Constraining the contribution of Gamma-Ray Bursts to the high-energy diffuse neutrino flux with 10 yr of ANTARES data

Albert, A.; André, M.; Anghinolfi, M.; Anton, G.; Ardid, M.; Aubert, J.J.; Aublin, J.; Baret, B.; Basa, S.; Belhorma, B.; Bertín, V.; Biagi, S.; Bissinger, M.; Boumaaza, J.; Bouta, M.; Bouwhuis, M. C.; Brânzaş, H.; Bruijn, R.; Brünner, J.; Busto, J.; Capone, A.; Caramete, L.; Carr, J.; Celli, S.; Chabab, M.; Chau, Thien Nhan; Moursli, R. Cherkaoui El; Chiarusi, T.; Circella, M.; Coleiro, A.; Colomer-Molla, M.; Coniglione, R.; Coyle, P.; Creusot, A.; Díaz, Antonio; Wasseige, Gwenhaël de; Deschamps, A.; Distefano, C.; Palma, I. Di; Domi, Alba; Donzaud, C.; Dornic, D.; Drouhin, D.; Eberl, T.; Khayati, N. El; Enzenhöfer, A.; Ettahiri, A.; Fermani, P.; Ferrara, G.; Filippini, F.; Fusco, L.; Glotin, Hervé; Gozzini, R.; Graf, Κ.; Guidi, C.; Hallmann, S.; Haren, Hans van; Heijboer, A.; Hello, Y.; Hernández-Rey, J. J.; Hößl, J.; Hofestädt, J.; Huang, F.; Illuminati, G.; James, C. W.; Jong, M. de; Jong, P. de; Jongen, M.; Kadler, M.; Kalekin, O.; Katz, U.; Khan-Chowdhury, N. R.; Kouchner, A.; Kreykenbohm, I.; Kulikovskiy, V.; Lahmann, R.; Breton, R. Le; Lefèvre, D.; Leonora, E.; Levi, G.; Lincetto, Massimiliano; Lopez-Coto, D.; Loucatos, S.; Maggi, G.; Mańczak, J.; Marcelin, M.; Margiotta, A.; Marinelli, A.; Martínez-Mora, J. A.; Mazzou, S.; Melis, K.; Migliozzi, P.; Möser, Michael; Moussa, A.; Müller, R.; Nauta, L.; Navas, S.; Nezri, E.; Núñez-Castiñeyra, A.; O’Fearraigh, B.; Organokov, M.; Păvălaş, G. E.; Pellegrino, C.; Perrin-Terrin, M.; Piattelli, P.; Poirè, C.; Popa, V.; Pradier, T.; Randazzo, N.; Reck, S.; Riccobene, G.; Sánchez-Losa, A.; Samtleben, D. F. E.; Sanguineti, M.; Sapienza, P.; Schnabel, J.; Schüßler, F.; Spurio, M.; Stolarczyk, Th.; Strandberg, B.; Taiuti, M.; Tayalati, Y.; Thakore, T.; Tingay, S. J.; Trovato, A.; Vallage, B.; Elewyck, V. Van; Versari, F.; Viola, S.; Vivolo, D.; Wilms, J.; Zegarelli, A.; Zornoza, J. D.; Zúñiga, J.

doi:10.1093/mnras/staa3503

Cited by 35 publications

(49 citation statements)

References 90 publications

(132 reference statements)

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“…A strategy based on pseudoexperiments, simulating with high statistics a measurement's result, and on the optimisation of the cut on the track reconstruction quality maximising the Model Discovery Potential (MDP), is implemented. See [10] for further details.…”

Section: Analysis Methodsmentioning

confidence: 99%

“…photon spectrum, fluence and redshift, are collected from published results of Swift , Fermi and Konus-Wind . For more details regarding the selection criteria see [10].…”

Section: Pos(icrc2021)965mentioning

confidence: 99%

“…As the neutrino flux is expected to be extremely sensitive to the Lorentz factor [19], a treatment of the additional systematics associated with adopting a different method for deriving Γ (e.g. [20]) is also presented in [10].…”

Section: Pos(icrc2021)965mentioning

confidence: 99%

“…Only track-like events reconstructed within 10 • in radius from the expected GRB position and in temporal correlation with the duration of the prompt gamma-ray emission are selected, namely those falling within a search time window around the GRB occurrence (T search ∼ T 90 ). Both in signal and background estimations, the different environmental conditions in the deep sea and the variation of data-taking efficiency are taken into account, as explained in more details in [10].…”

Section: Signal and Background Estimationmentioning

confidence: 99%

“…For this reason, the innovative search for astrophysical muon neutrinos from GRBs, already presented in [10], is here summarised. This work focuses on improving the predictions on the expected neutrino fluences from GRBs, by considering the wealth of information accumulated so far thanks to the many astronomical observations, rather than assuming some fixed standard values that do not correctly reproduce the properties of the source sample.…”

Section: Introductionmentioning

confidence: 99%

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Constraining the contribution of Gamma-Ray Bursts to the high-energy diffuse neutrino flux with 10 years of ANTARES data

