Search results for "SCALAR"

showing 10 items of 1002 documents

Vacuum Topology of the Two Higgs Doublet Model

2011

We perform a systematic study of generic accidental Higgs-family and CP symmetries that could occur in the two-Higgs-doublet-model potential, based on a Majorana scalar-field formalism which realizes a subgroup of GL(8,C). We derive the general conditions of convexity and stability of the scalar potential and present analytical solutions for two non-zero neutral vacuum expectation values of the Higgs doublets for a typical set of six symmetries, in terms of the gauge-invariant parameters of the theory. By means of a homotopy-group analysis, we identify the topological defects associated with the spontaneous symmetry breaking of each symmetry, as well as the massless Goldstone bosons emergin…

PhysicsHigh Energy Physics - TheoryParticle physicsHyperchargeNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Spontaneous symmetry breakingScalar (mathematics)High Energy Physics::PhenomenologyMagnetic monopoleFOS: Physical sciencesScalar potentialTheoretical physicsTwo-Higgs-doublet modelHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Goldstone bosonHiggs bosonAstrophysics - Cosmology and Nongalactic AstrophysicsParticle Physics - Phenomenology
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Lagrangians for Massive Dirac Chiral Superfields

2016

A variant for the superspin one-half massive superparticle in $ 4D $, $ \mathcal{N}=1 $, based on Dirac superfields, is offered. As opposed to the current known models that use spinor chiral superfields, the propagating fields of the supermultiplet are those of the lowest mass dimensions possible: scalar, Dirac and vector fields. Besides the supersymmetric chiral condition, the Dirac superfields are not further constrained, allowing a very straightforward implementation of the path-integral method. The corresponding superpropagators are presented. In addition, an interaction super Yukawa potential, formed by Dirac and scalar chiral superfields, is given in terms of their component fields. T…

PhysicsHigh Energy Physics - TheoryParticle physicsNuclear and High Energy PhysicsCurrent (mathematics)Spinor010308 nuclear & particles physicsOperator (physics)High Energy Physics::LatticeDirac (software)Scalar (mathematics)High Energy Physics::PhenomenologyYukawa potentialFOS: Physical sciences01 natural sciencesMAJORANAHigh Energy Physics::TheoryHigh Energy Physics - Theory (hep-th)Supermultiplet0103 physical sciences010306 general physicsMathematical physics
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One-Loop Effective Action for Spherical Scalar Field Collapse

1997

We calculate the complete one-loop effective action for a spherical scalar field collapse in the large radius approximation. This action gives the complete trace anomaly, which beside the matter loop contributions, receives a contribution from the graviton loops. Our result opens a possibility for a systematic study of the back-reaction effects for a real black hole.

PhysicsHigh Energy Physics - TheoryPhysics and Astronomy (miscellaneous)GravitonCollapse (topology)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Action (physics)General Relativity and Quantum CosmologyBlack holeLoop (topology)General Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Anomaly (physics)Scalar fieldEffective action
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Scherk-Schwarz reduction of D=5 special and quaternionic geometry

2004

We give the N=2 gauged supergravity interpretation of a generic D=4, N=2 theory as it comes from generalized Scherk-Schwarz reduction of D=5, N=2 (ungauged) supergravity. We focus on the geometric aspects of the D=4 data such as the general form of the scalar potential and masses in terms of the gauging of a ``flat group''. Higgs and super-Higgs mechanism are discussed in some detail.

PhysicsHigh Energy Physics - TheoryPhysics and Astronomy (miscellaneous)Group (mathematics)SupergravityHigh Energy Physics::LatticeGauged supergravityHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaScalar potentialInterpretation (model theory)Reduction (complexity)High Energy Physics::TheoryHigh Energy Physics - Theory (hep-th)Higgs bosonFocus (optics)Particle Physics - TheoryMathematical physics
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Nonequilibrium dressing in a cavity with a movable reflecting mirror

2017

We consider a movable mirror coupled to a one-dimensional massless scalar field in a cavity. Both the field and the mirror's mechanical degrees of freedom are described quantum-mechanically, and they can interact each other via the radiation pressure operator. We investigate the dynamical evolution of mirror and field starting from a nonequilibrium initial state, and their local interaction which brings the system to a stationary configuration for long times. This allows us to study the time-dependent dressing process of the movable mirror interacting with the field, and its dynamics leading to a local equilibrium dressed configuration. Also, in order to explore the effect of the radiation …

