Atmospheric neutrinos are produced during cascades initiated by the interaction of primary cosmic rays with air nuclei. In this paper, a measurement of the atmospheric νμ + ¯νμ energy spectrum in the energy range 0.1–200 TeV is presented, using data collected by the ANTARES underwater neutrino telescope from 2008 to 2011. Overall, the measured flux is ∼25 % higher than predicted by the conventional neutrino flux, and compatible with the measurements reported in ice. The flux is compatible with a single power-law dependence with spectral index γmeas =3.58 ± 0.12. With the present statistics the contribution of prompt neutrinos cannot be established.

Measurement of the atmospheric ν μ energy spectrum from 100 GeV to 200 TeV with the ANTARES telescope / S. Adrián-Martínez;A. Albert;I. Al Samarai;M. André;M. Anghinolfi;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;R. Bruijn;J. Brunner;J. Busto;A. Capone;L. Caramete;C. Cârloganu;J. Carr;S. Cecchini;Z. Charif;Ph. Charvis;T. Chiarusi;M. Circella;F. Classen;L. Core;H. Costantini;P. Coyle;A. Creusot;C. Curtil;I. Dekeyser;A. Deschamps;G. Bonis;M. P. Decowski;C. Distefano;C. Donzaud;D. Dornic;Q. Dorosti;D. Drouhin;A. Dumas;T. Eberl;U. Emanuele;A. Enzenhöfer;J.-P. Ernenwein;S. Escoffier;K. Fehn;P. Fermani;V. Flaminio;F. Folger;U. Fritsch;L. A. Fusco;S. Galatà;P. Gay;S. Geißelsöder;K. Geyer;G. Giacomelli;V. Giordano;A. Gleixner;J. P. Gómez-González;K. Graf;G. Guillard;H. Haren;A. J. Heijboer;Y. Hello;J. J. Hernández-Rey;B. Herold;J. Hößl;C. W. James;M. Jong;M. Kadler;O. Kalekin;A. Kappes;U. Katz;P. Kooijman;A. Kouchner;I. Kreykenbohm;V. Kulikovskiy;R. Lahmann;E. Lambard;G. Lambard;G. Larosa;D. Lattuada;D. Lefèvre;E. Leonora;D. Lo Presti;H. Loehner;S. Loucatos;F. Louis;S. Mangano;M. Marcelin;A. Margiotta;J. A. Martínez-Mora;S. Martini;T. Michael;T. Montaruli;M. Morganti;H. Motz;C. Mueller;M. Neff;E. Nezri;D. Palioselitis;G. E. Păvălaş;C. Perrina;P. Piattelli;V. Popa;T. Pradier;C. Racca;R. Richter;C. Rivière;A. Robert;K. Roensch;A. Rostovtsev;D. F. E. Samtleben;M. Sanguineti;P. Sapienza;J. Schmid;J. Schnabel;S. Schulte;F. Schüssler;T. Seitz;R. Shanidze;C. Sieger;F. Simeone;A. Spies;M. Spurio;J. J. M. Steijger;Th. Stolarczyk;A. Sánchez-Losa;M. Taiuti;C. Tamburini;Y. Tayalati;A. Trovato;B. Vallage;C. Vallée;V. Elewyck;P. Vernin;E. Visser;S. Wagner;J. Wilms;E. Wolf;K. Yatkin;H. Yepes;J. D. Zornoza;J. Zúñiga. - In: THE EUROPEAN PHYSICAL JOURNAL. C, PARTICLES AND FIELDS. - ISSN 1434-6044. - STAMPA. - 73:(2013), pp. 2606-2606-12. [10.1140/epjc/s10052-013-2606-4]

Measurement of the atmospheric ν μ energy spectrum from 100 GeV to 200 TeV with the ANTARES telescope

