UCR

Department of Physics & Astronomy



Previous Colloquium and Videos


Previous Colloquium and Videos

DateSpeakerTitleAbstractVideo Link
March 16, 2017 Leslie Rosenberg - University of Washington Searching for Dark-Matter Axions The axion is a hypothetical elementary particle whose existence would explain the baffling absence of CP violation in the strong interactions. Axions also happen to be a compelling dark-matter candidate. Axions could comprise the overwhelming majority of mass in the universe, yet they would be extraordinarily difficult to detect. However, several experiments, either under construction or in operation, would be sensitive to even the more pessimistically coupled dark-matter axions. This talk reviews the state of these searches. Video
March 9, 2017 Elena Pierpaoli - USC The Cosmos seen through the Planck satellite eyes The Cosmic Microwave Background (CMB) radiation allows us to study processes of the very early Universe. The detailed study of its anisotropies with the Planck satellite allowed to determine cosmological parameters at unprecedented level of precision. As a byproduct, it also provided important results in several areas of astrophysics such as the detection of clusters through their Sunyavev-Zeldovich signature and characterization of Galactic emission at microwave and infrared wavelengths. The Planck satellite, which was launched in 2009, has completed collecting data and most results have recently been released. I will review the main achievements of the latest data release and interpretation, including the determination of main cosmological parameters, epoch of star formation, galaxy clusters detection and use. I will also discuss future prospects in CMB studies. Video 
March 2, 2017 Christoph Haselwandter - USC Physical Mechanisms of Membrane Protein Organization and Collective Function Cell membranes are one of the fundamental hallmarks of life. For many of their biological functions, cell membranes rely on the collective properties of lattices of interacting membrane proteins. Here we explore the general physical mechanisms and principles underlying supramolecular organization and collective function of membrane proteins, based on three model systems: (1) We show how the interplay of protein-induced lipid bilayer curvature deformations, topological defects in protein packing, and thermal effects can explain the observed symmetry and size of membrane protein polyhedral nanoparticles; (2) We predict that the observed four- and five-fold symmetric states of mechanosensitive ion channels yield characteristic lattice architectures of channel clusters, with distinctive collective gating properties; (3) We show that lipid bilayer-mediated elastic interactions between chemoreceptor trimers provide a physical mechanism for the observed self-assembly of chemoreceptor lattices, and may contribute to the cooperative signaling response of the chemotaxis system. Video
February 23, 2017 Harry Nelson - UCSB Touch the Dark Matter We know from astrophysical evidence that the vast majority of matter in our Universe neither absorbs nor emits light. Does this `Dark Matter' have any relation to the strong, electromagnetic, or weak interactions that comprise our `Standard Model' of particle physics? I'll discuss the current & future world program to detect the dark matter in terrestrial experiments, with particular emphasis on the intense competition among experiements that utilize liquid xenon. The flagship US dark matter experiment, LZ, is part of that competition, and just received final Department of Energy approval. Video
February 16, 2017 Nathaniel Craig - UCSB Is Nature Natural? The discovery of the Higgs boson at the LHC marks the culmination of a decades-long quest for the final piece of the Standard Model. But the discovery of the Higgs also adds new urgency to the hierarchy problem, namely the question of why the Higgs boson is so light despite its unique quantum sensitivity to much higher energy scales. This puzzle is made all the more challenging by the lack of evidence for conventional approaches to the hierarchy problem at the LHC and other experiments. In this talk I'll discuss the essential features of the hierarchy problem and its possible solutions, with a particular focus on new approaches to the problem that have emerged in the years following the Higgs discovery. These new approaches feature novel experimental signatures, add urgency to the measurement of Higgs properties, and may shed light on dark matter and other mysteries of the Standard Model. Video
February 9, 2017 ALice Shapley - UCLA The MOSFIRE Deep Evolution Field (MOSDEF) Survey: A Detailed Census of the Physics of Galaxy Formation in the Early Universe Understanding the formation and evolution of galaxies remains one of the great challenges of modern cosmology. Key outstanding questions include: What are the physical processes driving the formation of stars in individual galaxies? How do galaxies exchange material with their intergalactic environments? How do the impressive variety of galactic structures that we observe today assemble? How do supermassive black holes affect the evolution of their host galaxies? We present new results from the MOSFIRE Deep Evolution Field (MOSDEF) survey, a comprehensive census of the galaxy population during the peak epoch of activity in the universe ~10 billion years ago. In addition to providing an overview of the MOSDEF survey and its science, we focus on new results regarding the evolving physical conditions in star-forming regions towards higher redshift. Our new results suggest many exciting future observational directions for untangling the detailed nature of star formation in the early universe. Video
February 2, 2017 Hendrik Ohldag - Stanford Synchrotron Radiation Laboratory Ultrafast and Very Small: Discover Nanoscale Magnetism With Picosecond Time Resolution Using X-Rays Today’s magnetic device technology is based on complex magnetic alloys or multilayers that are patterned at the nanoscale and operate at gigahertz frequencies. To better understand the behavior of such devices one needs an experimental approach that is capable of detecting magnetization with nanometer and picosecond sensitivity. In addition, since devices contain different magnetic elements, a technique is needed that provides element-specific information about not only ferromagnetic but antiferromagnetic materials as well. Synchrotron based X-ray microscopy provides exactly these capabilities because a synchrotron produces tunable and fully polarized X-rays with energies between several tens of electron volts up to tens of kiloelectron volts. The interaction of tunable X-rays with matter is element-specific, allowing us to separately address different elements in a device. The polarization dependence or dichroism of the X-ray interaction provides a path to measure a ferromagnetic moment and its orientation or determine the orientation of the spin axis in an antiferromagnet. The wavelength of X-rays is on the order of nanometers, which enables microscopy with nanometer spatial resolution. And finally, a synchrotron is a pulsed X-ray source, with a pulse length of tens of picoseconds, which enables us to study magnetization dynamics with a time resolution given by the X-ray pulse length in a pump-probe fashion. The goal of this talk is to present an introduction to the field and explain the capabilities of synchrotron based X-ray microscopy, which is becoming a tool available at every synchrotron, to a diverse audience. The general introduction will be followed by a set of examples, depending on the audience, that may include properties of magnetic materials in rocks and meteorites, magnetic inclusions in magnetic oxides, interfacial magnetism in magnetic multilayers, and dynamics of nanostructured devices due to field and current pulses and microwave excitations. Video
January 19, 2017 Xiaoping Hu - UCR MRI: A Field with Endless Advances and Diverse Biomedical Applications Although MRI was invented more than 40 years ago and has been a routine diagnostic imaging modality in clinical practice for more than 30 years, it is still an area of active research with advances being continuously made. These advances have been brought about by technological developments and introduction of new biomedical applications. This talk will provide a brief review major milestones in MRI and highlight some recent advances, particularly those related to neuroimaging. Video
