1,426 research outputs found

    Of autoregressive continuous time model parameters estimation

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    This article revisits a sequential approach to the estimation of the parameter in a first-order autoregressive model (AR(1)) with continuous time. There is provided a numerical study to get a results of sequential estimations of the parameter in first-order autoregressive model with continuous time and is computed a stopping rule and the optimal time of observations. Also there is provided a comparing analysis of estimation results with using the sequential approach both the optimal time of observations

    g9/2g_{9/2} neutron strength in the N=29N=29 isotones and the 52^{52}Cr(d,pd,p)53^{53}Cr reaction

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    We performed a measurement of the 52^{52}Cr(d,p)53(d,p)^{53}Cr reaction at 16 MeV using the Florida State University Super-Enge Split-Pole Spectrograph (SE-SPS) and observed 26 states. While all of the states observed here had been seen in previous (d,p)(d,p) experiments, we changed five LL assignments from those reported previously and determined LL values for nine states that had not had such assignments made previously. The g9/2g_{9/2} neutron strength observed in 53^{53}Cr in the present work and in the N=29N=29 isotones 49^{49}Ca, 51^{51}Ti, and 55^{55}Fe via (d,p)(d,p) reactions is much smaller than the sum rule for this strength. Most of the observed L=4L=4 strength in these nuclei is located in states near 4 MeV excitation energy. The remaining g9/2g_{9/2} strength may be located in the continuum or may be fragmented among many bound states. A covariant density functional theory calculation provides support for the hypothesis that the g9/2g_{9/2} neutron orbit is unbound in 53^{53}Cr. The (α,3\alpha,^3He) reaction may provide a more sensitive probe for the missing g9/2g_{9/2} neutron strength. In addition, particle-γ\gamma coincidence experiments may help resolve some remaining questions in this nucleus.Comment: 15 pages, 5 figures. arXiv admin note: text overlap with arXiv:2212.0438

    Investigation of octupole collectivity near the A=72A =72 shape-transitional point

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    Enhanced octupole collectivity is expected in the neutron-deficient Ge, Se and Kr isotopes with neutron number N40N \approx 40 and has indeed been observed for 70,72^{70,72}Ge. Shape coexistence and configuration mixing are, however, a notorious challenge for theoretical models trying to reliably predict octupole collectivity in this mass region, which is known to feature rapid shape changes with changing nucleon number and spin of the system. To further investigate the microscopic configurations causing the prolate-oblate-triaxial shape transition at A72A \approx 72 and their influence on octupole collectivity, the rare isotopes 72^{72}Se and 74,76^{74,76}Kr were studied via inelastic proton scattering in inverse kinematics. While significantly enhanced octupole strength of 32\sim 32 Weisskopf units (W.u.) was observed for 72^{72}Se, only strengths of 15\sim 15 W.u. were observed for 74,76^{74,76}Kr. In combination with existing data, the new data clearly question a simple origin of enhanced octupole strengths around N=40N = 40. The present work establishes two regions of distinct octupole strengths with a sudden strength increase around the A=72A=72 shape transitional point

    The {\eta}'-carbon potential at low meson momenta

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    The production of η\eta^\prime mesons in coincidence with forward-going protons has been studied in photon-induced reactions on 12^{12}C and on a liquid hydrogen (LH2_2) target for incoming photon energies of 1.3-2.6 GeV at the electron accelerator ELSA. The η\eta^\prime mesons have been identified via the ηπ0π0η6γ\eta^\prime\rightarrow \pi^0 \pi^0\eta \rightarrow 6 \gamma decay registered with the CBELSA/TAPS detector system. Coincident protons have been identified in the MiniTAPS BaF2_2 array at polar angles of 2θp112^{\circ} \le \theta _{p} \le 11^{\circ}. Under these kinematic constraints the η\eta^\prime mesons are produced with relatively low kinetic energy (\approx 150 MeV) since the coincident protons take over most of the momentum of the incident-photon beam. For the C-target this allows the determination of the real part of the η\eta^\prime-carbon potential at low meson momenta by comparing with collision model calculations of the η\eta^\prime kinetic energy distribution and excitation function. Fitting the latter data for η\eta^\prime mesons going backwards in the center-of-mass system yields a potential depth of V = -(44 ±\pm 16(stat)±\pm15(syst)) MeV, consistent with earlier determinations of the potential depth in inclusive measurements for average η\eta^\prime momenta of \approx 1.1 GeV/cc. Within the experimental uncertainties, there is no indication of a momentum dependence of the η\eta^\prime-carbon potential. The LH2_2 data, taken as a reference to check the data analysis and the model calculations, provide differential and integral cross sections in good agreement with previous results for η\eta^\prime photoproduction off the free proton.Comment: 9 pages, 13 figures. arXiv admin note: text overlap with arXiv:1608.0607

    Photoproduction of eta mesons from the neutron: cross sections and double polarization observable E

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    Photoproduction of η\eta mesons from neutrons} \abstract{Results from measurements of the photoproduction of η\eta mesons from quasifree protons and neutrons are summarized. The experiments were performed with the CBELSA/TAPS detector at the electron accelerator ELSA in Bonn using the η3π06γ\eta\to3\pi^{0}\to6\gamma decay. A liquid deuterium target was used for the measurement of total cross sections and angular distributions. The results confirm earlier measurements from Bonn and the MAMI facility in Mainz about the existence of a narrow structure in the excitation function of γnnη\gamma n\rightarrow n\eta. The current angular distributions show a forward-backward asymmetry, which was previously not seen, but was predicted by model calculations including an additional narrow P11P_{11} state. Furthermore, data obtained with a longitudinally polarized, deuterated butanol target and a circularly polarized photon beam were analyzed to determine the double polarization observable EE. Both data sets together were also used to extract the helicity dependent cross sections σ1/2\sigma_{1/2} and σ3/2\sigma_{3/2}. The narrow structure in the excitation function of γnnη\gamma n\rightarrow n\eta appears associated with the helicity-1/2 component of the reaction

    Les Houches 2015: Physics at TeV colliders - new physics working group report

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    We present the activities of the 'New Physics' working group for the 'Physics at TeV Colliders' workshop (Les Houches, France, 1-19 June, 2015). Our report includes new physics studies connected with the Higgs boson and its properties, direct search strategies, reinterpretation of the LHC results in the building of viable models and new computational tool developments. Important signatures for searches for natural new physics at the LHC and new assessments of the interplay between direct dark matter searches and the LHC are also considered.Comment: Proceedings of the New Physics Working Group of the 2015 Les Houches Workshop, Physics at TeV Colliders, Les Houches 1-19 June 2015. 197 page

    Measurement of pi^0 photoproduction on the proton at MAMI C

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    Differential cross sections for the gamma p -> pi^0 p reaction have been measured with the A2 tagged-photon facilities at the Mainz Microtron, MAMI C, up to the center-of-mass energy W=1.9 GeV. The new results, obtained with a fine energy and angular binning, increase the existing quantity of pi^0 photoproduction data by ~47%. Owing to the unprecedented statistical accuracy and the full angular coverage, the results are sensitive to high partial-wave amplitudes. This is demonstrated by the decomposition of the differential cross sections in terms of Legendre polynomials and by further comparison to model predictions. A new solution of the SAID partial-wave analysis obtained after adding the new data into the fit is presented.Comment: 13 pages, 12 figures, 1 tabl
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