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NSR database version of May 10, 2024.

Search: Author = F.Hoyle

Found 5 matches.

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1960FO16      Ann.Phys.(New York) 10, 280 (1960)

W.A.Fowler, F.Hoyle

Nuclear cosmochronology

RADIOACTIVITY ²³²Th, ^235,238U(α); analyzed available data. ^206,207,208Pb; deduced the age of the Galaxy, relative abundances, cosmochronometry.

doi: 10.1016/0003-4916(60)90025-7
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1957BU66      Rev.Mod.Phys. 29, 547 (1957)

E.M.Burbidge, G.R.Burbidge, W.A.Fowler, F.Hoyle

Synthesis of the elements in stars

doi: 10.1103/RevModPhys.29.547
Citations: PlumX Metrics

1953HO81      Astrophys.J.Suppl.Ser. Sup 1, 121 (1953)

F.Hoyle

On nuclear reactions occurring in very hot stars. I. The synthesis of elements from carbon to nickel

NUCLEAR REACTIONS ⁴He(α, X)⁸Be, ⁸Be(α, γ)¹²C, ^12,13C, ^14,15N, ²⁰Ne(²⁰Ne, ¹⁶O), ^16,17,18O, ²⁴Mg, ²⁸Si, ³¹P, ³⁵Cl, ³⁶Ar(α, γ), ¹²C(¹²C, X)²⁴Mg, ²³Na, ²⁷Al(p, α), ¹⁷O(γ, n), ²⁰Ne(n, γ), (γ, α), ¹²C(¹³C, α), ²²Ne(α, n), ¹⁶O, ³²S, ³⁶Ar(γ, α), ¹²C(¹⁶O, X)²⁸Si, ¹⁶(¹⁶O, X)³²S, E not given; analyzed nuclear reaction synthesis in stars; deduced isotope yields. Breit-Wigner formalism.

RADIOACTIVITY ¹⁸F, ²³Mg(β⁺), ²⁴Mg(p), (α), (n), ²⁵Mg(α), ²⁸Si, ³²S(α), (n), (d); analyzed decay from excited states. deduced isotope yields.

doi: 10.1086/190005
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1953HO82      Phys.Rev. 92, 1095 N6 (1953)

F.Hoyle, D.N.F.Dunbar, W.A.Wenzel, W.Whaling

A State in C¹² Predicted from Astrophysical Evidence

NUCLEAR REACTIONS ⁸Be(α, γ)¹²C, E not given; calculated yield for yields, resonance states.

1946HO03      Mon.not.R.Astron.Soc. 106, 343 (1946)

F.Hoyle

The synthesis of the elements from hydrogen

doi: 10.1093/mnras/106.5.343
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