningful Summer

Felicia KeesingBiology Program


Time: 12:00 pm – 1:00 pm
Location: Reem-Kayden Center Laszlo Z. Bito '60 Auditorium
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Thursday, November 14, 2019

Psychology Internship Panel

Listen to students and alums who have participated in summer internships discuss their experiences, and learn about opportunities for the coming year. There will be an opportunity for Q&A as well as hearing about different internship opportunities.
Time: 4:45 pm – 6:00 pm
Location: Preston Theater
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Friday, November 15, 2019

Mapping Matter in Strong Gravity: Spectral-Timing of Black Holes and Neutron Stars

 

Abigail Stevens, ’11Michigan State University

One of the best laboratories to study strong-field gravity is the inner 100s of kilometers around black holes and neutron stars in binary systems with low-mass stars like our Sun. The X-ray light curves of these binary systems show variability on timescales from milliseconds to months — the shorter (sub-second) variability can appear as quasi-periodic oscillations (QPOs), which may be produced by general relativistic effects. My research looks at QPOs from black holes and neutron stars (as well as coherent X-ray pulsations from neutron stars) by fitting the phase-resolved energy spectra of these signals to constrain their physical origin and track their evolution in time. In this talk, I will introduce why black holes and neutron stars are interesting and discuss state-of-the-art “spectral-timing” analysis techniques for understanding more about them. I will also highlight open-source astronomy research software and the importance of mental wellbeing among students and early-career researchers.
Time: 12:00 pm – 1:00 pm
Location: Hegeman 107
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Sunday, November 17, 2019

Chemistry Study Room

Peer-led Chemistry study space


Time: 12:00 pm – 2:00 pm
Location: RCK Chemistry Pods
E-mail to Friend

Sunday, November 17, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Monday, November 18, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Tuesday, November 19, 2019

Chemistry Study Room 

Peed led study space for Chemistry 


Time: 5:00 pm – 10:00 pm
Location: RCK Chemistry pods
E-mail to Friend

Tuesday, November 19, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Wednesday, November 20, 2019

Chemistry Study Room 

Peed led study space for Chemistry 


Time: 5:00 pm – 10:00 pm
Location: RCK Chemistry pods
E-mail to Friend

Wednesday, November 20, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Thursday, November 21, 2019

Special Case Investigations in Virology:
Finding the Unexpected

Daryl Lamson, New York Department of Health


Time: 12:00 pm – 1:00 pm
Location: Reem-Kayden Center Laszlo Z. Bito '60 Auditorium
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Friday, November 22, 2019

Solar Microgrid Applications for Emerging Economies

Megan Kerins, ’06, Rocky Mountain Institute


Time: 12:00 pm – 1:00 pm
Location: Hegeman 107
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Sunday, November 24, 2019

Chemistry Study Room

Peer-led Chemistry study space


Time: 12:00 pm – 2:00 pm
Location: RCK Chemistry Pods
E-mail to Friend

Sunday, November 24, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Monday, November 25, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Tuesday, November 26, 2019

Chemistry Study Room 

Peed led study space for Chemistry 


Time: 5:00 pm – 10:00 pm
Location: RCK Chemistry pods
E-mail to Friend

Tuesday, November 26, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Wednesday, November 27, 2019

Chemistry Study Room 

Peed led study space for Chemistry 


Time: 5:00 pm – 10:00 pm
Location: RCK Chemistry pods
E-mail to Friend

Wednesday, November 27, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Sunday, December 1, 2019

Chemistry Study Room

Peer-led Chemistry study space


Time: 12:00 pm – 2:00 pm
Location: RCK Chemistry Pods
E-mail to Friend

Sunday, December 1, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Monday, December 2, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Tuesday, December 3, 2019

Chemistry Study Room 

Peed led study space for Chemistry 


Time: 5:00 pm – 10:00 pm
Location: RCK Chemistry pods
E-mail to Friend

Tuesday, December 3, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Wednesday, December 4, 2019

Chemistry Study Room 

Peed led study space for Chemistry 


Time: 5:00 pm – 10:00 pm
Location: RCK Chemistry pods
E-mail to Friend

Wednesday, December 4, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
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Thursday, December 5, 2019

Social Work, Mental Health, and Academic Behavioral Medicine: A Social Justice Approach to Clinical Practice, Research, and Teaching in Graduate Medical Education

Cynthia Kim, LCSW-R, Associate Program Director and Director of Behavioral Science, and Michelle Miller, LCSW, Behavioral Science Faculty and Mental Health Clinicia, Mid Hudson Family Medicine Residency Program – Institute for Family Health

