Search results for "PARTICLE PHYSICS"

showing 10 items of 6826 documents

Searching for a hidden sector in multiparticle production at LHC

2016

A hidden sector beyond the Standard Model can show up in multiparticle production altering inclusive correlations and factorial cumulants of multiplicity distributions. In this report such a study is advocated with a special emphasis on the searches at LHC.

Hidden sectorPhysicsFactorialParticle physicsLarge Hadron ColliderPhysicsQC1-999Physics beyond the Standard ModelMultiplicity (mathematics)CumulantParticle Physics - ExperimentEPJ Web of Conferences
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D6-brane model building onZ2×Z6: MSSM-like and left–right symmetric models

2015

Abstract We perform a systematic search for globally defined MSSM-like and left–right symmetric models on D6-branes on the T 6 / ( Z 2 × Z 6 × Ω R ) orientifold with discrete torsion. Our search is exhaustive for models that are independent of the value of the one free complex structure modulus. Preliminary investigations suggest that there exists one prototype of visible sector for MSSM-like and another for left–right symmetric models with differences arising from various hidden sector completions to global models. For each prototype, we provide the full matter spectrum, as well as the Yukawa and other three-point couplings needed to render vector-like matter states massive. This provides …

Hidden sectorQuarkPhysicsNuclear and High Energy PhysicsTheoretical physicsParticle physicsOrientifoldHigh Energy Physics::PhenomenologyYukawa potentialBraneAxionLeptonMinimal Supersymmetric Standard ModelNuclear Physics B
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Effects of modified theories of gravity on neutrino pair annihilation energy deposition near neutron stars

2020

We study the neutrino pairs annihilation into electron-positron pairs ($\nu+{\bar \nu}\to e^- + e^+$) near the surface of a neutron star. The analysis is performed in the framework of extended theories of gravity. The latter induce a modification of the minimum photon-sphere radius ($R_{ph}$) and the maximum energy deposition rate near to $R_{ph}$, as compared to ones of General Relativity. These results might lead to an efficient mechanism for generating GRBs.

High Energy Astrophysical Phenomena (astro-ph.HE)Astroparticle physicsPhysicsParticle physicsAnnihilation010504 meteorology & atmospheric sciencesGeneral relativityHigh-energy astronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Radius01 natural sciencesGeneral Relativity and Quantum CosmologyNeutron starHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Space and Planetary Science0103 physical sciencesNeutrinoGamma-ray burstAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysics0105 earth and related environmental sciences
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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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On the flavor composition of the high-energy neutrinos in IceCube

2016

The IceCube experiment has recently released 3 years of data of the first ever detected high-energy (>30 TeV) neutrinos, which are consistent with an extraterrestrial origin. In this talk, we compute the compatibility of the observed track-to-shower ratio with possible combinations of neutrino flavors with relative proportion (alpha_e:alpha_mu:alpha_tau). Although this observation is naively favored for the canonical (1:1:1) at Earth, once we consider the IceCube expectations for the atmospheric muon and neutrino backgrounds, this flavor combination presents some tension with data. We find that, for an astrophysical neutrino E_nu^{-2} energy spectrum, (1:1:1) at Earth is currently disfav…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsNuclear and High Energy PhysicsHigh energyParticle physicsMuon010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical scienceshigh-energy neutrinos01 natural sciencesIceCubeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)flavor ratios0103 physical sciencesEnergy spectrumHigh Energy Physics::ExperimentNeutrino010306 general physicsAstrophysics - High Energy Astrophysical PhenomenaFlavorNuclear and Particle Physics Proceedings
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Unifying leptogenesis, dark matter and high-energy neutrinos with right-handed neutrino mixing via Higgs portal

2016

We revisit a model in which neutrino masses and mixing are described by a two right-handed (RH) neutrino seesaw scenario, implying a strictly hierarchical light neutrino spectrum. A third decoupled RH neutrino, $N_{\rm DM}$ with mass $M_{\rm DM}$, plays the role of cold dark matter (DM) and is produced by the mixing with a source RH neutrino, $N_{\rm S}$ with mass $M_{\rm S}$, induced by Higgs portal interactions. The same interactions are also responsible for $N_{\rm DM}$ decays. We discuss in detail the constraints coming from DM abundance and stability conditions, showing that in the hierarchical case ($M_{\rm DM} \gg M_{\rm S}$) there is an allowed window on $M_{\rm DM}$, which necessar…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsParticle physicsCold dark matter010308 nuclear & particles physicsPhysics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesAstronomy and Astrophysics7. Clean energy01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Baryon asymmetryNeutrino detector13. Climate actionLeptogenesis0103 physical sciencesInvariant massHigh Energy Physics::ExperimentNeutrino010306 general physicsAstrophysics - High Energy Astrophysical Phenomena
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Modified majoron model for cosmological anomalies

