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Giampaolo Mannocchi (LNF), Dr Roberto Fusco-Femiano (IAPS/INAF)5/21/18, 8:45 AM
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Giorgio Parisi (ROMA1)5/21/18, 9:00 AM
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Dr Maria Alessandra Papa (Max Planck Inst. for Gravitational Physics)5/21/18, 9:25 AM
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Viviana Fafone (ROMA2)5/21/18, 9:50 AM
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Marica Branchesi (LNGS)5/21/18, 10:15 AM
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Dr alessandro chieffi (INAF)5/21/18, 11:00 AM
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Claudio Kopper (University of Alberta)5/21/18, 11:25 AM
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Prof. Chris Fryer (Los Alamos National Laboratory)5/21/18, 11:50 AM
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Dr Hendrik van Eerten (University of Bath)5/21/18, 12:15 PM
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Prof. Luciano Iess (Universita' La Sapienza)5/21/18, 5:00 PM
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Dr Oscar Straniero (INAF)5/21/18, 5:25 PM
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Dr Enzo Brocato (INAF - Osservatorio Astronomico di Roma)5/21/18, 5:50 PM
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Rita Dolesi (TIFP)5/21/18, 6:15 PM
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Carlo Gustavino (ROMA1)5/21/18, 6:40 PM
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Dr Lucie Linssen5/21/18, 7:15 PM
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Prof. Jordan Goodman (University of Maryland)5/22/18, 9:00 AM
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Giovanni Morlino (GSGC)5/22/18, 9:25 AM
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Prof. Felix Aharonian (DIAS, Dublin)5/22/18, 9:50 AM
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Dr Alessandra Lamastra (INAF-OAR ASI - SSDC)5/22/18, 10:15 AM
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Dr Brenda Dingus (Los Alamos National Lab)5/22/18, 11:00 AM
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Dr Iris Gebauer (KIT), Ms Manuela Vecchi (INFN)5/22/18, 11:25 AM
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Francesco Longo (TS)5/22/18, 12:00 PM
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Dr Carlotta Pittori (INAF-OAR/ASDC)5/22/18, 12:25 PM
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Pier Simone Marrocchesi (SI)5/22/18, 5:00 PM
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vitor de souza (ifsc-usp)5/22/18, 5:25 PM
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Dr Mario Edoardo Bertaina (TO)5/22/18, 5:50 PM
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Dr Marta Burgay (INAF - ORA Cagliari)5/22/18, 6:15 PM
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Dr Fabrizio Nicastro (INAF - OAR)5/22/18, 6:40 PM
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Dr Pavel Klimov (SINP MSU)5/22/18, 7:05 PM
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Dr Anna Nierenberg (University of California Irvine)5/23/18, 9:00 AM
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Prof. Salvatore Capozziello (NA)5/23/18, 9:25 AM
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Marco Castellano (INAF - Osservatorio Astronomico di Roma)5/23/18, 9:50 AM
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Dr Alfredo Davide Ferella (LNGS)5/23/18, 10:15 AM
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Prof. Elena Aprile (Columbia University)5/23/18, 11:00 AM
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Lea Di Noto (GE)5/23/18, 11:25 AM
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Stefano Dell'Oro (GSSI)5/23/18, 11:50 AM
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Dr Marcello Messina (Columbia University)5/23/18, 12:15 PM
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Prof. Ronald Cintra Shellard (Centro Brasileiro de Pesquisas Físicas)5/23/18, 12:40 PM
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Antonio Capone (University Sapienza of Roma)5/24/18, 9:00 AM
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Sara Buson (PD)5/24/18, 9:25 AM
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Marco Circella (BA)5/24/18, 9:50 AM
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Roberto Iuppa (TIFP)5/24/18, 10:15 AM
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Dr Zhiguo Yao (Institute of High Energy Physics, Beijing, China)5/24/18, 11:00 AM
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Prof. Anatoly Petrukhin (NRNU MEPhI)5/24/18, 11:25 AM
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Dr Elisabetta Bissaldi (BA)5/24/18, 11:50 AM
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Aldo Morselli (ROMA2)5/24/18, 12:15 PM
