3,044,815 research outputs found

    Spectroscopy of doubly charmed baryons: Ξcc+\Xi_{cc}^{+} and Ξcc++\Xi_{cc}^{++}

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    Using the quark-diquark approximation in the framework of Buchm\" uller-Tye potential model, we investigate the spectroscopy of doubly charmed baryons: Ξcc++\Xi_{cc}^{++} and Ξcc+\Xi_{cc}^{+}. Our results include the masses, parameters of radial wave functions of states with the different excitations of both diquark and light quark-diquark system. We calculate the values of fine and hyperfine splittings of these levels and discuss some new features, connected to the identity of heavy quarks, in the dynamics of hadronic and radiative transitions between the states of these baryons.Comment: 10 pages, Latex file, 1 fig, corrected some typo

    Radiative decays of the doubly charmed baryons in chiral perturbation theory

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    We have systematically investigated the spin-32\frac{3}{2} to spin-12\frac{1}{2} doubly charmed baryon transition magnetic moments to the next-to-next-to-leading order in the heavy baryon chiral perturbation theory (HBChPT). Numerical results of transition magnetic moments and decay widths are presented to the next-to-leading order: μΞcc++Ξcc++=2.35μN\mu_{\Xi_{cc}^{*++}\rightarrow\Xi_{cc}^{++}}=-2.35\mu_{N}, μΞcc+Ξcc+=1.55μN\mu_{\Xi_{cc}^{*+}\rightarrow\Xi_{cc}^{+}}=1.55\mu_{N}, μΩcc+Ωcc+=1.54μN\mu_{\Omega_{cc}^{*+}\rightarrow\Omega_{cc}^{+}}=1.54\mu_{N}, ΓΞcc++Ξcc++=22.0\Gamma_{\Xi_{cc}^{*++}\rightarrow\Xi_{cc}^{++}}=22.0 keV, ΓΞcc+Ξcc+=9.57\Gamma_{\Xi_{cc}^{*+}\rightarrow\Xi_{cc}^{+}}=9.57 keV, ΓΩcc+Ωcc+=9.45\Gamma_{\Omega_{cc}^{*+}\rightarrow\Omega_{cc}^{+}}=9.45 keV.Comment: arXiv admin note: text overlap with arXiv:1707.02765, arXiv:1706.0645

    A note on a problem in communication complexity

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    In this note, we prove a version of Tarui's Theorem in communication complexity, namely PHccBPPPccPH^{cc} \subseteq BP\cdot PP^{cc}. Consequently, every measure for PPccPP^{cc} leads to a measure for PHccPH^{cc}, subsuming a result of Linial and Shraibman that problems with high mc-rigidity lie outside the polynomial hierarchy. By slightly changing the definition of mc-rigidity (arbitrary instead of uniform distribution), it is then evident that the class MccM^{cc} of problems with low mc-rigidity equals BPPPccBP\cdot PP^{cc}. As BPPPccPSPACEccBP\cdot PP^{cc} \subseteq PSPACE^{cc}, this rules out the possibility, that had been left open, that even polynomial space is contained in MccM^{cc}

