Author Archive

Eclipses and Discoveries: in the Sun’s Shadow, the focus of a series of outreach talks in Gipuzkoa

In the run-up to this event, astrophysicist Silvia Bonoli (Ikerbasque, DIPC) and astrophysicist Mikel Falxa (DIPC) will give two talks in which they will review some of the most surprising discoveries made possible by eclipses

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Three CRM researchers take mathematics to the bars of Sabadell

On 20 May, three researchers from the Centre de Recerca Matemàtica spent the evening at two bars in Sabadell, explaining their work to anyone who turned up for a drink. They were taking part in Pint of Science Sabadell 2026, the local edition of an international festival that moves research out of the seminar room and into the pub.

Jens-Bastian Eppler and Tássio Naia, both postdoctoral researchers at the CRM, spoke in the English-language session «Big Questions, Tiny Solutions: Science Across Scales» at L’Estruch Bar. David Romero, head of the CRM’s Knowledge Transfer Unit, joined the session «Connexions invisibles» at The Wild Geese.

 

The talks

Jens-Bastian’s talk, Why the Brain Loves Categories, started from something we do without noticing: to make sense of the world, the brain sorts it. We file what we see into categories before we have time to think about it. He showed that those categories shift with the situation. Faced with an animal, the brain doesn’t always ask which species it is; often, what matters is whether it’s dangerous. The useful category depends on what you need to know at that moment.

Tássio Tássio Naia during his talk «Colorful questions and seating plans» at L’Estruch Bar, Pint of Science Sabadell 2026.

Tássio’s talk, Colorful questions and seating plans, was about how mathematics describes the relationships between things. Graphs, he explained, help us search efficiently and solve problems of arrangement. One example was the Oberwolfach problem: how to seat a group of people at several round tables, over several dinners, so that everyone ends up sitting next to everyone else exactly once.

David’s talk, «Cuando la montaña decide: cerebro, riesgo y complejidad», presented the work the CRM is doing within NeuroMunt, a cross-border European project on decision-making in the mountains. Rescues in Catalonia’s natural areas have risen by around 20% since the pandemic. Working from EEG signals and from the mathematics of complexity and dynamical systems, he described how that data can reveal something about the way the brain weighs risk and how people decide in real situations.

David Romero presenting «Cuando la montaña decide: cerebro, riesgo y complejidad» at The Wild Geese, Pint of Science Sabadell 2026.

Science in a bar tends to lean on the fields that tell easy stories, biology and physics above all. Mathematics is the rarer guest at these things. Three CRM researchers on the Sabadell bill meant it was on the menu, somewhere between the antimicrobial peptides and the energy communities. And moving research out of the seminar room and into a bar matters more than it used to: it puts science in the same room as people who would never sign up for a lecture.

 

About Pint of Science

The festival began with two neuroscientists at Imperial College London. In 2012, Michael Motskin and Praveen Paul ran an event called «Meet the Researchers», opening their labs to people living with neurodegenerative conditions such as Parkinson’s and Alzheimer’s. It worked well enough that they reversed the idea: if people will come to the lab to meet scientists, why not take the scientists to where the people already are? The first Pint of Science festival ran in May 2013, in three British cities.

By 2026, it reaches 27 countries across five continents, with Australia opening the three-day relay each May. In Spain, this was the eleventh edition: more than 1,300 researchers in 114 towns and cities, among them 29 rural areas taking part for the first time. Sabadell held its second edition, tripling its venues to three bars and putting on 43 talks, with a different language in each bar each night.

The Sabadell edition is run by a local committee, with the CRM among the collaborating institutions alongside the Universitat Autònoma de Barcelona (UAB), the Institut de Ciència de Materials de Barcelona (ICMAB-CSIC), the Institut Català de Nanociència i Nanotecnologia (ICN2), the Computer Vision Center (CVC), the ICTA-UAB and the Institut Català de Paleontologia (ICP). Full programme: pintofscience.es/events/sabadell

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Three CRM researchers take mathematics to the bars of Sabadell

Three CRM researchers take mathematics to the bars of Sabadell

On 20 May, three researchers from the Centre de Recerca Matemàtica spent the evening at two bars in Sabadell, explaining their work to anyone who turned up for a drink. They were taking part in Pint of Science Sabadell 2026, the local edition of an international…

CRM Comm

Pau Varela

CRMComm@crm.cat

 

The post Three CRM researchers take mathematics to the bars of Sabadell first appeared on Centre de Recerca Matemàtica.

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Seminar by Evangelos Afxonidis (Oviedo U. – ICTEA)

Image
seminar ICCUB
Seminar

Seminar by Evangelos Afxonidis (Oviedo U. – ICTEA)

Date
Place
Pere Pascual V5.07 Room

Abstract: TBA

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Revisiting gauge invariance and Reggeization of pion exchange

Revisiting gauge invariance and Reggeization of pion exchange

Montaña G.; Winney D.; Bibrzycki L.; Fernández-Ramírez C.; Foti G.; Hammoud N.; Mathieu V.; Perry R.J.; Pilloni A.; Rodas A.; Shastry V.; Smith W.A.; Szczepaniak A.P.
Physical Review D, Vol. 110, Num. 114012 (2024)
Article

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New constraints on gauged U1Lμ−Lτ models via Z − Z′ mixing

New constraints on gauged U1Lμ−Lτ models via Z − Z′ mixing

Asai K.; Miyao C.; Okawa S.; Tsumura K.
Journal of High Energy Physics, Vol. 2024, Num. 18 (2024)
Article

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A new method of reconstructing images of gamma-ray telescopes applied to the LST-1 of CTAO