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Dr Paolo Desiati (University of Wisconsin - Madison)5/24/18, 12:40 PM
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Juan Carlos Díaz Vélez (Universidad de Guadalajara)5/24/18, 5:00 PM
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Dr Lorenzo Natalucci (INAF/IAPS), Pietro Ubertini (ROMA2)5/24/18, 5:25 PM
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Dr Lorenzo Natalucci (INAF/IAPS)5/24/18, 5:50 PM
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Dr Fabrizio Fiore (INAF-OAR)5/24/18, 6:15 PM
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Simone Dell'Agnello (LNF)5/24/18, 6:40 PM
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Dr Mariateresa Crosta (INAF-OATo)5/24/18, 7:05 PM
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Elia Stefano Battistelli (ROMA1)5/25/18, 9:00 AM
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Giovanni Andrea Prodi (TIFP)5/25/18, 9:25 AM
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Dr Alessandra Corsi (Texas Tech University)5/25/18, 9:50 AM
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Dr Luigi Piro (IAPS/INAF)5/25/18, 10:15 AM
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Dr ELEONORA Troja (NASA/GSFC)5/25/18, 11:00 AM
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Prof. Gianfranco Bertone Bertone (ITP, Zurich & IAP, Paris)5/25/18, 11:25 AM
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Mr martino borsato (LAL Orsay)5/25/18, 11:50 AM
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Babette Dobrich (CERN)5/25/18, 12:15 PM
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Marco Incagli (PI)5/25/18, 12:40 PM
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Dr Maxim Pospelov (Perimeter Institute/University of Victoria)5/25/18, 5:00 PM
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Mauro Raggi (ROMA1)5/25/18, 5:25 PM
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Matthew David Moulson (LNF)5/25/18, 5:50 PM
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Dr Giuseppe Ruggiero (Scuola Normale Superiore, Pisa)5/25/18, 6:15 PM
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ludovico pontecorvo (INFN)5/25/18, 6:40 PM
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Vincenzo Maria Vagnoni (BO)5/25/18, 7:05 PM
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Dr Carla Signorini (European Space Agency)5/26/18, 9:00 AM
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Elisabetta Cavazzuti (T)5/26/18, 9:25 AM
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Prof. Angela Olinto (The University of Chicago)5/26/18, 9:50 AM
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Nadia Pastrone (TO)5/26/18, 10:15 AM
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Massimo Ferrario (LNF)5/26/18, 11:00 AM
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Umut Kose (INFN)5/26/18, 11:25 AM
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Dr Oscar Straniero (INAF)
Understanding stellar nucleosynthesis requires expertise in stellar modelling and nuclear physics. Hints and constraints to the nucleosynthesis models come from atmospheric abundance analysis of different stars, as obtained by means of high resolution spectroscopy, and measurements of solar (and pre-solar) composition, as obtained by combining, beside solar spectroscopy, the abundance...
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Stefano Dell'Oro (GSSI)
The current status of the neutrinoless double beta decay (0νββ) search is summarized, ex-
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ploiting the up-to-date knowledge of the oscillation parameters and of the recent theoretical
developments in the understanding of the 0νββ process, especially those concerning the nu-
clear description and its limitations. This also allows to infer expectations and uncertainties
for the experimental... -
21. Addressing the missing matter problem in galaxies through a new fundamental gravitational radiusProf. Salvatore Capozziello (Università di Napoli "Federico II")
We demonstrate that the existence of a Noether symmetry in extended
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theories of gravity gives rise to a further gravitational radius, besides
the standard Schwarzschild one, determining the dynamics at galactic
scales. By this feature, it is possible to explain the baryonic
Tully-Fisher relation, the rotation curve of gas-rich galaxies, and the
features of fundamental plane of ellipticals... -
Dr Alessandra Lamastra (INAF-OAR ASI - SSDC)
Various observations are revealing the widespread occurrence of mildly relativistic wide-angle AGN outflows, likely launched from accretion disks around supermassive black holes, and interacting strongly with the gas of their host galaxy.
