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Click here for:Date: | Thursday |
Time: | 1:30-3:00 PM |
Place: | 106A Studio Room, Classroom Building, OSU |
& Nielsen Hall, Room 365, OU | |
& Online Access | |
Inquiries: | joseph.haley@okstate.edu or kao@nhn.ou.edu |
Date: | Thursday |
Time: | 3:30-4:30 PM |
Place: | PS 110 |
Inquiries: | joseph.haley@okstate.edu or mario.borunda@okstate.edu |
Date: | Friday (bi)weekly |
Time: | 2:30 PM |
Place: | PS 147 |
Inquiries: | perk@okstate.edu or mario.borunda@okstate.edu |
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First Week of Classes
No talks scheduled
Second Week of Classes
Rescheduled to September 14 to avoid parking problems caused by football.
Speaker: | Mr. Shuo Dai |
Department of Physics | |
Oklahoma State University | |
Date: | Friday, September 1, 2017 |
Time: | 1:30 PM |
Place: | PS 147 |
Title: | Benchmarking DFT/TD-DFT Functionals for Frontier Orbital Energies Predictions on Organic Photovoltaic Molecules |
Speaker: | Dr. Bhupal Dev |
Department of Physics | |
Washington University, St. Louis, MO | |
Date: | Thursday, September 7, 2017 |
Time: | 1:30 PM |
Place: | 106A Studio Room, Classroom Building, OSU |
& Nielsen Hall, Room 365, OU | |
& Online Access | |
Title: | Flavorful Leptogenesis and Collider Signals |
Low-scale leptogenesis provides a unique opportunity to test the connection between two beyond the Standard Model phenomena, namely, neutrino mass and baryon asymmetry of the universe. We will elucidate this connection in the context of TeV-scale seesaw models with discrete flavor symmetries, in which case, the Dirac Yukawa couplings are completely dictated by the low-energy neutrino mixing parameters and the heavy neutrino masses. This scenario predicts distinctive correlated features in CP and lepton number/flavor violating observables, which could be used to probe this scenario at the high-energy frontier.
Speaker: | Dr. Bhupal Dev |
Department of Physics | |
Washington University, St. Louis, MO | |
Date: | Thursday, September 7, 2017 |
Time: | 3:30 PM |
Place: | PS 110 |
Title: | Neutrino as a Gateway to New Physics |
Neutrinos have played a crucial role in our understanding of the Universe. In particular, the discovery of neutrino oscillations has provided a concrete evidence for the existence of some new physics beyond the Standard Model. However, given the lack of information on the exact nature of the underlying new physics, it is crucial to take a broader, coherent approach by exploring possible connections with other empirically-supported clues. To this end, we will discuss a synergistic study using the neutrino portal at three interrelated frontiers of fundamental physics. The complementarity between various high and low-energy observables makes this study extremely useful, irrespective of the final outcome of the ongoing direct searches for new physics at the Large Hadron Collider.
Note: The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:00 PM. All students are welcome! Refreshments will be served.
Speaker: | Mr. Prashanth Chandran |
School of Chemical Engineering | |
Date: | Friday, September 8, 2017 |
Time: | 4:00 PM |
Place: | Engineering South 412 |
Title: | Computation of Liquid-Liquid Equilibrium from Molecular Simulations: |
Application to the Discovery of Desalination Solvents |
Speaker: | Mr. Kyle Stoltz |
Department of Physics | |
Date: | Friday, September 8, 2017 |
Time: | 4:30 PM |
Place: | Engineering South 412 |
Title: | Band Structures of Organic Polymers |
Speaker: | Dr. Kenneth D. Clinkenbeard |
Graduate College & | |
Department of Veterinary Pathobiology | |
Oklahoma State University | |
Date: | Thursday, September 14, 2017 |
Time: | 3:30 PM |
Place: | PS 110 |
Title: | Three Minute Thesis and Three Minute Presentations Competitions |
The three minute competitions help non-thesis masters and graduate certificate students (3MP) and thesis master’s and doctoral students (3MT) learn to present what they do as graduate students and how this is relevant to meeting societal needs in a concise, understandable and engaging manner. For the first time, both the 3MP and 3MT competitions will be offered in the fall semester. Cash prizes can be won by your students at the preliminary or college level ($100–$300) and for the OSU Finals ($500–$1,000).