Alternate pathways for using undergraduate psychology education and experience exist in multiple professional realms. One such pathway is in using a graduate degree in social work or psychology to transform, teach, and practice in the field of academic family medicine. Family doctors are at the forefront of research and practice in the evidence base that informs integrative healthcare, providing services ranging from care coordination to mental health—all predicated on the development of trauma-informed, culturally conscious, therapeutic relationships with their patients. This talk will provide insight into a social justice pathway and mission that hopes to help transform the future of health and mental health care.
Time: 4:45 pm – 6:00 pm
Location: Preston Theater
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Friday, December 6, 2019

From Structure to Function: Optics in the Sea

Amanda JonesUniversity of Pennsylvania


Time: 12:00 pm – 1:00 pm
Location: Hegeman 107
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Sunday, December 8, 2019

Chemistry Study Room

Peer-led Chemistry study space


Time: 12:00 pm – 2:00 pm
Location: RCK Chemistry Pods
E-mail to Friend

Sunday, December 8, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Monday, December 9, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Tuesday, December 10, 2019

Chemistry Study Room 

Peed led study space for Chemistry 


Time: 5:00 pm – 10:00 pm
Location: RCK Chemistry pods
E-mail to Friend

Tuesday, December 10, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Wednesday, December 11, 2019

Chemistry Study Room 

Peed led study space for Chemistry 


Time: 5:00 pm – 10:00 pm
Location: RCK Chemistry pods
E-mail to Friend

Wednesday, December 11, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Friday, December 13, 2019

Stacking Van der Waals Atomic Layers: Quest for New Materials by Designing

Philip Kim, Harvard University


Time: 12:00 pm – 1:00 pm
Location: Hegeman 107
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Sunday, December 15, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Monday, December 16, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Tuesday, December 17, 2019

Chemistry Study Room 

Peed led study space for Chemistry 


Time: 5:00 pm – 10:00 pm
Location: RCK Chemistry pods
E-mail to Friend

Tuesday, December 17, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Wednesday, December 18, 2019

Chemistry Study Room 

Peed led study space for Chemistry 


Time: 5:00 pm – 10:00 pm
Location: RCK Chemistry pods
E-mail to Friend

Wednesday, December 18, 2019

Math Study Room

SUNDAY–WEDNESDAY  •  HEG 308  •  7–10 PM

A place to work on math homework, study with classmates, or speak to a math tutor.
Time: 7:00 pm – 10:00 pm
Location: Hegeman 308
E-mail to Friend

Friday, January 10, 2020

First Citizen Science Class

Location: Bard College Campus
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Friday, January 10, 2020

Citizen Science Classes Begin

Mandatory check-in 10 am – 4 pm
RKC lobby - financial clearance, materials pick up, water test tube collection
Time: 10:00 am – 4:00 pm
Location: Bard College Campus
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Sunday, January 12, 2020

From Crises to Solutions: Drinking Water in the Twenty-First Century

Lecture by David Sedlak, author of Water 4.0


As a result of population growth, climate change, and pollution, the world’s drinking water supplies are under considerable stress. Over the past four decades, engineers and scientists working in water-stressed cities have created an array of new technologies that make it possible to purify water that would otherwise be unsafe to drink. However, the high cost and inflexibility of these systems currently prevents their use in all but the wealthiest cities. To expand access of these technologies to overcome the drinking water crises facing humanity, creative new policies and additional technological improvements will be needed. This talk will provide insight into the challenge of providing safe, affordable, and reliable drinking water in the coming decades. 
 
Time: 7:15 pm – 9:30 pm
Location: Fisher Center, Sosnoff Theater
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Monday, January 13, 2020 – Friday, January 17, 2020

Citizen Science Classes

Times vary by section. Two classes each day, approximately 2.5 hours per class. Classes will be held between 9:00 am and 5:00 pm.
  Location: Bard College Campus
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Tuesday, January 21, 2020 – Thursday, January 23, 2020

Citizen Science Classes

Times vary by section. Two classes each day, approximately 2.5 hours per class. Classes will be held between 9:00 am and 5:00 pm.
  Location: Bard College Campus
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Past Events

  • 2019
  • 2018
  • 2017
  • 2016
  • 2015
  • 2014
  • 2013
  • 2012
  • 2011
  • 2010
  • 2009
  • 2008

    • 2014

      Senior Project Poster Session

      December 11
      Reem-Kayden Center

      Students presenting: 

      Oliver Bruce, Michael DiRosa, Jacob Fauber, Andy Huynh, Caitlin Majewski, Henry Meyers, Cameron West, Clare Wheeler

