Search results for "nucleus"

showing 10 items of 1803 documents

Radio observations of active galactic nuclei with mm-VLBI

2017

Over the past few decades, our knowledge of jets produced by active galactic nuclei (AGN) has greatly progressed thanks to the development of very-long-baseline interferometry (VLBI). Nevertheless, the crucial mechanisms involved in the formation of the plasma flow, as well as those driving its exceptional radiative output up to TeV energies, remain to be clarified. Most likely, these physical processes take place at short separations from the supermassive black hole, on scales which are inaccessible to VLBI observations at centimeter wavelengths. Due to their high synchrotron opacity, the dense and highly magnetized regions in the vicinity of the central engine can only be penetrated when …

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsEvent Horizon TelescopeSupermassive black holeActive galactic nucleusOpacityFOS: Physical sciencesAstronomyAstronomy and AstrophysicsAstrophysics01 natural sciencesInterferometrySpace and Planetary Science0103 physical sciencesVery-long-baseline interferometryRadiative transferMillimeterAstrophysics - High Energy Astrophysical Phenomena010306 general physics010303 astronomy & astrophysicsThe Astronomy and Astrophysics Review
researchProduct

Numerical simulations of dynamics and emission from relativistic astrophysical jets

2013

Broadband emission from relativistic outflows (jets) of active galactic nuclei (AGN) and gamma-ray bursts (GRBs) contains valuable information about the nature of the jet itself, and about the central engine which launches it. Using special relativistic hydrodynamics and magnetohydronamics simulations we study the dynamics of the jet and its interaction with the surrounding medium. The observational signature of the simulated jets is computed using a radiative transfer code developed specifically for the purpose of computing multi-wavelength, time-dependent, non-thermal emission from astrophysical plasmas. We present results of a series of long-term projects devoted to understanding the dyn…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsHistoryJet (fluid)Active galactic nucleusAstrophysics::High Energy Astrophysical PhenomenaDynamics (mechanics)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsPlasmaAstrophysics01 natural sciences7. Clean energy010305 fluids & plasmasComputer Science ApplicationsEducationAfterglow13. Climate action0103 physical sciencesRadiative transferMagnetohydrodynamicsAstrophysics - High Energy Astrophysical PhenomenaBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsJournal of Physics: Conference Series
researchProduct

Computational general relativistic force-free electrodynamics

2020

General relativistic force-free electrodynamics is one possible plasma-limit employed to analyze energetic outflows in which strong magnetic fields are dominant over all inertial phenomena. The amazing images of black hole shadows from the galactic center and the M87 galaxy provide a first direct glimpse into the physics of accretion flows in the most extreme environments of the universe. The efficient extraction of energy in the form of collimated outflows or jets from a rotating BH is directly linked to the topology of the surrounding magnetic field. We aim at providing a tool to numerically model the dynamics of such fields in magnetospheres around compact objects, such as black holes an…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsInertial frame of referenceActive galactic nucleus010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaGalactic CenterFOS: Physical sciencesSpherical coordinate systemAstronomy and AstrophysicsComputational Physics (physics.comp-ph)Magnetar01 natural sciencesGalaxyBlack holeNeutron starSpace and Planetary ScienceQuantum electrodynamics0103 physical sciencesAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Physics - Computational Physics010303 astronomy & astrophysicsAstronomy & Astrophysics
researchProduct

Neutron skins of atomic nuclei: per aspera ad astra

2019

The complex nature of the nuclear forces generates a broad range and diversity of observational phenomena. Heavy nuclei, though orders of magnitude less massive than neutron stars, are governed by the same underlying physics, which is enshrined in the nuclear equation of state. Heavy nuclei are expected to develop a neutron-rich skin where many neutrons collect near the surface. Such a skin thickness is strongly sensitive to the poorly-known density dependence of the symmetry energy near saturation density. An accurate and model-independent determination of the neutron-skin thickness of heavy nuclei would provide a significant first constraint on the density dependence of the nuclear symmet…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsNuclear and High Energy Physicsintegumentary systemNuclear Theory010308 nuclear & particles physicsNuclear TheoryFOS: Physical sciencesElectron01 natural sciencesStandard ModelNuclear Theory (nucl-th)Nuclear physicsNeutron starOrders of magnitude (time)0103 physical sciencesAtomic nucleusNuclear astrophysicsNuclear forceNeutronNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentAstrophysics - High Energy Astrophysical PhenomenaNuclear Experiment
researchProduct

