Sommerfeld Theory Colloquium (ASC)

Sommerfeld Theory Colloquium (ASC)

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Sommerfeld Theory Colloquium (ASC) episodes

  • Topological Superconductivity and Unconventional pairing in Oxide Interfaces
    Sommerfeld Theory Colloquium, To pinpoint the microscopic mechanism for superconductivity has
    proven to be one of the most outstanding challenges in the physics of
    correlated quantum matter. Thus far, the most direct evidence for
    an electronic pairing mechanism is the observation of a new symmetry
    of the order-parameter, as done in the cuprate high-temperature
    superconductors. Like distinctions based on the symmetry of a locally
    defi�ned order-parameter, global, topological invariants allow for
    a sharp discrimination between states of matter that cannot be transformed
    into each other adiabatically. Here we propose an unconventional
    pairing state for the electron
    uid in two-dimensional oxide
    interfaces and establish a direct link to the emergence of nontrivial
    topological invariants. Topological superconductivity and Majorana edge states can then be used to detect the microscopic origin for
    superconductivity. In addition, we show that also the density wave
    states that compete with superconductivity sensitively depend on the
    nature of the pairing interaction. Our conclusion is based on the special
    role played by the spin-orbit coupling and the shape of the Fermi
    surface in SrTiO3/LaAlO3-interfaces and closely related systems.
    1 hr
  • Cosmology with Type Ia Supernovae: where do we stand today?
    Sommerfeld Theory Colloquium, The role of Type Ia supernovae in observational cosmology has evolved
    from being ”avant-garde” in the early 1990’s until today’s mature status of precision cosmology. Several large transient surveys have been detecting supernovae routinely, near and far, with the aim of probing what is causing the accelerated expansion of the Universe.
    With time, the focus has changed towards addressing the intricacies of astrophysical effects that could bias the fits of cosmological parameters,
    most notably the nature of dark energy. In this talk, aimed at high-energy physics theorists(!), I will try to convey the status of
    the field, high-lighting some progress and set-backs, based on studies
    of the closest Type Ia SN in modern time that exploded in the
    beginning of 2014 in the near-by galaxy M82.
    1 hr 6 min
  • Lattice gauge theory insights
    Sommerfeld Theory Colloquium, Various aspects of lattice gauge theory will be briefly discussed including, general principles, sources of systematic errors, dynamical fermions, QCD phenomenology, the FLAG project and, if time allows, some applications of lattice theory to other non-perturbative BSM phenomena.
    1 hr 12 min
  • Searching for New Forces Using Torsion Pendula
    Sommerfeld Theory Colloquium, Equivalence principle violation, deviations from the inverse-square
    law of gravity, and long-range interactions between particle spins
    o�er powerful tests of beyond-the-standard-model physics. Using a
    torsion pendulum, a technique that dates to the 18th century, is still
    the most sensitive way to search for these signatures of new physics.
    I will talk about how the experiments are done and give an update on the current and future status of such torsion balance experiments in the Eot-Wash group.
    57 min
  • A Closer Look at Black Holes
    Sommerfeld Theory Colloquium, Several new techniques are currently being employed to probe the strong gravitational fi�eld in the vicinity of black holes. Long baselineinterferometry at sub-millimeter wavelengths sets constraints on the
    silhouette of the black holes in the Galactic center (SgrA*) and M87.
    Stars which get tidally disrupted as they orbit too close to a single
    black hole are being discovered at cosmological distances. Electromagnetic counterparts of black hole binaries in galaxy mergers are being identifi�ed, and can be used to calibrate the rate of gravitational wave sources. Most interestingly, the recoil induced by the
    anisotropic emission of gravitational waves in the �nal plunge of binaries leaves unusual imprints on their host galaxies. Finally, the
    lecture will describe new constraints on the contribution of primordial black holes to the dark matter.
    1 hr 2 min
  • Higher-Spin Gravity and Higher Spin Black Holes in Three Dimensions
    Sommerfeld Theory Colloquium, Three-dimensional Einstein gravity has no local dynamical degree of
    freedom. Yet, it is far from being trivial when the cosmological constant is negative. (i) It admits black hole solutions. (ii) It easily allows for consistently interacting and tractable higher-spin extensions.
    (iii) It possesses remarkable asymptotic properties at infi�nity where
    an infi�nite-dimensional symmetry algebra emerges. These features
