Conveners
Plenary
- Jisuke Kubo (Kanazawa University)
Plenary
- Jun'ichi Yokoyama (The University of Tokyo)
Plenary
- Nicole Bell (University of Melbourne)
Plenary
- Gary Hill (University of Adelaide)
Plenary
- Christian Reichardt (University of Melbourne)
Plenary
- mihoko nojiri (KEK)
Plenary
- Antoine David Kouchner (Universite de Paris VII (FR))
Plenary
- Matthieu TRISTRAM (CNRS)
Plenary
- Csaba Balazs (Monash University)
Plenary
- Sang Pyo Kim (Kunsan National University)
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28/11/2016, 08:45
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Prof. David McClelland (ANU)28/11/2016, 09:00
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Shinji Tsujikawa (Tokyo University of Science)28/11/2016, 09:30
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Dr David Parkinson (University of Queensland)28/11/2016, 10:00
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Prof. Wei Wang (Sun Yat-Sen University)28/11/2016, 11:00
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Prof. Tsutomu Yanagida (University of Tokyo)28/11/2016, 11:30
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Jihn E. Kim (Kyung Hee University)28/11/2016, 12:00
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Paolo Gondolo (University of Utah)29/11/2016, 09:00
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Prof. Manfred Lindner (Max Planck Institut fuer Kernphysik, Heidelberg, Germany)29/11/2016, 09:30
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Lisa Randall (Harvard)29/11/2016, 10:00
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Roland Crocker (Australian National University)29/11/2016, 11:00
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Mercedes Paniccia (Universite de Geneve (CH))29/11/2016, 11:30
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Dr Jose Bellido (The University of Adelaide)29/11/2016, 12:00
Description of the Pierre Auger cosmic ray detector
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Measurements of the energy spectrum, the arrival directions and the mass composition.
Searches for high energy photons, neutrons, neutrinos and high energy magnetic monopoles. -
Prof. Misao Sasaki (Kyoto University)30/11/2016, 09:00
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Silvia Galli30/11/2016, 09:30
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Geraint Lewis (The University of Sydney)30/11/2016, 10:00
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Pat Scott (Imperial College)30/11/2016, 11:00
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Millie McDonald (University of Melbourne (AU))30/11/2016, 11:30
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Chia-Ming Kuo (National Central University (TW))30/11/2016, 12:00
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Alexander Kusenko01/12/2016, 09:00
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Clancy James (University of Erlangen-Nuernberg)01/12/2016, 09:30
ARCA (Astroparticle Research with Cosmics in the Abyss) is the high-energy neutrino telescope being built as part of the KM3NeT deep-sea research infrastructure. Optimised for a high angular resolution to neutrinos in the TeV-PeV regime, its main physics goals are the exploration of the high-energy astrophysical neutrino signal reported by IceCube, and the discovery of Galactic neutrino...
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Prof. Jenni Adams (University of Canterbury)01/12/2016, 10:00
The IceCube Neutrino Observatory is the world’s largest neutrino detector. Located at the South Pole, IceCube consists of a cubic kilometre of ice instrumented with 5160 photomultiplier tubes on 86 strings at a depth of 1.5-2.5 km. In this talk I will present the latest results concerning the high-energy neutrinos detected by IceCube. Plans for a next-generation IceCube detector, named...
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Prof. Eric Linder (UC Berkeley)01/12/2016, 11:00
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Dr Arman Shafieloo (KASI Daejeon)01/12/2016, 11:30
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David Wiltshire (University of Canterbury)01/12/2016, 12:00
The present epoch Universe is inhomogeneous on < 100/h Mpc scales, opening up the possibility of backreaction - that average cosmic expansion is significantly different from that of the standard FLRW geometry at late epochs. Realizing this possibility means confronting unsolved open questions in general relativity, in particular the nonlocal nature of gravitational energy in coarse-graining...
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Dr Regina Caputo (University of California, Santa Cruz)02/12/2016, 09:00
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Gavin Rowell (University of Adelaide)02/12/2016, 09:30
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Prof. Tamara Davis (University of Queensland)02/12/2016, 10:00
The Dark Energy Survey (DES) is in its fourth year of a five year observing program. We’re on our way to mapping 300 million galaxies and measuring 3000 type Ia supernovae for dark energy studies as well as monitoring 800 Active galaxies so we can use reverberation mapping to measure supermassive black hole masses across the last 12 billion years (to z~4). Over 525 nights DES combines a...
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Elisabetta Barberio (University of Melbourne (AU))02/12/2016, 11:00
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Raymond Volkas (The University of Melbourne)02/12/2016, 11:30
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02/12/2016, 12:00