January 12, 2017 Mark Alber - UCR Combined Multi-scale Computational and Experimental Studies of Bacterial Swarming and Blood Clot Formation Surface motility such as swarming is thought to precede biofilm formation during infection. Population of bacteria P. aeruginosa, major infection in hospitals, will be shown to efficiently propagate as high density waves that move symmetrically as rings within swarms towards the extending tendrils. Multi-scale model simulations suggest a mechanism of wave propagation as well as branched tendril formation at the edge of the population that depend upon competition between the changing viscosity of the bacterial liquid suspension and the liquid film boundary expansion caused by Marangoni forces. This collective mechanism of cell-cell coordination was shown to moderate swarming direction of individual bacteria to avoid antibiotics. In the second half of the talk, a novel three-dimensional multi-scale model will be described for simulating receptor-mediated adhesion of deformable platelets at the site of vascular injury under different shear rates of blood flow. The modeling approach couples submodels at three biological scales crucial for the early clot formation: novel hybrid cell membrane submodel to represent physiological elastic properties of a platelet, stochastic receptor–ligand binding submodel to describe cell adhesion kinetics and lattice Boltzmann submodel for simulating blood flow. Predictive model simulations revealed that platelet deformation, interactions between platelets in the vicinity of the vessel wall as well as the number of functional GPIba platelet receptors played significant roles in platelet adhesion to the injury site. Lastly, macro-scale model of blood clot deformation and deformation of blood vessel will be described. The model represents clot as a ternary complex fluid made of heterogeneously distributed platelets, fibrin network and plasma phases and takes into account mechanical properties of different phases. Video
December 1, 2016 Dr. Zvi Bern - UCLA A curious story of quantum gravity in the ultraviolet For the past 30 years nearly all theoretical physicists have believed that quantum field theories based on Einstein's general relativity necessarily must be ill-defined in the ultraviolet. This is the well known nonrenormalizability problem of gravity. But is it actually true, in general? We describe recent calculations that cast doubt on this simple picture and show that quantum gravity is much tamer in the ultraviolet than believed possible. The new calculations make use of enormous advances in our ability to compute scattering amplitudes in quantum field theory by relating gravity theories to gauge theories. Applications to black holes will be mentioned.  Video
November 17, 2016 Dr. Boris Shraiman - KITP Physics and Biology of Morphogenesis One hundred years ago, D'Arcy Thompson – a nineteenth century polymath, working at the turn of the twentieth century – wrote a monograph, "On Growth and Form", in which he pondered the geometry of living forms and how it emerges in the process of Morphogenesis. Thompson was ahead of his time. Since then, progress of Developmental Biology and Molecular Genetics uncovered many if not most of key genes and molecules involved in Morphogenesis, yet Thompson's agenda of understanding how developmental processes actually specify the geometry of tissues, limbs and organs is far from complete. A particular challenge is to bridge the gap between microscopic scales, where molecular mechanisms operate, and the macroscopic scales of animal "shape and form". This challenge offers much for a Physicist to think about. This talk will focus in particular on the mechanical aspects of morphogenesis i) examining the role of mechanical stress in regulation of growth and ii) seeking a quantitative understanding of tissue flows observed in morphogenesis. At the interface of Physics and Biology we will find some new biology and new physics.  Video
November 10, 2016 Dr. Rui-Rui Du - Rice Electronic Superhighway in Topological Insulators Electrical insulators commonly refer to the materials that prevent the flow of electricity. However, recent research demonstrates a type of topological insulators which has novel properties. Although electricity cannot flow through them, it can flow around their narrow outer edges. The material, called a "quantum spin Hall topological insulator", acts as an electronic superhighway. It is one of the building blocks needed to create future electronics and computers. In this talk I will show such insulators can be built from common compound semiconductors containing a double-layer of electrons and holes, which are created by band-gap engineering using molecular beam epitaxy and electrostatic gates. The material supports quantized helical edge modes. Amazingly, due the interactions between electron and holes, the material can become a superconductor, where the pairing of electron and holes resembles the Cooper pair in ordinary superconductors.  Video
November 3, 2016 Dr. Ehud Altman - Berkeley Ergodicity, entanglement and many-body localization in quantum dynamics. Do quantum many-body systems necessarily come to thermal equilibrium after a long enough time evolution? The conventional wisdom has long been that they do and that, in the process, any quantum information encoded in the initial state is lost irretrievably. Thus the dynamics of many interacting particles becomes effectively classical. But these ingrained notions of thermalization and ergodicity have recently been called into question. In this talk I will discuss how ergodicity can break down in disordered quantum systems through the phenomenon of many-body localization. In contrast to thermalizing fluids, quantum correlations can persist through time evolution of the localized state even at high energy densities. Thus, investigating the many-body localization transition offers a concrete route to address fundamental unsolved questions concerning the boundary between classical and quantum physics in the macroscopic world. I will emphasize the important role that quantum entanglement plays in current attempts to understand this fascinating dynamical phase transition. Finally I will present recent progress in confronting the emerging theoretical understanding of many-body localization with experimental tests using systems of ultra-cold atoms.  Video
October 27, 2016 Dr. Barry Barish - Caltech LIGO and the Detection of Gravitational Waves Einstein predicted the existence of gravitational waves 100 years ago. They have been recently observed from pairs of merging Black Holes by the Laser Interferometer Gravitational-wave Observatory (LIGO). The physics of gravitational waves, the detection technique, the observations, including latest results, and implications will all be discussed.  Video
October 13, 2016 Stephen Kane - San Francisco State University Analyzing Alien Worlds: A Multidisciplinary Approach to Characterizing Exoplanets About the Speaker: Stephen Kane has been researching planets orbiting other stars for more than 20 years. He has discovered and characterized hundreds of exoplanets, including Kepler-186f, which is the smallest planet yet found in the Habitable Zone of a star. After spending many years working at the NASA Exoplanet Science Institute, Kane is now an Associate Professor of Astrophysics at San Francisco State University (SFSU). He is the Chair of the Kepler Habitable Zone Working Group and the Director of the Planetary Research Laboratory at SFSU. Stephen is involved in several upcoming and ongoing NASA missions in ways that dovetail seamlessly with the UCR-based team of the NASA Astrobiology Institute. His work with the Deep Space Climate Observatory is the first major effort to use Earth's rotation and albedo to model modern Earth as an exoplanet. He is also leading a project to use the future James Webb Space Telescope to detect evidence for volcanic activity on terrestrial planets discovered with TESS, the Transiting Exoplanet Survey Satellite scheduled for launch in 2017. Abstract: The number of exoplanet discoveries has increased dramatically over the past several decades, requiring a planetary classification system to encompass the enormous diversity among worlds. Exoplanetary science can be broadly divided into categories of detection, characterization, and habitability. Kane's research has allowed him to address leading questions in all three areas: detecting multi-planet systems, determining the stability of planetary orbits, analyzing planetary atmospheres, and predicting the effects of both planetary orbit and geological activity on habitability. In this seminar, he will present highlights from his survey of potentially transiting exoplanets and his role in recent exoplanet discoveries. He will also present the results from his newly published catalog of Kepler planets in the habitable zones of their host stars and describe the methodology he developed for distinguishing between Earth and Venus analogs. Finally, he will describe future opportunities from both ground and space-based observatories that will be used to provide a more complete understanding of comparative planetology.  
