seminari 2024
from
Monday, January 1, 2024 (12:00 AM)
to
Monday, December 30, 2024 (2:00 AM)
Monday, January 1, 2024
Tuesday, January 2, 2024
Wednesday, January 3, 2024
Thursday, January 4, 2024
Friday, January 5, 2024
Saturday, January 6, 2024
Sunday, January 7, 2024
Monday, January 8, 2024
Tuesday, January 9, 2024
11:00 AM
Spider silks are like potatoes: so many possibilities
-
Gabriele Greco
(
Uni Trento & Swedish Uni of Agricultural Sciences
)
Spider silks are like potatoes: so many possibilities
Gabriele Greco
(
Uni Trento & Swedish Uni of Agricultural Sciences
)
11:00 AM - 12:00 PM
Room: 412C
Spiders are often reviled, but their silks and webs are commonly viewed in awe and have fascinated humankind. From raising the interest of ancient philosophers to the practical outcomes in societies, spider silks have always been part of our culture and, thus, of our scientific development. The “wow effect” for spiders and their silks initially comes from the good use that the animals make of these protein-based fibers to solve many challenges that were imposed by natural selection. How can a spider lift animals thousands of times heavier? How can spiders fly? How can spiders build structures that can even stop small birds? Nature has designed silk to be produced at environmentally friendly conditions and to have exceptional mechanical and biological properties, reasons for which spider silks have deeply been investigated in these decades for their possible applications in biomedical technology, the textile industry, and soft electronics. Thus, this diversity in materials and structural applications makes spider silks' scientific outcomes potentially infinite. This seminar aims to delve into the recent discoveries related to spider silk, and the possibility of producing this material artificially at a scale compatible with industrial production using an environmentally friendly green protocol.
Wednesday, January 10, 2024
Thursday, January 11, 2024
Friday, January 12, 2024
Saturday, January 13, 2024
Sunday, January 14, 2024
Monday, January 15, 2024
Tuesday, January 16, 2024
Wednesday, January 17, 2024
Thursday, January 18, 2024
3:00 PM
Lepton flavour violating decays into axion-like particles
-
Lorenzo Calibbi
(
Nankai University, School of Physics, P. R. China
)
Lepton flavour violating decays into axion-like particles
Lorenzo Calibbi
(
Nankai University, School of Physics, P. R. China
)
3:00 PM - 4:00 PM
Room: 412C
Pseudo Nambu-Goldstone bosons — also known as axion-like particles (ALPs) — with flavour-violating couplings to the Standard Model (SM) leptons are a consequence of spontaneously-broken global U(1) symmetries within a wide class of models. In this seminar, I will present some explicit examples where such lepton-flavour-violating (LFV) ALP scenarios are realised. A general prediction thereof is the occurrence of flavour-violating decays of SM leptons into a light axion-like particle, which would typically escape detection at experiments searching for rare muon and tau decays. I will discuss the bounds set on this exotic signature by past experiments, as well as the prospects at upcoming searches for LFV muon and tau decays. I will focus in particular on a proposal for a modified setup of the MEG II experiment that would be maximally sensitive to an ALP coupling to right-handed leptonic currents. I will also compare the sensitivity of LFV experiments to the leptonic ALP couplings with astrophysical constraints, such as bounds from stellar evolution, and with the regions of the parameter space where the ALP constitutes a dark matter candidate.
Friday, January 19, 2024
Saturday, January 20, 2024
Sunday, January 21, 2024
Monday, January 22, 2024
Tuesday, January 23, 2024
Wednesday, January 24, 2024
Thursday, January 25, 2024
Friday, January 26, 2024
Saturday, January 27, 2024
Sunday, January 28, 2024
Monday, January 29, 2024
Tuesday, January 30, 2024
Wednesday, January 31, 2024
Thursday, February 1, 2024
Friday, February 2, 2024
Saturday, February 3, 2024
Sunday, February 4, 2024
Monday, February 5, 2024
Tuesday, February 6, 2024
Wednesday, February 7, 2024
Thursday, February 8, 2024
2:00 PM
Optical polarimetry of explosive transients
-
Ferdinando Patat
(
Observing Programmes Office - Head, European Southern Observatory
)
Optical polarimetry of explosive transients
Ferdinando Patat
(
Observing Programmes Office - Head, European Southern Observatory
)
2:00 PM - 3:00 PM
Room: 412C
Polarimetry is a photon-starving technique which allows to extract geometrical information that cannot be obtained with any other method. In my seminar I will briefly review the basic concepts, present the application to explosive events (mainly on supernovae) and discuss the results obtained so far. I will also briefly go through the cases of kilonovae, other exotic transients and a recent application to the problem of the spinning axis tilt of a BH in a binary system.
