Search results for "Lorentz"

showing 10 items of 187 documents

Kinetic power of quasars and statistical excess of MOJAVE superluminal motions

2012

The MOJAVE survey contains 101 quasars with a total of 354 observed radio components that are different from the radio cores, among which 95% move with apparent projected superluminal velocities with respect to the core, and 45% have projected velocities larger than 10c (with a maximum velocity 60c). Doppler boosting effects are analyzed to determine the statistics of the superluminal motions. We integrate over all possible values of the Lorentz factor the values of the kinetic energy corresponding to each component. The calculation of the mass in the ejection is carried out by assuming the minimum energy state. This kinetic energy is multiplied by the frequency at which the portions of the…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)Cosmology and Nongalactic Astrophysics (astro-ph.CO)Superluminal motionLine-of-sightAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsQuasarAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsKinetic energysymbols.namesakeLorentz factorSpace and Planetary ScienceEddington luminositysymbolsAstrophysics - High Energy Astrophysical PhenomenaDoppler effectAstrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic AstrophysicsAstronomy & Astrophysics
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Derivation of the physical parameters of the jet in S5 0836+710 from stability analysis

2019

A number of extragalactic jets show periodic structures at different scales that can be associated with growing instabilities. The wavelengths of the developing instability modes and their ratios depend on the flow parameters, so the study of those structures can shed light on jet physics at the scales involved. In this work, we use the fits to the jet ridgeline obtained from different observations of S5 B0836$+$710 and apply stability analysis of relativistic, sheared flows to derive an estimate of the physical parameters of the jet. Based on the assumption that the observed structures are generated by growing Kelvin-Helmholtz (KH) instability modes, we have run numerical calculations of s…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)Internal energyAstrophysics::High Energy Astrophysical PhenomenaComputer Science::Information RetrievalFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsRadius01 natural sciencesInstabilityComputational physicsWavelengthsymbols.namesakeLorentz factorOrders of magnitude (time)Mach numberSpace and Planetary Science0103 physical sciencessymbolsHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical Phenomena010306 general physics010303 astronomy & astrophysicsAstronomy & Astrophysics
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Linear theory of the Rayleigh–Taylor instability at a discontinuous surface of a relativistic flow

2017

We address the linear stability of a discontinuous surface of a relativistic flow in the context of a jet that oscillates radially as it propagates. The restoring force of the oscillation is expected to drive a Rayleigh-Taylor instability (RTI) at the interface between the jet and its cocoon. We perform a linear analysis and numerical simulations of the growth of the RTI in the transverse plane to the jet flow with a uniform acceleration. In this system, an inertia force due to the uniform acceleration acts as the restoring force for the oscillation. We find that not only the difference in the inertia between the two fluids separated by the interface but also the pressure at the interface h…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)OscillationAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsMechanics01 natural sciencesInstabilityAccelerationLorentz factorsymbols.namesakeSpace and Planetary Science0103 physical sciencessymbolsRayleigh–Taylor instabilityRestoring forceAstrophysics - High Energy Astrophysical Phenomena010306 general physics010303 astronomy & astrophysicsLinear stabilityMonthly Notices of the Royal Astronomical Society
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Mass, zero mass and ... nophysics

2017

In this paper we demonstrate that massless particles cannot be considered as limiting case of massive particles. Instead, the usual symmetry structure based on semisimple groups like $U(1)$, $SU(2)$ and $SU(3)$ has to be replaced by less usual solvable groups like the minimal nonabelian group ${\rm sol}_2$. Starting from the proper orthochronous Lorentz group ${\rm Lor}_{1,3}$ we extend Wigner's little group by an additional generator, obtaining the maximal solvable or Borel subgroup ${\rm Bor}_{1,3}$ which is equivalent to the Kronecker sum of two copies of ${\rm sol}_2$, telling something about the helicity of particle and antiparticle states.