October 6,2016 Jesse Thaler - MIT New Physics Gets a Boost: Jet Substructure at the Large Hadron Collider Collisions at the Large Hadron Collider (LHC) are dominated by jets, collimated sprays of particles that arise from quantum chromodynamics (QCD) at high energies. With the remarkable performance of the ATLAS and CMS detectors, jets can now be characterized not just by their overall direction and energy but also by their substructure. In this talk, I highlight the increasingly important role that jet substructure is playing in searches for dark matter and other new physics at the LHC, especially when exploring extreme kinematic regimes involving large Lorentz boosts. I also explain how innovative theoretical studies of jet substructure have taught us surprising lessons about QCD, revealing new probes of hot dense matter and universal features of gauge theories.  
September 29, 2016 DR. Samindranath Mitra - PRL Editor Physics after the lab and the desk: Your work in PRL Physics research takes place mostly at your desk, at the keyboard, in the lab. You communicate results through posters, talks, and papers -- leading to, hopefully, wide dissemination and recognition. This sequence entails interacting with journal editors, referees, conference chairs, journalists, and so on. I will focus on this post-research collaborative process in physics, primarily through the lens that is Physical Review Letters.  
September 22, 2016 Dr. Brian Siana - UCR Dwarf Galaxies in the Early Universe: Finding and Characterizing the Other Half of Star Formation Small galaxies in the early universe are incredibly important. They comprise the majority of early star formation, reionized the hydrogen in the intergalactic medium and populated it with heavier elements. Furthermore, mysteries about the abundance and dynamics of dwarf galaxies today may be giving insights into the properties of dark matter or, alternatively, may arise from baryonic process during early star formation episodes. To understand these star formation episodes, we first have to see the dwarf galaxies. I will summarize our research using gravitational lenses to get a census of these previously unobservable dwarf galaxies, and to better characterize their star formation histories and ionizing emission.  
June 2, 2016 Henri Orland - CEA- Saclay, Paris Pseudoknots and knots in RNA After reviewing some elementary properties of RNA, we recall how secondary structures of RNA without pseudoknots can be computed using simple concepts of statistical physics. The situation is much more complex when dealing with RNA structures with pseudoknots. In that case, inspired by matrix field theory, we introduce a classification of pseudoknots in terms of their topological genus. The standard free energy parametrization is modified to include a penalty proportional to the genus of the RNA structure, and we present two algorithms to efficiently predict RNA structures with pseudoknots. In the last part of the talk, we address the question: Are there knots in RNA? To try to answer this question, we present a thorough study of the database of all known RNA structures.  
May 26, 2016 Harry Teplitz - IPAC Infrared Grism Spectroscopy from Space: Hubble Results and Preparing for New Missions Slitless grism spectroscopy is an efficient way for space telescopes to obtain large samples of low resolution spectra in the near infrared wavelength range. The Hubble Space Telescope’s Wide Field Camera 3 (WFC3) offers a powerful example of this technique. I will review current results from WISPs (WFC3 Infrared Spectroscopic Parallel survey), which observes “random” parallel fields 5 to 8 arcminutes away from primary observations taken by other instruments. The WISPs dataset includes almost 2000 hours of HST data, which have led to a range of discoveries in the study of galaxy evolution. In addition, WISP is the ideal pathfinder for planning the future WFIRST and Euclid missions, which will both employ near infrared grisms over thousands of square degrees of the extragalactic sky.  
May 19, 2016 Laura Sales - UCR Dwarf galaxies and their satellites as extreme probes of LCDM The cosmological scenario (Lambda Cold Dark Mater, LCDM) makes three clear predictions for the dark matter halos surrounding galaxies: 1) the number of halos steeply rises towards low-mass objects, 2) halos are "cuspy" at their centers and 3) there should be a wealth of substructure swarming around each of these halos. We use cosmological numerical simulations of halos and galaxies to explore these predictions and to compare them with available observational constraints, such as the Baryonic Tully-Fisher relation and the inventory of dwarfs (low-mass galaxies) in the Local Volume. The recent detection of several dwarf galaxies potentially associated with the Magellanic Clouds is an exciting discovery that confirms that the hierarchical nature of galaxy formation extends down to the faintest limits probed, just as predicted by LCDM. On the other hand, the extreme baryon content of some isolated dwarfs together with the large variety of rotation curve profiles for these objects presents a newly recognized challenge to the paradigm that still awaits resolution. Do we need to move beyond Cold Dark Matter?  
May 12, 2016 Arjun Dey - NOAO Mapping the Universe: A New Generation of Sky Surveys The Dark Energy Spectroscopic Instrument project, which will begin operations in 2019, will measure the expansion history of the universe to unprecedented precision and provide sub-percent constraints on the distance scale and the equation of state of dark energy. I will describe the current state of the project and the wide-field imaging surveys that are being undertaken in preparation for the DESI spectroscopic survey. These imaging surveys are using state-of-the-art red-sensitive cameras and will benefit a wide range of astrophysical studies. The data sets being created will have lasting legacy value, well into the LSST era.  
