These are a few of the seminars I have given over the past few years.

This talk argues that accidental approximate scaling symmetries are robust predictions of weakly coupled string vacua, and shows that their interplay with supersymmetry and other (generalised) internal symmetries underlies the ubiquitous appearance of no-scale supergravities in low-energy 4D EFTs. The talk goes on to identify four nested types of no-scale supergravities, and shows how leading quantum corrections can break scale invariance while preserving some no-scale properties (including non-supersymmetric flat directions). These ideas are used to classify corrections to the low-energy 4D supergravity action in perturbative 10D string vacua, including both bulk and brane contributions, leading to prediction for the Kahler potential at any fixed order in alpha’ and string loops that agree with all extant calculations. p-form fields play two important roles: they spawn many (generalised) shift symmetries; and space-filling 4-forms teach 4D physics about higher-dimensional phenomena like flux quantization. These robust symmetry arguments suffice to understand obstructions to finding classical de Sitter vacua, and suggest how to get around them in UV complete models.**Scaling the Landscape: Robust EFT Implications from UV Physics**

[See here for an online version of this talk given in Quantum Aspects of Spacetime & Matter, Max Planck Institute for Gravitational Physics, Potsdam, July 2020]

**From Wilson to Lindblad: Late-time Obstacles to Reliable Calculations with Horizons (and how Open EFTs can help)**Quantum systems in gravitational fields (particularly with horizons) are often plagued by paradoxical predictions at very late times. Examples include predictions for information loss in black holes and for properties of eternal inflation. This talk argues that generic problems exist making such predictions because perturbative methods generically fail at very late times. Similar issues arise in other areas of physics (like optics) and the tools there also work in a gravitational context. The talk describes a simple illustrative application of these tools to a qubit in Rindler space (ie an Unruh observer), and to a qubit in an inflationary (de Sitter) universe. The tools are shown to correct earlier results by Candelas and Sciama and show in detail how, when and why these techniques work.

[See here for an online version of this talk given to the particle physics group at Yale University, November 2020]

**The Future is Stochastic (Probably)**Precision calculations in de Sitter space (such as of inflationary predictions for primordial fluctuations) are often plagued by infrared problems and issues of secular time dependence. Similar issues about the breakdown of perturbation theory seem also to arise for information loss in black holes. This talk briefly summarizes how similar problems can arise in other areas of physics, and how they are dealt with when they do. It is argued that Master-Equation techniques used in areas like optics also apply to cosmology (and possibly black holes) and can tell us how to extract reliably late-time predictions. Applied to inflation they lead to Starobinsky’s stochastic methods (plus small but important corrections). This is argued to provide an explanation for why stochastic inflation seems to resum IR effects in simple examples, and allows these tools to be generalized to apply more broadly. I mention in passing the relevance of these tools to the problem of Schrodinger’s Cosmologist: how primordial fluctuations decohere sometime between their production during inflation and their observation early in the present Big Bang Epoch.

**Effective Field Theorie****s for Point Sources**This talk applies effective field theory to the back-reaction of sources with finite size but infinite mass. The main tool for calculating back-reaction is a general relation between a source’s effective action and the boundary conditions of `bulk’ fields in the near-source limit. As applied to the Maxwell (or Einstein) fields for point sources this boundary condition reproduces standard Gauss’ Law expressions, but the same arguments imply source-dependent boundary conditions for the Schrodinger (or Dirac) field of an orbiting particle. As applied to the quantum mechanics of a particle interacting with a source through an inverse-square potential EFTs remove the guess-work from the (well-known) ambiguities in the determination of boundary conditions at the origin, and provides a simple interpretation of the classical renormalization effects that are known to arise in this case. EFT arguments show why the RG evolution associated with this classical renormalization is likely universal for a great many types of point sources. The EFT boundary conditions also modify how finite-size effects alter bound-state orbits in the Coulomb problem, and in particular (for spinless particles) give them a non-standard dependence on the mass of the orbiting particle. Although they do not solve the `proton-radius puzzle’, these techniques provide a systematic few-parameter way to fit the effects of finite-size sources at the kHz level, as is required to extract precision tests of QED in such experiments.

**Acceleration, Then and Now**There is good evidence that the universe underwent an epoch of accelerated expansion sometime in its very early history, and that it is entering a similar phase now. The ‘Then’ part of this talk describes how the predictions of theories suggested by quantum gravity (specifically string theory) for the early epoch have fared when compared with recently announced observations from the Planck satellite. Although it is too early for these predictions to be regarded as being comprehensive, I argue that a survey of those that were made shows they broadly agree with what was seen.The talk’s second part (‘Now’) provides an update on an approach to solving the “cosmological constant problem”, which is a theoretical obstruction that makes it difficult to understand the origins of the present epoch of acceleration. (In a nutshell: observations agree well with what would be expected if the universe were now beginning to be dominated by the energy density of the vacuum, but the vacuum energy density required by observations is extremely tiny compared with all known calculations of its expected size.) In the approach described – Supersymmetric Large Extra Dimensions, or SLED – observations can be reconciled with a large vacuum energy because the energy curves the extra dimensions and not the ones we measure in cosmology. The update shows that various quantum effects did not ruin this picture, and the main remaining worry to to verify that the theory’s predictions do not alter the way other things gravitate in an observationally unacceptable way.