A new method of reconstructing images of gamma-ray telescopes applied to the LST-1 of CTAO

Abe K.; Abe S.; Abhishek A.; Acero F.; Aguasca-Cabot A.; Agudo I.; Alispach C.; Crespo N.A.; Ambrosino D.; Antonelli L.A.; Aramo C.; Arbet-Engels A.; Arcaro C.; Asano K.; Aubert P.; Baktash A.; Balbo M.; Bamba A.; Larriva A.B.; Barres de Almeida U.; Barrio J.A.; Jiménez L.B.; Batkovic I.; Baxter J.; González J.B.; Bernardini E.; Medrano J.B.; Berti A.; Bezshyiko I.; Bhattacharjee P.; Bigongiari C.; Bissaldi E.; Blanch O.; Bonnoli G.; Bordas P.; Borkowski G.; Brunelli G.; Bulgarelli A.; Burelli I
Astronomy and Astrophysics, Vol. 691, Num. A328 (2024)
Article

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Measurement of (Formula presented), (Formula presented), and (Formula presented) Decay Parameters Using (Formula presented) Decays

Measurement of (Formula presented), (Formula presented), and (Formula presented) Decay Parameters Using (Formula presented) Decays

Dekkers S.; Egede U.; Fujii Y.; Hadavizadeh T.; Henderson R.D.L.; Lane J.J.; Liu F.L.; Monk M.; Song R.; Walton E.J.; Ward J.A.; Bediaga I.B.; Camargo Magalhaes P.; Cruz Torres M.; De Freitas Carneiro Da Graca U.; De Miranda J.M.; dos Reis A.C.; Falcao L.N.; Gomes A.; Massafferri A.; Santoro L.; Sundfeld D.; Torres Machado D.; Amato S.; De Paula L.; Ferreira Rodrigues F.; Gandelman M.; Hicheur A.; Lopes J.H.; Nasteva I.; Nogarolli P.; Otalora Goicochea J.M.; Polycarpo E.; Rangel M.S.; Souza De P
Physical Review Letters, Vol. 133, Num. 261804 (2024)
Article

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Euclid: High-precision imaging astrometry and photometry from Early Release Observations I. Internal kinematics of NGC 6397 by combining Euclid and Gaia data

Euclid: High-precision imaging astrometry and photometry from Early Release Observations I. Internal kinematics of NGC 6397 by combining Euclid and Gaia data

Libralato M.; Bedin L.R.; Griggio M.; Massari D.; Anderson J.; Cuillandre J.-C.; Ferguson A.M.N.; Lançon A.; Larsen S.S.; Schirmer M.; Annibali F.; Balbinot E.; Dalessandro E.; Erkal D.; Kuzma P.B.; Saifollahi T.; Verdoes Kleijn G.; Kümmel M.; Nakajima R.; Correnti M.; Battaglia G.; Altieri B.; Amara A.; Andreon S.; Baccigalupi C.; Baldi M.; Balestra A.; Bardelli S.; Basset A.; Battaglia P.; Bonino D.; Branchini E.; Brescia M.; Brinchmann J.; Caillat A.; Camera S.; Capobianco V.; Carbone C.; Car
Astronomy and Astrophysics, Vol. 692, Num. A96 (2024)
Article

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Kasner eons in Lovelock black holes

Kasner eons in Lovelock black holes

Bueno P.; Cano P.A.; Hennigar R.A.; Li M.-D.
Physical Review D, Vol. 110, Num. 124015 (2024)
Article

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Measurement of the effective leptonic weak mixing angle

Measurement of the effective leptonic weak mixing angle

Aaij R.; Abdelmotteleb A.S.W.; Abellan Beteta C.; Abudinén F.; Ackernley T.; Adefisoye A.A.; Adeva B.; Adinolfi M.; Adlarson P.; Agapopoulou C.; Aidala C.A.; Ajaltouni Z.; Akar S.; Akiba K.; Albicocco P.; Albrecht J.; Alessio F.; Alexander M.; Aliouche Z.; Alvarez Cartelle P.; Amalric R.; Amato S.; Amey J.L.; Amhis Y.; An L.; Anderlini L.; Andersson M.; Andreianov A.; Andreola P.; Andreotti M.; Andreou D.; Anelli A.; Ao D.; Archilli F.; Argenton M.; Arguedas Cuendis S.; Artamonov A.; Artuso M.;
Journal of High Energy Physics, Vol. 2024, Num. 26 (2024)
Article

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Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Neutrino mass bounds from DESI 2024 are relaxed by Planck PR4 and cosmological supernovae

Allali I.J.; Notari A.
Journal of Cosmology and Astroparticle Physics, Vol. 2024, Num. 020 (2024)
Article

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The dynamics of massive gravity

Image
The dynamics of massive gravity
Seminar

The dynamics of massive gravity

Date
Place
DAM 7.24 Seminar Room

Abstract: The premise of massive gravity is deceptively simple – adding a mass term to the graviton action. Yet it was only in 2010 that a permissible non-linear massive gravity Lagrangian, now known as the dRGT Lagrangian, was first written down. Since then, dRGT theory has generated considerable interest, but many fundamental questions about it remain unanswered. In this talk, I will review the motivations and long history of massive gravity, before moving on to discuss some of our recent progress on understanding its dynamics. We shall learn how to study the characteristics of the massive graviton, seeing that the familiar helicity-2 components remain on the usual light cone. We will then put dRGT on a computer, and marvel at the complicated things that happen when we try to model perhaps the simplest gravitational phenomenon: spherical collapse. Most of the time, the result will turn out to look very different from a standard GR black hole.

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