May 5, 2016 Tony Tyson - UC Davis LSST and the physics of the dark universe The physics that underlies the accelerating cosmic expansion is unknown. This, "dark energy" and the equally mysterious "dark matter" comprise 96% of the mass-energy of the universe and are outside the standard model. Recent advances in optics, detectors, and information technology, has led to the design of a facility that will repeatedly image an unprecedented volume of the universe: LSST. For the first time, the sky will be surveyed wide, deep and fast. The history of astronomy has taught us repeatedly that there are surprises whenever we view the sky in a new way. I will focus on the technology of LSST, and review several independent probes of the nature of dark energy and dark matter. These new investigations will rely on the statistical precision obtainable with billions of galaxies.  
April 28, 2016 Kirill Shtengel - UCR Anyonics: Exotic circuitry with anyons, or how to build a Flux Capacitor Anyons (particularly non-Abelian anyons) are widely sought for the exotic fundamental physics they harbour as well as for their possible applications for quantum information processing. Currently, there are numerous blueprints for stabilizing the simplest type of non-Abelian anyon, a Majorana zero energy mode bound to a vortex or a domain wall. One such candidate system, a so-called "Majorana wire" can be made by judiciously interfacing readily available materials; the experimental evidence for the viability of this approach is presently emerging. Following this idea, we introduce a device fabricated from conventional fractional quantum Hall states, s-wave superconductors and insulators with strong spin-orbit coupling. Similarly to a Majorana wire, the ends of our “quantum wire” would bind "parafermions", exotic non-Abelian anyons which can be viewed as fractionalized Majorana zero modes.I will briefly discuss their properties and describe how such parafermions can be used to construct new and potentially useful circuit elements which include current and voltage mirrors, transistors for fractional charge currents and "flux capacitors".  
April 21, 2016 - Daniel Cox UC Davis Proteins as Molecular Legos: How Lessons Learned from Mad Cow Disease can be Applied to Novel Materials and Biotechnology The unregulated yet ordered self-assembly of large disordered proteins such as prion and tau contribute to neurodegenerative diseases like mad cow and Alzheimer’s. Nevertheless, organisms as diverse as yeast, spiders, lacewings, and E. coli bacteria have evolved mechanisms to harness these protein aggregation processes for their benefit, using the proteins effectively as “Molecular Legos”. In this talk I will discuss how related “beta solenoid” proteins can be engineered to undergo this self-assembly in a controlled way to produce remarkably stable and beautifully ordered structures that can be harnessed for nanotechnology and biotechnology applications including energy harvesting and biosensing. I will discuss the physics of the aggregation process, how you can measure it with Rayleigh scattering, and how you can measure the mechanical toughness with both computer simulations and high intensity ultrasound. We find that the filaments of our engineered beta solenoid proteins are stiff against bending and twist, and have a mechanical toughness comparable to Kevlar.  
April 14,2016 Bharat Ratra - Kansas State University Dark Energy: constant or time variable? (... and other open questions) Experiments and observations over the last two decades have persuaded cosmologists that (as yet undetected) dark energy is by far the main component of the energy budget of the universe. I review a few simple dark energy models and compare their predictions to observational data, to derive dark energy model-parameter constraints and to test consistency of different data sets. I conclude with a list of open cosmological questions.  
April 7, 2016 Alex Rudolph - California State Polytechnic University CAMPARE and Cal-Bridge: Engaging Underrepresented Students in Physics and Astronomy The level of participation by underrepresented minority (URM) and female students in physics and astronomy PhD programs is shamefully low (2-4% for URM v. 30% in the general population; 20% for women v. 50% in the general population). I will begin by discussing research into why these participation rates are so low for these groups, highlighting role the physics and general GRE tests play in suppressing diversity in our field, while providing little to no benefit in helping predict long-term success. I will then describe some alternative methods of conducting graduate admissions, including the role of programs like Cal-Bridge and CAMPARE. I will then describe these two California-wide, multi-institutional programs, CAMPARE and Cal-Bridge, with the common mission of increasing participation of underrepresented minorities and women in astronomy and physics through summer research opportunities, in the case of CAMPARE, scholarships in the case of Cal-Bridge, and significant mentoring and professional development in both programs, leading to an increase in their numbers completing bachelor’s degrees, and successfully pursuing a PhD in these fields. There are plans for an expansion of the Cal-Bridge program to include students interested in physics PhDs, as well as to make it statewide. I will be talking about how UCR physics and astronomy faculty can get involved in the program and these expansion efforts.  
March 31, 2016 Joshua Lui - UCR Shedding light on two-dimensional electrons in graphene and beyond Graphene, a single layer of carbon atoms, has stimulated intense scientific interest due to its distinctive electronic and mechanical properties. Graphene exhibits strong interactions with light over a broad spectral range. This enables us to examine its electronic and vibrational properties through optical spectroscopy. In addition to gaining understanding of the properties of single-layer graphene, we can also probe the behavior of electrons in few-layer graphene. This reveals the unique electronic and vibrational properties for graphene of each layer thickness and stacking order, as well as their distinct capability to induce an electrically tunable band gap. I will also highlight recent development of 2D materials beyond graph  
March 10, 2016 Evan Kirby - Caltech Dwarf Galaxies: Laboratories for Nucleosynthesis and Dark Matter The Milky Way is surrounded by dozens of dwarf galaxies. Although these galaxies contain as few as 1000 stars (compared to 100 billion stars in the Milky Way), they have masses equivalent to millions of stars. The extra mass suggests that dwarf galaxies are reservoirs for dark matter.  
March 3, 2016 Micahel M. Fogler - UC San Diego Hyperbolic waves in Nature: from nano to Terra Waves with hyperbolic dispersion relation are exotic yet surprisingly widespread phenomena that occur in anisotropic media with internal resonances. Such media have been investigated in numerous fields, ranging from engineering to condensed matter physics to optics to fluid dynamics and geophysics. Hyperbolic waves can be found in magnetic materials, in both usual and topological insulators, in superconductors, as well as in our oceans, beaches, atmosphere, and space. The characteristic lengths and frequencies of such waves vary vastly, from atomic to cosmic. However, they all exhibit certain common attributes, such as strict directionality, diverging density of states, and anomalous reflection. This talk will contain a primer on hyperbolic materials, a recipe for a death ray, and a report on our nano-optics studies of hyperbolic phonon-polaritons in new quasi-2D materials such as graphene and hexagonal boron nitride.  
