0000000000420156

AUTHOR

J. C. Arteaga-velázquez

showing 4 related works from this author

Long-lived particles at the energy frontier: the MATHUSLA physics case

2019

We examine the theoretical motivations for long-lived particle (LLP) signals at the LHC in a comprehensive survey of Standard Model (SM) extensions. LLPs are a common prediction of a wide range of theories that address unsolved fundamental mysteries such as naturalness, dark matter, baryogenesis and neutrino masses, and represent a natural and generic possibility for physics beyond the SM (BSM). In most cases the LLP lifetime can be treated as a free parameter from the $\mu$m scale up to the Big Bang Nucleosynthesis limit of $\sim 10^7$m. Neutral LLPs with lifetimes above $\sim$ 100m are particularly difficult to probe, as the sensitivity of the LHC main detectors is limited by challenging …

Physics::Instrumentation and DetectorsPhysics beyond the Standard ModelHEAVY MAJORANA NEUTRINOSGeneral Physics and Astronomy01 natural sciencesMathematical SciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)NaturalnessCERN LHC Coll: upgrade[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]neutrino: masslong-lived particlesPhysicsLarge Hadron Collidernew physicsCMShierarchy problemneutrinosHierarchy problemhep-phATLASDARK-MATTER SEARCHESCOSMIC-RAYSmissing-energyHigh Energy Physics - PhenomenologyLarge Hadron ColliderPhysical SciencesNeutrinoLIGHT HIGGS-BOSONParticle Physics - ExperimentParticle physicsGeneral PhysicsSTERILE NEUTRINOSPHI-MESON DECAYSnucleosynthesis: big bangDark matterFOS: Physical sciencesEXTENSIVE AIR-SHOWERSdark matterVECTOR GAUGE BOSON0103 physical sciences010306 general physicsnumerical calculationsParticle Physics - PhenomenologyLEFT-RIGHT SYMMETRYMissing energyhep-exbackgroundBaryogenesisdark matter: detectortriggersensitivityBaryogenesis[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]simplified modelsDOUBLE-BETA DECAYparticle: long-lived
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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; $>$ 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 ($>$ 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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