FORMATION OF LIGHT NUCLEI IN THE EXPANDING UNIVERSE

[11] HAYAKAWA SI, COMMUNICATION

[12] PROTON-NEUTRON CONCENTRATION RATIO IN THE EXPANDING UNIVERSE AT THE STAGES PRECEDING THE FORMATION OF THE ELEMENTS [J]. PROGRESS OF THEORETICAL PHYSICS, 1950, 5 (02): : 224 - 235

[13] THE SYNTHESIS OF THE ELEMENTS FROM HYDROGEN [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1946, 106 (05) : 343 - 383

[14] Hoyle F., 1954, ASTROPHYS J SUPPL, V1, P121, DOI [10.1086/190005, DOI 10.1086/190005]

[15] ABUNDANCES OF THE ELEMENTS [J]. REVIEWS OF MODERN PHYSICS, 1956, 28 (01) : 53 - 74

[16] POPULATIONS AND EVOLUTION OF STARS [J]. PROGRESS OF THEORETICAL PHYSICS, 1956, 15 (02): : 89 - 94

[11] HAYAKAWA SI, COMMUNICATION

[12] PROTON-NEUTRON CONCENTRATION RATIO IN THE EXPANDING UNIVERSE AT THE STAGES PRECEDING THE FORMATION OF THE ELEMENTS [J]. PROGRESS OF THEORETICAL PHYSICS, 1950, 5 (02): : 224 - 235

[13] THE SYNTHESIS OF THE ELEMENTS FROM HYDROGEN [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1946, 106 (05) : 343 - 383

[14] Hoyle F., 1954, ASTROPHYS J SUPPL, V1, P121, DOI [10.1086/190005, DOI 10.1086/190005]

[15] ABUNDANCES OF THE ELEMENTS [J]. REVIEWS OF MODERN PHYSICS, 1956, 28 (01) : 53 - 74

[16] POPULATIONS AND EVOLUTION OF STARS [J]. PROGRESS OF THEORETICAL PHYSICS, 1956, 15 (02): : 89 - 94