February 25, 2016 Jim Olsen - Princeton University Dispatches from the Energy Frontier: Latest results from the Large Hadron Collid In May, 2015 the Large Hadron Collider (LHC), the world’s highest energy particle collider, resumed operations after a two year shutdown. The downtime was used to prepare the machine and detectors for proton collisions at higher energy and intensities than have ever been achieved before. Following the discovery of the Higgs boson in 2012, which led to the awarding of the Nobel Prize in Physics to Peter Higgs and Rene Englert, the primary focus on the two large experiments, ATLAS and CMS, operating at the LHC is to search for signs of new particles or interactions that could either shed light on unexplained mysteries of the Standard Model of particle physics, or even provide evidence of unexpected phenomena not previously predicted. One interesting example of such a scenario was recently reported by ATLAS and CMS, where both experiments see an excess of events containing two photons that could be the first hint of a new particle with a mass near 750 GeV. In this colloquium I will present recent results from the LHC, including the diphoton excess and searches for supersymmetric particles and other exotic phenomena, as well as a host of new measurements establishing the Standard Model at the unprecedented energy of 13 TeV. I will close with a brief outlook on expectations for the LHC in the near and long term.  
February 18, 2016 Marusa Bradac - UC Davis Dark Matter and First Galaxies Light Up The Bullet Cluster has been the subject of intense research in the last few years. This system is remarkably well-suited to addressing outstanding issues in both cosmology and fundamental physics. I will present measurements of the composition of this system, show the evidence for existence of dark matter, and describe limits that we placed on the intrinsic properties of dark matter particles. I will also present results from a much larger sample of Bullet-like clusters, MACSJ0025-1222, A520, and DLSCL J0916.2+2951 among others.  
February 11, 2016 Itai Cohen - Cornell University Flight of the Fruit Fly There comes a time in each of our lives where we grab a thick section of the morning paper, roll it up and set off to do battle with one of nature’s most accomplished aviators - the fly. If however, instead of swatting we could magnify our view and experience the world in slow motion we would be privy to a world-class ballet full of graceful figure-eight wing strokes, effortless pirouettes, and astonishing acrobatics. After watching such a magnificent display, who among us could destroy this virtuoso? How do flies produce acrobatic maneuvers with such precision? What control mechanisms do they need to maneuver? More abstractly, what problem are they solving as they fly? Despite pioneering studies of flight control in tethered insects, robotic wing experiments, and fluid dynamics simulations that have revealed basic mechanisms for unsteady force generation during steady flight, the answers to these questions remain elusive. In this talk I will discuss our strategy for investigating these unanswered questions. I will begin by describing our automated apparatus for recording the free flight of fruit flies and our technique called Hull Reconstruction Motion Tracking (HRMT) for backing out the wing and body kinematics. I will then show that these techniques can be used to reveal the underlying mechanisms for flight maneuvers, wing actuation, and flight stability. Finally, I will comment on the implications of these discoveries for investigations aimed at elucidating the evolution of flight.  
February 4, 2016 Dan Stark - University of Arizona Galaxies in the Reionization Era Deep infrared images from the Hubble and Spitzer Space Telescopes have recently pushed the cosmic frontier back to just 500 million years after the Big Bang, delivering the first large sample of galaxies at redshifts between 7 and 10. Sometime in this redshift window the hydrogen in the intergalactic medium transitioned from mostly neutral to ionized. Over the past five years, our understanding of this process of reionization has improved greatly. The census of early galaxies derived from deep Hubble imaging has provided new insight into the role of star forming galaxies in driving reionization, while follow-up spectroscopy has constrained the timescale over which the transition happened. Most recently, deep MOSFIRE spectra have begun to provide the first glimpse of the physical nature of early galaxies, hinting at a very different population from what has been observed at lower redshifts. I will review the latest progress in our understanding of the first billion years of cosmic history and discuss the remaining challenges that must be addressed in advance of JWST.  
January 28, 2016 Mlke Roney - University of Victoria Applying Quantum Entanglement to Search for New Physics at TeV Energies Collisions of electrons and positrons can create B-meson particles in an entangled state. I will explain how the BABAR experiment has applied the associated Einstein–Podolsky– Rosen effect to study differences between matter and antimatter known as CP violation, as well as how it has used the effect to observe the “quantum arrow of time”. The Belle II/SuperKEKB facility that is currently being commissioned in Japan will extend these studies and will be sensitive to new physics at energies well above those available at the Large Hadron Collider. I will describe how it will do so and investigate the evidence for new physics published by BABAR and recently corroborated by the Belle and LHCb experiments.  
January 21, 2016 Tony Heinz - Departments of Applied Physics and Photon Science, Stanford University Two-Dimensional Materials - Graphene and Beyond Graphene, a single atomic layer of carbon atoms, has attracted great attention worldwide because of its potential for novel science and technology. Recently, this interest has expanded to the much wider class of two-dimensional materials that occur naturally as 2D layers of van-der-Waals crystals. While preserving graphene’s flexibility and tunability by external perturbations, atomically thin layers of this broader set of materials provides access to more varied electronic and optical properties, including semiconducting and insulating behavior. In our presentation, we will discuss the distinctive properties of these atomically thin 2D materials, emphasizing how they can be probed by light. For the prototypical system of graphene, the electronic response has been investigated from the THz to the UV, revealing many interesting physical properties of 2D Dirac fermions. Atomically thin layers of semiconductors in the family of transition metal dichalcogenides (MX2 where M = Mo, W and X = S, Se, Te) have also been investigated. Although weak light emitters as bulk crystals, at monolayer thickness these materials emit light efficiently. We will describe some of the surprising characteristics exhibited by these materials in the 2D limit, from their strong and anomalous excitonic effects to valley selective excitation and control.  
January 14, 2016 Bertrand Echenard - Caltech The Mu2e experiment: finding a needle in a trillion haystacks The Mu2e experiment at Fermilab will be the world's most sensitive search for neutrinoless muon-to-electron conversion, a charged lepton-flavor violating process. Although neutral lepton-flavor violation has been clearly established in the neutrino sector, no sign of charged lepton-flavor violation has been detected so far, despite decades of experimental searches. An observation would constitute an unambiguous sign of physics beyond the standard model, and severely constrain new theoretical models. The Mu2e experiment will improve the current sensitivity to muon-to-electron conversion by four orders of magnitude, and indirectly probe energy scales well beyond the reach of the LHC.  
January 7, 2016 Henk Postma - Cal State Northridge Towards rapid sequencing of individual DNA molecules with graphene nanogaps I will describe our lab's latest efforts in realizing a graphene nanogap device that may be used for sequencing individual DNA molecules. The technique is based on reading the base sequence of a single DNA molecule using a graphene nanogap to read the DNA’s transverse conductance. Because graphene is a single atom thick, single-base resolution of the conductance is readily obtained. The nonlinear current-voltage characteristic is used to determine the base type independent of nanogap-width variations that cause the current to change by 5 orders of magnitude. The expected sequencing error rate is 0% up to a nanogap width of 1.6 nm.  
