0000000000186393

AUTHOR

Joseph D. Lykken

showing 9 related works from this author

Neutrinos that violate CPT, and the experiments that love them

2002

Recently we proposed a framework for explaining the observed evidence for neutrino oscillations without enlarging the neutrino sector, by introducing CPT violating Dirac masses for the neutrinos. In this paper we continue the exploration of the phenomenology of CPT violation in the neutrino sector. We show that our CPT violating model fits the existing SuperKamiokande data at least as well as the standard atmospheric neutrino oscillation models. We discuss the challenge of measuring CP violation in a neutrino sector that also violates CPT. We point out that the proposed off-axis extension of MINOS looks especially promising in this regard. Finally, we describe a method to compute CPT violat…

PhysicsNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)MINOSCP violationHigh Energy Physics::ExperimentNeutrinoAtmospheric neutrinoNeutrino oscillationPhenomenology (particle physics)Physics Letters B
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Colliders as a simultaneous probe of supersymmetric dark matter and Terascale cosmology

2006

Terascale supersymmetry has the potential to provide a natural explanation of the dominant dark matter component of the standard lambda-CDM cosmology. However once we impose the constraints on minimal supersymmetry parameters from current particle physics data, a satisfactory dark matter abundance is no longer prima facie natural. This Neutralino Tuning Problem could be a hint of nonstandard cosmology during and/or after the Terascale era. To quantify this possibility, we introduce an alternative cosmological benchmark based upon a simple model of quintessential inflation. This benchmark has no free parameters, so for a given supersymmetry model it allows an unambiguous prediction of the da…

PhysicsInflation (cosmology)Nuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderAstrophysics (astro-ph)Dark matterHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaSupersymmetryAstrophysics::Cosmology and Extragalactic AstrophysicsParameter spaceAstrophysicsCMB cold spotCosmologyHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutralino
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A model of CPT violation for neutrinos

2002

Any local relativistic quantum field theory of Dirac-Weyl fermions conserves CPT. Here we examine whether a simple nonlocal field theory can violate CPT. We construct a new relativistic field theory of fermions, which we call ``homeotic'', which is nonlocal but causal and Lorentz invariant. The free homeotic theory is in fact equivalent to free Dirac theory. We show that a homeotic theory with a suitable nonlocal four-fermion interaction is causal and as a result has a well-defined perturbative S-matrix. By coupling a right-handed homeotic fermion to a left-handed Dirac-Weyl fermion, we obtain a causal theory of CPT-violating neutrino oscillations.

PhysicsCondensed Matter::Quantum GasesNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::LatticeDirac (software)High Energy Physics::PhenomenologyFísicaFOS: Physical sciencesFermionLorentz covarianceCausal theory of referenceHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Field theory (psychology)High Energy Physics::ExperimentQuantum field theoryNeutrinoNeutrino oscillationMathematical physics
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Ultrahigh-energy neutrino flux as a probe of large extra dimensions

2007

A suppression in the spectrum of ultrahigh-energy (UHE, >= 10^{18} eV) neutrinos will be present in extra-dimensional scenarios, due to enhanced neutrino-antineutrino annihilation processes with the supernova relic neutrinos. In the n>4 scenario, being n the number of extra dimensions, neutrinos can not be responsible for the highest energy events observed in the UHE cosmic ray spectrum. A direct implication of these extra-dimensional interactions would be the absence of UHE neutrinos in ongoing and future neutrino telescopes.

High Energy Physics - TheoryAstrofísicaParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxCosmic rayAstrophysics01 natural sciences7. Clean energyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesUltrahigh energy010306 general physicsPhysicsAnnihilation010308 nuclear & particles physicsAstrophysics (astro-ph)High Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysics3. Good healthHigh Energy Physics - PhenomenologySupernovaExtra dimensionsHigh Energy Physics - Theory (hep-th)13. Climate actionLarge extra dimensionHigh Energy Physics::ExperimentNeutrinoJournal of Cosmology and Astroparticle Physics
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Neutrinos as the messengers of CPT violation

2001

CPT violation has the potential to explain all three existing neutrino anomalies without enlarging the neutrino sector. CPT violation in the Dirac mass terms of the three neutrino flavors preserves Lorentz invariance, but generates independent masses for neutrinos and antineutrinos. This specific signature is strongly motivated by braneworld scenarios with extra dimensions, where neutrinos are the natural messengers for Standard Model physics of CPT violation in the bulk. A simple model of maximal CPT violation is sufficient to explain the exisiting neutrino data quite neatly, while making dramatic predictions for the upcoming KamLAND and MiniBooNE experiments. Furthermore we obtain a promi…

PhysicsNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsDirac (video compression format)High Energy Physics::PhenomenologyFísicaFOS: Physical sciencesLorentz covarianceStandard ModelMiniBooNEBaryogenesisHigh Energy Physics - PhenomenologyExtra dimensionsHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics::ExperimentNeutrino
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Minimal noncanonical cosmologies

2006

We demonstrate how much it is possible to deviate from the standard cosmological paradigm of inflation-assisted LambdaCDM, keeping within current observational constraints, and without adding to or modifying any theoretical assumptions. We show that within a minimal framework there are many new possibilities, some of them wildly different from the standard picture. We present three illustrative examples of new models, described phenomenologically by a noncanonical scalar field coupled to radiation and matter. These models have interesting implications for inflation, quintessence, reheating, electroweak baryogenesis, and the relic densities of WIMPs and other exotics.

Inflation (cosmology)PhysicsNuclear and High Energy PhysicsElectroweak interactionAstrophysics (astro-ph)FOS: Physical sciencesFísicaAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsBaryogenesisTheoretical physicsGeneral Relativity and Quantum CosmologyScalar fieldQuintessence
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Adding pseudo-observables to the four-lepton experimentalist’s toolbox

2018

The "golden" channel, in which the newly-discovered Higgs boson decays to four leptons by means of intermediate vector bosons, is important for determining the properties of the Higgs boson and for searching for subtle new physics effects. Different approaches exist for parametrizing the relevant Higgs couplings in this channel; here we relate the use of pseudo-observables to methods based on specifying the most general amplitude or Lagrangian terms for the $HVV$ interactions. We also provide projections for sensitivity in this channel in several novel scenarios, illustrating the use of pseudo-observables, and analyze the role of kinematic distributions and (ratios of) rates in such $H\to4\…

Nuclear and High Energy PhysicsParticle physicsHiggs PhysicsPhysics beyond the Standard ModelFOS: Physical sciencesKinematicsQC770-79801 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Nuclear and particle physics. Atomic energy. Radioactivity0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivitySensitivity (control systems)010306 general physicsHiggs Physics ; Beyond Standard ModelParticle Physics - PhenomenologyPhysics010308 nuclear & particles physicsComputer Science::Information RetrievalHigh Energy Physics::PhenomenologyObservablehep-ph3. Good healthHigh Energy Physics - PhenomenologyAmplitudeBeyond Standard ModelHiggs bosonlcsh:QC770-798LeptonCommunication channelJournal of High Energy Physics
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Quintessence, inflation and baryogenesis from a single pseudo-Nambu-Goldstone boson

2007

15 pages, 3 figures.-- ISI Article Identifier: 000250759700079.-- ArXiv pre-print available at: http://arxiv.org/abs/0707.3999

Nuclear and High Energy PhysicsParticle physicsProton decayCosmic microwave backgroundGenerationFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicssymbols.namesakePlanckBosonPhysicsHigh Energy Physics::PhenomenologyAstrophysics (astro-ph)BaryogenesisFísicaCosmology of Theories beyond the SMWater Cherenkov DetectorBaryogenesisGoldstone bosonLeptogenesissymbolsDark energyHigh Energy Physics::ExperimentQuintessence
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Self-accelerating solutions of scalar-tensor gravity

2007

Scalar-tensor gravity is the simplest and best understood modification of general relativity, consisting of a real scalar field coupled directly to the Ricci scalar curvature. Models of this type have self-accelerating solutions. In an example inspired by string dilaton couplings, scalar-tensor gravity coupled to ordinary matter exhibits a de Sitter type expansion, even in the presence of a {\it negative} cosmological constant whose magnitude exceeds that of the matter density. This unusual behavior does not require phantoms, ghosts or other exotic sources. More generally, we show that any expansion history can be interpreted as arising partly or entirely from scalar-tensor gravity. To dist…

PhysicsAstrofísicaGeneral relativityAstrophysics (astro-ph)FOS: Physical sciencesFísicaAstronomy and AstrophysicsCosmological constantAstrophysicsAstrophysicsGravitationTheoretical physicsHigh Energy Physics - PhenomenologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)De Sitter universeDark energyDilatonScalar fieldQuintessence
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