


Vol 82, No 1 (2019)
- Year: 2019
- Articles: 13
- URL: https://journal-vniispk.ru/1063-7788/issue/view/12184
Elementary Particles and Fields
Resonance States in Scattering of Slow Particles with Nonzero Orbital Angular Momentum by the Pöschl-Teller Potential
Abstract
The scattering of slow particles with nonzero orbital angular momentum in the field of a finite potential is considered. The respective scattering problem is solved in the Pais approximation. The inverse problem is solved for the Pöschl-Teller equation, and a general scheme for Pais resonances and a procedure for calculating scattering cross sections for resonance particles are formulated.



Neutrino-Oscillation Searches in the Short-Baseline Gallium Experiment BEST-2 with a 65Zn Source
Abstract
The possibility of employing a 65Zn source in the gallium experiment BEST-2 with the aim of constraining the region of allowed oscillation parameters is examined. The source activity required for the BEST-2 experiment is calculated, and the size of the source and its effect on the results of oscillation measurements are discussed along with the possibilities for producing such a source. Various schemes for implementing respective measurements are considered.



Decay of K0 to \({K^ + }{e^ - }{\bar \nu _e}\)
Abstract
The width of the neutral kaon with respect to its decay to a positively charged kaon, an electron, and an antineutrino is calculated. The branching ratios for the decay of KL and KS mesons to \({K^ + }{e^ - }{\bar \nu _e}\) are found to be about 4 × 10−9 and 10−11 respectively. The calculations presented in this article are also valid for neutral antikaons decaying to a negatively charged kaon, a positron, and a neutrino.



Nuclei
96gTc As an Alternative Gamma-Ray Emitter for Medical Diagnostics
Abstract
The possibility of employing the isotope 96gTc as a gamma-ray emitter in medical diagnostics is examined. Corresponding calculations by the TALYS-1.9 revealed that an irradiation of a 96Mo target with protons of energy E =12 → 6 MeV at a current of 100 μA for six (eight) hours makes it possible to produce 20 (26) GBq of the isotope 96gTc. In detecting gamma rays of energy in the range between 770 and 850 keV, the intensity of gamma rays from 96gTc is close to their intensity for 99mTc obtained in the reaction 100Mo(p, n), so that one can use96gTc as an alternative gamma-ray emitter.



Study of Earth’s Heat Flux by Means of Geoneutrino Detection
Abstract
The heat flux from the Earth’s interior and its connection with the number of neutrinos recorded by detectors at the Earth’s surface are discussed. The values predicted for the geoneutrino fluxes may be matched with experimental data, but the observed flux of the Earth’s internal heat requires the presence of a larger amount of radioactive elements. The amount of uranium and thorium within the Earth is constrained by measurements performed with the aid of modern geoneutrino detectors. This makes it possible to explain completely a flux of 50 TW. There are indications that the flux from the Earth’s interior is 200 to 250 TW. Such a flux could be explained only by the presence of a substantially larger amount of potassium in the Earth. In order to determine precisely the heat flux from the Earth’s interior, it is necessary to measure completely the flux of antineutrinos from all heat-releasing isotopes, including the flux of neutrinos from 40K decay. Possibly, this flux has already been observed at the Borexino detector.



New Data on Photoneutron Reaction Cross Sections for 76,78,80,82Se Nuclei
Abstract
The problem of reliability of the cross section data obtained for partial photoneutron reactions on 76,78,80,82Se nuclei in beams of quasimonoenergetic annihilation photons by means of neutron multiplicity sorting is discussed by employing objective physical criteria. It is shown that, because of substantial systematic uncertainties, experimental data on the (γ, 1n) and (γ, 2n) cross sections are unreliable. New data satisfying the reliability criteria are obtained for the partial photoneutron reaction cross sections for 76,78,82Se nuclei by an experimental—theoretical method for evaluating such cross sections and are compared with experimental data and with data evaluated earlier for the isotope 80Se. The evaluated integrated cross sections for the total photoneutron reactions on 76,78,80,82Se nuclei are compared with the predictions of the Thomas-Reiche-Kuhn classical dipole sum rule.



Cross Sections for K±N Scattering for Simulating Cumulative-Kaon Interactions in Nuclei
Abstract
Reliable cross sections for kaon-nucleon scattering are required for quantitatively estimating the effect of secondary interactions of cumulative K+ and K− mesons on their yields from various nuclei in proton-nucleus (pA) interactions at proton energies between 9 and 10 GeV and between 15 and 70 GeV. The preparation of these cross sections for a simulation code was a priority task that was solved for the kaon-momentum range between 0.35 and 2.75 GeV/c.



