Evolution of primordial perturbations and a fluctuating decay rate
暂无分享,去创建一个
[1] Birmingham,et al. Large scale curvature and entropy perturbations for multiple interacting fluids , 2002, astro-ph/0211602.
[2] T. Moroi,et al. Erratum to: “Effects of cosmological moduli fields on cosmic microwave background”: [Phys. Lett. B 522 (2001) 215] , 2002 .
[3] K. Enqvist,et al. Adiabatic CMB perturbations in pre - big bang string cosmology , 2001, hep-ph/0109214.
[4] T. Moroi,et al. Effects of cosmological moduli fields on cosmic microwave background , 2001, hep-ph/0110096.
[5] D. Lyth,et al. Generating the curvature perturbation without an inflaton , 2001, hep-ph/0110002.
[6] J. García-Bellido,et al. Metric perturbations in two-field inflation. , 1995, Physical review. D, Particles and fields.
[7] Hume A. Feldman,et al. Theory of cosmological perturbations , 1992 .
[8] S. Mollerach,et al. Isocurvature baryon perturbations and inflation. , 1990, Physical review. D, Particles and fields.
[9] Andrei Linde. Particle Physics and Inflationary Cosmology , 1987, Physics Today.
[10] H. Kodama,et al. Cosmological Perturbation Theory , 1984 .
[11] Michael S. Turner,et al. Spontaneous Creation of Almost Scale - Free Density Perturbations in an Inflationary Universe , 1983 .
[12] J. Bardeen,et al. Gauge Invariant Cosmological Perturbations , 1980 .