Search results for "Particle physics"

showing 10 items of 6826 documents

Unitarity constraint for threshold coherent pion photoproduction on the deuteron

1997

The contribution of the two-step process {gamma}d{r_arrow}pn{r_arrow}{pi}{sup 0}d to the imaginary part of the amplitude for coherent pion production on the deuteron is calculated at threshold exploiting unitarity constraints. The result shows that this absorptive process is not negligible and has to be considered in an extraction of the elementary neutron production amplitude from the {gamma}d{r_arrow}{pi}{sup 0}d cross section at threshold. {copyright} {ital 1997} {ital The American Physical Society}

Constraint (information theory)Nuclear physicsPhysicsNuclear and High Energy PhysicsParticle physicsPionAmplitudeDeuteriumUnitarityNeutronProduction (computer science)Few-body systemsPhysical Review C
researchProduct

Resonance of minimizers forn-level quantum systems with an arbitrary cost

2004

We consider an optimal control problem describing a laser-induced population transfer on a n-level quantum system. For a convex cost depending only on the moduli of controls ( i.e. the lasers intensities), we prove that there always exists a minimizer in resonance. This permits to justify some strategies used in experimental physics. It is also quite important because it permits to reduce remarkably the complexity of the problem (and extend some of our previous results for n=2 and n=3): instead of looking for minimizers on the sphere one is reduced to look just for minimizers on the sphere . Moreover, for the reduced problem, we investigate on the question of existence of strict abnormal mi…

Control and OptimizationMathematical analysisRegular polygonOptimal controlResonance (particle physics)ModuliPontryagin's minimum principleComputational MathematicsControl and Systems EngineeringQuantum systemRotating wave approximationApplied mathematicsQuantumMathematicsESAIM: Control, Optimisation and Calculus of Variations
researchProduct

Search for topological defect dark matter with a global network of optical magnetometers

2021

Ultralight bosons such as axion-like particles are viable candidates for dark matter. They can form stable, macroscopic field configurations in the form of topological defects that could concentrate the dark matter density into many distinct, compact spatial regions that are small compared with the Galaxy but much larger than the Earth. Here we report the results of the search for transient signals from the domain walls of axion-like particles by using the global network of optical magnetometers for exotic (GNOME) physics searches. We search the data, consisting of correlated measurements from optical atomic magnetometers located in laboratories all over the world, for patterns of signals p…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsAtomic Physics (physics.atom-ph)Particle physicsGeneral Physics and AstronomyFOS: Physical sciences53001 natural sciencesArticleHigh Energy Physics - ExperimentPhysics - Atomic PhysicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesDark energy and dark matterddc:530Atomic and molecular physics010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Studies of Relativistic Jets in Active Galactic Nuclei with SKA

2014

Relativistic jets in active galactic nuclei (AGN) are among the most powerful astrophysical objects discovered to date. Indeed, jetted AGN studies have been considered a prominent science case for SKA, and were included in several different chapters of the previous SKA Science Book (Carilli & Rawlings 2004). Most of the fundamental questions about the physics of relativistic jets still remain unanswered, and await high-sensitivity radio instruments such as SKA to solve them. These questions will be addressed specially through analysis of the massive data sets arising from the deep, all-sky surveys (both total and polarimetric flux) from SKA1. Wide-field very-long-baseline-interferometri…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleus010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsJet (particle physics)01 natural sciencesAstrophysical jet0103 physical sciencesVery-long-baseline interferometryInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsStar formationAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstrophysics - Astrophysics of GalaxiesGalaxyCharacterization (materials science)13. Climate actionAstrophysics of Galaxies (astro-ph.GA)Brightness temperatureAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic AstrophysicsProceedings of Advancing Astrophysics with the Square Kilometre Array — PoS(AASKA14)
researchProduct

Variations in fundamental constants at the cosmic dawn

2020

The observation of space-time variations in fundamental constants would provide strong evidence for the existence of new light degrees of freedom in the theory of Nature. Robustly constraining such scenarios requires exploiting observations that span different scales and probe the state of the Universe at different epochs. In the context of cosmology, both the cosmic microwave background and the Lyman-α forest have proven to be powerful tools capable of constraining variations in electromagnetism, however at the moment there do not exist cosmological probes capable of bridging the gap between recombination and reionization. In the near future, radio telescopes will attempt to measure the 21…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic microwave backgroundFOS: Physical sciencesContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesCosmologyRadio telescopeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesReionizationcosmology of theories beyond the SMAstrophysiquePhysicsCOSMIC cancer database010308 nuclear & particles physicsSpectral densityhep-phAstronomy and AstrophysicsAstronomieHigh Energy Physics - Phenomenologyparticle physics-cosmology connectionastro-ph.CODark AgesreionizationAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

The transient gravitational-wave sky

2013

Interferometric detectors will very soon give us an unprecedented view of the gravitational-wave sky, and in particular of the explosive and transient Universe. Now is the time to challenge our theoretical understanding of short-duration gravitational-wave signatures from cataclysmic events, their connection to more traditional electromagnetic and particle astrophysics, and the data analysis techniques that will make the observations a reality. This paper summarizes the state of the art, future science opportunities, and current challenges in understanding gravitational-wave transients.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)Explosive materialmedia_common.quotation_subjectELECTROMAGNETIC COUNTERPARTSFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologySPIN-DOWN LIMIT0103 physical sciencesPRESUPERNOVA EVOLUTIONCORE-COLLAPSE010306 general physics010303 astronomy & astrophysicsARMED SPIRAL INSTABILITYmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Astroparticle physicsPhysicsGAMMA-RAY BURSTSNEUTRINO PAIR ANNIHILATIONGravitational waveAstronomyMASS BLACK-HOLESUniverseBAR-MODE INSTABILITYInterferometrySkyData analysisTransient (oscillation)Astrophysics - High Energy Astrophysical PhenomenaDRIVEN SUPERNOVAgravitational waves neutron stars black holesAstrophysics - Cosmology and Nongalactic AstrophysicsClassical and Quantum Gravity
researchProduct

Do metric fluctuations affect the Higgs dynamics during inflation?

