Search results for "lower bounds"

showing 10 items of 259 documents

Reconciling tensor and scalar observables in G-inflation

2018

The simple $m^2\phi^2$ potential as an inflationary model is coming under increasing tension with limits on the tensor-to-scalar ratio $r$ and measurements of the scalar spectral index $n_s$. Cubic Galileon interactions in the context of the Horndeski action can potentially reconcile the observables. However, we show that this cannot be achieved with only a constant Galileon mass scale because the interactions turn off too slowly, leading also to gradient instabilities after inflation ends. Allowing for a more rapid transition can reconcile the observables but moderately breaks the slow-roll approximation leading to a relatively large and negative running of the tilt $\alpha_s$ that can be …

High Energy Physics - TheoryPhysicsInflation (cosmology)Spectral indexCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsScalar (mathematics)Cosmic microwave backgroundFOS: Physical sciencesAstronomy and AstrophysicsObservableContext (language use)General Relativity and Quantum Cosmology (gr-qc)01 natural sciencesUpper and lower boundsGeneral Relativity and Quantum CosmologyTheoretical physicsHigh Energy Physics - Theory (hep-th)0103 physical sciencesTensor010306 general physicsAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Proof II: Lower Bounds

2019

In this chapter we give a lower bound on \(\ln \det S_{\delta ,z}\) which is valid with high probability, and then using also the upper bounds of Chap. 16, we conclude the proof of Theorem 15.3.1 with the help of Theorem 12.1.2.

High probabilityCombinatoricsUpper and lower boundsMathematics
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Quantum search of spatial regions

2003

Can Grover's algorithm speed up search of a physical region - for example a 2-D grid of size sqrt(n) by sqrt(n)? The problem is that sqrt(n) time seems to be needed for each query, just to move amplitude across the grid. Here we show that this problem can be surmounted, refuting a claim to the contrary by Benioff. In particular, we show how to search a d-dimensional hypercube in time O(sqrt n) for d at least 3, or O((sqrt n)(log n)^(3/2)) for d=2. More generally, we introduce a model of quantum query complexity on graphs, motivated by fundamental physical limits on information storage, particularly the holographic principle from black hole thermodynamics. Our results in this model include a…

Holographic principleDiscrete mathematicsQuantum PhysicsComputational complexity theoryFOS: Physical sciencesComputer Science::Software EngineeringGraph theoryGeneral Relativity and Quantum Cosmology (gr-qc)Unitary matrixUpper and lower boundsGeneral Relativity and Quantum CosmologyCombinatoricsHypercubeQuantum Physics (quant-ph)Black hole thermodynamicsQuantum computerMathematics44th Annual IEEE Symposium on Foundations of Computer Science, 2003. Proceedings.
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On an Inequality for Legendre Polynomials

2020

This paper is concerned with the orthogonal polynomials. Upper and lower bounds of Legendre polynomials are obtained. Furthermore, entropies associated with discrete probability distributions is a topic considered in this paper. Bounds of the entropies which improve some previously known results are obtained in terms of inequalities. In order to illustrate the results obtained in this paper and to compare them with other results from the literature some graphs are provided.

Inequalitylcsh:MathematicsGeneral Mathematicsmedia_common.quotation_subject010102 general mathematicsGegenbauerlcsh:QA1-939Legendre01 natural sciencesChebyshev filterUpper and lower bounds010101 applied mathematicsChebyshevOrthogonal polynomialsComputingMethodologies_SYMBOLICANDALGEBRAICMANIPULATIONComputer Science (miscellaneous)Probability distributionOrder (group theory)Applied mathematics0101 mathematicsEngineering (miscellaneous)Legendre polynomialshypergeometric representationmedia_commonMathematicsMathematics
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Dark matter from gravitational particle production at reheating

2015

We show that curvature induced particle production at reheating generates adiabatic dark matter if there are non-minimally coupled spectator scalars weakly coupled to visible matter. The observed dark matter abundance implies an upper bound on spectator masses $m$ and non-minimal coupling values $\xi$. For example, assuming quadratic inflation, instant reheating and a single spectator scalar with only gravitational couplings, the observed dark matter abundance is obtained for $m\sim 0.1$ GeV and $\xi \sim 1$. Larger mass and coupling values of the spectator are excluded as they would lead to overproduction of dark matter.

Inflation (cosmology)PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsNuclear TheoryDark matterScalar (mathematics)FOS: Physical sciencesAstronomy and AstrophysicsDecoupling (cosmology)AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsCurvature7. Clean energy01 natural sciencesUpper and lower boundsGravitationGeneral Relativity and Quantum CosmologyHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesParticle010306 general physicsNuclear ExperimentAstrophysics - Cosmology and Nongalactic Astrophysics
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Upper bound on the tensor-to-scalar ratio in GUT-scale supersymmetric hybrid inflation

2014

We explore the upper bound on the tensor-to-scalar ratio r in supersymmetric (F-term) hybrid inflation models with the gauge symmetry breaking scale set equal to the value 2.86⋅1016 GeV2.86⋅1016 GeV, as dictated by the unification of the MSSM gauge couplings. We employ a unique renormalizable superpotential and a quasi-canonical Kähler potential, and the scalar spectral index nsns is required to lie within the two-sigma interval from the central value found by the Planck satellite. In a sizable region of the parameter space the potential along the inflationary trajectory is a monotonically increasing function of the inflaton, and for this case, r≲2.9⋅10−4r≲2.9⋅10−4, while the spectral index…