Zegarelli¹,

Celli²

2021

Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021)

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Addressing the origin of the observed diffuse astrophysical neutrino flux is one of the main challenges in the context of the neutrino astronomy nowadays. Among several astrophysical sources, Gamma-Ray Bursts (GRBs) are considered interesting candidates to be explored. Indeed, being the most powerful explosions observable in the Universe, they are potentially able to achieve the energetics required to reproduce the neutrino flux. Thus, they are expected to provide at least some contribution to the astrophysical diffuse neutrino flux. Within the framework of the fireball model, mesons can be produced during photo-hadronic interactions occurring in the internal shocks between shells emitted by the central engine; from their decays, high-energy gamma rays and neutrinos are expected to be generated. Within this scenario, the results of a stacked search for astrophysical muon neutrinos performed in space and time coincidence with 784 GRBs in the period 2007-2017 using ANTARES data are presented. The neutrino flux expectation from each GRB detectable by ANTARES was calculated in the framework of the classical internal shock model. Given the absence of coincident neutrinos, the contribution of the detected GRB population to the neutrino diffuse flux is constrained to be less than 10% around 100 TeV. In addition, the systematic uncertainties on the diffuse flux are computed by propagating to the stacked limit the uncertainties on the model parameters for each individual burst.

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Section: Analysis Methodsmentioning

confidence: 99%

“…photon spectrum, fluence and redshift, are collected from published results of Swift , Fermi and Konus-Wind . For more details regarding the selection criteria see [10].…”

Section: Pos(icrc2021)965mentioning

confidence: 99%

Section: Pos(icrc2021)965mentioning

confidence: 99%

Section: Signal and Background Estimationmentioning

confidence: 99%

Section: Introductionmentioning

confidence: 99%

See 3 more Smart Citations

Constraining the contribution of Gamma-Ray Bursts to the high-energy diffuse neutrino flux with 10 years of ANTARES data

Zegarelli¹,

Celli²

2021

Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021)

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Neutrino search from γ-ray bursts during the prompt and X-ray afterglow phases using 10 years of IceCube public data

Lucarelli¹,

Oganesyan²,

Montaruli³

et al. 2023

A&A

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Neutrino emission from γ-ray bursts (GRBs) has been sought for a long time, and stringent limits on the most accredited GRB emission models have been obtained from IceCube. Multiwavelength GRB observations of the last decades have improved our knowledge of the GRB emission parameters, such as the Lorentz factor and the luminosity, which can vary from one GRB to another by several orders of magnitude. Empirical correlations among such parameters have been identified during the prompt phase, with direct implications on GRB models. In this work, we use the PSLab open-access code, developed for IceCube data analyses, to search for individual neutrino emission from the prompt and afterglow phases of selected GRBs, and for stacking emission from the ensemble of such GRBs. For the afterglow phase, we focus on GRBs with X-ray flares and plateaus in particular. While past stacking searches assumed the same GRB fluence at Earth, we present a stacking scheme based on physically motivated GRB weights. Moreover, we conceive a new methodology for the prompt phase that uses the empirical correlations to infer the GRB luminosity and Lorentz factor, when redshift measurements are not available. We do not observe any significant neutrino excess. Hence, we set constraints on the GRB neutrino fluxes and on relevant GRB parameters, including the magnetic field in the jet. Notably, the baryon loading is found to be less than ten for typical GRB jets.

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TeV emission from Gamma Ray Bursts, checking the hadronic model

Guetta¹,

Gagliardini²,

Celli³

et al. 2023

EPJ Web Conf.

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Gamma-Ray Bursts (GRBs) are the most luminous explosions in the Universe. Their luminous prompt emission makes them detectable from cosmological distances. Most GRBs have been detected below a few MeV, however at least a hundred GRBs have been detected at high (0.1 GeV) energies and observed up to tens of GeV with the Fermi Large Area Telescope (LAT). Some GRBs have been observed at (0.1–1) TeV by ground-based imaging atmospheric Cherenkov telescopes. To date, the high energy emission mechanism is not understood. In this paper we review the possible leptonic and hadronic mechanisms capable of producing the ∼ TeV emission detected in GRBs. In paricular we concentrate on the hadronic origin of this radiation component and discuss in detail the numerical simulation elaborated to reproduce the observed sub-TeV observations of GRB190114C.

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Constraining the contribution of Gamma-Ray Bursts to the high-energy diffuse neutrino flux with 10 yr of ANTARES data

Cited by 35 publications

References 90 publications

Constraining the contribution of Gamma-Ray Bursts to the high-energy diffuse neutrino flux with 10 years of ANTARES data

Constraining the contribution of Gamma-Ray Bursts to the high-energy diffuse neutrino flux with 10 years of ANTARES data

Neutrino search from γ-ray bursts during the prompt and X-ray afterglow phases using 10 years of IceCube public data

TeV emission from Gamma Ray Bursts, checking the hadronic model

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