Laura Eisenberger

Since 01/10/2024:
PhD candidate at the Institute for Theoretical Physics and Astrophysics / Chair of Astronomy of the Julius-Maximilians-University, Würzburg, Germany
Supervisor: Dr. Thomas Siegert

01/04/2021 – 29/01/2024:
Physics studies (M.Sc.) at Julius-Maximilians-University, Würzburg, Germany

15/09/2017 – 31/03/2021:
Physics studies (B.Sc.) at Julius-Maximilians-University, Würzburg, Germany

30/06/2017:
Abitur, Werner-von-Siemens-Gymnasium, Weißenburg, Germany

18/07/1999:
Born in Weißenburg i. Bay., Germany

The MeV Signature of Cold Dark Matter Annihilation

Use the full high-energy spectral energy distribution of secondary and tertiary photons, resulting from the interaction of charged dark matter (DM) annihilation products, together with prompt emission and compare this model to INTEGRAL/SPI and Fermi/LAT data:

	Prompt and secondary DM emission model

Consider all observed Local Volume Galaxies as unbiased tracers of the DM distribution:

Construct the cosmic gamma-ray background and its angular power spectrum in the MeV range to explore the potential of the expected COSI data.