Friday, February 9, 2024
Saturday, February 10, 2024
Sunday, February 11, 2024
Monday, February 12, 2024
Tuesday, February 13, 2024
Wednesday, February 14, 2024
Thursday, February 15, 2024
Friday, February 16, 2024
Saturday, February 17, 2024
Sunday, February 18, 2024
Monday, February 19, 2024
3:00 PM
Geant4 simulations of applications of oriented crystals breaking down the challenges in accelerator physics, particle physics and space science Project TRILLION
-
Alex Sytov
(
Marie Curie Fellow, UniFe
)
Geant4 simulations of applications of oriented crystals breaking down the challenges in accelerator physics, particle physics and space science Project TRILLION
Alex Sytov
(
Marie Curie Fellow, UniFe
)
3:00 PM - 4:00 PM
Room: 412C
Crystalline structure is a unique environment for strong-field QED effects involving both high-energy charged particles and photons. A small piece of crystal material aligned with the particle beam can be used as an intense source of X- and gamma-ray radiation, a positron source for future e+e- colliders, a beam manipulation instrument in accelerators and colliders, a compact crystalline calorimeter for high-energy physics experiments and gamma-ray space telescopes and a compact ultrahigh gradient plasma wake-field accelerator as well. The Marie Skłodowska-Curie Actions Global Fellowships, Project TRILLION GA n. 101032975 is dedicated to steering and radiation effects in oriented crystals and their applications implementation into Geant4. In this seminar various applications of the new Geant4 model of electromagnetic effects in oriented crystals mentioned above will be presented.
Tuesday, February 20, 2024
Wednesday, February 21, 2024
Thursday, February 22, 2024
Friday, February 23, 2024
Saturday, February 24, 2024
Sunday, February 25, 2024
Monday, February 26, 2024
Tuesday, February 27, 2024
Wednesday, February 28, 2024
Thursday, February 29, 2024
Friday, March 1, 2024
Saturday, March 2, 2024
Sunday, March 3, 2024
Monday, March 4, 2024
Tuesday, March 5, 2024
3:00 PM
Decoding solar complexity: small-scale phenomena impacting upper atmospheric processes
-
Santiago Vargas Domínguez
(
University of Colombia
)
Decoding solar complexity: small-scale phenomena impacting upper atmospheric processes
Santiago Vargas Domínguez
(
University of Colombia
)
3:00 PM - 4:00 PM
Room: 412C
Recent advancements in solar instrumentation have revolutionized our ability to study solar phenomena, particularly at small spatial scales and high temporal resolutions. These tiny features play a pivotal role as fundamental building blocks for myriad processes from the photosphere to the upper layers of the solar atmosphere. This presentation delves into observational evidence showcasing the intricate interplay between small-scale magnetic flux emergence, magnetic concentrations, and convective plasma flows in the photosphere. We use multi-wavelength time series data from ground-based and space-borne solar telescopes to elucidate the complex dynamics underlying solar activity and its implications for the broader understanding of solar phenomena.
Wednesday, March 6, 2024
Thursday, March 7, 2024
Friday, March 8, 2024
Saturday, March 9, 2024
Sunday, March 10, 2024
Monday, March 11, 2024
Tuesday, March 12, 2024
Wednesday, March 13, 2024
Thursday, March 14, 2024
Friday, March 15, 2024
Saturday, March 16, 2024
Sunday, March 17, 2024
Monday, March 18, 2024
Tuesday, March 19, 2024
Wednesday, March 20, 2024
Thursday, March 21, 2024
Friday, March 22, 2024
Saturday, March 23, 2024
Sunday, March 24, 2024
Monday, March 25, 2024
11:30 AM
Small scale CMB (and foregrounds) cosmological information.
-
Laura Salvati
(
Orsay IAS
)
Small scale CMB (and foregrounds) cosmological information.
Laura Salvati
(
Orsay IAS
)
11:30 AM - 12:30 PM
Room: C300
Analysis of CMB primary temperature and polarisation anisotropies of recent experiments provide the tightest constraints on cosmological parameters. A crucial step of this analysis is the modelling of foreground signals due to the interaction between CMB photons and structures, in their path from the last scattering surface to the observer. Foregrounds are in general modelled with simple templates, obtained e.g. from numerical simulations and at fixed cosmology. These foregrounds though contain cosmological information, as well as information on the astrophysical processes that shape the structure of the recent Universe. A proper modelling of these components can therefore lead to improvement in the general constraining power of cosmological parameters. In this talk I will focus on the modelling of the Sunyaev-Zeldovich effects (thermal and kinetic, tSZ and kSZ), able to track the hot and ionised gas distribution in the recent Universe. Adding this full modelling of tSZ and kSZ in the CMB cosmological analysis, combing Planck and SPT observations, I will show the improvement in the cosmological constraining power. I will also describe a Machine Learning approach to provide a fast and accurate evaluation of tSZ and kSZ power spectrum up to very high multipoles.
