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NSR database version of April 29, 2024.

Search: Author = G.A.Gamow

Found 30 matches.

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1968GA28      Phys.Rev.Lett. 20, 1310 (1968)

G.Gamow

Observational Properties of the Homogeneous and Isotropic Expanding Universe

doi: 10.1103/PhysRevLett.20.1310
Citations: PlumX Metrics

1967GA22      Phys.Rev.Lett. 19, 759 (1967), Erratum Phys.Rev.Lett. 19, 1000 (1967)

G.Gamow

Electricity, Gravity, and Cosmology

doi: 10.1103/PhysRevLett.19.759
Citations: PlumX Metrics

1967GA23      Phys.Rev.Lett. 19, 913 (1967)

G.Gamow

Variability of Elementary Charge and Quasistellar Objects

doi: 10.1103/PhysRevLett.19.913
Citations: PlumX Metrics

1952GA01      Phys.Rev. 86, 251 (1952)

G.Gamow

The Role of Turbulence in the Evolution of the Universe

doi: 10.1103/PhysRev.86.251
Citations: PlumX Metrics

1950GA01      Phys.Rev. 79, 743 (1950)

G.Gamow, C.Longmire

The Problem of Red Giants and Cepheid Variables

doi: 10.1103/PhysRev.79.743
Citations: PlumX Metrics

1949GA22      Rev.Mod.Phys. 21, 367 (1949)

G.Gamow

On Relativistic Cosmogony

doi: 10.1103/RevModPhys.21.367
Citations: PlumX Metrics

1948AL02      Phys.Rev. 73, 803 (1948)

R.A.Alpher, H.Bethe, G.Gamow

The Origin of Chemical Elements

doi: 10.1103/PhysRev.73.803
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1948AL03      Phys.Rev. 74, 1198 (1948), Erratum Phys.Rev. 75, 701 (1949)

R.A.Alpher, R.Herman, G.A.Gamow

Thermonuclear Reactions in the Expanding Universe

NUCLEAR REACTIONS Li, Be, B(p, X), E=2 keV; calculated elemental abundances of light elements.

doi: 10.1103/PhysRev.74.1198.2
Citations: PlumX Metrics

1947GA01      Phys.Rev. 71, 550 (1947)

G.Gamow

Probability of Nuclear Meson-Absorption

doi: 10.1103/PhysRev.71.550.2
Citations: PlumX Metrics

1946GA01      Phys.Rev. 70, 572 (1946); Erratum Phys.Rev. 71, 273 (1947)

G.Gamow

Expanding Universe and the Origin of Elements

doi: 10.1103/PhysRev.70.572.2
Citations: PlumX Metrics

1945GA01      Phys.Rev. 67, 120 (1945)

G.Gamow

The Red-Giant Stage of Stellar Evolution

doi: 10.1103/PhysRev.67.120.2
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1945GA02      Rev.Mod.Phys. 17, 125 (1945)

G.Gamow, G.Keller

A Shell Source Model for Red Giant Stars

doi: 10.1103/RevModPhys.17.125
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1944GA01      Phys.Rev. 65, 20 (1944)

G.Gamow

The Evolution of Contracting Stars

doi: 10.1103/PhysRev.65.20
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1941GA01      Phys.Rev. 59, 617 (1941)

G.Gamow

Relative Importance of Different Elements for Neutrino Production

NUCLEAR REACTIONS 1H(p, X)2H, 2H(d, n), 4He(3He, X)7Be, E<1 MeV; analyzed available data; deduced energy losses, stellar temperatures.

doi: 10.1103/PhysRev.59.617
Citations: PlumX Metrics

1941GA02      Phys.Rev. 59, 539 (1941)

G.Gamow, M.Schoenberg

Neutrino Theory of Stellar Collapse

NUCLEAR REACTIONS 3He(e-, X)3H, 56Fe(e-, X)56Mn, E not given; analyzed available data; deduced urca processes, energy loss through neutrino emissions.

doi: 10.1103/PhysRev.59.539
Citations: PlumX Metrics

1940GA01      Phys.Rev. 58, 1117 (1940)

G.Gamow, M.Schoenberg

The Possible Role of Neutrinos in Stellar Evolution

doi: 10.1103/PhysRev.58.1117
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1939GA01      Phys.Rev. 55, 654 (1939)

