Conveners
Plenary: I
- Gianfranco Bertone
Plenary: II
- Diego Blas Temino (CERN)
Plenary: III
- Teresa Montaruli
- Domenico Della Volpe (Universitè de Genève)
Plenary: IV
- Mathias Garny (CERN)
Plenary: V
- Martin Kunz (Unknown)
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Christoph Renner (Université de Genève), Eckhard Elsen (CERN)12/09/2016, 09:20Invited Contributions
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Margherita Primavera (Univ. + INFN), Margherita Primavera (Universita del Salento (IT))12/09/2016, 09:50
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Francesco Costanza (Deutsches Elektronen-Synchrotron (DE))12/09/2016, 10:10
With the increase in center-of-mass energy, a new energy frontier has been opened by the Large Hadron Collider. More than 25 fb^-1 of proton-proton collisions at sqrt(s)=13 TeV have been delivered to both ATLAS and CMS experiments during 2016. This enormous dataset can be used to test the Standard Model in a complete new regime with tremendous precision and it has the potential to unveil new...
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Ulrich Andreas Haisch (University of Oxford (GB))12/09/2016, 11:00
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Marc Schumann (University of Bern)12/09/2016, 11:30
There is overwhelming indirect evidence that dark matter exists, however, the dark matter particle has not yet been directly detected in laboratory experiments. In order to be able to identify the rare dark matter interactions with the target nuclei, such instruments have to feature a very low threshold and an extremely low radioactive background. They are therefore installed in underground...
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Igor Garcia Irastorza (Universidad de Zaragoza (ES))12/09/2016, 12:00
Axions are a natural consequence of the Peccei-Quinn mechanism, the most compelling solution to the strong-CP problem. Similar axion-like particles (ALPs) also appear in a number of possible extensions of the Standard Model, notably in string theories. Both axions and ALPs are very well motivated candidates for the Dark Matter, and in addition would be copiously produced at the stellar cores....
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Bruce Allen (Max Planck Society/Albert Einstein Institute Hannover)13/09/2016, 09:30
This talk follows announcements earlier this year by the LIGO and Virgo Scientific Collaborations, based on data from the first
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four-month observing run the advanced LIGO gravitational wave
detectors (aLIGO). In two instances, on 14.9.2015 and on 26.12.2015, we have directly detected the gravitational waves emitted by the final orbits and merger of massive black hole binary systems. I... -
Scott Hughes (Massachusetts Institute of Technology)13/09/2016, 10:00
In the past year, the LIGO-Virgo Collaboration announced the first secure detection of gravitational waves. This discovery heralds the beginning of gravitational wave astronomy: the use of gravitational waves as a tool for studying the dense and dynamical universe. In this talk, I will describe the full spectrum of gravitational waves, from Hubble-scale modes, through waves with periods of...
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Naoko Kurahashi (Drexel University)13/09/2016, 11:00
Abstract: IceCube's discovery of a diffuse flux of astrophysical neutrinos started a new era of neutrino astronomy.I will review the multiple diffuse analyses in IceCube that observe the astrophysical flux, and what each can tell us. Then I will focus on spatial analyses that aim to identify the sources of such astrophysical neutrinos. This will be followed by an attempt to reconcile all...
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Mark Vagins (Kavli IPMU/UTokyo)13/09/2016, 11:30
A core-collapse supernova is a nearly perfect neutrino bomb. While capable of outshining its entire host galaxy, this stunning light show represents just a small portion of the explosion. Indeed, each such cataclysmic event typically radiates two orders of magnitude more energy as low-energy neutrinos than it does as electromagnetic radiation or as kinetic shockwaves. Consequently, MeV-scale...
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Thomas Gaisser (Bartol Research Institute)13/09/2016, 12:00
The discovery of astrophysical neutrinos at high energy by IceCube raises a host of questions: What are the sources? Is there a Galactic as well as an extragalactic component? How does the astrophysical spectrum continue to lower energy where the dominant signal is from atmospheric neutrinos? Is there a measureable flux of cosmogenic neutrinos at higher energy? What is the connection to cosmic...