Tuesday, March 26, 2024
11:30 AM
Axion thermal production: recent advances and future challenges
-
Luca Di Luzio
(
Istituto Nazionale di Fisica Nucleare
)
Axion thermal production: recent advances and future challenges
Luca Di Luzio
(
Istituto Nazionale di Fisica Nucleare
)
11:30 AM - 12:30 PM
Room: C400
After reviewing the experimental landscape for axion searches, I will focus on axion thermal production in the early universe, highlighting the recent progresses in the calculation of the axion thermalization rate in the non-perturbative QCD regime. Additionally, I will address the critical theoretical components that are still missing for a robust prediction of the axion's thermal abundance. This understanding is crucial for evaluating the potential sensitivity of next generation CMB experiments.
Wednesday, March 27, 2024
Thursday, March 28, 2024
Friday, March 29, 2024
Saturday, March 30, 2024
Sunday, March 31, 2024
Monday, April 1, 2024
Tuesday, April 2, 2024
Wednesday, April 3, 2024
Thursday, April 4, 2024
Friday, April 5, 2024
Saturday, April 6, 2024
Sunday, April 7, 2024
Monday, April 8, 2024
Tuesday, April 9, 2024
4:00 PM
Beam Physics Research in IOTA/FAST at Fermilab
-
Giulio Stancari
(
Fermilab
)
Beam Physics Research in IOTA/FAST at Fermilab
Giulio Stancari
(
Fermilab
)
4:00 PM - 5:00 PM
Room: 412C
The Fermilab Accelerator Science and Technology (FAST) facility at Fermilab is dedicated to research and education in beam physics. It comprises a photoinjector, a superconducting electron linac and a storage ring, the Integrable Optics Test Accelerator (IOTA). Recent results include the implementation of nonlinear integrable lattices and the suppression of resonances and instabilities; the demonstration of optical stochastic cooling, which uses a particle’s radiation to finely control its dynamics; the observation of the motion of single electrons; and the measurement of the classical and quantum properties of undulator radiation. In the linac, experiments on high-efficiency gamma-ray sources and on noise in intense electron bunches are under way. The IOTA proton injector, currently under construction, will enable the program on space-charge-dominated beams. Some research areas under study are beam dynamics with electron lenses; the interplay between instabilities, space-charge, feedback systems and electron cooling; and crystalline ion beams. In this presentation, results and plans are highlighted, together with opportunities for collaboration.
Wednesday, April 10, 2024
2:30 PM
Why do we want to go beyond the Standard Model? and how?
-
Stefano Morisi
(
Università di Napoli
)
Why do we want to go beyond the Standard Model? and how?
Stefano Morisi
(
Università di Napoli
)
2:30 PM - 3:30 PM
Room: 412C
From one side gravity suggests that quantum field theories are low energy approximation of a more fundamental theory, on the other side phenomenology tell us that we need to go beyond the standard model. Neutrino physics is one of the most important motivation besides baryon asymmetry and the dark problem. In this talk I focus on the origin of neutrino mass from a model building point of view and I discuss possible way and strategy of extension. As an example I show the case where the electroweak group SU(2) x U(1) is extended to SU(3) x U(1). This model is named 331.
Thursday, April 11, 2024
Friday, April 12, 2024
Saturday, April 13, 2024
Sunday, April 14, 2024
Monday, April 15, 2024
Tuesday, April 16, 2024
11:30 AM
Reconciling HST, JWST and Planck
-
Dott.ssa Ruchika
(
Università di Roma La Sapienza
)
Reconciling HST, JWST and Planck
Dott.ssa Ruchika
(
Università di Roma La Sapienza
)
11:30 AM - 12:30 PM
Room: 412C
In the era of precision cosmology, recent observations from missions like the Planck satellite and the SH0ES team using the Hubble Space Telescope (HST) have challenged the standard model of cosmology, ΛCDM. Notably, discrepancies in the measurement of the Hubble constant from cosmic microwave background (CMB) and local measurements using Cepheids and supernovae have emerged, suggesting potential shortcomings in our understanding of cosmology. Additionally, discoveries from the James Webb Space Telescope (JWST) have unveiled a significant density of massive galaxies at high redshifts, posing further challenges to the ΛCDM. Despite conservative assumptions about galaxy formation, these findings may not align with any of the current cosmological models. I will talk about cosmological tensions utilizing most of the cosmological probes from high, low, intermediate, and local redshifts along with various proposed solutions to these cosmological tensions and highlighting their limitations compared to the ΛCDM. I will discuss about how important it is now to do critical reassessment of the basic assumptions of inverse distance ladder and standard distance ladder proposing solutions such as allowing possibility of new physics such as negative cosmological constant or G-transition hypothesis/ PLR break in cepheids. Furthermore, while assuming ΛCDM and no systematics in the current JWST results, we propose that there may be an unknown systematic error in current large angular scale CMB polarization measurements, or new physics is required to explain the discrepancy.
