채경육 교수

Introduction 1. Carmaux, 1850-1890 2. The Craft of the Glassworker 3. Glassworkers and Miners: A Contrast 4. Mechanization 5. Socialism 6. The Strike of 1895 7. New Glassworkers and Old, 1896-1914 Epilogue: Three Portraits Appendix Bibliography Notes Index

We present the first comprehensive geochemical data (major elements and 31 trace elements by XRF and INAA) for the metamorphic cordierite-orthoamphibole (anthophyllite-gedrite) rocks (COR) that occur in the Early Proterozoic (~1.85 Ga) Svecofennian supracrustal rocks at Orijärvi, Finland, (eight samples) and associated cummingtonite-biotite-plagioclase gneisses five samples). COR (57.3-76.9 wt % SiO₂) are distinguished from (50.4-61.7 wt % SiO₂) by lower Sc, Cr, and Co, and by higher Zr, Hf, Nb,

The $^{18}\mathrm{Ne}(\ensuremath{\alpha},p)^{21}\mathrm{Na}$ reaction plays a crucial role in the $(\ensuremath{\alpha},p)$ process, which leads to the rapid proton capture process in x-ray bursts. The reaction rate depends upon properties of $^{22}\mathrm{Mg}$ levels above the $\ensuremath{\alpha}$ threshold at 8.14 MeV. Despite recent studies of these levels, only the excitation energies are known for most with no constraints on the spins. We have studied the $^{24}\mathrm{Mg}(p,t)^{22}\mathr

The interference effects among ${J}^{\ensuremath{\pi}}=3/{2}^{+}$ resonances in the $^{18}\mathrm{F}+p$ system have not been previously measured. $R$-matrix calculations show that the cross sections above the ${E}_{c.m.}=665$ keV resonance are sensitive to the interference between the ${E}_{c.m.}=8$, 38, and 665 keV resonances. An excitation function for the $^{1}\mathrm{H}$($^{18}\mathrm{F}$,\ensuremath{\alpha})$^{15}\mathrm{O}$ reaction has been measured in the energy range of ${E}_{c.m.}=663\

Michael S. Smith, Free Trade versus Protection in the Early Third Republic: Economic Interests, Tariff Policy, and the Making of the Republican Synthesis, French Historical Studies, Vol. 10, No. 2 (Autumn, 1977), pp. 293-314

The level structure of $^{22}\mathrm{Na}$ has been studied at the Holifield Radioactive Ion Beam Facility in Oak Ridge National Laboratory using the $^{24}\mathrm{Mg}$($p$,$^{3}\mathrm{He}$)$^{22}\mathrm{Na}$ reaction. Proton beams of 41 and 41.5 MeV were generated by the 25-MV tandem accelerator and bombarded isotopically enriched $^{24}\mathrm{Mg}$ targets. Angular distributions of recoiling $^{3}\mathrm{He}$ particles were extracted by using a segmented annular silicon strip detector array. S

A Computational Infrastructure for Nuclear Astrophysics has been developed to streamline the inclusion of the latest nuclear physics data in astrophysics simulations. The infrastructure consists of a platform‐independent suite of computer codes that is freely available online at nucastrodata.org. Features of, and future plans for, this software suite are given.

Knowledge of the 3He(3He,2p)4He reaction is important for understanding stellar burning and solar neutrino production. Previous measurements have found a surprisingly large rise in the cross section at low energies that could be due to a low-energy resonance in the 3He + 3He (6Be) system or electron screening. In the 6Be nucleus, however, no excited states have been observed above the first 2+ state at E x = 1.67 MeV up to 23 MeV, even though several are expected. The 2H(7Be,3H)6Be reaction has