Forthcoming events in this series
Axion Cosmology
Abstract
Axions are ubiquitous in string theory compactifications. They are
pseudo goldstone bosons and can be extremely light, contributing to
the dark sector energy density in the present-day universe. The
mass defines a characteristic length scale. For 1e-33 eV<m< 1e-20
eV this length scale is cosmological and axions display novel
effects in observables. The magnitude of these effects is set by
the axion relic density. The axion relic density and initial
perturbations are established in the early universe before, during,
or after inflation (or indeed independently from it). Constraints
on these phenomena can probe physics at or beyond the GUT scale. I
will present multiple probes as constraints of axions: the Planck
temperature power spectrum, the WiggleZ galaxy redshift survey,
Hubble ultra deep field, the epoch of reionisation as measured by
cmb polarisation, cmb b-modes and primordial gravitational waves,
and the density profiles of dwarf spheroidal galaxies. Together
these probe the entire 13 orders of magnitude in axion mass where
axions are distinct from CDM in cosmology, and make non-trivial
statements about inflation and axions in the string landscape. The
observations hint that axions in the range 1e-22 eV<m<1e-20 eV may
play an interesting role in structure formation, and evidence for
this could be found in the future surveys AdvACT (2015), JWST, and
Euclid (>2020). If inflationary B-modes are observed, a wide range
of axion models including the anthropic window QCD axion are
excluded unless the theory of inflation is modified. I will also
comment briefly on direct detection of QCD axions.
A geometric interpretation of algebraic quantum mechanics
Abstract
We treat the problem of geometric interpretation of the formalism
of algebraic quantum mechanics as a special case of the general problem of
extending classical 'algebra - geometry' dualities (such as the
Gel'fand-Naimark theorem) to non-commutative setting.
I will report on some progress in establishing such dualities. In
particular, it leads to a theory of approximate representations of Weyl
algebras
in finite dimensional "Hilbert spaces". Some calculations based on this
theory will be discussed.
Symmetries, K-theory, and the Bott periodicity of topological phases
Abstract
Topological phases of matter exhibit Bott-like periodicity with respect to
time-reversal, charge conjugation, and spatial dimension. I will explain how
the non-commutative topology in topological phases originates very generally
from symmetry data, and how operator K-theory provides a powerful and
natural framework for studying them.
Gravity as (gauge theory)^2: from amplitudes to black holes
Abstract
We will discuss the relation between perturbative gauge theory and
perturbative gravity, and look at how this relation extends to some exact
classical solutions. First, we will review the double copy prescription that
takes gauge theory amplitudes into gravity amplitudes, which has been
crucial to progress in perturbative studies of supergravity. Then, we will
see how the relation between the two theories can be made manifest when we
restrict to the self-dual sector, in four dimensions. A key role is played
by a kinematic algebraic structure mirroring the colour structure, which can
be extended from the self-dual sector to the full theory, in any number of
dimensions. Finally, we will see how these ideas can be applied also to some
exact classical solutions, namely black holes and plane waves. This leads to
a relation of the type Schwarzschild as (Coulomb charge)^2.
Matrix geometries
Abstract
The talk will give a definition of matrix geometries, which are
particular types of finite real spectral triple that are useful for
approximating manifolds. Examples include fuzzy spheres and also the
internal space of the standard model. If time permits, the relation of
matrix geometries with 2d state sum models will also be sketched.
Operator Expansion Algebras
Abstract
Quantum field theory (QFT) originated in physics in the context of
elementary particles. Although, over the years, surprising and profound
connections to very diverse branches of mathematics have been discovered,
QFT does not have, as yet, found a universally accepted "standard"
mathematical formulation. In this talk, I shall outline an approach to QFT
that emphasizes its underlying algebraic structure. Concretely, this is
represented by a concept called "Operator Product Expansion". I explain the
properties of such expansions, how they can be constructed in concrete QFT
models, and the emergent relationship between "perturbation theory" on the
physics side and
"Hochschild cohomology" on the physics side. This talk is based on joint
work
with Ch. Kopper and J. Holland from Ecole Polytechnique, Paris.
The inflationary origin of the seeds of cosmic structure: quantum theory and the need for novel physics
Abstract
The observations of the first traces of cosmic structure in the
Cosmic Microwave Background are in excellent agreement with the
predictions of Inflation. However as we shall see, that account
is not fully satisfactory, as it does not address the transition
from an homogeneous and isotropic early stage to a latter one
lacking those symmetries. We will argue that new physics along the
lines of the dynamical quantum state reduction theories is needed
to account for such transition and, motivated by Penrose's ideas
suggest that quantum gravity might be the place from where
this new physics emerges. Moreover we will show that observations
can be used to constrain the various phenomenological proposals
made in this regard.
Forest formula for Epstein-Glaser renormalization: new results and perspectives
Gravity induced by noncommutative spacetime
Abstract
The talk is based on my paper with E. Beggs appearing in Class. Quantum
Gravity.
Working within a bimodule approach to noncommutative geometry, we show that
even a small amount of noncommutativity drastically constrains the moduli
space of
noncommutative metrics. In particular, the algebra [x,t]=x is forced to have
a geometry
corresponding to a gravitational source at x=0 so strong that even light
cannot
escape. This provides a non-trivial example of noncommutative Riemannian
geometry
and also serves as an introduction to some general results.
Almost Calabi-Yau algebras associated to SU(3) modular invariants
Abstract
The modular invariant partition functions for SU(2) and SU(3)
conformal field theories have been classified. The SU(2) theory is closely
related to the preprojective algebras of Coxeter-Dynkin quivers. The
analogous finite dimensional superpotential algebras, which we call almost
Calabi-Yau algebras, associated to the SU(3) invariants will be discussed.
Manifestation of Quantum Field Nonlocality in a Toy Quantum Optical Configuration
Quantum information processing in spacetime
Abstract
Cutting-edge experiments in quantum communications are reaching regimes
where relativistic effects can no longer be neglected. For example, there
are advanced plans to use satellites to implement teleportation and quantum
cryptographic protocols. Relativistic effects can be expected at these
regimes: the Global Positioning System (GPS), which is a system of
satellites that is used for time dissemination and navigation, requires
relativistic corrections to determine time and positions accurately.
Therefore, it is timely to understand what are the effects of gravity and
motion on entanglement and other quantum properties exploited in quantum
information.
In this talk I will show that entanglement can be created or degraded by
gravity and non-uniform motion. While relativistic effects can degrade the
efficiency of teleportation between moving observers, the effects can also
be exploited in quantum information. I will show that the relativistic
motion of a quantum system can be used to perform quantum gates. Our
results, which will inform future space-based experiments, can be
demonstrated in table-top experiments using superconducting circuits.