Francesco Saverio Cafagna
(BA)
14/09/15, 09:15
Cosmic Ray and Astrophysical Neutrino Detection
PAMELA is taking date in Space since nine years, heralding a new era in precision cosmic ray physics. The measurements of both particle and antiparticle components of cosmic rays, is providing interesting information concerning the origin and propagation of both galactic and solar cosmic rays.
The measured antiparticle component shows features that can be interpreted in terms of dark matter...
Carmelo Sgro'
(PI)
14/09/15, 09:40
Cosmic Ray and Astrophysical Neutrino Detection
The Fermi Large Area Telescope (LAT) is a space-based observatory conceived to study high-energy gamma rays, but also capable to detect charged cosmic-ray electrons and positrons.It is operating in low Earth orbit since June 2008 and thanks to its large acceptance, has collected the largest high-energy cosmic-ray electron sample to date, with more than 10k events above 1 TeV. The new Pass 8...
Prof.
Bruna Bertucci
(PG)
14/09/15, 10:05
Cosmic Ray and Astrophysical Neutrino Detection
The Alpha Magnetic Spectrometer (AMS) experiment operates since
May 2011 on board of the International Space Station to search for primordial anti-matter, to study the light anti-matter components in the Cosmic Rays (CR) and to perform a precision study of the CR composition and energy spectrum. More than 60 billion events have been collected by the instrument up to now thanks to its large...
Paolo Montini
(ROMA2)
14/09/15, 10:30
Cosmic Ray and Astrophysical Neutrino Detection
The ARGO—YBJ experiment has been in stable data taking for more than five years at the Yangbajing cosmic ray observatory (Tibet, P.R. China, 4300 m a.s.l.). The detector collected about 5X10^11 events in a wide energy range from few TeVs up to the PeV region. In this work we summarize the latest results in cosmic ray physics particularly focusing on the cosmic ray energy spectrum. The results...
Dr.
William Hanlon
(University of Utah, Department of Physics and Astronomy and High Energy Astrophysics Institute)
14/09/15, 12:00
Cosmic Ray and Astrophysical Neutrino Detection
The Telescope Array Project (TA) is the largest cosmic ray observatory in the northern hemisphere and has entered its eighth year of data collection exploring astrophysical phenomena at the highest ends of the cosmic ray energy spectrum. New additions to TA have expanded its reach down to lower parts of the energy spectrum thus allowing it to probe over an unprecedented 4.5 decades of energy...
Prof.
Teresa Montaruli
(Geneve University)
14/09/15, 12:30
Cosmic Ray and Astrophysical Neutrino Detection
In this contribution we summarize the selected highlights of IceCube in the domain of high-energy astrophysics and particle physics. We discuss the highest-energy neutrino detection and its interpretation after 4 years of data. The high energy non-atmospheric component is seen also in other analyses with smaller significance, for instance when using muon neutrinos coming from the Northern...
Daniele De Gruttola
(NA)
14/09/15, 13:00
Cosmic Ray and Astrophysical Neutrino Detection
The Extreme Energy Events (EEE) Project is an experiment, managed by the Fermi Centre, for the study of extremely high-energy cosmic rays, which exploits the Multagap Resistive Plate Chamber (MRPC) technology. The excellent time resolution and good tracking capability of this detector allows us to study Extensive Air Showers with an array of telescopes distributed all over the Italian...
Roberto Aloisio
(GSSI)
14/09/15, 15:30
Interplay between LHC and UHECR physics
The main experimental evidences of UHECR will be reviewed with a particular emphasis on the propagation of these extremely energetic particles and the subsequent production of secondary cosmogenic neutrinos and gamma rays. The cross analysis of the observations of different messengers is of paramount importance in the study of UHECR, principally to determine the physical conditions associated...
Lorenzo Cazon
(LIP)
14/09/15, 16:00
Interplay between LHC and UHECR physics
Extensive air showers are the result of billions of particle reactions initiated by single cosmic rays at ultra-high energy. Their characteristics are sensitive both to the mass of the primary cosmic ray and to the details of hadronic interactions, including energies and kinematic regions beyond those tested by human-made accelerators.
We report on how the Pierre Auger Observatory is...
