TeV Diffuse Emission From the Inner Galaxy

Amid Nayerhoda; Francisco Salesa Greus; Sabrina Casanova

doi:10.3389/fspas.2018.00008

TeV Diffuse Emission From the Inner Galaxy

Amid Nayerhoda (Institute of Nuclear Physics PAN, Kraków, Poland) Francisco Salesa Greus (Max Planck Institute for Nuclear Physics, Heidelberg, Germany) Sabrina Casanova (Institute of Nuclear Physics PAN, Kraków, Poland)

Journal: Frontiers in Astronomy and Space Sciences • 2018-04-01 • Frontiers Media S.A. • ISSN: 2296-987X

Abstract

The TeV diffuse emission from the Galactic plane is produced by multi TeV electrons and nuclei interacting with radiation fields and ambient gas, respectively. Measurements of the TeV diffuse emission help constrain CR origin and transport properties. We present a preliminary analysis of HAWC diffuse emission data from the inner Galaxy. The HAWC measurements will be used to constrain particle transport properties close to the Galaxy center correlating the HAWC maps with predictions of the DRAGON code.

Subjects & Keywords

# Astronomy # Geophysics. Cosmic physics # high energy astrophysics # inner galaxy # gamma rays # diffuse emission # cosmic rays # interstellar medium

How to Cite this Article

                    Amid Nayerhoda, Francisco Salesa Greus, Sabrina Casanova (2018). "TeV Diffuse Emission From the Inner Galaxy". Frontiers in Astronomy and Space Sciences. https://doi.org/10.3389/fspas.2018.00008                

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Open Access (DOAJ)

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Identifiers & Provenance

DOI: 10.3389/fspas.2018.00008 ↗
Primary Index: DOAJ