Search results for "oscillation"

showing 10 items of 1257 documents

Ultralight dark photon as a model for early universe dark matter

2019

Dark photon is a massive vector field which interacts only with the physical photon through the kinetic mixing. This coupling is assumed to be weak so that the dark photon becomes almost unobservable in processes with elementary particles, but can serve as a dark matter particle. We argue that in very early Universe ($z>3000$) this vector field may have the equation of state of radiation ($w=1/3$) but later behaves as cold dark matter ($w=0$). This may slightly change the expansion rate of the Universe at early time and reduce the value of the sound horizon of baryon acoustic oscillations (standard ruler). As a result, in this model the value of the Hubble constant appears to be larger than…

PhysicsParticle physicsCold dark matterCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsEquation of state (cosmology)Dark matterOrder (ring theory)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsCoupling (probability)01 natural sciencesDark photonsymbols.namesakeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencessymbolsBaryon acoustic oscillations010306 general physicsHubble's lawAstrophysics - Cosmology and Nongalactic Astrophysics
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Constraints on electromagnetic form factors of sub-GeV dark matter from the cosmic microwave background anisotropy

2021

We consider dark matter which have non-zero electromagnetic form factors like electric/magnetic dipole moments and anapole moment for fermionic dark matter and Rayleigh form factor for scalar dark matter. We consider dark matter mass $m_\chi > \cal{ O}({\rm MeV})$ and put constraints on their mass and electromagnetic couplings from CMB and LSS observations. Fermionic dark matter with non-zero electromagnetic form factors can annihilate to $e^+ e^-$ and scalar dark matter can annihilate to $2\gamma$ at the time of recombination and distort the CMB. We analyze dark matter with multipole moments with Planck and BAO observations. We find upper bounds on anapole moment $g_{A}<7.163\times 10^{3} …

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Magnetic momentScalar (mathematics)Dark matterForm factor (quantum field theory)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsHigh Energy Physics - PhenomenologyElectric dipole momentHigh Energy Physics - Phenomenology (hep-ph)Baryon acoustic oscillationsMultipole expansionMagnetic dipoleAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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Resurrection of large lepton number asymmetries from neutrino flavor oscillations

2016

We numerically solve the evolution equations of neutrino three-flavor density matrices, and show that, even if neutrino oscillations mix neutrino flavors, large lepton number asymmetries are still allowed in certain limits by Big Bang Nucleosynthesis (BBN).

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and Detectors010308 nuclear & particles physicsHigh Energy Physics::LatticeAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical sciences01 natural sciencesLepton numberNuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesis0103 physical sciencesMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationFlavorAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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Zooming in on neutrino oscillations with DUNE

2018

We examine the capabilities of the DUNE experiment as a probe of the neutrino mixing paradigm. Taking the current status of neutrino oscillations and the design specifications of DUNE, we determine the experiment's potential to probe the structure of neutrino mixing and CP violation. We focus on the poorly determined parameters $\theta_{23}$ and $\delta_{CP}$ and consider both two and seven years of run. We take various benchmarks as our true values, such as the current preferred values of $\theta_{23}$ and $\delta_{CP}$, as well as several theory-motivated choices. We determine quantitatively DUNE's potential to perform a precision measurement of $\theta_{23}$, as well as to test the CP vi…

PhysicsParticle physicsCurrent (mathematics)010308 nuclear & particles physicsFOS: Physical sciences01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNeutrino010306 general physicsNeutrino oscillationMixing (physics)
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X-ray photons from late-decaying majoron dark matter

2008

An attractive way to generate neutrino masses as required to account for current neutrino oscillation data involves the spontaneous breaking of lepton number. The resulting majoron may pick up a mass due to gravity. If its mass lies in the kilovolt scale, the majoron can play the role of late-decaying Dark Matter (LDDM), decaying mainly to neutrinos. In general the majoron has also a sub-dominant decay to two photons leading to a mono-energetic emission line which can be used as a test of the LDDM scenario. We compare expected photon emission rates with observations in order to obtain model independent restrictions on the relevant parameters. We also illustrate the resulting sensitivities w…

