Search results for " Detectors"

showing 10 items of 2027 documents

Physics beyond colliders at CERN: beyond the Standard Model working group report

2019

The Physics Beyond Colliders initiative is an exploratory study aimed at exploiting the full scientific potential of the CERN's accelerator complex and scientific infrastructures through projects complementary to the LHC and other possible future colliders. These projects will target fundamental physics questions in modern particle physics. This document presents the status of the proposals presented in the framework of the Beyond Standard Model physics working group, and explore their physics reach and the impact that CERN could have in the next 10–20 years on the international landscape.

HIGH-ENERGYHigh energyaxionsPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsPhysics beyond the Standard Model01 natural sciencesHigh Energy Physics - Experimentdark matter: couplingHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)photon: coupling[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Detectors and Experimental Techniquesphysics.ins-detPHOTON VETO DETECTORdark sectorPhysicsLarge Hadron Colliderneutrino: pair productionnew physics: search forlepton: flavor: violationdark matter: pair productionhep-phInstrumentation and Detectors (physics.ins-det)photon: invisible decayNEUTRAL HEAVY-LEPTONSHigh Energy Physics - PhenomenologyLIGHTCERN LHC Collphoton: mixingSystems engineeringParticle Physics - ExperimentNuclear and High Energy PhysicsCERN LabacceleratorPHI-MESON DECAYSExploratory researchFOS: Physical sciences530dark matterStandard ModelELECTRIC-DIPOLE MOMENTacceleratorsVECTOR GAUGE BOSONSEARCH0103 physical sciencesDARK-MATTERddc:530K: semileptonic decay[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]particle physics010306 general physicsvector boson: postulated particleCP CONSERVATIONbeyond standard ModelParticle Physics - Phenomenologylepton: universalityphoton: hidden sectorbeyond standard Model; dark matter; dark sector; axions; particle physics; acceleratorshep-ex010308 nuclear & particles physicscoupling constantCERN SPSlandscapeAccelerators and Storage Ringsdark matter: mediation[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Fundamental physicsPhysics::Accelerator Physicsaxion: solarJournal of Physics G: Nuclear and Particle Physics
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Searching for long-lived particles beyond the Standard Model at the Large Hadron Collider

2020

Particles beyond the Standard Model (SM) can generically have lifetimes that are long compared to SM particles at the weak scale. When produced at experiments such as the Large Hadron Collider (LHC) at CERN, these longlived particles (LLPs) can decay far from the interaction vertex of the primary proton–proton collision. Such LLP signatures are distinct from those of promptly decaying particles that are targeted by the majority of searches for new physics at the LHC, often requiring customized techniques to identify, for example, significantly displaced decay vertices, tracks with atypical properties, and short track segments. Given their non-standard nature, a comprehensive overview of LLP…

HIGH-ENERGYbeyond the Standard Modellarge hadron colliderPhysics::Instrumentation and DetectorsPROTON-PROTON COLLISIONSPhysics beyond the Standard Modelbeyond the standard model01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)high-luminosity lhcHigh Energy Physics - Phenomenology (hep-ph)MAGNETIC MONOPOLESlong-lived [particle]high-energy collider experimentsdecay: vertexscattering [p p][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]long-lived particlesQCproposed [detector]Physicslifetimedark gauge forcesLarge Hadron ColliderCMSROOT-S=13 TEVroot-s=13 tevPhysicsnew physics: search forscale: electroweak interactionhep-phATLASelectroweak interaction [scale]vertex [decay]upgrade [detector]High Energy Physics - Experiment; High Energy Physics - Experiment; High Energy Physics - Phenomenologydetector: upgradeSettore FIS/02 - Fisica Teorica Modelli e Metodi Matematiciprimary [vertex]ddc:High Energy Physics - PhenomenologyCERN LHC CollLarge Hadron Colliderbaryon asymmetryvertex: primaryLHCcolliding beams [p p]exclusion limitspp collisionsParticle Physics - ExperimentsignatureNuclear and High Energy PhysicsParticle physicsp p: scatteringCERN LabPAIR PRODUCTIONcollider phenomenologyreviewFOS: Physical sciencesDARK GAUGE FORCES530search for [new physics]BARYON ASYMMETRY0103 physical sciencesddc:530010306 general physicsnumerical calculationsParticle Physics - PhenomenologyEXCLUSION LIMITSmagnetic monopolesPP COLLISIONS010308 nuclear & particles physicshep-exbackgroundbibliographyshowersMAJORANA NEUTRINOSCollisiontracksLHC-Bdetector: proposedhigh-luminosity LHCpair productionMATHUSLAPhysics and Astronomy[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]proton-proton collisionshigh-energymajorana neutrinosparticle: long-livedp p: colliding beamsPhysics BSMexperimental results
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A procedure to evaluate coincidence-summing correction values in gamma-ray spectrometry with HPGe detectors

