Calendar

Nov
28
Mar
Detecting Muonphilic Scalars at Neutrino Facilities (Dr. Duncan Rocha, University of Chicago) @ Aula 603
Nov 28@2:00 pm–4:00 pm

Neutrino experiments such as MiniBooNE and MicroBooNE produce a large quantity of secondary muons. This provides an
interesting opportunity to search for BSM particles that may
preferentially couple to the muon. In my talk, I will present a
scenario where neutrino experiments are particularly suitable for
studying BSM models, and show how these experiments have excluded
certain regions where a BSM scalar could explain the g-2 anomaly.

Nov
29
Mer
Equivariant localization for AdS/CFT (Pietro Benetti Genolini, Université de Genève) @ Aula 500 e online
Nov 29@2:30 pm–3:30 pm

Seminario di Fisica Teorica-

On a space with a group action, the equivariant localization theorem allows one to compute integrals using only local information. We shall see how this can be applied to AdS/CFT to compute various supersymmetric gravity observables without solving the equations of motion, using just topological information.

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Dic
6
Mer
Testing the assumptions of LCDM (Matteo Martinelli, INAF – OAR) @ Aula 500 e online
Dic 6@2:30 pm–3:30 pm

Seminario di Fisica Teorica-

The standard cosmological model (LCDM) has shown a great ability to explain cosmological observations throughout the past 3 decades. Despite this, several of its component are still a mystery from the theoretical point of view; together with the observational tensions recently found between different measurements of its parameters, this motivates the search for alternative models or, at least, a thorough testing of LCDM.
In this talk, I will focus mostly on tests of one of the crucial assumptions done in cosmology, i.e. that General Relativity is a good description of gravity at cosmological scale, showing recent constraints and how upcoming surveys might improve our knowledge.
In addition to this I will also show results on other more fundamental assumptions, namely the validity of the Distance Duality Relation and on the possible variation of the fine-structure constant. Finally, I will also briefly summarize how new cosmological observables might shed new light on the dark component of the standard cosmological model.

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Dic
13
Mer
Dynamical mass generation and boundary phase transitions in AdS (Coppetti, Oxford University) @ Aula 500 e online
Dic 13@2:00 pm–3:00 pm

Seminario di Fisica Teorica-

Abstract: I will review the old idea of studying QFTs on AdS background to control strong coupling effects. We study dynamical mass generation in some 2d asymptotically free theories in AdS backgrounds. At weak coupling a Dirichlet boundary condition ensures that the bulk field is exactly massless.

At strong coupling a marginal boundary singlet operator appears, destabilizing the BCFT and leading to a boundary phase transition. The endpoint of this boundary flow allows for a massive bulk phase and interpolates with the flat spacetime physics. We conjecture that such a phenomenon is also responsible for confinment in 4d gauge theories on AdS background.

Based on work to appear with Lorenzo di Pietro, Shota Komatsu and Ziming Ji.

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Dic
21
Gio
Fracton gravity from spacetime dipole symmetry (Dr Alessio Caddeo, Oviedo U.) @ Aula 500 e online
Dic 21@2:30 pm–3:30 pm

Seminario di Fisica Torica

In this talk, I will present a fracton gravity gauge theory based on a covariant version of the monopole-dipole-momentum algebra. In the presence of a suitable background field, the theory includes a massive two-form and a massless symmetric two-index tensor. The latter transforms only under longitudinal diffeomorphisms, making the massless sector similar to linearized gravity, but with additional modes of lower spin. I will show that the theory can be consistently coupled to a curved background metric and discuss its possible interaction terms with itself and with matter. In addition, I will present a map between solutions of linearized gravity in Kerr-Schild form and solutions of fracton gravity coupled to matter.

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Gen
17
Mer
Positivity Constraints on Lorentz-breaking EFTs (Paolo Criminelli, ICTP) @ Aula 500 e online
Gen 17@2:30 pm–3:30 pm

Seminario di Fisica Teorica-

The coefficients of the operators of an effective field theory (EFT) are constrained to satisfy certain inequalities, under the (mild) assumption that the UV completion satisfies general requirements of causality and unitarity. We begin the extension of these ideas to theories where the Lorentz symmetry is spontaneously broken, as it happens in cosmology and condensed matter physics. Constraints are derived using dispersive arguments for the 2-point function of conserved currents and of the stress-energy tensor.

