Sep 26 | Thu | UGRI-SURE students | SIAM-IMA Chapter Seminar | |||
13:30 | ||||||
LT5, Hicks | ||||||
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Sep 27 | Fri | UGRI-SURE students | SIAM-IMA Chapter Seminar | |||
13:30 | ||||||
LT5, Hicks | ||||||
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Oct 2 | Wed | Mariana Carrillo González (Imperial College London) | Cosmology, Relativity and Gravitation | |||
15:00 | Self-dual Cosmology | |||||
Hicks Seminar Room J11 | ||||||
Abstract: One of the simplest subsectors of gravitational physics in asymptotically flat spacetimes is the so-called self-dual sector. From a particle physics perspective, this subsector only contains three-point interactions between gravitons of (++—) helicities. This is equivalent to spacetimes with Riemann tensors equal to their Hodge dual. Hidden symmetries of gravitational physics, such as double copy relations that allow us to write gravity as the square of a gauge theory, are explicitly realized in these spacetimes. Additionally, this sector is related to infinite-dimensional algebras arising in celestial holography. In this talk, I will describe an extension of this sector to cosmological spacetimes. This can be seen as a time deformation of the flat space version and gives rise to time-deformed versions of the flat space symmetries. I will show how to build this description and showcase its hidden simplicity. I will also focus on two special cases with additional novel features, including self-dual radiation and self-dual coasting cosmologies. |
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Oct 3 | Thu | Nicolas Poirier (Univ. of Oslo, Rosseland Centre for Solar Physics, RoCS (NO)) | SP2RC/ESPOS seminar | |||
10:00 | Transverse oscillations in coronal loops and photospheric driving: combining high-resolution coronal and photospheric diagnostics together | |||||
Zoom | ||||||
Abstract: Sustained kink oscillations in coronal loops have long been observed in TRACE, SDO/AIA, and more recently in SolO/EUI images. Although their properties are quite well-known now, their driver and excitation mechanism remain under active debate. In this talk I will give an overview over the different ideas/theories that discuss the role of photospheric driving in the generation of kink oscillations. We exploited an unique dataset of high-resolution coronal and photospheric observations taken recently by SolO/EUI/HRI and the Swedish 1-m Solar Telescope (SST) respectively during a dedicated coordinated campaign run in October 2023. Using the SST/CRISP data we estimated and quantified the strength of photospheric driving at the footpoints of active region coronal loops, that include pore, plage, enhanced-network and sunspot regions. We then looked at kink oscillation signatures in the same coronal loops within the EUI/HRI coronal images. An attempt was then made to link the photospheric and coronal results together. I will finally discuss the implications of this work on the driving and excitation mechanism of kink oscillations, and future perspectives. |
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Oct 3 | Thu | Adrian Miranda (Manchester) | Topology Seminar | |||
16:00 | Tricategorical Universal Properties Via Enriched Homotopy Theory | |||||
Hicks Seminar Room J11 | ||||||
Abstract: When considering (co)limits of categories, one might ask for (co)cones to only commute up to natural isomorphism, or for universal properties to only hold up to equivalences of categories. In a general bicategory K such universal properties are modelled by the notion of a bicategorical (co)limit, where equations/relations are only ever imposed on data in the highest available dimension. However, these notions can also be modelled up to equivalence via ordinary (co)limits enriched over V= Cat, provided that one restricts their attention to weights that are well behaved with respect to the canonical monoidal model structure on V. In this talk I will explain how the above story adapts to the setting involving (co)limits *of* two-dimensional categories (or more generally, *in* three-dimensional categories). This involves homotopically well-behaved (co)limits enriched over the base V now given by Lack's monoidal model structure on the category of 2-categories and 2-functors. Running examples for motivation include Kleisli and Eilenberg-Moore constructions for pseudomonads, including for those on monoidal bicategories, as well as strictification constructions on bicategories and pseudo-double categories. This talk is based on my recent preprint. |
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Oct 3 | Thu | Reetika Joshi (Rosseland Centre for Solar Physics (Norway)) | Plasma Dynamics Group | |||
16:00 | Anemone Solar Jets: Breakthroughs from SST Observations and Numerical Simulations | |||||
online / Google Meet | ||||||
Abstract: Solar jets are collimated plasma flows that move along magnetic field lines and are accelerated at low altitudes following magnetic reconnection. Many of these jets originate from anemone-shaped low-lying arcades, and the most impulsive ones tend to be relatively broader, often showing untwisting motions. In this talk, I will present typical observational signatures in the lower atmosphere that correspond to the coronal evolution of these impulsive jets. In our study, we analyzed an observed solar jet associated with a circular flare ribbon using high-resolution observations from the SST, coordinated with IRIS and SDO. We specifically compared observed features with those predicted by a generic 3D line-tied numerical simulation of reconnection-driven jets, conducted using the ARMS code. Three key features were identified in the SST observations: the formation of a hook along the circular ribbon, the gradual widening of the jet through the apparent displacement of its kinked edge toward (rather than away from) the presumed reconnection site, and the falling back of some jet plasma towards a footpoint offset from that of the jet itself. These features, which emerged naturally in the 3D numerical simulation without prior assumptions, were interpreted in the context of the 3D geometry of asymmetric swirled-anemone loops and their reconnection sequences with surrounding coronal loops. Given the relatively simple conditions under which the observed jet occurred, and the generic nature of the simulation with minimal assumptions, we predict that the specific features we identified and interpreted are likely typical of all impulsive jets. |
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Oct 4 | Fri | Auriplex (https://www.kehubmaths.co.uk/triage-workshops/) | Maths Knowledge Exchange Hub Triage Workshops | |||
10:00 | Real-time sounds separation for healthcare (hearing) application project | |||||
https://newton.us21.list-manage.com/track/click?u=1f88d1ca28e2385959c2201f0&id=2147ee60de&e=cfdba87233 | ||||||
Abstract: Effective hearing ability influences individuals’ overall quality of life, particularly in situations (such as in workplaces, meetings, classrooms, social gatherings, or using audio devices) where unwanted noise constantly tests and challenges our hearing/audio processing capabilities. In these situations, all existing hearing aids share a common underlying concept flaw (due to the fixed position of the microphone, limited audio processing power and the lack of user interactivity), resulting in people with hearing loss withdrawing from these social/work group situations. Our objective is to disrupt the worldwide hearing market with the development of a portable smartphone-controlled next generation Interactive Audio Sensor Hub (IASH) & AI Sound Tool technology. This challenge requires innovative real-time sounds separation techniques to overcome latency issues. The aim is to improve audio separation in real time while minimising the use of hardware and maximising the use of software, so that developments can be incorporated into existing devices. |
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Oct 9 | Wed | Michael Magee (Durham University) | Pure Maths Colloquium | |||