2009

The spectrometric analysis of a gamma-emitter sample measured in "close geometry" can be affected by errors due to coincidence-summing effects that can occur when two or more coincident photons (real coincidences) within the resolution time of the spectrometric system are emitted. The probability that these effects occur depends primarily on the nuclide decay scheme, the sample-detector distance and detector intrinsic-efficiency whereas results independent from the sample nuclide activity. Coincidence-summing corrections of the photopeak areas are requested, in particular, when the gamma ray spectrometric analysis is aimed to efficiency or activity determination. In this work is reported a …

HPge detectorsgamma-ray spectrometrySettore ING-IND/20 - Misure E Strumentazione Nuclearicoincidence-summing
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Fabrication of Bismuth Absorber Arrays for NTD-Ge Hard X-ray Microcalorimeters

2020

The high-spectral-resolution detection of hard X-rays (E > 20 keV) is a challenging and nearly unexplored area in space astrophysics. Traditionally hard X-ray detectors present moderate spectral resolutions, although few tens of eV one could open new frontiers in the study of nuclear processes and high-temperature plasma dynamics in energetic processes. This can be achieved by using cryogenic microcalorimeters. Within a research activity aimed at developing arrays of neutron transmutation-doped germanium (NTD-Ge) microcalorimeters for the high-spectral-resolution detection (about 50 eV@60 keV) of hard X-rays (20 keV < E<100 keV), we developed an electroplating process to fabricate …

Hard X-rays · Low-temperature detectors · NTD-Ge microcalorimeters ·Bismuth absorbers · Bismuth electroplatingMaterials scienceFabricationPhysics::Instrumentation and Detectorsbusiness.industryAstrophysics::High Energy Astrophysical PhenomenaDetectorX-raychemistry.chemical_elementGermaniumPlasmaCondensed Matter Physics01 natural sciencesAtomic and Molecular Physics and Optics010305 fluids & plasmasBismuthSettore FIS/05 - Astronomia E AstrofisicachemistryHard X-rays0103 physical sciencesOptoelectronicsGeneral Materials ScienceNeutron010306 general physicsbusiness
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Impact of CMS dijets in 5.02 TeV pPb and pp collisions on EPPS16 nuclear PDFs

2018

The CMS measurement of dijet pseudorapidity distributions in pPb versus pp collisions at 5.02 TeV provides a direct probe on nuclear gluon PDFs. We show that while the predicted pPb pseudorapidity distributions suffer from sizable free-proton PDF uncertainties, the ratios of the pPb and pp distributions are practically insensitive to scale and free-proton PDF choices. We find the CMS data on pPb to pp ratios to be in good agreement with the EPPS16 nuclear modifications. Using a non-quadratic extension of the Hessian PDF reweighting method, we study the impact of these data on the EPPS16 nuclear PDFs. Relative to EPPS16, we find stronger evidence for mid-x gluon antishadowing as well as indi…

Hessian matrixPhysicsParticle physicsScale (ratio)Physics::Instrumentation and DetectorsHigh Energy Physics::PhenomenologyNuclear TheoryFOS: Physical scienceshiukkasfysiikka114 Physical sciencesGluonHigh Energy Physics - Phenomenologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)13. Climate actionPseudorapiditysymbolsHigh Energy Physics::ExperimentydinfysiikkaNuclear Experiment
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On the peculiar long-term orbital evolution of the eclipsing accreting millisecond X-ray pulsar SWIFT J1749.4-2807