Paolo Lipari
(ROMA1)
14/09/15, 16:30
Interplay between LHC and UHECR physics
In this talk we review the concept of "universality" in the development
of very high energy cosmic rays showers. The main result
is that the distributions of photons and electrons in a shower
have shapes that are essentially determined by the
the stage of shower development (the shower age)
independently from the energy and identity of the primary particle.
The implications of...
Dr.
Hiroyuki Sagawa
(Institute for Cosmic Ray Research, the University of Tokyo)
14/09/15, 17:30
New Technology and Next generation of Experiments
The Telescope Array (TA) has an array of surface detectors (SD) 700 km^2 in area and three fluorescence telescope stations (FD) to explore the origin of ultra-high-energy cosmic rays.
We found evidence for the hotspot of arrival directions of the highest-energy cosmic rays above 5.7x10^19 eV, of which size is about 20 degrees in radius. To confirm what the origin of the hotspot is, we...
Claudio Di Giulio
(ROMA2)
14/09/15, 18:00
New Technology and Next generation of Experiments
The Pierre Auger Observatory have been taking data since 2004 and with the complete set of detectors since 2008, with an efficiency above 95%, with very low downtime. Our accurancy in the results have had a deep impact on the area of ultra high energy cosmic rays and new questions and open challenges call for an upgrade of the Observatory.
The planned detector upgrade is presented and the...
Giovanni Ambrosi
(PG)
14/09/15, 18:30
New Technology and Next generation of Experiments
The DAMPE experiment (DArk Matter Particle Explorer) is one of the five satellite missions in the frame- work of the Strategic Pioneer Research Program in Space Science of the Chinese Academy of Science (CAS). DAMPE is a powerful space telescope which has as main scientific objective the identification of possible Dark Matter signatures thanks to the capability to detect electrons and photons...
Dr.
ming xu
(Institute of High Energy Physics, Chinese Academy of Sciences / ISDC, University of Geneva)
14/09/15, 19:00
New Technology and Next generation of Experiments
The High Energy cosmic-Radiation Detection (HERD) facility is one of several space astronomy payloads onboard China's Space Station, which is planned for operation starting around 2020. It is designed as a next generation space facility focused on indirect dark matter search, precise cosmic ray spectrum and composition measurements up to the knee energy, and high energy gamma-ray monitoring...
Francesco Loparco
(BA)
15/09/15, 08:30
Gamma Rays Detection
The Fermi Gamma-ray Space Telescope was launched into Earth orbit in June 2008. The Large Area Telescope (LAT) is the main instrument onboard the Fermi satellite and is designed to be sensitive to gamma rays in the energy range from about 20 MeV up to more than 300 GeV. During its first seven years of operation, the LAT has provided an increasingly detailed portrait of the Universe's most...
Brian Humensky
(Columbia University)
15/09/15, 09:00
Gamma Rays Detection
VERITAS is a ground-based array of four 12-meter telescopes near Tucson, Arizona and is one of the world's most sensitive detectors of very high energy (VHE, E > 100 GeV) gamma rays. VERITAS has a broad scientific reach that addresses direct studies of cosmic-ray accelerators, the propagation of cosmic rays, and direct measurements of cosmic-ray spectra. Recent results include deep studies of...
Barbara De Lotto
(UD)
15/09/15, 09:30
Gamma Rays Detection
The MAGIC system of two 17 m diameter Atmospheric Gamma-ray Imaging Cherenkov Telescopes has undergone a major upgrade during the last years and is now completing its tenth observations cycle. In this talk I will present the detector’s performance and a selection of scientific highlights.
Dr.
Tristano Di Girolamo
(Università "Federico II" and INFN, Napoli)
15/09/15, 10:00
Gamma Rays Detection
The ARGO-YBJ air shower detector has been in stable data taking for five years at the YangBaJing Cosmic Ray Laboratory (Tibet, P.R. China, 4300m a.s.l.) with a duty cycle >86% and an energy threshold of a few hundreds of GeV. With the scaler mode technique, the minimum threshold of 1 GeV can be reached. In this talk a selection of results in gamma ray astronomy will be presented, including...
Prof.