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During the interaction, strong shocks are expected to form that can accelerate relativistic particles. The interactions of shock-accelerated particles... -
Dr Matteo Palermo (University of Hawaii at Manoa)
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Marco Circella (INFN Bari, Italy)
The ANTARES detector, located 40 km off the French coast, with an instrumented volume of more than 0.01 cubic kilometres, is the largest neutrino telescope in the Northern Hemisphere and the first one to be operated in the deep sea. It has been taking data continuously since 2007. The primary goal of such a telescope is to search for astrophysical neutrinos in the TeV-PeV range. The latest...
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Marco Castellano (INAF - Osservatorio Astronomico di Roma)
The investigation of distant galaxy formation and evolution is a powerful tool to constrain dark matter scenarios, supporting and in some cases surpassing other astrophysical and experimental probes. The recent completion of the Hubble Frontier Field (HFF) programme combining ultra-deep Hubble Space Telescope observations and the magnification power of gravitational lensing produced by...
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Dr Paolo Desiati (University of Wisconsin - Madison)
The IceCube Observatory is a neutrino telescope deployed at the geographic South Pole, aimed to detect and identify high energy neutrinos of astrophysical origin. IceCube is also able to detect cosmic rays with the 1 km^3 neutrino telescope buried 2500 meters under the Antarctic ice and with a dedicated 1 km^2 surface array. IceCube has analyzed data over the last several years to determine,...
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Giovanni Morlino (GSGC)
The Cosmic Ray (CR) physics has entered a new era driven by high precision measurements coming from direct detection (especially AMS-02 and PAMELA) as well as gamma-ray observations (Fermi-LAT). In this talk I will focus on how such data impact the understanding of the supernova remnant paradigm for the origin of CRs. In particular I will discuss advancements in the field concerning the three...
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Dr Alfredo Davide Ferella (LNGS)
Dark Matter is one of the most challenging puzzles of modern physics. Its undisputable evidence so far comes solely from its gravitational interaction, but it is believed to have particle nature. The Weakly Interacting Massive Particle (WIMP) still remains the best-motivated candidate. After a brief introduction and motivation to the WIMP paradigm, the WIMP direct detection principles will be...
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Mauro Raggi (ROMA1)
While accelerator particle physics has traditionally focused on exploring dark matter through high energy machines, inspired by the WIMP paradigm, testing dark-sectors hypothesis requires innovative low energy and high intensity beams.
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This scenario offers attractive opportunities to low energy machine and small size experiments with high sensitivity detectors. In this paper we will focus our... -
Dr Iris Gebauer (KIT)
With precision instruments like CALET, DAMPE and AMS in space a plethora of new experimental data from direct cosmic ray measurements has become available in recent years.
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The precision of the measurements reveals many unexpected features, some of which challenge our current understanding of cosmic ray acceleration and galactic transport.
This talk provides an overview over some of the most... -
Dr Marta Burgay (INAF - Osservatorio Astronomico di Cagliari)
In this talk I will review the main observational properties of Fast Radio Bursts, a fast growing family of millisecond-duration extragalactic radio flares, whose origin is still debated. I will report on the latest news, in particular relating on their multiwavelength follow-up and on the possibility to use FRBs as cosmological probes.
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Dr Elisabetta Bissaldi (BA)
The Fermi Gamma-Ray Burst Monitor (GBM) is the secondary instrument onboard the Fermi mission, which is celebrating its 10-yrs anniversary in Space in 2018. Fermi-GBM has a wide field of view, high uptime, and both in-orbit triggering and high time resolution continuous data acquisition, thus enabling offline searches for weaker transients. Fermi-GBM triggered on more than 2300 Gamma-Ray...
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Lucie Linssen (CERN)
In this talk an overview will be given of the future pp and e+e- collider studies currently hosted by CERN: FCC-hh, FCC-ee, HE-LHC and CLIC. For each of the projects the current status of the accelerator design and the corresponding performance parameters will presented. Similarly, the current baseline designs of the detectors and their performance will be shown. Highlights of the physics...