PhysicsHigh Energy Physics - TheoryQuantum Physics010308 nuclear & particles physicsNon-equilibrium thermodynamicsFOS: Physical sciencesHarmonic potential01 natural sciencesVacuum fluctuations. Energy density. Dynamical Casimir effectMassless particlesymbols.namesakeClassical mechanicsRadiation pressureHigh Energy Physics - Theory (hep-th)Bounded function0103 physical sciencessymbols010306 general physicsHamiltonian (quantum mechanics)Quantum Physics (quant-ph)Scalar fieldQuantum
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Field Fluctuations in a One-Dimensional Cavity with a Mobile Wall

2013

We consider a scalar field in a one-dimensional cavity with a mobile wall. The wall is assumed bounded by a harmonic potential and its mechanical degrees of freedom are treated quantum mechanically. The possible motion of the wall makes the cavity length variable, and yields a wall-field interaction and an effective interaction among the modes of the cavity. We consider the ground state of the coupled system and calculate the average number of virtual excitations of the cavity modes induced by the wall-field interaction, as well as the average value of the field energy density. We compare our results with analogous quantities for a cavity with fixed walls, and show a correction to the Casim…

PhysicsHigh Energy Physics - TheoryQuantum PhysicsField (physics)Degrees of freedom (physics and chemistry)FOS: Physical sciencesGeneral Physics and AstronomyField fluctuationMechanicsPotential energyCasimir effectCasimir effectClassical mechanicsHigh Energy Physics - Theory (hep-th)Quantum optomechanicNanotechnologyPhysics::Accelerator PhysicsQuantum Physics (quant-ph)Ground stateCavity wallScalar fieldQuantum
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Flavor vacuum entanglement in boson mixing

2021

Mixing transformations in quantum field theory are non-trivial, since they are intimately related to the unitary inequivalence between Fock spaces for fields with definite mass and fields with definite flavor. Considering the superposition of two neutral scalar (spin-0) bosonic fields, we investigate some features of the emerging condensate structure of the flavor vacuum. In particular, we quantify the flavor vacuum entanglement in terms of the von Neumann entanglement entropy of the reduced state. Furthermore, in a suitable limit, we show that the flavor vacuum has a structure akin to the thermal vacuum of Thermo Field Dynamics, with a temperature dependent on both the mixing angle and the…

PhysicsHigh Energy Physics - TheoryQuantum PhysicsField (physics)Scalar (physics)FOS: Physical sciencesQuantum entanglement01 natural sciences010305 fluids & plasmasFock spaceEntropy (classical thermodynamics)High Energy Physics - Theory (hep-th)Quantum mechanics0103 physical sciencesQuantum field theoryQuantum Physics (quant-ph)010306 general physicsMixing (physics)Boson
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Maxwell symmetries and some applications

2012

The Maxwell algebra is the result of enlarging the Poincar\'{e} algebra by six additional tensorial Abelian generators that make the fourmomenta non-commutative. We present a local gauge theory based on the Maxwell algebra with vierbein, spin connection and six additional geometric Abelian gauge fields. We apply this geometric framework to the construction of Maxwell gravity, which is described by the Einstein action plus a generalized cosmological term. We mention a Friedman-Robertson-Walker cosmological approximation to the Maxwell gravity field equations, with two scalar fields obtained from the additional gauge fields. Finally, we outline further developments of the Maxwell symmetries f…

PhysicsHigh Energy Physics - TheoryScalar (mathematics)Cartan formalismFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Mathematical Physics (math-ph)Cosmological constantNoncommutative geometryGeneral Relativity and Quantum Cosmologysymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)symbolsSpin connectionGauge theoryAbelian groupEinsteinMathematical PhysicsMathematical physics
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Matter Induced Bimetric Actions for Gravity

2011

The gravitational effective average action is studied in a bimetric truncation with a nontrivial background field dependence, and its renormalization group flow due to a scalar multiplet coupled to gravity is derived. Neglecting the metric contributions to the corresponding beta functions, the analysis of its fixed points reveals that, even on the new enlarged theory space which includes bimetric action functionals, the theory is asymptotically safe in the large $N$ expansion.

PhysicsHigh Energy Physics - TheoryScalar (mathematics)General Physics and AstronomyRenormalization group flowFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Fixed pointGeneral Relativity and Quantum CosmologyGravitationHigh Energy Physics - Theory (hep-th)BibliographyEffective actionMultipletMathematical physics
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Scattering amplitudes in affine gravity

2020

Affine gravity is a connection-based formulation of gravity that does not involve a metric. After a review of basic properties of affine gravity, we compute the tree-level scattering amplitude of scalar particles interacting gravitationally via the connection in a curved spacetime. We find that, while classically equivalent to general relativity, affine gravity differs from metric quantum gravity.

PhysicsHigh Energy Physics - TheorySpacetime010308 nuclear & particles physicsGeneral relativityScalar (physics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyScattering amplitudeHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)0103 physical sciencesQuantum gravityAffine transformation010306 general physicsMathematical physicsPhysical Review
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