Search results for "BD"

showing 10 items of 3363 documents

"Table 21" of "Test of CP invariance in vector-boson fusion production of the Higgs boson in the H → ττ channel in proton–proton collisions at s=13Te…

2020

Post-fit BDT distributions in the top-quark CR for the $\tau_{\mathrm{lep}}\tau_{\mathrm{lep}}$ DF channel. The size of the combined statistical, experimental, and theoretical uncertainties is given.

Higgs Production13000.0Proton-Proton ScatteringBDT ScoreHigh Energy Physics::PhenomenologyTau-Tau DecayHigh Energy Physics::ExperimentP P -> H + X
researchProduct

"Table 3" of "Test of CP invariance in vector-boson fusion production of the Higgs boson in the H → ττ channel in proton–proton collisions at s=13TeV…

2020

Post-fit BDT distributions after the VBF event selection for the $\tau_{\mathrm{lep}}\tau_{\mathrm{had}}$ analysis channel. The VBF signal is shown for $\mu = 0.73$ and $\tilde d = -0.01$. ''Other bkg'' denotes all background contributions not listed explicitly in the legend. The size of the combined statistical, experimental, and theoretical uncertainties is given. The exact value of the $p_{\mathrm{T}}$ cut on the leading lepton depends on the trigger.

Higgs Production13000.0Proton-Proton ScatteringBDT ScoreTau-Tau DecayHigh Energy Physics::ExperimentP P -> H + X
researchProduct

"Table 2" of "Test of CP invariance in vector-boson fusion production of the Higgs boson in the H → ττ channel in proton–proton collisions at s=13TeV…

2020

Post-fit BDT distributions after the VBF event selection for the $\tau_{\mathrm{lep}}\tau_{\mathrm{lep}}$ DF analysis channel. The VBF signal is shown for $\mu = 0.73$ and $\tilde d = -0.01$. ''Other bkg'' denotes all background contributions not listed explicitly in the legend. The size of the combined statistical, experimental, and theoretical uncertainties is given.

Higgs Production13000.0Proton-Proton ScatteringBDT ScoreTau-Tau DecayHigh Energy Physics::ExperimentP P -> H + X
researchProduct

"Table 1" of "Test of CP invariance in vector-boson fusion production of the Higgs boson in the H → ττ channel in proton–proton collisions at s=13TeV…

2020

Post-fit BDT distributions after the VBF event selection for the $\tau_{\mathrm{lep}}\tau_{\mathrm{lep}}$ SF analysis channel. The VBF signal is shown for $\mu = 0.73$ and $\tilde d = -0.01$. ''Other bkg'' denotes all background contributions not listed explicitly in the legend. The size of the combined statistical, experimental, and theoretical uncertainties is given. The exact value of the $p_{\mathrm{T}}$ cut on the leptons depends on the trigger.

Higgs Production13000.0Proton-Proton ScatteringBDT ScoreTau-Tau DecayHigh Energy Physics::ExperimentP P -> H + X
researchProduct

"Table 4" of "Test of CP invariance in vector-boson fusion production of the Higgs boson in the H → ττ channel in proton–proton collisions at s=13TeV…

2020

Post-fit BDT distributions after the VBF event selection for the $\tau_{\mathrm{had}}\tau_{\mathrm{had}}$ analysis channel. The VBF signal is shown for $\mu = 0.73$ and $\tilde d = -0.01$. ''Other bkg'' denotes all background contributions not listed explicitly in the legend. The size of the combined statistical, experimental, and theoretical uncertainties is given.

Higgs Production13000.0Proton-Proton ScatteringBDT ScoreTau-Tau DecayP P -> H + X
researchProduct

Astrophysical constraints on extended gravity models

2015

We investigate the propagation of gravitational waves in the context of fourth order gravity nonminimally coupled to a massive scalar field. Using the damping of the orbital period of coalescing stellar binary systems, we impose constraints on the free parameters of extended gravity models. In particular, we find that the variation of the orbital period is a function of three mass scales which depend on the free parameters of the model under consideration; we can constrain these mass scales from current observational data.