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Francesco Longo (TS)
After almost 10 years of data taking by the Large Area Telescope on board the Fermi Gamma-ray Space Telescope, we present an overview of the current status of high-energy gamma-ray astrophysics. Particular emphasis will be given to the broad range of time-domain astrophysics topics studied by the LAT and to the increasingly important multimessenger connections involving gamma-ray sources.
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Dr Carlotta Pittori (INAF-OAR/ASDC)
AGILE is an Italian Space Agency (ASI) space mission devoted to gamma-ray observations in the 30 MeV-50 GeV energy range, with simultaneous X-ray imaging in the 18-60 keV band. Launched in April 2007, the AGILE satellite is in its 11th year of operations in orbit, and it is substantially contributing to improve our knowledge of the high-energy gamma-ray sky. I will summarize some AGILE...
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ludovico pontecorvo (INFN)
After a brief description of the ATLAS and CMS detectors and their performance during the last year data taking, the main focus of the talk will be on
the latest physics results.
In particular, most recent measurements on the Higgs production and its decays, including differential measurements, will be illustrated together with selected topics on searches for new physics.
A very brief...
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Dr Anna Nierenberg (University of California Irvine)
Strong gravitational lensing, in which light is bent and distorted by massive objects, provides a powerful probe into the dark Universe. I will discuss strong gravitational lensing constraints on the abundance and mass of massive compact objects, as well as on the halo mass function and the free-streaming length of particle dark matter. I will conclude by describing how the next generation of...
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Pietro Ubertini (ROMA2)
The talk will summarize the scientific implication of the INTEGRAL observations of the LVC O2 run and, in particular, of the upper limits for the BH-BH mergers and the detection of the first prompt electromagnetic counterpart coincident with a GW170817.
Authors : UBERTINI, Pietro (IAPS-INAF), BAZZANO, Angela (IAPS-INAF) ; NATALUCCI, Lorenzo (INAF/IAPS) ; RODI, James (IAPS-INAF) et al...
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Dr Giuseppe Ruggiero (Lancaster University, UK)
The decay K+→π+νν, with a very precisely predicted branching ratio of less than 10^(-10), is one of the best candidates to reveal indirect effects of new physics at the highest mass scales. The NA62 experiment at CERN SPS is designed to measure the branching ratio of the K+→π+νν with a decay-in-flight technique, novel for this channel. NA62 took data in 2016, 2017 and another year run is...
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Prof. Ronald Cintra Shellard (Centro Brasileiro de Pesquisas Físicas)
LATTES, the Large Array Telescope for Tracking Energetic Sources, is being designed to be a detector sensitive to gamma rays with energies in the range from 100 GeV all the way up to 100 of TeVs, operating day and night, with a large field of view. The detector, to be installed at altitudes of about 5.000 m a.s.l. in the Andes mountains in South America, is based on a novel concept to detect...
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Dr Lea Di Noto (GE)
Low energy solar neutrinos, fundamental for the discovery of the neutrino flavour oscillation, are a unique tool to investigate the nuclear reactions that fuel the Sun. The Borexino experiment, based on a 270 ton ultra-pure liquid scintillator detector at Laboratori Nazionali del Gran Sasso, was conceived to measure solar neutrino fluxes in the MeV and sub-MeV energy range. The data taking...
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Prof. Jordan Goodman (University of Maryland)
Understanding the most energetic events in the Universe requires that we study them all the tools available to us. The means using the electromagnetic spectrum from radio to the highest energy gamma-rays, neutrinos, and gravitational waves. Wide-field instruments such as LIGO, IceCube, Fermi, SWIFT, and HAWC can provide prompt detection of events that can be followed up by pointed...
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Maria Cristina D'Amato (LNF)
my abstract
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Claudio Kopper (University of Alberta)
With the recent discovery of high-energy neutrinos of extraterrestrial origin by the IceCube neutrino observatory, neutrino astronomy is entering a new era. The highest-energy neutrinos observed to date exceed 1 PeV in energy, a regime of particular interest because the neutrinos should point back to the still elusive accelerators of the highest energy Galactic and extragalactic cosmic rays....