Wednesday, April 17, 2024
Thursday, April 18, 2024
Friday, April 19, 2024
Saturday, April 20, 2024
Sunday, April 21, 2024
Monday, April 22, 2024
Tuesday, April 23, 2024
Wednesday, April 24, 2024
Thursday, April 25, 2024
Friday, April 26, 2024
Saturday, April 27, 2024
Sunday, April 28, 2024
Monday, April 29, 2024
Tuesday, April 30, 2024
Wednesday, May 1, 2024
Thursday, May 2, 2024
Friday, May 3, 2024
Saturday, May 4, 2024
Sunday, May 5, 2024
Monday, May 6, 2024
Tuesday, May 7, 2024
Wednesday, May 8, 2024
Thursday, May 9, 2024
Friday, May 10, 2024
Saturday, May 11, 2024
Sunday, May 12, 2024
Monday, May 13, 2024
Tuesday, May 14, 2024
Wednesday, May 15, 2024
Thursday, May 16, 2024
Friday, May 17, 2024
Saturday, May 18, 2024
Sunday, May 19, 2024
Monday, May 20, 2024
Tuesday, May 21, 2024
Wednesday, May 22, 2024
Thursday, May 23, 2024
Friday, May 24, 2024
3:00 PM
An insight into the radon migration processes from geogenic sources to human health risk
-
Eleonora Benà
(
Department of Geoscience, University of Padova, Italy
)
An insight into the radon migration processes from geogenic sources to human health risk
Eleonora Benà
(
Department of Geoscience, University of Padova, Italy
)
3:00 PM - 4:00 PM
Room: 412C
Radon (222Rn) is a natural radioactive gas recognised as the main source of exposure to ionising radiation for the population. It represents a serious hazard to human health since it is considered a cancerogenic (WHO, 2009), in particular when it accumulates in indoor environments (i.e., Indoor Radon Concentration, IRC). At the European scale, the BSS Directive aims to reduce the indoor radon exposure, posing national reference levels and asking to the state member to define the so-called Radon Priority Areas (RPAs). Being Rn a natural gas, one of the main goals addressed by the geologist is to investigate the tectonic control on enhancing the geogenic radon component as a fundamental factor in radon hazard, and further radon risk assessment. In particular, the importance of the geogenic radon potential, originated by degassing processes in faulted areas, has been extensively investigated in recent years. This so-called Tectonically Enhanced Radon quantity can increase radon availability at surface and its ability to influx within buildings. Mapping the geogenic radon potential represents a crucial tool for both Rn hazard and Rn risk assessment and the first step to identify the Radon Priority Areas as required by the European regulation.
