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

Abstract:

This paper proposes to exploit gravitational lensing effects 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 magnification factor is estimated for each system assuming a singular isothermal profile 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 s-1. 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.

Año de publicación:

2014

Keywords:

  • gravitational lensing
  • neutrino astronomy

Fuente:

scopusscopus

Tipo de documento:

Article

Estado:

Acceso abierto

Áreas de conocimiento:

  • Física de partículas

Áreas temáticas:

  • Física
  • Cuerpos y fenómenos celestes específicos

Contribuidores:

Carr J.Carr J.
Dekeyser I.Dekeyser I.
Palioselitis D.Palioselitis D.
Geißelsöder S.Geißelsöder S.
Kreykenbohm I.Kreykenbohm I.
Enzenhöfer A.Enzenhöfer A.
Lambard E.Lambard E.
Loucatos S.Loucatos S.
Leonora E.Leonora E.
De Bonis G.De Bonis G.
Baret B.Baret B.
Geyer K.Geyer K.
Guillard G.Guillard G.
Giordano V.Giordano V.
Felis I.Felis I.
Dorosti Q.Dorosti Q.
Pradier T.Pradier T.
Fusco L.A.Fusco L.A.
Nezri E.Nezri E.
Galatà S.Galatà S.
Bormuth R.Bormuth R.
Biagi S.Biagi S.
Kooijman P.Kooijman P.
Migliozzi P.Migliozzi P.
Creusot A.Creusot A.
Kappes A.Kappes A.
Bou-Cabo M.Bou-Cabo M.
Fermani P.Fermani P.
Chiarusi T.Chiarusi T.
Deschamps A.Deschamps A.
Gay P.Gay P.
Gleixner A.Gleixner A.
Kadler M.Kadler M.
Costantini H.Costantini H.
H. Yepes-RamirezH. Yepes-Ramirez
Katz U.Katz U.
Dornic D.Dornic D.
Neff M.Neff M.
Bogazzi C.Bogazzi C.
Elsässer D.Elsässer D.
Graf K.Graf K.
Escoffier S.Escoffier S.
van Haren H.van Haren H.
Circella M.Circella M.
Ardid M.Ardid M.
Martinez-Mora J.A.Martinez-Mora J.A.
Herold B.Herold B.
Herrero A.Herrero A.
Lefèvre D.Lefèvre D.
Bruijn R.Bruijn R.
Hofestädt J.Hofestädt J.
Aubert J.J.Aubert J.J.
Mangano S.Mangano S.
Coyle P.Coyle P.
Core L.Core L.
Hugon C.Hugon C.
Anton G.Anton G.
Caramete L.Caramete L.
Kalekin O.Kalekin O.
Drouhin D.Drouhin D.
Capone A.Capone A.
Gómez-González J.P.Gómez-González J.P.
Kouchner A.Kouchner A.
Heijboer A.J.Heijboer A.J.
Margiotta A.Margiotta A.
Folger F.Folger F.
Michael T.Michael T.
Kießling D.Kießling D.
Dumas A.Dumas A.
Eberl T.Eberl T.
Pəvəlaš G.E.Pəvəlaš G.E.
Hößl J.Hößl J.
Albert A.Albert A.
Hello Y.Hello Y.
Racca C.Racca C.
Perrina C.Perrina C.
Kulikovskiy V.Kulikovskiy V.
Bouwhuis M.C.Bouwhuis M.C.
Müller C.Müller C.
Brunner J.Brunner J.
Barrios-Martí J.Barrios-Martí J.
Coniglione R.Coniglione R.
James C.W.James C.W.
Martini S.Martini S.
Lambard G.Lambard G.
De Rosa G.De Rosa G.
Fehn K.Fehn K.
Andre M.Andre M.
Busto J.Busto J.
Mathieu A.Mathieu A.
Basa S.Basa S.
Marcelin M.Marcelin M.
Lahmann R.Lahmann R.
Adrían-Martínez S.Adrían-Martínez S.
Bertin V.Bertin V.
Popa V.Popa V.
Hernndez-Rey J.J.Hernndez-Rey J.J.
Loehner H.Loehner H.
De Jong M.D.De Jong M.D.
Donzaud C.Donzaud C.
Distefano C.Distefano C.