Tag Archives: Evento scientifico

Speaker: Giorgio Dho (Istituto Nazionale di Fisica Nucleare) X-ray polarimetry is an observational technique with the potential to enrich our understanding of high-energy astrophysics by enabling the measurement of the polarization of X-rays emitted by exotic cosmic phenomena such as black holes, neutron stars, Gamma-Ray Bursts and more. This technique provides crucial insights into the magnetic field geometries and intensities, and emission mechanisms of these sources, offering valuable information that could improve the current knowledge of these astrophysical objects significantly. Currently, the IXPE space observatory, which features a photoelectric polarimeter with an active volume of 6.75 cm3, is the only instrument providing X-ray polarimetric measurements. The PRIN project “HypeX: High Yield Polarimetry Experiment in X-rays”, developed by a collaboration of GSSI, INFN and INAF researchers, aims to apply more modern experimental techniques for applications in X-ray polarization measurements in the energy range between 10 and 40 keV. One branch of the project, GPD3D, builds on the IXPE detector concept, a Time Projection Chamber (TPC) with GEM-based amplification stage. The goal is to achieve 3D track reconstruction and better polarimetric performances by employing more advanced readout and amplification systems, namely an InGrid structure readout by TimePix3 chip. On the other hand, the Xray-CMOS subproject inherits the knowhow and detector concept from the CYGNO/INITIUM directional dark matter experiment optimizing it to this physics search. The technology, a TPC with triple-GEM amplification stage and optical readout exploiting the sensitivity and granularity of sCMOS cameras and PMTs, aims to achieve 3D reconstruction and an …

Speaker: Giuseppe Gagliardi (Istituto Nazionale di Fisica Nucleare) The FNAL collaboration has measured the value of the muon anomalous magnetic moment, achieving an unprecedented precision of 0.2 ppm. From the theoretical perspective, it is crucial to match this experimentalprecision. The most challenging part of the theoretical calculation comes fromthe leading hadronic vacuum polarization (HVP) contribution Undefined control sequence \rmHVP, which must be determined with subpercent precision. In this seminar, I will review the latest lattice QCD results for, as well as for the subleading hadronic light-by-lightcontribution, and discuss the phenomenological impact of these results.

Speaker: Giacomo Ferrante (Montpellier University) Due to the infamous quadratic sensitivity of their masses to the UV scale, it is notoriously difficult to realise models where elementary scalar fields are light. Accidentally light scalars provide us with an interesting alternative to the wellknown cases of Nambu-Goldstone bosons (NGBs) and pseudo-NGBs. In models with spontaneous symmetry breaking by scalar fields in large group representations, we observe that some of the scalar masses can be loop-suppressed, even though there is no obvious symmetry argument preventing them from being generated at the tree-level. I will present the most minimal model, the SU(2) five-plet, with such accidentally light scalars, featuring compact tree-level flat directions lifted by loop corrections. I will sketch some potential applications, focusing, in particular, on constructing a model of hybrid inflation where the inflaton is an accidentally light scalar. This provides a robust realisation of hybrid inflation where the potential is naturally flat and protected from radiative corrections. At the end of inflation, tachyonic instability leads to the production of gravitational waves which, for a low inflationary scale, might be detected by upcoming experiments. Simple variations of the model can give rise to topological defects, such as unstable domain walls. Their dynamics produces a stochastic gravitational-wave background, which can be compatible with the recent detection by pulsar timing arrays.

Speaker: Kristjan Müürsepp (NICPB, Tallinn, Estonia) A pseudo Nambu-Goldstone boson (PNGB) coupled to a confining gauge group via an anomalous  term is characterised, during the confining phase transition, by a temperature dependent mass. I will study the possibility that a PNGB  coupled to a hidden gauge group  undergoing confinement  at a temperature different from the QCD  confining temperature could hit a level crossing with the QCD axion. This can  trigger axion-dark axion conversion. After describing the dynamics of the two axion system, I will address possible applications in cosmology.

Speaker: Oton Vazquez Doce (Istituto Nazionale di Fisica Nucleare) The study of three- and many-body dynamics has been a long-standing goal in nuclear physics, particularly for understanding the structure of light nuclei and describing neutron-rich and dense nuclear matter. In this seminar, a new experimental method to study three-body nuclear systems by measuring correlations in the momentum space of deuteron-hadron pairs produced in proton-proton collisions at the LHC is presented. The ALICE Collaboration has performed measurements of the Kaon-deuteron and proton-deuteron correlations analyzing high-multiplicity proton-proton collisions at sqrt(s) = 13 TeV [1]. The correlation functions are compared with effective two-body calculations anchored to results from Kaon-deuteron and proton-deuteron scattering experiments that provide an excellent description of the measured Kaon deuteron correlation but fail to describe the proton-deuteron system. This discrepancy can only be resolved by performing a full three-body calculation that accounts for the underlying three-nucleon dynamics. The analysis demonstrates that nucleons are the explicit degrees of freedom also in the correlations among light nuclei produced at short distances in hadronic collisions and opens the possibility of investigating the effect of genuine many-body nuclear interactions at the LHC in the future, including systems with strangeness and charm. [1] ALICE Collaboration, Phys. Rev. X 14, 031051 (2024)

