NSR Query Results
Output year order : Descending NSR database version of April 26, 2024. Search: Author = L.Kazakov Found 20 matches. 2007RO09 At.Energ. 101, 441 (2007); At.Energy 101, 897 (2007) V.A.Roshchenko, V.M.Piksaikin, L.E.Kazakov, G.G.Korolev Relative yield of delayed neutrons and half-life of their precursor nuclei with fissioning of 239Pu by 14.2-17.9 MeV neutrons NUCLEAR REACTIONS 239Pu(n, F), E=14.2-17.9 MeV; measured delayed neutron yields; deduced precursor nuclei average T1/2.
doi: 10.1007/s10512-006-0188-z
2006WI02 Phys.Rev. C 73, 015807 (2006) K.Wisshak, F.Voss, F.Kappeler, L.Kazakov Stellar neutron capture cross sections of the Lu isotopes NUCLEAR REACTIONS 175,176Lu(n, γ), E=3-225 keV; measured Eγ, capture σ; deduced Maxwellian averaged σ. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.73.015807
2006WI11 Phys.Rev. C 73, 045807 (2006) K.Wisshak, F.Voss, F.Kappeler, L.Kazakov, F.Becvar, M.Krticka, R.Gallino, M.Pignatari Fast neutron capture on the Hf isotopes: Cross sections, isomer production, and stellar aspects NUCLEAR REACTIONS 176,177,178,179,180Hf(n, γ), E=3-225 keV; measured Eγ, Iγ, capture σ; deduced Maxwellian-averaged σ. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.73.045807
2002IS13 Prog.Nucl.Energy 41, 117 (2002) S.G.Isaev, V.M.Piksaikin, L.E.Kazakov, V.A.Roshchenko Delayed Neutrons as a Probe of Nuclear Charge Distribution in Fission of Heavy Nuclei by Neutrons NUCLEAR REACTIONS 235U(n, F)87Br/88Br/89Br/91Br/137I/138I/139I/140I, E=thermal; measured delayed neutron yields; deduced fission product cumulative yields, most probable charge vs mass.
doi: 10.1016/S0149-1970(02)00008-2
2002PI18 At.Energ. 92, 135 (2002); At.Energy 92, 147 (2002) V.M.Piksaikin, L.E.Kazakov, G.G.Korolev, S.G.Isaev, V.A.Roshchenko, M.Z.Tarasko Relative Yield and Period of Individual Groups of Delayed Neutrons in 233U, 235U, and 239Pu Fission by Epithermal Neutrons NUCLEAR REACTIONS 233,235U, 239Pu(n, F), E ≈ 0-2 MeV; measured delayed neutron yields; deduced group parameters. Comparison with previous results.
doi: 10.1023/A:1015878706836
2002PI20 Prog.Nucl.Energy 41, 135 (2002) V.M.Piksaikin, L.E.Kazakov, V.A.Roshchenko, S.G.Isaev, G.G.Korolev, A.A.Goverdovski, R.G.Tertytchnyi Experimental Studies of the Absolute Total Delayed Neutron Yields from Neutron Induced Fission of 238U in the Energy Range 1-5 MeV NUCLEAR REACTIONS 238U(n, F), E=1-5 MeV; measured delayed neutron yields.
doi: 10.1016/S0149-1970(02)00010-0
2002PI21 Prog.Nucl.Energy 41, 203 (2002) V.M.Piksaikin, L.E.Kazakov, S.G.Isaev, M.Z.Tarasko, V.A.Roshchenko, R.G.Tertytchnyi, G.D.Spriggs, J.M.Campbell Energy Dependence of Relative Abundances and Periods of Delayed Neutrons from Neutron-Induced Fission of 235U, 238U, 239Pu in 6- and 8-Group Model Representation NUCLEAR REACTIONS 235U, 239Pu(n, F), E=thermal-5 MeV; 238U(n, F), E=1-5 MeV; measured delayed neutron yields; deduced group parameters.
doi: 10.1016/S0149-1970(02)00012-4
2002PI23 At.Energ. 92, 233 (2002); At.Energy 92, 254 (2002) V.M.Piksaikin, L.E.Kazakov, C.T.Isaev, G.G.Korolev, V.A.Roshchenko, R.G.Tertytchnyi Energy dependence of the relative yield and period of individual groups of delayed neutrons in 239Pu fission in primary-neutron energy range 0.37-4.97 MeV NUCLEAR REACTIONS 239Pu(n, F), E ≈ 0.4-5 MeV; measured delayed neutron yields, precursor average T1/2; deduced group parameters.
doi: 10.1023/A:1016050131272
2002WI11 Phys.Rev. C66, 025801 (2002) K.Wisshak, F.Voss, F.Kappeler, L.Kazakov Neutron capture cross sections for stellar Cd production NUCLEAR REACTIONS 110,111,112,113,114,116Cd(n, γ), E=3-225 keV; measured capture σ; deduced Maxwellian averaged σ. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.66.025801
2000WI08 Phys.Rev. C61, 065801 (2000) K.Wisshak, F.Voss, C.Arlandini, F.Kappeler, L.Kazakov Stellar Neutron Capture Cross Sections of the Yb Isotopes NUCLEAR REACTIONS 170,171,172,173,174,176Yb(n, γ), (n, X), E=3-225 keV; measured total, capture σ, isomer ratios; deduced Maxwellian averaged σ. Implications for stellar nucleosynthesis discussed.
doi: 10.1103/PhysRevC.61.065801
1999PI14 Yad.Fiz. 62, No 8, 1358 (1999); Phys.Atomic Nuclei 62, 1279 (1999) V.M.Piksaikin, S.G.Isaev, L.E.Kazakov, G.G.Korolev, B.D.Kuzminov, V.G.Pronyaev Features of the Energy Dependence of the Total Yields of Delayed Neutrons from 235U and 237Np Fission Induced by Fast Neutrons NUCLEAR REACTIONS 235U, 237Np(n, F), E=0.7-5.0 MeV; measured delayed neutron yields; deduced energy dependence.
