A NATURAL WAY OUT OF THE CONFLICT BETWEEN COSMIC STRINGS AND INFLATION

[11] LINDE AD, 1983, PHYS LETT B, V129, P177, DOI 10.1016/0370-2693(83)90837-7

[12] SCALAR FIELD FLUCTUATIONS IN THE EXPANDING UNIVERSE AND THE NEW INFLATIONARY UNIVERSE SCENARIO [J]. PHYSICS LETTERS B, 1982, 116 (05) : 335 - 339

[13] LINDE AD, 1986, MOD PHYS LETT A, V2, P81

[14] COSMIC STRINGS AND AN IMPROVED UPPER BOUND ON THE ENERGY DENSITY DURING INFLATION [J]. PHYSICS LETTERS B, 1987, 196 (02) : 126 - 128

[15] VORTEX-LINE MODELS FOR DUAL STRINGS [J]. NUCLEAR PHYSICS B, 1973, B 61 (SEP24) : 45 - 61

[16] IS INFLATION COMPATIBLE WITH STRING-INDUCED GALAXY FORMATION [J]. PHYSICS LETTERS B, 1987, 185 (1-2) : 34 - 38

[17] MAGNETIC MONOPOLES [J]. ANNUAL REVIEW OF NUCLEAR AND PARTICLE SCIENCE, 1984, 34 : 461 - 530

[18] SATO H, 1986, MOD PHYS LETT A, V1, P9

[19] 1ST-ORDER PHASE-TRANSITION OF A VACUUM AND THE EXPANSION OF THE UNIVERSE [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1981, 195 (02) : 467 - 479

[20] HEATING AFTER HIGHER DIMENSIONAL INFLATION [J]. NUCLEAR PHYSICS B, 1988, 297 (04) : 697 - 720

[11] LINDE AD, 1983, PHYS LETT B, V129, P177, DOI 10.1016/0370-2693(83)90837-7

[12] SCALAR FIELD FLUCTUATIONS IN THE EXPANDING UNIVERSE AND THE NEW INFLATIONARY UNIVERSE SCENARIO [J]. PHYSICS LETTERS B, 1982, 116 (05) : 335 - 339

[13] LINDE AD, 1986, MOD PHYS LETT A, V2, P81

[14] COSMIC STRINGS AND AN IMPROVED UPPER BOUND ON THE ENERGY DENSITY DURING INFLATION [J]. PHYSICS LETTERS B, 1987, 196 (02) : 126 - 128

[15] VORTEX-LINE MODELS FOR DUAL STRINGS [J]. NUCLEAR PHYSICS B, 1973, B 61 (SEP24) : 45 - 61

[16] IS INFLATION COMPATIBLE WITH STRING-INDUCED GALAXY FORMATION [J]. PHYSICS LETTERS B, 1987, 185 (1-2) : 34 - 38

[17] MAGNETIC MONOPOLES [J]. ANNUAL REVIEW OF NUCLEAR AND PARTICLE SCIENCE, 1984, 34 : 461 - 530

[18] SATO H, 1986, MOD PHYS LETT A, V1, P9

[19] 1ST-ORDER PHASE-TRANSITION OF A VACUUM AND THE EXPANSION OF THE UNIVERSE [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1981, 195 (02) : 467 - 479

[20] HEATING AFTER HIGHER DIMENSIONAL INFLATION [J]. NUCLEAR PHYSICS B, 1988, 297 (04) : 697 - 720