Prof.
Francis Halzen
(University of Wisconsin Madison)
9/25/17, 10:20 AM
High-energy neutrino observations and perspectives
Talk (20'+5')
The IceCube project has transformed a cubic kilometer of natural Antarctic ice into a neutrino detector. The instrument detects more than 100,000 neutrinos per year in the GeV-to-PeV energy range. Among those, we have isolated a flux of high-energy cosmic neutrinos. I will discuss the latest measurements of the cosmic neutrino flux and their implications for its possible origin(s). From the...
Dr
Markus Ackermann
(DESY)
9/25/17, 10:45 AM
High-energy neutrino observations and perspectives
Talk (20'+5')
IceCube is the world's most sensitive neutrino telescope located at the geographic South Pole. With the discovery of a flux of high-energy cosmic neutrinos it has opened a new window for astronomy. Neutrinos allow to study the most extreme environments of our universe even in regions from which photons cannot escape, and help to understand the mechanisms of particle acceleration in the cosmos....
Ms
Dorothea Samtleben
(NIKHEF, Amsterdam)
9/25/17, 11:10 AM
High-energy neutrino observations and perspectives
Talk (20'+5')
ANTARES, the largest underwater neutrino telescope in the Northern Hemisphere, has been continuously operating since 2007 in the Mediterranean Sea. The transparency of the water allows for a very good angular resolution in the reconstruction of signatures of interactions from neutrinos of all flavors. This results in unprecedented sensitivity for neutrino source searches in the Southern Sky...
Carlos de los Heros
(Uppsala University)
9/25/17, 11:35 AM
High-energy neutrino observations and perspectives
Talk (20'+5')
Large-scale neutrino telescopes offer interesting possibilities to address particle physics topics ranging from particle searches to neutrino oscillations or tests of fundamental laws. They can even do so at energy ranges not accessible to accelerators, providing a much desired complementarity to accelerator-based physics.
I will review recent results from the existing high-energy neutrino...
Prof.
Eli Waxman
(Weizmann Institute)
9/25/17, 1:30 PM
Astrophysical sources and backgrounds
Talk (20'+5')
The detection of high energy extra-terrestrial neutrinos by IceCube opens a new window for observations of the Universe. I will discuss the origin of these neutrinos, the clues that their detection provide towards the solution of the long standing question of the origin of cosmic-rays, and the prospects for identifying the cosmic-ray sources and for studying open questions in astro- and...
Dr
Rikard Enberg
(Uppsala University)
9/25/17, 1:55 PM
Astrophysical sources and backgrounds
Talk (20'+5')
The atmospheric neutrino flux is produced when cosmic rays collide with Earth's atmosphere. At very high energy, the prompt contribution to the neutrino flux, which comes from decays of charmed hadrons, dominates over the conventional flux, which comes from pion and kaon decays. This is due to the very short lifetime of the charmed hadrons, which therefore do not lose energy before they decay....
Dr
Walter Winter
(DESY)
9/25/17, 2:20 PM
Astrophysical sources and backgrounds
Talk (20'+5')
Gamma-ray bursts (GRBs) are the most energetic electromagnetic outburst class in the Universe, and candidates for the sources of the ultra-high energy cosmic rays (UHECRs). We discuss the neutrino flux associated with the prompt emission from GRBs, such as its possible contribution to the observed astrophysical neutrino flux, and we show the implications of recent stacking searches for...
Prof.
Elisa Resconi
9/25/17, 2:45 PM
Astrophysical sources and backgrounds
Talk (20'+5')
Prof.
Alexander Kusenko
(UCLA and Kavli IPMU)
9/25/17, 3:10 PM
Observed spectra of distant blazars show evidence of secondary gamma rays from interactions of cosmic rays with extragalactic photon radiation (EBL and CMB). The same interactions of cosmic rays are expected to produce a flux of neutrinos with energies peaked around 1 PeV. The spectrum and the isotropic distribution are consistent with IceCube observations. This association also implies that...