    make three-dimensional gravity a perfect "theoretical laboratory" in which to explore the conceptual issues related to (i), (ii) and (iii) in
    a simpler context. The talk will not only discuss three-dimensional
    gravity assuming no previous knowledge on the subject, but will also
    provide access to recent work where new results on points (i), (ii)
    and (iii) are developed.
    1 hr 16 min
  • Harmony of Scattering Amplitudes and Form Factors
    Sommerfeld Theory Colloquium, In this seminar I will describe some of the hidden structures recently
    discovered in the scattering amplitudes of elementary particles, such
    as those measured at the Large Hadron Collider. These structures are
    responsible for the mysterious simplicity of these quantities, which is
    completely obscured by a calculation based on textbook techniques
    such as Feynman diagrams. I will then move on to discuss form factors. These are slightly off-shell quantities and, similarly to amplitudes,
    are also much simpler than what expected based on conventional
    approaches. In particular I will focus on form factors of particular (half-BPS) operators in a special theory, known as N=4 super Yang-Mills, and briefly discuss some unexpected connections
    to scattering amplitudes in phenomenologically relevant theories.
    1 hr 17 min
  • Cascade of phase transitions near Quantum Critical Point
    Sommerfeld Theory Colloquium, In the standard picture of a quantum phase transition, a single quantum critical point separates the phases at zero temperature. Here
    we show that the two-dimensional case is considerably more complex. Instead of the single point separating the antiferromagnet from
    the normal metal, we have discovered a broad region between these two phases where the magnetic order is destroyed but certain areas of the Fermi surface are closed by a large gap. This gap reflects the formation of a novel quantum state characterized by a superposition of d-wave superconductivity and a quadrupole density wave
    (QDW), which builds a checkerboard pattern with a period incommensurate with that of the original spin density wave. At moderate temperatures both orders co-exist over comparatively large distances but thermal fluctuations destroy the long-range order. Below
    a critical temperature the
    fluctuations are less essential and super-
    conductivity becomes stable. Applying a magnetic field destroys the superconductivity but establishes QDW. In addition to these phases
    we obtain also a charge density wave (CDW) arising as a result of interaction of electrons with superconducting fluctuations. This phase
    is possible when the superconductivity is destroyed by either thermal fluctuations or a magnetic field. The results of our theory can serve as explanation of recent experiments on cuprates performed with the help of STM, NMR, hard and resonant soft X-ray scattering, sound
    propagation, and other techniques.
    1 hr 9 min
  • Einstein and Quantum Mechanics: It's Not What You Think
    Sommerfeld Theory Colloquium, Einstein is well known for his rejection of quantum mechanics in the form it emerged from the work of Heisenberg, Born and Schrodinger in 1926. Much less appreciated are the many seminal contributions
    he made to quantum theory prior to his �final scientifi�c verdict, that
    the theory was at best incomplete. In this talk I present an overview
    of Einsteins many conceptual breakthroughs and place them in historical context. I argue that Einstein, much more than Planck, introduced the concept of quantization of energy in atomic mechanics.
    Einstein proposed the photon, the fi�rst force-carrying particle discovered for a fundamental interaction, and put forward the notion of wave-particle duality, based on sound statistical arguments 14 years before De Broglies work. He was the fi�rst to recognize the intrinsic
    randomness in atomic processes, and introduced the notion of transition probabilities, embodied in the A and B coeffi�cients for atomic emission and absorption. He also preceded Born in suggesting the interpretation of wave fi�elds as probability densities for particles, photons, in the case of the electromagnetic �field. Finally, stimulated by
    Bose, he introduced the notion of indistinguishable particles in the
    quantum sense and derived the condensed phase of bosons, which is
    one of the fundamental states of matter at low temperatures. His
    work on quantum statistics in turn directly stimulated Schrodinger
    towards his discovery of the wave equation of quantum mechanics. It
    was only due to his rejection of the �final theory that he is not generally recognized as the most central �figure in this historic achievement
    of human civilization.
    1 hr 20 min

About Sommerfeld Theory Colloquium (ASC)

From the publisher's feed

The Arnold Sommerfeld Center for Theoretical Physics organizes regular colloquia about topics of current interest in the field of theoretical physics.

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