Energy production in stars

[1] A precise measurement of the mass difference Be-4(9)-Be-4(8); The stability of Be-4(8) [J]. PHYSICAL REVIEW, 1939, 55 (01): : 0107 - 0107

[2] On the question of the possibility of building elements in stars [J]. ZEITSCHRIFT FUR PHYSIK, 1929, 54 (9-10): : 656 - 665

[3] Evidence against He-5 [J]. PHYSICAL REVIEW, 1935, 48 (04): : 382 - 382

[4] BAINBRIDGE KT, 1938, PHYS REV, V53, pA922

[5] The neutrino [J]. NATURE, 1934, 133 : 689 - 690

[6] Coulomb energy of light nuclei [J]. PHYSICAL REVIEW, 1938, 54 (06): : 436 - 439

[7] The formation of deuterons by proton combination [J]. PHYSICAL REVIEW, 1938, 54 (04): : 248 - 254

[8] A method for treating large perturbations [J]. PHYSICAL REVIEW, 1938, 54 (11): : 955 - 967

[9] The binding energy of the deuteron [J]. PHYSICAL REVIEW, 1938, 53 (04): : 313 - 314

[10] BETHE HA, 1937, REV MOD PHYS, V9, P71

[1] A precise measurement of the mass difference Be-4(9)-Be-4(8); The stability of Be-4(8) [J]. PHYSICAL REVIEW, 1939, 55 (01): : 0107 - 0107

[2] On the question of the possibility of building elements in stars [J]. ZEITSCHRIFT FUR PHYSIK, 1929, 54 (9-10): : 656 - 665

[3] Evidence against He-5 [J]. PHYSICAL REVIEW, 1935, 48 (04): : 382 - 382

[4] BAINBRIDGE KT, 1938, PHYS REV, V53, pA922

[5] The neutrino [J]. NATURE, 1934, 133 : 689 - 690

[6] Coulomb energy of light nuclei [J]. PHYSICAL REVIEW, 1938, 54 (06): : 436 - 439

[7] The formation of deuterons by proton combination [J]. PHYSICAL REVIEW, 1938, 54 (04): : 248 - 254

[8] A method for treating large perturbations [J]. PHYSICAL REVIEW, 1938, 54 (11): : 955 - 967

[9] The binding energy of the deuteron [J]. PHYSICAL REVIEW, 1938, 53 (04): : 313 - 314

[10] BETHE HA, 1937, REV MOD PHYS, V9, P71