High Energy Physics - TheoryCosmology and Nongalactic Astrophysics (astro-ph.CO)Wave propagationFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological constantGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyTheory of relativityPulsarBinary starRELATIVITYphysics of the early universemodified gravityCOSMOLOGICAL CONSTANTANISOTROPYPhysicsGravitational waveAstronomy and AstrophysicsSUPERNOVAEPULSARgravitational waves / theoryLAMBDASupernovaStarsDERIVATIVE QUANTUM-GRAVITY; COSMOLOGICAL CONSTANT; LAGRANGIANS; RELATIVITY; SUPERNOVAE; ANISOTROPY; LAMBDA; PULSARClassical mechanicsHigh Energy Physics - Theory (hep-th)LAGRANGIANSDERIVATIVE QUANTUM-GRAVITYAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Effective interactions in Ricci-Based Gravity below the non-metricity scale

2020

We show how minimally-coupled matter fields of arbitrary spin, when coupled to Ricci-Based Gravity theories, develop non-trivial effective interactions that can be treated perturbatively only below a characteristic high-energy scale $\Lambda_Q$. Our results generalize to arbitrary matter fields those recently obtained for spin 1/2 fields in \cite{Latorre:2017uve}. We then use this interactions to set bounds on the high-energy scale $\Lambda_Q$ that controls departures of Ricci-Based Gravity theories from General Relativity. Particularly, for Eddington-inspired Born-Infeld gravity we obtain the strong bound $ |\kappa|<3.5 \times 10^{-14} \text{ m}^5 \text{kg}^{-1}\text{s}^{-2} $.

High Energy Physics - TheoryGravity (chemistry)Physics and Astronomy (miscellaneous)General relativityFOS: Physical sciencesScale (descriptive set theory)lcsh:AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Lambda01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationHigh Energy Physics - Phenomenology (hep-ph)Born–Infeld model0103 physical scienceslcsh:QB460-466lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsEngineering (miscellaneous)Spin-½Mathematical physicsPhysics010308 nuclear & particles physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)lcsh:QC770-798
researchProduct

Differential Regularization of a Non-relativistic Anyon Model

1994

Differential regularization is applied to a field theory of a non-relativistic charged boson field $\phi$ with $\lambda (\phi {}^{*} \phi)^2$ self-interaction and coupling to a statistics-changing $U(1)$ Chern-Simons gauge field. Renormalized configuration-space amplitudes for all diagrams contributing to the $\phi {}^{*} \phi {}^{*} \phi \phi$ 4-point function, which is the only primitively divergent Green's function, are obtained up to 3-loop order. The renormalization group equations are explicitly checked, and the scheme dependence of the $\beta$-function is investigated. If the renormalization scheme is fixed to agree with a previous 1-loop calculation, the 2- and 3-loop contributions …

High Energy Physics - TheoryPhysicsFOS: Physical sciencesLie groupFísicaRenormalization groupSymmetry groupLambdaRenormalizationHigh Energy Physics - Theory (hep-th)Quantum mechanicsRegularization (physics)Gauge theoryBoson
researchProduct

Dark energy cosmologies for codimension-two branes

2005

A six-dimensional universe with two branes in the "football-shaped" geometry leads to an almost realistic cosmology. We describe a family of exact solutions with time dependent characteristic size of internal space. After a short inflationary period the late cosmology is either of quintessence type or turns to a radiation dominated Friedmann universe where the cosmological constant appears as a free integration constant of the solution. The radiation dominated universe with relativistic fermions is analyzed in detail, including its dimensional reduction.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsBig RipFOS: Physical sciencesNon-standard cosmologyLambda-CDM modelCosmological constantAstrophysics::Cosmology and Extragalactic AstrophysicsMetric expansion of spaceTheoretical physicsGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)De Sitter universeQuantum cosmologyScale factor (cosmology)
researchProduct

Gravitational waves in the presence of a cosmological constant

2011

We derive the effects of a non-zero cosmological constant $\Lambda$ on gravitational wave propagation in the linearized approximation of general relativity. In this approximation we consider the situation where the metric can be written as $g_{\mu\nu}= \eta_{\mu\nu}+ h_{\mu\nu}^\Lambda + h_{\mu\nu}^W$, $h_{\mu\nu}^{\Lambda,W}<< 1$, where $h_{\mu\nu}^{\Lambda}$ is the background perturbation and $h_{\mu\nu}^{W}$ is a modification interpretable as a gravitational wave. For $\Lambda \neq 0$ this linearization of Einstein equations is self-consistent only in certain coordinate systems. The cosmological Friedmann-Robertson-Walker coordinates do not belong to this class and the derived linearized…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsCosmologiaGravitational waveGeneral relativityPlane waveFísicaFOS: Physical sciencesCosmological constantGeneral Relativity and Quantum Cosmology (gr-qc)LambdaGeneral Relativity and Quantum CosmologyGravitational wavesCosmologySupernovaGeneral Relativity and Quantum CosmologyAmplitudeHigh Energy Physics - Theory (hep-th)Ones gravitacionalsQuantum mechanicsMinkowski space
researchProduct