14:00 | Convergence of unitary representations of discrete groups | |||||
Hicks Seminar Room J11 | ||||||
Abstract: Let $G$ be an infinite discrete group; e.g. hyperbolic $3$-manifold group. Finite dimensional unitary representations of G of fixed dimension are usually very hard to understand. However, there are interesting notions of convergence of such representations as the dimension tends to infinity. One notion — strong convergence — is of interest both from the point of view of $G$ alone but also through recently realized applications to spectral gaps of locally symmetric spaces. For example, this notion bypasses (unconditionally) the use of Selberg's Eigenvalue Conjecture in obtaining existence of large area hyperbolic surfaces with near-optimal spectral gaps. The talk is a broadly accessible discussion on these themes, based on joint works with W. Hide, L. Louder, D. Puder, J. Thomas. |
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Oct 9 | Wed | Tiziano Schiavone (GGI Firenze) | Cosmology, Relativity and Gravitation | |||
15:15 | An effective Hubble constant in f(R) modified gravity | |||||
Hicks Seminar Room J11 | ||||||
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Oct 9 | Wed | Jack Davidson (Sheffield) | ShEAF: postgraduate pure maths seminar | |||
16:00 | Algebraic K-Theory for Number Theorists | |||||
Hicks Seminar Room J11 | ||||||
Abstract: Algebraic K-theory is a powerful invariant of rings (and more generally of ring spectra) which contains information about topology, geometry and number theory. In this talk, we will outline the basics of the theory and survey some applications to number theory, in particular to the Kummer–Vandiver conjecture. We aim to motivate why number theorists should care about an a priori homotopy theoretic notion. (Note: if you ask me questions about number theory I will forcefully eject you from J11). |
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Oct 10 | Thu | James Cranch (Sheffield) | Topology Seminar | |||
16:00 | ||||||
Hicks Seminar Room J11 | ||||||
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Oct 11 | Fri | Julia Schneider (Sheffield) | Algebraic Geometry Reading Seminar | |||
13:30 | Introduction to the Minimal Model Program and Sarkisov link factorisation | |||||
Hicks Seminar Room J11 | ||||||
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Oct 14 | Mon | Gong Show - 5 minutes talks | ||||
14:00 | ||||||
Hicks Seminar Room J11 | ||||||
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Oct 14 | Mon | Gong Show - 5 minutes talks | Algebraic Geometry Seminar | |||
15:00 | ||||||
Hicks Seminar Room J11 | ||||||
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Oct 14 | Mon | Gong Show - 5 minutes talks | Algebraic Geometry Seminar | |||
16:00 | ||||||
Hicks Seminar Room J11 | ||||||
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Oct 16 | Wed | Herbert Gangl (Durham University) | Pure Maths Colloquium | |||
14:00 | The beauty of Zagier's Polylogarithm Conjecture | |||||
Hicks Seminar Room J11 | ||||||
Abstract: Dirichlet related the residue at $s=1$ of the Dedekind zeta function of a number field $F$ (a slight generalisation of the famous Riemann zeta function) to two important arithmetical notions: the size of the ideal class group and the `volume' of the unit group in the number ring $O_F$ of $F$. Generalising this surprising connection, the special values of the Dedekind zeta function of a number field $F$ at integer argument n should, according to Zagier's Polylogarithm Conjecture, be expressed via a determinant of $F$-values of the $n$-th polylogarithm function. Goncharov laid out a vast program incorporating this conjecture using properties of multiple polylogarithms and the structure of a motivic Lie coalgebra. In this impressionist talk I intend to give a rough idea of the developments from the early days on, avoiding most of the technical bits, and also hint at a number of recent results for higher weight, some in joint work with, or developed by, S.Charlton, D.Radchenko as well as D.Rudenko and his collaborators. |
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Oct 16 | Wed | Suddhasattwa Brahma (Edinburgh) | Cosmology, Relativity and Gravitation | |||
15:15 | Nonlocal quantum effects in the Early Universe | |||||
Hicks Seminar Room J11 | ||||||
Abstract: Although inflation is widely regarded as the standard paradigm for the early universe, our understanding of its dynamics is necessarily incomplete. In this talk, I will treat inflation as an open quantum system and derive, in a systematic manner, quantum corrections to cosmological observables due to interactions with unobservable environments. For instance, the "cosmological horizon" is an example of a spacetime boundary that restricts our observable degrees of freedom while still allowing energy and information to flow across it into hidden sectors. Borrowing techniques from Quantum Information Theory, I will show how an Open Effective Field Theory formalism can incorporate non-unitary effects in cosmology and describe dissipation and decoherence of primordial fluctuations. I will emphasize that the out-of-equilibrium nature of gravitational systems necessarily result in non-Markovian dynamics and how this can lead to transient negative growth of entanglement entropy during inflation. |
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Oct 17 | Thu | Guillem Castelló i Barceló (Univ. of the Balearic Islands UIB, Solar Physics group (ES)) | SP2RC/ESPOS seminar | |||
10:00 | Spectral analysis of solar filaments using Convolutional-Neural Networks (CNNs) | |||||
Zoom | ||||||
Abstract: Solar filaments (also called prominences when seen off-disk) are solar atmospheric structures consisting of dense, cool plasma clouds floating within the sun's corona. Since the beginning of solar observations, it has been seen that the prominences oscillate with a wide variety of motions. These periodic motions are very common, but there are no systematic studies of these oscillations. It has recently been shown that spectral analysis of solar filaments is a powerful tool to identify oscillations in these structures. With this technique, the power spectral density (PSD) is calculated for each pixel of the Halpha images. To differentiate between a detection or a spurious oscillation, it is necessary to determine the background noise. We have seen that this background noise is a combination of red and white noise. The red-noise nature of the PSD is problematic in their study since most of the statistical tools developed to identify real oscillations from the noise are for white-noise PSD. The most appropriate approach for this problem is the usage of Bayesian statistics and Monte Carlo Markov Chains (MCMC). MCMC methods can be computationally expensive and have been proven to be too slow for our research aims, so we tackle this problem with deep learning techniques, specifically Convolutional Neural Networks (CNNs). We developed two neural networks, which reproduce the same outcomes as the MCMC methods. Both have been trained with synthetic data as well as real data from the MCMC methods. The results obtained show negligible differences with the results from the MCMC methods but with the advantage of computing times orders of magnitude smaller. |
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Oct 17 | Thu | Daniel Graves (Leeds) | Topology Seminar | |||
16:00 | ||||||
Hicks Seminar Room J11 | ||||||
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Oct 18 | Fri | BT (https://www.kehubmaths.co.uk/triage-workshops/) | Maths Knowledge Exchange Hub Triage Workshops | |||
10:00 | Convex and quasiconvex optimization in cellular radio networks | |||||
https://newton.us21.list-manage.com/track/click?u=1f88d1ca28e2385959c2201f0&id=d2d3d8a61e&e=cfdba87233 | ||||||