      Advisers:
      Rebecca Thomas, Matthew Deady, Keith O’Hara, James Belk, Csilla Szabo, Sven Anderson, Sarah Dunphy-Lelii, Christopher LaFratta



      Watching the Wave Function Collapse

      December 3
      Hegeman 107

      Recent advances in superconducting quantum bits and quantum limited amplifiers have enabled a number of experiments that probe fundamental questions in quantum optics, open quantum systems, and continuous measurement. I will describe recent experiments where we use weak, continuous measurement to monitor the evolution of a superconducting qubit as it evolves in competition between driven evolution and the random evolution associated with measurement. By tracking individual quantum trajectories that evolve between an arbitrary choice of initial and final states we can deduce the most probable path through quantum state space. These results reveal the rich interplay between measurement dynamics, typically associated with wave function collapse, and unitary evolution of the quantum state as described by the Schrödinger equation.


      Using the Earth as a Polarized Electron Source to Search for Long-Range Spin-Spin Interactions

      November 19
      Hegeman 107

      Many extensions of the standard model of particle physics predict the existence of long-range spin-spin interactions. We have developed an approach which uses the Earth as a polarized spin source to investigate these interactions.  We combine recent deep-Earth geophysics and geochemistry results with precise tabulations of the geomagnetic field to create a comprehensive map of electron polarization within the Earth.  We examine possible long-range interactions between these spin-polarized geoelectrons and the spin-polarized electrons and nucleons in three laboratory experiments.  By combining our model and the results from these experiments we establish new stringent bounds on torsion gravity and possible long-range spin-spin forces associated with the virtual exchange of either spin-one axial bosons or unparticles.  The resulting bound on the spin-spin force between an electron and a neutron is one million times smaller than their gravitational attraction.



      Believing We're Seeing the Big Bang*
      (*or, a time shortly thereafter)

      November 12
      Hegeman 107

      Not long after the Big Bang (in cosmic time), the universe went through a transition from being filled with hot, glowing, opaque plasma to being a dark and transparent nursery for the formation of stars and galaxies. An afterglow of light from that early plasma epoch still lingers, giving us a glimpse of a very different universe more than thirteen billion years ago. Observations of this microwave-wavelength light (called the Cosmic Microwave Background, or CMB) have enabled profound insights into cosmic structure and history and helped to establish the current standard cosmological model.  

      In recent years, some of the most important CMB discoveries have been made by ground-based telescopes, including the South Pole Telescope. Studying the CMB from the ground is exceptionally difficult because the earth's atmosphere glows in microwaves — ten million times brighter than the faint signals we hope to discern from deep space. In this talk I will describe some clever observing and data analysis tricks we use to disentangle CMB signal from atmospheric noise, and reveal what goes on behind the scenes to turn raw and messy South Pole Telescope data into something we "believe" — compelling new evidence to test and refine cosmological models.


      Quantum Mechanics in Non-Inertial Reference Frames

      October 22
      Hegeman 107

      Among the key physical principles that underlie quantum mechanics are the principle of superposition (quantum states can be combined to produce other states) and the principle of relativity (all inertial reference frames are equivalent). These two principles are synthesized and implemented in quantum theory by means of unitary representations of the relevant spacetime symmetry group—Galilei group in the nonrelativistic case and the Poincare group in the relativistic case. In fact, much of the essential structure of quantum mechanics is determined by these group representations. They provide us with a means to derive and understand emblematic features of the theory, such as the Heisenberg commutation relations, Schrodinger equation and discrete values of angular momentum.  However, since the principle of relativity as encoded in Galilei and Poincare groups is a statement about inertial reference frames, a quantum theory based on these groups is also a theory, much like Newton's mechanics,  that holds in inertial reference frames. In this talk, I will present my recent attempts to expand the notion of relativity to include accelerating, noninertial reference frames and develop a quantum theory grounded on the unitary representations of the groups of transformations that tie together noninertial reference frames. I will discuss how the resulting formalism allows us to understand the nature and role of some signature features of noninertial reference frames, including fictitious forces and the equivalence principle,  in the quantum setting.

      The Invention of Blue: The 2014 Nobel Prize in Physics

      October 15
      Hegeman 107

      Fall in the Hudson Valley and the trees are displaying their full array of colors, but noticeably absent from this spectrum is blue. A similar absence had for many decades left a vacancy in the production of artificial light. While the semiconductor revolution brought with it computational advances in the form of transistors, energy advances in the form of photovoltaic solar panels, and illumination advances in the form of light emitting diodes, the creation of a solid state source of purely blue light remained elusive. In this talk I’ll give an overview of how Isamu Akasaki, Hiroshi Amano, and Shuji Nakamura, the 2014 Nobel Laureates in physics, overcame technical and non-technical barriers to create the first sources of blue light, and explain why this color holds the key to setting off a 21st century revolution in energy efficiency.


