Zobrazeno 1 - 10
of 88
pro vyhledávání: '"S. Almaraz-Calderon"'
Autor:
A.D. Ayangeakaa, R.V.F. Janssens, C.Y. Wu, J.M. Allmond, J.L. Wood, S. Zhu, M. Albers, S. Almaraz-Calderon, B. Bucher, M.P. Carpenter, C.J. Chiara, D. Cline, H.L. Crawford, H.M. David, J. Harker, A.B. Hayes, C.R. Hoffman, B.P. Kay, K. Kolos, A. Korichi, T. Lauritsen, A.O. Macchiavelli, A. Richard, D. Seweryniak, A. Wiens
Publikováno v:
Physics Letters B, Vol 754, Iss C, Pp 254-259 (2016)
The quadrupole collectivity of low-lying states and the anomalous behavior of the 02+ and 23+ levels in 72Ge are investigated via projectile multi-step Coulomb excitation with GRETINA and CHICO-2. A total of forty six E2 and M1 matrix elements connec
Externí odkaz:
https://doaj.org/article/e1c433f5a4634caba7dde0dbaf5fbb43
Autor:
E. Lopez-Saavedra, S. Almaraz-Calderon, B. W. Asher, L. T. Baby, N. Gerken, K. Hanselman, K. W. Kemper, A. N. Kuchera, A. B. Morelock, J. F. Perello, E. S. Temanson, A. Volya, I. Wiedenhöver
Publikováno v:
Physical Review Letters. 129
Autor:
T. L. Tang, C. R. Hoffman, B. P. Kay, I. A. Tolstukhin, S. Almaraz-Calderon, B. W. Asher, M. L. Avila, Y. Ayyad, K. W. Brown, D. Bazin, J. Chen, K. A. Chipps, P. A. Copp, M. Hall, H. Jayatissa, H. J. Ong, D. Santiago-Gonzalez, D. K. Sharp, J. Song, S. Stolze, G. L. Wilson, J. Wu
Publikováno v:
Physical Review C. 105
Autor:
G. Lotay, D. T. Doherty, R. V. F. Janssens, D. Seweryniak, H. M. Albers, S. Almaraz-Calderon, M. P. Carpenter, A. E. Champagne, C. J. Chiara, C. R. Hoffman, C. Iliadis, A. Kankainen, T. Lauritsen, S. Zhu
Publikováno v:
Physical Review C. 105
Autor:
J. F. Perello, S. Almaraz-Calderon, B. W. Asher, L. T. Baby, C. Benetti, K. W. Kemper, E. Lopez-Saavedra, G. W. McCann, A. B. Morelock, V. Tripathi, I. Wiedenhöver, B. Sudarsan
Publikováno v:
Physical Review C. 105
Autor:
E, Lopez-Saavedra, S, Almaraz-Calderon, B W, Asher, L T, Baby, N, Gerken, K, Hanselman, K W, Kemper, A N, Kuchera, A B, Morelock, J F, Perello, E S, Temanson, A, Volya, I, Wiedenhöver
Publikováno v:
Physical review letters. 129(1)
A near-threshold proton resonance in ^{11}B at E_{ex}=11.44±0.04 MeV is observed via the reaction ^{10}Be(d,n)^{11}Be→^{10}Be+p in inverse kinematics, measured with a beam of the radioactive isotope ^{10}Be. The resonance energy at E_{res}=211(40)
Autor:
N. Gerken, S. Almaraz-Calderon, B. W. Asher, E. Lopez-Saveedra, L. T. Baby, K. W. Kemper, A. Morelock, J. F. Perello, A. Volya, I. Wiedenhöver
Publikováno v:
Physical Review C. 104
Autor:
A.B. Morelock, J.F. Perello, S. Almaraz-Calderon, B.W. Asher, K. Brandenburg, J. Derkin, G. Hamad, Y. Jones-Alberty, E. Lopez Saavedra, T. Massey, Z. Meisel, N. Singh, D. Soltesz, S.K. Subedi, A. Voinov, J. Warren
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 1034:166759
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:
S, Almaraz-Calderon, K E, Rehm, N, Gerken, M L, Avila, B P, Kay, R, Talwar, A D, Ayangeakaa, S, Bottoni, A A, Chen, C M, Deibel, C, Dickerson, K, Hanselman, C R, Hoffman, C L, Jiang, S A, Kuvin, O, Nusair, R C, Pardo, D, Santiago-Gonzalez, J, Sethi, C, Ugalde
Publikováno v:
Physical review letters. 119(7)
The existence of ^{26}Al (t_{1/2}=7.17×10^{5} yr) in the interstellar medium provides a direct confirmation of ongoing nucleosynthesis in the Galaxy. The presence of a low-lying 0^{+} isomer (^{26}Al^{m}), however, severely complicates the astrophys