Inflation can save cosmic strings

Details Inflation can save cosmic strings Inflation can save cosmic strings

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phrvl..63..712y&link_type=abstract

Physical Review Letters, Volume 63, Issue 7, August 14, 1989, pp.712-715

Physics

41

Particle-Theory And Field-Theory Models Of The Early Universe

Scientific paper

A new scenario of cosmic strings is presented which is free from the gravitational-radiation constraints imposed on their line density by the primordial nucleosynthesis and the timing data of a millisecond pulsar. In this scenario the phase transition is induced nonthermally during the inflation so that it is not necessary to assume Friedmann-Robertson-Walker universe in thermal equilibrium at the outset.

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