BIAGI, SIMONE;FUSCO, LUIGI ANTONIO;GIACOMELLI, GIORGIO MARIA;MARGIOTTA, ANNARITA;SPURIO, MAURIZIO;
2013

Abstract

Atmospheric neutrinos are produced during cascades initiated by the interaction of primary cosmic rays with air nuclei. In this paper, a measurement of the atmospheric νμ + ¯νμ energy spectrum in the energy range 0.1–200 TeV is presented, using data collected by the ANTARES underwater neutrino telescope from 2008 to 2011. Overall, the measured flux is ∼25 % higher than predicted by the conventional neutrino flux, and compatible with the measurements reported in ice. The flux is compatible with a single power-law dependence with spectral index γmeas =3.58 ± 0.12. With the present statistics the contribution of prompt neutrinos cannot be established.
2013
Measurement of the atmospheric ν μ energy spectrum from 100 GeV to 200 TeV with the ANTARES telescope / S. Adrián-Martínez;A. Albert;I. Al Samarai;M. André;M. Anghinolfi;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;R. Bruijn;J. Brunner;J. Busto;A. Capone;L. Caramete;C. Cârloganu;J. Carr;S. Cecchini;Z. Charif;Ph. Charvis;T. Chiarusi;M. Circella;F. Classen;L. Core;H. Costantini;P. Coyle;A. Creusot;C. Curtil;I. Dekeyser;A. Deschamps;G. Bonis;M. P. Decowski;C. Distefano;C. Donzaud;D. Dornic;Q. Dorosti;D. Drouhin;A. Dumas;T. Eberl;U. Emanuele;A. Enzenhöfer;J.-P. Ernenwein;S. Escoffier;K. Fehn;P. Fermani;V. Flaminio;F. Folger;U. Fritsch;L. A. Fusco;S. Galatà;P. Gay;S. Geißelsöder;K. Geyer;G. Giacomelli;V. Giordano;A. Gleixner;J. P. Gómez-González;K. Graf;G. Guillard;H. Haren;A. J. Heijboer;Y. Hello;J. J. Hernández-Rey;B. Herold;J. Hößl;C. W. James;M. Jong;M. Kadler;O. Kalekin;A. Kappes;U. Katz;P. Kooijman;A. Kouchner;I. Kreykenbohm;V. Kulikovskiy;R. Lahmann;E. Lambard;G. Lambard;G. Larosa;D. Lattuada;D. Lefèvre;E. Leonora;D. Lo Presti;H. Loehner;S. Loucatos;F. Louis;S. Mangano;M. Marcelin;A. Margiotta;J. A. Martínez-Mora;S. Martini;T. Michael;T. Montaruli;M. Morganti;H. Motz;C. Mueller;M. Neff;E. Nezri;D. Palioselitis;G. E. Păvălaş;C. Perrina;P. Piattelli;V. Popa;T. Pradier;C. Racca;R. Richter;C. Rivière;A. Robert;K. Roensch;A. Rostovtsev;D. F. E. Samtleben;M. Sanguineti;P. Sapienza;J. Schmid;J. Schnabel;S. Schulte;F. Schüssler;T. Seitz;R. Shanidze;C. Sieger;F. Simeone;A. Spies;M. Spurio;J. J. M. Steijger;Th. Stolarczyk;A. Sánchez-Losa;M. Taiuti;C. Tamburini;Y. Tayalati;A. Trovato;B. Vallage;C. Vallée;V. Elewyck;P. Vernin;E. Visser;S. Wagner;J. Wilms;E. Wolf;K. Yatkin;H. Yepes;J. D. Zornoza;J. Zúñiga. - In: THE EUROPEAN PHYSICAL JOURNAL. C, PARTICLES AND FIELDS. - ISSN 1434-6044. - STAMPA. - 73:(2013), pp. 2606-2606-12. [10.1140/epjc/s10052-013-2606-4]
S. Adrián-Martínez;A. Albert;I. Al Samarai;M. André;M. Anghinolfi;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;R. Bruijn;J. Brunner;J. Busto;A. Capone;L. Caramete;C. Cârloganu;J. Carr;S. Cecchini;Z. Charif;Ph. Charvis;T. Chiarusi;M. Circella;F. Classen;L. Core;H. Costantini;P. Coyle;A. Creusot;C. Curtil;I. Dekeyser;A. Deschamps;G. Bonis;M. P. Decowski;C. Distefano;C. Donzaud;D. Dornic;Q. Dorosti;D. Drouhin;A. Dumas;T. Eberl;U. Emanuele;A. Enzenhöfer;J.-P. Ernenwein;S. Escoffier;K. Fehn;P. Fermani;V. Flaminio;F. Folger;U. Fritsch;L. A. Fusco;S. Galatà;P. Gay;S. Geißelsöder;K. Geyer;G. Giacomelli;V. Giordano;A. Gleixner;J. P. Gómez-González;K. Graf;G. Guillard;H. Haren;A. J. Heijboer;Y. Hello;J. J. Hernández-Rey;B. Herold;J. Hößl;C. W. James;M. Jong;M. Kadler;O. Kalekin;A. Kappes;U. Katz;P. Kooijman;A. Kouchner;I. Kreykenbohm;V. Kulikovskiy;R. Lahmann;E. Lambard;G. Lambard;G. Larosa;D. Lattuada;D. Lefèvre;E. Leonora;D. Lo Presti;H. Loehner;S. Loucatos;F. Louis;S. Mangano;M. Marcelin;A. Margiotta;J. A. Martínez-Mora;S. Martini;T. Michael;T. Montaruli;M. Morganti;H. Motz;C. Mueller;M. Neff;E. Nezri;D. Palioselitis;G. E. Păvălaş;C. Perrina;P. Piattelli;V. Popa;T. Pradier;C. Racca;R. Richter;C. Rivière;A. Robert;K. Roensch;A. Rostovtsev;D. F. E. Samtleben;M. Sanguineti;P. Sapienza;J. Schmid;J. Schnabel;S. Schulte;F. Schüssler;T. Seitz;R. Shanidze;C. Sieger;F. Simeone;A. Spies;M. Spurio;J. J. M. Steijger;Th. Stolarczyk;A. Sánchez-Losa;M. Taiuti;C. Tamburini;Y. Tayalati;A. Trovato;B. Vallage;C. Vallée;V. Elewyck;P. Vernin;E. Visser;S. Wagner;J. Wilms;E. Wolf;K. Yatkin;H. Yepes;J. D. Zornoza;J. Zúñiga
File in questo prodotto:
Eventuali allegati, non sono esposti

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/372743
 Attenzione

Attenzione! I dati visualizzati non sono stati sottoposti a validazione da parte dell'ateneo

Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus 68
  • ???jsp.display-item.citation.isi??? 51
social impact