Search results for "baryon number"

showing 10 items of 28 documents

Baryon Asymmetry Resulting from FCQPT in the Early Universe

2014

This Chapter does not follow the main line of the book that is the theory of HF compounds but illustrates how the ideas of FC may be applicable to describe a very dissimilar system. Namely, here we consider a novel mechanism for explaining the matter-antimatter asymmetry of the universe. We assume that the universe starts from completely symmetric state and then, as it cools down, it undergoes a quantum phase transition, which in turn causes an asymmetry between matter and anti-matter. As we shall see the quantum phase transition is represented by FCQPT. The mechanism does not require the baryon number violating interactions or \({\textit{CP}}\) violation at a microscopic level. The state F…

Quantum phase transitionPhysicsParticle physicsBaryon asymmetrymedia_common.quotation_subjectAntimatterQuantum critical pointSupersymmetryBaryon numberAsymmetryUniversemedia_common
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Baryon resonances in nuclei

2005

The field of baryon resonances in nuclei is reviewed. Theoretical developments and experimental evidence as well are discussed. Special emphasis is laid on electromagnetic processes for the two nucleon system. Some aspects of real isobars in nuclei are touched upon.

Nuclear physicsPhysicsBaryonField (physics)Nuclear TheoryIsobarForm factor (quantum field theory)Baryon numberNuclear ExperimentNucleonNuclear matter
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Bag models and hadron structure

2008

We review the fundamental ideas leading to the basic assumptions behind the bag model description of hadron structure and explore in some detail the so called MIT bag model. We discuss the relevance of chiral symmetry and incorporate it in a bag model scheme by adding a pion field. We show perturbative techniques of calculating gluonic and pionic effects. We discuss the consequences of the solitonic nature of the hedgehog solution of the pion field and introduce the skyrmion bag model. We end up by drawing some conclusions of our study and discussing recent developments in this area.

Chiral anomalyPhysicsModel descriptionParticle physicsPionField (physics)SkyrmionHigh Energy Physics::PhenomenologyNuclear TheoryStructure (category theory)Baryon numberChiral symmetry breaking
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The baryon number two system in the Chiral Soliton Model

2012

We study the interaction between two B = 1 states in a chiral soliton model where baryons are described as non-topological solitons. By using the hedgehog solution for the B = 1 states we construct three possible B = 2 configurations to analyze the role of the relative orientation of the hedgehog quills in the dynamics. The strong dependence of the intersoliton interaction on these relative orientations reveals that studies of dense hadronic matter using this model should take into account their implications.

PhysicsMatterNuclear TheoryHadronNuclear TheoryHigh Energy Physics::PhenomenologyFOS: Physical sciencesAtomic and Molecular Physics and OpticsChiral solitonBaryonOrientation (vector space)Nuclear Theory (nucl-th)Theoretical physicsFísica nuclearBaryon number
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Anomalous dynamics triggered by a non-convex equation of state in relativistic flows

2017

The non-monotonicity of the local speed of sound in dense matter at baryon number densities much higher than the nuclear saturation density ($n_0 \approx 0.16\,$fm$^{-3}$) suggests the possible existence of a non-convex thermodynamics which will lead to a non-convex dynamics. Here, we explore the rich and complex dynamics that an equation of state (EoS) with non-convex regions in the pressure-density plane may develop as a result of genuinely relativistic effects, without a classical counterpart. To this end, we have introduced a phenomenological EoS, whose parameters can be restricted heeding to causality and thermodynamic stability constraints. This EoS shall be regarded as a toy-model wi…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsEquation of state (cosmology)Plane (geometry)Nuclear TheoryFluid Dynamics (physics.flu-dyn)FOS: Physical sciencesAstronomy and AstrophysicsPhysics - Fluid DynamicsApprox01 natural sciencesCausality (physics)Complex dynamicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceSpeed of sound0103 physical sciencesBaryon numberAstrophysics - High Energy Astrophysical PhenomenaRelativistic quantum chemistry010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Mathematical physics
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A full picture of large lepton number asymmetries of the Universe