**Good Things from the Back-reaction of Higher Codimension Branes**Randall-Sundrum models are examples of co-dimension one braneworlds for which back-reaction plays an important role, with the warping produced by the branes changing the nature of the low-energy effective theory in an important way. Yet back-reaction for higher-codimension branes remains much less well-explored. In particular, the fields sourced by higher co-dimension objects generically diverge at the positions of the sources, complicating the calculation of the properties of the bulk from those of the sources. This talk describes a solution to this matching problem for codimension-two branes, and uses the result to show how back-reacting codimension-two systems can have surprising properties – such as by providing de Sitter solutions to higher-dimensional supergravity (despite the existence of various no-go theorems), naturally exponentially large dimensions (as could be useful for the hierarchy problem), and volume-suppressed on-brane curvatures compared with the typical scale of on-brane physics (as could be useful for the cosmological constant problem).

**Effective Field Theory/Modified Gravity: The View from Below**We live at a time of contradictory messages about how successfully we understand gravity. General Relativity seems to work very well in the Earth’s immediate neighbourhood, but arguments abound that it needs modification at very small and/or very large distances. This talk tries to put this discussion into the broader context of similar situations in other areas of physics, and summarizes some of the lessons which our good understanding of gravity in the solar system has for proponents for its modification over very long and very short distances. The main message is that effective theories (in the technical sense of effective) provide the natural (and arguably only known) precise language for framing proposals. Its framework is also useful, inasmuch as it makes some modifications seem more plausible than others, though there are also some surprises.

**Extra Dimensions, the Cosmological Constant Problem and the LHC**Two uncertainties define the prevailing attitude toward the LHC: uncertainty about what new physics it may find (if any); and disappointment with the prospects of finding just a “vanilla” standard-model Higgs. These are wrapped in dissatisfaction with the “technical naturalness” arguments which (when applied to the hierarchy problem) help suggest what we should be looking for. The dissatisfaction arises because of a wide-spread despair about finding a technically natural solution to the cosmological constant problem, despite much effort spent seeking it. In this talk I describe a mechanism within supersymmetric extra-dimensional theories that allows the low-energy effective cosmological constant naturally to be of order the Kaluza-Klein scale. If this is the solution to the cosmological constant problem, then it requires extra dimensions that are both very supersymmetric and large enough to be relevant to the LHC. For the LHC it implies in particular two hard predictions, and two (so-far successful) general expectations. The predictions are (1) many missing energy channels, with a gravity scale at or just above 10 TeV; and (2) the existence of string excitations of standard-model particles, likely *below* 10 TeV. The (so far – successful) general expectations are that no MSSM particles exist to be discovered, despite the low-energy supersymmetry; and (2) the Higgs is likely to be vanilla.

**AdS/QHE: Towards a Holographic Description of Quantum Hall Experiments**Many experimental features of Quantum Hall systems seem to be well-described by the phenomenological assumption that the dynamics of the charge carriers enjoys a large duality symmetry group: a level-two subgroup of SL(2,Z) acting on the Hall and Ohmic conductivities. What has been missing is an understanding of how this symmetry might emerge from the underlying properties of the electrons, or from any other kind of strongly interacting system. After describing the experimental evidence for the symmetry, this talk describes a first step towards a theoretical understanding by showing how the required symmetry emerges naturally from an AdS/CFT description of 2+1 dimensional charge carriers. This suggests that AdS/CFT techniques may provide a natural language for describing Quantum Hall systems.

**Colourful Things the LHC Might See Early**It is widely believed that existing electroweak data requires a Standard Model (SM) Higgs to be light, while electroweak and flavour physics constraints require other scalars charged under the SM gauge couplings to be heavy. New Higgs-like scalars that are also colour octets – well-motivated in the sense that they arise in models having approximate custodial symmetry and minimal flavour violation – provide counter-examples to both of these statements since the scalars can be all simultaneously light (~ 100 GeV} or heavy (~ 1 TeV}, without running afoul of direct searches and electroweak precision measurements.

**Are Inflationary Predictions Sensitive to Very High Energy Physics?**It has been proposed that the successful inflationary description of density perturbations on cosmological scales is sensitive to the details of physics at extremely high (trans-Planckian) energies. I will critically analyse this idea by examining how inflationary predictions depend on higher-energy scales within a simple model where the higher-energy physics is well understood. The result is the best of all possible worlds: inflationary predictions are robust against the vast majority of high-energy effects, but *can* be sensitive to some effects in certain circumstances, in a way which does not violate ordinary notions of decoupling. This implies both that the comparison of inflationary predictions with CMB data is meaningful, and that it is also worth searching for small deviations from the standard results in the hopes of learning about very high energies.

**String/Brane Cosmology**String theory is our best candidate for a theory of the physics at very short distances, but is very much a theory in search of an observable application. Conversely, scalar field theories can successfully describe the phenomenology of inflation or dark energy, but have proven difficult to embed into a realistic theory of short distances. However, the branes arising in string theory can have strong implications for the naturalness problems which obstruct this embedding. This is interesting in itself, since short distance physics (like string theory) normally decouples from long-distance phenomena (like cosmology). But can cosmology and string theory help answer each other’s problems? This talk describes recent progress in bringing these ideas together.