Physics seminars
from
Thursday, 1 January 2026 (15:00)
to
Thursday, 31 December 2026 (17:00)
Monday, 29 December 2025
Tuesday, 30 December 2025
Wednesday, 31 December 2025
Thursday, 1 January 2026
Friday, 2 January 2026
Saturday, 3 January 2026
Sunday, 4 January 2026
Monday, 5 January 2026
Tuesday, 6 January 2026
Wednesday, 7 January 2026
Thursday, 8 January 2026
Friday, 9 January 2026
Saturday, 10 January 2026
Sunday, 11 January 2026
Monday, 12 January 2026
Tuesday, 13 January 2026
Wednesday, 14 January 2026
Thursday, 15 January 2026
Friday, 16 January 2026
Saturday, 17 January 2026
Sunday, 18 January 2026
Monday, 19 January 2026
Tuesday, 20 January 2026
Wednesday, 21 January 2026
Thursday, 22 January 2026
Friday, 23 January 2026
Saturday, 24 January 2026
Sunday, 25 January 2026
Monday, 26 January 2026
Tuesday, 27 January 2026
15:00
A Roadmap to Strong-Field QED: Concepts, Experiments, and the LUXE Program
-
Ivo Schulthess
(
ETH Zurich
)
A Roadmap to Strong-Field QED: Concepts, Experiments, and the LUXE Program
Ivo Schulthess
(
ETH Zurich
)
15:00 - 16:00
Room: Room 412 C - Ferrara
Strong-field QED describes the interaction of charged particles and photons with electromagnetic fields so intense that non-linear and non-perturbative effects become experimentally accessible, enabling phenomena such as non-linear Compton scattering and non-linear Breit–Wheeler pair production. These effects are not only of fundamental interest in the laboratory but are also relevant to extreme astrophysical environments, such as the magnetospheres of neutron stars. This talk provides a roadmap of strong-field QED, introducing the key concepts and physical regimes and reviewing the main experimental approaches pursued today, including crystals, beam–beam interactions, and collisions between electrons or photons and high-intensity laser pulses. Particular emphasis is placed on the LUXE experiment at DESY, which will probe this regime with high precision using the 16.5 GeV electron beam of the European XFEL and an ultra-intense optical laser. Finally, the potential of high-energy photons from strong-field interactions for beam-dump–type new physics searches is discussed.
Wednesday, 28 January 2026
Thursday, 29 January 2026
Friday, 30 January 2026
Saturday, 31 January 2026
Sunday, 1 February 2026
Monday, 2 February 2026
Tuesday, 3 February 2026
Wednesday, 4 February 2026
11:00
Euclid Q1 galaxy clustering and its cross-correlations with CMB lensing
-
Margherita Lembo
(
IAP, Paris, France
)
Euclid Q1 galaxy clustering and its cross-correlations with CMB lensing
Margherita Lembo
(
IAP, Paris, France
)
11:00 - 12:00
Room: Room 412 C - Ferrara
Combining Cosmic Microwave Background (CMB) and large-scale structure (LSS) observations provides a powerful way to probe the evolution of the Universe from recombination to the present day, test gravity on cosmological scales, and constrain the nature of dark matter and dark energy. In this talk, I present the first measurements of galaxy clustering from the Euclid Q1 data release and its cross-correlation with CMB lensing convergence maps from Planck and the Atacama Cosmology Telescope. We detect the signal at high significance and find excellent agreement with expectations from simulations and the Planck 2018 cosmological model. I will discuss robustness tests against observational systematics, tomographic measurements, and early constraints on galaxy bias and redshift uncertainties. These results demonstrate the strong potential of Euclid–CMB cross-correlations to deliver robust cosmological constraints and to mitigate systematics in future Euclid data releases. zoom: https://cern.zoom.us/j/65644266180?pwd=xdfyl67pQ0zfWjyFui5klxnsSRb8WZ.1
Thursday, 5 February 2026
Friday, 6 February 2026
10:00
Cosmic strings and domain walls: CMB constraints and the role of B-modes
-
Luca Caloni
(
Universidade de Coimbra, Coimbra, Portugal
)
Cosmic strings and domain walls: CMB constraints and the role of B-modes
Luca Caloni
(
Universidade de Coimbra, Coimbra, Portugal
)
10:00 - 11:00
Room: Room 412 C - Ferrara
