Venues for the plenaries and parallel sessions: Auditorio Novo 1 (Physics), Sala Jayme Tiomno (Physics), Auditorio G (IAG)
Welcome and plenary talks
Venue: Auditorio Novo 1 (Physics, Main Building, ground floor)
09:20-09:30 | Coordinators | Welcome |
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09:30-10:00 | Masahide Yamaguchi | Why do we still consider dynamical models of dark energy ? |
10:00-10:30 | Horatiu Nastase | Solving cosmology puzzles with holographic cosmology |
10:30-11:00 | Coffee break | |
11:00-11:30 | Masami Ouchi | Cosmic reionization and galaxy formation over the history of the Universe |
11:30-12:00 | Ivone Albuquerque | The DarkSide Experiment: Venturing into the low mass region |
12:00-12:30 | Alex Wuensche de Souza | The BINGO Telescope: update status review |
14:00-14:30 | Teruaki Suyama | Primordial black holes - perspectives in gravitational-wave astronomy |
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14:30-15:00 | Roderik Overzier | The growth history of supermassive black holes |
15:00-15:30 | Tomo Takahashi | Probing the early Universe with 21cm line |
15:30-16:00 | Coffee break | |
16:00-16:30 | Elcio Abdalla | Whispers of the Universe: theoretical and observational developments in the BINGO project |
16:30-17:00 | Fabio Iocco | Determining the distribution of Dark Matter in the Milky Way |
17:00-17:30 | Hidenobu Yajima | Cosmological simulations of galaxy formation in protocluster regions |
Morning: plenaries, discussion session and parallel sessions;
afternoon: external activities; evening: dinner
Venue: Auditorio Novo 1 (Physics, Main Building, ground floor)
09:30-10:00 | Daisuke Yamauchi | Cosmology and dark energy with future HI galaxy surveys |
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10:00-10:30 | Elisa Ferreira | Unified Superfluid Dark Sector |
10:30-10:50 | Raul Abramo | The interplay between the dark sector and galaxy evolution |
10:50-11:15 | Coordinators | Discussion |
11:15-11:45 | Coffee break |
Dark Matter (Auditorio Novo 1) | Dark Energy (Sala Jayme Tiomno) | |
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11:45-12:10 | Yuichiro Tada
Aspects of primordial black hole as dark matter |
Toyokau Sekiguchi
Probing dark energy with redshifted 21cm line observations |
12:10-12:35 | Edivaldo Moura Santos
Anisotropies in the flux of ultra-high energy cosmic rays |
Karin Fornazieri
BINGO forecasting for non-gaussian features in 21cm intensity mapping |
12:35-13:00 | Kazumi Kashiyama
Detectability of Small-Scale Dark Matter Clumps with Pulsar Timing Arrays |
Carolina Queiroz
Quasars and large-scale structure |
Morning: parallel sessions;
afternoon: Astronomy Colloquium & parallel sessions
Venues: Auditorio Novo 1 and Sala Jayme Tiomno (Physics); Auditorium G and Auditorium 2 (Astronomy)
Dark Matter (Auditorio Novo 1) | Galaxies (Sala Jayme Tiomno) | |
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09:30-09:55 | Ippei Obata
Optical Interferometric Search for Axion Dark Matter |
Antonio Montero-Dorta
The halo-galaxy connection |
09:55-10:20 | Tomohiro Fujita
Search for Axion Dark Matter with New Approaches |
Jun Toshikawa
Systematic Study of Protoclusters Based on Wide-field Survey |
10:20-10:45 | María Beníto Castaño
Searching for new physics (and DM): implications of uncertainties in the determination of DM distribution in the Milky Way |
Ken Mawatari
Panoramic view of large-scale structure of galaxies and surrounding gas in a high-redshift proto-cluster |
10:45-11:00 | Coffee break | |
11:00-11:25 | Naoya Kitajima
Axion dark matter in a neutron star magnetosphere |
Henrique Xavier
Stellar systematics in photometric galaxy surveys and applications to WISExSuperCOSMOS catalog |
11:25-11:50 | Aion Viana
Indirect searches of dark matter with gamma-rays |
Sunmyon Chon
Formation of the super massive black hole in the cosmological simulation |
11:50-12:15 | Fabio Chibana
Redshift space distortions in the presence of non-minimally coupled dark matter |
Cristina Furlanetto
Strong lensing and ALMA: resolving the nature of high-redshift galaxies detected by Herschel |
Dark Energy (Auditorio Novo 1) | Galaxies (Astronomy Auditorium 2) | |
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15:30-15:55 | Rampei Kimura
New aspects of massive gravity |
Rogerio Monteiro
Merging galaxy clusters and the search for self-interacting dark matter |
15:55-16:20 | Antonino Troja
Non-Gaussian likelihood: why we don't need covariance to estimate cosmological parameters |
Singo Hirano
Environmental dependence of the first star formation |
16:20-16:45 | Yuki Sakakihara
Cosmological solutions in bounded curvature models |
Oli Dors Jr.
The nature of high-z Ly-alpha emitters |
16:45-17:10 | Larissa Santos
Reconstructing the CMB B-mode power spectrum using the ABS method |
Kohji Tsumura
Observation of the Cosmic Infrared Background from the outside of the Solar system |