Saturday, May 25, 2024
Sunday, May 26, 2024
Monday, May 27, 2024
Tuesday, May 28, 2024
Wednesday, May 29, 2024
Thursday, May 30, 2024
Friday, May 31, 2024
Saturday, June 1, 2024
Sunday, June 2, 2024
Monday, June 3, 2024
Tuesday, June 4, 2024
Wednesday, June 5, 2024
Thursday, June 6, 2024
Friday, June 7, 2024
Saturday, June 8, 2024
Sunday, June 9, 2024
Monday, June 10, 2024
Tuesday, June 11, 2024
Wednesday, June 12, 2024
Thursday, June 13, 2024
Friday, June 14, 2024
Saturday, June 15, 2024
Sunday, June 16, 2024
Monday, June 17, 2024
Tuesday, June 18, 2024
Wednesday, June 19, 2024
Thursday, June 20, 2024
Friday, June 21, 2024
Saturday, June 22, 2024
Sunday, June 23, 2024
Monday, June 24, 2024
Tuesday, June 25, 2024
Wednesday, June 26, 2024
Thursday, June 27, 2024
2:30 PM
Geoneutrino observation: KamLAND and future plans
-
Taichi Sakai
(
Tohoku University, Research Center for Neutrino Science, Sendai (Japan)
)
Geoneutrino observation: KamLAND and future plans
Taichi Sakai
(
Tohoku University, Research Center for Neutrino Science, Sendai (Japan)
)
2:30 PM - 3:30 PM
Room: 412C
The decay of radiogenic isotopes - such as uranium, thorium, and potassium - within the Earth generates radiogenic heat, driving Earth's dynamics. These isotopes also produce geo-neutrinos (anti-electron neutrinos), which serve as the only direct means of observing Earth's internal heat content. Knowledge of the Earth's internal heat content through Geo-neutrino observations can provide significant clues to the structure of the Earth's interior. Further research could also be used to understand the evolution and composition of the Earth. KamLAND experiment is located 1000 m underground at the Kamioka mine in Gifu prefecture, Japan, and has been in operation since 2002. KamLAND experiment marked the world's first observation of geo-neutrinos in 2005. Since then, KamLAND has observed geo-neutrinos continuously with 1 kt liquid scintillator. Machine learning is currently being used and applied in a variety of fields. I am also applying machine learning to the KamLAND experiment to achieve a significant reduction in background and particle identification. This presentation will also present future plans. KamLAND2 is a detector scheduled to start in 2027 and is expected to have higher performance than the current KamLAND due to several technical updates. OBD (Ocean Bottom Detector) is a next-generation detector that is currently under development, and unlike conventional detectors, it makes observations at the bottom of the ocean. By making observations at the bottom of the ocean, Geo-neutrinos from the mantle can be observed directly without the influence of the continental crust.
Friday, June 28, 2024
Saturday, June 29, 2024
Sunday, June 30, 2024
Monday, July 1, 2024
Tuesday, July 2, 2024
Wednesday, July 3, 2024
Thursday, July 4, 2024
Friday, July 5, 2024
Saturday, July 6, 2024
Sunday, July 7, 2024
Monday, July 8, 2024
Tuesday, July 9, 2024
Wednesday, July 10, 2024
Thursday, July 11, 2024
Friday, July 12, 2024
Saturday, July 13, 2024
Sunday, July 14, 2024
Monday, July 15, 2024
11:00 AM
Cosmoglobe DR2: Global analysis of the microwave and infrared sky
-
Katrine Wehus
Cosmoglobe DR2: Global analysis of the microwave and infrared sky
Katrine Wehus
11:00 AM - 12:00 PM
Room: 412C
Two lessons learned from Planck was the importance of global analysis of instrumental, astrophysical and cosmological parameters as well as the usefulness of joint analysis of multiple datasets for component separation purposes. These lessons has been further developed into a coherent pipeline for global analysis of multiple datasets by BeyondPlanck and Cosmoglobe, which has been successfully applied to joint end-to-end analysis of raw data from Planck LFI and WMAP. The recent Cosmoglobe Data Release 2 generalizes this to the infrared spectrum, performing a reanalysis of the COBE-DIRBE raw data, supported by Planck HFI, WISE, Gaia and COBE-FIRAS. Expanding the upper frequency range of the Cosmoglobe Sky Model from 1 to 240 THz requires a drastically altered thermal dust model, as well as adding models for starlight, CII line emission and dynamical Zodical light emission. This global analysis leads to the strongest constraints on the cosmic infrared background (CIB) spectrum from DIRBE published to date. I will give an introduction to global analysis before presenting our latest results.
12:00 PM
Commander4 and OpenHFI -- massively parallel end-to-end Bayesian CMB analysis
-
Hans Kristian Eriksen
Commander4 and OpenHFI -- massively parallel end-to-end Bayesian CMB analysis
Hans Kristian Eriksen
12:00 PM - 1:00 PM
Room: 412C
I will present a recently funded Open Science ERC AdG program that aims to implement a single massively parallel end-to-end framework called "Commander4" for the joint analysis of past, present and future CMB experiments. This framework will build on the existing Commander code that was used by Planck for component separation, and subsequently generalized by the BeyondPlanck and Cosmoglobe projects to derive new state-of-the-art frequency maps for Planck LFI, WMAP and DIRBE. However, the existing code only scales well up to O(10^2) computing cores. Commander4 aims to improve this scaling to O(10^5) cores, as required for next-generation experiments such as Simons Observatory and LiteBIRD. The first application of this new code, however, will be a re-analysis of the raw uncalibrated Planck HFI time-ordered data. This work will be organized in a new collaboration called OpenHFI, as part of the larger Cosmoglobe effort. All interested parties are warmly invited to join this work, both on the Commander4 framework itself and Planck HFI.