Abstract: Certain optimization problems in cellular radio networks (such as are used in 4G and 5G) give rise to non-convex problems, well-known to be difficult to solve with exact algorithms. However, some problems of interest are quasiconvex, and these can typically be solved by reduction to a sequence of convex subproblems. But though such methods are theoretically exact, in practice they often show instabilities due to the ill-conditioning or poor scaling of the sub-problems. This project thus aims to improve on existing solution techniques for quasiconvex optimization problems. Complicated nonlinear constraints also have to be taken into consideration. The particular application of current interest is reducing energy consumption in network operations, while maintaining a good service to users of the network. |
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Oct 18 | Fri | Evgeny Shinder (Sheffield) | Algebraic Geometry Reading Seminar | |||
13:30 | Singularities and cones | |||||
Hicks Seminar Room J11 | ||||||
Abstract: https://www.overleaf.com/read/xcytbwbcktmr#e142a4 |
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Oct 21 | Mon | Luca Giovenzana (Sheffield) | Algebraic Geometry Seminar | |||
14:00 | Mirror symmetry for degenerations and fibrations of K3 surfaces | |||||
Hicks Seminar Room J11 / J11 | ||||||
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Oct 21 | Mon | Fenglong You (Nottingham) | Algebraic Geometry Seminar | |||
15:30 | Gromov—Witten invariants beyond maximal contacts | |||||
Hicks Seminar Room J11 | ||||||
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Oct 22 | Tue | (Sheffield) | Topology Reading Group | |||
16:00 | Double Categories | |||||
Hicks Seminar Room J11 | ||||||
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Oct 23 | Wed | Alex Fink (Queen Mary University of London) | Pure Maths Colloquium | |||
14:00 | Matroid inequalities from algebraic geometry | |||||
Hicks Seminar Room J11 | ||||||
Abstract: Matroids are combinatorial structures that track ``independence'' relations on a set. A key example is linear independence of some linear functions on a vector space. Not all matroids come from a vector space, but those that don't behave in surprising algebraic ways as if they do. Breakthroughs of the last decade have opened a kit of tools from, and inspired by, algebraic geometry to prove inequalities for matroids, among them the ``matroid Hodge theory'' of June Huh and others. I'll start by motivating matroids, and aim to end with enough about my work in progress with Andy Berget to show how its central tool is different to matroid Hodge theory. |
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Oct 23 | Wed | Rishav Roshan (Southampton) | Cosmology, Relativity and Gravitation | |||
15:15 | Using Gravitational Waves to see the Early Universe | |||||
Hicks Seminar Room J11 | ||||||
Abstract: Gravitational waves are a unique probe of the early Universe, as the Universe is transparent to gravitational radiation right back to the beginning. Here, I will summarise some of the different scopes of primordial events like annihilation of topological defects and evaporation of primordial black holes that could lead to a detectable stochastic gravitational wave background. Any such background would shed light on what (if anything) lies beyond the Standard Model, sometimes at remarkably high scales. We overview the range of strategies for detecting a stochastic gravitational wave background before delving deep into three major primordial events that can source such a background. |
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Oct 23 | Wed | Daniel Bassett (Sheffield) | ShEAF: postgraduate pure maths seminar | |||
16:15 | Modularity and Fermat's Last Theorem | |||||
Hicks Seminar Room J11 | ||||||
Abstract: Fermat's Last Theorem was one of the most famous and oldest unsovled problems in mathematics until its resolution by Andrew Wiles in 1994. The final step of the proof was a highly technical proof of a special case of the modularity theorem that I could not hope to describe in an hour. Instead, I will introduce the relevant objects to explore how the modularity theorem allows you to deduce Fermat's last theorem, and discuss how they show up in much of modern number theory research. |
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Oct 25 | Fri | Alexey Elagin (Sheffield) | Algebraic Geometry Reading Seminar | |||
13:30 | Minimal model program | |||||
Hicks Seminar Room J11 | ||||||
Abstract: https://www.overleaf.com/read/xcytbwbcktmr#e142a4 |
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Oct 29 | Tue | Samrat Sen (Instituto de Astrofisica de Canarias) | Plasma Dynamics Group | |||
16:00 | Hot meets cold: From eruption to post-flare rain | |||||
C07 (Amy Johnson Building) | ||||||
Abstract: Erupting magnetic flux ropes (MFRs) play an important role in producing solar flares, whereas fine-scale condensed coronal rain is often found in post-flare loops. However, the formation of the MFRs in the pre-flare stage and how this leads to coronal rain in a post-eruption magnetic loop is not fully understood. In this talk, I will address how these two interdisciplinary aspects are interconnected through numerical modeling. To do this, we perform a resistive-magnetohydrodynamic simulation to explore the evolution of sheared magnetic arcades to explore the formation, and eruption of MFRs, followed by the appearance of coronal rain in the post-flare loops. The system is in mechanical imbalance at the initial state, and evolves self-consistently in a non-adiabatic atmosphere under the influence of radiative losses, thermal conduction, and background heating. The system relaxes to a semi-equilibrium state from its initial mechanical imbalance condition after a short transient temporal evolution. After this period, a series of erupting MFRs is formed due to spontaneous magnetic reconnection, and current sheets are created underneath the erupting flux ropes. Gradual development of thermal imbalance is noticed at a loop top in the post-eruption phase, which leads to catastrophic cooling and formation of cool-condensations. The dynamical and thermodynamic properties of these cool-condensations are in good agreement with observations of post-flare coronal rain. The presented simulation supports the development and eruption of multiple MFRs, and the formation of coronal rain in post-flare loops, which is one of the key aspects to reveal the coronal heating mystery in the solar atmosphere. |
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Oct 29 | Tue | (Sheffield) | Topology Reading Group | |||
16:00 | Double Categories | |||||
Hicks Seminar Room J11 | ||||||
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Oct 30 | Wed | Shiladitya Porey (Shiv Nadar U.) | Cosmology, Relativity and Gravitation | |||
15:00 | Primordial Dark Sector Relics from Inflation: An Additional Way to Probe Viable Inflationary Models | |||||
Blackboard Collaborate | ||||||
Abstract: We investigate the production of non-thermal dark matter (DM) particles, heavy sterile neutrinos from the inflaton, and beyond the Standard Model free-streaming relativistic particles during the reheating era, which is preceded by a slow-roll inflationary epoch. We consider benchmark values for slow-roll single-field inflationary scenarios satisfying current bounds obtained from Planck-BICEP Cosmic Microwave Background (CMB) data. Then, for those benchmark values, we calculate the permissible range of the coupling between the DM particle and the inflaton (y_χ) and the mass of the DM particle (m_χ) for the production of enough DM to explain the total Cold Dark Matter (CDM) mass density of the present universe while satisfying CMB measurements and other cosmological bounds. For slow-roll inflation with quartic potential and non-minimal coupling between inflaton and gravity, we consider the scenario of leptogenesis via the decay of sterile neutrinos produced from the decay of inflaton, and compare the results obtained following both metric and Palatini theory of gravity. Then, we consider inflaton decay as the source of this dark radiation (DR), and use the CMB data from Planck-2018 to constrain the branching fraction for the production of DR from the decay of inflaton, and identify the parameter space involving couplings and mass of the inflaton that will be within the reach of next-generation CMB experiments like spt-3g, CMB-S4, CMB-Bharat, PICO, CMB-HD, etc. |
