Spring 2015

Colloquia - Spring 2015

January 13 -

"Title: TBA"

Abstract:

January 20 -

"Title: TBA"

Abstract:

January 27 -

"Title: TBA"

Abstract:

February 3 -

"Title: TBA"

Abstract:

February 10 -

"Title: TBA"

Abstract:

February 17 - Sam Zeller, Fermi National Accelerator Laboratory (POSTPONED)

"Title: Opening a New Chapter in Neutrino Physics"

Abstract: Neutrinos are among the most abundant particles in the universe and they influence an enormous range of physics. Neutrinos allow us to search for new forces of nature, they measure the composition of the earth's crust, they tell us how the sun works, and they allow us to peer into the inner workings of a supernova explosion. Despite all that we have learned from these special particles, there remains a surprising amount of information we still do not know about neutrinos themselves. The discovery of neutrino masses and mixing over a decade ago has raised a large number of challenging questions about neutrinos. After briefly reviewing what we have learned about neutrinos so far, we will examine the open questions, explain why these questions are interesting, and discuss plans for answering them in future experiments. The coming years promise to be very exciting as we move in new directions to better understand these unique subatomic particles and their connections to the world we live in.

February 24 - TBA

"Title: TBA"

Abstract:

March 3 - Sam Zeller, Fermi National Accelerator Laboratory

"Title: Opening a New Chapter in Neutrino Physics"

Abstract: Neutrinos are among the most abundant particles in the universe and they influence an enormous range of physics. Neutrinos allow us to search for new forces of nature, they measure the composition of the earth's crust, they tell us how the sun works, and they allow us to peer into the inner workings of a supernova explosion. Despite all that we have learned from these special particles, there remains a surprising amount of information we still do not know about neutrinos themselves. The discovery of neutrino masses and mixing over a decade ago has raised a large number of challenging questions about neutrinos. After briefly reviewing what we have learned about neutrinos so far, we will examine the open questions, explain why these questions are interesting, and discuss plans for answering them in future experiments. The coming years promise to be very exciting as we move in new directions to better understand these unique subatomic particles and their connections to the world we live in.

March 10 - Spring Break

"Title: TBA"

Abstract:

March 17 -

"Title: TBA"

Abstract:

March 24 - Chang-Beom Eom, University of Wisconsin (Cancelled)

"Title: TBA"

Abstract:

March 31 -

"Title: TBA"

Abstract:

April 7 -

"Title: TBA"

Abstract:

April 14 - Dr. Greg Kalicy, The Annual Sigma Pi Sigma Induction Ceremony

"Title: Developing DIRC Technology, a Personal Journey Around the World "

Abstract:

April 21 - Andrei Derevianko, University of Nevada-Reno

"Title: Hunting for dark matter with GPS and atomic clocks"

Abstract: Atomic clocks are arguably the most accurate scientific instruments ever build. Modern clocks are astonishing timepieces guaranteed to keep time within a second over the age of the Universe. Attaining this accuracy requires that the quantum oscillator be well protected from environmental noise and perturbations well controlled and characterized. This opens intriguing prospects of using clocks to study subtle effects, and it is natural to ask if such accuracy can be harnessed for dark matter searches.

The cosmological applications of atomic clocks so far have been limited to searches of the uniform-in-time drift of fundamental constants. We point out that a transient in time change of fundamental constants (translating into clocks being sped up or slowed down) can be induced by dark matter objects that have large spatial extent, and are built from light non-Standard Model fields. The stability of this type of dark matter can be dictated by the topological reasons. We argue that correlated networks of atomic clocks, such as atomic clocks onboard satellites of the GPS
constellation, can be used as a powerful tool to search for the topological defect dark matter. In other words, one could envision using GPS as a 50,000 km-aperture dark-matter detector.

Details: A. Derevianko and M. Pospelov, Nature Phys. 10, 933 (2014)

April 28 - Senior Thesis Presentations

Old Dominion University
Department of Physics

Physics Undergraduate Seniors' Day

Tuesday April 28, 2015

Senior Thesis Presentations
2:15 - 2:45 pm.
Refreshments in OCNPS First floor Atrium


2:45 - 2:55 pm.
Welcome and Introduction in Scale-Up (OCNPS 142 - 144)


3:00 - 5:00 pm.
Senior Thesis Presentations
Scale-Up Room OCNPS 142-144 and ECSB 1202 Auditorium (CAVE)

Senior Thesis Presenters
(Two Parallel Sessions)

