Search results for "amplitud"

showing 10 items of 1171 documents

Testing Rate Dependent corrections on timing mode EPIC-pn spectra of the accreting Neutron Star GX 13+1

2014

When the EPIC-pn instrument on board XMM-Newton is operated in Timing mode, high count rates (>100 cts/s) of bright sources may affect the calibration of the energy scale, resulting in a modification of the real spectral shape. The corrections related to this effect are then strongly important in the study of the spectral properties. Tests of these calibrations are more suitable in sources which spectra are characterised by a large number of discrete features. Therefore, in this work, we carried out a spectral analysis of the accreting Neutron Star GX 13+1, which is a dipping source with several narrow absorption lines and a broad emission line in its spectrum. We tested two different co…

High Energy Astrophysical Phenomena (astro-ph.HE)Physicsaccretion accretion discs line: identification stars: neutron X-rays: binaries X-rays: galaxies X-rays: individual: (GX 13+1)Spectral shape analysisAccretion (meteorology)Absorption spectroscopyAstrophysics::High Energy Astrophysical PhenomenaContinuum (design consultancy)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics - Astrophysics of GalaxiesSpectral lineNeutron starAmplitudeidentification stars: neutron X-rays: binaries X-rays: galaxies X-rays: individual: (GX 13+1) [accretion accretion discs line]Settore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Emission spectrumAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)
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To d , or not to d : recent developments and comparisons of regularization schemes

2017

We give an introduction to several regularization schemes that deal with ultraviolet and infrared singularities appearing in higher-order computations in quantum field theories. Comparing the computation of simple quantities in the various schemes, we point out similarities and differences between them.

High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Physics and Astronomy (miscellaneous)FOS: Physical sciencesRenormalization regularization scattering amplitudesEngineering (miscellaneous); Physics and Astronomy (miscellaneous)Perturbative quantum filed theory high energy physicsEngineering (miscellaneous)
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Analytic Form of the Two-Loop Planar Five-Gluon All-Plus-Helicity Amplitude in QCD

2015

Virtual two-loop corrections to scattering amplitudes are a key ingredient to precision physics at collider experiments. We compute the full set of planar master integrals relevant to five-point functions in massless QCD, and use these to derive an analytical expression for the two-loop five-gluon all-plus-helicity amplitude. After subtracting terms that are related to the universal infrared and ultraviolet pole structure, we obtain a remarkably simple and compact finite remainder function, consisting only of dilogarithms.

High Energy Physics - Theory530 PhysicsFOS: Physical sciencesGeneral Physics and Astronomy10192 Physics Institute01 natural scienceslaw.inventionHigh Energy Physics - Phenomenology (hep-ph)law0103 physical sciences010306 general physicsColliderMathematical physicsPhysicsQuantum chromodynamics010308 nuclear & particles physicsHelicity3100 General Physics and AstronomyGluonScattering amplitudeLoop (topology)Massless particleHigh Energy Physics - PhenomenologyAmplitudeHigh Energy Physics - Theory (hep-th)Quantum electrodynamicsPhysical Review Letters
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Matter Dependence of the Four-Loop Cusp Anomalous Dimension

2019

We compute analytically the matter-dependent contributions to the quartic Casimir term of the four-loop light-like cusp anomalous dimension in QCD, with $n_f$ fermion and $n_s$ scalar flavours. The result is extracted from the double pole of a scalar form factor. We adopt a new strategy for the choice of master integrals with simple analytic and infrared properties, which significantly simplifies our calculation. To this end we first identify a set of integrals whose integrands have a dlog form, and are hence expected to have uniform transcendental weight. We then perform a systematic analysis of the soft and collinear regions of loop integration and build linear combinations of integrals w…

High Energy Physics - Theory530 PhysicsHigh Energy Physics::LatticeScalar (mathematics)FOS: Physical sciencesGeneral Physics and Astronomy10192 Physics Institute01 natural sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Feynman diagrams Form factors Perturbation theory Perturbative QCD Quantum field theory Scattering amplitudes Supersymmetric field theoriesQuartic function0103 physical sciencesFeynman diagramQuantum field theory010306 general physicsLinear combinationMathematical physicsQuantum chromodynamicsPhysics010308 nuclear & particles physicsPropagatorPerturbative QCD3100 General Physics and AstronomyHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)symbolsPhysical Review Letters
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Enhanced local-type inflationary trispectrum from a non-vacuum initial state

2011

We compute the primordial trispectrum for curvature perturbations produced during cosmic inflation in models with standard kinetic terms, when the initial quantum state is not necessarily the vacuum state. The presence of initial perturbations enhances the trispectrum amplitude for configuration in which one of the momenta, say $k_3$, is much smaller than the others, $k_3 \ll k_{1,2,4}$. For those squeezed configurations the trispectrum acquires the so-called local form, with a scale dependent amplitude that can get values of order $ \epsilon ({k_1}/{k_3})^2$. This amplitude can be larger than the prediction of the so-called Maldacena consistency relation by a factor $10^6$, and can reach t…

High Energy Physics - TheoryAstrofísicaGravitacióCosmology and Nongalactic Astrophysics (astro-ph.CO)Vacuum stateFOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsCurvatureKinetic energy01 natural sciencesGeneral Relativity and Quantum CosmologyQuantum state0103 physical sciencesSensitivity (control systems)010306 general physicsMathematical physicsPhysicsCosmologia010308 nuclear & particles physicsOrder (ring theory)Astronomy and AstrophysicsAmplitudeHigh Energy Physics - Theory (hep-th)TrispectrumAstrophysics - Cosmology and Nongalactic Astrophysics
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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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Space-like (vs. time-like) collinear limits in QCD: Is factorization violated?

