Search results for "control systems"

showing 10 items of 590 documents

Search for an electric charge of the neutron

2018

The electrical neutrality of the neutron is linked to the electric charge quantization. It is not understood yet if the electric charge is quantized or not. Since the discovery of the neutron, many attempts have been made to measure its electric charge ${q}_{n}$ directly and indirectly. We present a method to search for a possible ${q}_{n}$ by means of an optical setup using ultracold neutrons. In a first run, a statistical sensitivity of $\ensuremath{\delta}{q}_{n}=2.4\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}20}\text{ }\text{ }e/\sqrt{\mathrm{day}}$ is achieved. Possible improvements to increase this sensitivity down to $\ensuremath{\delta}{q}_{n}\ensuremath{\approx}1\ifmmode\…

PhysicsMeasurement methodpotential: electrostatic010308 nuclear & particles physicscharge: electricStatistical sensitivitymeasurement methodssensitivity01 natural sciencesElectric chargeelectric fieldcharge: quantizationn: energy eigenstateElectric field0103 physical sciencesoptical[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]NeutronSensitivity (control systems)Atomic physics010306 general physicsmirrorstatisticalexperimental resultsn: charge: upper limit
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Probing chiral interactions up to next-to-next-to-next-to-leading order in medium-mass nuclei

2019

We study ground-state energies and charge radii of closed-shell medium-mass nuclei based on novel chiral nucleon-nucleon (NN) and three-nucleon (3N) interactions, with a focus on exploring the connections between finite nuclei and nuclear matter. To this end, we perform in-medium similarity renormalization group (IM-SRG) calculations based on chiral interactions at next-to-leading order (NLO), N$^2$LO, and N$^3$LO, where the 3N interactions at N$^2$LO and N$^3$LO are fit to the empirical saturation point of nuclear matter and to the triton binding energy. Our results for energies and radii at N$^2$LO and N$^3$LO overlap within uncertainties, and the cutoff variation of the interactions is w…

PhysicsNuclear Theory010308 nuclear & particles physicsNuclear TheoryBinding energyStarke Wechselwirkung und exotische Kerne – Abteilung BlaumFOS: Physical sciencesOrder (ring theory)Charge (physics)Renormalization groupNuclear matter01 natural sciencesNuclear Theory (nucl-th)0103 physical sciencesSensitivity (control systems)Atomic physicsNuclear Experiment010306 general physicsNuclear theoryPhysical Review C
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Position resolution of the prototype AGATA triple-cluster detector from an in-beam experiment

2009

AGATA belongs to a new generation of gamma-ray detector arrays for nuclear spectroscopy at present in its final stage of development. The detectors of these new arrays will be based on 36-fold electronically segmented coaxial germanium diodes operated in position sensitive mode. An in-beam test of the AGATA prototype triple cluster detector was carried out with the purpose of demonstrating the feasibility of such detectors and in order to measure the most sensitive parameters for their overall performance. An inverse kinematics reaction was performed, using a (48)Ti beam at an energy of 100MeV, impinging on a deuterated titanium tat-get. The results from the analysis of the experimental dat…

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsbusiness.industryPhysics::Instrumentation and DetectorsMonte Carlo methodDetectorγ-ray instrumentsgamma-ray instruments[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciencesOpticsPosition (vector)0103 physical sciencesAGATASensitivity (control systems)Coaxial010306 general physicsbusinessInstrumentationBeam (structure)Position-sensitive germanium detectorsDiode
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Half-life ofTi44

1983

The half-life of $^{44}\mathrm{Ti}$ has been measured to be ${T}_{\frac{1}{2}}=54.2\ifmmode\pm\else\textpm\fi{}2.1$ yr, somewhat higher than previously published values of 46.4\ifmmode\pm\else\textpm\fi{}1.7 and 48.2\ifmmode\pm\else\textpm\fi{}0.9 yr. The present value was obtained from the specific activity and the radioisotope concentration of several Ti${\mathrm{O}}_{2}$ samples, each spiked with a $^{44}\mathrm{Ti}$ activity of about 1.2 \ensuremath{\mu}Ci. The specific activity was measured via the 1157 keV $\ensuremath{\gamma}$ line from the decay of the $^{44}\mathrm{Sc}$ daughter. $^{44}\mathrm{Ti}$/Ti concentrations were measured with the Argonne FN tandem accelerator in conjunctio…

PhysicsNuclear and High Energy PhysicsAnalytical chemistryHalf-lifeHeavy ionSensitivity (control systems)Tandem acceleratorAccelerator mass spectrometryPhysical Review C
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Fine structure of the Gamow-Teller resonance revealed in the decay of150Ho2−isomer

2003

The $\ensuremath{\gamma}$ rays following the $72s$ ${}^{150}\mathrm{Ho}$ ${2}^{\ensuremath{-}}$ Gamow-Teller $\ensuremath{\beta}$ decay have been investigated with the CLUSTER CUBE setup, an array of six EUROBALL CLUSTER Ge detectors in close cubic geometry, providing a $\ensuremath{\gamma}$ ray detection sensitivity of $2\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}5}$ per $\ensuremath{\beta}$-parent decay for $\ensuremath{\gamma}$-ray energies up to 5 MeV. The fine structure of the Gamow-Teller resonance at 4.4-MeV excitation in ${}^{150}\mathrm{Dy}$ has been studied. The resolved levels are compared with Shell Model predictions.

PhysicsNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaNuclear TheorySHELL modelStructure (category theory)ResonanceSensitivity (control systems)Atomic physicsNuclear ExperimentExcitationPhysical Review C
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Development and calibration of the tracking Compton/Pair telescope MEGA

2005

Abstract We describe the development and tests of the prototype for a new telescope for Medium Energy Gamma-ray Astronomy (MEGA) in the energy band 0.4–50 MeV. As a successor to COMPTEL and EGRET (at low energies), MEGA aims to improve the sensitivity for astronomical sources by at least an order of magnitude. It could thus fill the severe sensitivity gap between scheduled or operating hard-X-ray and high-energy gamma-ray missions and open the way for a future Advanced Compton Telescope. MEGA records and images γ-rays by completely tracking Compton and Pair creation events in a stack of double-sided Si-strip track detectors surrounded by a pixelated CsI calorimeter. A scaled down prototype …

PhysicsNuclear and High Energy PhysicsCalorimeter (particle physics)Physics::Instrumentation and Detectorsbusiness.industryAstrophysics::High Energy Astrophysical PhenomenaCompton telescopeAstrophysics::Instrumentation and Methods for AstrophysicsMega-Tracking (particle physics)law.inventionTelescopeOpticsStack (abstract data type)lawCalibrationSensitivity (control systems)businessInstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Does interferometry probe thermalization?

2009

We carry out a systematic study of interferometry radii in ultrarelativistic heavy-ion collisions within a two-dimensional transport model. We compute the transverse radii R_o and R_s as a function of p_t for various values of the Knudsen number, which measures the degree of thermalization in the system. They converge to the hydrodynamical limit much more slowly (by a factor 3) than elliptic flow. This solves most of the HBT puzzle for central collisions: R_o/R_s is in the range 1.1-1.2 for realistic values of the Knudsen number, much closer to experimental data ($\simeq 1$) than the value 1.5 from hydrodynamical calculations. The p_t dependence of R_o and R_s, which is usually said to refl…

PhysicsNuclear and High Energy PhysicsDegree (graph theory)Nuclear TheoryElliptic flowFOS: Physical sciencesNuclear Theory (nucl-th)Knudsen flowThermalisationAmplitudeSensitivity (control systems)Knudsen numberAtomic physicsEccentricity (mathematics)Nuclear Experiment
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Coulomb shifts and shape changes in the mass 70 region

2007

The technique of recoil beta tagging has been developed which allows prompt gamma decays in nuclei from excited states to be correlated with electrons from their subsequent short-lived beta decay. This technique is ideal for studying nuclei very far from stability and improves in sensitivity for very short-lived decays and for high decay Q-values. The method has allowed excited states in 78Y to be observed for the first time, as well as an extension in the knowledge of T=1 states in 74Rb. From this new information it has been possible to compare Coulomb energy differences (CED) between T=1 states in 70Br/70Se, 74Rb/74Kr, and 78Y/78Sr. The A=70 CED exhibit an anomalous behavior which is inco…

PhysicsNuclear and High Energy PhysicsGamma rayNuclear structureFOS: Physical sciencesElectronRecoilExcited stateDouble beta decayCoulombSensitivity (control systems)Atomic physicsNuclear Experiment (nucl-ex)Nuclear Experiment
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Optimal β-beam at the CERN-SPS

2006

In this talk, based on the work [J. Burguet-Castell et al., Nucl. Phys. B 725 (2005) 306], we present an analysis of the sensitivity to the mixing angle θ 13 and the CP-violating phase δ that could be achieved by a β-beam experiment based at the SPS accelerator at CERN. We estimate the optimal γ boost of the 6He and 18Ne ions for the proposed baseline CERN-Frejus (130 km), and also perform a simultaneous optimization of the ion boost and the baseline. A possible improvement of the current SPS accelerator is considered as well. After comparing the sensitivities of all relevant setups, we conclude that a β-beam running at the maximum acceleration achievable by the SPS, γ = 150 / 250 , and wit…

PhysicsNuclear and High Energy PhysicsLarge Hadron Colliderbusiness.industryPhase (waves)Electrical engineeringAtomic and Molecular Physics and OpticsIonNuclear physicsAccelerationSensitivity (control systems)Simultaneous optimizationbusinessBeam (structure)Nuclear Physics B - Proceedings Supplements
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Theoretical predictions for the direct detection of neutralino dark matter in the NMSSM

2004

We analyse the direct detection of neutralino dark matter in the framework of the Next-to-Minimal Supersymmetric Standard Model. After performing a detailed analysis of the parameter space, taking into account all the available constraints from LEPII, we compute the neutralino-nucleon cross section, and compare the results with the sensitivity of detectors. We find that sizable values for the detection cross section, within the reach of dark matter detectors, are attainable in this framework. For example, neutralino-proton cross sections compatible with the sensitivity of present experiments can be obtained due to the exchange of very light Higgses with $m_{h_1^0}\lsim 70$ GeV. Such Higgses…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsDark matterHigh Energy Physics::PhenomenologyAstrophysics (astro-ph)FOS: Physical sciencesSupersymmetryParameter spaceAstrophysics01 natural sciencesNext-to-Minimal Supersymmetric Standard ModelHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNeutralinoBibliographyHigh Energy Physics::ExperimentSensitivity (control systems)010306 general physicsMinimal Supersymmetric Standard Model
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