Search results for "BT"

showing 10 items of 1498 documents

High-precision comparison of the antiproton-to-proton charge-to-mass ratio

2015

Invariance under the charge, parity, time-reversal (CPT) transformation$^{1}$ is one of the fundamental symmetries of the standard model of particle physics. This CPT invariance implies that the fundamental properties of antiparticles and their matter-conjugates are identical, apart from signs. There is a deep link between CPT invariance and Lorentz symmetry—that is, the laws of nature seem to be invariant under the symmetry transformation of spacetime—although it is model dependent$^{2}$. A number of high-precision CPT and Lorentz invariance tests—using a co-magnetometer, a torsion pendulum and a maser, among others—have been performed$^{3}$, but only a few direct high-precision CPT tests …

PhysicsAntiparticleParticle physicsMultidisciplinaryCPT symmetryLorentz transformationLorentz covarianceBaryonsymbols.namesakeStandard-Model ExtensionAntiprotonQuantum mechanicsAntimattersymbolsPräzisionsexperimente - Abteilung BlaumParticle Physics - Experiment
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More on the determination of the coronal heating function from Yohkoh data

2002

Two recent works have analyzed a solar large and steady coronal loop observed with Yohkoh/SXT in two filter passbands to infer the distribution of the heating along it. Priest et al. (2000) modelled the distribution of the temperature obtained from filter ratio method with an analytical approach, and concluded that the heating was uniform along the loop. Aschwanden (2001) found that a uniform heating led to an unreasonably large plasma column depth along the line of sight, and, using a two component loop model, that a footpoint-heated model loop (with a minor cool component) yields more acceptable physical solutions. We revisit the analysis of the same loop system, considering conventional …

PhysicsBackground subtractionLine-of-sightAstrophysics (astro-ph)FluxFOS: Physical sciencesAstronomy and AstrophysicsCoronal loopFunction (mathematics)AstrophysicsComputational physicslaw.inventionLoop (topology)Filter (large eddy simulation)Space and Planetary SciencelawHydrostatic equilibrium
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On the importance of background subtraction in the analysis of coronal loops observed with TRACE

2010

In the framework of TRACE coronal observations, we compare the analysis and diagnostics of a loop after subtracting the background with two different and independent methods. The dataset includes sequences of images in the 171 A, 195 A filter bands of TRACE. One background subtraction method consists in taking as background values those obtained from interpolation between concentric strips around the analyzed loop. The other method is a pixel-to-pixel subtraction of the final image when the loop had completely faded out, already used by Reale & Ciaravella 2006. We compare the emission distributions along the loop obtained with the two methods and find that they are considerably differen…

PhysicsBackground subtractionTrace (linear algebra)Subtractionastrofisica Fisica solare Sun: corona Sun: X-rays gamma rays method: data analysisFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsSTRIPSCoronal loopFilter (signal processing)law.inventionComputational physicsLoop (topology)Settore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencelawSolar and Stellar Astrophysics (astro-ph.SR)Interpolation
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Analysis of a multi-wavelength time-resolved observation of a coronal loop

2005

Several items on the diagnostics and interpretation of coronal loop observations are under debate. In this work, we analyze a well-defined loop system detected in a time-resolved observation in several spectral bands. The dataset includes simultaneous images in the TRACE 171 A, 195 A and 284 A bands, and Yohkoh/SXT, and two rasters taken with SoHO/CDS in twelve relevant lines. The loop is initially best visible in the TRACE 195 A filter band, and later in the 171 A filter band, with correspondence with the CDS raster images at log T \~ 6.0-6.1. We have taken as pixel-by-pixel background the latest TRACE, Yohkoh and CDS images where the loop has faded out. We examine the loop morphology evol…

PhysicsBackground subtractionbusiness.industryAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsSpectral bandsCoronal loopAstrophysicsLight curveSpectral lineRatio distributionLoop (topology)corona – Sun : X-rays gamma raysOpticsUV radiation – SunSpace and Planetary ScienceFilter (video)business
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Dispersion relations applied to double-folding potentials from chiral effective field theory

2020

We present a determination of optical potentials using the double-folding method based on chiral effective field theory nucleon-nucleon interactions at next-to-next-to-leading order combined with dispersion relations to constrain the imaginary part. This approach is benchmarked on O16-O16 collisions, and extended to the C12-C12 and C12-O16 cases. Predictions derived from these potentials are compared to data for elastic scattering at energies up to 1000 MeV, as well as for fusion at low energy. Without adjusting parameters, excellent agreement with experiment is found. In addition, we study the sensitivity of the corresponding cross sections to the nucleon-nucleon interactions and nuclear d…

PhysicsElastic scattering010308 nuclear & particles physicsNuclear TheoryStarke Wechselwirkung und exotische Kerne – Abteilung BlaumOrder (ring theory)Généralités7. Clean energy01 natural sciencesPhysique atomique et nucléaireFolding (chemistry)Low energyDispersion relation0103 physical sciencesEffective field theorySensitivity (control systems)Atomic physicsNuclear Experiment010306 general physicsNuclear theoryPhysical Review C
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Isotope shift of40,42,44,48Ca in the 4s2S1/2→ 4p2P3/2transition

2015

We report on improved isotope shift measurements of the isotopes 40,42,44,48Ca in the 4s2S1/2→4p2P3/2 transition using collinear laser spectroscopy. Accurately known isotope shifts in the 4s2S1/2→4p2P1/2 (D1) transition were used to calibrate the ion beam energy with an uncertainty of ΔU ≈ ± 0.25 V. The accuracy in the D2 transition was improved by a factor of 5–10. A King-plot analysis of the two transitions revealed that the field shift factor in the D2 line is about 1.8(13)% larger than in the D1 transition which is ascribed to relativistic contributions of the 4p1/2 wave function.