    Chondrocalcinosis is common in the absence of knee involvement

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    Introduction: We aimed to describe the distribution of radiographic chondrocalcinosis (CC) and to examine whether metacarpophalangeal joint (MCPJ) calcification and CC at other joints occurs in the absence of knee involvement. Methods: This was a cross-sectional study embedded in the Genetics of Osteoarthritis and Lifestyle study (GOAL). All participants (n = 3,170) had radiographs of the knees, hands, and pelvis. These were scored for radiographic changes of osteoarthritis (OA), for CC at knees, hips, symphysis pubis, and wrists, and for MCPJ calcification. The prevalence of MCPJ calcification and CC overall, at each joint, and in the presence or absence of knee involvement, was calculated. Results: The knee was the commonest site of CC, followed by wrists, hips, and symphysis pubis. CC was more likely to be bilateral at knees and wrists but unilateral at hips. MCPJ calcification was usually bilateral, and less common than CC at knees, hips, wrists, and symphysis pubis. Unlike that previously reported, CC commonly occurred without any knee involvement; 44.4% of wrist CC, 45.9% of hip CC, 45.5% of symphysis pubis CC, and 31.3% of MCPJ calcification occurred in patients without knee CC. Those with meniscal or hyaline articular cartilage CC had comparable ages (P = 0.21), and neither preferentially associated with fibrocartilage CC at distant joints. Conclusions: CC visualized on a plain radiograph commonly occurs at other joints in the absence of radiographic knee CC. Therefore, knee radiographs alone are an insufficient screening test for CC. This has significant implications for clinical practice, for epidemiologic and genetic studies of CC, and for the definition of OA patients with coexistent crystal deposition

    Estimate of the Hadronic Production of the Doubly Charmed Baryon Ξcc\Xi_{cc} under GM-VFN Scheme

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    Hadronic production of the doubly charmed baryon Ξcc\Xi_{cc} (Ξcc++\Xi^{++}_{cc} and Ξcc+\Xi^{+}_{cc}) is investigated under the general-mass variable-flavor-number (GM-VFN) scheme. The gluon-gluon fusion mechanism and the intrinsic charm mechanisms, i.e. via the sub-processes g+g(cc)[3S1]3ˉ+cˉ+cˉg+g\to(cc)[^3S_1]_{\bar 3}+\bar{c}+\bar{c}, g+g(cc)[1S0]6+cˉ+cˉg+g\to(cc)[^1S_0]_6+\bar{c}+\bar{c}; g+c(cc)[3S1]3ˉ+cˉg+c\to (cc)[^3S_1]_{\bar 3}+\bar{c}, g+c(cc)[1S0]6+cˉg+c\to (cc)[^1S_0]_6+\bar{c} and c+c(cc)[3S1]3ˉ+gc+c\to (cc)[^3S_1]_{\bar 3}+g, c+c(cc)[1S0]6+gc+c\to (cc)[^1S_0]_6+g, are taken into account in the investigation, where (cc)[3S1]3ˉ(cc)[^3S_1]_{\bar 3} (in color {\bf 3ˉ\bar 3}) and (cc)[1S0]6(cc)[^1S_0]_6 (in color {\bf 6}) are two possible SS-wave configurations of the doubly charmed diquark pair (cc)(cc) inside the baryon Ξcc\Xi_{cc}. Numerical results for the production at hadornic colliders LHC and TEVATRON show that both the contributions from the doubly charmed diquark pairs (cc)[1S0]6(cc)[^1S_0]_6 and (cc)[3S1]3ˉ(cc)[^3S_1]_{\bar 3} are sizable with the assumption that the two NRQCD matrix elements are equal, and the total contributions from the `intrinsic' charm mechanisms are bigger than those of the gluon-gluon fusion mechanism. For the production in the region of small transverse-momentum ptp_t, the intrinsic mechanisms are dominant over the gluon-gluon fusion mechanism and they can raise the theoretical prediction of the Ξcc\Xi_{cc} by almost one order.Comment: 26 pages, 8 figure

    Solution to the Cosmological Constant Problem in a Regge Quantum Gravity Model

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    We show that it is possible to solve the cosmological constant (CC) problem in a discrete quantum gravity theory based on Regge calculus by using the effective action approach and a special path-integral measure. The effective cosmological constant is given as a sum of 3 terms: the classical CC, the quantum gravity CC and the matter CC. Since the observations can only measure the sum of these 3 terms, we can choose the classical CC to be equal to the negative value of the matter CC. Hence the effective CC is given only by the quantum gravity CC, which is determined by the path-integral measure. Since the path-integral measure depends on a free parameter, this parameter can be chosen such that the effective CC gives the observed value.Comment: v4: published version. arXiv admin note: substantial text overlap with arXiv:1407.112
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