Cosmic strings and domain walls are topological defects arising from the spontaneous breaking of new symmetries in the early Universe, as predicted in several beyond the Standard Model scenarios. In this talk, I will briefly introduce the physics of defect networks and discuss their impact on cosmological observables, with particular emphasis on their signatures in the Cosmic Microwave Background. I will then present constraints derived from current CMB data, highlighting in particular the role of B-mode polarization. Finally, I will outline prospects for upcoming CMB experiments and their potential to significantly improve sensitivity to topological defects. zoom: https://cern.zoom.us/j/64532006687?pwd=Bj4hXXbb2t6MZnFlXq0vCTE4EPXrPu.1
Saturday, 7 February 2026
Sunday, 8 February 2026
Monday, 9 February 2026
Tuesday, 10 February 2026
Wednesday, 11 February 2026
Thursday, 12 February 2026
Friday, 13 February 2026
14:30
Coincidence and anti-coincidence gamma ray spectroscopy in radionuclide identification
-
Sheldon Landsberger
(
Nuclear and Radiation Engineering Program Walker Department of Mechanical Engineering University of Texas at Austin, USA
)
Coincidence and anti-coincidence gamma ray spectroscopy in radionuclide identification
Sheldon Landsberger
(
Nuclear and Radiation Engineering Program Walker Department of Mechanical Engineering University of Texas at Austin, USA
)
14:30 - 15:30
Room: Room 412 C - Ferrara
The two most challenging aspects of gamma ray spectrometry are to achieve spectral free interferences and to attain the lowest possible detection limits and ultimately low uncertainties. In nuclear forensics isotopic ratios or elemental ratios in environmental analyses need to have the individual results at low uncertainties for meaningful interpretations. Over the last decades gamma-gamma coincidence and anti-coincidence (Compton suppression) methods have been used for variety radionuclide identifications for passive counting of naturally occurring radioactive material (NORM), special nuclear materials (239Pu), fission products and neutron activation analysis (NAA) for environmental, geological, and biological samples. One real major advantage of these methods is that spectral interferences can be significantly reduced as in the case of Compton suppression or be eliminated as in gamma-gamma coincidence, while also reducing the Compton continuum and decreasing detection limits. For instance, the determination of 137Cs in soil with Compton suppression can be determined at less than 1 Bq/kg for only a twenty-gram sample. In neutron activation analysis elements such as arsenic and cadmium in biological specimens can be determined with detection limits at the ng/g level, which cannot be determined using traditional NAA methods. There are a host of elements determined by NAA that have benefitted using gamma-gamma coincidence and anti-coincidence methods. And in many cases, elements that are seldom or never reported, can now be effectively determined incorporating epithermal neutrons where the resonance integrals for several elements are high. An overview of these methods will be delineated with specific examples. Zoom: https://cern.zoom.us/j/68713119184?pwd=HbCsVLUEbBC7JtpriZza6iUr5OylYN.1
Saturday, 14 February 2026
Sunday, 15 February 2026
Monday, 16 February 2026
Tuesday, 17 February 2026
Wednesday, 18 February 2026
Thursday, 19 February 2026
Friday, 20 February 2026
Saturday, 21 February 2026
Sunday, 22 February 2026
Monday, 23 February 2026
Tuesday, 24 February 2026
Wednesday, 25 February 2026
Thursday, 26 February 2026
Friday, 27 February 2026
Saturday, 28 February 2026
Sunday, 1 March 2026
Monday, 2 March 2026
Tuesday, 3 March 2026
Wednesday, 4 March 2026
Thursday, 5 March 2026
Friday, 6 March 2026
11:00
CHRONOS: A Cryogenic Sub-Hz Torsion-Bar Speed-Meter for Stochastic Gravitational-Wave Background Searches
-
Yuki Inoue
(
National Central University, Taiwan
)
CHRONOS: A Cryogenic Sub-Hz Torsion-Bar Speed-Meter for Stochastic Gravitational-Wave Background Searches
Yuki Inoue
(
National Central University, Taiwan
)
11:00 - 12:00
Room: Room 412 C - Ferrara
