Search results for "SCALAR"

showing 10 items of 1002 documents

Search for the effect of massive bodies on atomic spectra and constraints on Yukawa-type interactions of scalar particles

2016

We propose a new method to search for hypothetical scalar particles that have feeble interactions with Standard-Model particles. In the presence of massive bodies, these interactions produce a non-zero Yukawa-type scalar-field magnitude. Using radio-frequency spectroscopy data of atomic dysprosium, as well as atomic clock spectroscopy data, we constrain the Yukawa-type interactions of a scalar field with the photon, electron, and nucleons for a range of scalar-particle masses corresponding to length scales $ > 10$ cm. In the limit as the scalar-particle mass $m_\phi \to 0$, our derived limits on the Yukawa-type interaction parameters are: $\Lambda_\gamma \gtrsim 8 \times 10^{19}$ GeV, $\Lam…

Particle physicsGeneral PhysicsPhotonAtomic Physics (physics.atom-ph)General Physics and Astronomychemistry.chemical_elementFOS: Physical sciencesElectron01 natural sciencesphysics.atom-phMathematical SciencesPhysics - Atomic PhysicsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)EngineeringHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsSpectroscopyPhysics010308 nuclear & particles physicshep-exScalar (physics)Yukawa potentialhep-phHigh Energy Physics - PhenomenologychemistryPhysical SciencesDysprosiumNucleonScalar field
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Effective Majorana mass matrix from tau and pseudoscalar meson lepton number violating decays

2018

An observation of any lepton number violating process will undoubtedly point towards the existence of new physics and indirectly to the clear Majorana nature of the exchanged fermion. In this work, we explore the potential of a minimal extension of the Standard Model via heavy sterile fermions with masses in the $[ 0.1 - 10]$ GeV range concerning an extensive array of "neutrinoless" meson and tau decay processes. We assume that the Majorana neutrinos are produced on-shell, and focus on three-body decays. We conduct an update on the bounds on the active-sterile mixing elements, $|U_{\ell_\alpha 4} U_{\ell_\beta 4}|$, taking into account the most recent experimental bounds (and constraints) a…

Particle physicsNuclear and High Energy PhysicsMesonPhysics beyond the Standard ModelFOS: Physical sciences7. Clean energy01 natural sciencesPseudoscalar mesonHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)double-beta decay: (0neutrino)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityNeutrino Physics010306 general physicsnumerical calculationslepton number: violationPhysicsneutrino: heavy: decay010308 nuclear & particles physicsnew physicsHigh Energy Physics::Phenomenologyneutrino: Majorana: massFermionneutrino: sterileMass matrixsensitivityLepton numberMAJORANAHigh Energy Physics - Phenomenologypseudoscalar meson: decay[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Beyond Standard Modellcsh:QC770-798neutrino: Majorana[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experimenttau: decayNeutrinoneutrino: mixing
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Spin alignment and violation of the OZI rule in exclusive ω and ϕ production in pp collisions

2014

Exclusive production of the isoscalar vector mesons $\omega$ and $\phi$ is measured with a 190 GeV$/c$ proton beam impinging on a liquid hydrogen target. Cross section ratios are determined in three intervals of the Feynman variable $x_{F}$ of the fast proton. A significant violation of the OZI rule is found, confirming earlier findings. Its kinematic dependence on $x_{F}$ and on the invariant mass $M_{p\mathrm{V}}$ of the system formed by fast proton $p_\mathrm{fast}$ and vector meson $V$ is discussed in terms of diffractive production of $p_\mathrm{fast}V$ resonances in competition with central production. The measurement of the spin density matrix element $\rho_{00}$ of the vector mesons…

Particle physicsNuclear and High Energy PhysicsOZI rule testPOLARIZATIONProtonMesonPROTON-PROTON COLLISIONS; LOW-ENERGY PHOTOPRODUCTION; ZWEIG-IIZUKA RULE; MESON PRODUCTION; EXPERIMENTAL TESTS; SELECTION RULE; POLARIZATION; NUCLEON; PIONIsoscalarPROTON-PROTON COLLISIONSMESON PRODUCTIONNuclear TheoryEXPERIMENTAL TESTS530OZI ruleHigh Energy Physics - ExperimentNuclear physicstestPIONInvariant masslcsh:Nuclear and particle physics. Atomic energy. RadioactivityLOW-ENERGY PHOTOPRODUCTIONVector mesonNuclear ExperimentNUCLEONNuclear ExperimentSpin-½PhysicsHigh Energy Physics::PhenomenologySELECTION RULEBaryonOZI ruleZWEIG-IIZUKA RULElcsh:QC770-798High Energy Physics::ExperimentParticle Physics - Experiment
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Observing Higgs boson production through its decay into gamma-rays: A messenger for Dark Matter candidates

