Search results for " singularity"

showing 10 items of 203 documents

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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Conifold Transitions and Mirror Symmetry for Calabi-Yau Complete Intersections in Grassmannians

1997

In this paper we show that conifold transitions between Calabi-Yau 3-folds can be used for the construction of mirror manifolds and for the computation of the instanton numbers of rational curves on complete intersection Calabi-Yau 3-folds in Grassmannians. Using a natural degeneration of Grassmannians $G(k,n)$ to some Gorenstein toric Fano varieties $P(k,n)$ with conifolds singularities which was recently described by Sturmfels, we suggest an explicit mirror construction for Calabi-Yau complete intersections $X \subset G(k,n)$ of arbitrary dimension. Our mirror construction is consistent with the formula for the Lax operator conjectured by Eguchi, Hori and Xiong for gravitational quantum c…

High Energy Physics - TheoryNuclear and High Energy PhysicsInstantonPure mathematicsConifoldComplete intersectionFOS: Physical sciencesFano planeMathematics - Algebraic GeometryMathematics::Algebraic GeometryHigh Energy Physics - Theory (hep-th)FOS: MathematicsCalabi–Yau manifoldGravitational singularityMathematics::Differential GeometryMirror symmetryAlgebraic Geometry (math.AG)Mathematics::Symplectic GeometryQuantum cohomologyMathematics
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Mathematical properties of nested residues and their application to multi-loop scattering amplitudes

2021

Journal of high energy physics 02(2), 112 (2021). doi:10.1007/JHEP02(2021)112

High Energy Physics - TheoryNuclear and High Energy PhysicscausalityComputationFeynman graphpoleFOS: Physical sciencesDuality (optimization)Mathematical proof01 natural sciences530Theoretical physicsHigh Energy Physics - Phenomenology (hep-ph)NLO Computations0103 physical sciencesddc:530lcsh:Nuclear and particle physics. Atomic energy. Radioactivitystructure010306 general physicsRepresentation (mathematics)Mathematical PhysicsPhysics010308 nuclear & particles physicsscattering amplitudeMathematical Physics (math-ph)QCD PhenomenologysingularityScattering amplitudeHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Iterated functionlcsh:QC770-798dualityGravitational singularityMathematical structure
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Cosmon Lumps and Horizonless Black Holes

2008

We investigate non-linear, spherically symmetric solutions to the coupled system of a quintessence field and Einstein gravity. In the presence of a scalar potential, we find regular solutions that to an outside observer very closely resemble Schwarzschild black holes. However, these cosmon lumps have neither a horizon nor a central singularity. A stability analysis reveals that our static solutions are dynamically unstable. It remains an open question whether analogous stable solutions exist.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsAstrophysics (astro-ph)FOS: Physical sciencesScalar potentialAstrophysicssymbols.namesakeGeneral Relativity and Quantum CosmologyClassical mechanicsSingularityHigh Energy Physics - Theory (hep-th)symbolsSchwarzschild metricGravitational singularityCircular symmetryEinsteinSchwarzschild radiusQuintessence
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Semiclassical zero-temperature corrections to Schwarzschild spacetime and holography

2005

Motivated by the quest for black holes in AdS braneworlds, and in particular by the holographic conjecture relating 5D classical bulk solutions with 4D quantum corrected ones, we numerically solve the semiclassical Einstein equations (backreaction equations) with matter fields in the (zero temperature) Boulware vacuum state. In the absence of an exact analytical expression for in four dimensions we work within the s-wave approximation. Our results show that the quantum corrected solution is very similar to Schwarzschild till very close to the horizon, but then a bouncing surface for the radial function appears which prevents the formation of an event horizon. We also analyze the behavior of…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsCosmologiaQuantum field theory in curved spacetimeEvent horizonWhite holeKerr metricFOS: Physical sciencesNaked singularityGeneral Relativity and Quantum Cosmology (gr-qc)Partícules (Física nuclear)General Relativity and Quantum CosmologyBlack holeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum mechanicsDeriving the Schwarzschild solutionSchwarzschild radiusPhysical Review D
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Quantum gravity effects near the null black hole singularity

1998

The structure of the Cauchy Horizon singularity of a black hole formed in a generic collapse is studied by means of a renormalization group equation for quantum gravity. It is shown that during the early evolution of the Cauchy Horizon the increase of the mass function is damped when quantum fluctuations of the metric are taken into account.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsEvent horizonCauchy horizonFOS: Physical sciencesNaked singularityGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyBlack holeGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Gravitational singularityBlack hole thermodynamicsRing singularityBlack hole complementarityPhysical Review D
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Causal representation of multi-loop Feynman integrands within the loop-tree duality