PhysicsField (physics)Ion beamIsotopeIsotopic shiftPräzisionsexperimente - Abteilung BlaumAtomic physicsCondensed Matter PhysicsSpectroscopyAtomic and Molecular Physics and OpticsShift factorLine (formation)Journal of Physics B: Atomic, Molecular and Optical Physics
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Seeing Double:ASASSN-18bt Exhibits a Two-Component Rise in the Early-Time K2 Light Curve

2018

On 2018 Feb. 4.41, the All-Sky Automated Survey for SuperNovae (ASAS-SN) discovered ASASSN-18bt in the K2 Campaign 16 field. With a redshift of z=0.01098 and a peak apparent magnitude of B_{max}=14.31, ASASSN-18bt is the nearest and brightest SNe Ia yet observed by the Kepler spacecraft. Here we present the discovery of ASASSN-18bt, the K2 light curve, and pre-discovery data from ASAS-SN and the Asteroid Terrestrial-impact Last Alert System (ATLAS). The K2 early-time light curve has an unprecedented 30-minute cadence and photometric precision for an SN~Ia light curve, and it unambiguously shows a ~4 day nearly linear phase followed by a steeper rise. Thus, ASASSN-18bt joins a growing list o…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Field (physics)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsRadiusindividual (ASASSN-18bt SN 2018oh) [supernovae]Light curve01 natural sciencesPower lawRedshiftSupernovaApparent magnitude13. Climate actionSpace and Planetary ScienceAsteroid0103 physical sciencesQD010306 general physicsAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsQCQB
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Dealing with contaminants in Coulomb excitation of radioactive beams

2020

Abstract Data analysis of the Coulomb excitation experiment of the exotic 206Hg nucleus, recently performed at CERN’s HIE-ISOLDE facility, needs to account for the contribution to target excitation due to the strongly-present beam contaminant 130Xe. In this paper, the contamination subtraction procedure is presented.

PhysicsHistoryLarge Hadron Collider010308 nuclear & particles physicsCoulomb excitationSubtraction proceduretutkimuslaitteetCoulomb excitationContaminationhiukkaskiihdyttimet01 natural sciencesAccelerators and Storage Rings3100Computer Science ApplicationsEducationNuclear physics0103 physical sciencesPhysics::Accelerator PhysicsNuclear Physics - Experiment010306 general physicsNuclear ExperimentydinfysiikkaBeam (structure)ExcitationRadioactive beams
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Theg-factor of highly charged ions

2015

Highly charged ions provide a unique opportunity to test our understanding of atomic properties under extreme conditions: The electric field strength seen by an electron bound to a nucleus at the distance of the Bohr radius ranges from 1010 V/cm in hydrogen to1016 V/cm in hydrogenlike uranium. The theory of quantum electrodynamics (QED) allows for calculation e.g. of binding energies, transition probabilities or magnetic moments. While at low fields QED is tested to very high precision, new, hypothetical nonlinear effects like photon- photon interaction or a violation of Lorentz symmetry may occur in strong fields which then would lead to an extension of the Standard Model. The ultra-high p…

PhysicsHistoryPhotonMagnetic momentHighly charged ionElectronComputer Science ApplicationsEducationIonStandard ModelElectric fieldPräzisionsexperimente - Abteilung BlaumAtomic physicsBohr radiusJournal of Physics: Conference Series
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Cu charge radii reveal a weak sub-shell effect at N=40

2016

Collinear laser spectroscopy on Cu58-75 isotopes was performed at the CERN-ISOLDE radioactive ion beam facility. In this paper we report on the isotope shifts obtained from these measurements. State-of-the-art atomic physics calculations have been undertaken in order to determine the changes in mean-square charge radii δ(r2)A,A′ from the observed isotope shifts. A local minimum is observed in these radii differences at N=40, providing evidence for a weak N=40 sub-shell effect. However, comparison of δ(r2)A,A′ with a droplet model prediction including static deformation deduced from the spectroscopic quadrupole moments, points to the persistence of correlations at N=40.

PhysicsIon beamIsotope010308 nuclear & particles physicsModel predictionShell (structure)Charge (physics)[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesPhysique atomique et nucléaire0103 physical sciencesQuadrupolePhysics::Accelerator PhysicsPhysics::Atomic PhysicsPräzisionsexperimente - Abteilung BlaumAtomic physicsDeformation (engineering)010306 general physicsSpectroscopyNuclear Experiment
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