Abstract: The sub-Hz frequency band represents one of the last unexplored frontiers in gravitational-wave (GW) astronomy. Access to this regime opens a unique observational window onto cosmological stochastic gravitational-wave backgrounds (SGWB), early-Universe phase transitions, cosmic strings, and low-frequency compact binaries beyond the reach of current ground-based interferometers. In this talk, I will present CHRONOS (Cryogenic sub-Hz cROss torsion-bar detector with quantum NOn-demolition Speed meter), a novel interferometric concept designed to probe the 0.1–10 Hz band from the ground. CHRONOS combines a cross torsion-bar topology with a Sagnac speed-meter configuration, implementing quantum non-demolition (QND) measurement principles to suppress radiation-pressure noise at low frequencies. In contrast to conventional position-meter Michelson interferometers, the rotational speed-meter observable intrinsically modifies the quantum noise coupling, enabling stable low-frequency performance. By operating cryogenic sapphire test masses, the detector further reduces thermal noise and aims to achieve quantum-noise-limited sensitivity in the sub-Hz regime. I will first outline the interferometer topology and the associated quantum-noise behavior that distinguish rotational speed-meter measurements from traditional configurations. I will then present the projected sensitivity and noise budget of CHRONOS, highlighting the achievable performance in the sub-Hz band. Finally, I will discuss the prospects for stochastic gravitational-wave background searches, including sensitivity projections to cosmological models. CHRONOS provides a complementary path toward extending terrestrial gravitational-wave detection into the sub-Hz domain, bridging the frequency gap between existing ground-based detectors and future space missions, and opening new opportunities for probing fundamental physics and cosmology. zoom: https://cern.zoom.us/j/63349754507?pwd=TbxHYvQV1jCX5YIHHDYYfua1DdEwpP.1
Saturday, 7 March 2026
Sunday, 8 March 2026
Monday, 9 March 2026
Tuesday, 10 March 2026
15:00
Fundamental Physics with Cosmic Microwave Background Observations
-
Masashi Hazumi
(
INFN Visiting Scientist on leave from KEK/IPNS Tsukuba
)
Fundamental Physics with Cosmic Microwave Background Observations
Masashi Hazumi
(
INFN Visiting Scientist on leave from KEK/IPNS Tsukuba
)
15:00 - 16:00
Room: Room 412 C - Ferrara
Particle cosmology aims to uncover the fundamental laws of physics that govern the Universe. Our research today is driven by five outstanding mysteries: cosmic inflation, baryon asymmetry, neutrino properties, dark matter, and dark energy. In addition, two recent observational hints—possible parity violation in cosmological signals and indications of dynamical dark energy—suggest that new physics may be within reach. Resolving any of these questions would profoundly transform particle physics and our understanding of the Universe. Among the many observational probes, measurements of the cosmic microwave background (CMB) play a key role. After reviewing past CMB observations, I will introduce the projects I am currently involved in, with particular emphasis on the Simons Observatory and LiteBIRD. I will conclude by discussing the emerging synergy between CMB measurements and gravitational-wave observations, and how their combination may open new windows onto fundamental physics. Zoom: https://cern.zoom.us/j/67644485998?pwd=xWBE2XzKEioRiXMwMCnaAxGMXJ7LXG.1
Wednesday, 11 March 2026
Thursday, 12 March 2026
Friday, 13 March 2026
Saturday, 14 March 2026
Sunday, 15 March 2026
Monday, 16 March 2026
Tuesday, 17 March 2026
Wednesday, 18 March 2026
Thursday, 19 March 2026
Friday, 20 March 2026
Saturday, 21 March 2026
Sunday, 22 March 2026
Monday, 23 March 2026
Tuesday, 24 March 2026
Wednesday, 25 March 2026
Thursday, 26 March 2026
Friday, 27 March 2026
Saturday, 28 March 2026
Sunday, 29 March 2026
Monday, 30 March 2026
Tuesday, 31 March 2026
Wednesday, 1 April 2026
Thursday, 2 April 2026
Friday, 3 April 2026
Saturday, 4 April 2026
Sunday, 5 April 2026
Monday, 6 April 2026
Tuesday, 7 April 2026
14:00
Beyond the Cosmological Constant: The Dark Energy Quest
-
Pietro Ghedini
Beyond the Cosmological Constant: The Dark Energy Quest
Pietro Ghedini
14:00 - 15:00
Room: Room 412 C - Ferrara