This workshop will focus on the continuing development of the scientific case for a 22 GeV upgrade to CEBAF made possible by recent novel advances in accelerator technology. CEBAF’s envisioned capabilities, at the highest luminosities, will enable exciting opportunities that give scientists the full suite of tools necessary to comprehensively understand how QCD builds hadronic matter in the valence region. Through this workshop, JLab and its user community will continue to build the science case with descriptions and concrete projections for experiments that would become possible with an upgrade. We encourage our users and others interested to submit talks and ideas on the scientific topics listed below. Physics Topics: Charmed and light hadron spectroscopy Structure of hadrons: Form Factors, Parton Distribution Functions, TMDs, GPDs, Fragmentation Functions, Fracture Functions QCD in Nuclei and associated Nuclear Modifications and Dynamics Low energy tests of the Standard Model and physics beyond the Standard Model

EuPRAXIA@SPARC_LAB is a cutting-edge research project that will be realized in the INFN Frascati National Laboratories in Italy, focusing on advanced accelerator technologies. It is part of the broader EuPRAXIA initiative, aimed at developing the world’s first plasma-based accelerator with user applications. Given the advance in the project development, we are focusing our effort on the potentiality of the new facility in a wide scientific perspective, including FEL applications, but extending to other fields in which our photon and particle sources can contribute. To this end, LNF is organizing a Workshop on “Fundamental research and applications with the EuPRAXIA facility at LNF”, to be held at Laboratori Nazionali di Frascati of INFN on December 4-6, 2024. The workshop will be articulated in three sessions. The first session will be devoted to the presentation of the EuAPS and EuPRAXIA@SPARC_LAB facilities, aimed at introducing the characteristics and peculiarities of the different sources that will be available in the next years in Frascati. The second session will explore a possible research program in the field of fundamental physics. The different beams that the facility will provide will allow to explore different areas of physical research, from nuclear processes (such as beta decay in plasma, fusion reactions among light nuclei in the laser-induced plasma, laser vs ECR induced plasma applications and potentialities for nuclear physics), to QED measurements and laboratory astrophysics. The third session will be devoted to photon science with FEL and betatron sources, such as high-resolution imaging and spectroscopy, enabling breakthroughs in …

Speaker: Vsevolod Chestnov (Istituto Nazionale di Fisica Nucleare) The percent-level precision achieved by experiments at the LargeHadron Collider demands theoretical predictions of comparable accuracy, necessitating higher-order perturbative corrections to scattering amplitudes. Traditionally, these corrections are computed by reducing the Feynman integralexpansion of an amplitude to a finite basis of linearly independent elements, followed by numerical evaluation. However, multi-scale processes posesignificant computational challenges, motivating the development ofcomplementary approaches. In this talk, I will review recent advances in Feynman integral calculus, highlighting mathematical techniques rooted in algebraic geometry, finite fieldreconstruction, and twisted cohomology theory. I will also discuss alternativereduction strategies based on the so-called “transverse integration identities”and explore how these innovations can enhance traditional computational methods to address the demands of modern precision physics.

Speaker: Pavel Fileviez Perez (Case Western Reserve University) The different theories for neutrino masses are discussed. We show possible connections between the origin of neutrino masses and the properties of dark matter candidates in new theories for physics beyond the Standard Model. We discuss minimal gauge theories for neutrino masses where the neutrinos are predicted to be Dirac or Majorana fermions. We find that the upper bound on the effective number of relativistic species provides a strong constraint in the scenarios with Dirac neutrinos. In the context of theories where the lepton number is a local gauge symmetry spontaneously broken at the low scale, the existence of dark matter is predicted from the condition of anomaly cancellation. We show that we could test simple gauge theories for neutrino masses at current or future experiments.

Un lungo cammino: le nuove sfide della scienza aperta Secondo convegno nazionale del gruppo di lavoro Open Science della CoPER

 Aula Bruno Touschek – Laboratori Nazionali di Frascati INFN 27 Novembre, ore 14.00 -18.30
- 28 Novembre, ore 8.30 – 14.00 Pagina web https://agenda.infn.it/e/ConvegnoOpenscienceCoPER2024 Organizzazione Locale: Lia Sabatini, Irene Piergentili, Davide Cirillo, Antonino Cupellini, Roberto Campagnola, Giulia Chiaraluce (INFN – LNF) Giorgia Migliorelli, Sara Santorsa (CNR) Comitato Scientifico: Stefano Bianco (INFN), Anna Grazia Chiodetti (INGV),  Mario Locati (INGV), Giovanni De Simone (CNR), Roberta Vigni (ISPRA), Paolo Valente (INFN) Il gruppo di lavoro Open Science della Consulta dei Presidenti degli Enti pubblici di ricerca (CoPER) – in collaborazione con il gruppo di lavoro Valutazione – organizza il suo secondo convegno nelle giornate del 27  e 28 novembre 2024 a Frascati presso i Laboratori Nazionali di Frascati dell’Istituto Nazionale di Fisica Nucleare.  L’obiettivo del convegno è sia di fare il punto sul lavoro svolto e sulle prospettive a breve e medio termine, sia di realizzare collegamenti  esterni a CoPER per stabilire o rafforzare sinergie nel complesso mondo della Scienza Aperta. Il gdl Open Science nasce nel dicembre 2021  per favorire il coordinamento sulla tematica della scienza aperta tra gli enti di ricerca e tra gli enti di ricerca e le università rappresentate dalla Conferenza dei rettori delle università italiane (CRUI).  Il programma dei lavori adotta gli assi di intervento individuati dal Piano Nazionale Scienza Aperta – PNSA (accesso alle pubblicazioni scientifiche, valutazione della ricerca, Open Data). Il convegno prevede una sessione  il pomeriggio del 27 novembre ed una sessione  …