Search results for "Nuclear and high energy physics"

showing 10 items of 8241 documents

Probing Planck scale physics with IceCube

2005

Neutrino oscillations can be affected by decoherence induced e.g. by Planck scale suppressed interactions with the space-time foam predicted in some approaches to quantum gravity. We study the prospects for observing such effects at IceCube, using the likely flux of TeV antineutrinos from the Cygnus spiral arm. We formulate the statistical analysis for evaluating the sensitivity to quantum decoherence in the presence of the background from atmospheric neutrinos, as well as from plausible cosmic neutrino sources. We demonstrate that IceCube will improve the sensitivity to decoherence effects of ${\cal O}(E^2/M_{\rm Pl})$ by 17 orders of magnitude over present limits and, moreover, that it ca…

High Energy Physics - TheoryAstrofísicaNuclear and High Energy PhysicsParticle physicsField theory (Physics)Quantum decoherenceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics7. Clean energy01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesTeoria quànticaNeutrinsSensitivity (control systems)Neutrinos010306 general physicsNeutrino oscillationPhysicsCOSMIC cancer database010308 nuclear & particles physicsAstrophysics (astro-ph)Teoria de camps (Física)High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Orders of magnitude (time)13. Climate actionQuantum theoryQuantum gravityNeutrinoPhysical Review D
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Two-twistor particle models and free massive higher spin fields

2015

We present D=3 and D=4 models for massive particles moving in a new type of enlarged spacetime, with D-1 additional vector coordinates, which after quantization lead to the towers of massive higher spin (HS) free fields. Two classically equivalent formulations are presented: one with a hybrid spacetime/bispinor geometry and a second described by a free two-twistor dynamics with constraints. After quantization in the D=3 and D=4 cases, the wave functions are given as functions on the SL(2,R) and SL(2,C) group manifolds respectively, and describe arbitrary on-shell momenta and spin degrees of freedom. Finally, the D=6 case and possible supersymmetric extensions are mentioned.

High Energy Physics - TheoryBispinorPhysicsNuclear and High Energy PhysicsSpacetimeCoordinate vectorFOS: Physical sciencesMathematical Physics (math-ph)First quantizationSupersymmetryTwistor theoryAdS/CFT correspondenceQuantization (physics)Classical mechanicsHigh Energy Physics - Theory (hep-th)Mathematical PhysicsMathematical physicsJournal of High Energy Physics
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A model for the very early universe

2008

A model with N species of massless fermions interacting via (microscopic) gravitational torsion in de Sitter spacetime is investigated in the limit N->infinity. The U_V(N)*U_A(N) flavor symmetry is broken dynamically irrespective of the (positive) value of the induced four-fermion coupling. This model is equivalent to a theory with free but massive fermions fluctuating about the chiral condensate. When the fermions are integrated out in a way demonstrated long ago by Candelas and Raine, the associated gap equation together with the Friedmann equation predict that the Hubble parameter vanishes. Introducing a matter sector (subject to a finite gauge symmetry) as a source for subsequent cos…

High Energy Physics - TheoryChiral anomalyPhysicsNuclear and High Energy PhysicsHigh Energy Physics::LatticeFriedmann equationsHigh Energy Physics::PhenomenologyFOS: Physical sciencesFermionMassless particleHigh Energy Physics - PhenomenologyGeneral Relativity and Quantum Cosmologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)De Sitter universesymbolsAxionGauge symmetryHubble's lawMathematical physicsJournal of High Energy Physics
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Implications for dark matter direct detection in the presence of LIGO-motivated primordial black holes

2019

We discuss formation of dark matter (DM) mini-halos around primordial black holes (PBHs) and its implication on DM direct detection experiments, including axion searches. Motivated by LIGO observations, we consider $f_{\textrm{DM}} \simeq 0.01$ as the fraction of DM in PBHs with masses $10 M_{\odot} - 70 M_{\odot}$. In this case, we expect the presence of dressed PBHs after Milky Way halo formation with mini-halo masses peaked around $M_{\textrm{halo}} \sim (50-55) M_{\textrm{PBH}}$. We analyze the effect of tidal forces acting on dressed PBHs within the Milky Way galaxy. In the solar neighborhood, the mini-halos are resistant against tidal disruption from the mean-field potential of the ga…