Note: The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:00 PM. All students are welcome! Refreshments will be served.
Speaker: | Dr. Bhaskar Dutta | |
Interim Director and Professor | ||
George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy | ||
& 2017 OSU Physics Distinguished Alumnus | ||
Department of Physics and Astronomy | ||
Texas A&M University, College Station, TX | ||
Date: | Friday, September 22, 2017 | |
Time: | 1:30 PM | |
Place: | Chemistry Conference room, PS 116, OSU | |
& Nielsen Hall, Room 365, OU | ||
& Online Access | ||
Title: | Z' Models for B-Anomalies at the LHC |
Speaker: | Dr. Bhaskar Dutta | |
Interim Director and Professor | ||
George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy | ||
Department of Physics and Astronomy | ||
Texas A&M University, College Station, TX | ||
Date: | Friday, September 22, 2017 | |
Time: | 3:30 PM | |
Place: | PS 110 | |
Title: | Particle Theory Models and Dark Matter: A Status Update |
The recent results from the ongoing Large Hadron Collider, various direct and indirect dark matter detection experiments and data from PLANCK satellite observations have introduced considerable constraints on the particle physics model ideas related to dark matter. This talk will address the current status of particle physics models and their predictions for the upcoming experiments.
Note: Dr. Dutta is also honored as Distinguished Alumnus by the College of Arts and Sciences.
Note: The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:00 PM. All students are welcome! Refreshments will be served.
Speaker: | Mr. Shuo Dai |
Department of Physics | |
Oklahoma State University | |
Date: | Monday, September 25, 2017 |
Time: | 9:00 AM |
Place: | PS 147 |
Title: | Density Functional Theory and Time-Dependent-DFT Modeling of Organic Photovoltaic Materials |
Speaker: | Dr. Raman P. Singh |
Associate Dean for Engineering at OSU-Tulsa | |
Helmerich Family Endowed Chair Professor of Engineering | |
Professor & Head, School of Material Science and Engineering | |
Professor, School of Mechanical & Aerospace Engineering | |
Director, Helmerich Research Center, Tulsa | |
Date: | Thursday, September 28, 2017 |
Time: | 3:30 PM |
Place: | PS 110 |
Title: | Quantifying UV Degradation at the Carbon Fiber-Matrix Interphase using AFM Indentation |
This talk presents recent results on studies conducted to investigate the effects of ultraviolet (UV) exposure of composite materials. Ultraviolet radiation causes photocatalytic degradation in polymers leading to material degradation. While numerous studies have been done to characterize the effects of UV exposure on the macro-scale properties of bulk polymers and composite materials, the effects of UV degradation on the interphase and in near-fiber regions are not clearly understood.
In this work we implement AFM indentation based force-mapping to investigate the effect of UV exposure on the interphase region of carbon fiber composites. Samples exposed to ultraviolet (UV) chamber for 24 hours at 0.68 W/m2/nm irradiance at 340 nm and 60oC. Force mapping was used to generate “full-field” load-displacement indentation curves, which were then analyzed using the Oliver–Pharr model to determine elastic modulus. In this manner it was possible to create 32×32 and 64×64 arrays of elastic modulus values in the interphase region and the near-fiber region. For neat CFRP sample and interphase region of thickness 100–200 μm was observed. While for UV exposed samples a distinct interphase region was not observed. This is attributed to the increase in chemical cross-linking of the epoxy resin due to UV exposure around the carbon fiber. The presentation concludes with an overview of research activities and capabilities at the Helmerich Research Center and discusses areas of possible collaboration.
Note: The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:00 PM. All students are welcome! Refreshments will be served.
Speaker: | Dr. Cassie S. Mitchell | |
Assistant Professor, Biomedical Engineering | ||
Principal Investigator, Laboratory for Pathology Dynamics | ||
Georgia Institute of Technology & Emory University School of Medicine | ||
Date: | Friday, September 29, 2017 | |
Time: | 4:00 PM | |
Place: | Engineering South 412 | |
Title: | After the Ice Bucket: Thawing Amyotrophic Lateral Sclerosis with Predictive Medicine |
Speaker: | Dr. Salahuddin Ahmad |
Department of Radiation Oncology and | |
Department of Radiological Sciences | |
University of Oklahoma Health Sciences Center (OUHSC) | |
Date: | Thursday, October 5, 2017 |
Time: | 3:30 PM |
Place: | PS 110 |
Title: | PS 110 |
Title: | Clinical and Research Profile of the Department of Radiation Oncology |
At the outset, the clinical, educational and research programs of the Department of Radiation Oncology at the University of Oklahoma HSC will be discussed. Two topics one on “Treatment Plan Evaluation and Optimization Based on Radiobiologic Parameters” and the other on “Advances in Proton and Heavy Ion Treatment” will then be presented.