Tuesday, July 16, 2024
Wednesday, July 17, 2024
Thursday, July 18, 2024
Friday, July 19, 2024
Saturday, July 20, 2024
Sunday, July 21, 2024
Monday, July 22, 2024
Tuesday, July 23, 2024
Wednesday, July 24, 2024
Thursday, July 25, 2024
Friday, July 26, 2024
Saturday, July 27, 2024
Sunday, July 28, 2024
Monday, July 29, 2024
Tuesday, July 30, 2024
Wednesday, July 31, 2024
Thursday, August 1, 2024
Friday, August 2, 2024
Saturday, August 3, 2024
Sunday, August 4, 2024
Monday, August 5, 2024
Tuesday, August 6, 2024
Wednesday, August 7, 2024
Thursday, August 8, 2024
Friday, August 9, 2024
Saturday, August 10, 2024
Sunday, August 11, 2024
Monday, August 12, 2024
Tuesday, August 13, 2024
Wednesday, August 14, 2024
Thursday, August 15, 2024
Friday, August 16, 2024
Saturday, August 17, 2024
Sunday, August 18, 2024
Monday, August 19, 2024
Tuesday, August 20, 2024
Wednesday, August 21, 2024
Thursday, August 22, 2024
Friday, August 23, 2024
Saturday, August 24, 2024
Sunday, August 25, 2024
Monday, August 26, 2024
Tuesday, August 27, 2024
Wednesday, August 28, 2024
Thursday, August 29, 2024
Friday, August 30, 2024
Saturday, August 31, 2024
Sunday, September 1, 2024
Monday, September 2, 2024
Tuesday, September 3, 2024
Wednesday, September 4, 2024
Thursday, September 5, 2024
Friday, September 6, 2024
Saturday, September 7, 2024
Sunday, September 8, 2024
Monday, September 9, 2024
Tuesday, September 10, 2024
Wednesday, September 11, 2024
Thursday, September 12, 2024
Friday, September 13, 2024
Saturday, September 14, 2024
Sunday, September 15, 2024
Monday, September 16, 2024
Tuesday, September 17, 2024
Wednesday, September 18, 2024
Thursday, September 19, 2024
Friday, September 20, 2024
Saturday, September 21, 2024
Sunday, September 22, 2024
Monday, September 23, 2024
Tuesday, September 24, 2024
Wednesday, September 25, 2024
Thursday, September 26, 2024
Friday, September 27, 2024
Saturday, September 28, 2024
Sunday, September 29, 2024
Monday, September 30, 2024
12:30 PM
Presentazione del progetto "Einstein Telescope" a Ferrara
Presentazione del progetto "Einstein Telescope" a Ferrara
12:30 PM - 5:30 PM
Room: 412C
Tuesday, October 1, 2024
Wednesday, October 2, 2024
Thursday, October 3, 2024
Friday, October 4, 2024
Saturday, October 5, 2024
Sunday, October 6, 2024
Monday, October 7, 2024
Tuesday, October 8, 2024
Wednesday, October 9, 2024
Thursday, October 10, 2024
Friday, October 11, 2024
Saturday, October 12, 2024
Sunday, October 13, 2024
Monday, October 14, 2024
Tuesday, October 15, 2024
Wednesday, October 16, 2024
Thursday, October 17, 2024
Friday, October 18, 2024
Saturday, October 19, 2024
Sunday, October 20, 2024
Monday, October 21, 2024
Tuesday, October 22, 2024
11:30 AM
PTOLEMY: capturing relic neutrinos to study the first second of the Universe
-
Marcello Messina
(
Istituto Nazionale di Fisica Nucleare
)
PTOLEMY: capturing relic neutrinos to study the first second of the Universe
Marcello Messina
(
Istituto Nazionale di Fisica Nucleare
)
11:30 AM - 12:30 PM
Room: 412C
The Universe has expanded significantly since the early thermal epoch known as the neutrino decoupling, one second after the start. We have evidence of this expansion in many forms: the Hubble Expansion, the dim afterglow of the hot plasma epoch (Cosmic Microwave Background) and the abundances of light elements (Big Bang Nucleosynthesis). The epoch of neutrino decoupling produced a fourth pillar of confirmation – the Cosmic Neutrino Background (CNB). In our current understanding, the CNB was created in the first second after elementary particles spontaneously filled the void of the early Universe. Recent experimental advances open up new opportunities to directly detect the CNB through the process of neutrino capture on tritium, an achievement which would profoundly extend the sensitivity of precision cosmology data. PTOLEMY, an experiment at the Gran Sasso National Laboratory in Italy, is a novel method of 2D target surfaces, fabricated from graphene, that forms a basis for a large-scale relic neutrino detector. Recent PTOLEMY publications [1,2] describe the underlying technique for achieving CNB sensitivity and redefines the future direction of neutrino mass measurements. The discussion of PTOLEMY focusses on experimental challenges, recent developments and the path forward to discovery sensitivity. References: 1) M.G. Betti et al., "A Design for an Electromagnetic Filter for Precision Energy Measurements at the Tritium Endpoint”, Progress in Particle and Nuclear Physics, 106, (2019) 120-131 2) M.G. Betti et al., "Neutrino physics with the PTOLEMY project”, Journal of Cosmology and Astroparticle Physics, 07, (2019) 047,
