Conveners
Plenary
- Gianfranco Bertone
Plenary
- Luca Grandi (The University of Chicago)
Plenary
- celine boehm
Plenary
- Emanuela Dimastrogiovanni (The University of New South Wales)
Plenary
- Miroslav Filipovic (Western Sydney University)
Plenary
- Francesca Calore (LAPTh, CNRS)
Plenary
- Michael Schmidt (UNSW Sydney)
Plenary
- Csaba Balazs (Monash University)
Plenary
- Jenni Adams (University of Canterbury)
Plenary
- Susumu Inoue (RIKEN)
-
celine boehm02/12/2019, 09:00Dark matterOral
Plenary talk
Go to contribution page -
Kalliopi Petraki (Sorbonne Université)02/12/2019, 09:30Dark matterOral
Plenary talk
Go to contribution page -
Luca Grandi (The University of Chicago)02/12/2019, 10:00Dark matterOral
Plenary talk
Go to contribution page -
Nicole Bell (University of Melbourne)02/12/2019, 11:00Dark matterOral
Plenary talk
Go to contribution page -
Jingjing ZANG (Purple Mountain Obsevatory,CAS)02/12/2019, 11:30Dark matterOral
Plenary talk
Go to contribution page -
Thomas Nathan Thorpe (Gran Sasso Science Institute (IT))02/12/2019, 12:00Dark matterOral
Dual phase noble liquid Time Projection Chambers (TPCs) offer a competitive and scalable way to search for dark matter directly via elastically scattering off of detector target nuclei and electrons. The Global Argon Dark Matter Collaboration (GADMC) is undertaking an ambitious global program from the extraction and purification of Underground Argon (UAr), depleted in 39Ar which reduces the...
Go to contribution page -
Gregory Lane (Australian National University)02/12/2019, 12:30Dark matterOral
For almost 20 years, the DAMA experiment has observed annual modulations
Go to contribution page
in the signal from heavily-shielded, ultra-pure NaI scintillator
crystals housed in the Gran Sasso underground laboratory. This
modulation is consistent with expectations for the motion of the earth
through a galactic dark matter halo, but is in conflict with results
from other dark matter direct detection... -
joseph silk (IAP)03/12/2019, 09:00Dark matterOral
Plenary talk
Go to contribution page -
Xuelei Chen (National Astronomical Observatories, Chinese Academy of Science)03/12/2019, 09:30CosmologyOral
Plenary talk
Go to contribution page -
Prof. Geraint Lewis (The University of Sydney)03/12/2019, 10:00Dark matterOral
Plenary talk
Go to contribution page -
Jan Hamann (The University of New South Wales)03/12/2019, 11:00CosmologyOral
Plenary talk
Go to contribution page -
Torsten Bringmann (University of Oslo)03/12/2019, 11:30CosmologyOral
Plenary talk
Go to contribution page -
Yvonne Wong (The University of New South Wales)03/12/2019, 12:00CosmologyOral
Plenary talk
Go to contribution page -
Shivani Bhandari03/12/2019, 12:30Extragalactic sourcesOral
Fast Radio Bursts (FRBs) which are exotic millisecond duration radio bursts, are currently the hot topic in the field of transient astronomy. The discovery of FRBs has stimulated a range of theoretical investigations to understand their origin and physics as well as observational efforts around the world to search for more such bursts. In the recent decade or so, we have learned a lot about...
Go to contribution page -
Tsvi Piran (The Hebrew University)04/12/2019, 09:00Extragalactic sourcesOral
Plenary talk
Go to contribution page -
Anne Green (University of Sydney)04/12/2019, 09:30Galactic sourcesOral
Plenary talk
Go to contribution page -
Prof. Yasunobu Uchiyama (Rikkyo University)04/12/2019, 10:00Galactic sourcesOral
Plenary talk
Go to contribution page -
Mikhail Malkov (UCSD)04/12/2019, 11:00Oral
Plenary talk
Go to contribution page -
Shunsaku Horiuchi (Virginia Tech)04/12/2019, 11:30Galactic sourcesOral
The center of the Milky Way galaxy provides a promising target to search for signatures of dark matter self-annihilation or decay into Standard Model particles. However, competing high-energy astrophysical processes are complex and must be modeled with care. I will review on-going studies of the so-called "Galactic Center Excess" discovered in Fermi-LAT data. I will discuss recent developments...