2012

We consider the singular behaviour of QCD scattering amplitudes in kinematical configurations where two or more momenta of the external partons become collinear. At the tree level, this behaviour is known to be controlled by factorization formulae in which the singular collinear factor is universal (process independent). We show that this strict (process-independent) factorization is not valid at one-loop and higher-loop orders in the case of the collinear limit in space-like regions (e.g., collinear radiation from initial-state partons). We introduce a generalized version of all-order collinear factorization, in which the space-like singular factors retain some dependence on the momentum a…

High Energy Physics - TheoryNLO COMPUTATIONSNuclear and High Energy PhysicsHADRONIC COLLIDERSCiencias FísicasFOS: Physical sciencesPartonSpace (mathematics)01 natural sciences//purl.org/becyt/ford/1 [https]MomentumHigh Energy Physics - Phenomenology (hep-ph)Factorization0103 physical sciences010306 general physicsMathematical physicsQuantum chromodynamicsPhysics010308 nuclear & particles physicsFísicaCharge (physics)//purl.org/becyt/ford/1.3 [https]Scattering amplitudeAstronomíaHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Gravitational singularityCIENCIAS NATURALES Y EXACTAS
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Double collinear splitting amplitudes at next-to-leading order

2013

We compute the next-to-leading order (NLO) QCD corrections to the $1 \to 2$ splitting amplitudes in different dimensional regularization (DREG) schemes. Besides recovering previously known results, we explore new DREG schemes and analyze their consistency by comparing the divergent structure with the expected behavior predicted by Catani's formula. Through the introduction of scalar-gluons, we show the relation among splittings matrices computed using different schemes. Also, we extended this analysis to cover the double collinear limit of scattering amplitudes in the context of QCD+QED.

High Energy Physics - TheoryNLO COMPUTATIONSNuclear and High Energy PhysicsParticle physicsHADRONIC COLLIDERSCiencias FísicasFOS: Physical sciencesContext (language use)01 natural sciences//purl.org/becyt/ford/1 [https]Dimensional regularizationHigh Energy Physics - Phenomenology (hep-ph)Consistency (statistics)0103 physical sciencesLimit (mathematics)010306 general physicsMathematical physicsQuantum chromodynamicsPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísica//purl.org/becyt/ford/1.3 [https]Scattering amplitudeAstronomíaHigh Energy Physics - PhenomenologyAmplitudeHigh Energy Physics - Theory (hep-th)Cover (topology)CIENCIAS NATURALES Y EXACTASJournal of High Energy Physics
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Triple collinear splitting functions at NLO for scattering processes with photons

2014

We present splitting functions in the triple collinear limit at next-to-leading order. The computation was performed in the context of massless QCD+QED, considering only processes which include at least one photon. Through the comparison of the IR divergent structure of splitting amplitudes with the expected known behavior, we were able to check our results. Besides that we implemented some consistency checks based on symmetry arguments and cross-checked the results among them. Studying photon-started processes, we obtained very compact results.

High Energy Physics - TheoryNLO COMPUTATIONSNuclear and High Energy PhysicsParticle physicsPhotonCiencias FísicasComputationFOS: Physical sciencesContext (language use)01 natural sciences//purl.org/becyt/ford/1 [https]High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsQuantum chromodynamicsPhysics010308 nuclear & particles physicsScatteringFísica//purl.org/becyt/ford/1.3 [https]Symmetry (physics)AstronomíaMassless particleHigh Energy Physics - PhenomenologyAmplitudeHigh Energy Physics - Theory (hep-th)CIENCIAS NATURALES Y EXACTASJournal of High Energy Physics
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Analytic result for the nonplanar hexa-box integrals.

2019

In this paper, we analytically compute all master integrals for one of the two non-planar integral families for five-particle massless scattering at two loops. We first derive an integral basis of 73 integrals with constant leading singularities. We then construct the system of differential equations satisfied by them, and find that it is in canonical form. The solution space is in agreement with a recent conjecture for the non-planar pentagon alphabet. We fix the boundary constants of the differential equations by exploiting constraints from the absence of unphysical singularities. The solution of the differential equations in the Euclidean region is expressed in terms of iterated integral…

High Energy Physics - TheoryNuclear and High Energy Physics530 PhysicsDifferential equationFOS: Physical sciencesBoundary (topology)10192 Physics InstituteSpace (mathematics)01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Perturbative QCD0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityCanonical form3106 Nuclear and High Energy PhysicsScattering Amplitudes010306 general physicsMathematical physicsPhysicsBasis (linear algebra)010308 nuclear & particles physicsScattering amplitudeHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)lcsh:QC770-798Gravitational singularityConstant (mathematics)
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