This paper proposes to exploit gravitational lensing eects to improve the sensitivity of neutrino telescopes to the intrinsic neutrino emission of distant blazar populations. This strategy is illustrated with a search for cosmic neutrinos in the direction of four distant and gravitationally lensed Flat-Spectrum Radio Quasars. The magnication factor is estimated for each system assuming a singular isothermal prole for the lens. Based on data collected from 2007 to 2012 by the ANTARES neutrino telescope, the strongest constraint is obtained from the lensed quasar B0218+357, providing a limit on the total neutrino luminosity of this source of 1:08 1046 erg s1. This limit is about one order of magnitude lower than those previously obtained in the ANTARES standard point source searches with non-lensed Flat-Spectrum Radio Quasars.

Constraining the neutrino emission of gravitationally lensed Flat-Spectrum Radio Quasars with ANTARES data

BIAGI, SIMONE;FUSCO, LUIGI ANTONIO;MARGIOTTA, ANNARITA;SPURIO, MAURIZIO;
2014

Abstract

This paper proposes to exploit gravitational lensing eects to improve the sensitivity of neutrino telescopes to the intrinsic neutrino emission of distant blazar populations. This strategy is illustrated with a search for cosmic neutrinos in the direction of four distant and gravitationally lensed Flat-Spectrum Radio Quasars. The magnication factor is estimated for each system assuming a singular isothermal prole for the lens. Based on data collected from 2007 to 2012 by the ANTARES neutrino telescope, the strongest constraint is obtained from the lensed quasar B0218+357, providing a limit on the total neutrino luminosity of this source of 1:08 1046 erg s1. This limit is about one order of magnitude lower than those previously obtained in the ANTARES standard point source searches with non-lensed Flat-Spectrum Radio Quasars.
S. Adrián-Martínez;A. Albert;M. André;G. Anton;M. Ardid;J.-J. Aubert;B. Baret;J. Barrios-Martí;S. Basa;V. Bertin;S. Biagi;C. Bogazzi;R. Bormuth;M. Bou-Cabo;M.C. Bouwhuis;R. Bruijn;J. Brunner;J. Busto;A. Capone;L. Caramete;J. Carr;T. Chiarusi;M. Circella;R. Coniglione;L. Core;H. Costantini;P. Coyle;A. Creusot;G. De Rosa;I. Dekeyser;A. Deschamps;G. De Bonis;C. Distefano;C. Donzaud;D. Dornic;Q. Dorosti;D. Drouhin;A. Dumas;T. Eberl;D. Elsässer;A. Enzenhöfer;S. Escoffier;K. Fehn;I. Felis;P. Fermani;F. Folger;L.A. Fusco;S. Galatà;P. Gay;S. Geißelsöder;K. Geyer;V. Giordano;A. Gleixner;J.P. Gómez-González;K. Graf;G. Guillard;H. van Haren;A.J. Heijboer;Y. Hello;J.J. Hernández-Rey;B. Herold;A. Herrero;J. Hößl;J. Hofestädt;C. Hugon;C.W. James;M. de Jong;M. Kadler;O. Kalekin;A. Kappes;U. Katz;D. Kießling;P. Kooijman;A. Kouchner;I. Kreykenbohm;V. Kulikovskiy;R. Lahmann;E. Lambard;G. Lambard;D. Lefèvre;E. Leonora;H. Loehner;S. Loucatos;S. Mangano;M. Marcelin;A. Margiotta;J.A. Martínez-Mora;S. Martini;A. Mathieu;T. Michael;P. Migliozzi;C. Müller;M. Neff;E. Nezri;D. Palioselitis;G.E. Păvălaš;C. Perrina;V. Popa;T. Pradier;C. Racca;G. Riccobene;R. Richter;K. Roensch;A. Rostovtsev;M. Saldaña;D.F.E. Samtleben;A. Sánchez-Losa;M. Sanguineti;J. Schmid;J. Schnabel;S. Schulte;F. Schüssler;T. Seitz;C. Sieger;A. Spies;M. Spurio;J.J.M. Steijger;Th. Stolarczyk;M. Taiuti;C. Tamburini;Y. Tayalati;A. Trovato;M. Tselengidou;C. Tönnis;B. Vallage;C. Vallée;V. Van Elewyck;E. Visser;D. Vivolo;S. Wagner;J. Wilms;E. de Wolf;K. Yatkin;H. Yepes;J.D. Zornoza;J. Zúñiga;E.E. Falco
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/382044
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