LOFAR measures the hotspot advance speed of the high-redshift blazar S5 0836+710

2019

Our goal is to study the termination of an AGN jet in the young universe and to deduce physical parameters of the jet and the intergalactic medium. We use LOFAR to image the long-wavelength radio emission of the high-redshift blazar S5 0836+710 on arcsecond scales between 120 MHz and 160 MHz. The LOFAR image shows a compact unresolved core and a resolved emission region about 1.5 arcsec to the southwest of the radio core. This structure is in general agreement with previous higher-frequency radio observations with MERLIN and the VLA. The southern component shows a moderately steep spectrum with a spectral index of about $\gtrsim -1$ while the spectral index of the core is flat to slightly i…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSpectral indexActive galactic nucleusProper motion010308 nuclear & particles physicsRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLOFARAstrophysics - Astrophysics of Galaxies01 natural sciencesRedshiftSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)0103 physical sciencesIntergalactic travelAstrophysics - High Energy Astrophysical PhenomenaBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsAstronomy & Astrophysics
researchProduct

QCD and Strongly Coupled Gauge Theories: Challenges and Perspectives

2014

We dedicate this document to the memory of Mikhail Polikarpov, who passed away in July 2013. Misha worked with us for decades as a convener of the “Confinement” section of the Quark Confinement and Hadron Spectrum Series. He guided and expanded the scientific discussion of that topic, inspiring and under taking new research avenues. From its initial conception, he supported the enterprise of this document and organized Sect. 8, writing the part on confinement himself. He attracted the XIth Conference on Quark Confinement and the Hadron Spectrum to St. Petersburg (September 8-12, 2014; see http://phys.spbu.ru/confxi.html). His warm and kind personality, his high sense of humor, his ideas in …

High Energy Physics - TheoryEFFECTIVE-FIELD-THEORYNuclear TheoryPhysics and Astronomy (miscellaneous)Physics beyond the Standard ModelReviewHEAVY-ION COLLISIONSnucl-ex7. Clean energyCosmologyHigh Energy Physics - ExperimentQUARK-GLUON PLASMADEEP-INELASTIC SCATTERINGHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Gauge theoryNuclear Experiment (nucl-ex)Nuclear ExperimentQuantum chromodynamicsPhysics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]hep-thHigh Energy Physics - Lattice (hep-lat)hep-phddc:High Energy Physics - PhenomenologyYANG-MILLS THEORYastro-ph.COAstrophysics - Cosmology and Nongalactic AstrophysicsPB-PB COLLISIONSParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)nucl-th[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]530 PhysicsStrong interactionComplex systemFOS: Physical scienceshep-lat[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]CHIRAL PERTURBATION-THEORY114 Physical sciencesELECTRIC-DIPOLE MOMENTNuclear Theory (nucl-th)Theoretical physicsHigh Energy Physics - Latticeddc:530Engineering (miscellaneous)Particle Physics - Phenomenologyhep-ex[PHYS.HLAT]Physics [physics]/High Energy Physics - Lattice [hep-lat]NUCLEUS-NUCLEUS COLLISIONSPerspective (graphical)FísicaRADIATIVE ENERGY-LOSSFlow (mathematics)High Energy Physics - Theory (hep-th)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]European Physical Journal C
researchProduct

Heavy quarkonium: progress, puzzles, and opportunities

2011

A golden age for heavy quarkonium physics dawned a decade ago, initiated by the confluence of exciting advances in quantum chromodynamics (QCD) and an explosion of related experimental activity. The early years of this period were chronicled in the Quarkonium Working Group (QWG) CERN Yellow Report (YR) in 2004, which presented a comprehensive review of the status of the field at that time and provided specific recommendations for further progress. However, the broad spectrum of subsequent breakthroughs, surprises, and continuing puzzles could only be partially anticipated. Since the release of the YR, the BESII program concluded only to give birth to BESIII; the $B$-factories and CLEO-c flo…