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Babette Dobrich (CERN)
The NA62 experiment at CERN is designed to measure precisely the rare decay K+→π+νν. The intensity and energy of the primary (proton) and secondary (Kaon) beams, as well as the hermetic detector coverage and overall geometry, give in addition the opportunity to search for hypothesized weakly-coupled particles. I will review these opportunities, present results and sketch the prospects of...
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Prof. Gianfranco Bertone Bertone (ITP, Zurich & IAP, Paris)
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Antonio Capone (ROMA1)
The SKK measured fluxes of solar neutrinos are the first example of the possible use of neutrino fluxes to identify, and locate, a neutrino source. The detection of neutrinos originated in the SN_1987-A as a counterpart of its optical observation has been the first example of a multi-messenger event. High Energy neutrino astronomy has been proposed, and after the IceCube discovery of the...
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Prof. Chris Fryer (Los Alamos National Laboratory)
The first gravitational-wave detection of the merger of a neutron star binary (GW170817) corroborated many theories on the nature of these events while at the same time, displaying a number of surprises. Although long-believed to be an engine for gamma-ray bursts, the off-angle detection of gamma-rays suggests a wider jet opening angle than previously believed. Similarly, the inferred rate...
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Elisabetta Cavazzuti (T)
In this talk I will go through the current operating science missions and experiments to which ASI participates and which are giving relevant contributions to the astrophysics and particle physics. Starting from PAMELA via AMS to CALET in the cosmic rays study and starting from INTEGRAL via Swift, AGILE, Fermi, NuSTAR in the high energy astrophysics branch. I will discuss also the future...
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Dr Alessandra Corsi (Texas Tech University)
On 2017 August 17, the field of gravitational-wave (GW) astronomy made the big leagues with a dazzling discovery. After several GW detections of black hole (BH)-BH mergers with no convincing electromagnetic counterparts, advanced LIGO and Virgo scored their first direct detection of GWs from a binary neutron star (NS) merger, an event dubbed GW170817. Soon after the GW discovery, GW170817...
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Dr Brenda Dingus (Los Alamos National Lab)
“The HAWC Observatory: Detecting the Highest Energy Gamma-Rays”
The High Altitude Water Cherenkov (HAWC) is a continuously operating (>95% on-time), wide field-of-view (~2 sr) observatory located at 14000’ above sea level near Puebla, Mexico. HAWC observes ~2/3 of the sky each day and had detected nearly 50 sources of which about one quarter were previously unknown. Several of these...
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Dr Pavel Klimov (SINP MSU)
TUS (Tracking Ultraviolet Set-up) is the first orbital detector of extreme energy cosmic rays (EECR). It was launched into orbit on April 28, 2016, as a part of the scientific payload of the Lomonosov satellite mission. The detector is aimed to test the technique of measuring UV fluorescent and Cherenkov radiation of extensive air showers (EAS) generated by primary cosmic rays with energies...
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Dr Mario Edoardo Bertaina (TO)
The origin and nature of Ultra-High Energy Cosmic Rays (UHECRs) remain unsolved in contemporary astroparticle physics. To give an answer to these questions is rather challenging because of the extremely low flux of a few per km^2 per century at extreme energies such as E > 5 × 10^19eV.
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The objective of the JEM-EUSO program, Extreme Universe Space Observatory, is the realization of a space... -
Dr martino borsato (USdC)
Investigating the origin of Dark Matter, so far observed only through its gravitational interaction, is one of the most important goals of the LHC. Indeed, the ATLAS, CMS and LHCb experiments have a vast and diverse program of analyses related to Dark Matter.
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I will briefly review the latest results in LHC searches for events with missing energy plus a single object (jet, Z, Higgs, top quark)... -
Manuela Vecchi (University of Groningen/University of São Paulo)
Recent results by space borne experiments took cosmic ray data to a precision level. These new results are now able to challenge the conventional scenarios for cosmic ray production and acceleration in the Milky Way, also leaving the room for new, exotic sources.