Presenter CAVE Time SCALE-UP Presenter
Katheryne McMahan
Scintillator Testing and Repair for the Large Acceptance Detector at Jefferson Lab.
C1 3:00 - 3:15 pm. S1 Mathieu Ehrhart
Beamline Magnet Studies for the Heavy Photon Search Experiment at Jefferson Lab.
Cameron Nunez
Comparing Phase Shifts of the Finite Potential Well to that of the Periodically Bound Case.
C2 3:15 - 3:30 pm. S2 Matthew Vogel
Neutrino Oscillations in Vacuum and Matter.
Nathaniel Schirle
Signal Propagation and Attenuation in Different Cable Types.
C3 3:30 - 3:45 pm. S3 Cory Gruber
Modeling Transverse Structure of the Pion Distribution Amplitude.
Sean Babcock
Investigation of the Effects of Recombination Processes on the Performance of Organic Bulk Heterojunction Photovoltaics.
C4 3:45 - 4:00 pm. S4 Victoria Lagerquist
Observation of Symbiotic Binary Systems in Cygnus.
Jon-Michael Glick
Mechanics of the Double Pendulum and An Analytic Study of the Logistic Function and Chaos.
C5 4:00 - 4:15 pm. S5 Christopher Cotnoir
A Hybrid Nature-Inspired Algorithm for a Multidimensional Nonlinear Optimization with Applications to Biology.
Mark Stefani
Wavelet-Based Noise-Reduction Techniques in Tomography With Application to Plasma and Accelerator Physics.
C6 4:15 - 4:30 pm. S6 Frank Berardi
NMR for Polarized Nuclei in an Inhomogeneous Magnetic RF Field.
David Gary
Elastic Scattering as a measure of Luminosity in an Electron-Ion Collider.
C7 4:30 - 4:45.pm. S7 Anthony Sciola
Charge Exchange Process for Impact Between Low-Z Ions and Atomic Hydrogen.
Josh Frechem
Photometric Survey of Symbiotic Binary Systems in the Northern Hemisphere Using the Goddard Robotic Telescope.
C8 4:45 - 5:00 pm. S8 Sonja Schimmers-Wood
The Testing of Scintillation Detectors for the CLAS TOF system.

January 13 -

"Title: TBA"

Abstract:

January 20 -

"Title: TBA"

Abstract:

January 27 -

"Title: TBA"

Abstract:

February 3 -

"Title: TBA"

Abstract:

February 10 -

"Title: TBA"

Abstract:

February 17 - Sam Zeller, Fermi National Accelerator Laboratory (POSTPONED)

"Title: Opening a New Chapter in Neutrino Physics"

Abstract: Neutrinos are among the most abundant particles in the universe and they influence an enormous range of physics. Neutrinos allow us to search for new forces of nature, they measure the composition of the earth's crust, they tell us how the sun works, and they allow us to peer into the inner workings of a supernova explosion. Despite all that we have learned from these special particles, there remains a surprising amount of information we still do not know about neutrinos themselves. The discovery of neutrino masses and mixing over a decade ago has raised a large number of challenging questions about neutrinos. After briefly reviewing what we have learned about neutrinos so far, we will examine the open questions, explain why these questions are interesting, and discuss plans for answering them in future experiments. The coming years promise to be very exciting as we move in new directions to better understand these unique subatomic particles and their connections to the world we live in.

February 24 - TBA

"Title: TBA"

Abstract:

March 3 - Sam Zeller, Fermi National Accelerator Laboratory

"Title: Opening a New Chapter in Neutrino Physics"

Abstract: Neutrinos are among the most abundant particles in the universe and they influence an enormous range of physics. Neutrinos allow us to search for new forces of nature, they measure the composition of the earth's crust, they tell us how the sun works, and they allow us to peer into the inner workings of a supernova explosion. Despite all that we have learned from these special particles, there remains a surprising amount of information we still do not know about neutrinos themselves. The discovery of neutrino masses and mixing over a decade ago has raised a large number of challenging questions about neutrinos. After briefly reviewing what we have learned about neutrinos so far, we will examine the open questions, explain why these questions are interesting, and discuss plans for answering them in future experiments. The coming years promise to be very exciting as we move in new directions to better understand these unique subatomic particles and their connections to the world we live in.

