NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = E.Lampi Found 7 matches. 1950FR61 Phys.Rev. 78, 508 (1950) G.Freier, M.Fulk, E.E.Lampi, J.H.Williams Total Cross Section Of C, O, Mg, Si, And S For Fast Neutrons NUCLEAR REACTIONS C(n, x), O(n, x), Mg(n, x), Si(n, x), S(n, x), E=530 keV-4.8 MeV; measured products; deduced σ, σ(E). Data were imported from EXFOR entry 11294.
doi: 10.1103/PhysRev.78.508
1950LA56 Phys.Rev. 80, 853 (1950) E.E.Lampi, G.D.Freier, J.H.Williams The Total Scattering Cross Section Of Neutrons By Hydrogen And Carbon NUCLEAR REACTIONS 1H(n, x), C(n, x), E=798 keV-4.9 MeV; measured products; deduced σ, σ(E). Data were imported from EXFOR entry 12644.
doi: 10.1103/PhysRev.80.853
1949BL66 Phys.Rev. 75, 1678 (1949) J.M.Blair, G.Freier, E.E.Lampi, W.Sleator, Jr. The Scattering of Deuterons by Helium at Deuteron Energies from 0.9 to 3.5 MeV
doi: 10.1103/PhysRev.75.1678
1949FR20 Phys.Rev. 75, 1345 (1949) G.Freier, E.Lampi, W.Sleator, J.H.Williams Angular Distribution of 1- to 3.5-MeV Protons Scattered by He4
doi: 10.1103/PhysRev.75.1345
1948BL33 Phys.Rev. 74, 1594 (1948) J.M.Blair, G.Freier, E.Lampi, W.Sleator, J.H.Williams The angular distribution of 1 to 3.5 MeV deuterons scattered by deuterons NUCLEAR REACTIONS 2H(d, d), E=960 keV-3.5 MeV; measured products, 2H; deduced σ(θ). Data were imported from EXFOR entry A1217.
doi: 10.1103/PhysRev.74.1594
1948BL34 Phys.Rev. 74, 1599 (1948) J.M.Blair, G.Freier, E.Lampi, W.Sleator, J.H.Williams The angular distributions of the products of the D-D reaction : 1 to 3.5 MeV NUCLEAR REACTIONS 2H(d, n), 2H(d, p), E=960 keV-3.5 MeV; measured products, 3He, Eν, Iν; deduced σ(θ). Data were imported from EXFOR entry A1079.
doi: 10.1103/PhysRev.74.1599
1948BL35 Phys.Rev. 74, 553 (1948) J.M.Blair, G.Freier, E.Lampi, W.Sleator, Jr., J.H.Williams The scattering of 2.4 to 3.5 MeV protons by protons NUCLEAR REACTIONS 1H(p, p), E=2.4-3.5 MeV; measured products, Eπ, Iπ; deduced σ(θ). Data were imported from EXFOR entry A1117.
doi: 10.1103/PhysRev.74.553
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