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Oct 30 | Wed | Henry Rice | ShEAF: postgraduate pure maths seminar | |||
16:15 | Bott Periodicity In Complex Topological K-Theory | |||||
Hicks Seminar Room J11 | ||||||
Abstract: Bott periodicity was originally proved in the context of homotopy theory however in the realm of topological K-Theory it gains tremendous significance by making the K cohomology functor periodic. This is a very surprising fact as topological K-theory is defined geometrically through isomorphism classes of vector bundles. In the 1960s, Bott and Atiyah gave a proof of this flavour (for the real and complex cases) inspired by their work on elliptic boundary valued problems. The proof is a rich blend of analysis, topology and geometry, utilising the deep connection between vector bundles and functional analysis. In this seminar I aim to introduce vector bundles, Topological K-Theory and give a (very rough) sketch of the proof (with pictures). |
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Oct 31 | Thu | Juan Esteban Agudelo (Observatorio Astronómico Nacional de Colombia, Universidad Nacional de Colombia) | SP2RC/ESPOS seminar | |||
10:00 | Solar spectropolarimetric inversions applying Deep Learning techniques | |||||
Online / Zoom | ||||||
Abstract: Recent advancements in spectropolarimetric instrumentation, such as the new facilities at the GREGOR and DKIST telescopes, have generated vast amounts of data with each observation. This increase in data volume results in longer processing times, heightened demands on computational resources, and an expanded carbon footprint, complicating scientific development timelines. The numerical inversion codes used for data analysis, based on radiative transfer models, are inherently complex. Modern projects focused on the solar atmosphere and its magnetic field require additional assumptions, significantly increasing processing times for each pixel. To address this challenge, new methods are being developed, leveraging modern data processing algorithms from statistics and machine learning. We are testing a 1D convolutional neural network model inspired by the 1D parallel atmosphere model of radiative transfer to enhance spectropolarimetric inversions and achieve significant reductions in processing times, as demonstrated in previous studies. Our approach aims to integrate physical constraints into the learning process, allowing the model to not only replicate inversions but also gain insights into the underlying physics. The data for our project was synthesized using state-of-the-art codes for magnetohydrodynamics (MURaM) and radiative transfer under non-local thermodynamic equilibrium (NICOLE). Preliminary results without physical constraints show loss rates approaching 10-3 order of magnitude and Pearson correlations of the order of 0.8 on average along different optical depths inverted in the process for thermodynamic quantities. |
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Oct 31 | Thu | Spectral Sequences Reading Group (Jake Saunders) | ||||
11:00 | ||||||
Hicks Seminar Room J11 | ||||||
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Oct 31 | Thu | Emily Roff (Edinburgh) | Topology Seminar | |||
16:00 | ||||||
Hicks Seminar Room J11 | ||||||
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Nov 4 | Mon | Julia Schneider (Sheffield) | Algebraic Geometry Seminar | |||
14:00 | ||||||
Hicks Seminar Room J11 | ||||||
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Nov 4 | Mon | Giulia Gugiatti (Edinburgh) | Algebraic Geometry Seminar | |||
15:30 | ||||||
Hicks Seminar Room J11 | ||||||
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Nov 5 | Tue | (Sheffield) | Topology Reading Group | |||
16:00 | Double Categories | |||||
Hicks Seminar Room J11 | ||||||
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Nov 6 | Wed | Jake Saunders | ShEAF: postgraduate pure maths seminar | |||
13:00 | tba | |||||
Hicks Seminar Room J11 | ||||||
Abstract: tba |
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Nov 6 | Wed | Rohini Ramadas (University of Warwick) | Pure Maths Colloquium | |||
14:00 | Complex dynamics via algebraic geometry | |||||
Hicks Seminar Room J11 | ||||||
Abstract: Complex dynamics began in the early 1900s with the study of iterating polynomial functions with complex coefficients. This simple idea gives rise to beautiful fractal pictures such as the Mandelbrot set, as well as interesting mathematical questions of many different flavours (algebraic, analytic, topological, arithmetic, etc.). The field gained momentum in the 1980s due to work of Thurston, Douady-Hubbard, Sullivan, and others, connecting these dynamical questions to surface topology and the theory of 3-manifolds. The last decade has seen many breakthroughs achieved via new tools from number theory, measure theory and algebraic geometry. I will discuss some of these recent developments, highlighting the interplay between topology on one hand and algebraic geometry/number theory on the other hand. |
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Nov 6 | Wed | Dr Kieran Kalair (Smith Institute) | SIAM-IMA Chapter Seminar | |||
14:00 | Mathematics and explainable machine learning to support a zero-carbon grid. | |||||
K14 | ||||||
Abstract: The Smith Institute are a mathematics, data science and AI consultancy based in Oxford that solve practical, novel problems using these approaches. I will talk about what we do, and focus on a specific project we have been working on over the last 3 years – called Dynamic Reserve Setting – which looks at how much ‘spare capacity’ needs to be held to secure the GB energy grid. In this problem we care about explainability in our modelling, understanding extreme events in our data, and capturing non-linear relationships that exist in the energy grid. I will talk about both our modelling approach and how we feed results into practical usage. I will end with examples of other problems and methodologies we have worked on. |
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Nov 6 | Wed | Rita Neves (Sheffield) | Cosmology, Relativity and Gravitation | |||
15:15 | An adiabatic approach to the trans-Planckian problem in loop quantum cosmology | |||||
Hicks Seminar Room J11 | ||||||
Abstract: One of the criticisms of the inflationary paradigm is that scales that are observable today were trans-Planckian at the onset of inflation. This questions the validity of standard results regarding the primordial power spectrum. Standard cosmology also ignores pre-inflationary dynamics, since it loses predictability close to the initial singularity. Loop Quantum Cosmology (LQC) is an approach to the quantisation of cosmological models. It provides effective pre-inflationary dynamics where the big-bang singularity is resolved in terms of a quantum bounce that connects a contracting epoch of the Universe with an expanding one. In this talk, we investigate the trans-Planckian problem in two models of LQC. We find that one of the models avoids the issue altogether by generating less e-folds of inflation, such that the observable modes never become trans-Planckian. On the other hand, the other model suffers from this problem, as observable modes become trans-Planckian during a time when they lose adiabaticity, making their primordial power spectrum susceptible to changes due to trans-Planckian physics. |
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Nov 7 | Thu | Cheuk Yu Mak (Sheffield) | Topology Seminar | |||
16:00 | ||||||
Hicks Seminar Room J11 | ||||||
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Nov 8 | Fri | Luca Giovenzana (Sheffield) | Algebraic Geometry Reading Seminar | |||
13:30 | Mori dream spaces and related topics | |||||