Dr
Markus Ahlers
(UW-Madison)
9/25/17, 3:35 PM
The recent observation of TeV-PeV neutrinos by IceCube has opened a new window to the high-energy Universe. These high-energy astrophysical neutrinos are expected to originate from cosmic-ray interactions with gas and radiation. The origin of the IceCube signal is presently unknown and various Galactic and extragalactic source candidates have been proposed. Multi-messenger studies can help to...
Giuseppe Di Sciascio
(ROMA2)
9/25/17, 4:40 PM
Multimessenger physics
Talk (20'+5')
The riddle of the origin of Cosmic Rays is unsolved since more than one century. The identification of the galactic sources able to accelerate particles beyond PeV energies is certainly one of the main open problems of high energy astrophysics. High energy gamma ray (and neutrino) observations are an essential probe of CRs, if gamma rays (and neutrinos) are produced by CRs interacting close to...
Prof.
Enrique Zas
(IGFAE - University of Santiago)
9/25/17, 5:05 PM
Multimessenger physics
Talk (20'+5')
Roberto Aloisio
(Gran Sasso Science Institute)
9/25/17, 5:30 PM
Multimessenger physics
Talk (20'+5')
We review the main features of ultra high energy cosmic rays propagation and the production of secondary cosmogenic particles such as neutrinos and gamma rays. We discuss the capabilities of the present and future observatories in the detection of these secondary particles, that has a paramount importance in constraining models for ultra high energy cosmic rays acceleration.
Prof.
Takeo Moroi
9/25/17, 5:55 PM
New physics at high-energy neutrino telescopes
Talk (20'+5')
Dr
Arman Esmaili
(Pontifícia Universidade Católica do Rio de Janeiro)
9/25/17, 6:20 PM
New physics at high-energy neutrino telescopes
Talk (20'+5')
I will discuss the possibility to interpret the IceCube data by PeV mass scale decaying Dark Matter. The generic signatures of this scenario, including its energy spectrum as well as the peculiar anisotropies will be discussed. Also possible future checks of this scenario by EAS experiments, both by detecting the prompt gamma ray flux from decaying dark matter, or the induced anisotropies in...
Maurizio Spurio
(BO)
9/26/17, 9:00 AM
High-energy neutrino observations and perspectives
Talk (20'+5')
New windows in the study of the high-energy universe have been opened by large volume detectors in underground laboratories or underwater/ice, huge surface shower arrays, particle detectors sent into space and by gravitational wave interferometers. Neutrino observations play a central role in multi-messenger strategies in astrophysics, cosmology and particle physics. The talk intends to survey...
Giorgio Maria Riccobene
(LNS)
9/26/17, 9:25 AM
High-energy neutrino observations and perspectives
Talk (20'+5')
Aldo Morselli
(ROMA2)
9/26/17, 9:50 AM
High-energy neutrino observations and perspectives
Talk (20'+5')
Measurement of cosmic rays and gamma rays made with satellites can give very useful information on present and future High Energy Neutrinos data. Here we will review the most important connections
Dr
Dariusz Gora
(Institute of Nuclear Physics Polish Academy of Sciences, PL-31342 Krakow, Poland)
9/26/17, 10:15 AM
The MAGIC telescopes, located at the Roque de los Muchachos
Observatory (2200 a.s.l.) in the Canary Island of La Palma,
are placed on the top of a mountain, from where a window of visibility of
about $5^{\circ}$ in zenith and $80^{\circ}$ in azimuth is open in the
direction of the surrounding ocean. This allows to search for a signature
of particle showers induced by earth-skimming cosmic...
Pasquale Di Bari
(University of Southampton)
9/26/17, 11:20 AM
New physics at high-energy neutrino telescopes
Talk (20'+5')
Dr
Viviana Niro
(ITP, Heidelberg)
9/26/17, 11:45 AM
New physics at high-energy neutrino telescopes
Talk (20'+5')
We discuss a left-right symmetric extension of the Standard Model in which the three additional right-handed neutrinos play a central role in explaining the baryon asymmetry of the Universe, the dark matter abundance and the ultra energetic signal detected by the IceCube experiment. The energy spectrum and neutrino flux measured by IceCube are ascribed to the decays of the lightest...
