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NSR database version of May 10, 2024.

Search: Author = T.A.Krylovetskaya

Found 5 matches.

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2000KO68      Bull.Rus.Acad.Sci.Phys. 64, 747 (2000)

I.V.Kopytin, T.A.Krylovetskaya

Photobeta Decay of the Stable Nucleus as a Basis of a New p-Nucleus Synthesis Model

NUCLEAR REACTIONS ⁷⁴Ge, ⁸⁰Se, ¹⁰⁸Pd, ^112,114Cd, ^130,132Xe, ¹³⁶Ba, ¹⁶⁴Dy, ¹⁸⁰Hf, ¹⁹⁶Pt(γ, e), E not given; calculated reaction rate as a function of stellar temperature and reaction threshold. Origin of neutron-deficient stable isotopes discussed.

RADIOACTIVITY ⁷⁴As, ⁸⁰Br, ¹⁰⁸Ag, ^112,114In, ^130,132Cs, ¹³⁶La, ¹⁶⁴Ho, ¹⁸⁰Ta, ¹⁹⁶Au(β^-); calculated decay probability for the ground and excited states following (γ, e) reactions in stellar environments. Origin of neutron-deficient stable isotopes discussed.

1999KO45      Bull.Rus.Acad.Sci.Phys. 63, 26 (1999)

I.V.Kopytin, T.A.Krylovetskaya, T.A.Churakova

Neutron-Induced Collisional β Decay of Stable Nuclei

NUCLEAR REACTIONS ¹⁰⁸Pd(n, X), E(cm)=3-20 MeV; calculated collision-induced β decay σ.

1998KO46      Yad.Fiz. 61, No 9, 1589 (1998); Phys.Atomic Nuclei 61, 1479 (1998)

I.V.Kopytin, T.A.Krylovetskaya

Collision-Induced Beta Decay of Nuclei in a Coulomb Field and Origin of By-Passed Isotopes

NUCLEAR REACTIONS ⁹⁶Mo(p, p'), (α, α'), (⁷Li, ⁷Li'), (¹⁶O, ¹⁶O'), ⁸⁰Se(p, p'), (²⁸Si, ²⁸Si'), (⁵⁶Fe, ⁵⁶Fe'), ¹¹⁴Cd, ¹⁹⁰Os(p, p'), (e, e'), E(cm) < 50 MeV; calculated collision-induced β decay σ; deduced stellar nucleosynthesis implications.

1998KO51      Bull.Rus.Acad.Sci.Phys. 62, 46 (1998)

I.V.Kopytin, T.A.Krylovetskaya

Model of Synthesis of By-Passed Nuclei in Star Matter

1996KO40      Bull.Rus.Acad.Sci.Phys. 60, 147 (1996)

I.V.Kopytin, M.A.Dolgopolov, T.A.Krylovetskaya

New Mechanism for Nucleosynthesis of By-Passed Nuclei

NUCLEAR STRUCTURE A=74-184; calculated by-passed nuclei relative abundance. Collisional β-decay based mechanism.