Cosmological constraints on string scale and coupling arising from tachyonic instability

Feb, 2005
12 pages
Published in:
  • JHEP 08 (2005) 084
e-Print:
Report number:
  • NORDITA-2005-18,
  • HIP-2005-07-TH

Citations per year

2005200720092011201301234567
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 MS/MP104M_S/M_P\leq 10^{-4} for string coupling gs<0.1g_{s}<0.1, hence improving the existing bounds. If tachyon fluctuations during inflation are not negligible, we find the stringent constraint gs109g_s\sim 10^{-9} for MS/MP<103M_{S}/M_{P}<10^{-3}. 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