Note: The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:00 PM. All students are welcome! Refreshments will be served.
Speaker: | Dr. Jacques H.H. Perk |
Department of Physics | |
Oklahoma State University | |
Date: | Friday, October 6, 2017 |
Time: | 1:30 PM |
Place: | PS 147 |
Title: | Clifford Algebra (Majorana Fermion) Approach to Quantum Spin Chains and 2-Dimensional Ising Models |
Speaker: | Dr. Vibhudutta Awasthi |
Sandra K and David L Gilliland Chair in Nuclear Pharmacy | |
Department of Pharmaceutical Sciences, College of Pharmacy | |
University of Oklahoma Health Sciences Center (OUHSC) | |
Date: | Thursday, October 12, 2017 |
Time: | 3:30 PM |
Place: | PS 110 |
Title: | Research Imaging Facility in OUHSC for Drug and Formulation Development |
According to the Critical Path Initiative of FDA and NCI, development of imaging biomarkers is vital in addressing the expedited and cost-effective development of new drugs. The Research Imaging Facility (RIF) is the first public facility in Oklahoma to provide molecular imaging capability for research. At present, the RIF provides positron emission tomography (PET), single photon emission tomography (SPECT), and X-ray computed tomography (CT) imaging services. In addition, a dedicated low energy cyclotron is available to produce positron-emitting radionuclides for synthesis of radiopharmaceuticals. These equipment are leveraged by biomedical researchers in OUHSC as well as investigators in Oklahoma to hasten pre-clinical phase in the development of therapeutic or diagnostic agents.
With an overall objective of engendering cross-institution collaboration, the presenter(s) of this seminar will introduce the audience to nuclear imaging in general and our service capabilities in particular. In one instance, we have applied molecular imaging to answer critical developmental questions about artificial oxygen carriers. We use PET and SPECT to demonstrate that nano-particulate liposome-encapsulated hemoglobin (LEH) circulates in the body for a prolonged duration, carries oxygen in blood, and delivers oxygen to the brain for improved cerebral metabolism. Further applications of nuclear imaging and radiochemistry in drug development will be shared.
Note: The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:00 PM. All students are welcome! Refreshments will be served.
Speaker: | Dr. Kyle A. Copeland | |
Federal Aviation Administration, Civil Aerospace Medical Institute | ||
Oklahoma City | ||
Date: | Thursday, October 19, 2017 | |
Time: | 3:30 PM | |
Place: | PS 110 | |
Title: | Health Physics in Aerospace Environments |
Ionizing radiation exposure is a known source of health risks. Besides the shipment of radioactive materials, there are other natural sources of ionizing radiation that must be considered such as solar and galactic cosmic radiation. Measurements of doses from these radiations are insufficient to build empirical models that meet current operational needs, and massive deployment of good quality instruments on aircraft is considered impractical. In addition to dosimetry issues, modeling the cosmic radiation environment in the atmosphere is a complex problem. While predominantly protons, cosmic ray primaries of other elements occur at fluences that cannot be neglected if calculations are to be reasonably accurate. Over the past three decades the FAA’s Radiobiology Research Team has used the deterministic radiation transport software LUIN and more recently the Monte Carlo radiation transport software MCNPX to build software (called CARI) to calculate flight doses and evaluate solar proton events. The two approaches are compared in terms of limitations and advantages.
Note: The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:00 PM. All students are welcome! Refreshments will be served.