2017

A large lepton number asymmetry of (0.1−1) at present Universe might not only be allowed but also necessary for consistency among cosmological data. We show that, if a sizeable lepton number asymmetry were produced before the electroweak phase transition, the requirement for not producing too much baryon number asymmetry through sphalerons processes, forces the high scale lepton number asymmetry to be larger than about 03. Therefore a mild entropy release causing (10-100) suppression of pre-existing particle density should take place, when the background temperature of the Universe is around T = (10−2-102) GeV for a large but experimentally consistent asymmetry to be present today. We also …

PhysicsParticle physics010308 nuclear & particles physicsEntropy productionmedia_common.quotation_subjectHigh Energy Physics::PhenomenologyElectroweak interactionAstronomy and Astrophysics01 natural sciencesLepton numberAsymmetryUniverse0103 physical sciencesHigh Energy Physics::ExperimentBaryon number010303 astronomy & astrophysicsEntropy (arrow of time)Vacuum expectation valuemedia_commonJournal of Cosmology and Astroparticle Physics
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Topological structure of dense hadronic matter

2007

8 pages, 4 figures.-- ISI Article Identifier: 000244425500052.

PhysicsNuclear and High Energy PhysicsParticle physicsMesonMesonsHigh Energy Physics::PhenomenologyNuclear TheoryHadronStructure (category theory)FísicaHomogeneous spaceHigh Energy Physics::ExperimentSolitonBaryon numberVector mesonNuclear ExperimentGround stateSkyrmion matterSymmetries
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Diffusion processes involving multiple conserved charges: a first study from kinetic theory and implications to the fluid-dynamical modeling of heavy…

2020

The bulk nuclear matter produced in heavy ion collisions carries a multitude of conserved quantum numbers: electric charge, baryon number, and strangeness. Therefore, the diffusion processes associated to these conserved charges cannot occur independently and must be described in terms of a set of coupled diffusion equations. This physics is implemented by replacing the traditional diffusion coefficients for each conserved charge by a diffusion coefficient matrix, which quantifies the coupling between the conserved quantum numbers. The diagonal coefficients of this matrix are the usual charge diffusion coefficients, while the off-diagonal entries describe the diffusive coupling of the charg…

High Energy Physics - TheoryNuclear TheoryFOS: Physical sciencesPartonhiukkasfysiikka114 Physical sciences01 natural sciencesElectric chargeNuclear Theory (nucl-th)Matrix (mathematics)diffuusio (fysikaaliset ilmiöt)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesDiffusion (business)010306 general physicsCoefficient matrixPhysics010308 nuclear & particles physicsdiffusionCharge (physics)Quantum numberHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)transport phenomenaQuantum electrodynamicsBaryon numberydinfysiikkarelativistic heavy-ion collisions
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Baryogenesis and dark matter from B mesons

2019

We present a new mechanism of Baryogenesis and dark matter production in which both the dark matter relic abundance and the baryon asymmetry arise from neutral $B$ meson oscillations and subsequent decays. This set-up is testable at hadron colliders and $B$-factories. In the early Universe, decays of a long lived particle produce $B$ mesons and anti-mesons out of thermal equilibrium. These mesons/anti-mesons then undergo CP violating oscillations before quickly decaying into visible and dark sector particles. Dark matter will be charged under Baryon number so that the visible sector baryon asymmetry is produced without violating the total baryon number of the Universe. The produced baryon a…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)MesonProton decayDark matterHadronNuclear TheoryFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences7. Clean energyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Baryon asymmetry0103 physical sciences010306 general physicsNuclear ExperimentPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyBaryonBaryogenesisHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentBaryon numberAstrophysics - Cosmology and Nongalactic Astrophysics
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ΔL=3 processes: Proton decay and the LHC

2018

We discuss lepton number violation in three units. From an effective field theory point of view, ΔL=3 processes can only arise from dimension 9 or higher operators. These operators also violate baryon number, hence many of them will induce proton decay. Given the high dimensionality of these operators, in order to have a proton half-life in the observable range, the new physics associated to ΔL=3 processes should be at a scale as low as 1 TeV. This opens up the possibility of searching for such processes not only in proton decay experiments but also at the LHC. In this work we analyze the relevant d=9, 11, 13 operators which violate lepton number in three units. We then construct one simple…

PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsProton decayPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologyObservable01 natural sciencesLepton numberComputer Science::Digital Libraries0103 physical sciencesEffective field theoryHigh Energy Physics::ExperimentBaryon number010306 general physicsPhenomenology (particle physics)Physical Review
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