Wayne Springer
(University of Utah)
15/09/15, 10:30
Gamma Rays Detection
HAWC is a continuously operated, wide field of view detector comprised of three hundred 200,000 liter water Cherenkov detectors, each instrumented with four photomultipliers providing charge and timing information. HAWC covers approximately ~22,000 m2 at an altitude of 4100m and reliably estimates the energy and arrival direction of gamma and cosmic rays with significant sensitivity over...
Dr.
Michael Unger
(NYU&KIT)
15/09/15, 11:30
Interplay between LHC and UHECR physics
The interpretation of extensive air shower measurements, produced by
ultra-high energy cosmic rays, relies on the correct modelling of the
hadron-air interactions that occur during the shower development. The
majority of hadronic particles is produced at equivalent beam energies
below the TeV range. NA61/SHINE is a fixed target experiment using
secondary beams produced at CERN using the...
Massimo Bongi
(FI)
15/09/15, 12:00
Interplay between LHC and UHECR physics
LHCf is an experiment designed to study the very-forward emission of neutral particles produced in proton-proton and proton-nucleus collisions at the LHC. The detectors consists of a pair of electromagnetic sampling calorimeters installed on both sides of the ATLAS interaction point IP1 at a distance of 140 m, covering the pseudorapidity range from 8.6 to infinity. The experiment has...
Benedetto Giacobbe
(BO)
15/09/15, 12:30
Interplay between LHC and UHECR physics
A review of the results of the ATLAS forward physics program will be given. This includes a complete set of proton-proton cross section measurements at $\sqrt{s} = 7 TeV$, diffractive physics studies using rapidity gaps, forward jet production and energy flow as a function of pseudorapidity. The ATLAS future perspectives will also be discussed, focused on the phase 1 upgrade project AFP,...
Vincenzo Branchina
(CT)
15/09/15, 13:00
Interplay between LHC and UHECR physics
The analysis of the stability condition of the electroweak vacuum (and
then of our Universe as a whole) is of the greatest importance for our
understanding of physics beyond the Standard Model. The possibility
that cosmic rays could destabilize the present state of our Universe,
and that the cosmic ray induced vacuum decay could be faster than the
spontaneous decay has been investigated...
Prof.
Stephane Coutu
(Penn State University)
15/09/15, 15:15
Cosmic Ray and Astrophysical Neutrino Detection
With an accumulated exposure of over 50,000 km^2 sr yr, the Auger Observatory has the largest statistical sample of ultra-high energy cosmic rays. We will present highlights of recent results from Auger, including details of the energy spectrum, sensitivity to primary composition, searches for anisotropies and candidate sources, and searches for neutral cosmic messengers. Explorations of...
thomas gaisser
(University of Delaware)
15/09/15, 15:40
Cosmic Ray and Astrophysical Neutrino Detection
IceCube, with its surface array IceTop, detects three different components of extensive air showers: the total signal at the surface, GeV muons in the periphery of the showers and TeV muons in the deep array of IceCube. The spectrum is measured with high resolution from the knee to the ankle with IceTop. Composition and spectrum are extracted from events seen in coincidence by the surface...
Andrea Chiavassa
(Universita` degli Studi di Torino)
15/09/15, 16:10
Cosmic Ray and Astrophysical Neutrino Detection
The KASCADE-Grande experiment operated since 2003 to 2012 measuring cosmic rays in the 10^16-10^18 eV energy range.
In this talk I will show and discuss the main results obtained in the study of the primary spectrum (that cannot be described by a single power law in this energy range), chemical composition (a steepening of the haevy component spectrum and a hardening of the light one have...
Prof.
Vasily Prosin
(Skobeltsyn Institute of Nuclear Physics of Lomonosov Moscow State University)
15/09/15, 16:40
Cosmic Ray and Astrophysical Neutrino Detection
The experimental data of Tunka-133 obtained during 5 years of observation and preliminary data from the Tunka-HiSCORE prototype array with its first 9 stations allowed a study of primary cosmic rays in the wide energy range 3x10^14 – 10^18 eV.
Reconstruction of the depth-of-shower maximum Xmax by an analysis of the Cherenkov light lateral distribution and the pulse width provides a...