Hicks Seminar Room J11 | ||||||
Abstract: https://www.overleaf.com/read/xcytbwbcktmr#e142a4 |
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Nov 12 | Tue | James Rawson (Warwick) | Number Theory seminar | |||
14:00 | Computing Tangent Spaces to Eigenvarieties | |||||
Hicks Seminar Room J11 / Google Meet | ||||||
Abstract: Eigenvarieties are a geometric realisation of p-adic families of modular forms, and their geometry is correspondingly mysterious. In this talk, I will concentrate on smoothness and illustrate a method for computing p-adic approximations to tangent spaces to these spaces via modular symbols. For Bianchi modular forms, this gives a way of verifying the Birch--Swinnerton-Dyer conjecture in rank 0 for the corresponding elliptic curve by a result of Loeffler and Zerbes. |
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Nov 13 | Wed | Gavin Brown (University of Warwick) | Pure Maths Colloquium | |||
14:00 | Flops and noncommutative potentials | |||||
Hicks Seminar Room J11 | ||||||
Abstract: I give an overview of a project with Michael Wemyss to classify simple 3-fold flops. This amounts to understanding when a smooth rational curve (i.e. the Riemann sphere) inside a complex 3-dimensional manifold can be contracted. (One might think of this as a 3d analogue of shrinking the central axis of a Moebius strip to a point, and indeed one could do an unnecessarily elaborate analysis of that situation by the same methods.) In fact, this large family of surgery operations is central to 3d complex geometry, but has nevertheless resisted classification, or even the construction of a set of representative examples. Being a manifold, one can describe the situation by glueing together patches - and it is enough to glue together two copies of the affine space C^3 by a simple formula .. but with lots of free parameters, most of which do not contract. However finding good (i.e. contractible) glue functions (or even classifying them) seems to be a bit needle-in-a-haystack. Instead, we translate the problem to one of classifying noncommutative germs f(x,y) [or equivalently certain complete local algebras up to isomorphism], where the necessary criteria seem more amenable. That context feels much like the classical singularity theory of function germs in the style of Arnold (types ADE and all that), and we can solve enough of that problem to construct all flops and to provide a classification. From one point of view, I’d like to give some idea of what Theorems 5.1 and 5.4 of the following expository tea-time article mean: https://arxiv.org/abs/2410.21500 |
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Nov 13 | Wed | Theo Anton (Queen Mary) | Cosmology, Relativity and Gravitation | |||
15:15 | Generalised tests of gravity in cosmology | |||||
Hicks Seminar Room J11 | ||||||
Abstract: A plethora of modified theories of gravity have been proposed over the last few decades. Testing them all observationally is a considerable challenge, so it is advantageous to develop theory-independent approaches that constrain deviations from General Relativity in a systematic way. Many of the most precise such constraints to date are obtained from astrophysical measurements, for which deviations from GR are described by the parameterised post-Newtonian (PPN) parameters. Some attempts have been made to perform similarly general tests on cosmological scales, but it is not clear that they refer to the same couplings as the PPN formalism does, and so interpreting results from these disparate regimes physically is difficult and potentially misleading. With that problem in mind, I will introduce a framework, called parameterised post-Newtonian cosmology, that allows information from cosmological and astrophysical regimes to be combined consistently. I will present novel constraints on the evolution of the PPN parameters over cosmic history, using data from CMB anisotropies and Solar System experiments concurrently, and I will explain how these ideas can be applied further to test cosmological gravity to high precision. |
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Nov 14 | Thu | Natalia Bajnokova (Univ. of Glasgow, School of Physics & Astronomy (UK) ) | SP2RC/ESPOS seminar | |||
10:00 | First joint NuSTAR and Solar Orbiter/STIX X-ray observations of solar microflares | |||||
Online / Zoom | ||||||
Abstract: Small solar flares, or microflares (GOES B class and fainter), are frequent bursts of energy released in the Sun’s atmosphere, exhibiting heating and particle acceleration similar to that of large flares. X-ray observations provide direct diagnostics to study these processes by examining thermal emission from the hot flare loops and non-thermal emission from accelerated electrons. We present analysis of the X-ray emission from small solar flares jointly observed with the Nuclear Spectroscopic Telescope Array (NuSTAR) and the Spectrometer Telescope for Imaging X-rays (STIX) on Solar Orbiter, providing different viewing angles of each event. NuSTAR is a highly sensitive X-ray imaging spectrometer that can directly image the Sun from 2.5 keV using focusing optics. STIX is an imaging spectrometer which instead uses indirect optics but has detectors capable of handling a wide range of solar X-ray fluxes from 4 to 150 keV. NuSTAR is in Earth orbit, whereas STIX is orbiting the Sun, so the two instruments combined can give different viewing angles of solar X-ray emission, providing a clearer picture of the flare’s structure. Combining analysis of NuSTAR and STIX’s X-ray spectra, we can take advantage of their different strengths, gaining a better understanding of the energy release in solar flares. We present observations of flares from June 2020 (on-disk for both instruments) and September 2022 (occulted for NuSTAR but on-disk for STIX - allowing us to probe a pre-flare non-thermal coronal source with NuSTAR and bright lower atmosphere flare emission with STIX). |
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Nov 14 | Thu | Fabio Reale (Palermo) | Plasma Dynamics Group | |||
15:00 | The Solar Melting Pot: Impulsive Heating in the Solar Corona | |||||
meet.google.com/rvs-aezw-gwy | ||||||
Abstract: Observations in the EUV and X-rays tell us that the solar corona is dominated by the magnetic field. The solar photosphere drags and stresses the field, thus leading to the release of magnetic energy into heat and plasma dynamics. Different scales can be involved, ranging from tiny and elusive impulsive events, called nanoflares, to large events which can even influence human activities, like flares and eruptions, but magnetic reconnection might play a major role in all cases. However, a fully realistic description would require including highly non-linear effects on several spatial and temporal scales which are unfeasible today. I will discuss MHD modeling in the light of comparison and diagnostics from present-day and forth-coming observations. |
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Nov 15 | Fri | Vanellus (https://www.kehubmaths.co.uk/triage-workshops/) | Maths Knowledge Exchange Hub Triage Workshops | |||
10:00 | Reduced-order fluid and thermal modelling for Triply Periodic Minimal Surfaces | |||||
Abstract: Triply Periodic Minimal Surfaces (TMPS) have found applications in high-performance heat exchangers, where engineers want to maximise the surface area to volume ratio to get the best heat transfer performance. These types of designs have only recently become feasible to manufacture thanks to metal 3D printing. However, their performance is poorly characterised, in large part due to challenges in simulating them. Traditional methods for simulating heat exchangers (i.e. Computational Fluid Dynamics) involve creating a high-quality mesh for the entire domain and solving PDEs using the finite volume/element method. The problem is, for heat exchangers with thousands of TMPS unit cells, this quickly becomes computationally intractable both to produce the mesh and solve the equations. We want to explore how we can exploit the periodic structure of these surfaces to create reduced-order models in order to make solving for key quantities such as pressure drop and heat transfer coefficients tractable. Designing more efficient heat exchangers is vital in a wide range of application areas, such as cooling high-powered GPUs, cooling the batteries of electric cars, and increasing turbomachinery efficiency. Vanellus are an early stage startup based in Cambridge, where we are developing GPU-accelerated modelling tools for fluid and thermal problems on complex geometries. |
