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A New Exactly Solvable Inflation Model and Its Power Spectrum
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LI Xin-Zhou;LIU Dao-Jun;HAO Jian-Gang |
Shanghai United Center for Astrophysics, Shanghai Normal University, Shanghai 200234
Institute for Theoretical Physics, East China University of Science and Technology, Shanghai 200237 |
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Cite this article: |
LI Xin-Zhou, LIU Dao-Jun, HAO Jian-Gang 2003 Chin. Phys. Lett. 20 192-194 |
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Abstract We present a new exactly solvable inflation model in which inflation can stop automatically, and in the approximately de Sitter limit, we give its power spectrum which can be tested in the future observations of cosmic microwave background anisotropy.
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Keywords:
04.20.-q
98.80.Cq
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Published: 01 February 2003
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PACS: |
04.20.-q
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(Classical general relativity)
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98.80.Cq
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(Particle-theory and field-theory models of the early Universe (including cosmic pancakes, cosmic strings, chaotic phenomena, inflationary universe, etc.))
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