Search results for "Mathematical physics"

showing 10 items of 2687 documents

Flavour mixing transport theory and resonant leptogenesis

2021

We derive non-equilibrium quantum transport equations for flavour-mixing fermions. We develop the formalism mostly in the context of resonant leptogenesis with two mixing Majorana fermions and one lepton flavour, but our master equations are valid more generally in homogeneous and isotropic systems. We give a hierarchy of quantum kinetic equations, valid at different approximations, that can accommodate helicity and arbitrary mass differences. In the mass-degenerate limit the equations take the familiar form of density matrix equations. We also derive the semiclassical Boltzmann limit of our equations, including the CP-violating source, whose regulator corresponds to the flavour coherence d…

High Energy Physics - TheoryDensity matrixNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesSemiclassical physicsQC770-798hiukkasfysiikkakosmologia01 natural sciences114 Physical sciencesHigh Energy Physics - Phenomenology (hep-ph)Nuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesMaster equationThermal Field Theory010306 general physicscosmology of theories beyond the SMMixing (physics)Mathematical physicsPhysicsThermal quantum field theory010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFermionCosmology of Theories beyond the SMthermal field theory3. Good healthHigh Energy Physics - PhenomenologyMAJORANACP violationHigh Energy Physics - Theory (hep-th)LeptogenesisAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
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The Complete Solution of the Classical SL(2,ℝ/U(1) Gauged WZNW Field Theory

1998

We prove that any gauged WZNW model has a Lax pair representation, and give explicitly the general solution of the classical equations of motion of the SL(2,R)/U(1) theory. We calculate the symplectic structure of this solution by solving a differential equation of the Gelfand-Dikii type with initial state conditions at infinity, and transform the canonical physical fields non-locally onto canonical free fields. The results will, finally, be collected in a local B\"acklund transformation. These calculations prepare the theory for an exact canonical quantization.

High Energy Physics - TheoryDifferential equationCanonical quantizationFOS: Physical sciencesEquations of motionStatistical and Nonlinear PhysicsState (functional analysis)Type (model theory)Nonlinear Sciences::Exactly Solvable and Integrable SystemsHigh Energy Physics - Theory (hep-th)Lax pairField theory (psychology)Mathematical PhysicsSymplectic geometryMathematical physicsMathematicsCommunications in Mathematical Physics
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Differential equations for Feynman integrals beyond multiple polylogarithms

2017

Differential equations are a powerful tool to tackle Feynman integrals. In this talk we discuss recent progress, where the method of differential equations has been applied to Feynman integrals which are not expressible in terms of multiple polylogarithms.

High Energy Physics - TheoryDifferential equationFeynman integralRepresentation (systemics)FOS: Physical sciencesFeynman graphHigh Energy Physics - Phenomenologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Transformation (function)High Energy Physics - Theory (hep-th)ComputingMethodologies_SYMBOLICANDALGEBRAICMANIPULATIONsymbolsFeynman diagramMathematical physicsMathematicsProceedings of 13th International Symposium on Radiative Corrections (Applications of Quantum Field Theory to Phenomenology) — PoS(RADCOR2017)
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Electromagnetic Duality Anomaly in Curved Spacetimes

2016

The source-free Maxwell action is invariant under electric-magnetic duality rotations in arbitrary spacetimes. This leads to a conserved classical Noether charge. We show that this conservation law is broken at the quantum level in presence of a background classical gravitational field with a non-trivial Chern-Pontryagin invariant, in a parallel way to the chiral anomaly for massless Dirac fermions. Among the physical consequences, the net polarization of the quantum electromagnetic field is not conserved.

High Energy Physics - TheoryElectromagnetic fieldFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesakeGravitational field0103 physical sciences010306 general physicsQuantumMathematical PhysicsMathematical physicsPhysicsChiral anomalyQuantum PhysicsConservation law010308 nuclear & particles physicsMathematical Physics (math-ph)Invariant (physics)Classical mechanicsHigh Energy Physics - Theory (hep-th)Dirac fermionsymbolsNoether's theoremQuantum Physics (quant-ph)Physical Review Letters
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Reflexions on Mahler: Dessins, Modularity and Gauge Theories

