Year: 2022

TERRIFIC PRIMER. “Dark Matter in Astrophysics/Cosmology” by Anne M. Green, School of Physics and Astronomy, University of Nottingham. https://lnkd.in/e6ifiQMn View in LinkedIn

THE SLANT. “These lecture notes aim to provide an introduction to dark matter from the perspective of astrophysics/cosmology.” https://lnkd.in/e6ifiQMn View in LinkedIn

THE START. “We look at the observational evidence for dark matter, from observations of galaxies, galaxy clusters, the anisotropies in the cosmic microwave background radiation and large scale structure.” https://lnkd.in/e6ifiQMn View in LinkedIn

BACKGROUND. “A brief introduction to cosmology, at the level of an undergraduate/bachelors course, focusing on the topics that are most relevant for DM.” (DM = dark matter). https://lnkd.in/e6ifiQMn View in LinkedIn

THE BEAST. “We move on to the observational evidence for cold, non-baryonic dark matter, on scales ranging from individual galaxies to the Universe as a whole. Understanding the distribution of DM, in particular within the Milky Way, is crucial for its detection.” (DM = dark matter). https://lnkd.in/e6ifiQMn View in LinkedIn

THE WORLD AS WE DO NOT KNOW IT. “Some in quantum physics have have stated that information absolutely travels from future to past as well as from past to future.” https://lnkd.in/ezYv-wzR View in LinkedIn

Distant stars captured by Hubble could so easily be the internal anatomy of a greater creature. https://lnkd.in/eWq3Y_st View in LinkedIn

TUTORIAL. “We look at what observations can tell us about the nature of DM, focusing on warm and self-interacting DM.” (DM = dark matter). https://lnkd.in/e6ifiQMn View in LinkedIn

DISTRIBUTION. “To detect dark matter we need to know how it’s distributed, in particular in the Milky Way, so next we overview relevant results from numerical simulations and observations.” https://lnkd.in/e6ifiQMn View in LinkedIn

TWO TYPES. “Finally, we conclude by looking at what astrophysical and cosmological observations can tell us about the nature of dark matter, focusing on two particular cases: warm and self-interacting dark matter.” https://lnkd.in/e6ifiQMn View in LinkedIn