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Nov 15 | Fri | Markus Szymik (Sheffield) | Algebraic Geometry Reading Seminar | |||
13:30 | Sarkisov link decomposition and relations statements | |||||
Hicks Seminar Room J11 | ||||||
Abstract: https://www.overleaf.com/read/xcytbwbcktmr#e142a4 |
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Nov 18 | Mon | Pavel Sechin (Regensburg) | Algebraic Geometry Seminar | |||
14:00 | ||||||
Hicks Seminar Room J11 | ||||||
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Nov 18 | Mon | Alexey Elagin | Algebraic Geometry Seminar | |||
15:30 | ||||||
Hicks Seminar Room J11 | ||||||
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Nov 19 | Tue | Ariel Weiss (The Ohio State University) | Number Theory seminar | |||
14:00 | ||||||
Hicks Seminar Room J11 / Google Meet | ||||||
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Nov 20 | Wed | Jason Semeraro (University of Loughborough) | Pure Maths Colloquium | |||
14:00 | Fusion-stable representations of finite groups | |||||
Hicks Seminar Room J11 | ||||||
Abstract: This is joint work with my PhD student Tom Lawrence. For a prime p, the p-decomposition matrix D of a finite group G records the way each irreducible ordinary representation of G breaks up into irreducible p-Brauer characters under reduction modulo p. Multiplying D by its transpose yields the Cartan matrix, whose determinant is well-known to be a power of p. A representation of a Sylow p-subgroup S of G is fusion-stable if it is left invariant by the conjugation action of G. After first fixing a basis B of fusion-stable representations of S one can consider an analogue of D for fusion-stable representations which records how each irreducible ordinary representation of G breaks up in B under restriction to S. It turns out this matrix has many properties analogous to those of the classical decomposition matrix, and using them one can show that the modulus square of the determinant of the fusion-stable character table (columns indexed by G-classes of p-elements, rows by elements of B) is always a particular power of p independent of the choice of B. I conjectured that the same result holds for any saturated fusion system on S and I'll provide some evidence for this by explicitly computing with some infinite families of exotic examples. If time permits I will also explain how this project fits within the larger framework of "exotic representation theory" whose aim to extend results about ordinary representations to the settings of fusion systems, spetses and other related structures. |
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Nov 20 | Wed | Dr Ross Drummond (University of Sheffield (EEE)) | SIAM-IMA Chapter Seminar | |||
14:00 | Robustifying neural networks: The view from Control Theory | |||||
K14, Hicks / Google Meet | ||||||
Abstract: This talk will describe some results on applying ideas from robust control theory to design and interpret neural networks. The basic idea is to use results from absolute stability theory to train neural networks with robustness guarantees built in. Furthermore, a method to represent model predictive control directly in terms of a neural network is also discussed. The overriding goal is to turn robustness analysis problems for neural networks into synthesis problems to overcome some of their limitations. |
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Nov 20 | Wed | Enrico Specogna (Sheffield) | Cosmology, Relativity and Gravitation | |||
15:15 | Model-independent Tests for General Relativity | |||||
Hicks Seminar Room J11 | ||||||
Abstract: General relativity (GR) is the gravitational framework that underpins the standard model of cosmology, the ΛCDM model; its predictions have been widely tested at astrophysical and cosmological scales, often with remarkable precision. However, our inability to directly observe the constituents of this model's so-called 'dark sector' (i.e., dark matter and dark energy), along with the tensions characterising some of its parameters, prompts us to question the validity of GR at cosmological scales. That implies substituting GR with a modified gravity theory (MG) that can, for instance, explain the observed accelerated expansion of the universe without the need to introduce a cosmological constant (Λ). How can we test if a MG cosmology is sustained by current observations? Because MG theories are numerous, we can turn to general, model-independent parameterizations of gravity, able to capture the phenomenology of several classes of deviations from GR at once. In this talk, I will present two such parameterizations: the μ/Σ framework and the growth index γ. I will show how they can be used to solve a discrepancy within different cosmic microwave background measurements (CMB) known as the 'lensing anomaly', while also explaining the apparent MG detection reported by the Planck CMB telescope as a collateral effect of the same anomaly. |
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Nov 20 | Wed | Nathan Blacher | ShEAF: postgraduate pure maths seminar | |||
16:15 | When are noncommutative rings actually commutative? | |||||
Hicks Seminar Room J11 | ||||||
Abstract: In 1945 Jacobson proved that if each element x of a ring satisfies x^n=x for some n>1, then the ring is commutative. This was the first of an ongoing series of celebrated commutativity theorems, and we will discuss some examples and a new approach introduced a few years ago. Beyond identities like Jacobson's, are there different kinds of properties that force a ring to be commutative? Ring theory often studies noncommutative areas which resemble the better understood world of commutative algebra. We will see that sometimes if you get close you end up inside. |
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Nov 21 | Thu | Willow Bevington (Edinburgh) | Topology Seminar | |||
16:00 | ||||||
Hicks Seminar Room J11 | ||||||
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Nov 22 | Fri | Julia Schneider (Sheffield) | Algebraic Geometry Reading Seminar | |||
13:30 | Combinatorics of ample models | |||||
Hicks Seminar Room J11 | ||||||
Abstract: https://www.overleaf.com/read/xcytbwbcktmr#e142a4 |
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Nov 26 | Tue | Neil Dummigan | Number Theory seminar | |||
14:00 | Residual paramodularity of a certain Calabi-Yau 3-fold | |||||
Hicks Seminar Room J11 / Google Meet | ||||||
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Nov 26 | Tue | Simon Willerton (Sheffield) | MiaowMiaow (2d category theory) seminar | |||
16:00 | Internal categories, categorification and (pseudo-)double categories | |||||
Hicks Seminar Room J11 | ||||||
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Nov 27 | Wed | Cheuk Yu Mak (University of Sheffield) | Pure Maths Colloquium | |||
14:00 | From area preserving homeomorphism groups to symplectic Khovanov homology and beyond | |||||
Hicks Seminar Room J11 | ||||||
Abstract: In the first half of the talk, I will explain some recent breakthroughs in the study of the area preserving homeomorphism groups of surfaces using Floer theory. After that, I will explain what happens when we try to generalize it to higher dimensions and the relation to Khovanov homology as well as the Hilbert schemes of points. No prior knowledge on Floer theory or symplectic geometry is assumed. |
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Nov 27 | Wed | Pablo Rodolfo Baldivieso Monasterios (University of Sheffield (EEE)) | SIAM-IMA Chapter Seminar | |||
