Search results for " Cosmology"

showing 10 items of 1486 documents

Manifestations of dark matter and variations of fundamental constants in atoms and astrophysical phenomena

2015

We present an overview of recent developments in the detection of light bosonic dark matter, including axion, pseudoscalar axion-like and scalar dark matter, which form either a coherently oscillating classical field or topological defects (solitons). We emphasise new high-precision laboratory and astrophysical measurements, in which the sought effects are linear in the underlying interaction strength between dark matter and ordinary matter, in contrast to traditional detection schemes for dark matter, where the effects are quadratic or higher order in the underlying interaction parameters and are extremely small. New terrestrial experiments include measurements with atomic clocks, spectros…

High Energy Physics - TheoryNuclear Theory (nucl-th)High Energy Physics - PhenomenologyCosmology and Nongalactic Astrophysics (astro-ph.CO)High Energy Physics - Phenomenology (hep-ph)Nuclear TheoryHigh Energy Physics - Theory (hep-th)Atomic Physics (physics.atom-ph)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsPhysics - Atomic PhysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Quantum transport and the phase space structure of the Wightman functions

2019

We study the phase space structure of exact quantum Wightman functions in spatially homogeneous, temporally varying systems. In addition to the usual mass shells, the Wightman functions display additional coherence shells around zero frequency $k_0=0$, which carry the information of the local quantum coherence of particle-antiparticle pairs. We find also other structures, which encode non-local correlations in time, and discuss their role and decoherence. We give a simple derivation of the cQPA formalism, a set of quantum transport equations, that can be used to study interacting systems including the local quantum coherence. We compute quantum currents created by a temporal change in a par…

High Energy Physics - TheoryNuclear and High Energy PhysicsAstrophysics and AstronomyLEPTOGENESISCosmology and Nongalactic Astrophysics (astro-ph.CO)Quantum decoherencegr-qcFOS: Physical sciencesSemiclassical physicsGeneral Relativity and Quantum Cosmology (gr-qc)114 Physical sciences01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityThermal Field Theory010306 general physicsQuantumELECTROWEAK BARYOGENESISParticle Physics - PhenomenologyPhysicsThermal quantum field theory010308 nuclear & particles physicsGeneral Relativity and Cosmologyhep-thhep-phFermionFERMIONSBaryogenesisHigh Energy Physics - PhenomenologyCP violationClassical mechanicsHigh Energy Physics - Theory (hep-th)Phase spaceastro-ph.COlcsh:QC770-798Quantum Dissipative SystemsParticle Physics - TheoryAstrophysics - Cosmology and Nongalactic AstrophysicsCoherence (physics)
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Efficient resummation of high post-Newtonian contributions to the binding energy

2021

A factorisation property of Feynman diagrams in the context the Effective Field Theory approach to the compact binary problem has been recently employed to efficiently determine the static sector of the potential at fifth post-Newtonian (5PN) order. We extend this procedure to the case of non-static diagrams and we use it to fix, by means of elementary algebraic manipulations, the value of more than one thousand diagrams at 5PN order, that is a substantial fraction of the diagrams needed to fully determine the dynamics at 5PN. This procedure addresses the redundancy problem that plagues the computation of the binding energy with respect to more "efficient" observables like the scattering an…

High Energy Physics - TheoryNuclear and High Energy PhysicsBlack HolesComputationFOS: Physical sciencesBinary numberContext (language use)General Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesake0103 physical sciencesEffective field theoryFeynman diagramlcsh:Nuclear and particle physics. Atomic energy. RadioactivityStatistical physicsAlgebraic numberResummation010306 general physicsPhysics010308 nuclear & particles physicsEffective Field TheoriesObservableHigh Energy Physics - Theory (hep-th)symbolslcsh:QC770-798Classical Theories of GravityJournal of High Energy Physics
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Hairy black-holes in shift-symmetric theories

2020

Scalar hair of black holes in theories with a shift symmetry are constrained by the no-hair theorem of Hui and Nicolis, assuming spherical symmetry, time-independence of the scalar field and asymptotic flatness. The most studied counterexample is a linear coupling of the scalar with the Gauss-Bonnet invariant. However, in this case the norm of the shift-symmetry current $J^2$ diverges at the horizon casting doubts on whether the solution is physically sound. We show that this is not an issue since $J^2$ is not a scalar quantity, since $J^\mu$ is not a diff-invariant current in the presence of Gauss-Bonnet. The same theory can be written in Horndeski form with a non-analytic function $G_5 \s…

High Energy Physics - TheoryNuclear and High Energy PhysicsBlack HolesCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmology0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsPhysical quantityMathematical physicsPhysics010308 nuclear & particles physicsScalar (physics)Black HoleInvariant (physics)Linear couplingSettore FIS/02 - Fisica Teorica Modelli e Metodi MatematiciHigh Energy Physics - Theory (hep-th)astro-ph.COlcsh:QC770-798Circular symmetryScalar fieldClassical Theories of GravityAstrophysics - Cosmology and Nongalactic AstrophysicsCounterexample
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Cosmological Constant and Local Gravity

2010

We discuss the linearization of Einstein equations in the presence of a cosmological constant, by expanding the solution for the metric around a flat Minkowski space-time. We demonstrate that one can find consistent solutions to the linearized set of equations for the metric perturbations, in the Lorentz gauge, which are not spherically symmetric, but they rather exhibit a cylindrical symmetry. We find that the components of the gravitational field satisfying the appropriate Poisson equations have the property of ensuring that a scalar potential can be constructed, in which both contributions, from ordinary matter and Lambda > 0, are attractive. In addition, there is a novel tensor potentia…