December 3, 2015 James Bullock - UCI Dwarf Galaxies, the Local Group, and Cosmology The Local Group and the tiny galaxies that surround the Milky Way provide unique and detailed data sets for testing ideas in cosmology and galaxy formation. In this talk I will discuss how numerical simulations coupled with local "near-field" observations are informing our understanding of dark matter, the formation of the first galaxies, and the physical processes that act at the threshold of galaxy formation.  
November 19, 2015 DR. Thorsten Emig - MIT and CNRS Paris Geometrically constrained fluctuations The modification of (quantum and thermal) fluctuations due to geometrical constraints give rise to a plethora of effects in equilibrium and non-equilibrium systems. Prominent examples include QED and critical Casimir interactions between macroscopic bodies, van der Waals forces between atoms and surfaces, and heat radiation and transfer. I shall review recent theoretical and experimental progress in the field, with applications extending from nano-systems over soft matter to urban physics.  
November 12, 2015 John Chalker - Oxford Geometrically frustrated magnets and spin liquids Magnetic materials and theoretical models of them provide standard paradigms in condensed matter physics for the idea of ordering, in which interactions lead to a limited number of symmetry-related low-temperature states. Geometrical frustration is interesting as a way of making something different happen. Frustrated magnets have interactions that compete with each other, and they fluctuate between many different states even at low temperature. In this sense they provide an analogue for spin systems of the liquid phase of ordinary matter. Spin liquids, however, turn out to be much more interesting in important ways than ordinary liquids: in their low-energy states the microscopic magnetic moments are ``dissolved" by fluctuations and re-form as new degrees of freedom, often involving emergent gauge fields and fractionalised quasiparticles. I aim to present a simple overview of ideas in this field and to summarise some recent work on the dynamics of an exactly solvable model -- the Kitaev honeycomb model -- that has a spin liquid ground state.  
November 5, 2015 Qian Niu - UT Austin Orbital Magnetism and Landau Levels A semiclassical theory of electron dynamics is derived which is accurate to second order in the magnetic field. We show how various geometric effects exhibit in the magnetic susceptibility as well as in the orbital magnetization. We also obtain a simple relation between the Landau level index and the magnetic response functions. One can thus obtain accurate Landau levels from first principles calculations, or measure the magnetic response functions from Landau level data.  
October 29, 2015 Alan Rein - NCI Putting the Pieces Together: The Building Block of HIV-1 Virus Particles and How it is Assembled AIDS is caused by a virus called HIV-1. We will describe the replication cycle of the virus. A single virus-coded protein, “Gag”, is the building block of HIV-1 virus particles. We are studying the mechanisms by which several thousand Gag molecules are assembled into an “immature” HIV-1 particle and analyzing the structure of these particles. In a subsequent step in the viral life cycle, the Gag proteins in the immature particle are cleaved. These “maturation cleavages” result in a global reorganization of the particle and are absolutely required for viral infectivity. New results on a molecular switch triggering particle assembly will be presented.  
October 22, 2015 Arun Paramekanti - U Toronto Band topology meets correlations - from solid state to cold atoms. The mathematics of topology plays an important role in many recently discovered effects in solid state matter, ranging from the quantum anomalous Hall effect to the quantum spin Hall effect and its higher dimensional generalizations. Recent work on cold atoms has also realized such physics by designing novel optical lattices and using lasers to create artificial orbital magnetic fields for neutral atomic gases. The interplay of such topological phases and interparticle interactions is a largely open field of research. The talk will give an introduction to this field and discuss some of our theoretical work, including the discovery of unusual forms of magnetism in spin-orbit coupled oxides and atomic gases, oxide heterostructures as platforms to realize quantum anomalous Hall phases, and emergence of novel phases at topological quantum critical points. more details» copy to my calendar  
October 15, 2015 Chung-Pei Ma - UC Berkeley Supermassive Black Holes in Nearby Galaxies Black holes are among the most fascinating astrophysical objects and have long entranced the public. For over three decades, the giant elliptical galaxy Messier 87 has hosted the most massive known black hole in the local universe. New kinematic data and improved models in the past few years have substantially expanded and revised dynamical measurements of black hole masses at the centers of nearby galaxies. I will describe recent progress in discovering black holes beyond ten billion solar masses in ongoing surveys of massive elliptical galaxies. I will present updated scaling relations between the black hole mass and host galaxy properties, and discuss the implications for the formation of massive galaxies and the predicted gravity waves from merging supermassive black hole binaries.  
October 8, 2015 Samir D Mathur - Ohio State Resolution of the black hole information paradox Some 40 years ago Hawking found a remarkable contradiction: if we accept the standard behavior of gravity in regions of low curvature, then the evolution of black holes will violate quantum mechanics. Resolving this paradox would require a basic change in our understanding of spacetime and/or quantum theory. In recent years the paradox has found an interesting resolution through string theory. While quantum gravity is normally expected to be important only at distances of order planck length, the situation changes when a large number N of particles are involved, as for instance in the situation where we make a large black hole. Then the length scale of quantum gravity effects grows with N, altering the black hole structure to a "fuzzball"; this effect resolves the paradox.  
October 1, 2015 John Martinis - UCSB What’s next after Moore’s law: quantum computing As microelectronics technology nears the end of exponential growth over time, known as Moore’s law, there is a renewed interest in new computing paradigms. I will discuss recent research at UCSB on superconducting quantum bits, as well as our recent start at Google to build a useful quantum computer to solve machine learning problems. Two qubit experiments will be highlighted, one to simulate a chemical reaction that finds a cross section, and a second to extend the lifetime of a qubit state using quantum error correction.  
June 4, 2015 Michael Rich - UCLA The Central Bulge of our Galaxy: New Insights and Mysteries Half of the light in the local Universe arises from the old stars in elliptical galaxies and bulges of spiral galaxies. At the center of our Galaxy lies a region called the "bulge" consisting of stars older and generally more metal rich than those in the disk, and hosting the Milky Way's central black hole. The central bulge population of our Milky Way is 700 times closer than the nearest similar stars in M31, providing a remarkable opportunity to learn the age, composition, kinematics, structure, and origin of this population. Present cold dark matter models suggest that the Milky Way and similar galaxies should have been bombarded by the infall of satellite galaxies during their lifetime and galaxies with bulges like that of our Milky Way would be predicted to not have survived in the form we observe today. I will discuss two new survey programs: one uses the Dark Energy Camera at the Cerro Tololo Observatory to image the central 1000 parsecs of the Milky way, and the other survey aims to measure the composition of giants just a few parsecs distant from the Milky Way's central supermassive black hole. We also consider what the next generation of ground- and space- based telescopes may uncover.  
