864 research outputs found

    Services within a busy period of an M/M/1 queue and Dyck paths

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    We analyze the service times of customers in a stable M/M/1 queue in equilibrium depending on their position in a busy period. We give the law of the service of a customer at the beginning, at the end, or in the middle of the busy period. It enables as a by-product to prove that the process of instants of beginning of services is not Poisson. We then proceed to a more precise analysis. We consider a family of polynomial generating series associated with Dyck paths of length 2n and we show that they provide the correlation function of the successive services in a busy period with (n+1) customers

    Az „Idegbizottság” szerepe a homoszexualitás magyarországi dekriminalizációjában

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    Tanulmányunkban a másként „megoldhatatlannak” tűnő társadalmi kérdések medikalizációjának menetét illusztráljuk egy 20. századi magyarországi történeti példán keresztül: a homoszexuális cselekmények 1961-es magyarországi dekriminalizációjának hátterét vizsgáljuk meg 1958-ból származó, korábban ismeretlen levéltári források fényében

    Constraining Big Bang lithium production with recent solar neutrino data

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    The 3He({\alpha},{\gamma})7Be reaction affects not only the production of 7Li in Big Bang nucleosynthesis, but also the fluxes of 7Be and 8B neutrinos from the Sun. This double role is exploited here to constrain the former by the latter. A number of recent experiments on 3He({\alpha},{\gamma})7Be provide precise cross section data at E = 0.5-1.0 MeV center-of-mass energy. However, there is a scarcity of precise data at Big Bang energies, 0.1-0.5 MeV, and below. This problem can be alleviated, based on precisely calibrated 7Be and 8B neutrino fluxes from the Sun that are now available, assuming the neutrino flavour oscillation framework to be correct. These fluxes and the standard solar model are used here to determine the 3He(alpha,gamma)7Be astrophysical S-factor at the solar Gamow peak, S(23+6-5 keV) = 0.548+/-0.054 keVb. This new data point is then included in a re-evaluation of the 3He({\alpha},{\gamma})7Be S-factor at Big Bang energies, following an approach recently developed for this reaction in the context of solar fusion studies. The re-evaluated S-factor curve is then used to re-determine the 3He({\alpha},{\gamma})7Be thermonuclear reaction rate at Big Bang energies. The predicted primordial lithium abundance is 7Li/H = 5.0e-10, far higher than the Spite plateau.Comment: Final accepted version, some typos corrected, in the press at Phys. Rev.

    Novel Design of a Model Reference Adaptive Controller for Soft Tissue Operations

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    Model Reference Adaptive Controllers (MRAC) have dual functionality: besides guaranteeing precise trajectory track- ing of the controlled system, they have to provide an “external control loop” with the illusion that it controls a physical system of prescribed dynamic properties, i.e., the “reference system”. The MRACs are designed traditionally by Lyapunov’s 2 nd method that is mathematically complicated, requiring strong skills from the designer. Adaptive controllers alternatively designed by the use of Robust Fixed Point Transformations (RFPT) operate according to Banach’s Fixed Point Theorem , and are normally simple iterative constructions that also have a standard variant for MRAC design. This controller assumes a single actuator that is driven adaptively. Master–Slave Systems form a distinct class of practical applications, in which two arms—the master and the slave—operate simultaneously. The movement of the master must be tracked precisely by the slave in spite of the quite different forces exerted by them. In the present paper, a soft tissue-cutting operation by a master–slave structure is simulated. The master arm has a simple torque–reference friction model, and is driven by the surgeon. The obtained master arm trajectory has to be precisely tracked by the electric DC motor driven slave system, which is in dynamic interaction with the actual tissue under operation. It is shown via simulations that the RFPT-based design can efficiently solve such tasks without considerable mathematical complexity

    Determination of gamma-ray widths in 15^{15}N using nuclear resonance fluorescence

