A search for neutrino emission from the Fermi bubbles with the ANTARES telescope

被引：0

作者：

S. Adrián-Martínez

A. Albert

I. Al Samarai

M. André

G. Anton

S. Anvar

M. Ardid

T. Astraatmadja

J.-J. Aubert

B. Baret

J. Barrios-Martí

S. Basa

V. Bertin

S. Biagi

C. Bigongiari

C. Bogazzi

B. Bouhou

M. C. Bouwhuis

J. Brunner

J. Busto

A. Capone

L. Caramete

C. Cârloganu

J. Carr

S. Cecchini

Z. Charif

Ph. Charvis

T. Chiarusi

M. Circella

F. Classen

R. Coniglione

L. Core

H. Costantini

P. Coyle

A. Creusot

C. Curtil

G. De Bonis

I. Dekeyser

A. Deschamps

C. Donzaud

D. Dornic

Q. Dorosti

D. Drouhin

A. Dumas

T. Eberl

U. Emanuele

A. Enzenhöfer

J.-P. Ernenwein

S. Escoffier

K. Fehn

机构：

[1] Universitat Politècnica de València,Institut d’Investigació per a la Gestió Integrada de les Zones Costaneres (IGIC)

[2] GRPHE,Laboratory of Applied Bioacoustics

[3] Institut universitaire de technologie de Colmar,Erlangen Centre for Astroparticle Physics

[4] CPPM,Direction des Sciences de la Matière

[5] Aix-Marseille Université,IFIC, Instituto de Física Corpuscular, Edificios Investigación de Paterna, CSIC

[6] CNRS/IN2P3,LAM, Laboratoire d’Astrophysique de Marseille

[7] Technical University of Catalonia,Laboratoire de Physique Corpusculaire

[8] INFN,Kernfysisch Versneller Instituut (KVI)

[9] Sezione di Genova,Institut für Theoretische Physik und Astrophysik

[10] Friedrich-Alexander-Universität Erlangen-Nürnberg,Instituut voor Hoge

[11] Institut de recherche sur les lois fondamentales de l’Univers,Energie Fysica

[12] Service d’Electronique des Détecteurs et d’Informatique,Dr. Remeis

[13] CEA Saclay,Sternwarte and ECAP

[14] Nikhef,Skobeltsyn Institute of Nuclear Physics

[15] Science Park,Département de Physique Nucléaire et Corpusculaire

[16] APC,IPHC

[17] Université Paris Diderot,Institut Pluridisciplinaire Hubert Curien

[18] CNRS/IN2P3,Laboratory of Physics of Matter and Radiations

[19] CEA/IRFU,undefined

[20] Observatoire de Paris,undefined

[21] Sorbonne Paris Cité,undefined

[22] Universitat de València,undefined

[23] Pôle de l’Étoile Site de Château-Gombert,undefined

[24] INFN,undefined

[25] Sezione di Bologna,undefined

[26] Dipartimento di Fisica dell’Università,undefined

[27] INFN,undefined

[28] Sezione di Roma,undefined

[29] Dipartimento di Fisica dell’Università La Sapienza,undefined

[30] Institute for Space Sciences,undefined

[31] Clermont Université,undefined

[32] Université Blaise Pascal,undefined

[33] CNRS/IN2P3,undefined

[34] Géoazur,undefined

[35] Université Nice Sophia-Antipolis,undefined

[36] CNRS/INSU,undefined

[37] IRD,undefined

[38] Observatoire de la Côte d’Azur,undefined

[39] INFN,undefined

[40] Sezione di Bari,undefined

[41] INFN,undefined

[42] Laboratori Nazionali del Sud (LNS),undefined

[43] Mediterranean Institute of Oceanography (MIO),undefined

[44] Aix-Marseille University,undefined

[45] Universit du Sud Toulon-Var,undefined

[46] CNRS-INSU/IRD UM 110,undefined

[47] Université Paris-Sud,undefined

[48] University of Groningen,undefined

[49] INFN,undefined

[50] Sezione di Pisa,undefined

来源：

The European Physical Journal C | 2014年 / 74卷

关键词：

Atmospheric Neutrino; Neutrino Flux; Neutrino Telescope; Neutrino Emission; Neutrino Event;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

Analysis of the Fermi-LAT data has revealed two extended structures above and below the Galactic Centre emitting gamma rays with a hard spectrum, the so-called Fermi bubbles. Hadronic models attempting to explain the origin of the Fermi bubbles predict the emission of high-energy neutrinos and gamma rays with similar fluxes. The ANTARES detector, a neutrino telescope located in the Mediterranean Sea, has a good visibility to the Fermi bubble regions. Using data collected from 2008 to 2011 no statistically significant excess of events is observed and therefore upper limits on the neutrino flux in TeV range from the Fermi bubbles are derived for various assumed energy cutoffs of the source.

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