685 research outputs found

    Triaxial deformation in 10Be

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    The triaxial deformation in 10^{10}Be is investigated using a microscopic α+α+n+n\alpha+\alpha+n+n model. The states of two valence neutrons are classified based on the molecular-orbit (MO) model, and the π\pi-orbit is introduced about the axis connecting the two α\alpha-clusters for the description of the rotational bands. There appear two rotational bands comprised mainly of Kπ=0+K^\pi = 0^+ and Kπ=2+K^\pi = 2^+, respectively, at low excitation energy, where the two valence neutrons occupy Kπ=3/2−K^\pi = 3/2^- or Kπ=1/2−K^\pi = 1/2^- orbits. The triaxiality and the KK-mixing are discussed in connection to the molecular structure, particularly, to the spin-orbit splitting. The extent of the triaxial deformation is evaluated in terms of the electro-magnetic transition matrix elements (Davydov-Filippov model, Q-invariant model), and density distribution in the intrinsic frame. The obtained values turned out to be Îł=15o∌20o\gamma = 15^o \sim 20^o.Comment: 15 pages, latex, 3 figure

    Performance analysis of time slicing in DVB-H

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    TV is the biggest media and the last one missing from mobile phones. Digital Video Broadcasting for Handhelds (DVB-H) is the latest development from the DVB Project targeting handheld, battery powered devices such as mobile telephones, PDAs(Personal Digital Assistants), etc. Time Division Multiplexing (TDM) is the technology that is usually used in computer and telecommunication systems. Time slicing is one of the characteristics that makes it possible to broadcast high resolution TV programes and fast IP data services to battery powered handheld terminals. This paper discusses the characteristics and advantages of Time slicing algorithm in DVB-H and presents the performance analysis of time slicing in DVB-H through both theoretical analysis and software simulation

    Important role of the spin-orbit interaction in forming the 1/2^+ orbital structure in Be isotopes

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    The structure of the second 0^+ state of ^{10}Be is investigated using a microscopic α+α+n+n\alpha+\alpha+n+n model based on the molecular-orbit (MO) model. The second 0^+ state, which has dominantly the (1/2^+)^2 configuration, is shown to have a particularly enlarged α−α\alpha-\alpha structure. The kinetic energy of the two valence neutrons occupying along the α−α\alpha-\alpha axis is reduced remarkably due to the strong α\alpha clustering and, simultaneously, the spin-orbit interaction unexpectedly plays important role to make the energy of this state much lower. The mixing of states with different spin structure is shown to be important in negative-parity states. The experimentally observed small-level spacing between 1^- and 2^- (~ 300 keV) is found to be an evidence of this spin-mixing effect. ^{12}{Be} is also investigated using α+α+4n\alpha+\alpha+4n model, in which four valence neutrons are considered to occupy the (3/2^-)^2(1/2^+)^2 configuration. The energy surface of ^{12}Be is shown to exhibit similar characteristics, that the remarkable α\alpha clustering and the contribution of the spin-orbit interaction make the binding of the state with (3/2^-)^2(1/2^+)^2 configuration properly stronger in comparison with the closed p-shell (3/2^-)^2(1/2^-)^2 configuration.Comment: 14 pages, 4 figure

    Search for three alpha states around an 16^{16}O core in 28^{28}Si

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    We investigate the existence of weakly coupled gas-like states comprised of three α\alpha particles around an 16^{16}O core in 28^{28}Si. We calculate the excited states in 28^{28}Si using the multi-configuration mixing method based on the 16^{16}O + 3α\alpha cluster model. We also include the 16^{16}O + 12^{12}C and 24^{24}Mg + α\alpha basis wave functions prepared by the generator coordinate method. To identify the gas-like states, we calculate the isoscalar monopole transition strengths and the overlap of the obtained states with the geometrical cluster wave function and the Tohsaki-Horiuchi-Schuck-R\"{o}pke (THSR) wave function. The results show that the obtained fourth and twelfth states significantly overlap with the THSR wave function. These two states clearly coexist with the 16^{16}O + 12^{12}C cluster states, emerging at similar energies. The calculated isoscalar monopole strengths between those two states are significantly large, indicating that the states are members of the excitation mode. Furthermore, the calculated root-mean-squared (RMS) radii for these states also suggest that a layer of gas-like three α\alpha particles could exist around the surface of the 16^{16}O core, which can be described as a "two-dimensional gas" in the intermediate state before the Hoyle-like three α\alpha states emerge.Comment: 5 pages, 3 figure
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