2020

The vacuum expectation value $v_s$ of a Higgs triplet field $\Delta$ carrying two units of lepton number $L$ induces neutrino masses $\propto v_s$. The neutral component of $\Delta$ gives rise to two Higgs particles, a pseudoscalar $A$ and a scalar $S$. The most general renormalizable Higgs potential $V$ for $\Delta $ and the Standard-Model Higgs doublet $\Phi$ does not permit the possibility that the mass of either $A$ or $S$ is small, of order $v_s$, while the other mass is heavy enough to forbid the decay $Z\to A S$ to comply with LEP 1 data. We present a model with additional dimension-6 terms in $V$, in which this feature is absent and either $A$ or $S$ can be chosen light. Subsequentl…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologyFOS: Physical sciencesOrder (ring theory)01 natural sciencesLepton numberPseudoscalarHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHiggs bosonddc:530High Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical Phenomena010306 general physicsAstrophysics - Cosmology and Nongalactic AstrophysicsVacuum expectation valueMajoronBosonPhysical Review D
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Updated collider and direct detection constraints on Dark Matter models for the Galactic Center gamma-ray excess

2016

Utilizing an exhaustive set of simplified models, we revisit dark matter scenarios potentially capable of generating the observed Galactic Center gamma-ray excess, updating constraints from the LUX and PandaX-II experiments, as well as from the LHC and other colliders. We identify a variety of pseudoscalar mediated models that remain consistent with all constraints. In contrast, dark matter candidates which annihilate through a spin-1 mediator are ruled out by direct detection constraints unless the mass of the mediator is near an annihilation resonance, or the mediator has a purely vector coupling to the dark matter and a purely axial coupling to Standard Model fermions. All scenarios in w…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Large Hadron ColliderAnnihilation010308 nuclear & particles physicsPhysics beyond the Standard ModelDark matterGalactic CenterFOS: Physical sciencesAstronomy and AstrophysicsFermion01 natural sciencesStandard ModelPseudoscalarHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesAstrophysics - High Energy Astrophysical Phenomena010306 general physicsAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Hidden sector dark matter and the Galactic Center gamma-ray excess: a closer look

2017

Stringent constraints from direct detection experiments and the Large Hadron Collider motivate us to consider models in which the dark matter does not directly couple to the Standard Model, but that instead annihilates into hidden sector particles which ultimately decay through small couplings to the Standard Model. We calculate the gamma-ray emission generated within the context of several such hidden sector models, including those in which the hidden sector couples to the Standard Model through the vector portal (kinetic mixing with Standard Model hypercharge), through the Higgs portal (mixing with the Standard Model Higgs boson), or both. In each case, we identify broad regions of parame…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsParticle physicsHyperchargeCosmology and Nongalactic Astrophysics (astro-ph.CO)Large Hadron Collider010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyDark matterFOS: Physical sciencesAstronomy and AstrophysicsContext (language use)01 natural sciencesStandard ModelHidden sectorHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Antiproton0103 physical sciencesHiggs bosonAstrophysics - High Energy Astrophysical Phenomena010306 general physicsAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Robustness of cosmological axion mass limits

2015

We present cosmological bounds on the thermal axion mass in an extended cosmological scenario in which the primordial power spectrum of scalar perturbations differs from the usual power-law shape predicted by the simplest inflationary models. The power spectrum is instead modeled by means of a "piecewise cubic Hermite interpolating polynomial" (PCHIP). When using Cosmic Microwave Background measurements combined with other cosmological data sets, the thermal axion mass constraints are degraded only slightly. The addition of the measurements of $\sigma_8$ and $\Omega_m$ from the 2013 Planck cluster catalogue on galaxy number counts relaxes the bounds on the thermal axion mass, mildly favouri…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsParticle physicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsCosmic microwave backgroundScalar (mathematics)Cosmic background radiationFOS: Physical sciencesFísicaSpectral densityAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesCosmologysymbols.namesake13. Climate action0103 physical sciencessymbolsPlanckNeutrino010306 general physicsAstrophysics - High Energy Astrophysical PhenomenaAxionAstrophysics - Cosmology and Nongalactic Astrophysics
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