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In this talk we will give an overview of the latest results of the cosmic ray fluxes, and some possible interpretations will be... -
Dr Zhiguo Yao (IHEP, Beijing)
The Large High Altitude Air Shower Observatory (LHAASO) is under construction at the Mountain Haizishan (4410m a.s.l.), Sichuan Province, China. LHAASO comprises of 4 major kinds of detector arrays, such as the Electro-magnetic particle Detector (ED) array, the Muon Detector (MD) array, the Water Cherenkov Detector Array (WCDA), and the Wide-Field-of-view air Cherenkov Telescope Array (WFCTA)....
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Dr Mariateresa Crosta (INAF-OATo)
As of April 25th the second release of the Gaia catalogue (DR2) becomes available to the scientific community worldwide. It contains the five-parameter astrometric solution (positions on the sky, parallaxes, and proper motions) for more than 1.3 billion sources, with a limiting magnitude of G = 21 and a bright limit of G ≈ 3, and median radial velocities for more than 7.2 million stars. The...
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Dr Lorenzo Natalucci (INAF/IAPS)
Since 2015, AHEAD (Integrated Activities in the High Energy Astrophysics Domain) is providing a framework to bring together Europe's science community working in this highly competitive field. AHEAD is an ongoing project funded by the EU Horizon 2020 programme for Research Infrastructures, with the main goal of integrating efforts by the European science community and keeping them at the...
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Aldo Morselli (ROMA2)
The Cherenkov Telescope Array (CTA) will be the next generation gamma-ray observatory, open to the scientific community, to investigate the very-high-energy emission from a large variety of celestial sources in the 20 GeV - 300 TeV energy range. The full array, distributed over two sites, one in the northern and one in the southern hemisphere, will provide whole-sky coverage and will...
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Marco Incagli (PI)
The Muon g-2 experiment at Fermilab will measure the anomalous magnetic moment of the muon to a precision of 140 parts per billion, which is a factor of four improvement over the previous E821 measurement at Brookhaven. The experiment will also extend the search for the muon electric dipole moment (EDM) by approximately two orders of magnitude. Both of these measurements are made by combining...
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Dr Alessandro Chieffi (IAPS)
I will discuss the range of possible masses of the remnants that are left by the explosion of a massive stars as well as current uncertainties in their estimates. I will show that current stellar models easily predict masses in the range of those observed by the LIGO-VIRGO collaboration
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Dr Fabrizio Nicastro (INAF - OAR)
It has been known for decades that the observed number of baryons in the local Universe falls about 30-40% short of the total number of baryons predicted by Big-Bang Nucleosynthesis and inferred by density fluctuations of the Cosmic Microwave Background. While theory provides a reasonable solution to this paradox, by locating the missing baryons in hot and tenuous filamentary gas connecting...
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Nadia Pastrone (TO)
Muon-based accelerators have the potential to enable facilities at both the Intensity and the Energy Frontiers in Particle Physics. A Muon Collider has the ability to study the direct (s-channel) production of scalar resonances like the Higgs boson while extending operations to a multi-TeV energy region enables a new field of measurements and discoveries. The traditional approach for these...
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vitor de souza (ifsc-usp)
The most energetic particles ever detected can impose several constrains on our understanding of Nature. However, the most fundamental human questions in the context of ultra-high energetic particles have not been satisfactorily answered yet: Where do they come from? What are they? How are they created? In the last decade, the Pierre Auger Observatory has allowed us to progress decisively in...
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Dr Marcello Messina (NYU Abu Dhabi)
The first part the seminar will be about a novel idea for the detection Cosmological Relic Neutrinos (CRN) and more in general, for the detection of neutrinos of vanishing energy. This idea is described in detail in the paper [1]. The method is based on the fact that neutrino interactions on beta-instable nuclei have the key feature of requiring no energy threshold for the neutrino...
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Juan Carlos Díaz Vélez (Universidad de Guadalajara)
We present updated results on the joint analysis of the arrival direction distribution of Galactic cosmic rays by the High-Altitude Water Cherenkov (HAWC) Observatory (located at 19$^\circ$ N) and the IceCube Neutrino Observatory (located at 90$^\circ$ S). We describe the methods used to combine the IceCube and HAWC data, including an improved reconstruction method that can recover the...
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