The Heavy Composition of UHECR p (A,Z) Based on work with: Dan - PowerPoint PPT Presentation

Apr 14, 2023 •149 likes •386 views

The Heavy Composition of UHECR p (A,Z) Based on work with: Dan Hooper Subir Sarkar + astro-ph/0910.1842 astro-ph/1007.1306 e UHECR Air Showers UHECR Air Showers Recent Measurements of Moments by Auger Interpretation

The Heavy Composition of UHECR p γ (A,Z) Based on work with: Dan Hooper Subir Sarkar + astro-ph/0910.1842 astro-ph/1007.1306 γ γ γ γ e
UHECR Air Showers
UHECR Air Showers
Recent Measurements of Moments by Auger
Interpretation - What Does this Mean for Source Composition? Assume Source Energy Distribution: Spectral index and max energy are considered in the range: + Assume Sources have a uniform Spatial Dist.
Iron Only Composition? hard to fit both of these simultaneously for Iron
Iron Only Composition? Cause of difficulty in fitting both and simultaneously for Iron
Silicon Only Composition? reasonable fits obtained, though hard spectral index required is worrying
Nitrogen Only Composition? poor spectral fit is a problem for Nitrogen only composition
Nitrogen Only Composition? reason poor spectral fit is a problem for Nitrogen only composition
(Silicon) Magnetic Field- B=0 G
(Silicon) Magnetic Field- B=0.1 nG
(Silicon) Magnetic Field- B=0.3 nG
Other Handles on the UHECR Composition Nitrogen (Z=7) Silicon (Z=14) Iron (Z=26)
Other Handles on the UHECR Composition Nitrogen (Z=7) Silicon (Z=14) Iron (Z=26) Basically proportional to Z/A for a E max >>E GZK
Other Handles on the UHECR Composition Nitrogen (Z=7) Silicon (Z=14) Iron (Z=26)
Other Handles on the UHECR Composition Nitrogen (Z=7) Silicon (Z=14) Iron (Z=26)
Summary If pure composition at source is assumed: Heavy(ish) composition required; Difficult to get good agreement with Iron only composition to both and data; The presence of a ~0.1 nG extragalactic magnetic fields can help improve fits; The UHECR photon fraction has some potential to differentiate the composition.
Extra Slides
Mixed Composition Scenario? 50 % protons + 50% Silicon
Proton Only Scenario Still Possible? work by Ulrich et al. Change Interaction (Karlsruhe) Properties: astro-ph/0906.0418 1) cross-section 2) multiplicity 3) elasticity Modify these properties with logarithmic scaling from values at 10 18 eV
Change Interaction Properties: 1) cross-section
A Challenge for this Interpretation- muons

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