14:00 | A robust solution to the plug and play problem: a study of interconnectedness. | |||||
K14, Hicks / Google Meet | ||||||
Abstract: Networked systems are a collection of dynamical systems interconnected via physical or digital links. These networks are ubiquitous in the modern world and range from power networks to the financial system. A particular feature of these networks is their size changes over time: new elements are added, and some old elements are removed. The control of these systems presents a significant challenge. Classical techniques are monolithic, and changes in size or the interconnection structure may require a complete redesign of controllers. The plug-and-play paradigm necessitates controllers with reconfiguration capabilities to adapt to such structural changes. In contrast, coalitional control offers a control methodology inherently capable of reconfiguration. In this talk, we discuss how the reconfiguration properties of a coalitional controller arise via partitioning the network's set of elements. We endow each of these elements with robust distributed predictive controllers designed to withstand interconnections through invariant sets. The size of the interconnections parameterises these invariant sets; the shrinkage of these sets allows each agent to tolerate exogenous disturbances. The addition of new elements to a network is modelled as a disturbance. Upon adding a new element, its neighbouring elements coalesce to manage transients. We show that this controller allows us to conclude the asymptotic stability of the equilibrium point and constraint satisfaction of the overall network. |
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Nov 27 | Wed | Sergio Sevillano Muñoz (Durham) | Cosmology, Relativity and Gravitation | |||
15:15 | Screening mechanisms in scalar-tensor theories from a particle perspective | |||||
Hicks Seminar Room J11 | ||||||
Abstract: Scalar-tensor theories are a popular extension of gravity where an extra scalar degree of freedom non-minimally couples to the gravitational sector. Despite existing experimental tests for such modifications from general relativity, there is still no conclusive evidence for or against these theories. A possible reason for this is the presence of screening mechanisms, which can hide the scalar field’s effects (such as long-range forces) in high-density environments, making them undetectable for our local experiments and observations. In this talk, I will use field theory to demonstrate that screening mechanisms can also be expressed as Beyond Standard Model physics. This perspective reveals possible phenomenological implications that don't rely on new long-range forces. In particular, I will focus on how screening mechanisms can lead to spatially dependent masses for elementary particles in the Standard Model. |
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Nov 27 | Wed | Matt Antrobus (Manchester) | ShEAF: postgraduate pure maths seminar | |||
16:15 | Algebra on the second floor | |||||
Hicks Seminar Room J11 | ||||||
Abstract: Research in mathematics is exploring a dark house; spending months tripping over furniture and slamming into walls until finally you find a light switch. Imagine if in your exploration, you found a second floor. (Alternative title: A Gentle introduction to Homological Algebra) |
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Nov 28 | Thu | Jeffersson Agudelo Rueda (Northumbria Univ., Solar Physics Group (UK)) | SP2RC/ESPOS seminar | |||
10:00 | Turbulence and reconnection: exploring the role of kinetic fluctuations on the formation of plasmoids in a current sheet and how to include small-scale phenomena on large-scale systems | |||||
Online / Zoom | ||||||
Abstract: Magnetic reconnection and turbulence are two phenomena that are often invoked to address outstanding open questions as the energy dissipation problem and the heating and acceleration of the solar wind. These two phenomena are closely related to each other in a wide range of plasmas. Turbulent fluctuations can emerge in critical regions of reconnection events, and magnetic reconnection can occur as a product of the turbulent cascade. In this seminar I present some results exploring the interlink between turbulence and reconnection. This talk is divided in two sections, the first one Exploring the Effect of Driving Turbulent-like Fluctuations on a Harris Current Sheet Configuration and the Formation of Plasmoids and the second one Characterising Sub-Grid-Scale Effects on the Ohms Law Terms in Hybrid Simulations of Turbulence at the Earth’s Magnetosheath. The connecting thread is the non-linear and multi-scale nature of turbulence and reconnection as well as the importance of the small-scale dynamics on the large-scale one. In the first study, we perform 2D particle-in-cell simulations of a reconnecting Harris current sheet in the presence of turbulent fluctuations to explore the effect of turbulence on the reconnection process in collisionless non-relativistic pair-plasmas. We find that the presence of a turbulent field can affect the onset and evolution of magnetic reconnection. Moreover, we observe the existence of a scale dependent amplitude of magnetic field fluctuations above which these fluctuations can disrupt the growing of magnetic islands. These fluctuations provide thermal energy to the particles within the current sheet and preferential perpendicular thermal energy to the background population. In our second study we address the challenge that poses the modelling of large-scale systems while accounting for the small-scale phenomena by characterising the contribution of the small-scale dynamic terms on the generalized Ohms law in Vlasov-Hybrid simulations of turbulence in Earth’s magnetosheath. This with the aim of providing insight on Sub-Grid-Scale models that can be incorporated in Large Eddy Simulations. Our results are highly relevant to the future modelling of large-scale turbulent plasmas such as magnetospheres, the solar wind, the solar atmosphere, and other astrophysical systems. |
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Nov 28 | Thu | Henry Rice (Spectral Sequences Reading Group) | ||||
13:00 | ||||||
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Nov 28 | Thu | Oscar Randal-Williams (Cambridge) | Topology Seminar | |||
16:00 | Configuration spaces as commutative monoids | |||||
Hicks Seminar Room J11 | ||||||
Abstract: The 1-point compactification of the space of unordered configurations of n points in a compact manifold M is well-known to be homotopy invariant in M. In fact the collection of all these spaces have further structure: they form a commutative monoid object, by superposition of configurations. I will show how this commutative monoid object has a simple (derived) presentation, and explain various consequences for the homology of configuration spaces which can be derived from this. |
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Nov 29 | Fri | TBC | Algebraic Geometry Reading Seminar | |||
13:30 | Constructing group homomorphisms from the Cremona groups | |||||
Hicks Seminar Room J11 | ||||||
Abstract: https://www.overleaf.com/read/xcytbwbcktmr#e142a4 |
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Dec 2 | Mon | Nic Freeman (Sheffield) | ||||
13:00 | Mean curvature flow and the motion of hybrid zones | |||||
LT3 | ||||||
Abstract: Hybrid zones are thin interfaces between populations that are genetically distinct, but still able to interbreed. They are maintained by a fine balance between natural selection and movement across space. The talk will focus on modelling the motion of hybrid zones, as time passes, based on a connection between Brownian motion and curvature flow. |
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Dec 2 | Mon | James Jones (Loughborough) | Algebraic Geometry Seminar | |||
14:00 | Tyurin Degenerations of K3 Surfaces of Degree 4 | |||||
Hicks Seminar Room J11 / J11 | ||||||