2021

The numerical evaluation of multi-loop scattering amplitudes in the Feynman representation usually requires to deal with both physical (causal) and unphysical (non-causal) singularities. The loop-tree duality (LTD) offers a powerful framework to easily characterise and distinguish these two types of singularities, and then simplify analytically the underling expressions. In this paper, we work explicitly on the dual representation of multi-loop Feynman integrals generated from three parent topologies, which we refer to as Maximal, Next-to-Maximal and Next-to-Next-to-Maximal loop topologies. In particular, we aim at expressing these dual contributions, independently of the number of loops an…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsDuality (mathematics)PropagatorDual representation01 natural sciencesAlgebraHigh Energy Physics - Phenomenologysymbols.namesakeIntegerSimple (abstract algebra)Perturbative QCD0103 physical sciencessymbolslcsh:QC770-798Feynman diagramlcsh:Nuclear and particle physics. Atomic energy. RadioactivityGravitational singularityScattering Amplitudes010306 general physicsRepresentation (mathematics)Duality in Gauge Field TheoriesJournal of High Energy Physics
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Infrared singularities of QCD amplitudes with massive partons

2009

A formula for the two-loop infrared singularities of dimensionally regularized QCD scattering amplitudes with an arbitrary number of massive and massless legs is derived. The singularities are obtained from the solution of a renormalization-group equation, and factorization constraints on the relevant anomalous-dimension matrix are analyzed. The simplicity of the structure of the matrix relevant for massless partons does not carry over to the case with massive legs, where starting at two-loop order new color and momentum structures arise, which are not of the color-dipole form. The resulting two-loop three-parton correlations can be expressed in terms of two functions, for which some genera…

High Energy Physics - TheoryPhysicsQuantum chromodynamicsNuclear and High Energy PhysicsParticle physics530 PhysicsFOS: Physical sciencesPartonSymmetry (physics)Scattering amplitudeMassless particleHigh Energy Physics - PhenomenologyMatrix (mathematics)High Energy Physics - Phenomenology (hep-ph)FactorizationHigh Energy Physics - Theory (hep-th)Gravitational singularityMathematical physics
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Quantum Backreaction on Three-Dimensional Black Holes and Naked Singularities

2016

We analytically investigate backreaction by a quantum scalar field on two rotating Ba\~nados-Teitelboim-Zanelli (BTZ) geometries: that of a black hole and that of a naked singularity. In the former case, we explore the quantum effects on various regions of relevance for a rotating black hole space-time. We find that the quantum effects lead to a growth of both the event horizon and the radius of the ergosphere, and to a reduction of the angular velocity, compared to the unperturbed values. Furthermore, they give rise to the formation of a curvature singularity at the Cauchy horizon and show no evidence of the appearance of a superradiant instability. In the case of a naked singularity, we f…

High Energy Physics - Theoryblack hole: rotationeffect: quantumvelocitysemiclassicalEvent horizonperturbationspace-time: black holeGeneral Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)angular momentum01 natural sciencesErgospherePenrose processGeneral Relativity and Quantum Cosmologyhorizon[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc][ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]black hole: BTZGeneral Relativity and Quantum CosmologyQuantum mechanics0103 physical sciencescurvature: singularity010306 general physicsRing singularityPhysics010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]formationNaked singularitycoupling: conformalstabilityfield theory: scalarBlack holeClassical mechanicsHigh Energy Physics - Theory (hep-th)Apparent horizonback reaction: quantum[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]massGravitational singularitysuperradianceblack hole: geometry
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Born–Infeld inspired modifications of gravity

2017

General Relativity has shown an outstanding observational success in the scales where it has been directly tested. However, modifications have been intensively explored in the regimes where it seems either incomplete or signals its own limit of validity. In particular, the breakdown of unitarity near the Planck scale strongly suggests that General Relativity needs to be modified at high energies and quantum gravity effects are expected to be important. This is related to the existence of spacetime singularities when the solutions of General Relativity are extrapolated to regimes where curvatures are large. In this sense, Born-Infeld inspired modifications of gravity have shown an extraordin…

High Energy Physics - Theorystar: compactcosmological model[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]space-time: black holeGeneral Physics and AstronomyAstrophysics01 natural sciencesGeneral Relativity and Quantum Cosmology[ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]Gravitationquantum gravity: effectBorn–Infeld gravityPhysicsenergy: highBlack holes[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]formationCosmologyregularizationcurvaturewormhole[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational singularitySingularitiesAstrophysics - Cosmology and Nongalactic AstrophysicsGravity (chemistry)Cosmology and Nongalactic Astrophysics (astro-ph.CO)General relativityEarly universegeneral relativity: solutionFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Theoretical physicsGeneral Relativity and Quantum Cosmologyspace-time: singularity0103 physical sciencesunitaritystructureWormholeinflation010306 general physicsCompact objectsSpacetime010308 nuclear & particles physicsscale: PlanckBlack holeBorn-Infeld modelHigh Energy Physics - Theory (hep-th)gravitationQuantum gravity[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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