High Energy Physics - TheoryNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)De Sitter spaceFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyDe Sitter universeLinearized gravity0103 physical sciencesMinkowski spaceSchwarzschild metric010303 astronomy & astrophysicsMathematical physicsPhysicsInhomogeneous cosmology010308 nuclear & particles physicsGeneral Relativity and CosmologyFísicaClassical mechanicsLorenz gauge conditionHigh Energy Physics - Theory (hep-th)Einstein field equationsAstrophysics - Cosmology and Nongalactic Astrophysics
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Chirality transfer and chiral turbulence in gauge theories

2020

Chirality transfer between fermions and gauge fields plays a crucial role for understanding the dynamics of anomalous transport phenomena such as the Chiral Magnetic Effect. In this proceeding we present a first principles study of these processes based on classical-statistical real-time lattice simulations of strongly coupled QED $(e^2N_f=64)$. Our simulations demonstrate that a chirality imbalance in the fermion sector triggers chiral plasma instabilities in the gauge field sector, which ultimately lead to the generation of long range helical magnetic fields via a self-similar turbulent cascade of the magnetic helicity.

High Energy Physics - TheoryNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)High Energy Physics::Latticechiral plasma instabilitiesFOS: Physical sciences01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Magnetic helicity0103 physical sciencesGauge theory010306 general physicsPhysicsChirality transferchiral turbulence010308 nuclear & particles physicsmagnetogensisHigh Energy Physics::PhenomenologyFermionPlasmaMagnetic fieldHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)CascadeQuantum electrodynamicsChirality (chemistry)Transport phenomenaAstrophysics - Cosmology and Nongalactic Astrophysics
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Tensor bounds on the hidden universe

2018

During single clock inflation, hidden fields (i.e. fields coupled to the inflaton only gravitationally) in their adiabatic vacua can ordinarily only affect observables through virtual effects. After renormalizing background quantities (fixed by observations at some pivot scale), all that remains are logarithmic runnings in correlation functions that are both Planck and slow roll suppressed. In this paper we show how a large number of hidden fields can partially compensate this suppression and generate a potentially observable running in the tensor two point function, consistently inferable courtesy of a large $N$ resummation. We detour to address certain subtleties regarding loop correction…

High Energy Physics - TheoryNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectCosmic microwave backgroundFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)ddc:500.201 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesakeTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityTensorPlanck010306 general physicsmedia_commonPhysicsInflation (cosmology)Slow roll010308 nuclear & particles physicsScalar (physics)InflatonCosmology of Theories beyond the SMUniverseHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)symbolslcsh:QC770-798Renormalization Regularization and RenormalonsAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
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Non-equilibrium dynamics of a scalar field with quantum backreaction

2021

We study the dynamical evolution of coupled one- and two-point functions of a scalar field in the 2PI framework at the Hartree approximation, including backreaction from out-of-equilibrium modes. We renormalize the 2PI equations of motion in an on-shell scheme in terms of physical parameters. We present the Hartree-resummed renormalized effective potential at finite temperature and critically discuss the role of the effective potential in a non-equilibrium system. We follow the decay and thermalization of a scalar field from an initial cold state with all energy stored in the potential, into a fully thermalized system with a finite temperature. We identify the non-perturbative processes of …

High Energy Physics - TheoryNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)quantum dissipative systemsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)QC770-798hiukkasfysiikkakosmologia114 Physical sciences01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Nuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesThermal Field Theory010306 general physics010308 nuclear & particles physicsthermal field theoryHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Nonperturbative Effectsnonperturbative effectskvanttikenttäteoriaQuantum Dissipative SystemsAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
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Constraints on Conformal Windows from Holographic Duals

2009

We analyze a beta function with the analytic form of Novikov-Shifman-Vainshtein-Zakharov result in the five dimensional gravity-dilaton environment. We show how dilaton inherits poles and fixed points of such beta function through the zeros and points of extremum in its potential. Super Yang-Mills and supersymmetric QCD are studied in detail and Seiberg's electric-magnetic duality in the dilaton potential is explicitly demonstrated. Non-supersymmetric proposals of similar functional form are tested and new insights into the conformal window as well as determinations of scheme-independent value of the anomalous dimension at the fixed point are presented.

High Energy Physics - TheoryNuclear and High Energy PhysicsGeneral Physics and AstronomyDuality (optimization)FOS: Physical sciencesConformal mapFixed point01 natural sciencesTheoretical physicssymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesGauge theory010306 general physicsBeta functionPhysics010308 nuclear & particles physicsHigh Energy Physics - Lattice (hep-lat)Astronomy and AstrophysicsAdS/CFT correspondenceHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)symbolsSeiberg dualityDilaton
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Dynamical generation of wormholes with charged fluids in quadratic Palatini gravity

2014

The dynamical generation of wormholes within an extension of General Relativity (GR) containing (Planck's scale-suppressed) Ricci-squared terms is considered. The theory is formulated assuming the metric and connection to be independent (Palatini formalism) and is probed using a charged null fluid as a matter source. This has the following effect: starting from Minkowski space, when the flux is active the metric becomes a charged Vaidya-type one, and once the flux is switched off the metric settles down into a static configuration such that far from the Planck scale the geometry is virtually indistinguishable from that of the standard Reissner-Nordstr\"om solution of GR. However, the innerm…

High Energy Physics - TheoryNuclear and High Energy PhysicsGeneral relativityPhysical constantDynamical generation of wormholesFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Curvature01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationTheoretical physicsGeneral Relativity and Quantum CosmologySingularityFísica Aplicada0103 physical sciencesMinkowski spaceWormhole010306 general physicsQuantumPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsHigh Energy Physics - Theory (hep-th)Astrophysics - High Energy Astrophysical PhenomenaQuadratic Palatini gravityCharged fluids
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