Marco Pallavicini
(GE)
16/09/15, 09:00
New Technology and Next generation of Experiments
The talk will outline the status and the medium / long term prospectivesof INFN Astroparticle and Fundamental Physics commission in the study of cosmic radiation, both with ground/sea based detectors and from space.
Giuseppe Di Sciascio
(ROMA2)
16/09/15, 09:30
New Technology and Next generation of Experiments
Despite large progresses in building new detectors and in the analysis techniques, the key questions concerning the origin, acceleration and propagation of Galactic Cosmic Rays are still open. A number of new extensive air showers arrays is in progress.
The most ambitious and sensitive project between them is LHAASO, a new generation multi-component experiment to be installed at very high...
Ciro Bigongiari
(TO)
16/09/15, 10:00
New Technology and Next generation of Experiments
The Cherenkov Telescope Array (CTA) is planned to be the next generation ground based observatory for very high energy (VHE) gamma-ray astronomy. It will provide a full sky-coverage by featuring an array of imaging atmospheric Cherenkov telescopes both in the northern and southern hemispheres.
Sites close to Cerro Paranal (Chile) and on La Palma (Spain) have been recently chosen for final...
Annarita Margiotta
(BO)
16/09/15, 10:30
New Technology and Next generation of Experiments
KM3NeT is a distributed research infrastructure comprising a network of deep-sea neutrino telescopes in the Mediterranean Sea. It will consist of building blocks of 115 vertical detection units anchored at the seabed, connected to shore. Each detection unit carries 18 optical modules equipped with 31 3” photomultipliers. Two configurations are defined to detect neutrinos in different ranges of...
Dr.
Frank Schröder
(Karlsruhe Institute of Technology (KIT))
16/09/15, 11:30
New Technology and Next generation of Experiments
Radio measurements yield calorimetric information on the electromagnetic shower component around the clock. However, until recently it was not clear whether radio measurements can compete in accuracy with established night-time techniques like air-Cherenkov or fluorescence detection. Due to recent progress in the radio technique as well as in the understanding of the emission mechanisms, the...
Francesco Saverio Cafagna
(BA)
16/09/15, 12:00
New Technology and Next generation of Experiments
The JEM-EUSO mission, on board of the International Space Station (ISS), has the primary objective of doing astrophysics detecting extreme energy cosmic rays (EECRs), above 3x10^19eV. This Extreme Universe Space Observatory (EUSO), will be the first space mission to be devoted to the study of this energy range with the aim of extending the knowledge on sources, spectra and composition of...
Prof.
Daniele Fargion
(ROMA1)
16/09/15, 12:30
New Technology and Next generation of Experiments
PeV neutrino has been found in ICECUBE. The mixing along galactic distance guarantee the presence of PeV Tau neutrinos among astrophysical signals, whose direct detection is subject of deep research since a decade at different UHECR experiments , mostly at EeV energies; these UHE tau neutrino while skimming the Earth (Horizontal Tau airshowers) may shower upward to the sky.
The EeV tau...
antonio codino
(university of Perugia and INFN)
16/09/15, 15:00
Cosmic Ray: Theoretical Implications
According to recent measurements the tendency of the chemical composition above the ankle is characterized by increasing fractions of intermediate and heavy nuclei and a dominance of light nuclei around the ankle featured by a minimum of the log(A) profile. Calculations of the chemical composition in the range 3.5x10**18-5x10**19 eV according to new principles are reported and compared with...
Dr.
Armando Di Matteo
(INFN L'Aquila), Dr.
Aurelio Grillo
(LNGS INFN)
16/09/15, 15:30
Cosmic Ray: Theoretical Implications
Ultra High Energy Cosmic Rays experimental data are now of very good statistical significance even in the region of the expected GZK feature. The identification of their sources requires sophisticate analysis of their propagation in the extra galactic space. When looking at the details of this propagation some unforeseen features emerge. I will discuss some of these "surprises".
Ralf Ulrich
(KIT)
16/09/15, 16:00
Cosmic Ray: Theoretical Implications
With the LHC basically reaching its design beam energy the measurements most relevant for the cosmic ray community are becoming available. First data do not indicate major difficulties within the existing interaction models. An eventual new generation of updated models to describe LHC data at 13TeV will further lower the model discrepancies at ultra-high energies. The cosmic ray community has...