High Energy Physics - TheoryNuclear TheoryPhysics and Astronomy (miscellaneous)High Energy Physics::LatticeTevatronB-C MESON; QCD SUM-RULES; NUCLEUS COLLISIONSAtomic01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Broad spectrumHigh Energy Physics - Phenomenology (hep-ph)Particle and Plasma Physicseffective field theoryBatavia TEVATRON CollNuclear Experiment (nucl-ex)Nuclear ExperimentNuclear ExperimentBrookhaven RHIC CollQuantum chromodynamicsPhysicsQuantum PhysicsLarge Hadron ColliderHigh Energy Physics - Lattice (hep-lat)lattice field theoryHERAQuarkoniumNuclear & Particles PhysicsCLEOB-C MESONHigh Energy Physics - PhenomenologyDESY HERA Stordecay [quarkonium]Jefferson LabParticle physicsFOS: Physical sciencesnonrelativistic [quantum chromodynamics]DeconfinementB-factoryNuclear Theory (nucl-th)High Energy Physics - Latticescattering [heavy ion]QCD SUM-RULES0103 physical sciencesNuclearddc:530010306 general physicsEngineering (miscellaneous)Particle Physics - Phenomenologyproduction [quarkonium]BES010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyplasma [quark gluon]FísicaMoleculartetraquarkHigh Energy Physics - Theory (hep-th)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]hadron spectroscopy [meson]hadron spectroscopy [quarkonium]High Energy Physics::Experimentheavy [quarkonium]NUCLEUS COLLISIONSThe European Physical Journal C
researchProduct

Forward dijets in proton-nucleus collisions at next-to-leading order: the real corrections

2021

Using the CGC effective theory together with the hybrid factorisation, we study forward dijet production in proton-nucleus collisions beyond leading order. In this paper, we compute the "real" next-to-leading order (NLO) corrections, i.e. the radiative corrections associated with a three-parton final state, out of which only two are being measured. To that aim, we start by revisiting our previous results for the three-parton cross-section presented in our previous paper. After some reshuffling of terms, we deduce new expressions for these results, which not only look considerably simpler, but are also physically more transparent. We also correct several errors in this process. The real NLO …

High Energy Physics - Theorydijet: productionNuclear and High Energy PhysicsParticle physicsNuclear TheoryProton[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]splittingFOS: Physical sciencescollinearParton01 natural sciencesColor-glass condensateNuclear Theory (nucl-th)DGLAP equationHigh Energy Physics - Phenomenology (hep-ph)FactorizationfactorizationNLO Computations0103 physical sciencesRadiative transferEffective field theoryradiative correctionlcsh:Nuclear and particle physics. Atomic energy. Radioactivitypartonheavy ion phenomenology010306 general physicsp nucleus: scatteringPhysicsNLO computationshybrid010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]higher-order: 1Heavy Ion PhenomenologyGluonHigh Energy Physics - PhenomenologyDGLAPHigh Energy Physics - Theory (hep-th)kinematics[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]color glass condensatelcsh:QC770-798
researchProduct

Spectroscopy of short-lived radioactive molecules: A sensitive laboratory for new physics

2019

The study of molecular systems provides exceptional opportunities for the exploration of the fundamental laws of nature and for the search for physics beyond the Standard Model of particle physics. Measurements of molecules composed of naturally occurring nuclei have provided the most stringent upper bounds to the electron electric dipole moment to date, and offer a route to investigate the violation of fundamental symmetries with unprecedented sensitivity. Radioactive molecules - where one or more of their atoms possesses a radioactive nucleus - can contain heavy and deformed nuclei, offering superior sensitivity for EDM measurements as well as for other symmetry-violating effects. Radium …

High Energy Physics - TheoryexceptionalNuclear Theory[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]collinearFOS: Physical sciencesnucleus: structure function[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)ionizationPhysics::Atomic PhysicsNuclear Experiment (nucl-ex)Nuclear ExperimentNuclear Experimentenhancementnew physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]stabilitysensitivitylaserradiumelectron: electric momentHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)radioactivity[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]many-body problemnucleus: deformation
researchProduct

Forward J /ψ production in proton-nucleus collisions at high energy

2015

Inclusive production of J/ψ mesons, especially at forward rapidities, is an important probe of small-x gluons in protons and nuclei. In this paper we reevaluate the production cross sections in the color glass condensate framework, where the process is described by a large x gluon from the probe splitting into a quark pair and eikonally interacting with the target proton or nucleus. Using a standard collinear gluon distribution for the probe and an up-to-date dipole cross section fitted to HERA data to describe the target we achieve a rather good description of the cross section in proton-proton collisions, although with a rather large normalization uncertainty. More importantly, we show th…

High Energy Physics::PhenomenologyNuclear Theoryproton-nucleus collisionsfysiikkaNuclear Experiment
researchProduct