5,673 research outputs found

    Chi-square (χ<sup>2</sup>) analysis of observed and expected ratios of the combined CF(Pa) x SF(Mx) F2 progeny from Gross <i>et al</i>. [15] and the CF(Pa) x SF(Tx) F2 progeny from O’Quin <i>et al</i>. [13] with and without scleral ossicles due to a genotypic threshold at 1–4 loci.

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    Chi-square (χ2) analysis of observed and expected ratios of the combined CF(Pa) x SF(Mx) F2 progeny from Gross et al. [15] and the CF(Pa) x SF(Tx) F2 progeny from O’Quin et al. [13] with and without scleral ossicles due to a genotypic threshold at 1–4 loci.</p

    Chi-square (χ<sup>2</sup>) analysis of observed and expected ratios of CF(Pa) x SF(Mx) F2 progeny from Gross <i>et al</i>. [15] with and without scleral ossicles due to a genotypic threshold at 1–4 loci.

    No full text
    Chi-square (χ2) analysis of observed and expected ratios of CF(Pa) x SF(Mx) F2 progeny from Gross et al. [15] with and without scleral ossicles due to a genotypic threshold at 1–4 loci.</p

    Electromagnetic annihilation rates of chi(c0) and chi(c2) with both relativistic and QCD radiative corrections

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    We estimate the electromagnetic decay rates of chi(c0)--&gt;gamma gamma and chi c(2)--&gt;gamma gamma by taking into account both relativistic and QCD radiative corrections. The decay rates are derived in the Bethe-Salpeter formalism and the QCD radiative corrections are included in accordance with the factorization assumption. Using a QCD-inspired interquark potential, we obtain relativistic BS wave functions of chi(c0) and chi(c2) by solving the BS equation for the corresponding (2S+1)L(J) states. Our numerical result for the ratio R=Gamma(chi(c0)--&gt;gamma gamma)/Gamma(chi(c2)--&gt;gamma gamma) is about 11-13, which agrees with the update E760 experiment data. Explicit calculations show that in addition to the QCD radiative corrections which may increase the ratio R by about a factor of 2, the relativistic corrections due to spin-dependent interquark forces induced by gluon exchange also enhance the ratio R substantially and its value is insensitive to the choice of parameters that characterize the interquark potential. Our expressions for the decay widths are identical with that obtained in the NRQCD theory to the next-to-leading order in upsilon(2) and alpha(s). Moreover, we have determined two new coefficients in the nonperturbative matrix elements for these decay widths.http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:A1996VA66200028&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=8e1609b174ce4e31116a60747a720701Astronomy &amp; AstrophysicsPhysics, Particles &amp; FieldsSCI(E)28ARTICLE32123-21315
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