1999VO02 Phys.Rev. C59, 1154 (1999) F.Voss, K.Wisshak, C.Arlandini, F.Kappeler, L.Kazakov, T.Rauscher Stellar Neutron Capture Cross Sections of Pr and Dy Isotopes NUCLEAR REACTIONS 141Pr, 160,161,162,163,164Dy(n, γ), E=3-225 keV; measured total, capture σ; deduced Maxwellian averaged neutron capture σ at stellar energies. Astrophysical implications discussed.
doi: 10.1103/PhysRevC.59.1154
1998PI12 At.Energ. 85, 51 (1998); At.Energy 85, 479 (1998) V.M.Piksaikin, Yu.F.Balakshev, S.G.Isaev, L.E.Kazakov, G.G.Korolev, V.I.Milshin Measurement of the Energy Dependence of the Parameters of Delayed Neutrons Accompanying Fission of 237Np by Fast Neutrons NUCLEAR REACTIONS 237Np(n, F), E=fast; measured delayed neutrons intensity vs time, energy; deduced parameters. Data from this article have been entered in the EXFOR database. For more information, access X4 dataset41322. 1998WI04 Phys.Rev. C57, 391 (1998) K.Wisshak, F.Voss, F.Kappeler, L.Kazakov, G.Reffo Stellar Neutron Capture Cross Sections of the Nd Isotopes NUCLEAR REACTIONS 142,143,144,145,146Nd(n, γ), E=3-225 keV; measured total, capture σ(En); deduced Maxwellian averaged σ at kT=10-100 keV, astrophysical s-process implications.
doi: 10.1103/PhysRevC.57.391
1997WI13 Nucl.Phys. A621, 270c (1997) K.Wisshak, F.Voss, F.Kappeler, L.Kazakov Neutron Capture in Neodymium Isotopes: Implications for the s-process NUCLEAR REACTIONS 142,143,144,145,146,148Nd(n, γ), E=10, 30 keV; measured capture σ. Other data compared, astrophysical s-process implications.
doi: 10.1016/S0375-9474(97)00253-4
1996WI14 Phys.Rev. C54, 1451 (1996) K.Wisshak, F.Voss, Ch.Theis, F.Kappeler, K.Guber, L.Kazakov, N.Kornilov, G.Reffo Stellar Neutron Capture Cross Sections of the Tin Isotopes NUCLEAR REACTIONS 114,115,116,117,118,120Sn(n, γ), E=3-225 keV; measured capture σ(E); deduced Maxwellian averaged σ for stellar temperatures kT=10 to 100 keV.
doi: 10.1103/PhysRevC.54.1451
1995WI25 Phys.Rev. C52, 2762 (1995) K.Wisshak, F.Voss, F.Kappeler, K.Guber, L.Kazakov, N.Kornilov, M.Uhl, G.Reffo Stellar Neutron Capture Cross Sections of the Gd Isotopes NUCLEAR REACTIONS 152,154,155,156,157,158Gd(n, γ), E=3-225 KeV; measured σ(E); deduced Maxwellian averaged cross section for kT=10 to 100 keV.
doi: 10.1103/PhysRevC.52.2762
1989TI03 Yad.Fiz. 50, 609 (1989) V.M.Timokhov, M.V.Bokhovko, A.G.Isakov, L.E.Kazakov, V.N.Kononov, G.N.Manturov, E.D.Poletaev, V.G.Pronyaev Neutron Capture, Total Cross Sections and Average Resonance Parameters for Tin Isotopes NUCLEAR REACTIONS 112,114,115,116,117,118,119,120,122,124Sn(n, γ), E=20-450 keV; measured capture σ(E). 112,114,115,116,117,118,119,120,122,124Sn(n, X), E=20-1400 keV; measured total σ(E); deduced s-, p-wave potential scattering radii, model parameters. 113,115,116,117,118,119,121,122,123,125Sn deduced s-, p-wave, γ-strength functions. Data from this article have been entered in the EXFOR database. For more information, access X4 dataset40960. 1988KA26 At.Energ. 64, 152 (1988) L.E.Kazakov, V.N.Kononov, G.N.Manturov, E.D.Poletaev Radiative-Capture Cross Sections and Neutron Transmissions for 236U in the Region of Forbidden Resonances NUCLEAR REACTIONS 236U(n, γ), E=6-420 keV; measured radiative capture σ(E). 236U(n, X), E < 1 MeV; measured transmission; deduced σ(E). Other data input. Data from this article have been entered in the EXFOR database. For more information, access X4 dataset40890. 1985KO16 Nucl.Instrum.Methods 236, 361 (1985) V.N.Kononov, E.D.Poletaev, M.V.Bohovko, L.E.Kazakov, V.M.Timokhov, P.P.Dyachenko, L.S.Kutsaeva, E.A.Seregina, A.Lajtai, J.Kecskemeti Neutron Detection Efficiency of a Thick Lithium Glass Detector NUCLEAR REACTIONS 16O(n, n'γ), E=25-2000 keV; measured neutron detection efficiency. 16O deduced resonance effect. Thick NE-912 lithium glass scintillator.
doi: 10.1016/0168-9002(85)90929-5
Back to query form Note: The following list of authors and aliases matches the search parameter L.Kazakov: , L.E.KAZAKOV |