期刊
THEORETICAL AND MATHEMATICAL PHYSICS
卷 148, 期 1, 页码 895-909出版社
MAIK NAUKA/INTERPERIODICA/SPRINGER
DOI: 10.1007/s11232-006-0086-5
关键词
strings; string field theory; cosmology; branes; tachyon; phantom; dark energy; big rip
We construct an exact solution of the Friedmann equations with a phantom scalar matter field originating in string field theory and show the absence of the big-rip singularity. The notable features of the model are a ghost sign of the kinetic term and a special polynomial form of the effective tachyon potential. The constructed solution is stable under small fluctuations of the initial conditions and special variations of the form of the potential.
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