PhysicsParticle physicsDark matterAstrophysics (astro-ph)High Energy Physics::PhenomenologyCosmic background radiationFOS: Physical sciencesFísicaAstronomy and AstrophysicsAstrophysicsLepton numberHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryHiggs bosonHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationMajoron
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A Monochromatic Neutrino Beam to Obtain U(e3) and the CP Phase

2007

The goal for future neutrino facilities is the determination of the [Ue3] mixing and CP violation in neutrino oscillations. This will require precision experiments with a very intense neutrino source. The future experiments such as T2K, NOVA and Double CHOOZ will measure the [Ue3] mixing. In order to explore CP violation, we present a novel method to create a monochromatic neutrino beam based on the recent discovery of nuclei that decay fast through electron capture in a superallowed Gamow-Teller transition. The boost of such radioactive ions will generate an intense monochromatic directional neutrino beam when decaying at high energy in a storage ring with long straight sections. We show t…

PhysicsParticle physicsElectron capturePhysics beyond the Standard ModelHigh Energy Physics::PhenomenologyFísicaCHOOZSolar neutrino problemNuclear physicsCP violationMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationAIP Conference Proceedings
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Neutrino Spin Oscillations in External Gravitational Fields

2007

PhysicsParticle physicsGravitational fieldMeasurements of neutrino speedNeutrinoNeutrino oscillationSpin-½
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Predictive flavor symmetries of the neutrino mass matrix.

2007

Here we propose an $A_4$ flavour symmetry model which implies a lower bound on the neutrinoless double beta decay rate, corresponding to an effective mass parameter $M_{ee} \gsim 0.03$ eV, and a direct correlation between the expected magnitude of CP violation in neutrino oscillations and the value of $\sin^2\theta_{13}$, as well as a nearly maximal CP phase $\delta$.

PhysicsParticle physicsHigh Energy Physics::PhenomenologyGeneral Physics and AstronomyFOS: Physical sciencesFísicaMass matrixUpper and lower boundsMonod-Wyman-Changeux modelNuclear physicsHigh Energy Physics - PhenomenologyEffective mass (solid-state physics)High Energy Physics - Phenomenology (hep-ph)Double beta decayCP violationHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationPhysical review letters
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Disentangling genuine from matter-induced CP violation in neutrino oscillations

2018

We prove that, in any flavor transition, neutrino oscillation CP violating asymmetries in matter have two disentangled components: (a) a CPT-odd T-invariant term, non-vanishing iff there are interactions with matter; (b) a T-odd CPT-invariant term, non-vanishing iff there is genuine CP violation. As function of the baseline, these two terms are distinct L-even and L-odd observables, respectively. In the experimental region of terrestrial accelerator neutrinos, we calculate their approximate expressions from which we prove that, at medium baselines, the CPT-odd component is small and nearly $\delta$-independent, so it can be subtracted from the experimental CP asymmetry as a theoretical back…

PhysicsParticle physicsHistory010308 nuclear & particles physicsDirect evidencemedia_common.quotation_subjectHigh Energy Physics::PhenomenologyGeneral Physics and AstronomyFOS: Physical sciencesObservable01 natural sciencesAsymmetryComputer Science::Digital LibrariesComputer Science ApplicationsEducationHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesCP violationHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationLeptonmedia_common
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Azimuthally Differential Pion Femtoscopy in Pb-Pb Collisions at sNN=2.76  TeV

2017

We present the first azimuthally differential measurements of the pion source size relative to the second harmonic event plane in Pb-Pb collisions at a center-of-mass energy per nucleon-nucleon pair of √sNN = 2.76 TeV. The measurements have been performed in the centrality range 0%-50% and for pion pair transverse momenta 0.2 < kT < 0.7 GeV/c. We find that the Rside and Rout radii, which characterize the pion source size in the directions perpendicular and parallel to the pion transverse momentum, oscillate out of phase, similar to what was observed at the Relativistic Heavy Ion Collider. The final-state source eccentricity, estimated via Rside oscillations, is found to be significantly sma…

PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsOscillationmedia_common.quotation_subjectNuclear TheoryHadronGeneral Physics and Astronomy01 natural sciencesNuclear physicsTransverse planePion0103 physical sciencesRapidityEccentricity (behavior)Nuclear Experiment010306 general physicsRelativistic Heavy Ion Collidermedia_commonPhysical Review Letters
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