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    The stable nucleus 15^{15}N is the mirror of 15^{15}O, the bottleneck in the hydrogen burning CNO cycle. Most of the 15^{15}N level widths below the proton emission threshold are known from just one nuclear resonance fluorescence (NRF) measurement, with limited precision in some cases. A recent experiment with the AGATA demonstrator array determined level lifetimes using the Doppler Shift Attenuation Method (DSAM) in 15^{15}O. As a reference and for testing the method, level lifetimes in 15^{15}N have also been determined in the same experiment. The latest compilation of 15^{15}N level properties dates back to 1991. The limited precision in some cases in the compilation calls for a new measurement in order to enable a comparison to the AGATA demonstrator data. The widths of several 15^{15}N levels have been studied with the NRF method. The solid nitrogen compounds enriched in 15^{15}N have been irradiated with bremsstrahlung. The γ\gamma-rays following the deexcitation of the excited nuclear levels were detected with four HPGe detectors. Integrated photon-scattering cross sections of ten levels below the proton emission threshold have been measured. Partial gamma-ray widths of ground-state transitions were deduced and compared to the literature. The photon scattering cross sections of two levels above the proton emission threshold, but still below other particle emission energies have also been measured, and proton resonance strengths and proton widths were deduced. Gamma and proton widths consistent with the literature values were obtained, but with greatly improved precision.Comment: Final published version, minor grammar changes, 10 pages, 4 figures, 8 tables; An addendum is published where the last section is revised: T. Sz\"ucs and P. Mohr, Phys. Rev. C 92, 044328 (2015) [arXiv:1510.04956

    A stigmatizáció hatásai HIV-vel élő meleg férfiakra Magyarországon

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    Jelen tanulmány célja, hogy mélyinterjúk kvalitatív elemzése alapján rávilágítson a – közép-kelet európai régióban és különösen a Magyarországon – HIV-vel élő embereket érintő társadalmi stigmatizációs folyamatok összetevőire és következményeire. Az általunk készített interjúkban (n=28) a HIV-vel élő emberek sajátos igényeire és gondjaira, társadalmi beágyazottságukra és intézményi támogatottságukra, megküzdési stratégiáikra, és társadalmi működésük mintázataira fókuszáltunk, különös tekintettel a társadalmi stigmatizációra. A HIV-vel élő emberek által megélt tapasztalatok elemzése hozzájárulhat a HIV/SzTB (szexuális úton terjedő betegségek) fertőzések kockázati tényezőinek jobb megértéséhez, és egyúttal ahhoz, hogy célzottabb és hatékonyabb üzeneteket tudjunk megfogalmazni mind a megelőzés területén, mind a már HIV-vel élő embereknek szóló programokban a férfiakkal szexelő férfiaknak Közép-Kelet-Európában és elsősorban Magyarországon

    Cosmic-ray induced background intercomparison with actively shielded HPGe detectors at underground locations

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    The main background above 3\,MeV for in-beam nuclear astrophysics studies with γ\gamma-ray detectors is caused by cosmic-ray induced secondaries. The two commonly used suppression methods, active and passive shielding, against this kind of background were formerly considered only as alternatives in nuclear astrophysics experiments. In this work the study of the effects of active shielding against cosmic-ray induced events at a medium deep location is performed. Background spectra were recorded with two actively shielded HPGe detectors. The experiment was located at 148\,m below the surface of the Earth in the Reiche Zeche mine in Freiberg, Germany. The results are compared to data with the same detectors at the Earth's surface, and at depths of 45\,m and 1400\,m, respectively.Comment: Minor errors corrected; final versio

    Asymptotic scattering and duality in the one-dimensional three-state quantum Potts model on a lattice

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    We determine numerically the single-particle and the two- particle spectrum of the three-state quantum Potts model on a lattice by using the density matrix renormalization group method, and extract information on the asymptotic (small momentum) S-matrix of the quasiparticles. The low energy part of the finite size spectrum can be understood in terms of a simple effective model introduced in a previous work, and is consistent with an asymptotic S-matrix of an exchange form below a momentum scale p*. This scale appears to vanish faster than the Compton scale, mc, as one approaches the critical point, suggesting that a dangerously irrelevant operator may be responsible for the behaviour observed on the lattice
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