May 28, 2015 Brant Robertson - University of Arizona New Constraints on Cosmic Reionization from Planck and Hubble Space Telescope Understanding cosmic reionization requires the identification and characterization of early sources of hydrogen-ionizing photons. The 2012 Hubble Ultra Deep Field (UDF12) campaign acquired the deepest blank-field infrared images with the Wide Field Camera 3 aboard Hubble Space Telescope and, for the first time, systematically explored the galaxy population deep into the era when cosmic microwave background (CMB) data indicates reionization was underway. High-redshift observations with HST including UDF12, CANDELS, and the Frontier Fields provide the best constraints to date on the abundance, luminosity distribution, and spectral properties of early star-forming galaxies. We synthesize results from these HST campaigns and the most recent constraints from Planck CMB observations to infer redshift-dependent ultraviolet luminosity densities, reionization histories, and electron scattering optical depth evolution consistent with the available data. We review these results, and discuss future avenues for progress in understanding the epoch of reionization.  
May 21, 2015 Heather Knutson - Caltech Atmospheres of Extrasolar Planets in the Super-Earth Era Ongoing surveys of nearby stars have revealed an amazing diversity of planetary systems, many of which have characteristics that differ substantially from those of the solar system planets. Perhaps one of the biggest surprises to come out of these surveys was the discovery that "super-Earths" (planets between 1-10 times the mass of the Earth) are in fact the most common type of extrasolar planet. Despite the name we actually know very little about the compositions of these mysterious planets, and it has been suggested that this mass range may include both "water worlds" and "mini-Neptunes" with thick hydrogen envelopes in addition to more Earth-like terrestrial planets. In my talk I will explore current constraints on the compositions of planets with masses ranging from that of Neptune down into the super-Earth regime, and discuss the corresponding implications for our understanding of planet formation and evolution.  
May 14, 2015 Joel Primack - UCSC New Insights on Galaxy Formation from Comparisons of Simulated and Observed Galaxies Computer simulations and theoretical understanding have now reached a stage where simulations are increasingly able to tackle the complexity of galaxy formation and evolution. This talk will describe in particular the successes and challenges of high-resolution hydrodynamic galaxy simulations, now including radiative pressure feedback, in trying to understand the Hubble Space Telescope observations of galaxies during the period of most vigorous star formation (1 < z < 3, “Cosmic High Noon”) [1]. I used to think that galaxies form as disks, that forming galaxies are pretty smooth, and that galaxies generally grow in radius as they grow in mass — but we are now learning that all these statements are false. The majority of star-forming galaxies at z > 1 have recently been shown to have mostly elongated (prolate) stellar distributions [2] rather than disks or spheroids, and our simulations may explain why [3]. A large fraction of star-forming galaxies at redshifts 1 < z < 3 are found to have massive stellar clumps [4]; these originate from violent disk instabilities in our simulations [5-6], which also help to create compact spheroids (“nuggets”) through galaxy compaction [7-9]. We are trying to understand how angular momentum evolves as gas falls toward the inner galaxy and becomes stars [10]. The talk will also describe the Assembling Galaxies of Resolved Anatomy (AGORA) program to run high-resolution simulations using as much as possible the same initial conditions, physical assumptions, and output analysis procedures. AGORA will systematically compare galaxy simulations using a wide variety of computer codes with each other and with observations, and thus improve understanding of galaxy formation [11].  
May 7, 2015 Zhiqiang Mao - Tulane University Interplay between magnetism and superconductivity in iron chalcogenide The interplay between magnetism and superconductivity in Fe-based superconductor systems is currently a subject of intense studies. The iron chalcogenide Fe1+y(Te1-xSex) is of particular interest due to its unique magnetic properties. While the parent compound Fe1+yTe shows antiferromagnetism with (p,0) in-plane magnetic wave vector, the optimally doped sample displays superconductivity with (p,p) spin resonance. This contrasts with iron pnictides in which both the parent compound’s antiferromagnetism and the doped samples’ superconducting (SC) spin resonance are characterized by the in-plane Fermi surface nesting wave vector Qn = (p,p). The evolution from (p,0) magnetism to superconductivity with (p,p) spin resonance in iron chalcogenides is associated with coexistence of magnetic correlations at (p,0) and (p,p). The other remarkable difference between iron chalcogenide and iron pnictide superconductors is their phase diagrams. In iron pnictides, bulk superconductivity either emerges immediately following suppression of long-range (p,p) antiferromagnetic (AFM) order, or coexists with it in a particular composition range. In contrast, in iron chalcogenides, bulk superconductivity does not appear immediately following the suppression of long-range (p,0) AFM order. Instead, an intermediate phase with weak charge carrier localization appears between AFM order and bulk superconductivity for 0.09 < x < 0.3. In this talk, I will first present an overview on the results summarized above and then introduce our recent studies on the coupling between electronic and magnetic properties in this system. I will show the doping dependences of Sommerfeld coefficient ?, Hall coefficient RH and Hall angle as well as their relations with superconductivity. The origin of superconductivity suppression and charge carrier localization in the underdoped region will be discussed in terms of these experimental results.  
April 23, 2015 Alex Evilevitch - Carnegie Mellon University Physical Mechanisms of Viral Life-Cycle Herpesviruses are a leading cause of human viral disease, second only to influenza and cold viruses. Herpesviruses consist of a double-stranded (ds) DNA genome contained within a protein shell, termed the capsid, that is surrounded by an unstructured protein layer (the tegument) and a lipid-envelope. During viral replication, an ATP-dependent motor packages the genome into a preformed capsid through a unique opening created by the portal complex. Herpes Simplex virus type 1 (HSV-1) is a prototypical model system to study the general infection mechanisms of herpesviruses and other viruses that release their genome into the cell nucleus without capsid disassembly. We have recently shown that HSV-1 genome packaging creates an internal pressure of tens of atmospheres within the viral capsid. This pressure results from bending stress and repulsive forces acting on the tightly packaged DNA molecule. We also found that despite its liquid crystalline state inside the capsid, the DNA is fluid-like which facilitates its ejection into the cell nucleus during infection. The fluidity or, equivalently, mobility of the closely packaged DNA strands caused by interstrand repulsive interactions is regulated by the ionic environment of the cellular cytoplasm. Between rounds of replication, the virion must be sufficiently stable to ensure that the packaged genome is retained within the capsid. Conversely, during infection the virion must be unstable enough to allow genome release into the cell nucleus. A precise balance between these physical aspects of the viral capsid and its encapsidated genome is crucial to the viral replication cycle. Using HSV-1 as our primary model system, we investigate the roles of intracapsid DNA mobility and capsid stability for viral replication with respect to retention of the packaged genome inside the capsid and its subsequent ejection during infection. These studies provide new insights into the key mechanisms facilitating as well as inhibiting viral infectivity. This knowledge establishes a foundation for the design of novel mutation resistant drugs for herpesviruses.  
