Cosmological constraints on string scale and coupling arising from tachyonic instability
Feb, 2005
12 pages
Published in:
- JHEP 08 (2005) 084
e-Print:
- hep-th/0502185 [hep-th]
Report number:
- NORDITA-2005-18,
- HIP-2005-07-TH
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Abstract:
We demonstrate that string motivated inflation ending via tachyonic instability leaves a detectable imprint on the cosmic microwave background (CMB) radiation by virtue of the excitation of non-Gaussian gravitational fluctuations. The present WMAP bound on non-Gaussianity is shown to constrain the string scale by for string coupling , hence improving the existing bounds. If tachyon fluctuations during inflation are not negligible, we find the stringent constraint for . This case may soon be ruled out by the forthcoming CMB non-Gaussinianity bounds.- NON-GAUSSIANITY
- TACHYONS
- STRINGS
- INFLATION
- cosmological model
- string model
- fluctuation
- tachyon
- stability
- numerical calculations
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