0000000000535120

AUTHOR

Ernesto Belmont-moreno

showing 5 related works from this author

Charge separation relative to the reaction plane in Pb-Pb collisions atsNN=2.76  TeV

2013

Measurements of charge-dependent azimuthal correlations with the ALICE detector at the LHC are reported for Pb-Pb collisions at root s(NN) = 2.76 TeV. Two- and three-particle charge-dependent azimuthal correlations in the pseudorapidity range vertical bar eta vertical bar < 0.8 are presented as a function of the collision centrality, particle separation in pseudorapidity, and transverse momentum. A clear signal compatible with a charge-dependent separation relative to the reaction plane is observed, which shows little or no collision energy dependence when compared to measurements at RHIC energies. This provides a new insight for understanding the nature of the charge-dependent azimuthal co…

PhysicsParticle physicsRange (particle radiation)Large Hadron Collider010308 nuclear & particles physicsPlane (geometry)DetectorGeneral Physics and AstronomyCollision01 natural sciencesNuclear physicsAzimuthPseudorapidity0103 physical sciencesHigh Energy Physics::ExperimentImpact parameterNuclear Experiment010306 general physicsPhysical Review Letters
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Evidence that Ultra-High-Energy Gamma Rays are a Universal Feature Near Powerful Pulsars

2021

The highest-energy known gamma-ray sources are all located within 0.5 degrees of extremely powerful pulsars. This raises the question of whether ultra-high-energy (UHE; $&gt;$ 56 TeV) gamma-ray emission is a universal feature expected near pulsars with a high spin-down power. Using four years of data from the High Altitude Water Cherenkov (HAWC) Gamma-Ray Observatory, we present a joint-likelihood analysis of ten extremely powerful pulsars to search for UHE gamma-ray emission correlated with these locations. We report a significant detection ($&gt;$ 3$��$), indicating that UHE gamma-ray emission is a generic feature of powerful pulsars. We discuss the emission mechanisms of the gamma rays a…

Astroparticle physicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)High energyHigh-energy astronomyAstrophysics::High Energy Astrophysical PhenomenaGamma rayAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsPulsarSpace and Planetary ScienceFeature (computer vision)Astrophysics - High Energy Astrophysical Phenomena
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A survey of active galaxies at TeV photon energies with the HAWC gamma-ray observatory

2020

The High Altitude Water Cherenkov Gamma-Ray Observatory (HAWC) continuously detects TeV photons and particles within its large field-of-view, accumulating every day a deeper exposure of two thirds of the sky. We analyzed 1523~days of HAWC live data acquired over four and a half years, in a follow-up analysis of {138} nearby ($z<0.3$) active galactic nuclei from the {\em Fermi} 3FHL catalog culminating within $40^\circ$ of the zenith at Sierra Negra, the HAWC site. This search for persistent TeV emission used a maximum-likelihood analysis assuming intrinsic power-law spectra attenuated by pair production of gamma-ray photons with the extragalactic background light. HAWC clearly detects persi…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsActive galactic nucleusRadio galaxymedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaGamma rayFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsExtragalactic background lightSpace and Planetary ScienceObservatorySkyBlazarAstrophysics - High Energy Astrophysical PhenomenaCherenkov radiationmedia_common
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3HWC: The Third HAWC Catalog of Very-High-Energy Gamma-ray Sources

2020

We present a new catalog of TeV gamma-ray sources using 1523 days of data from the High Altitude Water Cherenkov (HAWC) observatory. The catalog represents the most sensitive survey of the Northern gamma-ray sky at energies above several TeV, with three times the exposure compared to the previous HAWC catalog, 2HWC. We report 65 sources detected at $\geq$ 5 sigma significance, along with the positions and spectral fits for each source. The catalog contains eight sources that have no counterpart in the 2HWC catalog, but are within $1^\circ$ of previously detected TeV emitters, and twenty sources that are more than $1^\circ$ away from any previously detected TeV source. Of these twenty new so…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)High energyHigh-energy astronomyAstrophysics::High Energy Astrophysical PhenomenaGamma rayAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsGamma-ray astronomyAstrophysics::Cosmology and Extragalactic AstrophysicsPulsarSpace and Planetary ScienceAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy Astrophysics
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J/ψPolarization inppCollisions ats=7  TeV

2012

The ALICE Collaboration has studied J/psi production in pp collisions at root s = 7 TeV at the LHC through its muon pair decay. The polar and azimuthal angle distributions of the decay muons were measured, and results on the J/psi polarization parameters lambda(theta) and lambda(phi) were obtained. The study was performed in the kinematic region 2: 5 < y < 4, 2 < p(t) < 8 GeV/c, in the helicity and Collins-Soper reference frames. In both frames, the polarization parameters are compatible with zero, within uncertainties.

PhysicsParticle physicsMuonLarge Hadron ColliderPhysics::Instrumentation and Detectors010308 nuclear & particles physicsGeneral Physics and AstronomyLambdaPolarization (waves)01 natural sciencesHelicityNuclear physicsAzimuthAngular distribution0103 physical sciencesHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsReference framePhysical Review Letters
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