Wednesday, October 23, 2024
Thursday, October 24, 2024
Friday, October 25, 2024
Saturday, October 26, 2024
Sunday, October 27, 2024
Monday, October 28, 2024
Tuesday, October 29, 2024
Wednesday, October 30, 2024
Thursday, October 31, 2024
Friday, November 1, 2024
Saturday, November 2, 2024
Sunday, November 3, 2024
Monday, November 4, 2024
11:30 AM
Detecting gravitational waves from inflation with LISA
-
Matteo Braglia
(
New York University
)
Detecting gravitational waves from inflation with LISA
Matteo Braglia
(
New York University
)
11:30 AM - 12:30 PM
Room: 412C
Inflationary mechanisms beyond the standard single-field slow-roll paradigm may give rise to Stochastic Gravitational Wave Backgrounds (SGWB) within the sensitivity range of the LISA satellite. This talk, a result of collaboration within the LISA Cosmology Working Group, delves into the potential of LISA in scrutinizing Early Universe Physics. Using a recently developed data analysis pipeline, I will present forecast constraints on the model parameters and discuss the implications of these forecasts for inflationary model builders. In passing, I will also discuss the impact that a large SGWB, which acts as an extra source of noise for LISA, may have on the detection of single events from binaries of Massive and Stellar Origin Black Holes, as well as Galactic White Dwarfs.
Tuesday, November 5, 2024
Wednesday, November 6, 2024
Thursday, November 7, 2024
Friday, November 8, 2024
Saturday, November 9, 2024
Sunday, November 10, 2024
Monday, November 11, 2024
Tuesday, November 12, 2024
Wednesday, November 13, 2024
Thursday, November 14, 2024
3:30 PM
Free-Streaming Neutrinos in the Early Universe
-
Benjamin Wallisch
(
Stockholm University
)
Free-Streaming Neutrinos in the Early Universe
Benjamin Wallisch
(
Stockholm University
)
3:30 PM - 4:30 PM
Room: 412C
Standard Model neutrinos decoupled from the primordial plasma about one second after the big bang and have been free-streaming through the cosmos ever since. This leaves a subtle imprint in the baryon acoustic oscillations as observed in the cosmic microwave background (CMB) and large-scale structure (LSS) of the universe. Through careful theoretical considerations of the underlying physics and observables, we have been able to extract and measure the neutrino-induced phase shift in current CMB and LSS observations. In this talk, I will present the theoretical background, new data analyses and forecasts for the free-streaming nature of neutrinos, and discuss some implications for physics beyond the Standard Model.
Friday, November 15, 2024
2:30 PM
Can an electron emit a photon of energy larger than its own?
-
Luca Serafini
(
Istituto Nazionale di Fisica Nucleare
)
Can an electron emit a photon of energy larger than its own?
Luca Serafini
(
Istituto Nazionale di Fisica Nucleare
)
2:30 PM - 3:30 PM
Room: 412C
The newly discovered effect of Full Inverse Compton Scattering has shown several implications to unexpected phenomena, like the achievement of extremely high accelerations with electrons coming to a sudden stop from relativistic velocities, therefore showing potentialities of detecting Unruh radiation, and opening a portal towards quantum gravity, and like the emission of photons with energy larger than that of the emitting electron, in apparent violation of energy conservation. We will discuss these new findings with an eye at the historical development, throughout the last century, in the understanding of QED electron-photon interactions, from the nuclear bomb development to the first studies on cosmic rays, to the development of modern Inverse Compton Scattering advanced sources of X/gamma rays. Full Inverse Compton Scattering can have significant impacts also in other fields like plasma physics, with the capability of trapping electrons (positrons) in magnetic bottles, with the spectral purification of broadband gamma ray photon beams, and with several possibile implications in the field of gamma ray cosmic sources. Ref. https://doi.org/10.1016/j.nima.2024.169964
Saturday, November 16, 2024
Sunday, November 17, 2024
Monday, November 18, 2024
Tuesday, November 19, 2024
Wednesday, November 20, 2024
Thursday, November 21, 2024
Friday, November 22, 2024
Saturday, November 23, 2024