2021

We provide a unified framework of Mahler measure, dessins d'enfants, and gauge theory. With certain physically motivated Newton polynomials from reflexive polygons, the Mahler measure and the dessin are in one-to-one correspondence. From the Mahler measure, one can construct a Hauptmodul for a congruence subgroup of the modular group, which contains the subgroup associated to the dessin. In brane tilings and quiver gauge theories, the modular Mahler flow gives a natural resolution of the inequivalence amongst the three different complex structures $\tau_{R,G,B}$. We also study how, in F-theory, 7-branes and their monodromies arise in the context of dessins. Moreover, we give a dictionary on…

High Energy Physics - TheoryF-theoryMathematics::Number Theory[PHYS.MPHY]Physics [physics]/Mathematical Physics [math-ph]FOS: Physical sciencesquivermembrane modelMathematics - Algebraic GeometryMathematics::K-Theory and HomologyFOS: MathematicsgroupNumber Theory (math.NT)modularstructureAlgebraic Geometry (math.AG)Mathematical PhysicsMathematics - Number Theory[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]monodromyresolutionMathematical Physics (math-ph)[PHYS.MPHY] Physics [physics]/Mathematical Physics [math-ph]High Energy Physics - Theory (hep-th)flowgauge field theory[PHYS.HTHE] Physics [physics]/High Energy Physics - Theory [hep-th]
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Hierarchies of geometric entanglement

2007

We introduce a class of generalized geometric measures of entanglement. For pure quantum states of $N$ elementary subsystems, they are defined as the distances from the sets of $K$-separable states ($K=2,...,N$). The entire set of generalized geometric measures provides a quantification and hierarchical ordering of the different bipartite and multipartite components of the global geometric entanglement, and allows to discriminate among the different contributions. The extended measures are applied to the study of entanglement in different classes of $N$-qubit pure states. These classes include $W$ and $GHZ$ states, and their symmetric superpositions; symmetric multi-magnon states; cluster s…

High Energy Physics - TheoryFOS: Physical sciencesMONOTONESQuantum entanglementSquashed entanglementMultipartite entanglementCombinatoricsSYSTEMSQuantum mechanicsMathematical PhysicsPhysicsQuantum PhysicsQUANTUM-MECHANICSCluster stateCURRENT SITUATIONQUANTUM-MECHANICS CURRENT SITUATION STATES SYSTEMS MONOTONESMathematical Physics (math-ph)Quantum PhysicsAtomic and Molecular Physics and OpticsCondensed Matter - Other Condensed MatterMultipartiteHigh Energy Physics - Theory (hep-th)STATESQubitBipartite graphW stateQuantum Physics (quant-ph)Other Condensed Matter (cond-mat.other)Physical Review A
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Massless positivity in graviton exchange

2021

We formulate Positivity Bounds for scattering amplitudes including exchange of massless particles. We generalize the standard construction through dispersion relations to include the presence of a branch cut along the real axis in the complex plane for the Maldestam variable $s$. In general, validity of these bounds require the cancellation of divergences in the forward limit of the amplitude, proportional to $t^{-1}$ and $\log(t)$. We show that this is possible in the case of gravitons if one assumes a Regge behavior of the amplitude at high energies below the Planck scale, as previously suggested in the literature, and that the concrete UV behaviour of the amplitude is uniquely determined…

High Energy Physics - TheoryField (physics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)hiukkasfysiikkakosmologia01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationeffective field theorycanonical quantum gravityDispersion relation0103 physical sciencessironta010306 general physicsquantum field theoryperturbation theoryMathematical physicsPhysics010308 nuclear & particles physicsGravitonFísicagravitaatioDark Energyalternative gravity theoriesBimetric Theoriesscattering amplitudesMassless particleScattering amplitudeAmplitudeHigh Energy Physics - Theory (hep-th)Complex planeGravitation
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Renormalisation group improvement in the stochastic formalism

2019

We investigate compatibility between the stochastic infrared (IR) resummation of light test fields on inflationary spacetimes and renormalisation group running of the ultra-violet (UV) physics. Using the Wilsonian approach, we derive improved stochastic Langevin and Fokker-Planck equations which consistently include the renormalisation group effects. With the exception of stationary solutions, these differ from the naive approach of simply replacing the classical potential in the standard stochastic equations with the renormalisation group improved potential. Using this new formalism, we exemplify the IR dynamics with the Yukawa theory during inflation, illustrating the differences between …