High Energy Physics - TheoryDISRUPTIONHALO MODELSPrimordial black holeAstrophysicsDark mini-halosdark matter direct detectionkosmologia01 natural sciencesGeneral Relativity and Quantum CosmologyLIMITSHigh Energy Physics - Phenomenology (hep-ph)BulgePhysicsprimordial black holeslcsh:QC1-999High Energy Physics - PhenomenologyBULGEMILKY-WAYLIGO-Virgo collaborationHaloAstrophysics - Cosmology and Nongalactic Astrophysicsaxion dark matterNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Axion dark matterMilky WayDark mattermustat aukotFOS: Physical sciencesPrimordial black holesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsDark matter direct detection114 Physical sciencespimeä ainedark mini-halos0103 physical sciences010306 general physicsAxionCP CONSERVATIONAstrophysics::Galaxy Astrophysics010308 nuclear & particles physicsCONSTRAINTSAstrophysics - Astrophysics of GalaxiesLIGOGalaxyHigh Energy Physics - Theory (hep-th)Astrophysics of Galaxies (astro-ph.GA)lcsh:Physics
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The 1-loop effective potential for the Standard Model in curved spacetime

2018

The renormalisation group improved Standard Model effective potential in an arbitrary curved spacetime is computed to one loop order in perturbation theory. The loop corrections are computed in the ultraviolet limit, which makes them independent of the choice of the vacuum state and allows the derivation of the complete set of $\beta$-functions. The potential depends on the spacetime curvature through the direct non-minimal Higgs-curvature coupling, curvature contributions to the loop diagrams, and through the curvature dependence of the renormalisation scale. Together, these lead to significant curvature dependence, which needs to be taken into account in cosmological applications, which i…

High Energy Physics - TheoryDe Sitter spaceVacuum stateUNIVERSEfield theories in higher dimensionskosmologia01 natural sciencesGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsHigh Energy Physics - Phenomenology (hep-ph)INFLATIONRADIATIVE-CORRECTIONSGauge theoryELECTROWEAK VACUUMMathematical physicsPhysics02 Physical SciencesPhysicshep-thhiukkasfysiikan standardimalliRENORMALIZATION-GROUP EQUATIONShep-phSPONTANEOUS SYMMETRY-BREAKINGNuclear & Particles PhysicsHigh Energy Physics - PhenomenologyHIGGS MASSPhysical SciencesGAUGE-THEORIESMathematics::Differential GeometryNuclear and High Energy Physicsgr-qcFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Curvatureclassical theories of gravityGeneral Relativity and Quantum Cosmology0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivityfield theories in lower dimensions010306 general physics01 Mathematical SciencesInflation (cosmology)Science & TechnologySpacetimeSTABILITYta114010308 nuclear & particles physicsgravitaatioLoop (topology)High Energy Physics - Theory (hep-th)INTERACTING SCALAR FIELDlcsh:QC770-798Perturbation theory (quantum mechanics)Journal of High Energy Physics
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Flavour mixing transport theory and resonant leptogenesis

2021

We derive non-equilibrium quantum transport equations for flavour-mixing fermions. We develop the formalism mostly in the context of resonant leptogenesis with two mixing Majorana fermions and one lepton flavour, but our master equations are valid more generally in homogeneous and isotropic systems. We give a hierarchy of quantum kinetic equations, valid at different approximations, that can accommodate helicity and arbitrary mass differences. In the mass-degenerate limit the equations take the familiar form of density matrix equations. We also derive the semiclassical Boltzmann limit of our equations, including the CP-violating source, whose regulator corresponds to the flavour coherence d…

High Energy Physics - TheoryDensity matrixNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesSemiclassical physicsQC770-798hiukkasfysiikkakosmologia01 natural sciences114 Physical sciencesHigh Energy Physics - Phenomenology (hep-ph)Nuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesMaster equationThermal Field Theory010306 general physicscosmology of theories beyond the SMMixing (physics)Mathematical physicsPhysicsThermal quantum field theory010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFermionCosmology of Theories beyond the SMthermal field theory3. Good healthHigh Energy Physics - PhenomenologyMAJORANACP violationHigh Energy Physics - Theory (hep-th)LeptogenesisAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
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Ricci-Based Gravity theories and their impact on Maxwell and nonlinear electromagnetic models

2019

Abstract We extend the correspondence between metric-affine Ricci-Based Gravity the- ories and General Relativity (GR) to the case in which the matter sector is represented by linear and nonlinear electromagnetic fields. This complements previous studies focused on fluids and scalar fields. We establish the general algorithm that relates the matter fields in the GR and RBG frames and consider some applications. In particular, we find that the so-called Eddington-inspired Born-Infeld gravity theory coupled to Maxwell electromag- netism is in direct correspondence with GR coupled to Born-Infeld electromagnetism. We comment on the potential phenomenological implications of this relation.