March 10 - Spring Break

"Title: TBA"

Abstract:

March 17 -

"Title: TBA"

Abstract:

March 24 - Chang-Beom Eom, University of Wisconsin (Cancelled)

"Title: TBA"

Abstract:

March 31 -

"Title: TBA"

Abstract:

April 7 -

"Title: TBA"

Abstract:

April 14 - Dr. Greg Kalicy, The Annual Sigma Pi Sigma Induction Ceremony

"Title: Developing DIRC Technology, a Personal Journey Around the World "

Abstract:

April 21 - Andrei Derevianko, University of Nevada-Reno

"Title: Hunting for dark matter with GPS and atomic clocks"

Abstract: Atomic clocks are arguably the most accurate scientific instruments ever build. Modern clocks are astonishing timepieces guaranteed to keep time within a second over the age of the Universe. Attaining this accuracy requires that the quantum oscillator be well protected from environmental noise and perturbations well controlled and characterized. This opens intriguing prospects of using clocks to study subtle effects, and it is natural to ask if such accuracy can be harnessed for dark matter searches.

The cosmological applications of atomic clocks so far have been limited to searches of the uniform-in-time drift of fundamental constants. We point out that a transient in time change of fundamental constants (translating into clocks being sped up or slowed down) can be induced by dark matter objects that have large spatial extent, and are built from light non-Standard Model fields. The stability of this type of dark matter can be dictated by the topological reasons. We argue that correlated networks of atomic clocks, such as atomic clocks onboard satellites of the GPS
constellation, can be used as a powerful tool to search for the topological defect dark matter. In other words, one could envision using GPS as a 50,000 km-aperture dark-matter detector.

Details: A. Derevianko and M. Pospelov, Nature Phys. 10, 933 (2014)

April 28 - Senior Thesis Presentations

Old Dominion University
Department of Physics

Physics Undergraduate Seniors' Day

Tuesday April 28, 2015

Senior Thesis Presentations
2:15 - 2:45 pm.
Refreshments in OCNPS First floor Atrium


2:45 - 2:55 pm.
Welcome and Introduction in Scale-Up (OCNPS 142 - 144)


3:00 - 5:00 pm.
Senior Thesis Presentations
Scale-Up Room OCNPS 142-144 and ECSB 1202 Auditorium (CAVE)

Senior Thesis Presenters
(Two Parallel Sessions)

Presenter CAVE Time SCALE-UP Presenter
Katheryne McMahan
Scintillator Testing and Repair for the Large Acceptance Detector at Jefferson Lab.
C1 3:00 - 3:15 pm. S1 Mathieu Ehrhart
Beamline Magnet Studies for the Heavy Photon Search Experiment at Jefferson Lab.
Cameron Nunez
Comparing Phase Shifts of the Finite Potential Well to that of the Periodically Bound Case.
C2 3:15 - 3:30 pm. S2 Matthew Vogel
Neutrino Oscillations in Vacuum and Matter.
Nathaniel Schirle
Signal Propagation and Attenuation in Different Cable Types.
C3 3:30 - 3:45 pm. S3 Cory Gruber
Modeling Transverse Structure of the Pion Distribution Amplitude.
Sean Babcock
Investigation of the Effects of Recombination Processes on the Performance of Organic Bulk Heterojunction Photovoltaics.
C4 3:45 - 4:00 pm. S4 Victoria Lagerquist
Observation of Symbiotic Binary Systems in Cygnus.
Jon-Michael Glick
Mechanics of the Double Pendulum and An Analytic Study of the Logistic Function and Chaos.
C5 4:00 - 4:15 pm. S5 Christopher Cotnoir
A Hybrid Nature-Inspired Algorithm for a Multidimensional Nonlinear Optimization with Applications to Biology.
Mark Stefani
Wavelet-Based Noise-Reduction Techniques in Tomography With Application to Plasma and Accelerator Physics.
C6 4:15 - 4:30 pm. S6 Frank Berardi
NMR for Polarized Nuclei in an Inhomogeneous Magnetic RF Field.
David Gary
Elastic Scattering as a measure of Luminosity in an Electron-Ion Collider.
C7 4:30 - 4:45.pm. S7 Anthony Sciola
Charge Exchange Process for Impact Between Low-Z Ions and Atomic Hydrogen.
Josh Frechem
Photometric Survey of Symbiotic Binary Systems in the Northern Hemisphere Using the Goddard Robotic Telescope.
C8 4:45 - 5:00 pm. S8 Sonja Schimmers-Wood
The Testing of Scintillation Detectors for the CLAS TOF system.