Students’ Fall Break: Friday, October 20
Speaker: | Dr. Elisabetta A. Matsumoto |
School of Physics | |
Georgia Institute of Technology | |
Date: | Friday, October 27, 2017 |
Time: | 3:30 – 4:30 PM |
Place: | Student Union, Rm. 416 |
Title: | Non-Euclidean Virtual Reality |
The properties of euclidean space seem natural and obvious to us, to the point that it took mathematicians over two thousand years to see an alternative to Euclid’s parallel postulate. The eventual discovery of hyperbolic geometry in the 19th century shook our assumptions, revealing just how strongly our native experience of the world blinded us from consistent alternatives, even in a field that many see as purely theoretical. Non-euclidean spaces are still seen as unintuitive and exotic, but with direct immersive experiences we can get a better Intuitive feel for them. The latest wave of virtual reality hardware, in particular the HTC Vive, tracks both the orientation and the position of the headset within a room-sized volume, allowing for such an experience. We use this nascent technology to explore the three-dimensional geometries of the Thurston/Perelman geometrization theorem. This talk focuses on our simulations of H3 and H2×E.
Speaker: | Mr. Utkarsh Kapoor |
School of Chemical Engineering | |
Date: | Friday, October 27, 2017 |
Time: | 4:00 PM |
Place: | Engineering South 412 |
Title: | TBA |
Speaker: | Mr. Atiya Banerjee |
School of Chemical Engineering | |
Date: | Friday, October 27, 2017 |
Time: | 4:30 PM |
Place: | Engineering South 412 |
Title: | TBA |
Speaker: | Dr. Alexander Khanov |
Department of Physics | |
Oklahoma State University | |
Date: | Thursday, November 2, 2017 |
Time: | 1:30 PM |
Place: | 106A Studio Room, Classroom Building, OSU |
& Nielsen Hall, Room 365, OU | |
& Online Access | |
Title: | Physics with the ATLAS Detector at the HL-LHC |
The High luminosity Large Hadron Collider (HL-LHC) project is a proposed upgrade to the LHC by year 2025. I will present and discuss the prospects for physics studies at the HL-LHC with a data set equivalent to 3000 fb-1, simulated in the upgrade ATLAS detector.
Speaker: | Ms. Minu Pilvankar |
School of Chemical Engineering | |
Date: | Friday, November 3, 2017 |
Time: | 4:00 PM |
Place: | Engineering South 412 |
Title: | A PK/PD Model of ACE Inhibition of Glucose-Stimulated Renin-Angiotensin System in Kidney Cells for Normal and Diabetic Cases |
Speaker: | Mr. Gentry Smith |
Department of Chemistry | |
Date: | Friday, November 3, 2017 |
Time: | 4:30 PM |
Place: | Engineering South 412 |
Title: | Small-Scale Folding |
Speaker: | Dr. William J. Gannon | |
Department of Physics and Astronomy | ||
Texas A&M University, College Station, TX | ||
Date: | Monday, November 6, 2017 | |
Time: | 4:00 PM | |
Place: | PS 110 | |
Title: | Exploring Quantum Magnetic Fluctuations in Low Dimensional Correlated Electron Systems |
Quantum magnetic fluctuations are one of the key concepts in modern condensed matter physics, and is a thread that ties together a vast array of topics, from the coherence of unconventional superconductivity to the entangled disorder of quantum spin liquids to name just two examples. In this talk, I will discuss why it is essential to understand quantum magnetic fluctuations in materials that host them and how we can use inelastic neutron scattering to probe these important phenomena. As a specific example, I will discuss how quantum magnetism is manifest in the correlated electron metal Yb2Pt2Pb and the observation of fractionalized one dimensional spin excitations, quasiparticle confinement, and longitudinally polarized quantum modes. Finally, I will discuss how these measurements can point to new and interesting research directions.
Note: The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:30 PM. All students are welcome! Refreshments will be served.
Speaker: | Dr. Chunhui Du |
Department of Physics | |
Harvard University | |
Date: | Thursday, November 9, 2017 |
Time: | 4:00 PM |
Place: | PS 110 |
Title: | Control and Local Measurement of the Spin Chemical Potential in a Magnetic Insulator |
In recent decades, a large scientific effort has focused on harnessing spin transport for providing insights into novel materials and low-dissipation information processing. We introduce single spin magnetometry based on nitrogen-vacancy (NV) centers in diamond as a new and generic platform to locally probe spin chemical potentials which essentially determine the flow of spin currents. We use this platform to investigate magnons in a magnetic insulator yttrium iron garnet (YIG) on a 100 nanometer length scale. We demonstrate that the local magnon chemical potential can be systematically controlled through both ferromagnetic resonance and electrical spin excitation, which agrees well with the theoretical analysis of the underlying multi-magnon processes. Our results open up new possibilities for nanoscale imaging and manipulation of spin-related phenomena in condensed-matter systems.
