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2020 IPS Conference
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Astrophysics (theory)
Category:
Lectures for this program:
| Lecture Time | Speaker | Lecture subject |
|---|---|---|
| 16:00-16:13 | Mor Rozner |
The aeolian-erosion barrier for the growth of metre-size objects in protoplanetary-discs Aeolian-erosion is a destructive process which can erode small-size planetary objects through their interaction with a g... |
| 16:13-16:26 | Filip Samuelsson [1,2] |
The problematic connection between low-luminosity gamma-ray bursts and ultra-high-energy cosmic rays Ultra-high-energy cosmic rays (UHECR) are the most energetic particles ever observed, having energies extending beyond 1... |
| 16:26-16:39 | Michal Wagman[1] |
Retardation Theory: A New Approach to the Dark Matter Problem The Dark Matter paradigm is the current leading hypothesis for reconciling discrepancies between observational phenomena... |
| 16:39-16:52 | Mukesh K Vyas |
Comptonization of seed photons with relativistic electrons and spectra of pulsars We study the modification of radiation spectrum through external Comptonization with relativistic electrons having eithe... |
| 16:52-17:05 | Kuan-Chou Hou |
Virial shocks in galaxy clusters In the theory of structure formation in the Universe, galaxy clusters are thought to grow by accreting surrounding mater... |
| 17:05-17:18 | Santanu Mondal |
Simulating the Fermi Bubbles The Fermi bubbles (FBs) are two giant, non-thermal, bipolar lobes extending \sim50^o in latitude above and below the Gal... |
| 17:18-17:30 | Jonathan Freundlich |
Core formation in dark matter haloes and ultra diffuse galaxies by outflow episodes induced by feedback While cold dark matter numerical simulations predict steep, `cuspy' density profiles for dark matter halos, observations... |