High Energy Physics - TheoryAntiparticle010308 nuclear & particles physicsGroup (mathematics)Generator (category theory)Applied MathematicsMathematics::Classical Analysis and ODEsFOS: Physical sciencesMathematical Physics (math-ph)01 natural sciencesHelicityLorentz groupGeneral Physics (physics.gen-ph)Physics - General PhysicsHigh Energy Physics - Theory (hep-th)Borel subgroupSolvable group0103 physical sciencesSymmetry (geometry)010306 general physicsMathematical PhysicsMathematical physicsMathematics
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Limits on neutrino Lorentz violation from multimessenger observations of TXS 0506+056

2019

The observation by the IceCube Collaboration of a high-energy ($E \gtrsim 200$ TeV) neutrino from the direction of the blazar TXS 0506+056 and the coincident observations of enhanced $\gamma$-ray emissions from the same object by MAGIC and other experiments can be used to set stringent constraints on Lorentz violation in the propagation of neutrinos that is linear in the neutrino energy: $\Delta v = - E/M_1$, where $\Delta v$ is the deviation from the velocity of light, and $M_1$ is an unknown high energy scale to be constrained by experiment. Allowing for a difference in neutrino and photon propagation times of $\sim 10$ days, we find that $M_1 \gtrsim 3 \times 10^{16}$ GeV. This improves …

High Energy Physics - TheoryNuclear and High Energy PhysicsHigh energyParticle physicsAstrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)Lorentz transformationgr-qcAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesComputer Science::Digital LibrariesGeneral Relativity and Quantum CosmologyIceCubesymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Coincident0103 physical sciences010306 general physicsBlazarParticle Physics - PhenomenologyHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEMultimessenger010308 nuclear & particles physicsGeneral Relativity and Cosmologyhep-thHigh Energy Physics::PhenomenologyLorentz violationGamma rayhep-phlcsh:QC1-999High Energy Physics - PhenomenologyPhoton propagationHigh Energy Physics - Theory (hep-th)Astrophysical neutrinosVelocity of lightsymbolsastro-ph.COHigh Energy Physics::ExperimentNeutrinoTXS 0506+056Astrophysics - High Energy Astrophysical PhenomenaParticle Physics - Theorylcsh:PhysicsBlazarsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysics Letters
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From multileg loops to trees (by-passing Feynman's Tree Theorem)

2008

We illustrate a duality relation between one-loop integrals and single-cut phase-space integrals. The duality relation is realised by a modification of the customary +i0 prescription of the Feynman propagators. The new prescription regularizing the propagators, which we write in a Lorentz covariant form, compensates for the absence of multiple-cut contributions that appear in the Feynman Tree Theorem. The duality relation can be extended to generic one-loop quantities, such as Green's functions, in any relativistic, local and unitary field theories.

High Energy Physics - TheoryNuclear and High Energy PhysicsLorentz transformationPropagatorFOS: Physical sciencesFísicaField (mathematics)Unitary stateAtomic and Molecular Physics and OpticsDuality relationsymbols.namesakeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)symbolsFeynman diagramCovariant transformationTree (set theory)MathematicsMathematical physics
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Wilson Loop Form Factors: A New Duality

2017

We find a new duality for form factors of lightlike Wilson loops in planar $\mathcal N=4$ super-Yang-Mills theory. The duality maps a form factor involving an $n$-sided lightlike polygonal super-Wilson loop together with $m$ external on-shell states, to the same type of object but with the edges of the Wilson loop and the external states swapping roles. This relation can essentially be seen graphically in Lorentz harmonic chiral (LHC) superspace where it is equivalent to planar graph duality. However there are some crucial subtleties with the cancellation of spurious poles due to the gauge fixing. They are resolved by finding the correct formulation of the Wilson loop and by careful analyti…

