0000000000767390

AUTHOR

J. A. Martínez-mora

showing 4 related works from this author

Search for relativistic magnetic monopoles with the ANTARES neutrino telescope

2012

Magnetic monopoles are predicted in various unified gauge models and could be produced at intermediate mass scales. Their detection in a neutrino telescope is facilitated by the large amount of light emitted compared to that from muons. This paper reports on a search for upgoing relativistic magnetic monopoles with the ANTARES neutrino telescope using a data set of 116 days of live time taken from December 2007 to December 2008. The one observed event is consistent with the expected atmospheric neutrino and muon background, leading to a 90% C.L. upper limit on the monopole flux between 1.3 ¿ 10¿17 and 8.9 ¿ 10¿17 cm¿2 s¿1 sr¿1 for monopoles with velocity ß ¿ 0.625.

FLUXMuon backgroundParticle physicsGauge modelMagnetic monopolesAstrophysics::High Energy Astrophysical PhenomenaMagnetic monopoleneutrino telescopes; antares; magnetic monopoleFOS: Physical sciencesCosmic ray01 natural sciencesNuclear physics0103 physical sciencesNeutronFIELD010306 general physicsDETECTORCherenkov radiationZenithHigh Energy Astrophysical Phenomena (astro-ph.HE)NeutronsPhysicsSPECTRUMAtmospheric neutrinosMagnetic monopoleANTARES:Física::Acústica [Àrees temàtiques de la UPC]MuonCharged particles010308 nuclear & particles physicsAstronomy and AstrophysicsMonopols magnèticsUpper limitsNeutrino detectorMass scaleFISICA APLICADA[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Física nuclearData setsNeutrino telescopes[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)TelescopesAstroparticle Physics
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Deep sea tests of a prototype of the KM3NeT digital optical module: KM3NeT Collaboration

2014

The first prototype of a photo-detection unit of the future KM3NeT neutrino telescope has been deployed in the deep waters of the Mediterranean Sea. This digital optical module has a novel design with a very large photocathode area segmented by the use of 31 three inch photomultiplier tubes. It has been integrated in the ANTARES detector for in-situ testing and validation. This paper reports on the first months of data taking and rate measurements. The analysis results highlight the capabilities of the new module design in terms of background suppression and signal recognition. The directionality of the optical module enables the recognition of multiple Cherenkov photons from the same $^{40…

PhysicsPhotomultiplierPhotonPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsbusiness.industryPhysics::Instrumentation and DetectorsDetectorAstrophysics::Instrumentation and Methods for Astrophysics01 natural sciencesSignalPhotocathodeOpticsKM3NeT0103 physical sciences14. Life underwaterSensitivity (control systems)010306 general physicsbusinessEngineering (miscellaneous); Physics and Astronomy (miscellaneous)Engineering (miscellaneous)Cherenkov radiation
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Constraining the neutrino emission of gravitationally lensed Flat-Spectrum Radio Quasars with ANTARES data

2014

This paper proposes to exploit gravitational lensing effects to improve the sensitivity of neutrino telescopes to the intrinsic neutrino emission of distant blazar populations. This strategy is illustrated with a search for cosmic neutrinos in the direction of four distant and gravitationally lensed Flat-Spectrum Radio Quasars. The magnification factor is estimated for each system assuming a singular isothermal profile for the lens. Based on data collected from 2007 to 2012 by the ANTARES neutrino telescope, the strongest constraint is obtained from the lensed quasar B0218+357, providing a limit on the total neutrino luminosity of this source of 1.08×10^46 erg s-1. This limit is about one o…

Point sourceAstronomyAstrophysics::High Energy Astrophysical Phenomenagravitational lensingFOS: Physical sciencesgravitational lensing; neutrino astronomyAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesLuminosityneutrino astronomyNeutrino0103 physical sciencesSensitivity (control systems)Blazar010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)gravitational lensing; neutrino astronomy; Astronomy and AstrophysicsCOSMIC cancer database010308 nuclear & particles physicshigh energy astrophysical neutrinosAstrophysics::Instrumentation and Methods for AstrophysicsFísicaQuasarAstronomy and AstrophysicsGravitational lensFISICA APLICADANeutrinoMATEMATICA APLICADAAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Measurement of the atmospheric ?µ energy spectrum from 100 GeV to 200 TeV with the ANTARES telescope

2013

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 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 similar to 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 gamma (meas)=3.58 +/- 0.12. With the present statistics the contribution of prompt neutrinos cannot be established.

Astrofísica:Desenvolupament humà i sostenible::Medi ambient [Àrees temàtiques de la UPC]Physics and Astronomy (miscellaneous)Raigs còsmicsFluxOceanografia7. Clean energy01 natural scienceslaw.inventionlawUnderwater acousticsEnergy range 0.1 to 200 TeVNeutrino TelescopePhysicsRange (particle radiation)Spectral index[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]atmospheric neutrinoNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsLorentz Invariance ViolationFLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]OscillationsSoroll -- Aspectes ambientalsAstrophysics::High Energy Astrophysical PhenomenaCosmic rayddc:500.2MACRONuclear physicsTelescopeMUONSSEARCH0103 physical sciencesNeutrinsNeutrinos010306 general physicsEngineering (miscellaneous)Cosmic raysDETECTOR:Física::Acústica [Àrees temàtiques de la UPC]ANTARESAtmospheric neutrino antineutrino010308 nuclear & particles physicsAntares telescopeHigh Energy Physics::Phenomenology[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]13. Climate actionFISICA APLICADAlorentz invariance violation; neutrino oscillation; muonsHigh Energy Physics::ExperimentEnergy (signal processing)Bar (unit)European Physical Journal C
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