Search results for "The Standard Model"

showing 10 items of 466 documents

Impeded Dark Matter

2016

We consider dark matter models in which the mass splitting between the dark matter particles and their annihilation products is tiny. Compared to the previously proposed Forbidden Dark Matter scenario, the mass splittings we consider are much smaller, and are allowed to be either positive or negative. To emphasize this modification, we dub our scenario "Impeded Dark Matter". We demonstrate that Impeded Dark Matter can be easily realized without requiring tuning of model parameters. For negative mass splitting, we demonstrate that the annihilation cross-section for Impeded Dark Matter depends linearly on the dark matter velocity or may even be kinematically forbidden, making this scenario al…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsNuclear and High Energy PhysicsAnnihilation010308 nuclear & particles physicsPhysics beyond the Standard ModelDark matterCosmic microwave backgroundFOS: Physical sciencesObservableAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Negative mass0103 physical sciences010306 general physicsAstrophysics - High Energy Astrophysical PhenomenaLight dark matterDwarf galaxy
researchProduct

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
researchProduct

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
researchProduct

Looking at the axionic dark sector with ANITA

2020

The ANITA experiment has recently observed two anomalous events emerging from well below the horizon. Even though they are consistent with tau cascades, a high energy Standard Model or Beyond the Standard Model explanation is challenging and in tension with other experiments. We study under which conditions the reflection of generic radio pulses can reproduce these signals. We propose that these pulses can be resonantly produced in the ionosphere via axion-photon conversion. This naturally explains the direction and polarization of the events and avoids other experimental bounds.

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsPhysics beyond the Standard ModelFOS: Physical scienceslcsh:AstrophysicsPolarization (waves)01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Quantum electrodynamicslcsh:QB460-4660103 physical scienceslcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityIonosphereAstrophysics - High Energy Astrophysical Phenomena010306 general physicsEngineering (miscellaneous)Astronomia ObservacionsThe European Physical Journal C
researchProduct

Scalar contributions to b→c(u)τν transitions

2017

Abstract We perform a comprehensive analysis of scalar contributions in b → c τ ν transitions including the latest measurements of R ( D ( ⁎ ) ) , the q 2 differential distributions in B → D ( ⁎ ) τ ν , the τ polarization asymmetry for B → D ⁎ τ ν , and the bound derived from the total width of the B c meson. We find that scalar contributions with the simultaneous presence of both left- and right-handed couplings to quarks can explain the available data, specifically R ( D ( ⁎ ) ) together with the measured differential distributions. However, the constraints from the total B c width present a slight tension with the current data on B → D ⁎ τ ν in this scenario, preferring smaller values fo…

High Energy Physics - Phenomenology; High Energy Physics - Phenomenology; High Energy Physics - Experiment; Nuclear and High Energy PhysicsQuarkPhysicsNuclear and High Energy PhysicsParticle physicsMeson010308 nuclear & particles physicsPhysics beyond the Standard Modelmedia_common.quotation_subjectObservablePolarization (waves)01 natural sciences7. Clean energyAsymmetrylcsh:QC1-999High Energy Physics - ExperimentBaryonHigh Energy Physics - Phenomenology0103 physical sciencesCurrent vector010306 general physicslcsh:Physicsmedia_commonPhysics Letters B
researchProduct

QCD and Strongly Coupled Gauge Theories: Challenges and Perspectives

2014

We dedicate this document to the memory of Mikhail Polikarpov, who passed away in July 2013. Misha worked with us for decades as a convener of the “Confinement” section of the Quark Confinement and Hadron Spectrum Series. He guided and expanded the scientific discussion of that topic, inspiring and under taking new research avenues. From its initial conception, he supported the enterprise of this document and organized Sect. 8, writing the part on confinement himself. He attracted the XIth Conference on Quark Confinement and the Hadron Spectrum to St. Petersburg (September 8-12, 2014; see http://phys.spbu.ru/confxi.html). His warm and kind personality, his high sense of humor, his ideas in …

High Energy Physics - TheoryEFFECTIVE-FIELD-THEORYNuclear TheoryPhysics and Astronomy (miscellaneous)Physics beyond the Standard ModelReviewHEAVY-ION COLLISIONSnucl-ex7. Clean energyCosmologyHigh Energy Physics - ExperimentQUARK-GLUON PLASMADEEP-INELASTIC SCATTERINGHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Gauge theoryNuclear Experiment (nucl-ex)Nuclear ExperimentQuantum chromodynamicsPhysics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]hep-thHigh Energy Physics - Lattice (hep-lat)hep-phddc:High Energy Physics - PhenomenologyYANG-MILLS THEORYastro-ph.COAstrophysics - Cosmology and Nongalactic AstrophysicsPB-PB COLLISIONSParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)nucl-th[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]530 PhysicsStrong interactionComplex systemFOS: Physical scienceshep-lat[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]CHIRAL PERTURBATION-THEORY114 Physical sciencesELECTRIC-DIPOLE MOMENTNuclear Theory (nucl-th)Theoretical physicsHigh Energy Physics - Latticeddc:530Engineering (miscellaneous)Particle Physics - Phenomenologyhep-ex[PHYS.HLAT]Physics [physics]/High Energy Physics - Lattice [hep-lat]NUCLEUS-NUCLEUS COLLISIONSPerspective (graphical)FísicaRADIATIVE ENERGY-LOSSFlow (mathematics)High Energy Physics - Theory (hep-th)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]European Physical Journal C
researchProduct

