Conveners
Indirect Dark Matter searches
- Carlos Perez de los Heros (Uppsala University)
- Manuela Vecchi
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Roberto Aloisio (INFN)08/09/2022, 13:30
We will review the theoretical basis and models of Super Heavy Dark Matter and the search for signatures of their decay in the Auger Observatory data. From the lack of signal, it is possible to derive very stringent limits on the model parameters that connect the Auger Observatory data with cosmological models of the early universe and physics beyond the standard model.
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Nadir Marcelli (Istituto Nazionale di Fisica Nucleare)08/09/2022, 13:50
GAPS (General Anti-Particle Spectrometer) is a balloon-borne experiment designed to measure low-energy (< 0.25 GeV/n) cosmic antinuclei (i.e., antiprotons, antideuterons, and antihelium nuclei) as a signature of dark matter annihilation or decay. The experiment will conduct a series of long-duration balloon flights at high altitudes from Antarctica. According to viable beyond-the-Standard...
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Alejandra Aguirre-Santaella (Instituto de Física Teórica UAM-CSIC)08/09/2022, 14:10
In this work, we carry out a suite of specially-designed numerical simulations to shed further light on dark matter (DM) subhalo survival at mass scales relevant for gamma-ray DM searches, a topic subject to intense debate nowadays. Specifically, we have developed and employed an improved version of DASH, a GPU $N$-body code, to study the evolution of low-mass subhaloes inside a Milky Way-like...
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Joanna Berteaud (LAPTh, CNRS)08/09/2022, 14:30
For more than 20 years, the Compton telescope (COMPTEL) had provided the best measurments of the Galactic diffuse MeV spectrum. Recently, our analysis of 16 years of data from the SPectrometer on INTEGRAL (SPI) [Siegert et. al (2022)] measured this emission with a higher signal-to-noise ratio. At MeV energies, the dominant contribution to the diffuse emission comes from inverse Compton...
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Dr Ilias Cholis (Oakland University)08/09/2022, 14:50
The Galactic center excess (GCE) remains one of the most intriguing discoveries from the Fermi Large Area Telescope (LAT) observations. I will revisit characteristics of the GCE tested under an updated set of high-resolution galactic diffuse gamma-ray emission templates. This diffuse emission, which accounts for the bulk of the observed gamma rays, is ultimately due to cosmic-ray interactions...
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Celine Armand (University of Geneva)08/09/2022, 15:10
Cosmological and astrophysical probes suggest that dark matter (DM) would make up for 85% of the total matter content of the Universe. However, the determination of its nature remains one of the greatest challenges of fundamental physics. Assuming the $\Lambda$CDM model, Weakly Interacting Massive Particles (WIMPs) would annihilate into Standard Model particles, such as $\gamma$ rays, which...
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