Seminars this semester


   Series:

 
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
Hicks Seminar Room J11
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Nov 6 Wed Marco Fazzi (Sheffield) Cosmology, Relativity and Gravitation
15:15
Hicks Seminar Room J11
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Nov 7 Thu Willow Bevington (Edinburgh) 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
Hicks Seminar Room J11 / Google Meet
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Nov 13 Wed Gavin Brown (University of Warwick) Pure Maths Colloquium
14:00
Hicks Seminar Room J11
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Nov 13 Wed Theo Anton (Queen Mary) Cosmology, Relativity and Gravitation
15:15
Hicks Seminar Room J11
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Nov 14 Thu TBA (Univ. of Glasgow, School of Physics & Astronomy (UK) ) SP2RC/ESPOS seminar
10:00 TBA
Online / Zoom
  Abstract:
TBA
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Nov 15 Fri Vanellus (https://www.kehubmaths.co.uk/triage-workshops/) Maths Knowledge Exchange Hub Triage Workshops
10:00
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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 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 Enrico Specogna (Sheffield) Cosmology, Relativity and Gravitation
15:15
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 27 Wed Cheuk Yu Mak (University of Sheffield) Pure Maths Colloquium
14:00
Hicks Seminar Room J11
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Nov 27 Wed Sergio Sevillano Muñoz (Durham) Cosmology, Relativity and Gravitation
15:15
Hicks Seminar Room J11
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Nov 28 Thu TBA (Northumbria Univ., Solar Physics Group (UK)) SP2RC/ESPOS seminar
10:00 TBA
Online / Zoom
  Abstract:
TBA
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Nov 28 Thu Oscar Randal-Williams (Cambridge) Topology Seminar
16:00
Hicks Seminar Room J11
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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 3 Tue Ho Leung Fong (Sheffield) Number Theory seminar
14:00
Hicks Seminar Room J11 / Google Meet
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Dec 5 Thu Martin Palmer (Bucharest/Leeds) Topology Seminar
16:00
Hicks Seminar Room J11
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Dec 11 Wed Asma Hassanezhad (University of Bristol) Pure Maths Colloquium
14:00
Hicks Seminar Room J11
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Dec 11 Wed Cameron Bunney (Nottingham) Cosmology, Relativity and Gravitation
15:15
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
Hicks Seminar Room J11
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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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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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