Conveners
Afternoon session: Dark Matter Galactic Center
- Aldo Treves (Università Insubria)
Afternoon session: TBD
- Piero Rosati
Afternoon session
- Gregory Vereshchagin (ICRANet)
Afternoon session
- She-Sheng Xue (ICRANet, Physics Department, Sapienza University of Rome)
Afternoon session
- Yerlan Aimuratov (Fesenkov Astrophysical Institute / al-Farabi Kazakh National University)
Afternoon session
- Liang Li (ICRANet, Piazza della Repubblica 10, I-65122 Pescara, Italy)
Afternoon session
- Maria Dainotti (National Astronomical Observatory of Japan)
Afternoon session
- Carlos Raúl Argüelles (Universidad Nacional de La Plata)
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Rafael Yunis05/07/2022, 17:00
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Massimo Meneghetti06/07/2022, 15:00
I will discuss how strong lensing can be used to constrain the small-scale structure of galaxy clusters. I will discuss how recent observational results compare with predictions from numerical hydrodynamical simulations. In particular, I will show that current simulations in the context of the LCDM cosmological model fail to reproduce the observed abundance of galaxy-galaxy strong lensing...
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Valentina Crespi06/07/2022, 15:45
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José Fernando Rodriguez Ruiz07/07/2022, 15:00
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Prof. Johann Rafelski08/07/2022, 15:00
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Tsvi Piran (The Hebrew University)11/07/2022, 15:00
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Nikolaos Mavromatos (King's College London, Physics Department)11/07/2022, 15:45
I discuss a string inspired model of cosmology, characterised by
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gravitational anomalies and torsion, in the early stages,
which may provide a geometric origin of the entire dark sector of the
Universe, from a running-vacuum-model inflation to
axionic dark matter, the axion degrees of freedom being associated with
torsion. During inflation, the model may, under some circumstances, lead... -
Vahe Petrosian11/07/2022, 17:00
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Eleonora Troja (NASA/GSFC)12/07/2022, 15:00
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Bing Zhang (University of Nevada, Las Vegas)12/07/2022, 17:00
I will review the observational facts, the current theoretical framework, and the open questions in the studies of fast radio bursts, a type of mysterious transients prevailing in the radio sky.
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Laura Becerra Bayona13/07/2022, 15:45
In the IGC paradigm, a carbon-oxygen star (COcore) collapses and explodes in a supernova (SN), the material ejected in the explosion is gravitational attracted by its companion, a neutron star (NS), taking place a hypercritical accretion process onto it. For compact systems, the accretion rate could be enough high to lead the NS to reach its critical mass, collapse in a black hole (BH) and...
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13/07/2022, 17:00
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Chris Fryer (Los Alamos National Laboratory)14/07/2022, 15:45
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Jorge Armando Rueda Hernandez (ICRANet), Remo Ruffini (ICRANet, ICRA, INAF)14/07/2022, 17:00
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Liang Li (ICRANet, Piazza della Repubblica 10, I-65122 Pescara, Italy)