Inflation (cosmology)PhysicsNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)SuperpotentialScalar (mathematics)High Energy Physics::PhenomenologyFOS: Physical sciencesSupersymmetryInflatonUpper and lower boundsHigh Energy Physics - PhenomenologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Astrophysics - Cosmology and Nongalactic AstrophysicsMinimal Supersymmetric Standard ModelGauge symmetryPhysics Letters B
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The linear diophantine problem of Frobenius for subsets of arithmetic sequences

1997

Let A k = {a 1,. . . , a k } $ \subset \Bbb N $ with gcd (a 1,. . . , a k ) = 1. We shall say that a natural number n has a representation by a 1,. . . , a k if $ n =\sum \limits_{i=1}^{k}a_ix_i,\; x_i\in \Bbb N_0 $ . Let g = g (A k ) be the largest integer with no such representation. We then study the set A k = {a,ha + d,ha + 2d,..., ha + (k - 1) d} h,d > 0, gcd (a,d) = 1). If l k denotes the greatest number of elements which can be omitted without altering g (A k ), we show that ¶¶ $ 1-{4 \over \sqrt k} \le {l_k\over k} \le 1 - {3\over k}, $ ¶¶ provided a > k, or a = k with $ d \ge 2 h \sqrt {k} $ . The lower bound can be improved to 1 - 4 / k if we choose a > (k - 4) k + 3. Moreover, we…

IntegerGeneral MathematicsDiophantine equationNatural numberArithmeticUpper and lower boundsMathematicsArchiv der Mathematik
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On the dynamics of the AB Doradus system

2006

We present an astrometric analysis of the binary systems ABDorA /ABDorC and ABDorBa / ABDorBb. These two systems of well-known late-type stars are gravitationally associated and they constitute the quadruple ABDoradus system. From the astrometric data available at different wavelengths, we report: (i) a determination of the orbit of ABDorC, the very low mass companion to ABDorA, which confirms the mass estimate of 0.090Msun reported in previous works; (ii) a measurement of the parallax of ABDorBa, which unambiguously confirms the long-suspected physical association between this star and ABDorA; and (iii) evidence of orbital motion of ABDorBa around ABDorA, which places an upper bound of 0.4…

KinematicsAB DorFOS: Physical sciencesBinary numberIndividualAstrophysicsLate-typeStar (graph theory)AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAUpper and lower boundsAstrometry ; Stars ; Kinematics ; Binaries ; Close ; Late-type ; Individual ; Rst 137 B ; AB DorRst 137 BPhysicsAstrophysics (astro-ph)BinariesAstronomy and AstrophysicsAstrometryStars:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Stars[SDU]Sciences of the Universe [physics]Space and Planetary ScienceOrbital motionOrbit (dynamics)UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Low MassParallaxClose:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Astronomy & Astrophysics
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A Linear Programming Method for Bounding Plastic Deformations

1988

A method for providing upper and lower bounds to plastic deformations is presented, which has the feature of being applicable both below and above the structure shakedown limit. The bounds provided are expressed in terms of some fictitious plastic strains obeying relaxed yielding laws, whose evaluation is made by means of a suitable LP-based algorithm.

Linear programmingFeature (computer vision)Bounding overwatchMathematical analysisStructure (category theory)GeometryLimit (mathematics)Upper and lower boundsMathematicsShakedown
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Adaptive Neural Stabilizing Controller for a Class of Mismatched Uncertain Nonlinear Systems by State and Output Feedback

2015

In this paper, first, an adaptive neural network (NN) state-feedback controller for a class of nonlinear systems with mismatched uncertainties is proposed. By using a radial basis function NN (RBFNN), a bound of unknown nonlinear functions is approximated so that no information about the upper bound of mismatched uncertainties is required. Then, an observer-based adaptive controller based on RBFNN is designed to stabilize uncertain nonlinear systems with immeasurable states. The state-feedback and observer-based controllers are based on Lyapunov and strictly positive real-Lyapunov stability theory, respectively, and it is shown that the asymptotic convergence of the closed-loop system to ze…

Lyapunov functionObserver (quantum physics)Computer Simulation; Feedback; Neural Networks (Computer); Nonlinear Dynamics; Control and Systems Engineering; Software; Information Systems; Human-Computer Interaction; Computer Science Applications1707 Computer Vision and Pattern Recognition; Electrical and Electronic EngineeringComputer Science Applications1707 Computer Vision and Pattern RecognitionNeural Networks (Computer)Nonlinear controlUpper and lower boundsFeedbackComputer Science ApplicationsHuman-Computer InteractionNonlinear systemsymbols.namesakeNonlinear DynamicsControl and Systems EngineeringControl theoryAdaptive systemStability theorysymbolsComputer SimulationNeural Networks ComputerElectrical and Electronic EngineeringSoftwareInformation SystemsMathematicsIEEE Transactions on Cybernetics
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