Understanding the nature of dark energy remains one of the central challenges in modern cosmology. In this seminar, I will present recent advances in probing extensions to the standard ΛCDM model using both observational and theoretical approaches. First, I discuss interacting dark energy models in which dark matter and dark energy interact non-gravitationally. In particular, I will highlight the importance of redshift space distortion measurements in narrowing the allowed parameter space, providing tight constraints on the interacting dark energy model considered. I then present a model-independent study of the cosmic evolution of dark energy using a non-parametric reconstruction method. Given the degeneracies between dark energy and neutrinos, we use the same formalism to reconstruct also the sum of neutrino masses. Our analysis indicates that deviations from a cosmological constant are generally small, though certain data combinations allow for phantom‑like dark energy evolution with implications for neutrino mass bounds. Together, these studies highlight the power (and importance) of combining different measurements to break degeneracies when trying to constrain a cosmological model. Zoom link: https://cern.zoom.us/j/63414047463?pwd=OAuE7B2AAjxU3ZPNr43sxuxdku3xQU.1
Wednesday, 8 April 2026
Thursday, 9 April 2026
Friday, 10 April 2026
Saturday, 11 April 2026
Sunday, 12 April 2026
Monday, 13 April 2026
Tuesday, 14 April 2026
Wednesday, 15 April 2026
Thursday, 16 April 2026
11:00
Co-propagating dielectric laser accelerators for compact high-gradient particle acceleration
-
Giuseppe Torrisi
(
Istituto Nazionale di Fisica Nucleare
)
Co-propagating dielectric laser accelerators for compact high-gradient particle acceleration
Giuseppe Torrisi
(
Istituto Nazionale di Fisica Nucleare
)
11:00 - 12:00
Room: Room 412 C - Ferrara
Dielectric Laser Accelerators (DLAs) are a promising approach for compact particle acceleration based on infrared lasers interacting with nanostructured dielectric materials. Operating at optical frequencies, these structures can sustain accelerating gradients well beyond the limits of conventional radio-frequency accelerators while enabling a drastic reduction of accelerator dimensions. Recent developments focus on extended dielectric waveguide structures supporting co-propagating electromagnetic modes synchronized with charged particle beams. This configuration enables longer interaction lengths and improved scalability compared with conventional transverse illumination schemes. This contribution presents recent advances in the design, modeling, and experimental investigation of dielectric interaction structures for particle acceleration in both sub-relativistic and relativistic regimes. Physics-based design methodologies and figures of merit for hollow-core dielectric waveguides are discussed, together with integrated beam dynamics simulations enabling co-design of electromagnetic structures and particle acceleration. This work is carried out within the European project EPITA (WP5: laser-driven acceleration) and within the INFN CSN5 iDLA project. zoom: https://cern.zoom.us/j/65647993989?pwd=ZBbo2rTJJL2PHUEz6ETTdJeea45c4O.1
Friday, 17 April 2026
Saturday, 18 April 2026
Sunday, 19 April 2026
Monday, 20 April 2026
Tuesday, 21 April 2026
Wednesday, 22 April 2026
Thursday, 23 April 2026
Friday, 24 April 2026
Saturday, 25 April 2026
Sunday, 26 April 2026
Monday, 27 April 2026
Tuesday, 28 April 2026
11:00
Understanding the Gamma-Ray Burst Diversity with Data-Driven Methods
-
Dimple
(
U. Birmingham, UK
)
Understanding the Gamma-Ray Burst Diversity with Data-Driven Methods
Dimple
(
U. Birmingham, UK
)
11:00 - 12:00
Room: Room 412 C - Ferrara
Gamma-ray bursts (GRBs) exhibit extraordinary diversity in their light curve morphologies and spectral characteristics, reflecting the complex physics of relativistic outflows and radiation mechanisms operating under extreme conditions. Traditionally, this diversity has been reduced to a small number of phenomenological classes (e.g., long vs. short, Type I vs. Type II); however, mounting observational evidence challenges these binary classification schemes and exposes their physical limitations. In this talk, I will explore whether GRB diversity can be leveraged as a diagnostic of underlying physical processes rather than treated as observational scatter, using a data-driven framework that combines unsupervised machine learning with prompt emission pulse characteristics. I will focus in particular on ongoing efforts to interpret the feature-space clusters identified by dimensionality reduction and clustering algorithms, and to assess whether these groupings trace meaningful physical differences in jet physics, radiation mechanisms, or progenitor properties, or instead arise from degeneracies in the observational parameter space. zoom: https://cern.zoom.us/j/64371309380?pwd=bUbpQazzFgZoWUkSOmV0IhZxrvkiAZ.1
