@article{fdi:010074818,
  title = {{T}he search for high-energy neutrinos coincident with fast radio bursts with the {ANTARES} neutrino 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}ublin, {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}oumaaza, {J}. and {B}ourret, {S}. and {B}ouwhuis, {M}. {C}. and {B}ranzas, {H}. 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 {C}habab, {M}. 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}olomer, {M}. 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}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}nzenhoer, {A}. and {E}ttahiri, {A}. and {F}assi, {F}. and {F}elis, {I}. and {F}ermani, {P}. and {F}errara, {G}. and {F}usco, {L}. and {G}ay, {P}. and {G}lotin, {H}. and {G}regoire, {T}. and {G}racia-{R}uiz, {R}. 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.},
  editor = {},
  language = {{ENG}},
  abstract = {{I}n the past decade, a new class of bright transient radio sources with millisecond duration has been discovered. {T}he origin of these so-called fast radio bursts ({FRB}s) is still a mystery, despite the growing observational efforts made by various multiwavelength and multimessenger facilities. {T}o date, many models have been proposed to explain {FRB}s, but neither the progenitors nor the radiative and the particle acceleration processes at work have been clearly identified. {I}n this paper, we assess whether hadronic processes may occur in the vicinity of the {FRB} source. {I}f they do, {FRB}s may contribute to the high-energy cosmic-ray and neutrino fluxes. {A} search for these hadronic signatures was carried out using the {ANTARES} neutrino telescope. {T}he analysis consists in looking for high-energy neutrinos, in the {T}e{V}-{P}e{V} regime, that are spatially and temporally coincident with the detected {FRB}s. {M}ost of the {FRB}s discovered in the period 2013-2017 were in the field of view of the {ANTARES} detector, which is sensitive mostly to events originating from the {S}outhern hemisphere. {F}rom this period, 12 {FRB}s were selected and no coincident neutrino candidate was observed. {U}pper limits on the per-burst neutrino fluence were derived using a power-law spectrum, d{N}/{DE} nu proportional to {E}-nu(-gamma), for the incoming neutrino flux, assuming spectral indexes gamma = 1.0, 2.0, 2.5. {F}inally, the neutrino energy was constrained by computing the total energy radiated in neutrinos, assuming different distances for the {FRB}s. {C}onstraints on the neutrino fluence and on the energy released were derived from the associated null results.},
  keywords = {acceleration of particles ; neutrinos ; astroparticle physics ; radio ; continuum: transients ; methods: data analysis},
  booktitle = {},
  journal = {{M}onthly {N}otices of the {R}oyal {A}stronomical {S}ociety},
  volume = {482},
  numero = {1},
  pages = {184--193},
  ISSN = {0035-8711},
  year = {2019},
  DOI = {10.1093/mnras/sty2621},
  URL = {https://www.documentation.ird.fr/hor/fdi:010074818},
}