2017

We show that the dynamics of the Higgs field during inflation is not affected by metric fluctuations if the Higgs is an energetically subdominant light spectator. For Standard Model parameters we find that couplings between Higgs and metric fluctuations are suppressed by $\mathcal{O}(10^{-7})$. They are negligible compared to both pure Higgs terms in the effective potential and the unavoidable non-minimal Higgs coupling to background scalar curvature. The question of the electroweak vacuum instability during high energy scale inflation can therefore be studied consistently using the Jordan frame action in a Friedmann--Lema\^itre--Robertson--Walker metric, where the Higgs-curvature coupling …

Cosmology and Nongalactic Astrophysics (astro-ph.CO)gr-qcSTANDARD MODELFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & AstrophysicsGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsGeneral Relativity and Quantum Cosmology0202 Atomic Molecular Nuclear Particle And Plasma PhysicsHigh Energy Physics - Phenomenology (hep-ph)EINSTEIN FRAMESELECTROWEAK VACUUMFIELDquantumfield theory on curved spaceScience & TechnologyPhysicsHigh Energy Physics::Phenomenologyhep-phNuclear & Particles PhysicsJORDANHigh Energy Physics - Phenomenology0201 Astronomical And Space SciencesMETASTABILITYparticle physics - cosmology connectionPhysical Sciencesastro-ph.COHigh Energy Physics::ExperimentEQUIVALENCEAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

In the realm of the Hubble tension—a review of solutions

2021

The $\Lambda$CDM model provides a good fit to a large span of cosmological data but harbors areas of phenomenology. With the improvement of the number and the accuracy of observations, discrepancies among key cosmological parameters of the model have emerged. The most statistically significant tension is the $4-6\sigma$ disagreement between predictions of the Hubble constant $H_0$ by early time probes with $\Lambda$CDM model, and a number of late time, model-independent determinations of $H_0$ from local measurements of distances and redshifts. The high precision and consistency of the data at both ends present strong challenges to the possible solution space and demand a hypothesis with en…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)satellite: PlanckPhysics and Astronomy (miscellaneous)gravitation: modelPhysics beyond the Standard ModelCosmic microwave backgroundFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsbaryon: oscillation: acoustic01 natural sciencesGeneral Relativity and Quantum CosmologyCosmologysymbols.namesakeTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)cosmological model: parameter space0103 physical sciencesstructurePlanckinflationcosmic background radiation: power spectrum010306 general physicsdark energyneutrino: interactionPhysicssupernova: Type IHubble constant010308 nuclear & particles physicsnew physicsmagnetic field: primordialtensionredshiftAstrophysics - Astrophysics of GalaxiesRedshiftrecombinationHigh Energy Physics - Phenomenology13. Climate actionAstrophysics of Galaxies (astro-ph.GA)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]relativisticsymbolsDark energy[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Phenomenology (particle physics)statisticalAstrophysics - Cosmology and Nongalactic AstrophysicsHubble's law
researchProduct

Radiative muon capture and the value of gP in nuclei

1990

Abstract Radiative muon capture by nuclei is analyzed by means of sum rule techniques, providing a total photon yield calculated with RPA precision. The measured yields relative to the ordinary muon capture rate are well reproduced for the nuclei 12C, 16O and 40Ca using a value of the pseudoscalar weak coupling constant gP enhanced by only 25% with respect to its canonical value. Therefore, the large renormalization of gP claimed up to now must be reconsidered.

Coupling constantNuclear physicsRenormalizationPseudoscalarPhysicsNuclear and High Energy PhysicsParticle physicsNuclear TheoryRadiative transferValue (computer science)Sum rule in quantum mechanicsPhoton yieldMuon capturePhysics Letters B
researchProduct

Unitarity Triangle from CP invariant quantities

2006

We construct the CKM unitarity triangle from CP invariant quantities, using the coupling constant of weak decays with flavor change from b to u, and the particle - antiparticle mixing probability in the B_s and B_d systems. Also included are new measurements of the coupling V_us in Kaon decays. Of the two solutions, one agrees perfectly with the triangle constructed from CP violating processes in the K and B meson systems. The common solution yields a triangle with an area of J/2 = (1.51 +/- 0.09) x 10^{-5} and a CP violating phase gamma = 63.1^o +/- 4.0^o.

Coupling constantPhysicsNuclear and High Energy PhysicsParticle physicsAntiparticleUnitarityHigh Energy Physics::PhenomenologyFOS: Physical sciencesInvariant (physics)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)CP violationB mesonHigh Energy Physics::Experiment
researchProduct