Past Events

  • Condensed Matter Seminar: "Tuning Quantum Materials with Uniaxial Strain"

    David Rittenhouse Laboratory, A4

    Abhay Narayan Pasupathy (Columbia University)

    What is the effect of stretching a crystal along a given direction by a small amount? In general, one might not expect much: a change in lattice constant, accompanied by corresponding changes in the electronic and vibrational properties of a crystal. I will describe a few cases of materials where the effect of stretching (ie, uniaxial strain) lead to large and unexpected effects.

  • HET & HEE Joint Seminar: "Composite Higgses"

    Center for Particle Cosmology

    Csaba Csaki (Cornell University)

  • High Energy Theory Seminar: "What Can Cosmology Tell Us About Gravity?"

    David Rittenhouse Laboratory, 2N36

    Levon Pogosian (Simon Fraser University)

    I will review the current status and future prospects of testing theories of gravity using data from large-scale structure surveys. I will then discuss certain aspects of the so-called model-independent tests of dark energy and modified gravity. One is the choice of priors when trying to constrain unknown functions of redshift. Another is the physical interpretation of such tests and their implications for particular types of modified gravity theories.

  • High Energy Theory Seminar: "Spinning Cosmology"

    David Rittenhouse Laboratory, 2N36

    Andrei Khmelnitsky (ICTP)

    We study the signatures left by new light particles with a spin on the primordial cosmological fluctuations. In distinction from the pure de Sitter background, where fields with spin have to be massive enough to satisfy the Higuchi bound, the inflation allows to host spinning particles that are parametrically lighter than the expansion rate. I introduce the description of the particles with spin in the context of the Effective Field Theory of Inflation and discuss the main signatures left by such particles on the primordial fluctuations.

  • Condensed Matter Seminar: "A change in stripes for cholesteric shells via anchoring in moderation"

    David Rittenhouse Laboratory, A4

    Lisa Tran (University of Pennsylvania)

    Chirality, ubiquitous in complex biological systems, can be controlled and quantified in synthetic materials such as cholesteric liquid crystal (CLC) systems. In this work, we study spherical shells of CLC under weak anchoring conditions. We induce anchoring transitions at the inner and outer boundaries using two independent methods: by changing the surfactant concentration or by raising the temperature close to the clearing point.

  • High Energy Theory Seminar: "Equivalence Principle in Scalar-tensor Theories"

    David Rittenhouse Laboratory, 2N36

    Lasma Alberte (ICTP)

    We study the question of whether the equivalence principle holds for extended objects moving on cosmological backgrounds in modified gravity theories. We do so within the framework of effective field theory of dark energy focusing in particular on the subclass corresponding to the Horndeski theories. These are the most general second order scalar-tensor theories with non-linear derivative self-interactions allowing the Vainshtein screening mechanism to operate on small scales.

  • Condensed Matter Seminar: "The Structure and Function of Organic-Inorganic Hybrid Perovskites"

    David Rittenhouse Laboratory, A4

    Cherie Kagan (University of Pennsylvania)

    Organic-inorganic hybrid perovskites represent a class of materials composed of corner sharing metal halide octahedra charge balanced by organic cations. The hybrid perovskites may be tailored in their composition and in their dimensionality. Research exploring hybrid perovskites skyrocketed in the past few years because of the remarkable, >20% power conversion efficiency demonstrated for the three-dimensional (3D) lead halide structures in solar cells, which currently rivals that of commercial silicon-based solar cells.

  • Astro Seminar: "Stellar Spin-orbit Misalignment"

    David Rittenhouse Laboratory, A4

    Joshua Winn (Princeton)

    In the Solar system, the planets follow orbits that are aligned with the Sun’s equatorial plane to within a few degrees.  But what about planets around other stars?  Many techniques are now available to measure the obliquities of planet-hosting stars, ranging from an effect predicted in the 19th century to several techniques relying on data from the Kepler space telescope.  Many exoplanetary systems show good alignment, as in the Solar system. We have also found planets on highly inclined orbits and even retrograde orbits.

  • High Energy Theory Seminar: "Topological Sectors, Supersymmetric Localization, and Holography"

    David Rittenhouse Laboratory, 2N36

    Silviu Pufu (Princeton University)

  • *Special* HET Seminar: "Many-body Localization: Breakdown of Thermalization in Quantum Matter"

    David Rittenhouse Laboratory, 4N12

    Arijeet Pal (Oxford)

    Until recently interacting many-particle systems governed by the laws of quantum mechanics were assumed to eventually reach thermal equilibrium, being described by equilibrium statistical physics. Rapid developments in theory and experiments in the last decade have established a phase of matter where this assumption is false, due to a phenomenon known as many-body localization (MBL). In this phase, the system undergoing unitary time dynamics retains the memory of the initial state in local observables for infinitely long times.