High Energy Physics - TheoryElectromagnetic fieldPhysicsNuclear and High Energy PhysicsGravity (chemistry)010308 nuclear & particles physicsGeneral relativityScalar (physics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyNonlinear systemTheoretical physicsHigh Energy Physics - Theory (hep-th)Electromagnetism0103 physical sciencesBeyond Standard Modellcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityElectromagnetic model010306 general physicsClassical Theories of GravityGeneral algorithmJournal of High Energy Physics
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Vacuum energy densities of a field in a cavity with a mobile boundary

2015

We consider the zero-point field fluctuations, and the related field energy densities, inside a one-dimensional and a three-dimensional cavity with a mobile wall. The mechanical degrees of freedom of the mobile wall are described quantum mechanically and they are fully included in the overall system dynamics. In this optomechanical system, the field and the wall can interact with each other through the radiation pressure on the wall, given by the photons inside the cavity or even by vacuum fluctuations. We consider two cases: the one-dimensional electromagnetic field and the three-dimensional scalar field, and use the Green's functions formalism, which allows extension of the results obtain…

High Energy Physics - TheoryElectromagnetic fieldPhysicsQuantum PhysicsNuclear and High Energy PhysicsPhotonQuantum Optomechanics Vacuum Fluctuations Vacuum Energy DensitiesZero-point energyFOS: Physical sciencesRadiation pressureVacuum energyHigh Energy Physics - Theory (hep-th)Quantum electrodynamicsQuantum Physics (quant-ph)Scalar fieldCavity wallQuantum fluctuation
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Real symplectic formulation of local special geometry

2006

We consider a formulation of local special geometry in terms of Darboux special coordinates $P^I=(p^i,q_i)$, $I=1,...,2n$. A general formula for the metric is obtained which is manifestly $\mathbf{Sp}(2n,\mathbb{R})$ covariant. Unlike the rigid case the metric is not given by the Hessian of the real function $S(P)$ which is the Legendre transform of the imaginary part of the holomorphic prepotential. Rather it is given by an expression that contains $S$, its Hessian and the conjugate momenta $S_I=\frac{\partial S}{\partial P^I}$. Only in the one-dimensional case ($n=1$) is the real (two-dimensional) metric proportional to the Hessian with an appropriate conformal factor.

High Energy Physics - TheoryHessian matrixPhysicsPure mathematicsNuclear and High Energy PhysicsHolomorphic functionFOS: Physical sciencesLegendre functionLegendre transformationsymbols.namesakeAssociated Legendre polynomialsHigh Energy Physics - Theory (hep-th)Real-valued functionMetric (mathematics)symbolsParticle Physics - TheorySymplectic geometryPhysics Letters B
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Cubic interactions of Maxwell-like higher spins

2017

We study the cubic vertices for Maxwell-like higher-spins in flat and (A)dS background spaces of any dimension. Reducibility of their free spectra implies that a single cubic vertex involving any three fields subsumes a number of couplings among different particles of various spins. The resulting vertices do not involve traces of the fields and in this sense are simpler than their Fronsdal counterparts. We propose an extension of both the free theory and of its cubic deformation to a more general class of partially reducible systems, that one can obtain from the original theory upon imposing trace constraints of various orders. The key to our results is a version of the Noether procedure al…

High Energy Physics - TheoryHigher Spin SymmetryPhysicsNuclear and High Energy PhysicsTransversalitySpins010308 nuclear & particles physicsFOS: Physical sciencesHigher Spin Gravity01 natural sciencesSpectral lineVertex (geometry)Settore FIS/02 - Fisica Teorica Modelli e Metodi Matematicisymbols.namesakeTheoretical physicsGauge Symmetry Higher Spin Gravity Higher Spin SymmetryHigh Energy Physics - Theory (hep-th)Gauge Symmetry0103 physical sciencessymbolslcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityGauge Symmetry Higher Spin Gravity Higher Spin SymmetryNoether's theorem010306 general physics
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