      Relaxation and Thermalization in Isolated Interacting Quantum Systems

      October 8
      Hegeman 107

      We consider one-dimensional isolated interacting quantum systems that are taken out of equilibrium instantaneously. Three aspects are addressed: (i) the relaxation process, (ii) the size of the temporal fluctuations after relaxation, (iii) the conditions to reach thermal equilibrium. The relaxation process and the size of the fluctuations depend on the interplay between the initial state and the Hamiltonian after the perturbation, rather than on the regime of the system. They may be very similar for both chaotic and integrable systems. The general picture associating chaos with the onset of thermalization is also further elaborated. It is argued that thermalization may not occur in the chaotic regime if the energy of the initial state is close to the edges of the spectrum, and it may occur in integrable systems provided the initial state is sufficiently delocalized.

      Bard Summer Research Institute Poster Session

      September 23
      Reem-Kayden Center

      Join faculty and students who participated in this year's Bard Summer Research Institute in presenting their work!


      Maker Faire!

      September 20

      The Science, Mathematics & Computing Division will be sending a bus down to the New York Hall of Science in Queens, NY on Saturday, September 20. Space on the bus is LIMITED. The bus will depart RKC promptly at 9 a.m. and return to campus at approximately 7 p.m.

      Tickets to get into the Faire and a spot in the van are $30.00.  

      CASH ONLY, EXACT CHANGE ONLY.
      Reservations will be accepted until Friday, September 12

      TO RESERVE YOUR TICKET AND A SPOT IN THE VAN, 
PLEASE SEE MEGAN KARCHER, RKC 219. Office hours are Monday-Friday, 8:00-4:00 p.m.


      Planetary Science From the Top Down:

      The Exoplanet Opportunity

      September 17
      Hegeman 107

      What started as a trickle in the mid 1990's is now a torrent, with over one thousand extrasolar planets currently known, and thousands of candidates awaiting confirmation. The study of exoplanets has already revolutionized our view of planet formation, and will soon do the same to our understanding of planetary atmospheres and interiors. The diversity of exoplanets gives us the leverage to crack hard problems in planetary science: cloud formation, atmospheric circulation, plate tectonics, etc. However, the characterization of exoplanets presents a challenge familiar to astronomers: our targets are so distant that we only see them as unresolved dots. I will describe how we can extract spatially-resolved snapshots of planets from such observations. These data are sufficient to constrain low-order climate models and therefore give us insight into the effects of clouds, heat transport, and geochemical cycling. Coarse measurements for a large number of planets are the perfect complement to detailed measurements of Solar System worlds. That is the exoplanet opportunity.

      Summer Research Presentations

      September 10
      Hegeman 107

      Quantum and Fractional Quantum Hall Effects in Hybrid Graphene
      Bard Nanolab,  Bard College
      By: Andrés Martinez de Velasco, Daniel Waldo, Maya Weingrod Sandor
      Graphene is a two-dimensional allotrope in which the classical Hall Effect exhibits a quantization of available electronic states in the material which produces ballistic--zero resistance--conduction. This can be seen in Hall voltage measurements at high magnetic fields where dips to zero in the transverse resistance and plateaus in the longitudinal resistance appear. This phenomenon is known as the Quantum Hall Effect and requires strong magnetic fields and very low temperatures for its observation. In order to study this phenomenon, samples of graphene on Boron Nitride were fabricated using a variety of techniques and procedures, ultimately yielding samples with various four terminal measurement options available.
      Transportation of Ultra-Stable Light via Optical Fiber Laser Interferometer Gravitational-Wave Observatory (LIGO)
      California Institute of Technology
      By: Emily Conant
      It has been demonstrated that polarization-maintaining single mode optical fiber can be used to transport frequency-stable light. It is desired to transport stable light to other labs in the building to serve as a frequency reference for various experiments investigating different sources of noise in gravitational-wave detectors. Stable light has been obtained from ultra-stable Fabry-P'{e}rot cavities by use of the Pound-Drever-Hall locking technique. We have mode matched stable light into the fiber and are using a double-pass acousto-optic modulator (AOM) configuration to cancel fiber phase noise. We use a beamsplitter to interfere the stable light and double passed light onto a photodiode as a homodyne detection, which is connected to a phase-locked loop (PLL) to measure the beat frequency. From there, we analyze the noise in the system by measuring the power spectral density of the PLL control signal with a spectrum analyzer. We have measured the expected dominant sources of noise in the system by using a similar PLL set-up and suppressed them.  We cancel the fiber phase noise by locking the optical beat to the signal generator in the PLL.  
      Characterization of Nanowires for Red LASER on {001} Silicon
      Center for Photonics and Multiscale Nanomaterials
      University of Michigan
      By: Trevor LaMountain
      As technology decreases in size, electronic systems, like those found on a microchip, encounter a scaling problem.  The resistance of a current carrying wire is inversely proportional to its cross-sectional area.  This large resistance in microelectronic systems leads to slower, less efficient devices.  Fortunately, photonics systems, using photons to carry information instead of electrons, do not encounter such scaling problems.  It is therefore desirable to replace certain components of microelectronic systems with photonics.  However, in order to create such an integrated system, we require a coherent light source (LASER) that can be constructed on the same {001} silicon substrate that modern microchips use.  In this talk I discuss the novel methods used to create a red-emitting laser structure on {001} silicon, and in particular highlight the material characterization methods used to measure the composition of alloys used in this device.