High Energy Physics - TheoryGAUGED NJL-MODELgr-qcHigh Energy Physics::LatticeFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstronomy & Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsHigh Energy Physics - Phenomenology (hep-ph)PROPAGATORFLATNESSHORIZON0201 Astronomical and Space Sciences0103 physical sciencesphysics of the early universeinflationINFLATIONARY UNIVERSE SCENARIOResummationMathematical physicsPhysicsScience & Technology010308 nuclear & particles physicsPhysicshep-thYukawa potentialhep-phAstronomy and AstrophysicsEXPANSIONNuclear & Particles Physicsquantum field theory on curved spaceFormalism (philosophy of mathematics)High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)particle physics - cosmology connectionINTERACTING SCALAR FIELDVACUUMPhysical Sciences0202 Atomic Molecular Nuclear Particle and Plasma PhysicsPHASE-TRANSITIONGENERATION
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Einstein, Planck and Vera Rubin: Relevant Encounters Between the Cosmological and the Quantum Worlds

2021

In Cosmology and in Fundamental Physics there is a crucial question like: where the elusive substance that we call Dark Matter is hidden in the Universe and what is it made of? that, even after 40 years from the Vera Rubin seminal discovery [1] does not have a proper answer. Actually, the more we have investigated, the more this issue has become strongly entangled with aspects that go beyond the established Quantum Physics, the Standard Model of Elementary particles and the General Relativity and related to processes like the Inflation, the accelerated expansion of the Universe and High Energy Phenomena around compact objects. Even Quantum Gravity and very exotic Dark Matter particle candid…

High Energy Physics - TheoryGeneral Physics and AstronomyNature of dark matter01 natural sciencesGeneral Relativity and Quantum CosmologyCosmologyClassical vs quantum cosmologyHigh Energy Physics - Phenomenology (hep-ph)010303 astronomy & astrophysicsQuantumMathematical PhysicsQuantum gravity and cosmologyPhysicsModification of general relativityChaplygin Gaslcsh:QC1-999CosmologyHigh Energy Physics - PhenomenologyExpansion of the UniversesymbolsGeneral RelativityGeneral relativityMaterials Science (miscellaneous)BiophysicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Metric expansion of spacesymbols.namesakeTheory of relativitySettore FIS/05 - Astronomia e Astrofisica0103 physical sciencesDark matterddc:530Cosmological ModelsPhysical and Theoretical ChemistryPlanckEinsteindark matter; galaxies; nature of dark matter; beyond standard model; modification of general relativity; quantum gravity and cosmology; expansion of the Universe010308 nuclear & particles physicsFísicaGalaxiesAstrophysics - Astrophysics of GalaxiesCosmosEpistemologyHigh Energy Physics - Theory (hep-th)quantum gravityAstrophysics of Galaxies (astro-ph.GA)Quantum gravityBeyond standard modellcsh:Physics
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k-Leibniz algebras from lower order ones: from Lie triple to Lie l-ple systems

2013

Two types of higher order Lie l-ple systems are introduced in this paper. They are defined by brackets with l > 3 arguments satisfying certain conditions, and generalize the well-known Lie triple systems. One of the generalizations uses a construction that allows us to associate a (2n - 3)-Leibniz algebra pound with a metric n-Leibniz algebra () pound over tilde by using a 2(n - 1)-linear Kasymov trace form for () pound over tilde. Some specific types of k-Leibniz algebras, relevant in the construction, are introduced as well. Both higher order Lie l-ple generalizations reduce to the standard Lie triple systems for l = 3.

High Energy Physics - TheoryGeneralized poisson structuresPure mathematicsTrace (linear algebra)SuperalgebrasEquationTriple systemSupertriple systemsOrder (ring theory)FOS: Physical sciencesStatistical and Nonlinear PhysicsLower orderMathematics - Rings and AlgebrasMathematical Physics (math-ph)Nambu mechanicsHigh Energy Physics - Theory (hep-th)Rings and Algebras (math.RA)Mathematics - Quantum AlgebraFOS: MathematicsQuantum Algebra (math.QA)Algebra over a fieldMathematical PhysicsMathematicsBranes
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