2017MNRAS.469..906A

Query : 2017MNRAS.469..906A

2017MNRAS.469..906A - Mon. Not. R. Astron. Soc., 469, 906-915 (2017/July-3)

Search for high-energy neutrinos from bright GRBs with ANTARES.

ALBERT A., ANDRE M., ANGHINOLFI M., ANTON G., ARDID M., AUBERT J.-J., AVGITAS T., BARET B., BARRIOS-MARTI J., BASA S., BERTIN V., BIAGI S., BORMUTH R., BOURRET S., BOUWHUIS M.C., BRUIJN R., BRUNNER J., BUSTO J., CAPONE A., CARAMETE L., CARR J., CELLI S., CHIARUSI T., CIRCELLA M., COELHO J.A.B., COLEIRO A., CONIGLIONE R., COSTANTINI H., COYLE P., CREUSOT A., DESCHAMPS A., DE BONIS G., DISTEFANO C., DI PALMA I., DONZAUD C., DORNIC D., DROUHIN D., EBERL T., EL BOJADDAINI I., ELSASSER D., ENZENHOFER A., FELIS I., FUSCO L.A., GALATA S., GAY P., GEISSELSODER S., GEYER K., GIORDANO V., GLEIXNER A., GLOTIN H., GREGOIRE T., GRACIA-RUIZ R., GRAF K., HALLMANN S., VAN HAREN H., HEIJBOER A.J., HELLO Y., HERNANDEZ-REY J.J., HOSSL J., HOFESTADT J., HUGON C., ILLUMINATI G., JAMES C.W., DE JONG M., JONGEN M., KADLER M., KALEKIN O., KATZ U., KIESSLING D., KOUCHNER A., KRETER M., KREYKENBOHM I., KULIKOVSKIY V., LACHAUD C., LAHMANN R., LEFEVRE D., LEONORA E., LOTZE M., LOUCATOS S., MARCELIN M., MARGIOTTA A., MARINELLI A., MARTINEZ-MORA J.A., MATHIEU A., MELE R., MELIS K., MICHAEL T., MIGLIOZZI P., MOUSSA A., MUELLER C., NEZRI E., PAVALAS G.E., PELLEGRINO C., PERRINA C., PIATTELLI P., POPA V., PRADIER T., QUINN L., RACCA C., RICCOBENE G., ROENSCH K., SANCHEZ-LOSA A., SALDANA M., SALVADORI I., SAMTLEBEN D.F.E., SANGUINETI M., SAPIENZA P., SCHNABEL J., SCHUSSLER F., SEITZ T., SIEGER C., SPURIO M., STOLARCZYK T., TAIUTI M., TAYALATI Y., TROVATO A., TSELENGIDOU M., TURPIN D., TONNIS C., VALLAGE B., VALLEE C., VAN ELEWYCK V., VIVOLO D., VIZZOCCA A., WAGNER S., WILMS J., ZORNOZA J.D. and ZUNIGA J.

Abstract (from CDS):

Gamma-ray bursts are thought to be sites of hadronic acceleration, thus neutrinos are expected from the decay of charged particles, produced in pγ interactions. The methods and results of a search for muon neutrinos in the data of the ANTARES neutrino telescope from four bright GRBs (GRB 080916C, GRB 110918A, GRB 130427A and GRB 130505A) observed between 2008 and 2013 are presented. Two scenarios of the fireball model have been investigated: the internal shock scenario, leading to the production of neutrinos with energies mainly above 100 TeV, and the photospheric scenario, characterized by a low-energy component in neutrino spectra due to the assumption of neutrino production closer to the central engine. Since no neutrino events have been detected in temporal and spatial coincidence with these bursts, upper limits at 90 per cent confidence level on the expected neutrino fluxes are derived. The non-detection allows for directly constraining the bulk Lorentz factor of the jet Γ and the baryon loading fp.

Abstract Copyright: © 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): acceleration of particles - neutrinos - gamma-ray burst: individual: GRB 080916C - gamma-ray burst: individual: GRB 110918A - gamma-ray burst: individual: GRB 130427A - gamma-ray burst: individual: GRB 130505A - gamma-ray burst: individual: GRB 130505A

Simbad objects: 4

goto Full paper

goto View the references in ADS

Number of rows : 4
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 GRB 110918A gB 02 10 09.39 -27 06 19.6           ~ 83 0
2 GRB 080916C gB 07 59 23.24 -56 38 16.8           ~ 386 0
3 GRB 130505A gB 09 17 21.9014988888 +01 42 03.426207768           ~ 94 0
4 SN 2013cq SN* 11 32 32.84 +27 41 56.2           SNIc 613 1

To bookmark this query, right click on this link: simbad:objects in 2017MNRAS.469..906A and select 'bookmark this link' or equivalent in the popup menu