2012

In this Letter, we study the gamma-ray signatures subsequent to the production of a Higgs boson in space by dark matter annihilations. We investigate the cases where the Higgs boson is produced at rest or slightly boosted and show that such configurations can produce characteristic bumps in the gamma-ray data. These results are relevant in the case of the Standard Model-like Higgs boson provided that the dark matter mass is about 63 GeV, 109 GeV or 126 GeV, but can be generalized to any other Higgs boson masses. Here, we point out that it may be worth looking for a 63 GeV line since it could be the signature of the decay of a Standard Model-like Higgs boson produced in space, as in the case…

Particle physicsNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesNeutralino annihilationElementary particle7. Clean energy01 natural sciencesNuclear physicssymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsLight dark matterBosonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]High Energy Physics::PhenomenologyScalar bosonHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Higgs bosonsymbolsHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaHiggs mechanismRoot-s=7 tev
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Measurement of the proton scalar polarizabilities at MAMI

2019

The electric (αE1) and magnetic (βM1) scalar polarizabilities describe the response of the nucleon to an applied electric or magnetic field. They are not only fundamental properties related to the internal structure and dynamics of the nucleon, but they are important also in other areas of physics, such as atomic structure. The values of αE1 and βM1 quoted by the Particle Data Group were determined using data on the unpolarized differential cross-section of the Compton scattering $\gamma p \to \gamma p$. The measurement of the beam asymmetry Σ3, provides an alternative approach to the extraction of the scalar polarizabilities, with different sensitivity and systematics compared to the unpol…

Particle physicsPhoton530 PhysicsQC1-999media_common.quotation_subject01 natural sciencesAsymmetryNuclear physicsPion0103 physical sciences500 Natural sciences and mathematicsNuclear Experiment010306 general physicsmedia_commonPhysics010308 nuclear & particles physicsLinear polarizationPhysicsCompton scatteringScalar (physics)Particle Data Group530 PhysikMagnetic field500 NaturwissenschaftenNucleonCrystal BallProceedings of XVII International Conference on Hadron Spectroscopy and Structure — PoS(Hadron2017)
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Photons, Photon Jets and Dark Photons at 750 GeV and Beyond

2016

In new physics searches involving photons at the LHC, one challenge is to distinguish scenarios with isolated photons from models leading to "photon jets". For instance, in the context of the 750 GeV diphoton excess, it was pointed out that a true diphoton resonance $S \to \gamma\gamma$ can be mimicked by a process of the form $p p \to S \to a a \to 4\gamma$, where $S$ is a new scalar with a mass of 750 GeV and $a$ is a light pseudoscalar decaying to two collinear photons. Photon jets can be distinguished from isolated photons by exploiting the fact that a large fraction of photons convert to an $e^+e^-$ pair inside the inner detector. In this note, we quantify this discrimination power, an…

Particle physicsPhotonPhysics and Astronomy (miscellaneous)Physics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaScalar (mathematics)collinearFOS: Physical sciencesPhysics::OpticsContext (language use)Jet (particle physics)01 natural sciencesDark photonHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)jet [photon]0103 physical sciencesddc:530010306 general physicspseudoscalarEngineering (miscellaneous)two-photonlifetimePhysicsnew physics010308 nuclear & particles physics750 GeV diphoton excesssensitivityPseudoscalarHigh Energy Physics - PhenomenologyCERN LHC CollHigh Energy Physics::ExperimentRegular Article - Theoretical Physics
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Search for massive colored scalars in four-jet final states in √s = 7 TeV proton–proton collisions with the ATLAS detector

2011

A search for pair-produced scalar particles decaying to a four-jet final state is presented. The analysis is performed using an integrated luminosity of 34 pb[superscript −1] recorded by the ATLAS detector in 2010. No deviation from the Standard Model is observed. For a scalar mass of 100 GeV (190 GeV) the limit on the scalar gluon pair production cross section at 95% confidence level is 1 nb (0.28 nb). When these results are interpreted as mass limits, scalar-gluons (hyperpions) with masses of 100 to 185 GeV (100 to 155 GeV) are excluded at 95% confidence level with the exception of a mass window of width about 5 GeV (15 GeV) around 140 GeV.

