NEW FORMULATION OF THE GENERAL THEORY OF RELATIVITY

[1] BERGMANN PG, 1942, INTRO THEORY RELATIV, P201

[2] BESANT WH, 1902, DYNAMICS, P207

[3] BONDI H, 1952, COSOMLOGY, P70

[4] ON THE INTERPRETATION OF FREUNDLICH RED-SHIFT FORMULA [J]. PROCEEDINGS OF THE PHYSICAL SOCIETY OF LONDON SECTION A, 1954, 67 (410): : 193 - 194

[5] FINLAYFREUNDLIC.E, 1954, NACHR AKAD WISS MPK

[6] RED-SHIFTS IN THE SPECTRA OF CELESTIAL BODIES [J]. PROCEEDINGS OF THE PHYSICAL SOCIETY OF LONDON SECTION A, 1954, 67 (410): : 192 - 193

[7] A NEW MODEL FOR THE EXPANDING UNIVERSE [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1948, 108 (05) : 372 - 382

[8] ON THE COSMOLOGICAL PROBLEM [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1949, 109 (03) : 365 - 371

[9] THE PHYSICAL MEANING OF AUXILIARY CONDITIONS IN THE THEORY OF GRAVITATIONAL WAVES [J]. CANADIAN JOURNAL OF PHYSICS, 1953, 31 (04) : 501 - 503

[10] DIE FORMULIERUNG DER ERHALTUNGSSATZE DER ENERGIE UND DES IMPULSES IN DER ALLGEMEINEN RELATIVITATSTHEORIE .2. [J]. ZEITSCHRIFT FUR PHYSIK, 1953, 134 (03): : 286 - 305

[1] BERGMANN PG, 1942, INTRO THEORY RELATIV, P201

[2] BESANT WH, 1902, DYNAMICS, P207

[3] BONDI H, 1952, COSOMLOGY, P70

[4] ON THE INTERPRETATION OF FREUNDLICH RED-SHIFT FORMULA [J]. PROCEEDINGS OF THE PHYSICAL SOCIETY OF LONDON SECTION A, 1954, 67 (410): : 193 - 194

[5] FINLAYFREUNDLIC.E, 1954, NACHR AKAD WISS MPK

[6] RED-SHIFTS IN THE SPECTRA OF CELESTIAL BODIES [J]. PROCEEDINGS OF THE PHYSICAL SOCIETY OF LONDON SECTION A, 1954, 67 (410): : 192 - 193

[7] A NEW MODEL FOR THE EXPANDING UNIVERSE [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1948, 108 (05) : 372 - 382

[8] ON THE COSMOLOGICAL PROBLEM [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1949, 109 (03) : 365 - 371

[9] THE PHYSICAL MEANING OF AUXILIARY CONDITIONS IN THE THEORY OF GRAVITATIONAL WAVES [J]. CANADIAN JOURNAL OF PHYSICS, 1953, 31 (04) : 501 - 503

[10] DIE FORMULIERUNG DER ERHALTUNGSSATZE DER ENERGIE UND DES IMPULSES IN DER ALLGEMEINEN RELATIVITATSTHEORIE .2. [J]. ZEITSCHRIFT FUR PHYSIK, 1953, 134 (03): : 286 - 305