G.Gamow, E.Teller

On the Origin of Great Nebulae

doi: 10.1103/PhysRev.55.654
Citations: PlumX Metrics

1939GA02      Phys.Rev. 55, 796 (1939)

G.Gamow

The Evolution of Red Giants

doi: 10.1103/PhysRev.55.796.2
Citations: PlumX Metrics

1939GA03      Phys.Rev. 55, 791 (1939)

G.Gamow, E.Teller

Energy Production in Red Giants

NUCLEAR REACTIONS 2H(p, X)3He, 3H(p, X)4He, 6Li(p, X), 7Li(p, 2α), 9Be(p, 2α), 10B(p, X)11C, 11B(p, 3α), 14N(p, X)15O, E not given; calculated energy released and capture probabilities.

doi: 10.1103/PhysRev.55.791
Citations: PlumX Metrics

1939GA04      Phys.Rev. 55, 718 (1939)

G.Gamow

Physical Possibilities of Stellar Evolution

doi: 10.1103/PhysRev.55.718
Citations: PlumX Metrics

1938GA01      Phys.Rev. 53, 608 (1938)

G.Gamow, E.Teller

The Rate of Selective Thermonuclear Reactions

NUCLEAR REACTIONS 4He(α, X)8Be, 8Be(n, X)9Be, E=2-4 KeV; calculated reaction rates, resonances.

doi: 10.1103/PhysRev.53.608
Citations: PlumX Metrics

1938GA02      Phys.Rev. 53, 595 (1938)

G.Gamow

Nuclear Energy Sources and Stellar Evolution

NUCLEAR REACTIONS 2H(d, t), 4He(p, X)5Li, 4He(α, X)8Be, 8Be(n, X)9Be, 9Be(p, 2α), E not given; calculated reaction rates; deduced stellar evolution, luminosities.

doi: 10.1103/PhysRev.53.595
Citations: PlumX Metrics

1938GA03      Phys.Rev. 53, 907 (1938)

G.Gamow

Tracks of Stellar Evolution

doi: 10.1103/PhysRev.53.907
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1938GA04      Phys.Rev. 54, 480 (1938)

G.Gamow

Tentative Theory of Novae

doi: 10.1103/PhysRev.54.480
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1937GA01      Phys.Rev. 51, 289 (1937)

G.Gamow, E.Teller

Some Generalizations of the β Transformation Theory

RADIOACTIVITY 1H(β+), 1NN(β-); analyzed available data; deduced emission probabilities for electrons/positrons and neutrinos.

doi: 10.1103/PhysRev.51.289
Citations: PlumX Metrics

1936BL02      Phys.Rev. 50, 260 (1936)

F.Bloch, G.Gamow

On the Probability of γ-Ray Emission

doi: 10.1103/PhysRev.50.260
Citations: PlumX Metrics

1936GA02      Phys.Rev. 49, 946 (1936)

G.Gamow

Possibility of Selective Phenomena for Fast Neutrons

RADIOACTIVITY 31P, 29Si(p), 28Al(β-) [from 27Al(α, X)31P, 25Mg(α, X)29Si, 28Si(n, X)29Si, E not given]; analyzed available data; deduced discrete groups of protons emitted, resonances, binding energies.

doi: 10.1103/PhysRev.49.946
Citations: PlumX Metrics

1936GA03      Phys.Rev. 49, 895 (1936)

G.Gamow, E.Teller

Selection Rules for the β-Disintegration

RADIOACTIVITY 212Bi, 212Pb(β-); analyzed available data; deduced selection rules.

doi: 10.1103/PhysRev.49.895
Citations: PlumX Metrics

1934GA01      Phys.Rev. 45, 728 (1934)

G.Gamow

Negative Protons and Nuclear Structure

NUCLEAR STRUCTURE 1H; analyzed available data; deduced possible existence of antiprotons.

doi: 10.1103/PhysRev.45.728
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1928GA01      Z.Phys. 51, 204 (1928)

G.Gamow

Zur Quantentheorie des Atomkernes

RADIOACTIVITY Rn, Ra, U(α); calculated α decay constant λ; deduced quantum mechanics tunneling effect.

doi: 10.1007/BF01343196
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Note: The following list of authors and aliases matches the search parameter G.A.Gamow: , G.A.GAMOW