New Physics and Astrophysical Searches for Dark Matter
APA
Profumo, S. (2015). New Physics and Astrophysical Searches for Dark Matter . Perimeter Institute. https://pirsa.org/15050032
MLA
Profumo, Stefano. New Physics and Astrophysical Searches for Dark Matter . Perimeter Institute, May. 05, 2015, https://pirsa.org/15050032
BibTex
@misc{ pirsa_PIRSA:15050032, doi = {10.48660/15050032}, url = {https://pirsa.org/15050032}, author = {Profumo, Stefano}, keywords = {Particle Physics}, language = {en}, title = {New Physics and Astrophysical Searches for Dark Matter }, publisher = {Perimeter Institute}, year = {2015}, month = {may}, note = {PIRSA:15050032 see, \url{https://pirsa.org}} }
Can we learn about New Physics with astronomical and astro-particle data? Understanding how this is possible is key to unraveling one of the most pressing mysteries at the interface of cosmology and particle physics: the fundamental, particle nature of the dark matter.
I will discuss some of the recent puzzling findings in astro-particle and astronomical observations that might be related to signals from dark matter. I will first review the status of explanations to the cosmic-ray positron excess, emphasizing how we might be able to discriminate between astrophysical sources and dark matter.
I will then discuss the evidence for an X-ray line at 3.5 keV, and present new results on systematic effects and on the role of previously underestimated astrophysical lines.
Finally, I will discuss a reported excess of gamma rays from the central regions of the Galaxy. I will address the question of whether we are possibly observing a signal from dark matter annihilation, how to test this hypothesis, and which astrophysical mechanisms constitute the relevant background.