48,198 research outputs found

    Silver-Mediated Direct sp(3) C-H Bond Functionalization

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    Direct sp(3) C-H bond functionalization is an efficient, straightforward, and powerful method to construct new C-X (X = C, N, F, S) bonds from nonfunctionalized aliphatic motif of organic molecules, which has been used in late-stage modification of complex molecules. In this chapter, the recent developments of silver-mediated direct sp(3) C-H functionalizations are reviewed, categorized by C-C bond formation (C-H insertion), C-N bond formation (intramolecular and intermolecular amination/amidation), C-F bond formation, and C-S bond formation.SCI(E)[email protected]

    Letter from C. H. Gensler, Havasupai Agency to Carl Hayden

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    Letter from C. H. Gensler expressing concern on behalf of the Havasupai Tribe regarding the proposed park boundaries

    Letter from Carl Hayden to C. H. Gensler

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    Letter from Carl Hayden to C. H. Gensler informing him of the proposed Grand Canyon National Park bill

    Letter from C. H. Gensler, Havasupai Agency to Carl Hayden

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    Letter from C. H. Gensler to Carl Hayden asking for a meeting in regards to the Havasupai pasture land in light of the national park bill

    Letter from Carl T. Hayden to C. H. Gensler, Havasupai Reservation

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    Letter from Carl T. Hayden to C. H. Gensler, Havasupai Indian Reservation, regarding Hualapai and Cataract Canyons geography

    Citations of the author H C Rajpoot

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    The list of the articles, research papers, theses, and book chapters globally citing the author H. C. Rajpoot</p

    Measurement of the ratio of prompt χ c to J / ψ production in pp collisions at √s = 7 TeV

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    The prompt production of charmonium χ c and J / ψ states is studied in proton-proton collisions at a centre-of-mass energy of √s = 7 TeV at the Large Hadron Collider. The χ c and J / ψ mesons are identified through their decays χ c → J / ψ γ and J / ψ → μ + μ - using 36 pb - 1 of data collected by the LHCb detector in 2010. The ratio of the prompt production cross-sections for χ c and J / ψ, σ (χ c → J / ψ γ) / σ (J / ψ), is determined as a function of the J / ψ transverse momentum in the range 2 < p T J / ψ < 15 GeV / c. The results are in excellent agreement with next-to-leading order non-relativistic expectations and show a significant discrepancy compared with the colour singlet model prediction at leading order, especially in the low p T J / ψ region

    VIBRATIONALLY EXCITED C6_6H

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    Author Institution: Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138; Division of Engineering and Applied Sciences, Harvard University, 29 Oxford Street, Cambridge, MA 02138.Following the detection of the linear carbon chain radical C6_6H in space, many rotational lines in the X2ΠX^2\Pi electronic ground state have been observed in a low pressure discharge at millimeter wavelengths} \underline{\textbf{197}}, 1 (1999).} and in a supersonic molecular beam at centimeter wavelengths} \underline{\textbf{122}}, 174308 (2005).}. In the course of a laboratory search for new reactive hydrocarbon molecules with 6 carbon atoms, several series of harmonically related lines with rotational constants near that of C6_6H in the ground vibrational state were observed in the millimeter-wave band. On the basis of the close agreement in rotational constants and intensities, two of the series were assigned to 2Σ^2\Sigma and 2Δ^2\Delta states of a low-lying excited bending vibrational level of C6_6H. The standard Hamiltonian with five spectroscopic constants reproduces the observed rotational spectrum of the 2Δ^2\Delta state, but several high-order distortion terms in the spin-rotation interaction are needed to reproduce the spectrum of the 2Σ^2\Sigma state of C6_6H and C6_6D. From the measured intensities of the rotational lines it appears that the 2Σ^2\Sigma state lies very close to ground but the 2Δ^2\Delta state lies much higher in energy. A brief summary of the laboratory spectrum and applications to the astronomical observations will be presented

    MICROWAVE SPECTROSCOPY OF TWO ISOELECTRONIC RADICALS: 2,4,6-HEPTATRIYNYL, H2CCCCCCCHH_{2}C-C\equiv C-C\equiv C-C\equiv C-H, AND 2,4-HEXADIYNYLNITRILE, H2CCCCCCNH_{2}C-C\equiv C-C\equiv C-C\equiv N

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    Author Institution: Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138; Division of Engineering and Applied Sciences, Harvard, Cambridge, MA; Department of Chemistry, Wesleyan University, Middletown, CTThe isoelectronic pair of radicals 2,4,6-heptatriynyl, H2CCCCCCCHH_{2}C-C\equiv C-C\equiv C-C\equiv C-H, and 2,4-hexadiynylnitrile, H2CCCCCCNH_{2}C-C\equiv C-C\equiv C-C\equiv N, were produced in a pulsed discharge supersonic jet and detected by Fourier transform microwave spectroscopy. Seven rotational transitions of the heptatriynyl radical from N=4N^{\prime} = 4 to 10 and six rotational transitions of the hexadiynyl-nitrile radical from N=4N^{\prime} = 4 to 9 in the Ka=0K_{a} = 0 ladder were observed between 6 and 17 GHz. For each species, over 50 hyperline components were measured and assigned with an uncertainty of 5 kHz. Precise rotational, centrifugal distortion, spin-rotation, and various hyperfine coupling constants were determined for both H2C7HH_{2}C_{7}H and H2C6NH_{2}C_{6}N

    AN EXHAUSTIVE ISOTOPIC STUDY OF THE ABUNDANT ASTRONOMICAL MOLECULE CYCLOPROPENYLIDENE, c-C3_3H2_2

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    Author Institution: Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA 02138, and School of Engineering \&amp; Applied Sciences, Harvard University, 29 Oxford St., Cambridge, MA 02138Cyclopropenylidene, c-C3_3H2_2, is the most widely distributed ring in our galaxy; it has been detected in more than 50 astronomical sources, and its isotopic species c-C3_3HD has been observed towards several dense cores in cold dark clouds. Because of the high observed abundance and large deuterium fractionation for this small hydrocarbon ring, other isotopic species of c-C3_3H2_2 may be good candidates for astronomical detection. For these reasons, an exhaustive isotopic study of c-C3_3H2_2 has now been undertaken in which rotational spectra of c-C3_3D2_2, c-C3_3HD, and the carbon--13 isotopic species of c-C3_3HD and c-C3_3H2_2 have been detected in the centimeter-wave band by Fourier transform microwave (FTM) spectroscopy between 10 and 40~GHz. For c-C3_3D2_2, millimeter- and submillimeter-wave spectra were subsequently measured between 140 and 400~GHz. Rotational and centrifugal distortion constants derived either from previous measurements or those predicted from theory are compared with the precise constants determined here. % ######################################################################
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