      Summer Research Presentations

      September 3
      Hegeman 107

      Single-molecule Conductance as a Tool for Understanding Solar Cell Efficiency
      Columbia University with the Energy Frontier Research Center 
in the Applied Physics and Mathematics Division
      By: Ingrid Stolt

      In this project, Scanning Tunneling Microscope-Break Junction (STM-BJ) techniques were used to measure the single-molecule conductance of a group of compounds each containing a different central unit (a molecule sandwiched  between a distinct pair of atom chains). Many of these central units have been implemented in the design of organic semiconductors for Organic Photovoltaic (OPV) devices. The goal was to use these conductance measurements to gain an understanding of the structural and electronic properties of these compounds in order to further understand why the central units lead to high/low  efficiency when used in OPVs. The presentation will be a summary of the measurements done on one particular compound and how the results can be interpreted.


      Electron spin resonance on-a-chip
      National High Magnetic Field Laboratory
      By: Henry Clark Travaligni

      We discuss Electron Spin Resonance Spectroscopy (ESR), and develop a room temperature measurement set up for ESR measurements performed on a high dielectric substrate.




      Pre-health Professions 101: How to Prepare

      August 25
      RKC 101

      Professor Frank Scalzo
      Health Professions Adviser, Bard CollegeProfessor Scalzo will introduce the pathways leading to post-baccalaureate degrees in the health professions, including allopathic medicine, osteopathic medicine, veterinary medicine, dentistry, optometry, etc. etc. The discussion will be tailored to the interests of the audience.  If you are interested in a health profession, but have not attended a similar previous discussion, you should attend this one.


      Senior Project Poster Session

      May 15
      Reem-Kayden Center

      Exploring Nanoscale Material Properties through Quantum Mechanics and High-Performance Computing

      April 22
      RKC 115

      Density functional theory (DFT) is a powerful method used to obtain solutions to the many-electron Schrӧdinger equation in condensed matter systems, and calculations using DFT are particularly well-suited for parallelization over as many as several thousand computer cores. DFT can be used to study the structural, electronic and vibrational properties of nano-structured materials from a first-principles perspective without the need for experimental parameterization. In this talk, I will discuss various DFT calculations and their applications to nano-materials of technological relevance, in particular materials for future device technology. Specific applications include mapping the free energy landscape for impurity diffusion across semiconductor interfaces, understanding the enhanced electrical conductance of ultra-small metallic  nanowires, and tuning the electronic properties of carbon nanotubes through the dielectric environment. These studies suggest new ways of manipulating quantum transport in atomic scale materials.


      Inelastic Collisions of NaK and NaCs Molecules with Atomic Perturbers

      April 17
      Hegeman 107

      I will discuss our studies of inelastic collisions of gas phase NaK and NaCs molecules with various atomic perturbers (Ar, He, K, Cs) using the spectroscopic technique optical-optical double resonance. The experiment is conducted by means of laser induced fluorescence (LIF) and polarization labeling (PL) spectroscopy. From the combination of LIF and PL spectra, we can determine certain properties of the inelastic collision. Such properties include perturber dependent collision rate coefficients, observations of strong propensities for ΔJ=even transitions in some cases, fraction of orientation lost in rotationally inelastic collisions, rate coefficients for vibration changing collisions, and collision line-broadening rates.