Go to contribution page -
Roland Crocker (Australian National University)04/12/2019, 12:00Galactic sourcesOral
Plenary talk
Go to contribution page -
Weiwei Xu (Shandong University (CN))04/12/2019, 12:30Dark matterOral
The Alpha Magnetic Spectrometer (AMS) was installed aboard the International Space Station on May 19, 2011. In eight years AMS has collected over 145 billion cosmic rays. AMS conducts searches for the origin of antimatter, dark matter, and new phenomena through the precision measurement of cosmic rays. The latest AMS results on cosmic ray positrons, electrons, antiprotons, protons, nuclei, and...
Go to contribution page -
Srubabati Goswami (physical research laboratory)05/12/2019, 09:00NeutrinosOral
Plenary talk
Go to contribution page -
Andrea Thamm (University of Melbourne (AU))05/12/2019, 09:30Particle physicsOral
Plenary talk
Go to contribution page -
Zurab Berezhiani (Univ. L'Aquila)05/12/2019, 10:00Particle physicsOral
Plenary talk
Go to contribution page -
Susan Scott05/12/2019, 11:00Gravitational waves and followupOral
Plenary talk
Go to contribution page -
Prof. Tara Murphy (University of Sydney)05/12/2019, 11:30Gravitational waves and followupOral
Plenary talk
Go to contribution page -
Kent Yagi05/12/2019, 12:00Gravitational waves and followupOral
Plenary talk
Go to contribution page -
Francesca Calore (LAPTh, CNRS)05/12/2019, 12:30Galactic sourcesOral
Plenary talk
Go to contribution page -
Dr Roberta Zanin (CTAO gGmbH)06/12/2019, 09:00Gamma raysOral
Very-high-energy (VHE) gamma-ray astroparticle physics is a relatively young field, and
Go to contribution page
observations over the past decade have surprisingly revealed almost two hundred VHE
emitters which appear to act as cosmic particle accelerators. These sources are an
important component of the Universe, influencing the evolution of stars and galaxies. At the
same time, they also act as a probe of... -
Dr Gavin Rowell (University of Adelaide)06/12/2019, 09:30Gamma raysOral
Astrophysical gamma-ray sources are sites of extreme particle acceleration. For gamma-ray sources in our galaxy, a key ingredient in understanding the nature of the underlying particles (leptons and/or hadrons) is knowledge of the interstellar gas (neutral and ionised), often traced by high frequency radio telescopes. For example, this gas can act as a target for cosmic ray collisions. In this...
Go to contribution page -
Gary Hill (University of Adelaide)06/12/2019, 10:00NeutrinosOral
The age of high energy neutrino astronomy has arrived, and the Universe has begun to reveal its secrets. IceCube has detected and characterised the astrophysical neutrino flux, and revealed evidence of the first source – the blazar TXS 0506+056 – which appears to be a cosmic particle accelerator. Upgraded and new detectors (IceCube Upgrade, KM3NET, IceCube-Gen2) are in various stages of...
Go to contribution page -
Troy Porter (Stanford University)06/12/2019, 11:00Cosmic raysOral
Cosmic ray data collected by experiments like Pamela, AMS-02, CALET, and
Go to contribution page
DAMPE show many spectral features that are not described by simple power
laws. These features may be giving information on the time-dependent
activity of individual cosmic ray sources, but the interpretation is
unclear. Because the same cosmic rays are interacting also in the
interstellar medium, these data are also... -
Bruce Dawson (University of Adelaide)06/12/2019, 11:30Cosmic raysOral
Plenary talk
Go to contribution page -
Zhen Cao (Institute of High Energy Physics, CAS, China)06/12/2019, 12:00Oral
Plenary talk
Go to contribution page -
Edna Ruiz-Velasco (MPIK)06/12/2019, 12:30
-
Elena Moretti (IFAE)06/12/2019, 12:45
-
Gianfranco Bertone06/12/2019, 13:00Dark matterOral
Plenary talk
Go to contribution page