Note: The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:30 PM. All students are welcome! Refreshments will be served.
Speaker: | Mr. Digesh Raut |
Department of Physics and Astronomy | |
University of Alabama | |
Date: | Monday, November 13, 2017 |
Time: | 1:00 PM |
Place: | PS 116/117, OSU |
& Nielsen Hall, Room 365, OU | |
& Online Access | |
Title: | Inflation, Dark Matter, and LHC Phenomenology in Minimal Gauged U(1)X Extension of SM |
In the context of gauged U(1) extension of SM, we discuss the cosmological inflation scenarios, dark matter physics, and LHC phenomenology. We consider minimal U(1)X extended SM, a generalization of the minimal U(1)B−L model which is realized as a linear combination of the SM U(1)Y and the U(1)B−L gauge symmetries. In addition to a B−L scalar and a new Z′ gauge boson, the model also includes three generations of right handed neutrinos (RHNs) for the anomaly cancellation. With an identification of the B−L scalar to be the inflaton field, we investigate inflection-point inflation which naturally accommodates inflation scenario with initial inflation scale below the Planck mass (φI ≲ MPl). For a renormalization group improved effective λφ4 potential to develop an inflection-point with inflationary predictions consistent with the current cosmological observations, the mass ratios among the Z′ gauge boson, the RHNs, and the inflaton are fixed. In the B−L limit with the gauge boson mass less than 1 TeV we find that the scenario can be tested in the future collider experiments such as the High-Luminosity LHC and the SHiP experiments. On the other extreme, we consider the scenario such that the U(1)X gauge symmetry is mostly oriented towards the SM U(1)Y direction and investigate a consistency between the inflationary predictions and the latest LHC Run-2 results on narrow resonance Z′ search with a di-lepton final state. Dark matter (DM) physics is another interesting possibility that we consider. Implementing Z2 parity to one of the RHNs, we investigate the possibility of “Z′-portal” DM scenario to explore the viable parameter region consistent with the relic abundance and state. Finally, we consider the prospect of RHN discovery at the LHC via Z′ boson decay. U(1)X model provides significant enhancement of the production cross section of the RHNs from Z′ decay in the future LHC experiments, which is crucial for the discovery of RHNs given that the production cross-section of Z′ boson via di-lepton resonance is severely constrained. Taking this into account, we conclude that the possibility of discovering the RHNs in the future implies that the Z′ boson will soon be discovered at the LHC.
Speaker: | Dr. Brian B. Zhou |
Institute for Molecular Engineering | |
University of Chicago | |
Date: | Monday, November 13, 2017 |
Time: | 4:00 PM |
Place: | PS 110 |
Title: | Shaping the Quantum Dynamics of Single Spins in Diamond |
Remarkable progress in the control of atomic-scale systems have confirmed the quantum foundation of our world, as well as inspired new paradigms for technological innovation. For its long spin coherence and optical interface, the nitrogen-vacancy (NV) center—an atomic defect in diamond—presents a premier platform for secure quantum communication and high-precision sensing. The common enabler of these applications is the ability to coherently manipulate quantum states with high speed and high fidelity. We demonstrate novel dynamical methods using resonant and near-resonant optical fields to control single NV spins with high spatial resolution and low power. To hybridize robustness with speed by overcoming conventional adiabatic speed limits, we engineer ‘superadiabatic’ dynamics to create and transfer arbitrary coherent states [1]. We then extend geometric quantum control to high-speed quantum gates by using non-adiabatic matrix holonomies [2]. These techniques are widely translatable and simplify the implementation of all-optical quantum networks.
Note: The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:30 PM. All students are welcome! Refreshments will be served.
