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Nuria Rius (Valencia University)02/12/2022, 10:00
I will discuss recent work about the possibility of Dark Matter interacting only gravitationally in extra dimensional scenarios.
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Maxim Laletin02/12/2022, 10:40
We study a novel dark matter (DM) production mechanism based on the freeze-in through the inverse of semi-annihilation process. A peculiar feature of this scenario is that the production rate is suppressed by a small initial abundance of DM and consequently creating the observed abundance requires much larger coupling values than for the usual freeze-in. We provide a concrete example model...
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Prof. Malcolm Fairbairn (Physics, King's College London)02/12/2022, 11:25
We consider axion stars which may explode at early times, changing the ionisation history of the Universe. We will explain the concept, the calculation and the constraints on parameter space.
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Alexander C Jenkins (University College London)02/12/2022, 12:05
Next-generation gravitational-wave (GW) observatories will provide exquisite measurements of the merger rate of high-redshift binary black holes (BBHs), detecting many thousands of these systems every year. The abundance of these binaries is a direct tracer of the early stages of star formation, and therefore of cosmic structure formation. This opens the possibility of using GW observations to...
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Gonzalo Herrera02/12/2022, 12:20
In this talk, I will discuss the attenuation of high energy neutrinos and photons produced in a blazar when they propagate through the dark matter spike around the central black hole and the halo of the host galaxy. In particular, I will discuss new constraints on the dark matter-neutrino and dark matter-photon scattering cross sections obtained from the observation by IceCube of a few...
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Julien Lesgourgues (TTK, RWTH Aachen University)
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