@article{fdi:010070989,
  title = {{N}ew constraints on all flavor {G}alactic diffuse neutrino emission with the {ANTARES} telescope},
  author = {{A}lbert, {A}. and {A}ndre, {M}. and {A}nghinolfi, {M}. and {A}nton, {G}. and {A}rdid, {M}. and {A}ubert, {J}. {J}. and {A}vgitas, {T}. and {B}aret, {B}. and {B}arrios-{M}arti, {J}. and {B}asa, {S}. and {B}elhorma, {B}. and {B}ertin, {V}. and {B}iagi, {S}. and {B}ormuth, {R}. and {B}ourret, {S}. and {B}ouwhuis, {M}. {C}. and {B}ruijn, {R}. and {B}runner, {J}. and {B}usto, {J}. and {C}apone, {A}. and {C}aramete, {L}. and {C}arr, {J}. and {C}elli, {S}. and {E}l {M}oursli, {R}. {C}. and {C}hiarusi, {T}. and {C}ircella, {M}. and {C}oelho, {J}. {A}. {B}. and {C}oleiro, {A}. and {C}oniglione, {R}. and {C}ostantini, {H}. and {C}oyle, {P}. and {C}reusot, {A}. and {D}iaz, {A}. {F}. and {D}eschamps, {A}. and {D}e {B}onis, {G}. and {D}istefano, {C}. and {D}i {P}alma, {I}. and {D}omi, {A}. and {D}onzaud, {C}. and {D}ornic, {D}. and {D}rouhin, {D}. and {E}berl, {T}. and {E}l {B}ojaddaini, {I}. and {E}l {K}hayati, {N}. and {E}lsasser, {D}. and {E}nzenhofer, {A}. and {E}ttahiri, {A}. and {F}assi, {F}. and {F}elis, {I}. and {F}usco, {L}. {A}. and {G}alata, {S}. and {G}ay, {P}. and {G}iordano, {V}. and {G}lotin, {H}. and {G}regoire, {T}. and {R}uiz, {R}. {G}. and {G}raf, {K}. and {H}allmann, {S}. and van {H}aren, {H}. and {H}eijboer, {A}. {J}. and {H}ello, {Y}ann and et al. and {ANTARES} {C}ollaboration},
  editor = {},
  language = {{ENG}},
  abstract = {{T}he flux of very high-energy neutrinos produced in our {G}alaxy by the interaction of accelerated cosmic rays with the interstellar medium is not yet determined. {T}he characterization of this flux will shed light on {G}alactic accelerator features, gas distribution morphology and {G}alactic cosmic ray transport. {T}he central {G}alactic plane can be the site of an enhanced neutrino production, thus leading to anisotropies in the extraterrestrial neutrino signal as measured by the {I}ce{C}ube {C}ollaboration. {T}he {ANTARES} neutrino telescope, located in the {M}editerranean {S}ea, offers a favorable view of this part of the sky, thereby allowing for a contribution to the determination of this flux. {T}he expected diffuse {G}alactic neutrino emission can be obtained, linking a model of generation and propagation of cosmic rays with the morphology of the gas distribution in the {M}ilky {W}ay. {I}n this paper, the so-called "gamma model" introduced recently to explain the high-energy gamma-ray diffuse {G}alactic emission is assumed as reference. {T}he neutrino flux predicted by the "gamma model" depends on the assumed primary cosmic ray spectrum cutoff. {C}onsidering a radially dependent diffusion coefficient, this proposed scenario is able to account for the local cosmic ray measurements, as well as for the {G}alactic gamma-ray observations. {N}ine years of {ANTARES} data are used in this work to search for a possible {G}alactic contribution according to this scenario. {A}ll flavor neutrino interactions are considered. {N}o excess of events is observed, and an upper limit is set on the neutrino flux of 1.1 (1.2) times the prediction of the "gamma model," assuming the primary cosmic ray spectrum cutoff at 5 (50) {P}e{V}. {T}his limit excludes the diffuse {G}alactic neutrino emission as the major cause of the "spectral anomaly" between the two hemispheres measured by {I}ce{C}ube.},
  keywords = {},
  booktitle = {},
  journal = {{P}hysical {R}eview {D}},
  volume = {96},
  numero = {6},
  pages = {art. 062001 [9 p.]},
  ISSN = {2470-0010},
  year = {2017},
  DOI = {10.1103/{P}hys{R}ev{D}.96.062001},
  URL = {https://www.documentation.ird.fr/hor/fdi:010070989},
}