Speaker: | Dr. Benjamin Kreis |
LHC Physics Center (LPC) | |
Fermilab | |
Date: | Thursday, November 16, 2017 |
Time: | 1:30 PM |
Place: | 106A Studio Room, Classroom Building, OSU |
& Nielsen Hall, Room 365, OU | |
& Online Access | |
Title: | Migrating Advanced Analysis Techniques to Fast Hardware for the CMS Phase 2 Trigger |
Speaker: | Dr. Peter. A. Dowben |
Department of Physics and Astronomy | |
University of Nebraska–Lincoln | |
Date: | Thursday, November 16, 2017 |
Time: | 3:30 PM |
Place: | PS 110 |
Title: | Electrically Controlled Surface Magnetism and Energy Savings in Solid State Electronics |
The problems faced by the increasing power density and decreasing device size in semiconductor technologies will be reviewed and an effort is made to motivate why spintronics may lead to energy savings in solid state electronics. The inherent non-volatility of long-range ordered magnetism adds functionality over today’s random access memory (RAM) elements. The latter require refresh power during operation and the information is lost when power is lost, not true of the nonvolatile magneto-electric device. Manipulation of magnetically ordered states by electrical means (the magneto-electric effect) is among the most promising approaches towards novel spintronic devices [1–4]. Indeed, voltage control of magnetism is a grand challenge of spintronics. The reasons that magnetoelectric devices lead to energy savings are simple enough: voltage control of a nonvolatile magnetic state virtually eliminates the need for large current densities, the accompanying power consumption, and detrimental Joule heating on writing and potentially also on reading. In this talk, the magneto-electron phenomena is reviewed. Exchange bias is reviewed. The interplay between band structure and boundary polarization has considerable significance in devices that rely on the magneto-electric phenomena and this too is reviewed. The context for this discussion is that one can then utilize the electrically switchable and nonvolatile boundary magnetization of magneto-electric antiferromagnets, such as chromia, to generate a voltage-controlled exchange field, which determines the carrier spin in the conducting channel or can be used to reverse magnetization or an adjacent ferromagnet. Such devices can actually “beat” silicon technologies in terms of energy cost.
Note: The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:00 PM. All students are welcome! Refreshments will be served.
Speaker: | Dr. Peter. A. Dowben |
Department of Physics and Astronomy | |
University of Nebraska–Lincoln | |
Date: | Friday, November 17, 2017 |
Time: | 9:30 AM |
Place: | PS 147 |
Title: | The History and Development of Boron Carbon Alloy Devices and Rare Earth Heterojunction Neutron Detectors |
Traditional neutron detectors have been large, delicate, cumbersome and expensive, with high power requirements. A SOLID STATE neutron detector would overcome many of these problems. We believe that there are neutron detector technologies, developed at the University of Nebraska and elsewhere, that can be substantially improved, possibly outclassing all other competing technologies for the monitoring and detecting of fissile and other neutron emitting radioactive materials in terms of expense of manufacture, device lifetime and power consumption. These technologies are based on the development of novel semiconductor materials, based on boron. These boron based materials have been used to measure the energy and flux of the steady state solar neutron flux from the sun. Note: solid state physicists can become astronomers.
Speaker: | Mr. Sherin Shanaka Paranahewage |
Department of Chemistry | |
Date: | Friday, November 17, 2017 |
Time: | 4:00 PM |
Place: | Engineering South 412 |
Title: | Dielectric Balancing of Molecules Improves Liquid-State and Molecular Transfer Properties |
Speaker: | Mr. Casey Williamson |
Department of Chemistry | |
Date: | Friday, November 17, 2017 |
Time: | 4:30 PM |
Place: | Engineering South 412 |
Title: | Molecular Simulations: What is it? Why do we care? |
Thanksgiving
Speaker: | Dr. Su, Dong |
SLAC National Accelerator Laboratory | |
Stanford University | |
Date: | Thursday, November 30, 2017 |
Time: | 1:30 PM |
Place: | 106A Studio Room, Classroom Building, OSU |
& Nielsen Hall, Room 365, OU | |
& Online Access | |
Title: | ATLAS Tracking Upgrade for High Luminosity LHC |
The upgrade of the LHC accelerator with factor of ∼5 increase in instantaneous luminosity is expected to usher the new era of High Luminosity LHC (HL-LHC) by 2025. This exciting physics prospect comes at the expense of a more challenging experimental environment with high radiation dose, high rate of concurrent pile up interactions and associated high data volume and high trigger rate. ATLAS is planning to replace the complete Inner Tracking system with an all silicon Inner Tracker (ITk). Selected topics related to the ITk upgrade will be discussed: high granularity radiation hard sensors, monolithic CMOS development and challenge of data transmission and powering. The related issues associated with the trigger and DAQ architecture will also be briefly discussed.