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Feb
27
Mar
Physics in Wonderland: esplorando i segreti dell’universo (Anna Marini e Bianca Bottino) @ Aula Magna DIFI
Feb 27@5:00 pm–6:30 pm

Si tratta di un evento all’interno dell’iniziativa “Un Mare di Scienza”, serie di conferenze di divulgazione scientifica organizzate dalla Scuola di Scienze Matematiche, Fisiche e Naturali.

Relatrici: Anna Marini (INFN) e Bianca Bottino (UNIGE)

I raggi cosmici sono messaggeri preziosi che ci aiutano a decifrare il nostro Universo. Attraverso la loro rivelazione possiamo captare segnali dallo spazio profondo. In questo incontro vedremo e utilizzeremo un rivelatore di raggi cosmici, partendo dai processi microscopici innescati dal passaggio dei raggi cosmici nella materia, per arrivare all’acquisizione di veri e propri segnali.

Feb
28
Mer
A History of Neutrino and its mass (Dr. Francesco Vissani LNGS Istituto Nazionale di Fisica Nucleare) @ Aula Magna
Feb 28@3:00 pm–4:00 pm

nell’ambito del workshop NuMass 2024

In this seminar, the history of the neutrino and its mass is recounted in six short chapters, with a bit of emphasis on the theoretical aspects:
1. Pauli’s proposal is presented, clarifying its significance and the context in which it arose, that of the earliest theories of the atomic nucleus.
2. The first beta-ray theory, due to Enrico Fermi, is described, clarifying its potential but also its formal and conceptual limitations.
3. Majorana’s ideas, from which the modern treatment of neutrinos and fermions in general originated, are illustrated.
4. Major advances in the next 30 years concern the existence of fermion families and the chiral structure of weak interactions, directly related to the hypothesis of neutrinos with zero mass.
5. Conceptions on the mass of neutrinos and the main ways to probe them are then summarised.
6. Prospects for development are briefly discussed in the last chapter of the story, which is the one yet to be written.

Feb
29
Gio
Odd Viscoelasticity (Prof.Piotr Surowka, Wrokaw U. of Science and Technology @ A601 e online
Feb 29@2:00 pm–3:00 pm

Seminario di Fisica Teorica

Active matter encompasses systems that are not in equilibrium, consisting of elements that either consume energy or exert work. Consequently, their macroscopic characteristics diverge significantly from those predicted by continuum field theories based on equilibrium statistical mechanics. Recent advancements in active matter research have prompted a reevaluation of the fundamental principles of materials science. This has led to the development of a novel theoretical framework known as odd(visco)elasticity. Traditional elasticity treats solids as continuous media that change shape in response to external forces. On a microscopic scale, applying force to a crystalline structure displaces its atoms, which then exert a counterforce to regain the crystal’s original configuration. However, this dynamics is fundamentally altered in active odd materials, where the response to applied forces includes not only compression or deformation but also deflection. In this presentation, I will provide an overview of the recent advancements in this field.

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Mar
6
Mer
COSMOLOGY OF THE QCD AXION: FROM THERMAL TO INFLATIONARY PRODUCTION (Alessio Notari, Universitat de Barcelona) @ Aula 501
Mar 6@2:00 pm–3:30 pm

Seminario Fisica Teorica

The axion is a hypothetical particle that could explain the absence of CP violation in QCD and has a very rich cosmological phenomenology.
In particular a population of thermally produced axions is expected to exist, in addition to a cold dark matter population. I discuss a new conservative bound on the axion mass, from production in the early universe from scattering with pions. In addition I will show that to exploit the reach of upcoming cosmological surveys, non-perturbative calculations above the QCD crossover are needed. Moreover I will also review production from other Standard Model particles (quarks, leptons).
Then, I will discuss the axion cold dark matter population, showing that its abundance depends on non-trivial evolution during primordial inflation.
Finally I will discuss the non-standard case of a heavy QCD axion, which could give rise to a detectable gravitational wave signal at Pulsar Timing Arrays or at interferometers.

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