0000000000704105

AUTHOR

Sonia El Hedri

showing 6 related works from this author

Perturbative unitarity constraints on the NMSSM Higgs Sector

2018

Abstract We place perturbative unitarity constraints on both the dimensionful and dimensionless parameters in the Next-to-Minimal Supersymmetric Standard Model (NMSSM) Higgs Sector. These constraints, plus the requirement that the singlino and/or Higgsino constitutes at least part of the observed dark matter relic abundance, generate upper bounds on the Higgs, neutralino and chargino mass spectrum. Requiring higher-order corrections to be no more than 41% of the tree-level value, we obtain an upper bound of 20 TeV for the heavy Higgses and 12 TeV for the charginos and neutralinos outside defined fine-tuned regions. If the corrections are no more than 20% of the tree-level value, the bounds …

PhysicsParticle physicsUnitarity010308 nuclear & particles physicsPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologyAstronomy and Astrophysics01 natural sciencesHiggs sectorCharginoSpace and Planetary Science0103 physical sciencesNeutralinoHiggs bosonHigh Energy Physics::ExperimentHiggsino010306 general physicsMinimal Supersymmetric Standard ModelPhysics of the Dark Universe
researchProduct

Perturbative unitarity constraints on gauge portals

2017

Abstract Dark matter that was once in thermal equilibrium with the Standard Model is generally prohibited from obtaining all of its mass from the electroweak phase transition. This implies a new scale of physics and mediator particles to facilitate dark matter annihilation. In this work, we focus on dark matter that annihilates through a generic gauge boson portal. We show how partial wave unitarity places upper bounds on the dark gauge boson, dark Higgs and dark matter masses. Outside of well-defined fine-tuned regions, we find an upper bound of 9 TeV for the dark matter mass when the dark Higgs and dark gauge bosons both facilitate the dark matter annihilations. In this scenario, the uppe…

PhysicsParticle physicsGauge boson010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyElectroweak interactionDark matterAstronomy and AstrophysicsElementary particleAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesStandard ModelSpace and Planetary Science0103 physical sciencesHiggs bosonGrand Unified Theory010306 general physicsBosonPhysics of the Dark Universe
researchProduct

Charged Higgs signals in tt¯H searches

2017

New scalars from an extended Higgs sector could have weak scale masses and still have escaped detection. In a type I two Higgs doublet model, for instance, even the charged Higgs can be lighter than the top quark. Because electroweak production of these scalars is modest, the greatest opportunity for their detection might come from rare top decays. For mass hierarchies of the type ${m}_{t}g{m}_{{H}^{+}}g{m}_{{A}^{0},{H}^{0}}$, the natural signal can arise from top quark pair production, followed by the decay chain $t\ensuremath{\rightarrow}b{H}^{+}$, ${H}^{+}\ensuremath{\rightarrow}{W}^{+(*)}{\ensuremath{\phi}}^{0}$, ${\ensuremath{\phi}}^{0}\ensuremath{\rightarrow}b\overline{b},{\ensuremath…

PhysicsParticle physicsTop quark010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyType (model theory)01 natural sciencesStandard ModelHiggs sectorTwo-Higgs-doublet modelPair production0103 physical sciencesHiggs bosonProduction (computer science)010306 general physicsPhysical Review D
researchProduct

Cornering Colored Coannihilation

2018

In thermal dark matter models, allowing the dark matter candidate to coannihilate with another particle can considerably loosen the relic density constraints on the dark matter mass. In particular, introducing a single strongly interacting coannihilation partner in a dark matter model can bring the upper bound on the dark sector energy scale from a few TeV up to about 10 TeV. While these energies are outside the LHC reach, a large part of the parameter space for such coannihilating models can be explored by future hadron colliders. In this context, it is essential to determine whether the current bounds on dark matter simplified models also hold in non-minimal scenarios. In this paper, we s…

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsDark matterHadronFOS: Physical sciencesContext (language use)Minimal modelsAstrophysics::Cosmology and Extragalactic AstrophysicsParameter space01 natural sciencesUpper and lower boundslaw.inventionHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)law0103 physical scienceslcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsColliderPhenomenological Models
researchProduct

Perturbative Unitarity Constraints on Charged/Colored Portals

2015

Dark matter that was once in thermal equilibrium with the Standard Model is generally prohibited from obtaining all of its mass from the electroweak or QCD phase transitions. This implies a new scale of physics and mediator particles needed to facilitate dark matter annihilations. In this work, we consider scenarios where thermal dark matter annihilates via scalar mediators that are colored and/or electrically charged. We show how partial wave unitarity places upper bounds on the masses and couplings on both the dark matter and mediators. To do this, we employ effective field theories with dark matter as well as three flavors of sleptons or squarks with minimum flavor violation. For Dirac (…

PhysicsParticle physicsUnitarity010308 nuclear & particles physicsPhysics beyond the Standard ModelDark matterElectroweak interactionHigh Energy Physics::PhenomenologyFOS: Physical sciencesAstronomy and Astrophysics01 natural sciencesUpper and lower boundsStandard ModelMAJORANAHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Space and Planetary Science0103 physical sciencesEffective field theoryHigh Energy Physics::Experiment010306 general physics
researchProduct

The coannihilation codex

2015

We present a general classification of simplified models that lead to dark matter (DM) coannihilation processes of the form DM + X $\rightarrow$ SM$_1$ + SM$_2$, where X is a coannihilation partner for the DM particle and SM$_1$, SM$_2$ are Standard Model fields. Our classification also encompasses regular DM pair annihilation scenarios if DM and X are identical. Each coannhilation scenario motivates the introduction of a mediating particle M that can either belong to the Standard Model or be a new field, whereby the resulting interactions between the dark sector and the Standard Model are realized as tree-level and dimension-four couplings. We construct a basis of coannihilation models, cl…

PhysicsParticle physicsNuclear and High Energy PhysicsAnnihilationLarge Hadron Collider010308 nuclear & particles physicsPhysicsElectroweak interactionDark matterFOS: Physical sciencesFermionQuantum number01 natural sciencesHigh Energy Physics - PhenomenologyMAJORANAHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesddc:530Hadronic CollidersSymmetry breaking010306 general physicsPhenomenological ModelsJournal of High Energy Physics
researchProduct