Wednesday, 29 April 2026
Thursday, 30 April 2026
Friday, 1 May 2026
Saturday, 2 May 2026
Sunday, 3 May 2026
Monday, 4 May 2026
Tuesday, 5 May 2026
Wednesday, 6 May 2026
Thursday, 7 May 2026
Friday, 8 May 2026
Saturday, 9 May 2026
Sunday, 10 May 2026
Monday, 11 May 2026
Tuesday, 12 May 2026
Wednesday, 13 May 2026
Thursday, 14 May 2026
09:00
Giornata Internazionale della Luce 2026
-
Federico Boscherini
(
DIFA - Department of Physics and Astronomy, University of Bologna
)
Donato Vincenzi
(
Dipartimento di Fisica e Scienze della Terra, UniFe
)
Giornata Internazionale della Luce 2026
Federico Boscherini
(
DIFA - Department of Physics and Astronomy, University of Bologna
)
Donato Vincenzi
(
Dipartimento di Fisica e Scienze della Terra, UniFe
)
09:00 - 13:00
Room: Room 412 C - Ferrara
9:00 -9:30 Registrazione 9:30 - 9:35 Apertura Seminario 9:35 - 10:35 **Prof. Boscherini “I sincrotroni e laser a elettroni liberi: sonde di avanguardia in fisica della materia”** 10:35 - 11:05 Pausa caffè con buffet 11:05 - 11:50 **Prof. Vincenzi “Concentratori solari a luminescenza e fotovoltaico: guidare la luce per la conversione solare“** 11:50 - 13:00 Visita ai laboratori **Lab Fotovoltaico:** Concentratori solari a luminescenza Spettroscopia di assorbimento a raggi X su elettrodi in Germanio poroso **Lab Sensori:** Sensori a stato solido, Spettroscopia infrarossa in riflettanza diffusa (DRIFT)
11:30
Making Data Speak: Data Visualization and Responsible AI
-
Carlo Zapponi
(
CISCO
)
Making Data Speak: Data Visualization and Responsible AI
Carlo Zapponi
(
CISCO
)
11:30 - 13:30
Good visualizations don't just show data, they tell a story. In this seminar, we'll cover what makes a visualization work, experiment with AI tools that can help you build better visuals faster, and develop a critical eye for where AI helps and where it misleads. Practical, hands-on, and designed for scientists who want to do more with their data.
Friday, 15 May 2026
Saturday, 16 May 2026
Sunday, 17 May 2026
Monday, 18 May 2026
Tuesday, 19 May 2026
14:30
Bio-Inspired Artificial Spider Silk Fibers: Promise and Pitfalls in Sustainable Textile Development
-
Gabriele Greco
(
Pavia University
)
Bio-Inspired Artificial Spider Silk Fibers: Promise and Pitfalls in Sustainable Textile Development
Gabriele Greco
(
Pavia University
)
14:30 - 15:30
Room: Room 412 C - Ferrara
The global reliance on petroleum-based fibers has created a major sustainability challenge, particularly within the fashion industry, where durability and low cost often come at significant environmental expense. Natural alternatives such as silkworm silk offer partial solutions, yet their current production systems remain resource-intensive and difficult to scale sustainably. Spider silk, renowned for its exceptional mechanical properties, provides a compelling biological model; however, farming spiders is inherently impractical, limiting its direct industrial application. Recent advances in bio-inspired materials science are opening new pathways through the development of synthetic bio-based fibers that emulate the structure and performance of natural silks while enabling scalable production. This seminar will present an overview of the latest progress in the design and processing of bio-inspired spider silk fibers, highlighting how interdisciplinary approaches are driving the transition toward truly sustainable textile materials. About the speaker: Gabriele Greco received his bachelor and master degree in physics from the University of Ferrara and his Ph.D. in mechanical engineering from the University of Trento. He is currently a lecturer of “Experimental Mechanics” and post-doctoral researcher at the University of Pavia and his research interests focus on the mechanics of protein-based materials, particularly focusing on artificial silk structures. His passion for spiders led him to co-found the Italian Society of Arachnology - Aracnofilia, in which he serves as vice president. Zoom: https://cern.zoom.us/j/69974978314?pwd=IfI7uTTsL73OiNSbzZvXDcuGN4Hdbp.1