Abstract: Moduli spaces of K3 surfaces have long been studied, beginning with the proof of the Torelli theorem for K3s in the 70s. The most well-known compactification of this moduli space is still probably the Baily-Borel compactification, whose boundary components consist of Type II and Type III degenerations. Meanwhile, the GIT compactification is able to explicitly describe the elements of its boundary components with equations. In this talk we consider the simplest Type II degenerations, which are called Tyurin degenerations. We explicitly demonstrate a correspondence between the Type II boundary components of the Baily-Borel and GIT compactifications of the moduli space of K3 surfaces of degree 4. Using this, we will classify all Tyurin degenerations of K3 surfaces of degree 4. |
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Dec 2 | Mon | Ideal Majtar (SISSA, Trieste) | Algebraic Geometry Seminar | |||
15:30 | Partition function of gauge theories on the blowup and non-perturbative topological strings | |||||
Hicks Seminar Room J11 / J11 | ||||||
Abstract: The low-energy theory of 4d N=2 supersymmetric gauge theories is encoded in the Seiberg-Witten (SW) curve, which is naturally related to an integrable system. In the presence of Omega-background, this integrable system is given by Painlevé equations. In this talk we will show that the Nekrasov partition functions of 4d SU(2) susy gauge theories on the blowup of spacetime are tau functions, which solve the Painlevé equations in Hirota bilinear form. These solutions can be expressed as expansions in terms of the moduli of the quantum SW curve, and the construction can be applied also to non-Lagrangian theories. Furthermore, these solutions have manifest modular properties that provide a natural non-perturbative completion of the corresponding topological string partition function and directly lead to the BCOV holomorphic anomaly equations of the topological string. |
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Dec 3 | Tue | Ho Leung Fong (Sheffield) | Number Theory seminar | |||
14:00 | Adjoint L-functions and my recent research | |||||
Hicks Seminar Room J11 / Google Meet | ||||||
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Dec 5 | Thu | Gong Show | Topology Seminar | |||
15:00 | ||||||
Hicks Seminar Room J11 | ||||||
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Dec 9 | Mon | Rob Noble (City University) | ||||
13:00 | Mathematical and Statistical Modelling seminar | |||||
LT3 | ||||||
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Dec 11 | Wed | Dr Carolanne Vouriot (University of Sheffield (School of Mechanical, Aerospace and Civil Engineering)) | SIAM-IMA Chapter Seminar | |||
14:00 | ||||||
K14, Hicks | ||||||
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Dec 11 | Wed | Cameron Bunney (Nottingham) | Cosmology, Relativity and Gravitation | |||
15:00 | ||||||
Hicks Seminar Room J11 | ||||||
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Dec 12 | Thu | TBA (Univ. College London, Mullard Space Science Lab, MSSL (UK) ) | SP2RC/ESPOS seminar | |||
10:00 | TBA | |||||
Online / Zoom | ||||||
Abstract: TBA |
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Dec 12 | Thu | Constanze Roitzheim (Kent) | Topology Seminar | |||
16:00 | Homotopy theory of finite total orders, trees and chicken feet | |||||
Hicks Seminar Room J11 | ||||||
Abstract: A transfer system is a graph on a lattice satisfying certain restriction and composition properties. They were first studied on the lattice of subgroups of a finite group in order to examine equivariant homotopy commutativity, which then unlocked a wealth of links to combinatorial methods. On a finite total order [n], transfer systems can be used to classify different homotopy theories on [n]. The talk will involve plenty of examples and not assume any background knowledge. |
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Dec 13 | Fri | These Hands Academy (https://www.kehubmaths.co.uk/triage-workshops/) | Maths Knowledge Exchange Hub Triage Workshops | |||
10:00 | Better Connected Care – a case for transformation | |||||
Abstract: “How can the use of the National Early Warning Score (NEWS) in care homes, combined with an analysis of wider determinants of health, improve the proactive management of deterioration in residents with long-term conditions, and reduce unnecessary hospital admissions?” These Hands Academy has provided care homes with the ability to record a NEWS score, which is the only validated tool used across the NHS to respond to deterioration. We have collected 18 months worth of clinical data across Leicester, Leicestershire and Rutland. Used proactively, we believe this data can help us start to understand how well people are living in care homes, often with long-term conditions. We would like to use this data as a benchmark for health care to understand social care and drive improvement, training and provision. However, we first need to understand the data more deeply in relation to the wider determinants of health and virtual ward provision, which is often siloed to a disease process. The analysis would support a case for transformation across the social care sectors to embed this proactive tool to manage deterioration and avoid unnecessary admissions that result in extended and harmful hospital stays. |
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Dec 16 | Mon | Nik Cunniffe (Cambridge University) | ||||
13:00 | Mathematical and Statistical Modelling seminar | |||||
LT3 | ||||||
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Dec 18 | Wed | Yuejia Zhai (Sheffield) | Cosmology, Relativity and Gravitation | |||
15:00 | ||||||
Hicks Seminar Room J11 | ||||||
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Dec 19 | Thu | Martin Palmer (Leeds/Bucharest) | Topology Seminar | |||
16:00 | ||||||
Hicks Seminar Room J11 | ||||||
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Jan 17 | Fri | Syngenta (https://www.kehubmaths.co.uk/triage-workshops/) | Maths Knowledge Exchange Hub Triage Workshops | |||
10:00 | Nonlinear toxicokinetic modelling – can mathematics allow analytical insight? | |||||
Abstract: ToxicoKinetic (TK) models are an important class of ordinary differential equation (ODE) based models that are useful for predicting internal dose for chemical risk assessment applications. These models help to understand the effect of the chemical on the body by analysing its absorption, distribution, metabolism, and excretion (ADME) properties. These effects are typically summarized using TK parameters such as clearance and volume of distribution which are useful for understanding the effects of a chemical on the body. TK models can range in complexity from ODE models with a single compartment to models containing hundreds of compartments. Each type of model from the simplest, one-compartment model, to more complex models have their own applications and can be used to gain valuable information from toxicokinetic data. This triage workshop relates to the ‘top down’ use of TK models – wherein the models are built based on fitting an ODE model to observed toxicokinetic data. Simple analysis of the data (referred to as non-compartmental analysis) can reveal whether the terms in the underlying ODE model should be linear or nonlinear. There is a plethora of literature on simple analytical approaches to understand and utilise the linear case but not the nonlinear case and the aim of this workshop is to explore whether advances can be made to extend the analysis into the nonlinear regime. Currently, a thorough fitting and analysis of a nonlinear TK model takes significant time. An advance in this area would significantly reduce this time investment and support more rapid, data informed decision making to support safe chemical design. |
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Jan 31 | Fri | Barworth Agriculture (https://www.kehubmaths.co.uk/triage-workshops/) | Maths Knowledge Exchange Hub Triage Workshops | |||
10:00 | TBA | |||||
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