14-17 October 2024
Union South, University of Wisconsin–Madison
US/Central timezone

Are Supernova Remnants as Cosmic Ray Factories? Yes, but…

16 Oct 2024, 16:00
45m
Northwoods Room (Union South, University of Wisconsin–Madison)

Northwoods Room

Union South, University of Wisconsin–Madison

1308 West Dayton Street

Speaker

Damiano Caprioli (University of Chicago)

Description

First-principles plasma simulations have been pivotal in helping developing a theory of ion and electron acceleration at shocks, and in particular in SNRs. I discuss what we have learned about particle acceleration efficiency, spectra, and maximum energy, and contrast these results with multi-wavelength emission from SNRs. Despite compelling evidence of hadron acceleration in these sources, there are both theoretical and observational open questions that prevent us from claiming that SNRs can accelerate CRs up to the knee.

Primary author

Damiano Caprioli (University of Chicago)

Presentation Materials