Wednesday, 20 May 2026
Thursday, 21 May 2026
Friday, 22 May 2026
Saturday, 23 May 2026
Sunday, 24 May 2026
Monday, 25 May 2026
Tuesday, 26 May 2026
Wednesday, 27 May 2026
Thursday, 28 May 2026
Friday, 29 May 2026
Saturday, 30 May 2026
Sunday, 31 May 2026
Monday, 1 June 2026
Tuesday, 2 June 2026
Wednesday, 3 June 2026
Thursday, 4 June 2026
Friday, 5 June 2026
Saturday, 6 June 2026
Sunday, 7 June 2026
Monday, 8 June 2026
Tuesday, 9 June 2026
Wednesday, 10 June 2026
Thursday, 11 June 2026
Friday, 12 June 2026
Saturday, 13 June 2026
Sunday, 14 June 2026
Monday, 15 June 2026
Tuesday, 16 June 2026
Wednesday, 17 June 2026
Thursday, 18 June 2026
Friday, 19 June 2026
Saturday, 20 June 2026
Sunday, 21 June 2026
Monday, 22 June 2026
Tuesday, 23 June 2026
Wednesday, 24 June 2026
Thursday, 25 June 2026
Friday, 26 June 2026
Saturday, 27 June 2026
Sunday, 28 June 2026
Monday, 29 June 2026
Tuesday, 30 June 2026
Wednesday, 1 July 2026
Thursday, 2 July 2026
Friday, 3 July 2026
Saturday, 4 July 2026
Sunday, 5 July 2026
Monday, 6 July 2026
Tuesday, 7 July 2026
Wednesday, 8 July 2026
Thursday, 9 July 2026
Friday, 10 July 2026
Saturday, 11 July 2026
Sunday, 12 July 2026
Monday, 13 July 2026
Tuesday, 14 July 2026
Wednesday, 15 July 2026
Thursday, 16 July 2026
Friday, 17 July 2026
Saturday, 18 July 2026
Sunday, 19 July 2026
Monday, 20 July 2026
Tuesday, 21 July 2026
Wednesday, 22 July 2026
Thursday, 23 July 2026
Friday, 24 July 2026
Saturday, 25 July 2026
Sunday, 26 July 2026
Monday, 27 July 2026
Tuesday, 28 July 2026
Wednesday, 29 July 2026
Thursday, 30 July 2026
Friday, 31 July 2026
Saturday, 1 August 2026
Sunday, 2 August 2026
Monday, 3 August 2026
Tuesday, 4 August 2026
Wednesday, 5 August 2026
Thursday, 6 August 2026
Friday, 7 August 2026
Saturday, 8 August 2026
Sunday, 9 August 2026
Monday, 10 August 2026
Tuesday, 11 August 2026
Wednesday, 12 August 2026
Thursday, 13 August 2026
Friday, 14 August 2026
Saturday, 15 August 2026
Sunday, 16 August 2026
Monday, 17 August 2026
Tuesday, 18 August 2026
Wednesday, 19 August 2026
Thursday, 20 August 2026
Friday, 21 August 2026
Saturday, 22 August 2026
Sunday, 23 August 2026
Monday, 24 August 2026
Tuesday, 25 August 2026
Wednesday, 26 August 2026
Thursday, 27 August 2026
Friday, 28 August 2026
Saturday, 29 August 2026
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Monday, 31 August 2026
Tuesday, 1 September 2026
Wednesday, 2 September 2026
Thursday, 3 September 2026
Friday, 4 September 2026
Saturday, 5 September 2026
Sunday, 6 September 2026
Monday, 7 September 2026
Tuesday, 8 September 2026
Wednesday, 9 September 2026
Thursday, 10 September 2026
Friday, 11 September 2026
Saturday, 12 September 2026
Sunday, 13 September 2026
Monday, 14 September 2026
Tuesday, 15 September 2026
Wednesday, 16 September 2026
Thursday, 17 September 2026
Friday, 18 September 2026
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Monday, 21 September 2026
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Wednesday, 23 September 2026
Thursday, 24 September 2026
Friday, 25 September 2026
Saturday, 26 September 2026
Sunday, 27 September 2026
Monday, 28 September 2026
Tuesday, 29 September 2026
Wednesday, 30 September 2026
Thursday, 1 October 2026
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Saturday, 3 October 2026
Sunday, 4 October 2026
Monday, 5 October 2026
Tuesday, 6 October 2026
Wednesday, 7 October 2026
Thursday, 8 October 2026
Friday, 9 October 2026
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Sunday, 11 October 2026
Monday, 12 October 2026
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Wednesday, 14 October 2026
Thursday, 15 October 2026
Friday, 16 October 2026
Saturday, 17 October 2026
Sunday, 18 October 2026
Monday, 19 October 2026
Tuesday, 20 October 2026
Wednesday, 21 October 2026
Thursday, 22 October 2026
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Sunday, 25 October 2026
Monday, 26 October 2026
Tuesday, 27 October 2026
Wednesday, 28 October 2026
Thursday, 29 October 2026
Friday, 30 October 2026
Saturday, 31 October 2026
Sunday, 1 November 2026
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Tuesday, 1 December 2026
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