Search results for "RADIOACTIVITY"

showing 10 items of 334 documents

Frame covariant nonminimal multifield inflation

2017

We introduce a frame-covariant formalism for inflation of scalar-curvature theories by adopting a differential geometric approach which treats the scalar fields as coordinates living on a field-space manifold. This ensures that our description of inflation is both conformally and reparameterization covariant. Our formulation gives rise to extensions of the usual Hubble and potential slow-roll parameters to generalized fully frame-covariant forms, which allow us to provide manifestly frame-invariant predictions for cosmological observables, such as the tensor-to-scalar ratio $r$, the spectral indices $n_{\cal R}$ and $n_T$, their runnings $\alpha_{\cal R}$ and $\alpha_T$, the non-Gaussianity…

High Energy Physics - TheoryPhysicsNuclear and High Energy Physics010308 nuclear & particles physicsScalar (mathematics)FOS: Physical sciencesObservableGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsParameter spaceCurvature01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)0103 physical sciencesHiggs bosonlcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityCovariant transformationBoundary value problem010306 general physicsEffective actionMathematical physicsNuclear Physics B
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One-loop effective action for a generic 2d dilaton gravity theory

1997

We study the one-loop effective action for a generic two-dimensional dilaton gravity theory conformally coupled to $N$ matter fields. We obtain an explicit expression for the effective action in the weak-coupling limit under a suitable restriction of the dilaton potential asymptotics. Our result applies to the CGHS model as well as to the spherically symmetric general relativity. The effective action is obtained by using the background-field method, and we take into account the loop contributions from all the fields in the classical action and from the ghosts. In the large-$N$ limit, and after an appropriate field redefinition, the one-loop correction takes the form of the Polyakov-Liouvill…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsField (physics)General relativityCGHS modelFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyAction (physics)Loop (topology)General Relativity and Quantum CosmologyHigh Energy Physics::TheoryHigh Energy Physics - Theory (hep-th)lcsh:QC770-798Dilatonlcsh:Nuclear and particle physics. Atomic energy. RadioactivityLimit (mathematics)Effective actionMathematical physicsNuclear Physics B
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Coordinate space calculation of two- and three-loop sunrise-type diagrams, elliptic functions and truncated Bessel integral identities

2019

We integrate three-loop sunrise-type vacuum diagrams in $D_0=4$ dimensions with four different masses using configuration space techniques. The finite parts of our results are in numerical agreement with corresponding three-loop calculations in momentum space. Using some of the closed form results of the momentum space calculation we arrive at new integral identities involving truncated integrals of products of Bessel functions. For the non-degenerate finite two-loop sunrise-type vacuum diagram in $D_0=2$ dimensions we make use of the known closed form $p$-space result to express the moment of a product of three Bessel functions in terms of a sum of Claussen polylogarithms. Using results fo…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsMathematical analysisElliptic functionFOS: Physical sciencesPosition and momentum spaceLoop (topology)High Energy Physics - Phenomenologysymbols.namesakeIdentity (mathematics)High Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Product (mathematics)symbolslcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityConfiguration spaceCoordinate spaceBessel function
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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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The two-loop five-particle amplitude in $\mathcal{N}=8$ supergravity

2019

We compute for the first time the two-loop five-particle amplitude in $\mathcal{N}=8$ supergravity. Starting from the known integrand, we perform an integration-by-parts reduction and express the answer in terms of uniform weight master integrals. The latter are known to evaluate to non-planar pentagon functions, described by a 31-letter symbol alphabet. We express the final result for the amplitude in terms of uniform weight four symbols, multiplied by a small set of rational factors. The amplitude satisfies the expected factorization properties when one external graviton becomes soft, and when two external gravitons become collinear. We verify that the soft divergences of the amplitude ex…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsPure mathematics010308 nuclear & particles physicsSupergravityFOS: Physical sciencesFunction (mathematics)01 natural sciencesSmall setScattering amplitudeAmplitudeFactorizationHigh Energy Physics - Theory (hep-th)0103 physical scienceslcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityLimit (mathematics)010306 general physicsScattering AmplitudesSupergravity ModelsN=8 Supergravity
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Modular invariant dynamics and fermion mass hierarchies around τ = i

2021

We discuss fermion mass hierarchies within modular invariant flavour models. We analyse the neighbourhood of the self-dual point $\tau=i$, where modular invariant theories possess a residual $Z_4$ invariance. In this region the breaking of $Z_4$ can be fully described by the spurion $\epsilon \approx \tau - i$, that flips its sign under $Z_4$. Degeneracies or vanishing eigenvalues of fermion mass matrices, forced by the $Z_4$ symmetry at $\tau=i$, are removed by slightly deviating from the self-dual point. Relevant mass ratios are controlled by powers of $|\epsilon|$. We present examples where this mechanism is a key ingredient to successfully implement an hierarchical spectrum in the lepto…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsSupersymmetric Standard Model010308 nuclear & particles physicsSpectrum (functional analysis)Compactification and String ModelsFermionQC770-798Invariant (physics)01 natural sciencesSymmetry (physics)High Energy Physics - PhenomenologyNuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesBeyond Standard ModelNeutrino Physics010306 general physicsEigenvalues and eigenvectorsLeptonMinimal Supersymmetric Standard ModelMathematical physicsSign (mathematics)Journal of High Energy Physics
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Neutrino pair annihilation ( $$\nu {\bar{\nu }}\rightarrow e^-e^+$$ ν ν ¯ → e - e + ) in the presence of quintessence surrounding a black hole