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Julie McEnery (NASA)14/09/2016, 09:30
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Lukasz Stawarz (Jagiellonian University)14/09/2016, 10:00
During the last decades, various classes of radio-loud active galactic nuclei have been established as sources of high-energy radiation extending over a very broad range from soft gamma-rays (photon energies E~MeV) up to very-high-energy gamma-rays (E>100 GeV). These include blazars of different types, as well as young and evolved radio galaxies. The observed gamma-ray emission from such...
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Stefano Gabici14/09/2016, 11:00
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Christoph Weniger (University of Amsterdam)14/09/2016, 11:30
Many theoretical ideas for the particle nature of dark matter exist. The most popular models often predict that dark matter particles self-annihilate or decay, giving rise to potentially detectable signatures in astronomical observations. I will summarize the current status of searches for such signatures and critically reassess recent claims for dark matter signals. I will further provide...
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Frank Linde (Nikhef National institute for subatomic physics (NL))14/09/2016, 12:00
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Julien Lesgourgues (TTK, RWTH Aachen University)15/09/2016, 09:30
The next generation of cosmological surveys (of large scale structures, CMB polarisation, 21cm line), approved (Euclid, SKA, ...) or submitted (COrE+, LiteBird), have the potential to return a lot of relevant information for particle physics. I will present and comment some of the most recent sensitivity forecasts related to neutrino physics, light relics and Dark Matter properties.
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Jesús Zavala Franco15/09/2016, 10:00
Although there is substantial gravitational evidence for the existence of dark matter, its particle nature remains one of the biggest mysteries in modern physics. The favourite theoretical model, Cold Dark Matter (CDM), assumes that non-gravitational dark matter interactions are irrelevant for galaxy formation and evolution.
Surprisingly, current astronomical observations allow significant...
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Stefan Schael (Rheinisch-Westfaelische Tech. Hoch. (DE))15/09/2016, 11:00
The Alpha Magnetic Spectrometer, AMS, is a general purpose high energy particle phys- ics detector. It was installed on the International Space Station, ISS, on 19 May 2011 to conduct a unique long duration mission of fundamental physics research in space. Knowledge of the precise rigidity dependence of the proton and helium flux is important in understanding the origin, acceleration, and...
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Torii Shoji15/09/2016, 11:30
The CALorimetric Electron Telescope (CALET) on the International Space Station is an experiment
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aimed at precise measurements of the various components of the cosmic-ray spectrum. Its main
scientific goal is to measure the electron + positron flux above 1 GeV and to explore the TeV region
where the energy resolution is of the order of 2-3%, which can provide valuable data for dark... -
Roger Blandford (Stanford University)15/09/2016, 12:00
Over the past decade, gamma ray astrophysics has entered the astrophysical mainstream. Extremely successful space-borne (GeV) and ground-based (TeV) detectors, combined with a multitude of partner telescopes, have revealed a fascinating “astroscape" of active galactic nuclei, pulsars, gamma ray bursts, supernova remnants, binary stars, star-forming galaxies, novae much more, exhibiting major...
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Ralf Matthias Ulrich (KIT - Karlsruhe Institute of Technology (DE))16/09/2016, 09:30
Many LHC measurements are already used to improve hadronic interaction models used in cosmic ray analyses. This already had a positive effect on the model dependence of crucial data analyses. Some of the data and the model tuning is reviewed. However, the LHC still has a lot more potential to provide crucial information. Since the start of Run2 the highest accelerator beam energies are reached...
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Xin Wu (Universite de Geneve (CH))16/09/2016, 10:00
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Fiorenza Donato (INFN - National Institute for Nuclear Physics)16/09/2016, 11:00
The data we are receiving from galactic cosmic rays are reaching an unprecedented precision, over very wide energy ranges. Nevertheless, many problems are still open, while new ones seem to appear when data happen to be redundant. We will discuss some paths to possible progress in the theoretical modelling and experimental exploration of the galactic cosmic
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radiation. -
Michelangelo Mangano (CERN)16/09/2016, 11:30
I outline the goals of the future LHC programme, and the current understanding of the physics potential of the possible next generation of lepton and hadron colliders.
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16/09/2016, 12:00