Sunday, November 24, 2024
Monday, November 25, 2024
2:30 PM
Pushing the Limits of Dark Matter Detection: New Insights from the XENONnT Experiment
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Giovanni Volta
(
Max-Planck-Institut fur Kernphysik, Heidelberg, Germany
)
Pushing the Limits of Dark Matter Detection: New Insights from the XENONnT Experiment
Giovanni Volta
(
Max-Planck-Institut fur Kernphysik, Heidelberg, Germany
)
2:30 PM - 3:30 PM
Room: 412C
Astrophysical and cosmological observations suggest the presence of a massive, non-luminous, non-relativistic, and non-baryonic dark matter component in the Universe. A well-motivated class of DM candidates is weakly interacting massive particles. Direct detection searches for WIMPs, with masses ranging from a few GeV/c² to tens of TeV/c², have been conducted using liquid xenon time projection chambers. These searches have yielded the most stringent limits to date on elastic spin-independent WIMP-nucleon cross-sections. In this context, the multi-staged XENON program at INFN Laboratori Nazionali del Gran Sasso aims to detect dark matter using two-phase liquid xenon time projection chambers of increasing size and sensitivity. The XENONnT experiment is the latest detector in the program, designed as an upgrade to its predecessor, XENON1T. It features an active target of 5.9 tonnes of cryogenic liquid xenon (with a total mass of 8.5 tonnes in the cryostat), along with many other novel systems (e.g., Radon background reduction and liquid purification). This seminar will focus on the recent achievements of the XENON experiment, presenting the WIMP search results and highlighting the experiment's extensive physics reach.
Tuesday, November 26, 2024
Wednesday, November 27, 2024
Thursday, November 28, 2024
Friday, November 29, 2024
Saturday, November 30, 2024
Sunday, December 1, 2024
Monday, December 2, 2024
Tuesday, December 3, 2024
3:00 PM
Introduction to laser diodes - 1
-
Massimo Vanzi
(
Istituto di Microelettronica e Microsistemi del CNR
)
Introduction to laser diodes - 1
Massimo Vanzi
(
Istituto di Microelettronica e Microsistemi del CNR
)
3:00 PM - 4:00 PM
Room: 412C
I seminari sono rivolti a studenti della laurea in Fisica e a studenti del dottorato di ricerca per illustrare i principi, la tecnologia costruttiva e il funzionamento di diodi ad emissione di luce laser. Verrà illustrata la modalità di fabbricazione epitassiale di giunzioni p-n e l’integrazione della eterostrutture con una cavità di confinamento per l’emissione della luce laser. Nel secondo seminario, verranno trattati i fenomeni di guasto caratteristici dei diodi laser e saranno presentate le metodologie di microscopia elettronica che vengono utilizzate per studiare i fenomeni di degrado. Link GMEET per lo streaming: https://meet.google.com/jby-xvgf-pre
Wednesday, December 4, 2024
3:00 PM
Introduction to laser diodes - 2
-
Massimo Vanzi
(
Istituto di Microelettronica e Microsistemi del CNR
)
Introduction to laser diodes - 2
Massimo Vanzi
(
Istituto di Microelettronica e Microsistemi del CNR
)
3:00 PM - 4:00 PM
Room: 412C
I seminari sono rivolti a studenti della laurea in Fisica e a studenti del dottorato di ricerca per illustrare i principi, la tecnologia costruttiva e il funzionamento di diodi ad emissione di luce laser. Verrà illustrata la modalità di fabbricazione epitassiale di giunzioni p-n e l’integrazione della eterostrutture con una cavità di confinamento per l’emissione della luce laser. Nel secondo seminario, verranno trattati i fenomeni di guasto caratteristici dei diodi laser e saranno presentate le metodologie di microscopia elettronica che vengono utilizzate per studiare i fenomeni di degrado. Link GMEET per lo streaming: https://meet.google.com/qcj-mjgi-vxj
Thursday, December 5, 2024
Friday, December 6, 2024
Saturday, December 7, 2024
Sunday, December 8, 2024
Monday, December 9, 2024
Tuesday, December 10, 2024
Wednesday, December 11, 2024
Thursday, December 12, 2024
Friday, December 13, 2024
Saturday, December 14, 2024
Sunday, December 15, 2024
Monday, December 16, 2024
Tuesday, December 17, 2024
Wednesday, December 18, 2024
Thursday, December 19, 2024
Friday, December 20, 2024
Saturday, December 21, 2024
Sunday, December 22, 2024
Monday, December 23, 2024
Tuesday, December 24, 2024
Wednesday, December 25, 2024
Thursday, December 26, 2024
Friday, December 27, 2024
Saturday, December 28, 2024
Sunday, December 29, 2024
Monday, December 30, 2024