Zobrazeno 1 - 10
of 47
pro vyhledávání: '"Y, Kashiv"'
Autor:
Lauren K. Callahan, P. Collon, M. Paul, M.L. Avila, B.B. Back, T.L. Bailey, A.M. Clark, C. Dickerson, J.P. Greene, H. Jayatissa, C.L. Jiang, Y. Kashiv, A.D. Nelson, J. McLain, R.C. Pardo, D. Potterveld, K.E. Rehm, R.N. Sahoo, R. Scott, D. Seweryniak, I. Tolstukhin, R. Vondrasek
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms. 532:7-12
Autor:
N. Kinoshita, M. Paul, Y. Kashiv, P. Collon, C. M. Deibel, B. DiGiovine, J. P. Greene, C. L. Jiang, S. T. Marley, R. C. Pardo, K. E. Rehm, D. Robertson, R. Scott, C. Schmitt, X. D. Tang, R. Vondrasek, A. Yokoyama
Publikováno v:
Science. 379:1307-1307
Publikováno v:
Physical Review C. 105
Publikováno v:
Physical Review C
Autor:
R. N. Sahoo, M. Paul, U. Köster, R. Scott, M. Tessler, A. Zylstra, M. L. Avila, C. Dickerson, H. Jayatissa, M.S. Kohen, J. McLain, R.C. Pardo, K. E. Rehm, I. Tolstukhin, R. Vondrasek, T. Bailey, L. Callahan, A. Clark, P. Collon, Y. Kashiv, A. Nelson
Publikováno v:
EPJ Web of Conferences. 284:01037
The cross-section of the thermal neutron capture 41Ar(n,γ)42Ar(t1/2=32.9 y) reaction was measured by irradiating a 40Ar sample at the high-flux reactor of Institut Laue-Langevin (ILL) Grenoble, France. The signature of the two-neutron capture has be
Autor:
M. Paul, R. N. Sahoo, M. Tessler, J. Jeet, C. Velsko, A. Zylstra, M. Avila, C. Dickerson, C. Fougères, H. Jayatissa, R. C. Pardo, K. E. Rehm, R. Scott, I. Tolstukhin, R. Vondrasek, T. Bailey, L. Callahan, A. M. Clark, P. Collon, Y. Kashiv, A. Nelson, U. Köster, H. F. R. Hoffmann, M. Pichotta, K. Zuber, T. Döring, R. Schwengner
Publikováno v:
EPJ Web of Conferences. 279:13004
The thermodynamical conditions and the neutron density produced in a laser-induced implosion of a deuterium-tritium (DT) filled capsule at the National Ignition Facility (NIF) are the closest laboratory analog of stellar conditions. We plan to invest
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Stellar ^{36,38}Ar(n,γ)^{37,39}Ar Reactions and Their Effect on Light Neutron-Rich Nuclide Synthesis
Autor:
M, Tessler, M, Paul, S, Halfon, B S, Meyer, R, Pardo, R, Purtschert, K E, Rehm, R, Scott, M, Weigand, L, Weissman, S, Almaraz-Calderon, M L, Avila, D, Baggenstos, P, Collon, N, Hazenshprung, Y, Kashiv, D, Kijel, A, Kreisel, R, Reifarth, D, Santiago-Gonzalez, A, Shor, I, Silverman, R, Talwar, D, Veltum, R, Vondrasek
Publikováno v:
Physical review letters. 121(11)
The ^{36}Ar(n,γ)^{37}Ar (t_{1/2}=35 d) and ^{38}Ar(n,γ)^{39}Ar (269 yr) reactions were studied for the first time with a quasi-Maxwellian (kT∼47 keV) neutron flux for Maxwellian average cross section (MACS) measurements at stellar energies. Gas s
Autor:
Robert N. Clayton, Andrew M. Davis, Z. Cai, Y. Kashiv, Stephen R. Sutton, Barry Lai, R. Gallino
Publikováno v:
The Astrophysical Journal. 713:212-219
Synchrotron X-ray fluorescence was used in this study for the first time to measure trace element abundances in single presolar grains. The abundances of Zr and Nb were determined in SiC grains of the KJF size-separate. These grains are most likely f
Publikováno v:
International Journal of Modern Physics E. 19:131-140
Evidence for the possible existence of a superheavy nucleus with atomic mass number A = 292 and abundance of about 1×10-12 relative to 232 Th has been found in a study of natural Th using inductively coupled plasma-sector field mass spectrometry. Th