Past Events

  • HET & HEE Joint Seminar: (TBA)

    Center for Particle Cosmology

    Josh Ruderman (NYU)

  • High Energy Theory Seminar: “Cosmology of a Fine-Tuned SUSY Higgs”

    David Rittenhouse Laboratory, 2N36

    Matthew Reece (Harvard)

    I will discuss some work in progress that explores whether a mildly fine-tuned Higgs boson, as in (mini-)split supersymmetry, can have interesting or observable cosmological consequences. As moduli fields oscillate, the Higgs can respond and perhaps acquire very large values along a D-flat direction. Possible consequences involve a burst of gravitational wave production and an altered estimate of the number of e-folds of inflation.

  • Condensed Matter Seminar: "Striped Ground States in the Hubbard Model"

    David Rittenhouse Laboratory, A4

    Steven White (University of California, Irvine)

    Solving the 2D Hubbard model is one of the most well-known outstanding problems in theoretical condensed matter physics. Various simulation techniques, such has DMRG and quantum Monte Carlo, have made dramatic strides in recent years, but they have still not provided clearcut answers for the nature of the ground state of the strong-coupling doped model.

  • High Energy Theory Seminar: "BMS Invariant Fluids"

    David Rittenhouse Laboratory, 2N36

    Robert Penna (Columbia University)

    The Bondi-van der Burg-Metzner-Sachs (BMS) group is the asymptotic symmetry group of asymptotically flat spacetime.  It is related to flat gravity in the same way that the conformal group is related to anti de Sitter gravity.  However, while the conformal group is well known throughout field theory, the BMS group is rather mysterious.  We show that the BMS group is closely related to infinite dimensional symmetry groups governing fluid dynamics.  We use a relationship between gravitating systems and lower dimensional fluids on their boundaries to give a new derivation of

  • High Energy Theory Seminar: "Entanglement at a Scale and Recovery Maps"

    David Rittenhouse Laboratory, 2N36

    Nima Lashkari (MIT)

    I discuss the amount of information in quantum field theory states reduced to a region, that cannot be recovered from its subregion density matrices. One can reconstruct the density matrix from its subregions using recovery maps. The vacuum of a conformal field theory is a quantum Markov state and the fixed point of both transformations. I define the entanglement of scaling as a measure of entanglement at a scale, and mention connections with C-theorems proofs in 2, 3 and 4 dimensions.

  • Astro Seminar:"Probes of Primordial Black Hole Dark Matter"

    David Rittenhouse Laboratory, A4

    Ely Kovetz (Johns Hopkins)

    The LIGO observatory has reported several detections of gravitational waves from the coalescence of binary black holes. We consider the extraordinary possibility that the detected events involving heavier masses are mergers of primordial black holes making up the dark matter in the Universe.

  • 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.