'Galactic rotation curves' presentation slideshows

The Observational Case For 7-8 GeV Dark Matter : Fermi, CoGeNT and DAMA

849 views • 72 slides

Gravitational Lensing: How to See the Dark

Gravitational Lensing: How to See the Dark. J. E. Bjorkman University of Toledo Department of Physics & Astronomy. The Dark Between the Light. Dark Matter. How do we know its there? Answer: It affects the motion of everything we can see. Cluster Simulation Rotation Velocities.

528 views • 36 slides

The Energy in our Universe

446 views • 30 slides

New Horizons Carlo Rubbia

New Horizons Carlo Rubbia. Fifty years after the Neutrino experimental discovery III International Workshop on: "Neutrino Oscillations in Venice". Cosmology : a few established facts.

331 views • 25 slides

DARK MATTER & GALACTIC ROTATION

2012. ASTRO SUMMER SCHOOL. DARK MATTER & GALACTIC ROTATION. In 1933, Fritz Zwicky calculated the mass of the Coma Cluster. More evidence was discovered by Vera Rubin who measured the rotation curves of many galaxies during the 1970s. The expected distribution of dark matter in the Milky Way.

460 views • 19 slides

Dark Matter in Cosmology

Dark Matter in Cosmology. Alessandro Palma Dottorato in Fisica XXII ciclo Corso di Cosmologia Prof. A. Melchiorri. Outlook. Why does Cosmology need Dark Matter (DM)? gravitational data from Galaxies and Clusters structure formation in the Universe lensing DM: observed relic density

288 views • 14 slides