Astronomy Colloquium - Tim Linden

Crab Nebula [NASA Chandra]
November 8, 2018
4:00PM - 5:00PM
1005 Smith Lab

Date Range
2018-11-08 16:00:00 2018-11-08 17:00:00 Astronomy Colloquium - Tim Linden The Rise of the Leptons: Emission from Pulsars will Dominate the next Decade of TeV Gamma-Ray AstronomyTim Linden - The Ohio State UniversityHAWC observations have detected extended TeV emission coincident with the Geminga and Monogem pulsars. In this talk, I will show that these detections have significant implications for our understanding of pulsar emission. First, the spectrum and intensity of these “TeV Halos” indicates that a large fraction of the pulsar spindown energy is efficiently converted into electron-positron pairs. This provides observational evidence necessitating pulsar interpretations of the rising positron fraction observed by PAMELA and AMS-02. Second, the isotropic nature of this emission provides a new avenue for detecting nearby pulsars with radio beams that are not oriented towards Earth. Third, these observations indicate that the total emission from unresolved pulsars produces the majority of the TeV gamma-ray flux observed from the Milky Way. 1005 Smith Lab America/New_York public

The Rise of the Leptons: Emission from Pulsars will Dominate the next Decade of TeV Gamma-Ray Astronomy

Tim Linden - The Ohio State University

HAWC observations have detected extended TeV emission coincident with the Geminga and Monogem pulsars. In this talk, I will show that these detections have significant implications for our understanding of pulsar emission. First, the spectrum and intensity of these “TeV Halos” indicates that a large fraction of the pulsar spindown energy is efficiently converted into electron-positron pairs. This provides observational evidence necessitating pulsar interpretations of the rising positron fraction observed by PAMELA and AMS-02. Second, the isotropic nature of this emission provides a new avenue for detecting nearby pulsars with radio beams that are not oriented towards Earth. Third, these observations indicate that the total emission from unresolved pulsars produces the majority of the TeV gamma-ray flux observed from the Milky Way.

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