High Energy Physics - TheoryNuclear and High Energy PhysicsWilson loopgauge fixingHigh Energy Physics::LatticeFOS: Physical sciencesDuality (optimization)Type (model theory)Superspace01 natural sciencesSuperspacesspace: EuclideanGeneral Relativity and Quantum CosmologyWilson loopQuantum mechanics0103 physical sciencesMinkowski spacelcsh:Nuclear and particle physics. Atomic energy. RadioactivityMinkowskiScattering Amplitudes010306 general physicssuperspaceMathematical physicsGauge fixingPhysicsform factor010308 nuclear & particles physicsEuclidean space[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]hep-thAnalytic continuationWilsonLoop (topology)chiralCERN LHC CollHigh Energy Physics - Theory (hep-th)’t Hooft and Polyakov loopslcsh:QC770-798dualitysupersymmetryParticle Physics - TheoryDuality in Gauge Field TheoriesLorentz
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Acceleration radiation, transition probabilities, and trans-Planckian physics

2010

An important question in the derivation of the acceleration radiation, which also arises in Hawking's derivation of black hole radiance, is the need to invoke trans-Planckian physics in describing the creation of quanta. We point out that this issue can be further clarified by reconsidering the analysis in terms of particle detectors, transition probabilities and local two-point functions. By writing down separate expressions for the spontaneous-and induced-transition probabilities of a uniformly accelerated detector, we show that the bulk of the effect comes from the natural (non-trans-Planckian) scale of the problem, which largely diminishes the importance of the trans-Planckian sector. T…

High Energy Physics - TheoryPhysicsAstrofísicaPhysics::General Physics010308 nuclear & particles physicsGeneral Physics and AstronomyFOS: Physical sciencesAcceleration (differential geometry)Scale (descriptive set theory)General Relativity and Quantum Cosmology (gr-qc)RadiationLorentz covariance01 natural sciencesGeneral Relativity and Quantum CosmologyPartícules (Física nuclear)Black holeTheoretical physicsHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyHawkingHigh Energy Physics - Theory (hep-th)0103 physical sciencesRadianceQuantum field theory010306 general physics
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Evolution of mixed particles interacting with classical sources

2006

We study the systems of scalar and spinor particles with mixing emitted by external classical sources. The particles wave functions exactly accounting for external sources are obtained directly from the Lorentz invariant wave equations in (3+1)-dimensional space-time. Then we discuss sources which are localized in space and emit harmonic radiation. We obtain that the considered scalar and spinor fields can be converted from one type to another due to the presence of the vacuum mixing. This phenomenon is shown to be analogous to neutrino flavor oscillations in vacuum since the calculated transition and survival probabilities coincide with the corresponding expressions for neutrino oscillatio…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsAntiparticleParticle physicsSpinor010308 nuclear & particles physicsScalar (physics)FOS: Physical sciencesLorentz covariance01 natural sciencesAtomic and Molecular Physics and OpticsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Quantum electrodynamics0103 physical sciencesNeutrino010306 general physicsWave functionNeutrino oscillationMixing (physics)Physics of Atomic Nuclei
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Space-Time Foam may Violate the Principle of Equivalence

2003

The interactions of different particle species with the foamy space-time fluctuations expected in quantum gravity theories may not be universal, in which case different types of energetic particles may violate Lorentz invariance by varying amounts, violating the equivalence principle. We illustrate this possibility in two different models of space-time foam based on D-particle fluctuations in either flat Minkowski space or a stack of intersecting D-branes. Both models suggest that Lorentz invariance could be violated for energetic particles that do not carry conserved charges, such as photons, whereas charged particles such electrons would propagate in a Lorentz-inavariant way. The D-brane …

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsGeneral Relativity and CosmologySpace timeAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsElectronGeneral Relativity and Quantum Cosmology (gr-qc)Lorentz covarianceAstrophysicsGeneral Relativity and Quantum CosmologyAtomic and Molecular Physics and OpticsCharged particleGluonHigh Energy Physics - PhenomenologyTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Minkowski spaceQuantum gravityPhenomenology (particle physics)
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