Dr
Sergio Palomares-Ruiz
(IFIC (UV-CSIC))
9/26/17, 12:10 PM
New physics at high-energy neutrino telescopes
Talk (20'+5')
The discovery of the high-energy neutrino flux by the IceCube detector has motivated a large number of studies in the literature to unravel their origin, from different scenarios within standard cosmic-ray sources to more exotic possibilities. In this talk, I will describe the evolution of the HESE data of IceCube and their main features and I will present the results of statistical analyses...
36.
Neutrino lines produced by DM annihilation: a model-building perspective for neutrino telescopes
Prof.
Thomas Hambye
9/26/17, 12:35 PM
New physics at high-energy neutrino telescopes
Talk (20'+5')
In the near future, neutrino telescopes are expected to improve their sensitivity to the flux of monochromatic neutrinos produced by dark matter (DM) in our galaxy. This is illustrated by a new limit on the corresponding cross section that we derive from public IceCube data. In this context, we study which DM models could pro- duce an observable flux of monochromatic neutrinos from DM...
Dr
Francesco Vissani
(Gssi)
9/26/17, 2:30 PM
Francesco Lorenzo Villante
(AQ)
9/26/17, 2:55 PM
The interaction of cosmic rays with the gas contained in our Galaxy is a guaranteed source of diffuse high energy neutrinos. We provide expectations for this component by considering different assumptions for the cosmic ray distribution in the Galaxy which are intended to cover the large uncertainty in cosmic ray propagation models. We calculate the angular dependence of the diffuse galactic...
Dmitri SEMIKOZ
(APC, Paris)
9/26/17, 3:20 PM
In this talk I'll discuss significance of the galactic component observation in the 4 years IceCube data. Also I'll review theoretical models, which can explain observed data both with Galactic and extra-galactic sources of neutrinos. In particular, I'll present model which at the same time explain UHECR and astrophysical neutrinos.
Michael Kachelriess
(NTNU)
9/26/17, 3:45 PM
I review attempts to explain in a unified way the experimental data on ultrahigh energy neutrinos and cosmic rays, using a single source class and obeying data on CR composition and limits on the extragalactic diffuse gamma-ray background.
Dario Grasso
(PI)
9/26/17, 4:50 PM
Astrophysical sources and backgrounds
Talk (20'+5')
The Galaxy is a guaranteed source of neutrinos produced by the interaction of cosmic rays (CRs) with the interstellar gas. According to conventional CR propagation models, however, this emission may be too weak to be detected even by Km3-scale neutrino telescopes. This expectation has to be revisited in the light of recent Fermi-LAT findings showing that the CR spectrum in the inner Galactic...
Antonio Marinelli
(PI)
9/26/17, 5:15 PM
Astrophysical sources and backgrounds
Talk (20'+5')
In this work we present a detailed study of the high-energy neutrino flux expectation from different diffuse regions of our Galaxy, like the Central Molecular Zone (CMZ), the Galactic Ridge and the Fermi Bubbles. The TeV gamma-ray observations from the mentioned regions, suggest a careful modeling of this guaranteed neutrino factories. We consider a recently introduced cosmic-ray transport...
Dr
Irene Di Palma
(ROMA1)
9/26/17, 5:40 PM
Carlo Mascaretti
(GSSI)
9/26/17, 7:00 PM
Poster
Silvia Celli
(Gran Sasso Science Institute)
9/26/17, 7:00 PM
Poster
Marco Chianese
(NA)
9/26/17, 7:00 PM
Poster
Ms
Immacolata Carmen Rea
(TUM)
9/26/17, 7:00 PM
Poster
Pablo Fernandez De Salas
(IFIC (CSIC - UV))
9/26/17, 7:00 PM
Poster
Dr
Mattia Manfredonia
(Dipartimento di Fisica Ettore Pancini, Universita' di Napoli Federico II)
9/26/17, 7:00 PM
Poster
Giulia Pagliaroli
(GSSI)
9/26/17, 7:00 PM
Poster
Rosa Mele
(N)
9/26/17, 7:00 PM
Poster