Particle physicsPhysics and Astronomy (miscellaneous)Ciências Naturais::Ciências FísicasAtlas detectorAstrophysics::High Energy Astrophysical Phenomena:Ciências Físicas [Ciências Naturais]Scalar (mathematics)FOS: Physical sciencesddc:500.27. Clean energy01 natural sciences530Partícules (Física nuclear)High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Fysikddc:530High Energy PhysicsPP Collisions010306 general physicsNuclear ExperimentEngineering (miscellaneous)Ciencias ExactasPhysicsATLAS detector010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleFísicascalarsSupersymmetryATLASmassive colored scalars; proton–proton collisions; ATLAS detectorGluonPair productionPhysical SciencesFísica nuclearproton-proton collisionsHigh Energy Physics::ExperimentLHCSupersymmetryParticle Physics - Experiment
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Spin-dependence of gravity-mediated dark matter in warped extra-dimensions

2021

We study the spin-dependence of Dark Matter (DM) particles which interact gravitationally with the Standard Model (SM) in an extra-dimensional Randall-Sundrum scenario. We assume that both the Dark Matter and the Standard Model are confined to the TeV (Infra-red) brane and only interact via gravitational mediators, namely Kaluza-Klein gravitons and the radion. We analyze the different DM annihilation channels and find that it is possible to achieve the presently observed relic abundance of Dark Matter, $\Omega_{\rm DM}$, within the freeze-out mechanism for DM particles of spin 0, 1/2 and 1. We study the region of the model parameter space for which $\Omega_{\rm DM}$ is achieved and compare …

Particle physicsPhysics and Astronomy (miscellaneous)Dark matterScalar (mathematics)FOS: Physical scienceslcsh:Astrophysics01 natural sciences7. Clean energyStandard ModelVector bosonHigh Energy Physics - Phenomenology (hep-ph)lcsh:QB460-4660103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsEngineering (miscellaneous)Spin-½High Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyGravitonHigh Energy Physics - PhenomenologyExtra dimensionslcsh:QC770-798DilatonAstrophysics - High Energy Astrophysical PhenomenaThe European Physical Journal C
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Phenomenology of scotogenic scalar dark matter

2020

We reexamine the minimal Singlet + Triplet Scotogenic Model, where dark matter is the mediator of neutrino mass generation. We assume it to be a scalar WIMP, whose stability follows from the same $\mathbb{Z} _{2}$ symmetry that leads to the radiative origin of neutrino masses. The scheme is the minimal one that allows for solar and atmospheric mass scales to be generated. We perform a full numerical analysis of the signatures expected at dark matter as well as collider experiments. We identify parameter regions where dark matter predictions agree with theoretical and experimental constraints, such as neutrino oscillations, Higgs data, dark matter relic abundance and direct detection searche…

Particle physicsPhysics and Astronomy (miscellaneous)Dark matterScalar (mathematics)FOS: Physical scienceslcsh:AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsComputer Science::Digital Libraries7. Clean energy01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:QB460-466lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsNeutrino oscillationEngineering (miscellaneous)Light dark matterPhysics010308 nuclear & particles physicsMass generationHigh Energy Physics - PhenomenologyComputer Science::Mathematical SoftwareHiggs bosonlcsh:QC770-798High Energy Physics::ExperimentNeutrinoPhenomenology (particle physics)
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The ultraviolet landscape of two-Higgs doublet models

2018

We study the predictions of generic ultraviolet completions of two-Higgs doublet models. We assume that at the matching scale between the two-Higgs doublet model and a ultraviolet complete theory -- which can be anywhere between the TeV and the Planck scale -- arbitrary but perturbative values for the quartic couplings are present. We evaluate the couplings down from the matching scale to the weak scale and study the predictions for the scalar mass spectrum. In particular, we show the importance of radiative corrections which are essential for both an accurate Higgs mass calculation as well as determining the stability of the electroweak vacuum. We study the relation between the mass splitt…

Particle physicsPhysics and Astronomy (miscellaneous)Scale (ratio)Scalar (mathematics)FOS: Physical scienceslcsh:Astrophysics01 natural sciencesStability (probability)High Energy Physics - Phenomenology (hep-ph)Quartic functionlcsh:QB460-4660103 physical sciencesRadiative transferddc:530lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsEngineering (miscellaneous)Physics010308 nuclear & particles physicsPhysicsElectroweak interactionHigh Energy Physics::PhenomenologyHigh Energy Physics - PhenomenologyMass spectrumHiggs bosonlcsh:QC770-798Regular Article - Theoretical Physics
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