2022

We present the pulsar timing analysis of the accreting millisecond X-ray pulsar SWIFT J1749.4-2807 monitored by NICER and XMM-Newton during its latest outburst after almost eleven years of quiescence. From the coherent timing analysis of the pulse profiles, we updated the orbital ephemerides of the system. Large phase jumps of the fundamental frequency phase of the signal are visible during the outburst, consistent with what was observed during the previous outburst. Moreover, we report on the marginally significant evidence for non-zero eccentricity ($e\simeq 4\times 10^{-5}$) obtained independently from the analysis of both the 2021 and 2010 outbursts and we discuss possible compatible sc…

High Energy Astrophysical Phenomena (astro-ph.HE)Accretiongeneral [Binaries]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesneutron [Stars]Astronomy and Astrophysicsstars: neutronX-rays: binariesSettore FIS/05 - Astronomia E Astrofisicabinaries: generalSpace and Planetary Scienceaccretion accretion discsbinaries [X-rays][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Accretion discs
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Inflation meets neutrinos

2019

Constraints on inflationary models typically assume only the standard models of cosmology and particle physics. By extending the neutrino sector to include a new interaction with a light scalar mediator ($m_{\phi}\sim$MeV), it is possible to relax these constraints, in particular via opening up regions of the parameter space of the spectral index $n_s$. These new interactions can be probed at IceCube via interactions of astrophysical neutrinos with the Cosmic Neutrino Background for nearly all of the relevant parameter space.

High Energy Astrophysical Phenomena (astro-ph.HE)High Energy Physics - PhenomenologyCosmology and Nongalactic Astrophysics (astro-ph.CO)High Energy Physics - Phenomenology (hep-ph)Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic Astrophysics
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The Flavour Composition of the High-Energy IceCube Neutrinos

2015

We present an in-depth analysis of the flavour and spectral composition of the 36 high-energy neutrino events observed after three years of observation by the IceCube neutrino telescope. While known astrophysical sources of HE neutrinos are expected to produce a nearly $(1:1:1)$ flavour ratio (electron : muon : tau) of neutrinos at earth, we show that the best fits based on the events detected above $E_\nu \ge 28$ TeV do not necessarily support this hypothesis. Crucially, the energy range that is considered when analysing the HE neutrino data can have a profound impact on the conclusions. We highlight two intriguing puzzles: an apparent deficit of muon neutrinos, seen via a deficit of track…

High Energy Astrophysical Phenomena (astro-ph.HE)High Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical sciencesHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaHigh Energy Physics - Experiment
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Validation of high voltage power supplies for the 1-inch photomultipliers of AugerPrime, the Pierre Auger Observatory upgrade

2022

In the framework of the upgrade of the Pierre Auger Observatory, a new high voltage module is being employed for the power supply of the 1-inch photomultiplier added to each water-Cherenkov detector of the surface array with the aim of increasing the dynamic range of the measurements. This module is located in a dedicated box near the electronics and comprises a low consumption DC-DC converter hosted inside an aluminum box. All the modules have undergone specific tests to verify their reliability in the extreme environmental conditions of the Argentinian pampa. In this paper, we describe the validation procedure and the facility developed to this aim. The successful results of the tests on …

High Energy Astrophysical Phenomena (astro-ph.HE)Physics - Instrumentation and DetectorsLarge detector systems for particle and astroparticle physicsCherenkov detectorsSettore FIS/01 - Fisica SperimentaleFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)Detector design and construction technologies and materialsAstrophysics - High Energy Astrophysical PhenomenaInstrumentationVoltage distributionsMathematical Physics
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High energy neutrino telescopes in the Northern Hemisphere

2012

We review the status and results of the high energy neutrino telescopes in the Northern Hemisphere, namely ANTARES and Baikal (NT200+).

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsNuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaDark matterAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomyFísicaAstrophysicsSolar neutrino problemPhysics::GeophysicsNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical PhenomenaNeutrino oscillationInstrumentationAstrophysics::Galaxy Astrophysics
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