2021

Quintessence fields, introduced to explain the speed-up of the Universe, might affect the geometry of spacetime surrounding black holes, as compared to the standard Schwarzschild and Kerr geometries. In this framework, we study the neutrino pairs annihilation into electron-positron pairs ($\nu{\bar \nu}\to e^-e^+$) near the surface of a neutron star, focusing, in particular, on the Schwarzschild-like geometry in presence of quintessence fields. The effect of the latter is to increase the minimum photon-sphere radius ($R_{ph}$), increasing in such a way the maximum energy deposition rate near to $R_{ph}$. The rate turns out to be several orders of magnitude greater than the rate computed in …

High Energy Physics - TheoryPhysicsParticle physicsAnnihilationPhysics and Astronomy (miscellaneous)General relativityAstrophysics::High Energy Astrophysical PhenomenaRadiusQC770-798AstrophysicsGeneral Relativity and Quantum CosmologyBlack holeQB460-466Neutron starGeneral Relativity and Quantum CosmologyNuclear and particle physics. Atomic energy. RadioactivityNeutrinoAstrophysics - High Energy Astrophysical PhenomenaEngineering (miscellaneous)Schwarzschild radiusQuintessenceEuropean Physical Journal C: Particles and Fields
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The geometry of branes and extended superspaces

1999

We argue that a description of supersymmetric extended objects from a unified geometric point of view requires an enlargement of superspace. To this aim we study in a systematic way how superspace groups and algebras arise from Grassmann spinors when these are assumed to be the only primary entities. In the process, we recover generalized spacetime superalgebras and extensions of supersymmetry found earlier. The enlargement of ordinary superspace with new parameters gives rise to extended superspace groups, on which manifestly supersymmetric actions may be constructed for various types of p-branes, including D-branes (given by Chevalley-Eilenberg cocycles) with their Born-Infeld fields. Thi…

High Energy Physics - TheoryPhysicsQuantum PhysicsNuclear and High Energy PhysicsSpinorSpacetimeFOS: Physical sciencesField (mathematics)Mathematical Physics (math-ph)SupersymmetrySuperspaceGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryTheoretical physicsHigh Energy Physics - Theory (hep-th)Brane cosmologylcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityPoint (geometry)BraneQuantum Physics (quant-ph)Mathematical PhysicsNuclear Physics B
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Consistent QFT description of non-standard neutrino interactions

2019

Neutrino oscillations are precision probes of new physics beyond the Standard Model. Apart from neutrino masses and mixings, they are also sensitive to possible deviations of low-energy interactions between quarks and leptons from the Standard Model predictions. In this paper we develop a systematic description of such non-standard interactions (NSI) in oscillation experiments within the quantum field theory framework. We calculate the event rate and oscillation probability in the presence of general NSI, starting from the effective field theory (EFT) in which new physics modifies the flavor or Lorentz structure of charged-current interactions between leptons and quarks. We also provide the…

High Energy Physics - TheoryQuarkNuclear and High Energy PhysicsParticle physicsPhysics beyond the Standard Modelfield theory01 natural sciencesStandard Modeleffective field theory0103 physical sciencesEffective field theorylcsh:Nuclear and particle physics. Atomic energy. RadioactivityNeutrino Physicsneutrino: massQuantum field theory010306 general physicsNeutrino oscillationnumerical calculationsneutrino: interactionPhysics010308 nuclear & particles physicsnew physicsHigh Energy Physics::Phenomenologyquantum mechanicsEffective Field Theories3. Good healthHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]lcsh:QC770-798neutrino: oscillationNeutrinoneutrino: mixingLepton
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Sterile Neutrinos, Black Hole Vacuum and Holographic Principle

2021

We construct an effective field theory (EFT) model that describes matter field interactions with Schwarzschild mini-black-holes (SBH's), treated as a scalar field, $B_0(x)$. Fermion interactions with SBH's require a random complex spurion field, $\theta_{ij}$, which we interpret as the EFT description of "holographic information," which is correlated with the SBH as a composite system. We consider Hawking's virtual black hole vacuum (VBH) as a Higgs phase, $\langle B_0 \rangle =V$. Integrating sterile neutrino loops, the field $\theta_{ij}$ is promoted to a dynamical field, necessarily developing a tachyonic instability and acquiring a VEV of order the Planck scale. For $N$ sterile neutrino…

High Energy Physics - TheorySterile neutrinoParticle physicsPhysics and Astronomy (miscellaneous)FOS: Physical scienceslcsh:AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:QB460-466Effective field theorylcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsVirtual black holeEngineering (miscellaneous)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyOrder (ring theory)Higgs phaseBlack holeHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)lcsh:QC770-798Scalar fieldSchwarzschild radius
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