Journal
ASTROPHYSICAL JOURNAL LETTERS
Volume 868, Issue 2, Pages -Publisher
IOP Publishing Ltd
DOI: 10.3847/2041-8213/aaeecf
Keywords
cosmic rays; diffusion; Galaxy: disk; gamma rays: diffuse background; neutrinos
Categories
Funding
- Centre National de la Recherche Scientifique (CNRS), France
- Commissariat a l'energie atomique et aux energies alternatives (CEA), France
- Commission Europeenne (FEDER fund), France
- Commission Europeenne (Marie Curie Program), France
- Institut Universitaire de France (IUF), France
- IdEx program, France
- UnivEarthS Labex program at Sorbonne Paris Cite, France [ANR-10-LABX-0023, ANR-11-IDEX-0005-02]
- Labex OCEVU, France [ANR-11-LABX-0060]
- A*MIDEX project, France [ANR-11-IDEX-0001-02]
- Region Ilede-France (DIM-ACAV), France
- Region Alsace (contrat CPER), France
- Region Provence-Alpes-Cote d'Azur, France
- Departement du Var, France
- Ville de La Seyne-sur-Mer, France
- Bundesministerium fur Bildung und Forschung (BMBF), Germany
- Istituto Nazionale di Fisica Nucleare (INFN), Italy
- Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands
- Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia
- National Authority for Scientific Research (ANCS), Romania
- Ministerio de Economia y Competitividad (MINECO): Plan Estatal de Investigacion (MINECO/FEDER), Spain [FPA2015-65150-C3-1-P, FPA2015-65150-C3-2-P, FPA2015-65150-C3-3-P]
- Severo Ochoa Centre of Excellence (MINECO), Spain
- MultiDark Consolider (MINECO), Spain
- Prometeo program (Generalitat Valenciana), Spain
- Grisolia program (Generalitat Valenciana), Spain
- Ministry of Higher Education, Scientific Research and Professional Training, Morocco
- USA-U.S. National Science Foundation-Office of Polar Programs
- USA-U.S. National Science Foundation-Physics Division
- USA-Wisconsin Alumni Research Foundation
- USA-Center for High Throughput Computing (CHTC) at the University of Wisconsin-Madison
- USA-Open Science Grid (OSG), Extreme Science and Engineering Discovery Environment (XSEDE), U.S. Department of Energy-National Energy Research Scientific Computing Center, Particle astrophysics research computing center at the University of Maryland
- USA-Institute for Cyber-Enabled Research at Michigan State University
- USA-Astroparticle physics computational facility at Marquette University
- Belgium-Fund for Scientific Research (FRS-FNRS)
- Belgium-Fund for Scientific Research (FWO)
- Belgium-FWO Odysseus programme
- Belgium-FWO Big Science programme
- Belgium-Belgian Federal Science Policy Office (Belspo)
- Germany-Bundesministerium fur Bildung und Forschung (BMBF)
- Germany-Deutsche Forschungsgemeinschaft (DFG)
- Germany-Helmholtz Alliance for Astroparticle Physics (HAP)
- Germany-Initiative and Networking Fund of the Helmholtz Association
- Germany-Deutsches Elektronen Synchrotron (DESY),
- Germany-High Performance Computing cluster of the RWTH Aachen
- Sweden-Swedish Research Council
- Sweden-Swedish Polar Research Secretariat
- Sweden-Swedish National Infrastructure for Computing (SNIC)
- Sweden-Knut and Alice Wallenberg Foundation
- Australia-Australian Research Council
- Canada-Natural Sciences and Engineering Research Council of Canada
- Canada-Calcul Quebec
- Canada-Compute Ontario
- Canada-Canada Foundation for Innovation
- Canada-WestGrid
- Canada-Compute Canada
- Denmark-Villum Fonden
- Denmark-Danish National Research Foundation (DNRF)
- New Zealand-Marsden Fund
- Japan-Japan Society for Promotion of Science (JSPS)
- Japan-Institute for Global Prominent Research (IGPR) of Chiba University
- Korea-National Research Foundation of Korea (NRF)
- Switzerland-Swiss National Science Foundation (SNSF)
- Villum Fonden [00013161] Funding Source: researchfish
- STFC [ST/P000770/1] Funding Source: UKRI
Ask authors/readers for more resources
The existence of diffuse Galactic neutrino production is expected from cosmic-ray interactions with Galactic gas and radiation fields. Thus, neutrinos are a unique messenger offering the opportunity to test the products of Galactic cosmic-ray interactions up to energies of hundreds of TeV. Here we present a search for this production using ten years of Astronomy with a Neutrino Telescope and Abyss environmental RESearch (ANTARES) track and shower data, as well as seven years of IceCube track data. The data are combined into a joint likelihood test for neutrino emission according to the KRA(gamma) model assuming a 5 PeV per nucleon Galactic cosmic-ray cutoff. No significant excess is found. As a consequence, the limits presented in this Letter start constraining the model parameter space for Galactic cosmic-ray production and transport.
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