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NSR database version of May 6, 2024.

Search: Author = V.I.Makhrin

Found 3 matches.

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2003BY03      Yad.Fiz. 66, 1731 (2003); Phys.Atomic Nuclei 66, 1683 (2003)

V.M.Bystritsky, V.V.Gerasimov, A.R.Krylov, S.S.Parzhitski, F.M.Penkov, O.M.Shvyryaev, V.A.Stolupin, G.N.Dudkin, B.A.Nechaev, V.M.Padalko, J.Wozniak, G.A.Mesyats, V.M.Bystritskii, V.I.Makhrin, N.A.Ratakhin

Measurement of the Astrophysical S Factor for dd Interaction at Ultralow Deuteron-Collision Energies Using the Inverse Z Pinch

NUCLEAR REACTIONS 2H(d, n), E(cm) ≈ 4 keV; measured σ; deduced astrophysical S-factor. Inverse Z pinch.

doi: 10.1134/1.1611583
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1263.

2001BY02      Yad.Fiz. 64, No 5, 920 (2001); Phys.Atomic Nuclei 64, 855 (2001)

V.M.Bystritsky, V.M.Bystritsky, S.A.Chaikovsky, M.Filipowicz, V.M.Grebenyuk, E.Gula, V.I.Makhrin, G.A.Mesyats, S.S.Parzhitsky, F.M.Penkov, N.A.Ratakhin, V.A.Sinebryukhov, S.A.Sorokin, V.A.Stolupin, E.N.Volkov, J.Wozniak

Astrophysical S Factor for dd Interaction at Ultralow Energies

NUCLEAR REACTIONS 2H(d, n), E=1.80, 2.06, 2.27 keV; measured astrophysical S-factors, σ. Linear-plasma technique.

doi: 10.1134/1.1378875
Citations: PlumX Metrics

1997BU11      Yad.Fiz. 60, No 8, 1349 (1997); Phys.Atomic Nuclei 60, 1217 (1997)

T.L.Bulgakov, V.M.Bystritsky, V.M.Bystritsky, S.A.Chaikovsky, M.Filipowicz, V.M.Grebenyuk, A.Gula, A.V.Luchinsky, V.I.Makhrin, G.A.Mesyats, S.S.Parzhitsky, N.A.Ratakhin, B.M.Sabirov, A.A.Sinebryukhov, V.A.Sinebryukhov, S.A.Sorokin, V.A.Stolupin, J.Wozniak

Measurement of the Cross Section for the Reaction d + d → 3He + n at Ultralow Collision Energies by the Z-Pinch Technique

NUCLEAR REACTIONS, ICPND 2H(d, n), E=0.44 keV; measured neutron production σ upper limit. 2H(p, γ), (d, n), (d, α), E not given; calculated σ.

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