Speaker: | Dr. Su, Dong |
SLAC National Accelerator Laboratory | |
Stanford University | |
Date: | Thursday, November 30, 2017 |
Time: | 3:30 PM |
Place: | PS 110 |
Title: | Higgs as a Tool for New Physics |
Since the discovery of the Standard Model like Higgs particle at 125 GeV at LHC in 2012, this last piece of corner stone of the Standard Model has also become of the launch pad for searches of physics beyond the Standard Model. The rich coupling network of the Higgs within the Standard Model has natural extensions toward possible portal to new physics scenarios such as the Dark Matter sector. We will discuss several selected topical areas ranging from exotic Higgs decays, Higgs as a decay signature of heavy new particles, and searches for additional Higgs bosons forming a broad new frontier in connection with the Higgs. This new adventure is also coupled to novel new experimental techniques to confront the challenge of high luminosity at LHC and take advantage of the new opportunities at the high energy. The development of physics signatures from objects, including Higgs, in the high Lorentz boost regime, and advanced heavy quark tag techniques will also be discussed.
Note: The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:00 PM. All students are welcome! Refreshments will be served.
Prefinals Week
Speaker: | Dr. Emrah Turgut |
School of Applied and Engineering Physics | |
Cornell University | |
Date: | Monday, December 4, 2017 |
Time: | 4:00 PM |
Place: | PS 110 |
Title: | Spin Dynamics of Topological Spin Textures in Chiral Magnets |
The chiral spin textures are a consequence of the anti-symmetric exchange interaction, which presents in the material systems with broken inversion symmetry, such as B20 FeGe. This interaction enables chiral magnetic order, including topologically non-trivial magnetic skyrmions, which display rich new magnetic phenomena and require low critical current densities to manipulate. This makes magnetic skyrmions a promising platform for power-efficient spintronics applications. Therefore, a deeper understanding of the static and dynamic magnetic properties of these materials will be a key step toward their application in spintronic devices. In this talk, I will present our study of both sputtered, epitaxial B20 FeGe and B20 FeGe grown using vapor transport. In particular, I will discuss microwave absorption spectroscopy (MAS) of bulk, single crystal FeGe with which we identify the spin dynamics of all magnetic phases. These results reveal the critical role of substrate-induced strain on the magnetic phases of B20 FeGe. To gain better control over strain and to tune the strength of anti-symmetric exchange, I grew B20 FeGe and MnxFe1−xGe on Si with MBE. After characterization using electron and X-ray diffraction, magnetometry, and cryo-Lorentz-STEM imaging, we study MAS of these films. We identify a new spin wave mode along the film thickness, with a wavelength that matches its helical period, enabling a new, simple method of quantitatively characterizing the anti-symmetric exchange.
Note: The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:30 PM. All students are welcome! Refreshments will be served.
Speaker: | Dr. Joseph Haley |
Department of Physics | |
Oklahoma State University | |
Date: | Thursday, December 7, 2017 |
Time: | 3:30 PM |
Place: | PS 110 |
Title: | Vector-like Quarks or: How I Learned to Stop Worrying and Love the Standard Model |
Despite its remarkable success in describing the subatomic world, the Standard Model leaves many unanswered questions (dark matter, matter-antimatter asymmetry, quantum gravity, …). One of the most pressing issues facing particle physics today is the so-called “hierarchy problem.”  According to the Standard Model, quantum mechanical corrections (from virtual top quarks) should cause the Higgs boson mass to blow up to a value near the Planck-scale, some 16 orders of magnitude larger than the observed value of 125 GeV. So there is either an extremely lucky cancellation that happens by chance or there is some new physics mechanism that naturally keeps the Higgs boson mass from blowing up to the Planck-scale. A wide range of beyond-the-SM theories have been proposed to solve the hierarchy problem and a common feature in many is the prediction of new particles called vector-like quarks. This colloquium will attempt to explain what they are, why they are interesting, and how we search for them using the ATLAS experiment at CERN.
Note: The traditional student-speaker chat will begin in Physical Sciences Room 147 at 3:00 PM. All students are welcome! Refreshments will be served.
Finals Week
No talks scheduled
No talks scheduled
No talks scheduled.
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This page was prepared by Helen Au-Yang and Jacques H.H. Perk.
jhhp@jperk.phy.okstate.edu