April 16, 2015 Mark Neyrinck - JHU How the Cosmological Dark-Matter Sheet Stretches and Folds up to form Cosmic Structures Structures in the Universe like galaxies, and filaments and clusters of galaxies, are essential components of the arrangement of matter on large scales. They form in analogy to the origami folding of a sheet of dark matter. I will discuss some new results about how this sheet stretches and bunches together in different places. An "origami approximation" is a toy model showing the kinds of structures that form, and the spins that can arise within them. This should help in understanding spin alignments between galaxies, relevant to the weak-lensing systematic effect of intrinsic ellipticity alignments.  
April 9, 2015 James Bullock - UCI Cosmology in the Local Universe The Milky Way and its local environment provide a number of important constraints in the nature of dark matter and galaxy formation on the smallest non-linear scales. In this talk I will review some recent developments and what these may be telling us about our current cosmological model.  
April 2, 2016 Robert Allen - UCR TBD TBD  
March 12, 2015 Javad Shabani - California Nano Systems Institute, UCSB InAs heterostructures with superconducting contacts It has been recently realized that materials with strong spin orbit coupling can lead to novel states of matter such as topological insulators and superconductors. This exciting development might lead to a number of useful applications ranging from spintronics to quantum computing. In particular, theory predicts that narrow band gap semiconductors with strong spin-obit coupling are a suitable platform for the realization of Majorana zero-energy modes, predicted to obey exotic non-Abelian braiding statistics. In this talk, we demonstrate the first realization of gate-defined wires where one-dimensional confinement is created using electrostatic potentials, on large area InAs two-dimensional electron systems (2DESs). The electronic properties of the parent 2DES are fully characterized in the region that wires are formed. This allows us to quantitatively compare the effect of disorder in gate- and etched-defined wires. We show that this scheme together with epitaxial growth of superconducting thin film on InAs heterostructures could provide new prospective solutions for scalable and complex wire networks.  
February 26, 2015 Victor Brar - Caltech Surface Plasmons and Impurity States in Graphene Graphene, an atomically thin sheet of carbon atoms, provides a unique platform to study quasiparticle interactions and to create optical metamaterials with novel properties. The 2D nature and linear band structure of graphene give rise to a semi-metal behavior, with tunable dielectric properties and a high electron mobility. In the DC regime, these properties allow graphene to display novel screening behavior in the presence of charged impurities, which I will show can be probed directly using scanning tunneling spectroscopy (STM). At optical (mid-IR) frequencies, the graphene dielectric function is strongly perturbed by the presence of collective excitations known as surface plasmon polaritons (SPPs), which are optical modes - supported by free carriers - that are bound to the graphene sheet. These modes show a number of remarkable properties, including a carrier density dependent dispersion relation, and wavelengths that are more than 100 times shorter than freespace. I will show how the surface plasmons in graphene can be harnessed to create infrared metasurfaces that have tunable optical properties. These materials will be shown to exhibit extreme light-matter interactions that can control the macroscopic absorption and emission properties of nanostructured dielectric stacks.  
February 19, 2015 Frank Wuerthwein - UCSD The Quest for Dark Matter at the LHC - A Supersymmetric perspective from CMS After the discovery of the Higgs Boson in Run 1 of the LHC, the new “holy grail” of collider physics is to be able to produce and study dark matter in the laboratory. In this talk, we will address the following questions: - Why do we think dark matter exists ? - How do we find & understand Dark Matter at the Large Hadron Collider (LHC) ? - Where are we now with the search ? - Where are we going within the next 20 years?  
February 12, 2015 Thorsten Emig - MIT TBA TBA  
January 29, 2015 Briaqn Keating - UCSD The Twisted Universe: The discovery of B-mode polarization The era of Cosmic Microwave Background B-mode polarization cosmology began in March 2014 with two landmark papers released within a week of each other. The BICEP2 telescope observed from the South Pole for three seasons (2010–2012) and released results showing an excess of B-modes in the degree angular scale range with >5 sigma significance. We find that this excess could not be explained by instrumental systematics and it was confirmed in cross-correlation with BICEP1 (at 100 and 150 GHz) and preliminary data from the Keck Array. The observed B-mode power spectrum was well-fit by a lensed-LCDM cosmological model with the addition of primordial tensor fluctuations. However, it is impossible to rule out foreground contamination and we are working alongside the Planck team to resolve this matter. I will discuss the BICEP2 experiment, observations, and data analysis. One week before the BICEP2 announcement, the POLARBEAR telescope (which observed from the Atacama Desert, Chile for one season 2012-2013) announced the first evidence for B-modes at sub-degree scales caused by gravitational lensing of the CMB’s E-modes by large scale structure at low-redshift. The combination of the BICEP2 and POLARBEAR results paves the way towards precision tests of inflation, foreground contamination as well as probes of other aspects of fundamental physics including measuring the number and masses of cosmological neutrinos.  
January 15, 2015 Jun Ye - JILA, National Institute of Standards and Technology and U Colorado Making the world’s best atomic clock The relentless pursuit of spectroscopy resolution has been a key drive for many scientific and technological breakthroughs over the past century, including the invention of laser and the creation of ultracold matter. State-of-the-art lasers now maintain optical phase coherence over many seconds and provide this piercing resolution across the entire visible spectrum. The new capability in control of light has enabled us to create and probe novel quantum matter via manipulation of dilute atomic and molecular gases at ultralow temperatures. For the first time, we control the quantum states of more than 1000 atoms so precisely that we achieve a more stable and accurate atomic clock than any existing atomic clocks, with both key ingredients for a clock reaching the 10-18 level. We are also on the verge of integrating novel many-body quantum states into the frontiers of precision metrology, ready to advance measurement precision beyond the standard quantum limit. Such advanced clocks will allow us to test the fundamental laws of nature and find applications among a wide range of technological frontiers.  

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