Deuteron Breakup Induced by 778-MeV Protons
Abstract
An experiment devoted to studying deuteron breakup induced by 778 MeV protons was performed with the aid of a deuterium bubble chamber. Experimental spectra are compared with results of calculations based on multiple-scattering theory that takes into account pole diagrams, elastic rescattering, and final-state interaction. The calculations in question describe a global behavior of the spectra, even though the theory itself was put forth for energies in the region around a few hundred GeV/c.



On the Properties of the Neutron-Rich Odd-Odd 130In Nucleus
Abstract
The properties of the odd-odd 130In nucleus, which neighbors the doubly magic neutron-rich 132Sn nucleus, are calculated in the random-phase approximation. Detailed calculations of the spectrum, electric quadrupole and magnetic dipole moments of levels, and gamma-decay properties of 130In are performed. The probability for the beta transition to this nucleus from the ground sate of the 130Cd nucleus is also calculated.



On The Contribution of the P and D Partial-Wave States to the Binding Energy of the Triton in the Bethe-Salpeter-Faddeev Approach
Abstract
The influence of the partial-wave states with nonzero orbital moment of the nucleon pair on the binding energy of the triton T(nnp) in the relativistic case is considered. The relativistic generalization of the Faddeev equation in the Bethe-Salpeter formalism is applied. Two-nucleon t matrix is obtained from the Bethe-Salpeter equation with separable kernel of nucleon-nucleon interaction of the rank one. The kernel form factors are the relativistic type of the Yamaguchi functions. The following two-nucleon partial-wave states are considered: 1S0, 3S1, 3D1, 3P0, 1P1, 3P1. The system of the integral equations are solved by using the iteration method. The binding energy of the triton and three-nucleon amplitudes are found. The contribution of the P and D states to the binding energy of triton is given.



Effect of the Splitting of Deep Nuclear Shells on the Structure of Multipole Resonances
Abstract
The effect of the splitting of nuclear shells lying substantially lower than the Fermi energy on the fragmentation of multipole resonances in cross sections for the excitation of nuclei is studied by considering the example of M6 and E1 resonances in self-conjugate sd-shell nuclei.



L-Shell Ionization during the Alpha Decay of Superheavy Nuclei from 117294Ts Tennessine Decay Chain and the Alpha Decay of the Polonium Isotope 84210Po
Abstract
The probabilities for L-shell ionization following the alpha decay of 117294Ts, 113286Nh, 109278Mt, and 105270Db superheavy nuclei from the decay chain of tennessine, which was synthesized at the Joint Institute for Nuclear Research (JINR Dubna), and the alpha decay of the isotope 84210Po are calculated and analyzed. The respective calculations rely on a quantum-mechanical model that takes into account alpha-particle tunneling through the Coulomb barrier of an atom. The relativistic electron wave functions obtained by the Dirac-Fock method were employed. The probabilities for L-shell ionization that were calculated here for the isotope 84210Po are in better agreement with experimental data than the results of earlier calculations. In contrast to what we have for K-shell ionization, where monopole transitions make a dominant contribution to the ionization probability, a significant contribution to the probability for L-shell ionization also comes from dipole and quadrupole transitions. The results of the present study will be of use in interpreting superheavy-element spectra obtained by methods of combined alpha, gamma, and electron-conversion spectroscopy.



Influence of the Change in the Galactic-Nucleosynthesis Rate before the Formation of Solar System on the Determination of Age of The Universe
Abstract
The dependence of the region of physically admissible values of uranium-thorium isotope ratios on the short-term change in nucleosynthesis rate, which increases just before the formation of the Solar system, is studied. An additional admissible region associated with the presence of the isotope 244Pu and the effect of this region on the calculation of the age of the Universe, TU, are considered within galactic-nucleosynthsis theory. The size of the admissible region and its dependence on the short-term increase in the rate of heavy-element production (enhancement of nucleosynthsis) before the formation of the Solar System is discussed along with the consistency of the predictions for the above ratios with the region of admissible values. It is shown that an enhancement of nucleosynthesis is necessary for attaining agreement between the calculated ratios of cosmochronometer nuclei and the region of admissible values, but this enhancement should not lead to an increase in the abundances of heavy elements that is greater than 1 to 3% of the total amount of synthesized heavy elements.