Discrete Abelian gauge symmetries and axions

2015

We combine two popular extensions of beyond the Standard Model physics within the framework of intersecting D6-brane models: discrete Zn symmetries and Peccei-Quinn axions. The underlying natural connection between both extensions is formed by the presence of massive U(1) gauge symmetries in D-brane model building. Global intersecting D6-brane models on toroidal orbifolds of the type T6/Z2N and T6/Z2xZ2M with discrete torsion offer excellent playgrounds for realizing these extensions. A generation-dependent Z2 symmetry is identified in a global Pati-Salam model, while global left-right symmetric models give rise to supersymmetric realizations of the DFSZ axion model. In one class of the lat…

High Energy Physics - TheoryHistoryPhysics beyond the Standard ModelFOS: Physical sciencesD-brane01 natural sciencesEducationTheoretical physicsHigh Energy Physics::TheoryHigh Energy Physics - Phenomenology (hep-ph)Non-trivialGauge symmetries0103 physical sciencesAbelian group010306 general physicsAxionPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaCharge (physics)Gauge (firearms)16. Peace & justiceSymmetry (physics)Computer Science ApplicationsStandard Model (mathematical formulation)High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Homogeneous spaceStandard model
researchProduct

The see-saw portal at future Higgs Factories

2020

We consider an extension of the Standard Model with two right-handed singlet fermions with mass at the electroweak scale that induce neutrino masses, plus a generic new physics sector at a higher scale $\Lambda$. We focus on the effective operators of lowest dimension $d=5$, which induce new production and decay modes for the singlet fermions. We assess the sensitivity of future Higgs Factories, such as FCC-ee, CLIC-380, ILC and CEPC, to the coefficients of these operators for various center of mass energies. We show that future lepton colliders can test the cut-off of the theory up to $\Lambda \simeq 500 - 1000\;$TeV, surpassing the reach of future indirect measurements of the Higgs and $Z…

High Energy Physics - TheoryNuclear and High Energy PhysicsParticle physicsHiggs PhysicsPhysics beyond the Standard ModelFOS: Physical sciences7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentStandard ModelHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityNeutrino Physics010306 general physicsBeyond Standard Model; Higgs Physics; Neutrino PhysicsPhysics010308 nuclear & particles physicsComputer Science::Information RetrievalHigh Energy Physics::PhenomenologyFermionHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Beyond Standard ModelHiggs bosonlcsh:QC770-798High Energy Physics::ExperimentCenter of massElectroweak scaleNeutrinoLepton
researchProduct

Reloading the Axion in a 3-3-1 setup

2020

We generalize the idea of the axion to an extended electroweak gauge symmetry setup. We propose a minimal axion extension of the Singer-Valle-Schechter (SVS) theory, in which the standard model fits in $\mathrm{SU(3)_L\otimes U(1)_X}$, the number of families results from anomaly cancellation, and the Peccei-Quinn (PQ) solution to the strong-CP problem is implemented. Neutrino masses arise from a type-I Dirac seesaw mechanism, suppressed by the ratio of SVS and PQ scales, suggesting the existence of new physics at a moderate SVS scale. Novel features include an enhanced axion coupling to photons when compared to the DFSZ axion, as well as flavour-changing axion couplings to quarks.

High Energy Physics - TheoryNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelFOS: Physical sciencesStandard ModelHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics::TheoryAxionHigh Energy Physics - Phenomenology (hep-ph)Peccei-Quinn symmetryNeutrinosAxionGauge symmetryPhysicsElectroweak interactionHigh Energy Physics::Phenomenologylcsh:QC1-999High Energy Physics - PhenomenologySeesaw mechanismHigh Energy Physics - Theory (hep-th)Anomaly (physics)Neutrinolcsh:Physics
researchProduct

First Order Electroweak Phase Transition from (Non)Conformal Extensions of the Standard Model

2015

We analyse and compare the finite-temperature electroweak phase transition properties of classically (non)conformal extensions of the Standard Model. In the classically conformal scenarios the breaking of the electroweak symmetry is generated radiatively. The models feature new scalars coupled conformally to the Higgs sector as well as new fermions. We uncover the parameter space leading to a first order phase transition with(out) the Veltman conditions. We also discuss dark (matter) aspects of some of the models and compare with existing literature when appropriate. We observe that to accommodate both, a first order electroweak phase transition, and a phenomenologically viable dark matter …

High Energy Physics - TheoryNuclear and High Energy PhysicsPhase transitionParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard ModelDark matterFOS: Physical scienceshep-latTechnicolor7. Clean energy01 natural sciencesdark matterHiggs sectorStandard ModelHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Lattice0103 physical sciences010306 general physicsPhysicsta114010308 nuclear & particles physicshep-thHigh Energy Physics - Lattice (hep-lat)Electroweak interactionHigh Energy Physics::Phenomenologyhep-phSymmetry (physics)High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)astro-ph.COelectroweak phase transitionextensions of the standard modelAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct